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834 results on '"University of Warsaw (UW)"'

1. Degenerate Cahn-Hilliard equation: From nonlocal to local

Author: Charles Elbar, Jakub Skrzeczkowski, Sorbonne Université (SU), Laboratoire Jacques-Louis Lions (LJLL (UMR_7598)), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Modelling and Analysis for Medical and Biological Applications (MAMBA), Inria de Paris, Institut National de Recherche en Informatique et en Automatique (Inria)-Institut National de Recherche en Informatique et en Automatique (Inria)-Laboratoire Jacques-Louis Lions (LJLL (UMR_7598)), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institute of Mathematics [Warsaw], Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), and University of Warsaw (UW)-University of Warsaw (UW)
Subjects: Mathematics - Analysis of PDEs, Nonlocal Cahn-Hilliard equation, Applied Mathematics, FOS: Mathematics, Aggregation-Diﬀusion, [MATH]Mathematics [math], 35B40, 35D30, 35K25, 35K55, Singular limit, 2020 Mathematics Subject Classiﬁcation. 35B40, 35D30, 35K25, 35K55, Analysis, Analysis of PDEs (math.AP), Degenerate Cahn-Hilliard equation
Abstract: International audience; There has been recently an important interest in deriving rigorously the Cahn-Hilliard equation from the nonlocal equation, also called aggregation equation. So far, only non-degenerate mobilities were treated. Since we are motivated by models for the biomechanics of living tissues, it is useful to include degenerate motilities. In this framework, we present a new method to show the convergence of the nonlocal to the local degenerate Cahn-Hilliard equation. The method includes the use of nonlocal Poincar\'e and compactness inequalities.
Published: 2023
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2. On the limit problem arising in the kinetic derivation of the Cahn-Hilliard equation

Author: Elbar, Charles, Perthame, Benoît, Skrzeczkowski, Jakub, Laboratoire Jacques-Louis Lions (LJLL (UMR_7598)), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Modelling and Analysis for Medical and Biological Applications (MAMBA), Inria de Paris, Institut National de Recherche en Informatique et en Automatique (Inria)-Institut National de Recherche en Informatique et en Automatique (Inria)-Laboratoire Jacques-Louis Lions (LJLL (UMR_7598)), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institute of Mathematics [Warsaw], Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), and University of Warsaw (UW)-University of Warsaw (UW)
Subjects: Mathematics - Analysis of PDEs, [MATH.MATH-MP]Mathematics [math]/Mathematical Physics [math-ph], 2020 MSC: 35B40, 35D30, 35K25, 35K55, FOS: Mathematics, [MATH.MATH-AP]Mathematics [math]/Analysis of PDEs [math.AP], 35B40, 35D30, 35K25, 35K55, Analysis of PDEs (math.AP)
Abstract: The non-local degenerate Cahn-Hilliard equation is derived from the Vlasov equation with long-range attraction. We study the local limit as the delocalization parameter converges to 0. The difficulty arises from the degeneracy which requires compactness estimates, but all necessary a priori estimates can be obtained only on the nonlocal quantities yielding almost no information on the limiting solution itself. We introduce a novel condition on the nonlocal kernel which allows us to exploit the available nonlocal a priori estimates. The condition, satisfied by most of the kernels appearing in the applications, can be of independent interest. Our approach is flexible and systems can be treated as well., 15 pages + Appendix
Published: 2023

3. Static Analysis of Graph Database Transformations

Author: Boneva, Iovka, Groz, Benoit, Hidders, Jan, Murlak, Filip, Staworko, Slawomir, Centre de Recherche en Informatique, Signal et Automatique de Lille - UMR 9189 (CRIStAL), Centrale Lille-Université de Lille-Centre National de la Recherche Scientifique (CNRS), Linking Dynamic Data (LINKS), Inria Lille - Nord Europe, Institut National de Recherche en Informatique et en Automatique (Inria)-Institut National de Recherche en Informatique et en Automatique (Inria)-Centre de Recherche en Informatique, Signal et Automatique de Lille - UMR 9189 (CRIStAL), Centrale Lille-Université de Lille-Centre National de la Recherche Scientifique (CNRS)-Centrale Lille-Université de Lille-Centre National de la Recherche Scientifique (CNRS), Laboratoire Interdisciplinaire des Sciences du Numérique (LISN), Institut National de Recherche en Informatique et en Automatique (Inria)-CentraleSupélec-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Données et Connaissances Massives et Hétérogènes (LaHDAK), Institut National de Recherche en Informatique et en Automatique (Inria)-CentraleSupélec-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche en Informatique et en Automatique (Inria)-CentraleSupélec-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Science des Données (SDD), Institut National de Recherche en Informatique et en Automatique (Inria)-CentraleSupélec-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche en Informatique et en Automatique (Inria)-CentraleSupélec-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Birkbeck College [University of London], University of Warsaw (UW), Poland’s National Science Centre grant 2018/30/E/ST6/00042., Centre de Recherche en Informatique, Signal et Automatique de Lille - UMR 9189 [CRIStAL], Linking Dynamic Data [LINKS], Laboratoire Interdisciplinaire des Sciences du Numérique [LISN], Données et Connaissances Massives et Hétérogènes [LaHDAK], and University of Warsaw [UW]
Subjects: FOS: Computer and information sciences, [INFO.INFO-DB]Computer Science [cs]/Databases [cs.DB], Computer Science - Databases, graph databases, graph schemas, data transformations, Databases (cs.DB)
Abstract: International audience; We investigate graph transformations, defined using Datalog-like rules based on acyclic conjunctive two-way regular path queries (acyclic C2RPQs), and we study two fundamental static analysis problems: type checking and equivalence of transformations in the presence of graph schemas. Additionally, we investigate the problem of target schema elicitation, which aims to construct a schema that closely captures all outputs of a transformation over graphs conforming to the input schema. We show all these problems are in EXPTIME by reducing them to C2RPQ containment modulo schema; we also provide matching lower bounds. We use cycle reversing to reduce query containment to the problem of unrestricted (finite or infinite) satisfiability of C2RPQs modulo a theory expressed in a description logic.
Published: 2023

4. On the inviscid limit connecting Brinkman's and Darcy's models of tissue growth with nonlinear pressure

Author: Elbar, Charles, Skrzeczkowski, Jakub, Sorbonne Université (SU), Laboratoire Jacques-Louis Lions (LJLL (UMR_7598)), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Modelling and Analysis for Medical and Biological Applications (MAMBA), Inria de Paris, Institut National de Recherche en Informatique et en Automatique (Inria)-Institut National de Recherche en Informatique et en Automatique (Inria)-Laboratoire Jacques-Louis Lions (LJLL (UMR_7598)), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institute of Mathematics [Warsaw], Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), University of Warsaw (UW)-University of Warsaw (UW), and Jakub Skrzeczkowski was supported by National Science Center, Poland through project no.2018/30/M/ST1/00423.
Subjects: Mathematics - Analysis of PDEs, 35K45, 35K65, 35J60, 35Q92, 92C10, FOS: Mathematics, 2020 Mathematics Subject Classification. 35K45, 35K65, 35J60, 35Q92, 92C10, Brinkman's law, Darcy's law, [MATH]Mathematics [math], Nonlocal-to-local limit, Nonlocal equation, Inviscid limit, Tissue growth, Analysis of PDEs (math.AP)
Abstract: Several recent papers have addressed modelling of the tissue growth by the multi-phase models where the velocity is related to the pressure by one of the physical laws (Stoke's, Brinkman's or Darcy's). While each of these models has been extensively studied, not so much is known about the connection between them. In the recent paper (arXiv:2303.10620), assuming the linear form of the pressure, the Authors connected two multi-phase models by an inviscid limit: the viscoelastic one (of Brinkman's type) and the inviscid one (of Darcy's type). Here, we prove that the same is true for a nonlinear, power-law pressure. The new ingredient is that we use relation between the pressure $p$ and the Brinkman potential $W$ to deduce compactness in space of $p$ from the compactness in space of $W$., Comment: 13 pages + appendix + bibliography; in the new version a missing reference in the Appendix was added
Published: 2023
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5. The coordinated replication of Vibrio cholerae’s two chromosomes required the acquisition of a unique domain by the RctB initiator

Author: Fournes, Florian, Niault, Theophile, Czarnecki, Jakub, Tissier-Visconti, Alvise, Mazel, Didier, Val, Marie-Eve, Plasticité du Génome Bactérien - Bacterial Genome Plasticity (PGB), Institut Pasteur [Paris] (IP)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Sorbonne université - Faculté des Sciences et Ingénierie (SU FSI), Sorbonne Université (SU), Institute of Microbiology [Warsaw], Faculty of Biology [Warsaw], University of Warsaw (UW)-University of Warsaw (UW), Institut Pasteur, Institut National de la Santé et de la Recherche Médicale (INSERM), Centre National de la Recherche Scientifique [CNRS-UMR 3525], French National Research Agency, Jeunes Chercheurs [ANR-19-CE12-0001], Laboratoires d’Excellence [ANR-10-LABX-62-IBEID], F.F. was supported by ANR-10-LABX-62-IBEID and ANR-19-CE12-0001, T.N. was supported by the Ministère de l’Enseignement Supérieur et de la Recherche, J.C. was supported by Institut Pasteur (Cantarini foundation) [ANR-19-CE12-0001, ANR-10-LABX-62-IBEID]. Funding for open access charge: French National Research Agency [ANR-19-CE12-0001]., ANR-19-CE12-0001,RepliChroms,Contrôle de la Réplication chez les Bactéries à Multiple Chromosomes(2019), ANR-10-LABX-0062,IBEID,Integrative Biology of Emerging Infectious Diseases(2010), and Institut Pasteur [Paris]-Centre National de la Recherche Scientifique (CNRS)
Subjects: MESH: Signal Transduction, Models, Molecular, Protein Conformation, alpha-Helical, MESH: Sequence Homology, Amino Acid, AcademicSubjects/SCI00010, MESH: DNA Replication, MESH: Amino Acid Sequence, MESH: Base Sequence, Genome Integrity, Repair and Replication, MESH: Recombinant Proteins, MESH: Genetic Vectors, MESH: Replication Origin, Cloning, Molecular, MESH: Bacterial Proteins, Vibrio cholerae, MESH: Gene Expression Regulation, Bacterial, MESH: Escherichia coli, Chromosomes, Bacterial, Recombinant Proteins, MESH: Protein Conformation, beta-Strand, MESH: Models, Molecular, Protein Binding, Signal Transduction, DNA Replication, DNA, Bacterial, MESH: Chromosomes, Bacterial, Genetic Vectors, MESH: Sequence Alignment, MESH: Binding, Competitive, Replication Origin, Binding, Competitive, Bacterial Proteins, Escherichia coli, MESH: Protein Binding, MESH: Cloning, Molecular, [SDV.BBM]Life Sciences [q-bio]/Biochemistry, Molecular Biology, Protein Interaction Domains and Motifs, Amino Acid Sequence, MESH: Protein Conformation, alpha-Helical, MESH: Protein Interaction Domains and Motifs, Binding Sites, Base Sequence, Sequence Homology, Amino Acid, fungi, Gene Expression Regulation, Bacterial, MESH: DNA, Bacterial, MESH: Binding Sites, nervous system, Protein Conformation, beta-Strand, Sequence Alignment, MESH: Vibrio cholerae
Abstract: International audience; Vibrio cholerae, the pathogenic bacterium that causes cholera, has two chromosomes (Chr1, Chr2) that replicate in a well-orchestrated sequence. Chr2 initiation is triggered only after the replication of the crtS site on Chr1. The initiator of Chr2 replication, RctB, displays activities corresponding with its different binding sites: initiator at the iteron sites, repressor at the 39m sites, and trigger at the crtS site. The mechanism by which RctB relays the signal to initiate Chr2 replication from crtS is not well-understood. In this study, we provide new insights into how Chr2 replication initiation is regulated by crtS via RctB. We show that crtS (on Chr1) acts as an anti-inhibitory site by preventing 39m sites (on Chr2) from repressing initiation. The competition between these two sites for RctB binding is explained by the fact that RctB interacts with crtS and 39m via the same DNA-binding surface. We further show that the extreme C-terminal tail of RctB, essential for RctB self-interaction, is crucial for the control exerted by crtS. This subregion of RctB is conserved in all Vibrio, but absent in other Rep-like initiators. Hence, the coordinated replication of both chromosomes likely results from the acquisition of this unique domain by RctB.
Published: 2021
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6. Induced minors and well-quasi-ordering

Author: Jaroslaw Blasiok, Jean-Florent Raymond, Marcin Kamiński, Théophile Trunck, Department of Mathematics, Computer Science and Mechanics [Warsaw], University of Warsaw ( UW ), Institute of Informatics, University of Warsaw, Banacha 2, 02-097 Warsaw, Poland., Institute of Informatics, Université de Varsovie-Université de Varsovie, Faculty of Mathematics, Informatics, and Mechanics [Warsaw], Algorithmes, Graphes et Combinatoire ( ALGCO ), Laboratoire d'Informatique de Robotique et de Microélectronique de Montpellier ( LIRMM ), Université de Montpellier ( UM ) -Centre National de la Recherche Scientifique ( CNRS ) -Université de Montpellier ( UM ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de l'Informatique du Parallélisme ( LIP ), École normale supérieure - Lyon ( ENS Lyon ) -Université Claude Bernard Lyon 1 ( UCBL ), Université de Lyon-Université de Lyon-Institut National de Recherche en Informatique et en Automatique ( Inria ) -Centre National de la Recherche Scientifique ( CNRS ), Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), University of Warsaw (UW), Algorithmes, Graphes et Combinatoire (ALGCO), Laboratoire d'Informatique de Robotique et de Microélectronique de Montpellier (LIRMM), Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Modèles de calcul, Complexité, Combinatoire (MC2), Laboratoire de l'Informatique du Parallélisme (LIP), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Recherche en Informatique et en Automatique (Inria)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Recherche en Informatique et en Automatique (Inria)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM), Centre National de la Recherche Scientifique (CNRS)-Université de Lyon-Institut National de Recherche en Informatique et en Automatique (Inria)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-École normale supérieure - Lyon (ENS Lyon)-Centre National de la Recherche Scientifique (CNRS)-Université de Lyon-Institut National de Recherche en Informatique et en Automatique (Inria)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-École normale supérieure - Lyon (ENS Lyon), École normale supérieure - Lyon (ENS Lyon)-Université Claude Bernard Lyon 1 (UCBL), and Université de Lyon-Université de Lyon-Institut National de Recherche en Informatique et en Automatique (Inria)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Lyon (ENS Lyon)-Université Claude Bernard Lyon 1 (UCBL)
Subjects: FOS: Computer and information sciences, Discrete Mathematics (cs.DM), Well-quasi-ordering, Induced subgraph, G.2.2, 0102 computer and information sciences, [INFO.INFO-DM]Computer Science [cs]/Discrete Mathematics [cs.DM], [ MATH.MATH-CO ] Mathematics [math]/Combinatorics [math.CO], 01 natural sciences, Theoretical Computer Science, Combinatorics, [MATH.MATH-CO]Mathematics [math]/Combinatorics [math.CO], FOS: Mathematics, Combinatorial dichotomies, Mathematics - Combinatorics, Discrete Mathematics and Combinatorics, 0101 mathematics, ComputingMilieux_MISCELLANEOUS, Mathematics, Applied Mathematics, 010102 general mathematics, Complete graph, [ INFO.INFO-DM ] Computer Science [cs]/Discrete Mathematics [cs.DM], Graph theory, 16. Peace & justice, Graph, Vertex (geometry), Computational Theory and Mathematics, 010201 computation theory & mathematics, Combinatorics (math.CO), 05C, 06A07, Combinatorial theory, Induced minors, Computer Science - Discrete Mathematics
Abstract: A graph $H$ is an induced minor of a graph $G$ if it can be obtained from an induced subgraph of $G$ by contracting edges. Otherwise, $G$ is said to be $H$-induced minor-free. Robin Thomas showed that $K_4$-induced minor-free graphs are well-quasi-ordered by induced minors [Graphs without $K_4$ and well-quasi-ordering, Journal of Combinatorial Theory, Series B, 38(3):240 -- 247, 1985]. We provide a dichotomy theorem for $H$-induced minor-free graphs and show that the class of $H$-induced minor-free graphs is well-quasi-ordered by the induced minor relation if and only if $H$ is an induced minor of the gem (the path on 4 vertices plus a dominating vertex) or of the graph obtained by adding a vertex of degree 2 to the complete graph on 4 vertices. To this end we proved two decomposition theorems which are of independent interest. Similar dichotomy results were previously given for subgraphs by Guoli Ding in [Subgraphs and well-quasi-ordering, Journal of Graph Theory, 16(5):489--502, 1992] and for induced subgraphs by Peter Damaschke in [Induced subgraphs and well-quasi-ordering, Journal of Graph Theory, 14(4):427--435, 1990].
Published: 2019
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7. THz detectors based on Si-CMOS technology field effect transistors – advantages, limitations and perspectives for THz imaging and spectroscopy

Author: Dominique Coquillat, Jacek Marczewski, D. Obrebski, D. Yavorskiy, Przemyslaw Zagrajek, Pawel Kopyt, Cezary Kolacinski, Krzysztof Kucharski, Norbert Palka, Radoslaw Ryniec, Wojciech Knap, Daniel Tomaszewski, J. Lusakowski, Laboratoire Charles Coulomb (L2C), Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Institute of Experimental Physics [Warsaw] (IFD), Faculty of Physics [Warsaw] (FUW), and University of Warsaw (UW)-University of Warsaw (UW)
Subjects: Coupling, Radiation, Materials science, business.industry, Terahertz radiation, Detector, 020206 networking & telecommunications, 02 engineering and technology, 021001 nanoscience & nanotechnology, [PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph], CMOS, 0202 electrical engineering, electronic engineering, information engineering, Optoelectronics, General Materials Science, Field-effect transistor, Electrical and Electronic Engineering, 0210 nano-technology, business, Spectroscopy, Cmos process, Thz spectroscopy
Abstract: International audience; Recent advances in THz detection with the use of CMOS technology have shown that this option has the potential to be a leading method of producing low-cost THz sensors with integrated readout systems. This review paper, based on authors’ years of experience, presents strengths and weaknesses of this solution. The article gives examples of some hints, regarding radiation coupling and readout systems. It shows that silicon CMOS technology is well adapted to the production of inexpensive imaging systems for sub-THz frequencies. As an example paper presents the demonstrator of a multipixel Si-CMOS THz spectroscopic system allowing for chemical identification of lactose. The THz detectors embedded in this system were manufactured using the CMOS process.
Published: 2018
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8. MixInYeast: A Multicenter Study on Mixed Yeast Infections

Author: Julio García-Rodríguez, Lourdes Viñuela, Carole Cassagne, Juergen Prattes, Sevtap Arikan-Akdagli, Stéphane Bretagne, Aleksandra Barac, Juan Carlos Soto-Debran, Patricia Muñoz, Işın Akyar, Tomasz Jagielski, Hamid Badali, Danila Seidel, Carmen Barroso Castro, Rocio Tejero, Ana Perez-Ayala Balzola, Giuliana Lo Cascio, Arunaloke Chakrabarti, Sadegh Khodavaisy, María Carmen Martínez-Rubio, Maite Ruiz Pérez de Pipaón, Thanwa Wongsuk, Teresa Peláez, Ana Alastruey-Izquierdo, Yasemin Cag, Raphael Stauf, Elżbieta Ochman, Jörg Steinmann, Joseph Meletiadis, Ana Isabel Suárez-Barrenechea, Cornelia Lass-Flörl, Laura Trovato, Narda Medina, Celia Cardozo, Emmanuel Roilides, Juliette Guitard, Hossein Zarrinfar, Iwona Żak, Martin Hoenigl, Petr Hamal, Eric Dannaoui, University of Belgrade [Belgrade], Laboratoire de Parasitologie-Mycologie [CHU Saint Louis, Paris], Groupe Hospitalier Saint Louis - Lariboisière - Fernand Widal [Paris], Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP), Université Paris Cité (UPCité), Istanbul Medeniyet University [Istanbul, Turquie] (IMU), Vecteurs - Infections tropicales et méditerranéennes (VITROME), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut de Recherche Biomédicale des Armées [Brétigny-sur-Orge] (IRBA), Post Graduate Institute of Medical Education & Research [Chandigarh, India], Dynamic Microbiology - EA 7380 (DYNAMIC), École nationale vétérinaire - Alfort (ENVA)-Agence nationale de sécurité sanitaire de l'alimentation, de l'environnement et du travail (ANSES)-Université Paris-Est (UPE)-Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12), CHU Saint-Antoine [AP-HP], Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU), University of California [San Diego] (UC San Diego), University of California (UC), Medical University of Graz, Department of Applied Microbiology [Warsaw], Institute of Microbiology [Warsaw], Faculty of Biology [Warsaw], University of Warsaw (UW)-University of Warsaw (UW)-Faculty of Biology [Warsaw], University of Warsaw (UW)-University of Warsaw (UW), Biomedicina, Biotecnología y Salud Pública, Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut de Recherche Biomédicale des Armées (IRBA), Service de Parasitologie - Mycologie [CHU Saint-Antoine], Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU), and Acibadem University Dspace
Subjects: Microbiology (medical), polymicrobial infections, medicine.medical_specialty, Medizin, Plant Science, yeast, Article, Microbiology, Vaccine Related, 03 medical and health sciences, 0302 clinical medicine, [SDV.MHEP.CSC]Life Sciences [q-bio]/Human health and pathology/Cardiology and cardiovascular system, [SDV.MHEP.MI]Life Sciences [q-bio]/Human health and pathology/Infectious diseases, Amphotericin B, Biodefense, Epidemiology, Medicine, [SDV.MP.PAR]Life Sciences [q-bio]/Microbiology and Parasitology/Parasitology, 030212 general & internal medicine, Candida albicans, Prospective cohort study, lcsh:QH301-705.5, Ecology, Evolution, Behavior and Systematics, Candida, 0303 health sciences, [SDV.MHEP.ME]Life Sciences [q-bio]/Human health and pathology/Emerging diseases, biology, 030306 microbiology, business.industry, Prevention, Invasive candidiasis, invasive candidiasis, biology.organism_classification, medicine.disease, [SDV.MP.BAC]Life Sciences [q-bio]/Microbiology and Parasitology/Bacteriology, Yeast, Corpus albicans, 3. Good health, Infectious Diseases, Multicenter study, lcsh:Biology (General), [SDV.MP.VIR]Life Sciences [q-bio]/Microbiology and Parasitology/Virology, Antimicrobial Resistance, business, Infection, chrome agar, medicine.drug, mix infections
Abstract: Invasive candidiasis remains one of the most prevalent systemic mycoses, and several studies have documented the presence of mixed yeast (MY) infections. Here, we describe the epidemiology, clinical, and microbiological characteristics of MY infections causing invasive candidiasis in a multicenter prospective study. Thirty-four centers from 14 countries participated. Samples were collected in each center between April to September 2018, and they were sent to a reference center to confirm identification by sequencing methods and to perform antifungal susceptibility testing, according to the European Committee on Antimicrobial Susceptibility Testing (EUCAST). A total of 6895 yeast cultures were identified and MY occurred in 150 cases (2.2%). Europe accounted for the highest number of centers, with an overall MY rate of 4.2% (118 out of 2840 yeast cultures). Of 122 MY cases, the most frequent combinations were Candida albicans/C. glabrata (42, 34.4%), C. albicans/C. parapsilosis (17, 14%), and C. glabrata/C. tropicalis (8, 6.5%). All Candida isolates were susceptible to amphotericin B, 6.4% were fluconazole-resistant, and two isolates (1.6%) were echinocandin-resistant. Accurate identification of the species involved in MY infections is essential to guide treatment decisions. Funding: research grant and GileadSciences research grant. Sí
Published: 2021
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9. Faint objects in motion: the new frontier of high precision astrometry

Author: Jordi Portell, Ariel Goobar, Alain Léger, Barbara McArthur, Renaud Goullioud, Pat Scott, Carme Jordi, Katherine Freese, Douglas Spolyar, Antonaldo Diaferio, John A. Tomsick, Gary A. Mamon, Luisa Ostorero, Glenn J. White, Rory Barnes, Paulo J. V. Garcia, Eva Villaver, L. Chemin, Torsten A. Enßlin, Berry Holl, Warren R. Brown, Conrado Albertus, Malcolm Fridlund, Hamish A. Clark, Miguel de Val-Borro, Christophe Le Poncin-Lafitte, Fabien Malbet, Mariateresa Crosta, Jean-Pierre Prost, Ummi Abbas, Erik Høg, Celine Boehm, Morgane Fortin, Sergei A. Klioner, Ariane Lançon, Oleg Y. Gnedin, D. L. Harrison, Lukasz Wyrzykowski, Alcione Mora, Laura L. Watkins, Aldo S. Bonomo, Daniel Michalik, Philippe Thebault, Frederic Courbin, Nigel Hambly, Andrew D. Holland, Lucas Labadie, Micaela Oertel, Melvyn B. Davies, Manuel A.V. Ribeiro da Silva, Hervé Bouy, Andreas Quirrenbach, Alberto Krone-Martins, Wesley A. Traub, Rosemary F. G. Wyse, Vitor Cardoso, J. Schneider, Xavier Luri, Jeremy Darling, Marco Castellani, Arnaud Siebert, André Moitinho de Almeida, Matthew W. Muterspaugh, Mario G. Lattanzi, Neil J. Murray, A. J. Falcão, David Hobbs, Paulo Gordo, Mario Damasso, Monica Valluri, António Amorim, Jacques Laskar, Yoshiyuki Yamada, Mario Gai, Alexandre C. M. Correia, Leonidas A. Moustakas, João Alves, Alexis Brandeker, David Hall, Antonio da Silva, Guillem Anglada-Escudé, Nicholas A. Walton, Antoine Crouzier, Alessandro Sozzetti, M. Shao, A. Mourao, Malbet, F [0000-0002-8029-4226], Apollo - University of Cambridge Repository, National Aeronautics and Space Administration (US), Swiss National Science Foundation, Polish National Agency for Academic Exchange, Swedish National Space Agency, Fundação para a Ciência e a Tecnologia (Portugal), Australian Research Council, Agenzia Spaziale Italiana, Ministerio de Ciencia, Innovación y Universidades (España), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France, School of Physics [Sydney], The University of Sydney, CENTRA, Universidade de Lisboa, Queen Mary University of London (QMUL), Stockholm University, Ecole Polytechnique Fédérale de Lausanne (EPFL), Max Planck Institute for Astrophysics, Max-Planck-Gesellschaft, UNINOVA / CTS, Campus FCT/UNL, University of Texas at Austin [Austin], Observatoire Astronomique de l'Université de Genève (ObsGE), Université de Genève = University of Geneva (UNIGE), University of Cologne, Institut d'astrophysique spatiale (IAS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Aurora Technology BV, Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), INAF - Osservatorio Astrofisico di Torino (OATo), Istituto Nazionale di Astrofisica (INAF), Centro de Astrobiologia [Madrid] (CAB), Instituto Nacional de Técnica Aeroespacial (INTA)-Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), Universidad de Granada = University of Granada (UGR), University of Vienna [Vienna], Department of Astronomy [Seattle], University of Washington [Seattle], Laboratoire d'Astrophysique de Bordeaux [Pessac] (LAB), Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Harvard-Smithsonian Center for Astrophysics (CfA), Harvard University-Smithsonian Institution, INAF - Osservatorio Astronomico di Roma (OAR), University of Antofogasta, Department of Physics, University of Coimbra, Universidade de Coimbra [Coimbra], Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), University of Colorado [Boulder], Lund University [Lund], Dipartimento di Fisica [Torino], Università degli studi di Torino = University of Turin (UNITO), Istituto Nazionale di Fisica Nucleare, Sezione di Torino (INFN, Sezione di Torino), Istituto Nazionale di Fisica Nucleare (INFN), Copernicus Astronomical Center of the Polish Academy of Sciences (CAMK), Polish Academy of Sciences (PAN), Leiden Observatory [Leiden], Universiteit Leiden, Chalmers University of Technology [Gothenburg, Sweden], Faculdade de Engenharia da Universidade do Porto (FEUP), Universidade do Porto = University of Porto, University of Michigan [Ann Arbor], University of Michigan System, The Open University [Milton Keynes] (OU), University of Edinburgh, Institute of Astronomy [Cambridge], University of Cambridge [UK] (CAM), Lund Observatory, Niels Bohr Institute [Copenhagen] (NBI), Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH), Institut de Ciencies del Cosmos (ICCUB), Universitat de Barcelona (UB), Lohrmann Observatory, Technische Universität Dresden = Dresden University of Technology (TU Dresden), Observatoire astronomique de Strasbourg (ObAS), Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Systèmes de Référence Temps Espace (SYRTE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), ESA - ESTEC (Netherlands), Columbia State Community College, Laboratoire Univers et Théories (LUTH (UMR_8102)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Thales Alenia Space [Toulouse] (TAS), THALES [France], Heidelberg University, University of Queensland [Brisbane], Imperial College London, Instítuto de Astrofísica e Ciências do Espaço [Lisboa], Faculdade de Ciencias da Universidade de Lisboa, Space Sciences Laboratory [Berkeley] (SSL), University of California [Berkeley] (UC Berkeley), University of California (UC)-University of California (UC), Planetary Science Institute [Tucson] (PSI), European Space Agency (Baltimore) Space Telescope Science Institute (ESA), Space Science and Technology Department [Didcot] (RAL Space), STFC Rutherford Appleton Laboratory (RAL), Science and Technology Facilities Council (STFC)-Science and Technology Facilities Council (STFC), Astronomical Observatory [Warsaw], Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), Johns Hopkins University (JHU), Department of Physics [Kyoto], Kyoto Sangyo University, Theia, ANR-11-LABX-0013,FOCUS,Des détecteurs pour Observer l'Univers(2011), European Project: 787886,COSMICLENS, Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA), Université de Genève (UNIGE), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), University of Granada [Granada], Smithsonian Institution-Harvard University [Cambridge], Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Università degli studi di Torino (UNITO), Universiteit Leiden [Leiden], Universidade do Porto, University of Copenhagen = Københavns Universitet (KU)-University of Copenhagen = Københavns Universitet (KU), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Thales Alenia Space [Cannes], Thales Alenia Space, University of California [Berkeley], University of California-University of California, Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), Observatoire de Paris - Site de Paris (OP), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)
Subjects: Computer science, [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], PLANET, shape, 01 natural sciences, Space mission, Local universe, galaxies, 010303 astronomy & astrophysics, media_common, Earth and Planetary Astrophysics (astro-ph.EP), High Energy Astrophysical Phenomena (astro-ph.HE), [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Exoplanets, James Webb Space Telescope, Astrophysics::Instrumentation and Methods for Astrophysics, Local Group, Astrometry, Cosmology, neutron-stars, EQUATION-OF-STATE, 16. Peace & justice, GALAXIES, SHAPE, [SDU.ASTR.GA]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA], Astrophysics::Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), NEUTRON-STARS, black-hole, equation-of-state, media_common.quotation_subject, Milky Way, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, MASS, 0103 physical sciences, DARK-MATTER, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astrophysics::Galaxy Astrophysics, [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR], Astronomy, Astronomy and Astrophysics, Astrophysics - Astrophysics of Galaxies, Galaxy, Redshift, Universe, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], HYPERVELOCITY STARS, dark-matter, planet, Space and Planetary Science, Sky, Astrophysics of Galaxies (astro-ph.GA), BLACK-HOLE, GALACTIC-HALO, mass, galactic-halo, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], hypervelocity stars, Astrophysics - Earth and Planetary Astrophysics
Abstract: The authors would like to thank the researchers and engineers who are not coauthors of this paper but who have taken part and have brought their contribution to the proposed missions to ESA successive calls: NEAT (M3), micro-NEAT (S1), and Theia (M4 and M5). An extensive list of supporters for the science objectives is given in [17]. We thank also Arianna Gallo for her contribution in our investigation of the shape of the MilkyWay dark matter halo and Krzysztof A. Rybicki who generated the plots from Fig. 14. We are grateful to the anonymous referee who helped to improve the quality of the paper with his/her remarks. Concerning the funding of our work, we would like to acknowledge the support of many agencies or programs. R.B. acknowledges support from NASA’s Virtual Planetary Laboratory lead team under cooperative agreements NNA13AA93A. A.C.M.C. acknowledges support from CFisUC strategic project (UID/FIS/04564/2019). F.C. acknowledges support by the Swiss National Science Foundation (SNSF) and by the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (COSMICLENS: grant agreement No. 787886). M.F. received support from Polish National Science Centre (NCN) under Grant No. 2017/26/D/ST9/00591. M.F. gratefully acknowledge the support of the Swedish National Space Agency (DNR 65/19, 174/18). D.H. thanks the Swedish National Space Agency (SNSA/Rymdstyrelsen) for their support. A.M. thanks the Portugese Fundac¸ ˜ao para a Ciˆencia e a Tecnologia (FCT) through the Strategic Programme UID/FIS/00099/2019 for CENTRA. P.S. acknowledges support from the Australian Research Council under grant FT190100814. L.W. acknowledges support from the Polish NCN grants: Harmonia No. 2018/06M/ST9/00311 and Daina No. 2017/27/L/ST9/03221. The OATo team acknowledges partial funding by the Italian Space Agency (ASI) under contracts 2014-025-R.1.2015 and 2018-24-HH.0, and by a grant from the Italian Ministry of Foreign Affairs and International Cooperation (ASTRA). A.C. and F.M. acknowledge support by the LabEx FOCUS ANR-11-LABX-0013. The work of C.J., X.L. and J.P. was supported by the Spanish Ministry of Science, Innovation and University (MICIU/FEDER, UE) through grants RTI2018-095076-B-C21, ESP2016-80079-C2-1-R, and the Institute of Cosmos Sciences University of Barcelona (ICCUB, Unidad de Excelencia ’Mar´ıa de Maeztu’) through grants MDM-2014-0369 and CEX2019-000918-M. A.K.-M., A.A., V.C., P.G., P.G., A.M.A., A.M., M.S. were supported by Fundac¸ ˜ao para a Ciˆencia e a Tecnologia, with grants reference UIDB/00099/ 2020 and SFRH/BSAB/142940/2018 (P.G. only). A.D. and L.O. also acknowledge partial support from the Italian Ministry of Education, University and Research (MIUR) under the Departments of Excellence grant L.232/2016, and from the INFN grant InDark. G.J.W. gratefully acknowledges support of an Emeritus Fellowship from The Leverhulme Trust. EV is supported by Spanish grant PGC2018-101950-B-100. This research has made use of NASA’s Astrophysics Data System Bibliographic Services. Open access funding provided by Istituto Nazionale di Astrofisica within the CRUI-CARE Agreement., Sky survey telescopes and powerful targeted telescopes play complementary roles in astronomy. In order to investigate the nature and characteristics of the motions of very faint objects, a flexibly-pointed instrument capable of high astrometric accuracy is an ideal complement to current astrometric surveys and a unique tool for precision astrophysics. Such a space-based mission will push the frontier of precision astrometry from evidence of Earth-mass habitable worlds around the nearest stars, to distant Milky Way objects, and out to the Local Group of galaxies. As we enter the era of the JamesWebb Space Telescope and the new ground-based, adaptive-optics-enabled giant telescopes, by obtaining these high precision measurements on key objects that Gaia could not reach, a mission that focuses on high precision astrometry science can consolidate our theoretical understanding of the local Universe, enable extrapolation of physical processes to remote redshifts, and derive a much more consistent picture of cosmological evolution and the likely fate of our cosmos. Already several missions have been proposed to address the science case of faint objects in motion using high precision astrometry missions: NEAT proposed for the ESA M3 opportunity, micro-NEAT for the S1 opportunity, and Theia for the M4 and M5 opportunities. Additional new mission configurations adapted with technological innovations could be envisioned to pursue accurate measurements of these extremely small motions. The goal of this White Paper is to address the fundamental science questions that are at stake when we focus on the motions of faint sky objects and to briefly review instrumentation and mission profiles., NASA’s Virtual Planetary Laboratory NNA13AA93A, CFisUC strategic project (UID/FIS/04564/2019), Swiss National Science Foundation (SNSF), European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (COSMICLENS: grant agreement No. 787886), Polish National Science Centre (NCN) under Grant No. 2017/26/D/ST9/00591, Swedish National Space Agency (DNR 65/19, 174/18), Swedish National Space Agency (SNSA/Rymdstyrelsen), Portugese Fundacão para a Ciência e a Tecnologia (FCT) through the Strategic Programme UID/FIS/00099/2019 for CENTRA, Australian Research Council under grant FT190100814, Polish NCN grants: Harmonia No. 2018/06M/ST9/00311 and Daina No. 2017/27/L/ST9/03221, Italian Space Agency (ASI) under contracts 2014-025-R.1.2015 and 2018-24-HH.0, Italian Ministry of Foreign Affairs and International Cooperation (ASTRA), LabEx FOCUS ANR-11-LABX-0013, Spanish Ministry of Science, Innovation and University (MICIU/FEDER, UE) through grants RTI2018-095076-B-C21, ESP2016-80079-C2-1-R, Institute of Cosmos Sciences University of Barcelona (ICCUB, Unidad de Excelencia ’Mar´ıa de Maeztu’) through grants MDM-2014-0369 and CEX2019-000918-M, Fundacão para a Ciência e a Tecnologia, with grants reference UIDB/00099/ 2020 and SFRH/BSAB/142940/2018 (P.G. only), Italian Ministry of Education, University and Research (MIUR) under the Departments of Excellence grant L.232/2016, and from the INFN grant InDark, Emeritus Fellowship from The Leverhulme Trust, Spanish grant PGC2018-101950-B-100, Istituto Nazionale di Astrofisica within the CRUI-CARE Agreement
Published: 2021
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10. A global multinational survey of cefotaxime-resistant coliforms in urban wastewater treatment plants

Author: Yunho Lee, Manika Choudhury, Om Prakash, Donald Morrison, Hélène Guilloteau, Heidrun Mayrhofer, María Inmaculada Polo-López, Belen Esteban, Katarzyna Slipko, Leonardo Pantoja Munoz, Samira Nahim–Granados, José Manuel Guillén-Navarro, Marco Guida, Stela Krizanovic, Hemda Garelick, Pilar Caballero, Traore Ousmane, Marcos Quintela-Baluja, Sara Rodríguez-Mozaz, Helmut Bürgmann, Nikolina Udiković-Kolić, Carsten Ulrich Schwermer, Agnieszka Kalinowska, Milena Milaković, Ester Heath, Marta Piotrowska, Andrea Di Cesare, Célia M. Manaia, Ying Yang, Amy Pruden, Anne F.C. Leonard, Erica Donner, Tanel Telson, Christophe Merlin, Karin Beck, Ana Agüera, Anhony A Adegoke, Marie-Noëlle Pons, Bastian Herzog, Joana Abreu-Silva, Leonie Henn, Norbert Kreuzinger, Younggun Yoon, Stefanie Heß, Olga C. Nunes, Alice L. Petre, Despo Fatta-Kassinos, Gianluca Brunetti, Roberto B. M. Marano, Stella Michael, Thor A. Stenström, Ayella Maile-Moskowitz, Popi Karaolia, Joshua T. Bunce, Giovanni Libralato, Jérôme Ory, Yogesh Nimonkar, Alfieri Pollice, Aneta Luczkiewicz, Carlo Salerno, Andrew Scott, Shichun Zou, Antoni Oliver, Barbara Drigo, Isabel Martínez-Alcalá, Virginia Riquelme, Veljo Kisand, Anna Baraniak, William H. Gaze, Edward Topp, Edouard Jurkevitch, Isabel Henriques, Telma Fernandes, Eddie Cytryn, José Luis Balcázar, Marta Tacão, Thomas Schwartz, Thomas Jäger, Gianluca Corno, Mailis Laht, Thomas U. Berendonk, Roberto Rosal, Magdalena Popowska, Pawel Krzeminski, Connor L. Brown, Veritati - Repositório Institucional da Universidade Católica Portuguesa, Marano, R. B. M., Fernandes, T., Manaia, C. M., Nunes, O., Morrison, D., Berendonk, T. U., Kreuzinger, N., Telson, T., Corno, G., Fatta-Kassinos, D., Merlin, C., Topp, E., Jurkevitch, E., Henn, L., Scott, A., Hess, S., Slipko, K., Laht, M., Kisand, V., Di Cesare, A., Karaolia, P., Michael, S. G., Petre, A. L., Rosal, R., Pruden, A., Riquelme, V., Aguera, A., Esteban, B., Luczkiewicz, A., Kalinowska, A., Leonard, A., Gaze, W. H., Adegoke, A. A., Stenstrom, T. A., Pollice, A., Salerno, C., Schwermer, C. U., Krzeminski, P., Guilloteau, H., Donner, E., Drigo, B., Libralato, G., Guida, M., Burgmann, H., Beck, K., Garelick, H., Tacao, M., Henriques, I., Martinez-Alcala, I., Guillen-Navarro, J. M., Popowska, M., Piotrowska, M., Quintela-Baluja, M., Bunce, J. T., Polo-Lopez, M. I., Nahim-Granados, S., Pons, M. -N., Milakovic, M., Udikovic-Kolic, N., Ory, J., Ousmane, T., Caballero, P., Oliver, A., Rodriguez-Mozaz, S., Balcazar, J. L., Jager, T., Schwartz, T., Yang, Y., Zou, S., Lee, Y., Yoon, Y., Herzog, B., Mayrhofer, H., Prakash, O., Nimonkar, Y., Heath, E., Baraniak, A., Abreu-Silva, J., Choudhury, M., Munoz, L. P., Krizanovic, S., Brunetti, G., Maile-Moskowitz, A., Brown, C., Cytryn, E., The Robert H. Smith Faculty of Agriculture, Food and Environment, Department of Animal Sciences, The Hebrew University of Jerusalem (HUJ), Institute of Soil, Water and Environmental Sciences, Agricultural Research Organization - the Volcani Center, Centro de Química Fina e Biotecnologia (CQFB), Requimte, Universidade do Porto-Departamento de Química (DQ), Faculdade de Ciências e Tecnologia = School of Science & Technology (FCT NOVA), Universidade Nova de Lisboa = NOVA University Lisbon (NOVA)-Universidade Nova de Lisboa = NOVA University Lisbon (NOVA)-Faculdade de Ciências e Tecnologia = School of Science & Technology (FCT NOVA), Universidade Nova de Lisboa = NOVA University Lisbon (NOVA)-Universidade Nova de Lisboa = NOVA University Lisbon (NOVA)-Universidade do Porto-Departamento de Química (DQ), Universidade Nova de Lisboa = NOVA University Lisbon (NOVA)-Universidade Nova de Lisboa = NOVA University Lisbon (NOVA), Laboratory for Process Engineering, Environment, Biotechnology and Energy (LEPABE), Universidade do Porto, Edinburgh Napier University, Institute for Hydrobiology, Technische Universität Dresden = Dresden University of Technology (TU Dresden), Vienna University of Technology, Institute of Technology [Tartu, Estonia], University of Tartu, CNR Water Research Institute (IRSA), Consiglio Nazionale delle Ricerche (CNR), University of Cyprus (UCY), Laboratoire de Chimie Physique et Microbiologie pour les Matériaux et l'Environnement (LCPME), Institut de Chimie du CNRS (INC)-Université de Lorraine (UL)-Centre National de la Recherche Scientifique (CNRS), Agriculture and Agri-Food [Ottawa] (AAFC), Department of Biology, University of Western Ontario, University of Western Ontario (UWO), Estonian Environmental Research Centre (EKUK), Universidad de Alcalá - University of Alcalá (UAH), Virginia Tech [Blacksburg], Area de Quimica Inorganica - Centro de Investigacion en Energia Solar (CIESOL) (CIESOL), Universidad de Almería (UAL), Gdańsk University of Technology (GUT), University of Exeter Medical School, University of Exeter, Durban University of Technology, Universidad Nacional de Cuyo [Mendoza] (UNCUYO), Norwegian Institute for Water Research (NIVA), University of South Australia [Adelaide], Università degli studi di Napoli Federico II, Swiss Federal Insitute of Aquatic Science and Technology [Dübendorf] (EAWAG), Middlesex University [London], Universidade de Aveiro, Universidade de Coimbra [Coimbra], Universidad Católica San Antonio de Murcia (UCAM), Department of Applied Microbiology [Warsaw], Institute of Microbiology [Warsaw], Faculty of Biology [Warsaw], University of Warsaw (UW)-University of Warsaw (UW)-Faculty of Biology [Warsaw], University of Warsaw (UW)-University of Warsaw (UW), School of Engineering [Newcastle], Newcastle University [Newcastle], Plataforma Solar de Almeria – CIEMAT, Tabernas, Almeria, Laboratoire Réactions et Génie des Procédés (LRGP), Centre National de la Recherche Scientifique (CNRS)-Université de Lorraine (UL), Rudjer Boskovic Institute [Zagreb], Laboratoire Microorganismes : Génome et Environnement (LMGE), Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Centre National de la Recherche Scientifique (CNRS), CHU Clermont-Ferrand, Laboratorio EMATSA, Instituto Catalán de Investigación del Agua - ICRA (SPAIN) (ICRA), Institute of Functional Interfaces, Karlsruhe Institute of Technology (KIT), Sun Yat-Sen University [Guangzhou] (SYSU), Gwangju Institute of Science and Technology (GIST), Technische Universität Munchen - Université Technique de Munich [Munich, Allemagne] (TUM), NCMR, Jozef Stefan Institute [Ljubljana] (IJS), National Medicines Institute - Narodowy Instytut Leków [Warsaw] (NIL), Agricultural Research Organisation (ARO), Volcani Center, Universidade do Porto = University of Porto-Departamento de Química (DQ), Universidade Nova de Lisboa = NOVA University Lisbon (NOVA)-Universidade Nova de Lisboa = NOVA University Lisbon (NOVA)-Universidade do Porto = University of Porto-Departamento de Química (DQ), Universidade do Porto = University of Porto, National Research Council of Italy | Consiglio Nazionale delle Ricerche (CNR), University of Cyprus [Nicosia] (UCY), Agriculture and Agri-Food (AAFC), University of Naples Federico II = Università degli studi di Napoli Federico II, Université de Lorraine (UL)-Centre National de la Recherche Scientifique (CNRS), Marano, Robert BM, Fernandes, Telma, Manaia, Celia M, Nunes, Olga, Donner, Erica, Drigo, Barbara, Brunetti, Gianluca, and Cytryn, Eddie
Subjects: Cefotaxime, 010504 meteorology & atmospheric sciences, Coliforms, Antibiotic resistance, Sewage, Microorganismes -- Resistència als medicaments, Wastewater treatment, Wastewater, 010501 environmental sciences, 01 natural sciences, Surveys and Questionnaires, Microorganisms -- Drug resistance, ComputingMilieux_MISCELLANEOUS, lcsh:Environmental sciences, General Environmental Science, lcsh:GE1-350, 6. Clean water, Anti-Bacterial Agents, 3. Good health, Europe, Interdisciplinary Natural Sciences, Health, Sewage treatment, Biotechnology, medicine.drug, Life sciences, biology, Aigua -- Reutilització, Asia, Quantification methods, Aigües residuals -- Plantes de tractament, Culture and Communities, Water Purification, Applied microbiology, Water reuse, Environmental health, ddc:570, medicine, Microbiology Research Group, [SPI.GPROC]Engineering Sciences [physics]/Chemical and Process Engineering, antibiotic resistance, coliforms, ESBLs, wastewater treatment, wastewater reuse, Sewage disposal plants, Effluent, 0105 earth and related environmental sciences, [SDV.EE.SANT]Life Sciences [q-bio]/Ecology, environment/Health, Coliform, business.industry, Australia, Fecal coliform, Antibiotic resistance, Coliforms, ESBLs, Wastewater treatment, Water reuse, ESBL, North America, Environmental science, business
Abstract: The World Health Organization Global Action Plan recommends integrated surveillance programs as crucial strategies for monitoring antibiotic resistance. Although several national surveillance programs are in place for clinical and veterinary settings, no such schemes exist for monitoring antibiotic-resistant bacteria in the environment. In this transnational study, we developed, validated, and tested a low-cost surveillance and easy to implement approach to evaluate antibiotic resistance in wastewater treatment plants (WWTPs) by targeting cefotaxime-resistant (CTX-R) coliforms as indicators. The rationale for this approach was: i) coliform quantification methods are internationally accepted as indicators of fecal contamination in recreational waters and are therefore routinely applied in analytical labs; ii) CTX-R coliforms are clinically relevant, associated with extended-spectrum β-lactamases (ESBLs), and are rare in pristine environments. We analyzed 57 WWTPs in 22 countries across Europe, Asia, Africa, Australia, and North America. CTX-R coliforms were ubiquitous in raw sewage and their relative abundance varied significantly (
Published: 2020
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11. Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger S190814bv

Author: F. D'Ammando, Mattia Bulla, A. Fiore, P. T. O'Brien, Patricia Schady, T. Heikkilä, Matt Nicholl, Giorgos Leloudas, K. C. Chambers, Luciano Nicastro, Riccardo Ciolfi, Michela Mapelli, Armin Rest, R. Cutter, Tassilo Schweyer, J. Gillanders, G. De Cesare, Lorenzo Amati, L. Nuttal, Lána Salmon, Nancy Elias-Rosa, O. McBrien, A. Grado, David Alexander Kann, Ruben Salvaterra, P. D'Avanzo, M. T. Botticella, Johan P. U. Fynbo, M. G. Bernardini, Francesco Longo, Danny Steeghs, S. X. Yi, Peter G. Jonker, Eliana Palazzi, Y. D. Hu, Zhi-Ping Jin, Seppo Mattila, A. Gomboc, G. Ghirlanda, Alexis Coleiro, Sylvain Chaty, S. Yang, Elizabeth R. Stanway, D. R. Young, Rubina Kotak, Luca Izzo, Franz E. Bauer, Massimo Turatto, Christa Gall, A. Melandri, Eric Thrane, S. R. Oates, Francesca Onori, S. Srivastav, M. Branchesi, Michael S. Smith, Christopher W. Stubbs, Vincenzo Testa, Anders Jerkstrand, J. Japelj, Carlos González-Fernández, Elena Pian, Lluís Galbany, Luca Sbordone, Enrico Cappellaro, A. Possenti, Paul J. Groot, S. Rosetti, L. Denneau, Mark Kennedy, Jesper Sollerman, Klaas Wiersema, Chris M. Copperwheat, Cosimo Inserra, Kasper E. Heintz, E. C. Kool, M. de Pasquale, G. Greco, Krzysztof Ulaczyk, Daniel A. Perley, Om Sharan Salafia, Eugene A. Magnier, T. M. Reynolds, Andrew J. Levan, A. J. van der Horst, G. Stratta, B. Milvang-Jensen, Erkki Kankare, Darach Watson, B. Patricelli, N. B. Sabha, T. W. Chen, Kendall Ackley, Maria Letizia Pumo, Nial R. Tanvir, P. A. Evans, Michał J. Michałowski, S. Klose, R. L. C. Starling, A. J. Castro-Tirado, Sandra Savaglio, J. Quirola-Vásquez, Martin J. Dyer, Pietro Schipani, K. W. Smith, Lukasz Wyrzykowski, M. Della Valle, G. Pignata, S. D. Vergani, Jens Hjorth, A. S. B. Schultz, Mariusz Gromadzki, Saran Poshyachinda, Santiago González-Gaitán, Eugenio Maiorano, D. K. Galloway, Cesare Barbieri, V. D'Elia, Andrea Rossi, G. Ramsay, Seung-Lee Kim, Kornpob Bhirombhakdi, V. S. Dhillon, Enzo Brocato, Ilya Mandel, S. Benetti, J. D. Lyman, Sergio Campana, Fedor Getman, A. Sagués Carracedo, Kate Maguire, Arne Rau, A. S. Fruchter, John L. Tonry, B. P. Gompertz, Hanindyo Kuncarayakti, Kaj Wiik, Morgan Fraser, N. A. Walton, Stephan Rosswog, M. A.P. Torres, Claudia P. Gutiérrez, F. Ragosta, S. Piranomonte, A. Nicuesa Guelbenzu, S. H. Bruun, T. B. Lowe, M. E. Huber, S. J. Smartt, Gavin P. Lamb, S. Moran, Albino Perego, R. Eyles-Ferris, Stefano Covino, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia (INFN, Sezione di Perugia), Istituto Nazionale di Fisica Nucleare (INFN), INAF - Osservatorio Astronomico di Brera (OAB), Istituto Nazionale di Astrofisica (INAF), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Departamento de Astronomía y Astrofísica [Santiago], Pontificia Universidad Católica de Chile (UC), Instituto de Astrofísica de Andalucía (IAA), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Universitá degli Studi dell’Insubria = University of Insubria [Varese] (Uninsubria), Ecole Polytechnique Fédérale de Lausanne (EPFL), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, University of Sheffield [Sheffield], COBRA Research Institute, Eindhoven University of Technology, Aberystwyth University, AUTRES, Dark Cosmology Centre (DARK), Niels Bohr Institute [Copenhagen] (NBI), Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH)-Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH), Department of Physics [Pittsburgh], Carnegie Mellon University [Pittsburgh] (CMU), United States Geological Survey [Reston] (USGS), Faculty of Mathematics and Physics [Ljubljana] (FMF), University of Ljubljana, Department of Physics [Denver], University of Colorado [Denver], Laboratoire d'Acoustique de l'Université du Mans (LAUM), Le Mans Université (UM)-Centre National de la Recherche Scientifique (CNRS), Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome] (UNIROMA), Oskar Klein Centre [Stockholm], Stockholm University, SRON Netherlands Institute for Space Research (SRON), Astrophysics Research Centre [Belfast] (ARC), Queen's University [Belfast] (QUB), Finnish Centre for Astronomy with ESO (FINCA), University of Turku, Institut Lavoisier de Versailles (ILV), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS), Scottish Universities Physics Alliance, Institute for Astronomy (SUPA), University of Edinburgh, Department of Agricultural and Environmental Sciences – Production, Landscape, Agroenergy, Università degli Studi di Milano = University of Milan (UNIMI), Universidad Nacional de Entre Ríos [Argentine] (UNER), Istituto di Astrofisica Spaziale e Fisica Cosmica - Milano (IASF-MI), INAF - Osservatorio Astronomico di Roma (OAR), INAF - Osservatorio Astronomico di Cagliari (OAC), Max-Planck-Institut für Extraterrestrische Physik (MPE), Bioénergétique fondamentale et appliquée, Université Joseph Fourier - Grenoble 1 (UJF)-Institut National de la Santé et de la Recherche Médicale (INSERM), Università degli Studi di Milano-Bicocca = University of Milano-Bicocca (UNIMIB), University College Dublin [Dublin] (UCD), INAF-IASF Milano, Università della Calabria [Arcavacata di Rende] (Unical), INAF - Osservatorio Astronomico di Capodimonte (OAC), Woods Hole Oceanographic Institution (WHOI), National Institute of Water and Atmospheric Research [Wellington] (NIWA), Centre d'étude spatiale des rayonnements (CESR), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), University of Minnesota System, INAF - Osservatorio Astronomico di Padova (OAPD), Astronomical Observatory [Warsaw], Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), Astronomical Institute Anton Pannekoek (AI PANNEKOEK), University of Amsterdam [Amsterdam] (UvA), Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Institute of Astronomy [Cambridge], University of Cambridge [UK] (CAM), Department of Physics and Astronomy [Leicester], University of Leicester, UniVersity, Nano Science and Technology Program, Department of Chemistry, The Hong Kong UniVersity of Science and Technology, Clear Water Bay, Kowloon, Hong Kong, Hong Kong University of Science and Technology (HKUST), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Universitá degli Studi dell’Insubria, University of Copenhagen = Københavns Universitet (KU)-University of Copenhagen = Københavns Universitet (KU)-Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (KU)-University of Copenhagen = Københavns Universitet (KU), Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome], University of Milan, Università degli Studi di Milano-Bicocca [Milano] (UNIMIB), Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Université Fédérale Toulouse Midi-Pyrénées-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Ackley, K., Amati, L., Barbieri, C., Bauer, F. E., Benetti, S., Bernardini, M. G., Bhirombhakdi, K., Botticella, M. T., Branchesi, M., Brocato, E., Bruun, S. H., Bulla, M., Campana, S., Cappellaro, E., Castro-Tirado, A. J., Chambers, K. C., Chaty, S., Chen, T. -W., Ciolfi, R., Coleiro, A., Copperwheat, C. M., Covino, S., Cutter, R., D'Ammando, F., D'Avanzo, P., De Cesare, G., D'Elia, V., Della Valle, M., Denneau, L., De Pasquale, M., Dhillon, V. S., Dyer, M. J., Elias-Rosa, N., Evans, P. A., Eyles-Ferris, R. A. J., Fiore, A., Fraser, M., Fruchter, A. S., Fynbo, J. P. U., Galbany, L., Gall, C., Galloway, D. K., Getman, F. I., Ghirlanda, G., Gillanders, J. H., Gomboc, A., Gompertz, B. P., Gonzalez-Fernandez, C., Gonzalez-Gaitan, S., Grado, A., Greco, G., Gromadzki, M., Groot, P. J., Gutierrez, C. P., Heikkila, T., Heintz, K. E., Hjorth, J., Hu, Y. -D., Huber, M. E., Inserra, C., Izzo, L., Japelj, J., Jerkstrand, A., Jin, Z. P., Jonker, P. G., Kankare, E., Kann, D. A., Kennedy, M., Kim, S., Klose, S., Kool, E. C., Kotak, R., Kuncarayakti, H., Lamb, G. P., Leloudas, G., Levan, A. J., Longo, F., Lowe, T. B., Lyman, J. D., Magnier, E., Maguire, K., Maiorano, E., Mandel, I., Mapelli, M., Mattila, S., Mcbrien, O. R., Melandri, A., Michalowski, M. J., Milvang-Jensen, B., Moran, S., Nicastro, L., Nicholl, M., Nicuesa Guelbenzu, A., Nuttal, L., Oates, S. R., O'Brien, P. T., Onori, F., Palazzi, E., Patricelli, B., Perego, A., Torres, M. A. P., Perley, D. A., Pian, E., Pignata, G., Piranomonte, S., Poshyachinda, S., Possenti, A., Pumo, M. L., Quirola-Vasquez, J., Ragosta, F., Ramsay, G., Rau, A., Rest, A., Reynolds, T. M., Rosetti, S. S., Rossi, A., Rosswog, S., Sabha, N. B., Sagues Carracedo, A., Salafia, O. S., Salmon, L., Salvaterra, R., Savaglio, S., Sbordone, L., Schady, P., Schipani, P., Schultz, A. S. B., Schweyer, T., Smartt, S. J., Smith, K. W., Smith, M., Sollerman, J., Srivastav, S., Stanway, E. R., Starling, R. L. C., Steeghs, D., Stratta, G., Stubbs, C. W., Tanvir, N. R., Testa, V., Thrane, E., Tonry, J. L., Turatto, M., Ulaczyk, K., Van Der Horst, A. J., Vergani, S. D., Walton, N. A., Watson, D., Wiersema, K., Wiik, K., Wyrzykowski, L., Yang, S., Yi, S. -X., Young, D. R., National Aeronautics and Space Administration (US), University of Hawaii, Queen's University Belfast, Space Telescope Science Institute (US), National Research Foundation (South Africa), National Astronomical Research Institute of Thailand, University of Portsmouth, Instituto de Astrofísica de Canarias, Science and Technology Facilities Council (UK), Ministerio de Economía, Fomento y Turismo (Chile), Comisión Nacional de Investigación Científica y Tecnológica (Chile), Ministerio de Ciencia, Innovación y Universidades (España), European Commission, Danish National Research Foundation, Alexander von Humboldt Foundation, Villum Fonden, Fundação para a Ciência e a Tecnologia (Portugal), Polish National Agency for Academic Exchange, Centre National de la Recherche Scientifique (CNRS)-Le Mans Université (UM), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Low Energy Astrophysics (API, FNWI), and API Other Research (FNWI)
Subjects: Astronomy, ELECTROMAGNETIC COUNTERPARTS, Supernovae: general, general [Supernovae], Binary number, Astrophysics, 7. Clean energy, 01 natural sciences, GW170817, neutron, Supernovae: general [Gravitational waves, Stars], 010303 astronomy & astrophysics, QC, QB, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, astro-ph.HE, [PHYS]Physics [physics], HAWK-I, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], EJECTA, Astrophysics - Solar and Stellar Astrophysics, GRAVITATIONAL-WAVE SOURCE, ST/P000495/1, Space Science, Astrophysics - High Energy Astrophysical Phenomena, Gravitational wave, astro-ph.SR, astro-ph.GA, FOS: Physical sciences, Context (language use), MASS, NO, GAMMA-RAY BURST, Gravitational waves, 0103 physical sciences, ST/T007184/1, Solar and Stellar Astrophysics (astro-ph.SR), STFC, 010308 nuclear & particles physics, Near-infrared spectroscopy, KILONOVA, RCUK, Stars: neutron, Astronomy and Astrophysics, neutron [Stars], R-PROCESS NUCLEOSYNTHESIS, Astrophysics - Astrophysics of Galaxies, EVOLUTION, Black hole, Neutron star, Space and Planetary Science, [SDU]Sciences of the Universe [physics], Astrophysics of Galaxies (astro-ph.GA), ST/P000312/1, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Gravitational waves, Stars: neutron, Supernovae: general
Abstract: Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.--Full list of authors: Ackley, K.; Amati, L.; Barbieri, C.; Bauer, F. E.; Benetti, S.; Bernardini, M. G.; Bhirombhakdi, K.; Botticella, M. T.; Branchesi, M.; Brocato, E.; Bruun, S. H.; Bulla, M.; Campana, S.; Cappellaro, E.; Castro-Tirado, A. J.; Chambers, K. C.; Chaty, S.; Chen, T. -W.; Ciolfi, R.; Coleiro, A.; Copperwheat, C. M.; Covino, S.; Cutter, R.; D'Ammando, F.; D'Avanzo, P.; De Cesare, G.; D'Elia, V.; Della Valle, M.; Denneau, L.; De Pasquale, M.; Dhillon, V. S.; Dyer, M. J.; Elias-Rosa, N.; Evans, P. A.; Eyles-Ferris, R. A. J.; Fiore, A.; Fraser, M.; Fruchter, A. S.; Fynbo, J. P. U.; Galbany, L.; Gall, C.; Galloway, D. K.; Getman, F. I.; Ghirlanda, G.; Gillanders, J. H.; Gomboc, A.; Gompertz, B. P.; González-Fernández, C.; González-Gaitán, S.; Grado, A.; Greco, G.; Gromadzki, M.; Groot, P. J.; Gutiérrez, C. P.; Heikkilä, T.; Heintz, K. E.; Hjorth, J.; Hu, Y. -D.; Huber, M. E.; Inserra, C.; Izzo, L.; Japelj, J.; Jerkstrand, A.; Jin, Z. P.; Jonker, P. G.; Kankare, E.; Kann, D. A.; Kennedy, M.; Kim, S.; Klose, S.; Kool, E. C.; Kotak, R.; Kuncarayakti, H.; Lamb, G. P.; Leloudas, G.; Levan, A. J.; Longo, F.; Lowe, T. B.; Lyman, J. D.; Magnier, E.; Maguire, K.; Maiorano, E.; Mandel, I.; Mapelli, M.; Mattila, S.; McBrien, O. R.; Melandri, A.; Michałowski, M. J.; Milvang-Jensen, B.; Moran, S.; Nicastro, L.; Nicholl, M.; Nicuesa Guelbenzu, A.; Nuttal, L.; Oates, S. R.; O'Brien, P. T.; Onori, F.; Palazzi, E.; Patricelli, B.; Perego, A.; Torres, M. A. P.; Perley, D. A.; Pian, E.; Pignata, G.; Piranomonte, S.; Poshyachinda, S.; Possenti, A.; Pumo, M. L.; Quirola-Vásquez, J.; Ragosta, F.; Ramsay, G.; Rau, A.; Rest, A.; Reynolds, T. M.; Rosetti, S. S.; Rossi, A.; Rosswog, S.; Sabha, N. B.; Sagués Carracedo, A.; Salafia, O. S.; Salmon, L.; Salvaterra, R.; Savaglio, S.; Sbordone, L.; Schady, P.; Schipani, P.; Schultz, A. S. B.; Schweyer, T.; Smartt, S. J.; Smith, K. W.; Smith, M.; Sollerman, J.; Srivastav, S.; Stanway, E. R.; Starling, R. L. C.; Steeghs, D.; Stratta, G.; Stubbs, C. W.; Tanvir, N. R.; Testa, V.; Thrane, E.; Tonry, J. L.; Turatto, M.; Ulaczyk, K.; van der Horst, A. J.; Vergani, S. D.; Walton, N. A.; Watson, D.; Wiersema, K.; Wiik, K.; Wyrzykowski, Ł.; Yang, S.; Yi, S. -X.; Young, D. R., Context. Gravitational wave (GW) astronomy has rapidly reached maturity, becoming a fundamental observing window for modern astrophysics. The coalescences of a few tens of black hole (BH) binaries have been detected, while the number of events possibly including a neutron star (NS) is still limited to a few. On 2019 August 14, the LIGO and Virgo interferometers detected a high-significance event labelled S190814bv. A preliminary analysis of the GW data suggests that the event was likely due to the merger of a compact binary system formed by a BH and a NS. Aims. In this paper, we present our extensive search campaign aimed at uncovering the potential optical and near infrared electromagnetic counterpart of S190814bv. We found no convincing electromagnetic counterpart in our data. We therefore use our non-detection to place limits on the properties of the putative outflows that could have been produced by the binary during and after the merger. Methods. Thanks to the three-detector observation of S190814bv, and given the characteristics of the signal, the LIGO and Virgo Collaborations delivered a relatively narrow localisation in low latency - a 50% (90%) credible area of 5 deg2 (23 deg2) - despite the relatively large distance of 267 ± 52 Mpc. ElectromagNetic counterparts of GRAvitational wave sources at the VEry Large Telescope collaboration members carried out an intensive multi-epoch, multi-instrument observational campaign to identify the possible optical and near infrared counterpart of the event. In addition, the ATLAS, GOTO, GRAWITA-VST, Pan-STARRS, and VINROUGE projects also carried out a search on this event. In this paper, we describe the combined observational campaign of these groups. Results. Our observations allow us to place limits on the presence of any counterpart and discuss the implications for the kilonova (KN), which was possibly generated by this NS-BH merger, and for the strategy of future searches. The typical depth of our wide-field observations, which cover most of the projected sky localisation probability (up to 99.8%, depending on the night and filter considered), is r ∼ 22 (resp. K ∼ 21) in the optical (resp. near infrared). We reach deeper limits in a subset of our galaxy-targeted observations, which cover a total ∼50% of the galaxy-mass-weighted localisation probability. Altogether, our observations allow us to exclude a KN with large ejecta mass M 0.1 M- to a high (> 90%) confidence, and we can exclude much smaller masses in a sub-sample of our observations. This disfavours the tidal disruption of the neutron star during the merger. Conclusions. Despite the sensitive instruments involved in the campaign, given the distance of S190814bv, we could not reach sufficiently deep limits to constrain a KN comparable in luminosity to AT 2017gfo on a large fraction of the localisation probability. This suggests that future (likely common) events at a few hundred megaparsecs will be detected only by large facilities with both a high sensitivity and large field of view. Galaxy-targeted observations can reach the needed depth over a relevant portion of the localisation probability with a smaller investment of resources, but the number of galaxies to be targeted in order to get a fairly complete coverage is large, even in the case of a localisation as good as that of this event. © K. Ackley et al. 2020., Based on observations collected at the European Southern Observatory under ESO programmes 1102.D-0353(E), 1102.D0353(F), 1102.D-0353(Q), 1102.D-0353(G), 0103.D-0070(A), 0103.D-0070(B), 0103.D-0703(A), 0103.D-0722(A), 0103.A-9099(A), 198.D-2010(D) and 60.A9285(A). ATLAS is primarily funded through NEO NASA grants NN12AR55G, 80NSSC18K0284, and 80NSSC18K1575. The ATLAS science products have been made possible through the contributions of the University of Hawaii IfA, the Queen's University Belfast, the Space Telescope Science Institute, and the South African Astronomical Observatory. PanSTARRS is primarily funded through NEO NASA grants NASA Grants NNX08AR22G, NNX14AM74G. The PanSTARRS science products for LIGO-Virgo follow-up are made possible through the contributions of the University of Hawaii IfA and the Queen's University Belfast. The Gravitational-wave Optical Transient Observer (GOTO) project acknowledges the support of the Monash-Warwick Alliance; Warwick University; Monash University; She ffield University; Leicester University; Armagh Observatory & Planetarium; the National Astronomical Research Institute of Thailand (NARIT); University of Portsmouth; Turku University and the Instituto de Astrofisica de Canarias (IAC). Part of the funding for GROND was generously granted from the Leibniz-Prize to Prof. G. Hasinger (DFG grant HA 1850/28-1). The Liverpool Telescope is operated on the island of La Palma by Liverpool John Moores University in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias with financial support from the UK Science and Technology Facilities Council. The WHT and its override programme are operated on the island of La Palma by the Isaac Newton Group of Telescopes in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias; part of these data were taken under program (19A)N3. FEB thanks CONICYT Basal AFB-170002 and Chile's Ministry of Economy fund IC120009. MGB, PDA and AM acknowledge support from ASI grant I/004/11/3. MBr, EC, AP and SPi acknowledge support from MIUR (PRIN 2017 grant 20179ZF5KS). EB, EM and MT acknowledge funding from GRAWITA. SHB is indebted to the Danish National Research Foundation (DNRF132) for support. SCa acknowledges support from grant MAE0065741. EC acknowledges the support of the H2020 OPTICON programme 730890. TWC acknowledges the Humboldt Foundation and Marie Sklodowska-Curie grant 842471. MDP thanks Istanbul University for support. PAE acknowledges UKSA support. RAJEF is supported by an STFC studentship. MF is supported by a Royal Society -SFI University Research Fellowship. LG was funded by the EU H2020 programme under MSCA grant no. 839090. CG, JH and LI were supported by a research grant from VILLUM FONDEN (project 16599). CG and LI were supported by a research grant from VILLUM FONDEN (25501). GGh acknowledges the PRIN MIUR "Figaro" for financial support. AGo acknowledges financial support from the Slovenian Research Agency (grants P1-0031, I0-0033, and J1-8136). BPG, AJL and JDL acknowledge support from ERC grant 725246 (TEDE, PI Levan). SGG acknowledges support by FCT Fundacao para a Ciencia e Tecnologia and by Project PTDC/FIS-AST-31546. GGr acknowledges the ESCAPE H2020 project no. 824064. MG is supported by the Polish NCN MAESTRO grant 2014/14/A/ST9/00121. PJG acknowledges support from NOVA and from the South African NRF SARChI grant 111692. CPG and MS acknowledge support from EU/FP7-ERC grant no. 615929. KEH acknowledges support by a Project Grant from The Icelandic Research Fund. YDH acknowledges support from the China Scholarships Council. JJ acknowledges support from NOVA and NWO-FAPESP grant for instrumentation. AJ acknowledges funding from the European Research Council (ERC). ZPJ was supported by the Foundation for Distinguished Young Scholars of Jiangsu Province (no. BK20180050). PGJ acknowledges funding from the ERC under Consolidator Grant agreement no. 647208. DAK acknowledges Spanish research project RTI2018-098104-J-I00 (GRBPhot). SKl acknowledges support by DFG grant Kl 766/16-3. ECK acknowledges support from the GREAT research environment. GPL acknowledges support from STFC via grant ST/N000757/1. GL was supported by a research grant (19054) from VILLUM FONDEN. KM acknowledges support from the ERC (grant no. 758638). IM is partially supported by OzGrav (ARC project CE17010000). MMacknowledges support from ERC through ERC-2017-CoG no. 770017. MJM acknowledges the National Science Centre, Poland, grant 2018/30/E/ST9/00208. BMJ and DW are supported by Independent Research Fund Denmark grant DFF-7014-00017. MN is supported by a Royal Astronomical Society Research Fellowship. ANG acknowledges support by grant DFG Kl 766/16-3. PTOB acknowledges funding from STFC. SRO gratefully acknowledges the support of the Leverhulme Trust. FO acknowledges the support of the H2020 Hemera program, grant no. 730970. MAPT was supported by grants RYC-2015-17854 and AYA201783216-P. EP aknowledges financial support from INAF. GP is supported by the Millennium Science Initiative through grant IC120009. MLP is partially supported by a "Linea 2" project of the Catania University. JQV acknowledges support from CONICYT folio 21180886. TMR acknowledges the support of the Vilho, Yrjo and Kalle Vaisala Foundation. ARo acknowledges support from Premiale LBT 2013. SR is supported by VR grants 2016-03657_3 and the research environment grant GREAT, Dnr. 2016-06012, and the Swedish National Space board, Dnr. 107/16. OSS acknowledges the Italian Ministry of Research (MIUR) grant 1.05.06.13. LSa acknowledges the Irish Research Council Scholarship no. GOIPG/2017/1525. SJS acknowledges support from STFC Grant ST/P000312/1. ERS and DS acknowledge funding from UK STFC CG ST/P000495/1. RLCS acknowledges funding from STFC. DS acknowledges support from STFC via grant ST/T007184/1. SDV acknowledges the support of the CNES. LWsupported by Polish NCN DAINA 2017/27/L/ST9/03221. The Cosmic DAWN center is funded by the Danish National Research Foundation.
Published: 2020
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12. Magnetoelastic interaction in the two-dimensional magnetic material MnPS3 studied by first principles calculations and Raman experiments

Author: Alex Delhomme, Clément Faugeras, Andrés Saúl, Benoit Grémaud, Marek Potemski, Jan Suffczyński, Andrew R Wildes, A. Bogucki, Diana Vaclavkova, Piotr Kossacki, Laboratoire national des champs magnétiques intenses - Grenoble (LNCMI-G ), Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Institut National des Sciences Appliquées - Toulouse (INSA Toulouse), Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées, Institute of Experimental Physics [Warsaw] (IFD), Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), Institut Laue-Langevin (ILL), ILL, Centre de Physique Théorique - UMR 7332 (CPT), Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), CPT - E6 Nanophysique, Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS)-Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Centre Interdisciplinaire de Nanoscience de Marseille (CINaM), Aix Marseille Université (AMU)-Centre National de la Recherche Scientifique (CNRS), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), and Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)
Subjects: Materials science, Magnetism, Phonon, FOS: Physical sciences, 02 engineering and technology, 01 natural sciences, Condensed Matter - Strongly Correlated Electrons, Paramagnetism, symbols.namesake, 0103 physical sciences, Mesoscale and Nanoscale Physics (cond-mat.mes-hall), Antiferromagnetism, General Materials Science, [PHYS.COND]Physics [physics]/Condensed Matter [cond-mat], 010306 general physics, Condensed Matter - Mesoscale and Nanoscale Physics, Condensed matter physics, Strongly Correlated Electrons (cond-mat.str-el), [PHYS.PHYS]Physics [physics]/Physics [physics], Heisenberg model, Mechanical Engineering, General Chemistry, 021001 nanoscience & nanotechnology, Condensed Matter Physics, Mechanics of Materials, symbols, Density functional theory, Condensed Matter::Strongly Correlated Electrons, 0210 nano-technology, Raman spectroscopy, Raman scattering
Abstract: We report experimental and theoretical studies on the magnetoelastic interactions in MnPS$_3$. Raman scattering response measured as a function of temperature shows a blue shift of the Raman active modes at 120.2 and 155.1 cm$^{-1}$, when the temperature is raised across the antiferromagnetic-paramagnetic transition. Density functional theory (DFT) calculations have been performed to estimate the effective exchange interactions and calculate the Raman active phonon modes. The calculations lead to the conclusion that the peculiar behavior with temperature of the two low energy phonon modes can be explained by the symmetry of their corresponding normal coordinates which involve the virtual modification of the super-exchange angles associated with the leading antiferromagnetic (AFM) interactions., Comment: Main: 9 pages, 7 figures. Supplementary : 5 pages, 4 figures
Published: 2020
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13. Time-dependent shapes of a dissolving mineral grain: Comparisons of simulations with microfluidic experiments

Author: Piotr Szymczak, Vitaliy Starchenko, Anthony J. C. Ladd, Florian Osselin, Silvana Magni, Filip Dutka, Institute of Theoretical Physics [Warsaw], Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), Oak Ridge National Laboratory [Oak Ridge] (ORNL), UT-Battelle, LLC, Institut des Sciences de la Terre d'Orléans - UMR7327 (ISTO), Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Bureau de Recherches Géologiques et Minières (BRGM) (BRGM), Milieux Poreux - UMR7327, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Bureau de Recherches Géologiques et Minières (BRGM) (BRGM)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), University of Florida [Gainesville] (UF), Institute of Theoretical Physics, University of Warsaw (UW), Bureau de Recherches Géologiques et Minières (BRGM) (BRGM)-Observatoire des Sciences de l'Univers en région Centre (OSUC), PSL Research University (PSL)-PSL Research University (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Bureau de Recherches Géologiques et Minières (BRGM) (BRGM)-Observatoire des Sciences de l'Univers en région Centre (OSUC), and University of Florida [Gainesville]
Subjects: Dissolution rate, Gypsum, 010504 meteorology & atmospheric sciences, Gypsum dissolution, Flow (psychology), Microfluidics, Reactive surface area, Flux, Geology, Radius, Mechanics, engineering.material, 010502 geochemistry & geophysics, Pore scale modeling, 01 natural sciences, Boundary layer, Reaction rate constant, Geochemistry and Petrology, [SDU]Sciences of the Universe [physics], engineering, Dissolution, Simulation and experiment, 0105 earth and related environmental sciences
Abstract: International audience; Experimental observations of the dissolution of calcium sulfate by flowing water have been used to investigate the assumptions underlying pore-scale models of reactive transport. Microfluidic experiments were designed to observe changes in size and shape as cylindrical disks (radius 10 mm) of gypsum dissolved for periods of up to 40 days. The dissolution flux over the whole surface of the sample can be determined by observing the motion of the interface. However, in order to extract surface reaction rates, numerical simulations are required to account for diffusional hindrance across the concentration boundary layer; the geometry is too complex for analytic solutions.We have found that a first-principles simulation of pore-scale flow and transport, with a single value of the surface reaction rate, was able to reproduce the time sequence of sample shapes without any fitting parameters. The value of the rate constant is close to recent experimental measurements but much smaller than some earlier values. The shape evolution is a more stringent test of the validity of the method than average measurements such as effluent concentration, because it requires the correct flux at each point on the sample surface.
Published: 2020
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14. GaiaNIR: Combining optical and Near-Infra-Red (NIR) capabilities with Time-Delay-Integration (TDI) sensors for a future Gaia-like mission

Author: Hobbs, David, Høg, Erik, Mora, Alcione, Crowley, Cian, Mcmillan, Paul, Ranalli, Piero, Heiter, Ulrike, Jordi, Carme, Hambly, Nigel, Church, Ross, Anthony, Brown, Tanga, Paolo, Chemin, Laurent, Portail, Jordi, Jiménez-Esteban, Fran, Klioner, Sergei, Mignard, François, Fynbo, Johan, Wyrzykowski, Łukasz, Rybicki, Krzysztof, Anderson, Richard I., Cellino, Alberto, Fabricius, Claus, Davidson, Michael, Lindegren, Lennart, Fernandez Trincado, Jose Gregorio, Department of Chemistry, UCL, Christopher Ingold Laboratories, Uppsala University, Laboratoire de Cosmologie, Astrophysique Stellaire & Solaire, de Planétologie et de Mécanique des Fluides (CASSIOPEE), Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Centre d'Etude et de Recherches en Géodynamique et Astronomie (CERGA), Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Astronomical Observatory [Warsaw], Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), INAF - Osservatorio Astrofisico di Torino (OATo), Istituto Nazionale di Astrofisica (INAF), Open University of Israël, Univers, Transport, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UMR 6213) (UTINAM), Université de Franche-Comté (UFC), and Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: ESA recently called for new "Science Ideas" to be investigated in terms of feasibility and technological developments -- for technologies not yet sufficiently mature. These ideas may in the future become candidates for M or L class missions within the ESA Science Program. With the launch of Gaia in December 2013, Europe entered a new era of space astrometry following in the footsteps of the very successful Hipparcos mission from the early 1990s. Gaia is the successor to Hipparcos, both of which operated in optical wavelengths, and Gaia is two orders of magnitude more accurate in the five astrometric parameters and is surveying four orders of magnitude more stars in a vast volume of the Milky Way. The combination of the Hipparcos/Tycho-2 catalogues with the first early Gaia data release will give improved proper motions over a long ~25 year baseline. The final Gaia solution will also establish a new optical reference frame by means of quasars, by linking the optical counterparts of radio (VLBI) sources defining the orientation of the reference frame, and by using the zero proper motion of quasars to determine a non-rotating frame. A weakness of Gaia is that it only operates at optical wavelengths. However, much of the Galactic centre and the spiral arm regions, important for certain studies, are obscured by interstellar extinction and this makes it difficult for Gaia to deeply probe. Traditionally, this problem is overcome by switching to the infra-red but this was not possible with Gaia's CCDs. Additionally, to scan the entire sky and make global absolute parallax measurements the spacecraft must have a constant rotation and this requires that the CCDs operate in TDI mode, increasing their complexity.
Published: 2020

15. Similar factors underlie tree abundance in forests in native and alien ranges

Author: Florian Jansen, Robert K. Peet, Marco Moretti, Erwin Bergmeier, Brody Sandel, Cyrille Violle, Franz Essl, Holger Kreft, Ute Jandt, Michele De Sanctis, Masha T. van der Sande, Alvaro G. Gutiérrez, Helge Bruelheide, Marten Winter, Mária Šibíková, Thomas Wohlgemuth, Richard Field, Koen Kramer, Timothy J. S. Whitfeld, Marco Schmidt, Petr Pyšek, Fabio Attorre, Jan Pergl, Milan Chytrý, Peter B. Reich, Tiffany M. Knight, Oliver Purschke, Borja Jiménez-Alfaro, Stefan Klotz, Jens Kattge, Mark van Kleunen, Joern Pagel, Greg R. Guerin, Petr Petřík, Matteo Dainese, Valentin Golub, Wayne Dawson, Sylvia Haider, Ülo Niinemets, Jaime Fagúndez, Jürgen Dengler, Josep Peñuelas, Elizabeth Kearsley, Patrick Weigelt, Isabelle Aubin, Ecosystem and Landscape Dynamics (IBED, FNWI), Martin-Luther-Universität Halle Wittenberg (MLU), Department of Ecology, University of Warsaw (UW), Universität Bayreuth, Umweltbundesamt, University of Nottingham, UK (UON), Department of Biodiversity, Macroecology and Biogeography, Georg-August-Universität Göttingen, Inst. Biochem. & Biol., University of Potsdam, Institute of Botany, Czech Academy of Sciences [Prague] (ASCR), Martin-Luther-University Halle-Wittenberg, German Centre for Integrative Biodiversity Research, Masaryk University, Royal Institute of Technology (KTH), Department of Microelectronics and Information Technology, Kista Photonics Research Center (KPRC) (KTH), Royal Institute of Technology [Stockholm] (KTH ), Laboratoire d'hydrodynamique (LadHyX), École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Philips Research Europe - Hamburg, Sector Medical Imaging Systems, Philips Research, Max Planck Institute for Biogeochemistry (MPI-BGC), Max-Planck-Gesellschaft, Institut für Geowissenschaften, Eberhard Karls Universität Tübingen, Wageningen University and Research Centre [Wageningen] (WUR), Institute of Agricultural and Environmental Sciences, Estonian University of Life Sciences, Centre de Recerca Ecològica i Aplicacions Forestals (CREAF), Department of Forest Resources, University of Minnesota [Twin Cities], University of Minnesota System-University of Minnesota System, Centre d’Ecologie Fonctionnelle et Evolutive (CEFE), Université Paul-Valéry - Montpellier 3 (UM3)-Institut National de la Recherche Agronomique (INRA)-Centre international d'études supérieures en sciences agronomiques (Montpellier SupAgro)-École pratique des hautes études (EPHE)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud])-Institut national d’études supérieures agronomiques de Montpellier (Montpellier SupAgro), Swiss Federal Research Institute, Department of Ecology [Warsaw], Institute of Zoology [Warsaw], Faculty of Biology [Warsaw], University of Warsaw (UW)-University of Warsaw (UW)-Faculty of Biology [Warsaw], University of Warsaw (UW)-University of Warsaw (UW), Georg-August-University [Göttingen], Czech Academy of Sciences [Prague] (CAS), Masaryk University [Brno] (MUNI), Eberhard Karls Universität Tübingen = Eberhard Karls University of Tuebingen, Wageningen University and Research [Wageningen] (WUR), Estonian University of Life Sciences (EMU), University of Minnesota [Twin Cities] (UMN), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-École pratique des hautes études (EPHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre international d'études supérieures en sciences agronomiques (Montpellier SupAgro)-Institut National de la Recherche Agronomique (INRA)-Université Paul-Valéry - Montpellier 3 (UPVM)-Institut national d’études supérieures agronomiques de Montpellier (Montpellier SupAgro), and Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro)-Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro)-Institut de Recherche pour le Développement (IRD [France-Sud])
Subjects: 0106 biological sciences, Plant invasion, Introduced species, 01 natural sciences, Invasive species, Trees, forest, Abundance, Abundance (ecology), functional traits, Macroecology, ComputingMilieux_MISCELLANEOUS, 2. Zero hunger, Global and Planetary Change, abundance, Ecology, dissimilarity, global, plant invasion, trees, Global, PE&RC, Research Papers, 580: Pflanzen (Botanik), Habitat, [SDE]Environmental Sciences, Technologie and Innovatie, Knowledge Technology and Innovation, Kennis, Functional traits, Research Paper, Biogeography, Alien, Biology, 010603 evolutionary biology, tree abundance, forsts, ddc:570, Bosecologie en Bosbeheer, Forest, 577: Ökologie, Relative species abundance, Ecology, Evolution, Behavior and Systematics, 010604 marine biology & hydrobiology, 15. Life on land, Forest Ecology and Forest Management, abundance, dissimilarity, forest, functional traits, global, plant invasion, trees, Dissimilarity, [SDE.BE]Environmental Sciences/Biodiversity and Ecology, Biological invasion, Kennis, Technologie and Innovatie
Abstract: Netherlands Organisation for Scientific Research (NWO), Grant/Award Number: 019.171LW.023; German Research Foundation; German Research Foundation DFG, Grant/Award Number: 264740629; FONDECYT, Grant/Award Number: 11150835; CONICYT-PAI, Grant/Award Number: 82130046; 7th European Community Framework Programme, Grant/Award Number: FORECOFUN-SSA PIEF-GA-2010–274798; European Research Council Synergy, Grant/Award Number: ERC-SyG-2013-610028; Austrian Science Foundation, Grant/Award Number: I2086-B16; Czech Science Foundation, Centre of Excellence PLADIAS, Grant/Award Number: 14-15414S and RVO 67985939; EXPRO, Grant/Award Number: 19-28807X; VEGA, Grant/Award Number: 0051/1, van der Sande, M.T., Bruelheide, H., Dawson, W., Dengler, J., Essl, F., Field, R., Haider, S., van Kleunen, M., Kreft, H., Pagel, J., Pergl, J., Purschke, O., Pyšek, P., Weigelt, P., Winter, M., Attorre, F., Aubin, I., Bergmeier, E., Chytrý, M., Dainese, M., De Sanctis, M., Fagundez, J., Golub, V., Guerin, G.R., Gutiérrez, A.G., Jandt, U., Jansen, F., Jiménez-Alfaro, B., Kattge, J., Kearsley, E., Klotz, S., Kramer, K., Moretti, M., Niinemets, Ü., Peet, R.K., Penuelas, J., Petřík, P., Reich, P.B., Sandel, B., Schmidt, M., Sibikova, M., Violle, C., Whitfeld, T.J.S., Wohlgemuth, T., Knight, T.M.
Published: 2020
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16. Quasi-polynomial time approximation schemes for the Maximum Weight Independent Set Problem in H -free graphs

Author: Maria Chudnovsky, Marcin Pilipczuk, Michał Pilipczuk, Stéphan Thomassé, Department of Mathematics - Princeton University, Princeton University, Institute of Informatics [Warsaw], Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), University of Warsaw (UW)-University of Warsaw (UW), Institut Universitaire de France (IUF), Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.), Modèles de calcul, Complexité, Combinatoire (MC2), Laboratoire de l'Informatique du Parallélisme (LIP), École normale supérieure - Lyon (ENS Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Recherche en Informatique et en Automatique (Inria)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Lyon (ENS Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Recherche en Informatique et en Automatique (Inria)-Centre National de la Recherche Scientifique (CNRS), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), and Université de Lyon-Université de Lyon-Institut National de Recherche en Informatique et en Automatique (Inria)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL)
Subjects: FOS: Computer and information sciences, Discrete Mathematics (cs.DM), 010201 computation theory & mathematics, Computer Science - Data Structures and Algorithms, [INFO.INFO-DS]Computer Science [cs]/Data Structures and Algorithms [cs.DS], 0202 electrical engineering, electronic engineering, information engineering, Data Structures and Algorithms (cs.DS), 020206 networking & telecommunications, 0102 computer and information sciences, 02 engineering and technology, 01 natural sciences, ComputingMilieux_MISCELLANEOUS, Computer Science - Discrete Mathematics
Abstract: In the Maximum Independent Set problem we are asked to find a set of pairwise nonadjacent vertices in a given graph with the maximum possible cardinality. In general graphs, this classical problem is known to be NP-hard and hard to approximate within a factor of $n^{1-\varepsilon}$ for any $\varepsilon > 0$. Due to this, investigating the complexity of Maximum Independent Set in various graph classes in hope of finding better tractability results is an active research direction. In $H$-free graphs, that is, graphs not containing a fixed graph $H$ as an induced subgraph, the problem is known to remain NP-hard and APX-hard whenever $H$ contains a cycle, a vertex of degree at least four, or two vertices of degree at least three in one connected component. For the remaining cases, where every component of $H$ is a path or a subdivided claw, the complexity of Maximum Independent Set remains widely open, with only a handful of polynomial-time solvability results for small graphs $H$ such as $P_5$, $P_6$, the claw, or the fork. We show that for every graph $H$ for which Maximum Independent Set is not known to be APX-hard and SUBEXP-hard in $H$-free graphs, the problem admits a quasi-polynomial time approximation scheme and a subexponential-time exact algorithm in this graph class. Our algorithm works also in the more general weighted setting, where the input graph is supplied with a weight function on vertices and we are maximizing the total weight of an independent set., v2: added results on subexponential algorithms
Published: 2020
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17. Full orbital solution for the binary system in the northern Galactic disk microlensing event Gaia16aye

Author: Wyrzykowski, Ł., D’Ago, G., Hanlon, L., van Heerden, H., Ihanec, N., Jovanovic, M., Kopacki, G., Martin-Carrillo, A., Marais, J., Meintjes, P., Murphy, D., Van Soelen, B., Strubble, E., Szegedi, H., Vernet, D., Vince, O., van der Westhuizen, I., Wium, D., Zhuchkov, R. Ya., Wyrzykowski, Łukasz, Mróz, P., Rybicki, K., Gromadzki, M., Kołaczkowski, Z., Zieliński, M., Zieliński, P., Britavskiy, N., Gomboc, A., Sokolovsky, K., Hodgkin, S., Abe, L., Aldi, G., AlMannaei, A., Altavilla, G., Al Qasim, A., Anupama, G., Awiphan, S., Bachelet, E., Bakış, V., Baker, S., Bartlett, S., Bendjoya, P., Benson, K., Bikmaev, I., Birenbaum, G., Blagorodnova, N., Blanco-Cuaresma, S., Boeva, S., Bonanos, A., Bozza, V., Bramich, D., Bruni, I., Burenin, R., Burgaz, U., Butterley, T., Caines, H., Caton, D., Calchi Novati, S., Carrasco, J., Cassan, A., Čepas, V., Cropper, M., Chruślińska, M., Clementini, G., Clerici, A., Conti, D., Conti, M., Cross, S., Cusano, F., Damljanovic, G., Dapergolas, A., D'ago, G, de Bruijne, J., Dennefeld, M., Dhillon, V., Dominik, M., Dziedzic, J., Erece, O., Eselevich, M., Esenoglu, H., Eyer, L., Figuera Jaimes, R., Fossey, S., Galeev, A., Grebenev, S., Gupta, A., Gutaev, A., Hallakoun, N., Hamanowicz, A., Han, C., Handzlik, B., Haislip, J., Hardy, L., Harrison, D., Hoette, V., Horne, K., Hudec, R., Hundertmark, M., Ihanec 35, N, Irtuganov, E., Itoh, R., Iwanek, P., Janulis, R., Jelínek, M., Jensen, E., Kaczmarek, Z., Katz, D., Khamitov, I., Kilic, Y., Klencki, J., Kolb, U., Kouprianov, V., Kruszyńska, K., Kurowski, S., Latev, G., Lee, C.-H., Leonini, S., Leto, G., Lewis, F., Li, Z., Liakos, A., Littlefair, S., Lu, J., Manser, C., Mao, S., Maoz, D., Maskoliūnas, M., Maund, J., Melnikov, S., Ment, K., Mikołajczyk, P., Morrell, M., Mowlavi, N., Moździerski, D., Nazarov, S., Netzel, H., Nesci, R., Ngeow, C.-C., Norton, A., Ofek, E., Pakštienė, E., Palaversa, L., Pandey, A., Paraskeva, E., PAWLAK, M., Penny, M., Penprase, B., Piascik, A., Prieto, J., Qvam, J., Ranc, C., Rebassa-Mansergas, A., Reichart, D., Reig, P., Rhodes, L., Rivet, J.-P., Rixon, G., Roberts, D., Rosi, P., Russell, D., Zanmar Sanchez, R., Scarpetta, G., Seabroke, G., Shappee, B., Schmidt, R., Shvartzvald, Y., Sitek, M., Skowron, J., Śniegowska, M., Snodgrass, C., Soares, P., Spetsieri, Z., Stankevičiūtė, A., Steele, I., Street, R., Strobl, J., Tinjaca Ramirez, L., Tomasella, L., Tsapras, Y., Villanueva, S., 56, O, Wambsganss, J., Wiersema, K., Wilson, R., Yoldas, A., Ya, R, Zhukov, D., Zdanavičius, J., Zoła, S., Zubareva, A., Universitat Politècnica de Catalunya. Departament de Física, Universitat Politècnica de Catalunya. GAA - Grup d'Astronomia i Astrofísica, Obserwatorium Astronomiczne Uniwersytetu Warszawskiego, Instytut Astronomiczny Uniwersytetu Wrocławskiego, Instituto de Astrofìsica de Canarias, National Science Centre (Poland), European Commission, Ministry of Science and Higher Education (Poland), Science and Technology Facilities Council (UK), Foundation for Polish Science, Slovenian Research Agency, University of Crete, Foundation for Research and Technology, National Research Foundation of Korea, University of Leicester, European Space Agency, National Science Foundation (US), Ministerio de Economía y Competitividad (España), Universidad de Barcelona, Agenzia Spaziale Italiana, Royal Society (UK), Ministry of Science and Technology (Taiwan), The Ohio State University, Chinese Academy of Sciences, Villum Fonden, Research Council of Lithuania, Kazan Federal University, National Aeronautics and Space Administration (US), Ministry of Education, Science and Technological Development (Serbia), W. M. Keck Foundation, Astronomical Observatory [Warsaw], Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), School of Physics, University College Dublin, Ireland, University of Pretoria [South Africa], Clinical Center of Serbia (KCS), Science & Technology Facilities Council, University of St Andrews. School of Physics and Astronomy, University of St Andrews. St Andrews Centre for Exoplanet Science, and Ege Üniversitesi
Subjects: Astronomy, Estels binaris, gravitational lensing: micro, techniques: photometric, binaries: general, stars: individual: Gaia16aye-L, Astrophysics, 01 natural sciences, 7. Clean energy, Gaia16aye-L, Gravitational lenses, Bulge, Fotometria astronòmica, QB Astronomy, Astrophysics::Solar and Stellar Astrophysics, 010303 astronomy & astrophysics, QC, QB, Physics, Gravitational lensing micro, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomical photometry, 3rd-DAS, Orbital period, Radial velocity, Orbit, Astrophysics - Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Stars: individual: Gaia16aye-L, astro-ph.SR, individual: Gaia16aye [Stars], FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Gravitational microlensing, Gravitational lensing: micro, micro [Gravitational lensing], Double stars, 0103 physical sciences, Binaries: general, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Solar and Stellar Astrophysics (astro-ph.SR), Astrophysics::Galaxy Astrophysics, Orbital elements, general [Binaries], photometric [Techniques], Binaries, Astronomy and Astrophysics, Light curve, Stars, QC Physics, Space and Planetary Science, Física::Astronomia i astrofísica [Àrees temàtiques de la UPC], Techniques - photometric, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Techniques: photometric, astro-ph.IM
Abstract: Gaia16aye was a binary microlensing event discovered in the direction towards the northern Galactic disc and was one of the first microlensing events detected and alerted to by the Gaia space mission. Its light curve exhibited five distinct brightening episodes, reaching up to I = 12 mag, and it was covered in great detail with almost 25 000 data points gathered by a network of telescopes. We present the photometric and spectroscopic follow-up covering 500 days of the event evolution. We employed a full Keplerian binary orbit microlensing model combined with the motion of Earth and Gaia around the Sun to reproduce the complex light curve. The photometric data allowed us to solve the microlensing event entirely and to derive the complete and unique set of orbital parameters of the binary lensing system. We also report on the detection of the first-ever microlensing space-parallax between the Earth and Gaia located at L2. The properties of the binary system were derived from microlensing parameters, and we found that the system is composed of two main-sequence stars with masses 0.57 +/- 0.05 M-circle dot and 0.36 +/- 0.03 M-circle dot at 780 pc, with an orbital period of 2.88 years and an eccentricity of 0.30. We also predict the astrometric microlensing signal for this binary lens as it will be seen by Gaia as well as the radial velocity curve for the binary system. Events such as Gaia16aye indicate the potential for the microlensing method of probing the mass function of dark objects, including black holes, in directions other than that of the Galactic bulge. This case also emphasises the importance of long-term time-domain coordinated observations that can be made with a network of heterogeneous telescopes., Polish National Sci-ence Centre (NCN): HARMONIA NCN grant [2015/18/M/ST9/00544]; Polish National Sci-ence Centre (NCN): OPUS NCN grant [2015/17/B/ST9/03167]; Polish National Sci-ence Centre (NCN): DAINA NCN grant [2017/27/L/ST9/03221]; European CommissionEuropean CommissionEuropean Commission Joint Research Centre [312430, 730890]; Polish Ministry of Higher EducationMinistry of Science and Higher Education, Poland [3040/7.PR/2014/2, DIR/WK/2018/12]; MAESTRO NCN grant [2014/14/A/ST9/00121]; DDT programmes [SW2016b12, A34DDT3]; UK Science and Technology Facilities CouncilUK Research & Innovation (UKRI)Science & Technology Facilities Council (STFC); Foundation for Polish Science (Program START); National Science Center, PolandNational Science Centre, Poland [ETIUDA 2018/28/T/ST9/00096]; Slovenian Research AgencySlovenian Research Agency - Slovenia [P1-0031, J1-8136]; COST Action GWverseEuropean Cooperation in Science and Technology (COST) [CA16104]; National Research Foundation of KoreaNational Research Foundation of Korea [2017R1A4A1015178]; STFCUK Research & Innovation (UKRI)Science & Technology Facilities Council (STFC); European Space Agency under the NELIOTA program [4000112943]; GROWTH project - National Science Foundation [1545949]; MINECO (Spanish Ministry of Economy) [ESP2016-80079-C2-1-R, ESP2014-55996-C2-1-R, RTI2018-095076B-C21]; ICCUB (Unidad de Excelencia a Maria de Maeztu) [MDM-2014-0369]; Agenzia Spaziale Italiana (ASI)Agenzia Spaziale Italiana (ASI) [ASI I/058/10/0, ASI 2014-025-R.1.2015]; Royal Society Research GrantRoyal Society of London [RG170230]; Ministry of Science and Technology (Taiwan)Ministry of Science and Technology, Taiwan [104-2112-M-008-012MY3, 104-2923-M-008-004-MY5]; European Research Council under the European Union's Seventh Framework Programme (FP/2007-2013)/ERC Grant [320964]; Gordon and Betty Moore FoundationGordon and Betty Moore Foundation [GBMF5490]; NSFNational Science Foundation (NSF) [AST-1515927, AST-0908816, AST-1412587]; Mt. Cuba Astronomical Foundation; Center for Cosmology and AstroParticle Physics at the Ohio State UniversityOhio State University; Chinese Academy of Sciences South America Center for Astronomy (CAS-SACA); Villum Foundation; MINECO under the Ramon y Cajal programme [RYC-2016-20254]; MINECO [AYA2017-86274-P]; AGAUR grantAgencia de Gestio D'Ajuts Universitaris de Recerca Agaur (AGAUR) [SGR-661/2017]; Science and Technology Facilities CouncilUK Research & Innovation (UKRI)Science & Technology Facilities Council (STFC) [ST/P000541/1]; STFC consolidated grant [ST/M001296/1]; Research Council of LithuaniaResearch Council of Lithuania (LMTLT) [S-LL-19-2]; TUB.ITAKTurkiye Bilimsel ve Teknolojik Arastirma Kurumu (TUBITAK); IKI; KFU; AST; National Science Fund (Bulgaria)National Science Fund of Bulgaria [DN 18/13-12.12.2017]; Institute of Astronomy via research project "Study of ICRF radio-sources and fast variable astronomical objects"; NAO Rozhen, BAS, via research project "Study of ICRF radio-sources and fast variable astronomical objects"; Ministry of Education, Science and Technological Development of the Republic of Serbia [176011, 176004, 176021]; DFGGerman Research Foundation (DFG)European Commission [SPP 1992, WA 1074/11-1]; NCN [2016/21/B/ST9/01126]; MINECO Ramon y Cajal programme [AYA2017-86274-P, RYJ-2016-20254]; Robert Martin Ayers Sciences Fund; National Aeronautics and Space AdministrationNational Aeronautics & Space Administration (NASA) [NNX08AR22G]; National Science FoundationNational Science Foundation (NSF) [AST-1238877]; W. M. Keck FoundationW.M. Keck Foundation; ICCUB (Unidad de Excelencia 'Maria de Maeztu') [MDM-2014-0369]; [3.6714.2017/8.9], This work relies on the results from the European Space Agency (ESA) space mission Gaia. Gaia data are being processed by the Gaia Data Processing and Analysis Consortium (DPAC). Funding for the DPAC is provided by national institutions, in particular the institutions participating in the Gaia Multi-Lateral Agreement (MLA). The Gaia mission website is https://www.cosmos.esa.int/gaia.In particular we acknowledge Gaia Photomet-ric Science Alerts Team, website http://gsaweb.ast.cam.ac.uk/alerts.We thank the members of the OGLE team for discussions and support. We also would like to thank the Polish Children Fund (KFnRD) for support of an internship of their pupils in Ostrowik Observatory of the Warsaw Univ-ersity, during which some of the data were collected, in particular we thank: Robert Nowicki, Michal Por.ebski and Karol Niczyj. The work presented here has been supported by the following grants from the Polish National Sci-ence Centre (NCN): HARMONIA NCN grant 2015/18/M/ST9/00544, OPUS NCN grant 2015/17/B/ST9/03167, DAINA NCN grant 2017/27/L/ST9/03221, as well as European Commission's FP7 and H2020 OPTICON grants (312430 and 730890), Polish Ministry of Higher Education support for OPTICON FP7, 3040/7.PR/2014/2, MNiSW grant DIR/WK/2018/12. PMr and JS acknowledge support from MAESTRO NCN grant 2014/14/A/ST9/00121 to Andrzej Udal-ski. We would like to thank the following members of the AAVSO for their amazing work with collecting vast amounts of data: Teofilo Arranz, James Boardman, Stephen Brincat, Geoff Chaplin, Emery Erdelyi, Rafael Farfan, William Goff, Franklin Guenther, Kevin Hills, Jens Jacobsen, Raymond Kneip, David Lane, Fernando Limon Martinez, Gianpiero Locatelli, Andrea Mantero, Attila Madai, Peter Meadows, Otmar Nickel, Arto Oksanen, Luis Perez, Roger Pieri, Ulisse Quadri, Diego Rodriguez Perez, Frank Schorr, George Sjoberg, Andras Timar, Ray Tomlin, Tonny Vanmunster, Klaus Wenzel, Thomas Wikander. We also thank the amateur observers from around the world, in particular, Pietro Capuozzo, Leone Trascianelli, Igor Zharkov from Ardingly College and Angelo Tomassini, Karl-Ludwig Bath. We also thank Roger Pickard from the British Astronomical Association and Matthias Penselin from the German Haus der Astronomie association for their contributions. KS thanks Dr. Dmitry Chulkov and Dr. Panagiotis Gavras for the interesting discussion of stellar multiplicity. We acknowledge support of DDT programmes SW2016b12 (WHT) and A34DDT3 (TNG). The INT, TNG and WHT are operated on the island of La Palma by the Isaac Newton Group of Telescopes in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. The Liverpool Telescope is operated on the island of La Palma by Liverpool John Moores University in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias with financial support from the UK Science and Technology Facilities Council. SJF would like to thank the UCL students who assisted with the collection and checking of UCLO data for the observing campaign: Martina Aghopian, Ashleigh Arendt, Artem Barinov, Luke Barrett, Jasper Berry-Gair, Arjun Bhogal, Charles Bowesman, William Boyd, Andrei Cuceu, Michael Davies, Max Freedman, Gabriel Fu, Abirami Govindaraju, Iandeep Hothi, Clara Matthews Torres, Darius Modirrousta-Galian, Petru Neague, George Pattinson, Xiaoxi Song, and Brian Yu. P.Mr. acknowledges support from the Foundation for Polish Science (Program START) and the National Science Center, Poland (grant ETIUDA 2018/28/T/ST9/00096).; r r AC, AG and NI acknowledge the financial support from the Slovenian Research Agency (research core funding No. P1-0031 and project grant No. J1-8136)and networking support by the COST Action GWverse CA16104. Skinakas Observatory is a collaborative project of the University of Crete and the Foundation for Research and Technology-Hellas. Work by C.H. was supported by the grant (2017R1A4A1015178) of National Research Foundation of Korea. KW acknowledges funding from STFC, and thanks the University of Lei-cester for the investment in instrumentation. We gratefully acknowledge financial support by the European Space Agency under the NELIOTA program, contract No. 4000112943. This work has made use of data obtained with the Kryoneri Prime Focus Instrument, developed by the European Space Agency NELIOTA project on the 1.2 m Kryoneri telescope, which is operated by IAASARS, National Observatory of Athens, Greece. The Aristarchos tele-scope is operated on Helmos Observatory by the IAASARS of the National Observatory of Athens. This work was supported by the GROWTH project funded by the National Science Foundation under Grant No 1545949. This work was supported by the MINECO (Spanish Ministry of Economy) through grant ESP2016-80079-C2-1-R (MINECO/FEDER, UE) and ESP2014-55996-C2-1-R (MINECO/FEDER, UE) and MDM-2014-0369 of ICCUB (Unidad de Excelencia a Maria de Maeztu). This work was supported by the MINECO (Spanish Ministry of Economy) through grant ESP2016-80079-C2-1-R and RTI2018-095076B-C21 (MINECO/FEDER, UE), and MDM-2014-0369 of ICCUB (Unidad de Excelencia 'Maria de Maeztu'). The Joan Oro Telescope (TJO) of the Montsec Astronomical Observatory (OAdM) is owned by the Catalan Government and is operated by the Institute for Space Studies of Catalonia (IEEC). Support to this study has been provided by Agenzia Spaziale Italiana (ASI) through grants ASI I/058/10/0 and ASI 2014-025-R.1.2015. KW thanks Dipali Thanki and Ray McErlean for their technical support of the scientific programme of the University of Leicester observatory. This work was supported by Royal Society Research Grant RG170230. CCN thanks the funding from Ministry of Science and Technology (Taiwan) under the contracts 104-2112-M-008-012MY3 and 104-2923-M-008-004-MY5. The research leading to these results has received funding from the European Research Council under the European Union's Seventh Framework Programme (FP/2007-2013)/ERC Grant Agreement n. 320964 (WDTracer). We thank the Las Cumbres Observatory and its sta ff for its continuing support of the project. ASAS-SN is supported by the Gordon and Betty Moore Foundation through grant GBMF5490 to the Ohio State University and NSF grant AST-1515927. Development of ASAS-SN has been supported by NSF grant AST-0908816, the Mt. Cuba Astronomical Foundation, the Center for Cosmology and AstroParticle Physics at the Ohio State University, the Chinese Academy of Sciences South America Center for Astronomy (CAS-SACA), the Villum Foundation, and George Skestos. ARM acknowledges support from the MINECO under the Ramon y Cajal programme (RYC-2016-20254) and the AYA2017-86274-P grant, and the AGAUR grant SGR-661/2017. We acknowledge support from the Science and Technology Facilities Council (TB and RWW; ST/P000541/1). K.Horne acknowledges support from STFC consolidated grant ST/M001296/1. This work was partly supported by the Research Council of Lithuania, grant No. S-LL-19-2 Authors thank to TUB.ITAK, IKI, KFU, and AST for partial supports in using RTT150 (Russian-Turkish 1.5-m telescope in Antalya).; r r This work was partially funded by the subsidy 3.6714.2017/8.9 allocated to Kazan Federal University for the state assignment in the sphere of scientific activities. This research was partially supported by contract DN 18/13-12.12.2017 with the National Science Fund (Bulgaria). Work by YS was supported by an appointment to the NASA Postdoctoral Program at the Jet Propulsion Laboratory, California Institute of Technology, administered by Uni-versities Space Research Associ-ation through a contract with NASA. GD gratefully acknowledges the obser-ving grant support from the Institute of Astronomy and NAO Rozhen, BAS, via bilateral joint research project "Study of ICRF radio-sources and fast variable astronomical objects" (PI:G.Damljanovic). This work is a part of the Projects no. 176011 "Dynamics and kinematics of celestial bodies and systems", no. 176004 "Stellar physics" and no. 176021 "Visible and invisible matter in nearby galaxies: theory and observations" supported by the Ministry of Education, Science and Technological Development of the Republic of Serbia. YT acknowledges the support of DFG priority program SPP 1992 "Exploring the diversity of Extrasolar Planets" (WA 1074/11-1). This work of PMi, DM and ZK was supported by the NCN grant no. 2016/21/B/ST9/01126. ARM acknowledges support from the MINECO Ramon y Cajal programme RYJ-2016-20254 and grant AYA2017-86274-P and from the AGAUR grant SGR-661/2017. The work by C. R. was supported by an appointment to the NASA Postdoctoral Program at the Goddard Space Flight Center, administered by USRA through a contract with NASA. The Faulkes Telescope Project is an education partner of Las Cumbres Observatory (LCO). The Faulkes Telescopes are maintained and operated by LCO. This research was made possible through the use of the AAVSO Photomet-ric All-Sky Survey (APASS), funded by the Robert Martin Ayers Sciences Fund and NSF AST-1412587. The Pan-STARRS1 Surveys (PS1) and the PS1 public science archive have been made possible through contributions by the Institute for Astronomy, the University of Hawaii, the Pan-STARRS Project O ffice, the Max-Planck Society and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg and the Max Planck Institute for Extraterrestrial Physics, Garching, The Johns Hopkins University, Durham University, the University of Edinburgh, the Queen's University Belfast, the Harvard-Smithsonian Center for Astrophysics, the Las Cumbres Observatory Global Telescope Network Incor-porated, the National Central University of Taiwan, the Space Telescope Sci-ence Institute, the National Aeronautics and Space Administration under Grant No. NNX08AR22G issued through the Planetary Science Division of the NASA Science Mission Directorate, the National Science Foundation Grant No. AST-1238877, the University of Maryland, Eotvos Lorand University (ELTE), the Los Alamos National Laboratory, and the Gordon and Betty Moore Foundation. Some of the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Ins-titute of Technology, the University of California and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation.
Published: 2020
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18. Dissolution Phase Diagram in Radial Geometry

Author: Eirik Grude Flekkøy, Knut Jørgen Måløy, Piotr Szymczak, Renaud Toussaint, Le Xu, PoreLab [Oslo], Department of Physics [Oslo], Faculty of Mathematics and Natural Sciences [Oslo], University of Oslo (UiO)-University of Oslo (UiO)-Faculty of Mathematics and Natural Sciences [Oslo], University of Oslo (UiO)-University of Oslo (UiO)-Norwegian University of Science and Technology [Oslo] (NTNU), Norwegian University of Science and Technology (NTNU)-Norwegian University of Science and Technology (NTNU), Institute of Theoretical Physics [Warsaw], Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), Institut de physique du globe de Strasbourg (IPGS), and Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Materials science, [SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph], Materials Science (miscellaneous), Flow (psychology), Biophysics, General Physics and Astronomy, dissolution, Geometry, 01 natural sciences, Instability, 0103 physical sciences, reaction-infiltration, [PHYS.MECA.MEFL]Physics [physics]/Mechanics [physics]/Fluid mechanics [physics.class-ph], Physical and Theoretical Chemistry, 010306 general physics, Dissolution, Mathematical Physics, ComputingMilieux_MISCELLANEOUS, Phase diagram, [SPI.FLUID]Engineering Sciences [physics]/Reactive fluid environment, Hele-Shaw cell, lcsh:QC1-999, phase diagram, Damköhler numbers, instability, Hele-Shaw flow, Fracture (geology), Porous medium, lcsh:Physics
Abstract: International audience; Fractures play an important role as flow paths in porous media. When an undersaturated reactive fluid is flowing in a fracture, the dissolution process will alter the flow paths locally. Dissolution patterns grow slowly, but they may lead to a dramatic reorganization of the flow. Here, we study dissolution in a radial geometry, which is relevant for a number of practical applications, e.g., the acidization of oil reservoirs. Different dissolution patterns are presented in a phase diagram with the Péclet and Damköhler numbers as parameters. We also analyze quantitatively the density of wormholes and the relation between the aperture roughness and the ramified patterns.
Published: 2020
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19. A plethora of new R Coronae Borealis stars discovered from a dedicated spectroscopic follow-up survey

Author: Łukasz Wyrzykowski, Andrzej Udalski, Michael S. Bessell, P. Wils, Douglas L. Welch, Peter R. Wood, Przemek Mróz, Patrick Tisserand, Geoffrey C. Clayton, Devika Kamath, Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Australian National University (ANU), Louisiana State University (LSU), McMaster University [Hamilton, Ontario], Macquarie University, Astronomical Observatory [Warsaw], Faculty of Physics [Warsaw] (FUW), and University of Warsaw (UW)-University of Warsaw (UW)
Subjects: Long lasting, Milky Way, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, stars: evolution, 010303 astronomy & astrophysics, Follow up survey, Solar and Stellar Astrophysics (astro-ph.SR), Astrophysics::Galaxy Astrophysics, Physics, 010308 nuclear & particles physics, Astronomy and Astrophysics, supergiants, [PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR], stars: chemically peculiar, Stars, stars: carbon, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, Physics::Space Physics, Astrophysics::Earth and Planetary Astrophysics, Supergiant, methods: observational
Abstract: It is increasingly suspected that the rare R Coronae Borealis (RCB) stars - hydrogen-deficient and carbon-rich supergiant stars - are the products of mergers of CO/He white-dwarf binary systems in the intermediate mass regime ($0.615000$ K). Forty of these belong to the Milky Way and five are located in the Magellanic Clouds. We also confirmed that the long lasting candidate KDM 5651 is indeed a new Magellanic RCB star, increasing the total number of Magellanic Cloud RCB stars to 30. We have increased by $\sim$50\% the total number of RCB stars known, now reaching 147. We also include a list of 14 strong RCB candidates, most certainly observed during a dust obscuration phase. From the detection efficiency and success rate so far, we estimate that there should be no more than 500 RCB stars/HdC stars in the Milky Way., Comment: 34 pages, 20 figures
Published: 2020
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20. On the Maximum Weight Independent Set Problem in Graphs without Induced Cycles of Length at Least Five

Author: Stéphan Thomassé, Michał Pilipczuk, Maria Chudnovsky, Marcin Pilipczuk, Department of Mathematics - Princeton University, Princeton University, Institute of Informatics [Warsaw], Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), University of Warsaw (UW)-University of Warsaw (UW), Institut Universitaire de France (IUF), Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.), Modèles de calcul, Complexité, Combinatoire (MC2), Laboratoire de l'Informatique du Parallélisme (LIP), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Recherche en Informatique et en Automatique (Inria)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Recherche en Informatique et en Automatique (Inria)-Centre National de la Recherche Scientifique (CNRS), École normale supérieure - Lyon (ENS Lyon)-Université Claude Bernard Lyon 1 (UCBL), and Université de Lyon-Université de Lyon-Institut National de Recherche en Informatique et en Automatique (Inria)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Lyon (ENS Lyon)-Université Claude Bernard Lyon 1 (UCBL)
Subjects: FOS: Computer and information sciences, Discrete mathematics, Discrete Mathematics (cs.DM), General Mathematics, 010102 general mathematics, [INFO.INFO-DS]Computer Science [cs]/Data Structures and Algorithms [cs.DS], 0102 computer and information sciences, 01 natural sciences, Graph, Combinatorics, Computer Science::Discrete Mathematics, 010201 computation theory & mathematics, Independent set, Computer Science - Data Structures and Algorithms, Perfect graph, FOS: Mathematics, Mathematics - Combinatorics, Data Structures and Algorithms (cs.DS), Combinatorics (math.CO), 0101 mathematics, ComputingMilieux_MISCELLANEOUS, Computer Science - Discrete Mathematics, Mathematics
Abstract: A hole in a graph is an induced cycle of length at least $4$, and an antihole is the complement of an induced cycle of length at least $4$. A hole or antihole is long if its length is at least $5$. For an integer $k$, the $k$-prism is the graph consisting of two cliques of size $k$ joined by a matching. The complexity of Maximum (Weight) Independent Set (MWIS) in long-hole-free graphs remains an important open problem. In this paper we give a polynomial time algorithm to solve MWIS in long-hole-free graphs with no $k$-prism (for any fixed integer $k$), and a subexponential algorithm for MWIS in long-hole-free graphs in general. As a special case this gives a polynomial time algorithm to find a maximum weight clique in perfect graphs with no long antihole, and no hole of length $6$. The algorithms use the framework of minimal chordal completions and potential maximal cliques.
Published: 2020
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21. Approximating Longest Common Substring with k mismatches: Theory and Practice

Author: Gourdel, Garance, Kociumaka, Tomasz, Radoszewski, Jakub, Starikovskaya, Tatiana, Département d'informatique - ENS Paris (DI-ENS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut National de Recherche en Informatique et en Automatique (Inria)-Centre National de la Recherche Scientifique (CNRS), Scalable, Optimized and Parallel Algorithms for Genomics (GenScale), Inria Rennes – Bretagne Atlantique, Institut National de Recherche en Informatique et en Automatique (Inria)-Institut National de Recherche en Informatique et en Automatique (Inria)-GESTION DES DONNÉES ET DE LA CONNAISSANCE (IRISA-D7), Institut de Recherche en Informatique et Systèmes Aléatoires (IRISA), Université de Rennes (UR)-Institut National des Sciences Appliquées - Rennes (INSA Rennes), Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Université de Bretagne Sud (UBS)-École normale supérieure - Rennes (ENS Rennes)-Institut National de Recherche en Informatique et en Automatique (Inria)-CentraleSupélec-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT)-Université de Rennes (UR)-Institut National des Sciences Appliquées - Rennes (INSA Rennes), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT)-Institut de Recherche en Informatique et Systèmes Aléatoires (IRISA), Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Université de Bretagne Sud (UBS)-École normale supérieure - Rennes (ENS Rennes)-CentraleSupélec-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Bar-Ilan University [Israël], Institute of Informatics [Warsaw], Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), and University of Warsaw (UW)-University of Warsaw (UW)
Subjects: FOS: Computer and information sciences, 2012 ACM Subject Classification Theory of computation → Pattern matching phrases approximation algorithms, conditional lower bounds, Computer Science - Data Structures and Algorithms, 2012 ACM Subject Classification Theory of computation → Pattern matching phrases approximation algorithms string similarity LSH conditional lower bounds, Data Structures and Algorithms (cs.DS), [INFO]Computer Science [cs], Data_CODINGANDINFORMATIONTHEORY, approximation algorithms, string similarity, LSH
Abstract: In the problem of the longest common substring with k mismatches we are given two strings X, Y and must find the maximal length 𝓁 such that there is a length-𝓁 substring of X and a length-𝓁 substring of Y that differ in at most k positions. The length 𝓁 can be used as a robust measure of similarity between X, Y. In this work, we develop new approximation algorithms for computing 𝓁 that are significantly more efficient that previously known solutions from the theoretical point of view. Our approach is simple and practical, which we confirm via an experimental evaluation, and is probably close to optimal as we demonstrate via a conditional lower bound., LIPIcs, Vol. 161, 31st Annual Symposium on Combinatorial Pattern Matching (CPM 2020), pages 16:1-16:15
Published: 2020
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22. Jones' Conjecture in subcubic graphs

Author: Tomáš Masařík, Michał Pilipczuk, Wojciech Nadara, Andrea Munaro, Marthe Bonamy, François Dross, Marcin Pilipczuk, Bonamy, Marthe, Laboratoire Bordelais de Recherche en Informatique (LaBRI), Université de Bordeaux (UB)-Centre National de la Recherche Scientifique (CNRS)-École Nationale Supérieure d'Électronique, Informatique et Radiocommunications de Bordeaux (ENSEIRB), Institute of Mathematics [Warsaw], Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), University of Warsaw (UW)-University of Warsaw (UW), and University of Warsaw (UW)
Subjects: FOS: Computer and information sciences, Discrete Mathematics (cs.DM), [INFO.INFO-DS]Computer Science [cs]/Data Structures and Algorithms [cs.DS], [INFO.INFO-DS] Computer Science [cs]/Data Structures and Algorithms [cs.DS], [INFO.INFO-DM]Computer Science [cs]/Discrete Mathematics [cs.DM], Computer Science::Computational Complexity, Theoretical Computer Science, Combinatorics, Computer Science::Discrete Mathematics, [MATH.MATH-CO]Mathematics [math]/Combinatorics [math.CO], FOS: Mathematics, Discrete Mathematics and Combinatorics, Mathematics - Combinatorics, Mathematics, Conjecture, Applied Mathematics, [MATH.MATH-CO] Mathematics [math]/Combinatorics [math.CO], [INFO.INFO-DM] Computer Science [cs]/Discrete Mathematics [cs.DM], Computational Theory and Mathematics, Geometry and Topology, Combinatorics (math.CO), Computer Science - Discrete Mathematics
Abstract: We confirm Jones' Conjecture for subcubic graphs. Namely, if a subcubic planar graph does not contain $k+1$ vertex-disjoint cycles, then it suffices to delete $2k$ vertices to obtain a forest.
Published: 2019
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23. Upconverted electroluminescence via Auger scattering of interlayer excitons in van der Waals heterostructures

Author: Konstantin S. Novoselov, Vladimir I. Fal'ko, Maciej R. Molas, Andre K. Geim, Clément Faugeras, James Howarth, Mark Danovich, Andrzej Wysmołek, J. Binder, Kenji Watanabe, Marek Potemski, Freddie Withers, Takashi Taniguchi, Aleksey Kozikov, Department of Geology, Laboratoire national des champs magnétiques intenses - Grenoble (LNCMI-G ), Institut National des Sciences Appliquées - Toulouse (INSA Toulouse), Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), National Institute for Materials Science (NIMS), Institute of Experimental Physics [Warsaw] (IFD), Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), School of Physics and Astronomy [Manchester], and University of Manchester [Manchester]
Subjects: 0301 basic medicine, Physics::Instrumentation and Detectors, General Physics and Astronomy, 02 engineering and technology, Auger recombination, Condensed Matter::Superconductivity, Emission spectrum, lcsh:Science, ComputingMilieux_MISCELLANEOUS, Physics, upconversion, [PHYS]Physics [physics], education.field_of_study, Multidisciplinary, WSe2, 021001 nanoscience & nanotechnology, Condensed Matter::Mesoscopic Systems and Quantum Hall Effect, Excited state, Excitons, 0210 nano-technology, Materials for devices, light emitting diode (LED), Exciton, Science, Astrophysics::High Energy Astrophysical Phenomena, Population, Van der Waals heterostructures, FOS: Physical sciences, Electroluminescence, Molecular physics, Article, General Biochemistry, Genetics and Molecular Biology, Transition metal dichalcogenides, 03 medical and health sciences, Condensed Matter::Materials Science, National Graphene Institute, Nanoscience and technology, Mesoscale and Nanoscale Physics (cond-mat.mes-hall), Spontaneous emission, [PHYS.COND]Physics [physics]/Condensed Matter [cond-mat], education, Condensed Matter - Mesoscale and Nanoscale Physics, business.industry, Scattering, Condensed Matter::Other, Light emitting materials, General Chemistry, 2D materials, 030104 developmental biology, Semiconductor, ResearchInstitutes_Networks_Beacons/national_graphene_institute, lcsh:Q, business, MoS2
Abstract: The intriguing physics of carrier-carrier interactions, which likewise affect the operation of light emitting devices, stimulate the research on semiconductor structures at high densities of excited carriers, a limit reachable at large pumping rates or in systems with long-lived electron-hole pairs. By electrically injecting carriers into WSe$_2$/MoS$_2$ type-II heterostructures which are indirect in real and k-space, we establish a large population of typical optically silent interlayer excitons. Here, we reveal their emission spectra and show that the emission energy is tunable by an applied electric field. When the population is further increased by suppressing the radiative recombination rate with the introduction of an hBN spacer between WSe$_2$ and MoS$_2$, Auger-type and exciton-exciton annihilation processes become important. These processes are traced by the observation of an up-converted emission demonstrating that excitons gaining energy in non-radiative Auger processes can be recovered and recombine radiatively., Comment: accepted for publication in Nature Communications
Published: 2019
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24. Dispersion relation of the collective excitations in a resonantly driven polariton fluid

Author: Petr Stepanov, Ivan Amelio, Aristide Lemaître, Anna Minguzzi, Iacopo Carusotto, Jacqueline Bloch, Maxime Richard, Alberto Amo, J.-G. Rousset, Nanophysique et Semiconducteurs (NEEL - NPSC), Institut Néel (NEEL), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), BEC-INFM, Università degli Studi di Trento (UNITN), Institute of Experimental Physics [Warsaw] (IFD), Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), Centre de Nanosciences et Nanotechnologies (C2N (UMR_9001)), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 (PhLAM), Université de Lille-Centre National de la Recherche Scientifique (CNRS), Laboratoire de physique et modélisation des milieux condensés (LPM2C), Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), ANR-16-CE30-0021,QFL,Fluides Quantiques de Lumière(2016), and Nanophysique et Semiconducteurs (NPSC)
Subjects: 0301 basic medicine, Quantum fluid, Quantum fluids and solids, Exciton, Science, Polaritons, General Physics and Astronomy, FOS: Physical sciences, Physics::Optics, 02 engineering and technology, Article, General Biochemistry, Genetics and Molecular Biology, Superfluidity, 03 medical and health sciences, Dispersion relation, Quantum mechanics, Polariton, [PHYS.COND]Physics [physics]/Condensed Matter [cond-mat], lcsh:Science, Quantum, ComputingMilieux_MISCELLANEOUS, Physics, Condensed Matter::Quantum Gases, [PHYS]Physics [physics], Multidisciplinary, Bose-Einstein condensation, quantized vortices, liquid-helium, solitons, Condensed Matter::Other, General Chemistry, 021001 nanoscience & nanotechnology, 030104 developmental biology, Quantum hydrodynamics, Quantum Gases (cond-mat.quant-gas), Quasiparticle, lcsh:Q, Condensed Matter - Quantum Gases, 0210 nano-technology
Abstract: Exciton-polaritons in semiconductor microcavities constitute the archetypal realization of a quantum fluid of light. Under coherent optical drive, remarkable effects such as superfluidity, dark solitons or the nucleation of vortices have been observed, and can be all understood as specific manifestations of the condensate collective excitations. In this work, we perform a Brillouin scattering experiment to measure their dispersion relation \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\omega ({\bf{k}})$$\end{document}ω(k) directly. The results, such as a speed of sound which is apparently twice too low, cannot be explained upon considering the polariton condensate alone. In a combined theoretical and experimental analysis, we demonstrate that the presence of an excitonic reservoir alongside the polariton condensate has a dramatic influence on the characteristics of the quantum fluid, and explains our measurement quantitatively. This work clarifies the role of such a reservoir in polariton quantum hydrodynamics. It also provides an unambiguous tool to determine the condensate-to-reservoir fraction in the quantum fluid, and sets an accurate framework to approach ideas for polariton-based quantum-optical applications., Owing to its driven-dissipative nature, and its solid-state environment, a resonantly driven polariton condensate can be accompanied by an incoherent reservoir of excitons. Stepanov et al. demonstrate that this situation strongly modifies the spectrum of collective excitations, which determines many quantum hydrodynamic features in a polariton fluid.
Published: 2019
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25. Packing and covering immersion-expansions of planar sub-cubic graphs

Author: Jean-Florent Raymond, Dimitrios M. Thilikos, Archontia C. Giannopoulou, O-joung Kwon, Institut für Softwaretechnik und Theoretische Informatik [EECS-TUB], Fakultät Elektrotechnik und Informatik [TUB], Technische Universität Berlin (TU)-Technische Universität Berlin (TU), Technische Universität Berlin (TU), Algorithmes, Graphes et Combinatoire (ALGCO), Laboratoire d'Informatique de Robotique et de Microélectronique de Montpellier (LIRMM), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM), Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), University of Warsaw (UW), Department of Mathematics [Athens], National and Kapodistrian University of Athens (NKUA), Archontia C. Giannopoulou and O-joung Kwon have been supported by the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (ERC consolidator grant DISTRUCT, agreement No 648527). Part of the research of Archontia C. Giannopoulou took place while she was a post-doc at the Warsaw Center of Mathematics and Computer Science. O-joung Kwon has been supported by ERC Starting Grant PARAMTIGHT (No. 280152). Jean-Florent Raymond has been supported by the (Polish) National Science Centre grant PRELUDIUM 2013/11/N/ST6/02706. Dimitrios M. Thilikos has been supported by the ANR project DEMOGRAPH (ANR-16-CE40-0028)., ANR-16-CE40-0028,DE-MO-GRAPH,Décomposition de Modèles Graphiques(2016), Technische Universität Berlin ( TUB ) -Technische Universität Berlin ( TUB ), Technische Universität Berlin ( TUB ), Algorithmes, Graphes et Combinatoire ( ALGCO ), Laboratoire d'Informatique de Robotique et de Microélectronique de Montpellier ( LIRMM ), Université de Montpellier ( UM ) -Centre National de la Recherche Scientifique ( CNRS ) -Université de Montpellier ( UM ) -Centre National de la Recherche Scientifique ( CNRS ), Department of Mathematics, Computer Science and Mechanics [Warsaw], University of Warsaw ( UW ), National and Kapodistrian University of Athens, and ANR-16-CE40-0028,DEMOGRAPH,Décomposition de Modèles Graphiques ( 2016 )
Subjects: 010102 general mathematics, Neighbourhood (graph theory), [ INFO.INFO-DM ] Computer Science [cs]/Discrete Mathematics [cs.DM], 0102 computer and information sciences, [INFO.INFO-DM]Computer Science [cs]/Discrete Mathematics [cs.DM], [ MATH.MATH-CO ] Mathematics [math]/Combinatorics [math.CO], 01 natural sciences, Combinatorics, 010201 computation theory & mathematics, Graph power, [MATH.MATH-CO]Mathematics [math]/Combinatorics [math.CO], Graph minor, k-vertex-connected graph, Discrete Mathematics and Combinatorics, Cubic graph, Path graph, Bound graph, 0101 mathematics, Graph factorization, Mathematics
Abstract: International audience; A graph H is an immersion of a graph G if H can be obtained by some subgraph G after lifting incident edges. We prove that there is a polynomial function f : N × N → N, such that if H is a connected planar sub-cubic graph on h > 0 edges, G is a graph, and k is a non-negative integer, then either G contains k vertex/edge-disjoint subgraphs, each containing H as an immersion, or G contains a set F of f (k, h) vertices/edges such that G \ F does not contain H as an immersion.
Published: 2017
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26. Data Assimilation in Reduced Modeling

Author: Peter Binev, Albert Cohen, Guergana Petrova, Wolfgang Dahmen, Ronald A. DeVore, Przemysław Wojtaszczyk, Department of Mathematics [Columbia], University of South Carolina [Columbia], Laboratoire Jacques-Louis Lions (LJLL), Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Rheinisch-Westfälische Technische Hochschule Aachen (RWTH), Texas A&M University [College Station], Department of Mathematics [Texas] (TAMU), Institute of Applied Mathematics [Warsaw] (IMSM), Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), University of Warsaw (UW)-University of Warsaw (UW), European Project: 338977,EC:FP7:ERC,ERC-2013-ADG,BREAD(2014), Cohen, Albert, Breaking the curse of dimensionality: numerical challenges in high dimensional analysis and simulation - BREAD - - EC:FP7:ERC2014-01-01 - 2018-12-31 - 338977 - VALID, and Rheinisch-Westfälische Technische Hochschule Aachen University (RWTH)
Subjects: Statistics and Probability, 65D05, 68Q32, data assimilation MSC numbers: 62M45, 010103 numerical & computational mathematics, 01 natural sciences, Combinatorics, Intersection, Convergence (routing), FOS: Mathematics, Discrete Mathematics and Combinatorics, Applied mathematics, Mathematics - Numerical Analysis, Limit (mathematics), 0101 mathematics, Greedy algorithm, 62M45, 65D05, 68Q32, 97N50, Parametric statistics, Mathematics, Sequence, reduced modeling, Applied Mathematics, Numerical Analysis (math.NA), [MATH.MATH-NA] Mathematics [math]/Numerical Analysis [math.NA], Linear subspace, 010101 applied mathematics, Iterated function, Modeling and Simulation, optimal recovery, Statistics, Probability and Uncertainty, [MATH.MATH-NA]Mathematics [math]/Numerical Analysis [math.NA], 97N50
Abstract: We consider the problem of optimal recovery of an element $u$ of a Hilbert space $\mathcal{H}$ from $m$ measurements obtained through known linear functionals on $\mathcal{H}$. Problems of this type are well studied \cite{MRW} under an assumption that $u$ belongs to a prescribed model class, e.g. a known compact subset of $\mathcal{H}$. Motivated by reduced modeling for parametric partial differential equations, this paper considers another setting where the additional information about $u$ is in the form of how well $u$ can be approximated by a certain known subspace $V_n$ of $\mathcal{H}$ of dimension $n$, or more generally, how well $u$ can be approximated by each $k$-dimensional subspace $V_k$ of a sequence of nested subspaces $V_0\subset V_1\cdots\subset V_n$. A recovery algorithm for the one-space formulation, proposed in \cite{MPPY}, is proven here to be optimal and to have a simple formulation, if certain favorable bases are chosen to represent $V_n$ and the measurements. The major contribution of the present paper is to analyze the multi-space case for which it is shown that the set of all $u$ satisfying the given information can be described as the intersection of a family of known ellipsoids in $\mathcal{H}$. It follows that a near optimal recovery algorithm in the multi-space problem is to identify any point in this intersection which can provide a much better accuracy than in the one-space problem. Two iterative algorithms based on alternating projections are proposed for recovery in the multi-space problem. A detailed analysis of one of them provides a posteriori performance estimates for the iterates, stopping criteria, and convergence rates. Since the limit of the algorithm is a point in the intersection of the aforementioned ellipsoids, it provides a near optimal recovery for $u$., 27 pages
Published: 2017
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27. Predicting the likelihood of a live birth for women with endometriosis-related infertility

Author: Aude Jayot, Clémentine Owen, K. Nyangoh Timoh, Emile Daraï, Christophe Poncelet, Sofiane Bendifallah, Horace Roman, Michael Grynberg, Lionel Carbillon, Salma Touleimat, J. Boujenah, Vincent Lavoué, Emmanuelle Mathieu d'Argent, Louise Benoit, Centre d’Ecologie Fonctionnelle et Evolutive (CEFE), Université Paul-Valéry - Montpellier 3 (UPVM)-Institut National de la Recherche Agronomique (INRA)-Centre international d'études supérieures en sciences agronomiques (Montpellier SupAgro)-École Pratique des Hautes Études (EPHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud])-Institut national d’études supérieures agronomiques de Montpellier (Montpellier SupAgro), Service de gynécologie-obstétrique [Hôpital Jean Verdier, Bondy], Université Paris 13 (UP13)-Hôpital Jean Verdier [AP-HP], Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP), CHU Tenon [AP-HP], Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU), Institute of Experimental Physics [Warsaw] (IFD), Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), Service d'endocrinologie diabétologie, nutrition (Hôpital Jean Verdier), Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Hôpital Jean Verdier [AP-HP], Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Université Sorbonne Paris Nord, CHU Pontchaillou [Rennes], Expert Center in the Diagnosis and Multidisciplinary Management of Endometriosis / Centre expert de diagnostic et de prise en charge multidisciplinaire de l’endométriose [CHU Rouen], CHU Rouen, Normandie Université (NU)-Normandie Université (NU), Université Paris Descartes - Faculté de Médecine (UPD5 Médecine), Université Paris Descartes - Paris 5 (UPD5), Gamétogenèse et Qualité du Gamète - ULR 4308 (GQG), Université de Rouen Normandie (UNIROUEN), Normandie Université (NU)-Normandie Université (NU)-Université de Lille, Normandie Université (NU), Centre de Recherche Saint-Antoine (CRSA), Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Sorbonne Université (SU), Groupe de recherche clinique Centre Expert en Endométriose (GRC 6 - C3E), Sorbonne Université (SU), Université Paul-Valéry - Montpellier 3 (UM3)-Institut National de la Recherche Agronomique (INRA)-Centre international d'études supérieures en sciences agronomiques (Montpellier SupAgro)-École pratique des hautes études (EPHE)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud])-Institut national d’études supérieures agronomiques de Montpellier (Montpellier SupAgro), CHU Tenon [APHP], Institute of Experimental Physics, Warsaw University, University of Warsaw (UW), Department of Endocrinology-Diabetology-Nutrition, Université Paris 13 (UP13), Gamétogenèse et Qualité du Gamète (GQG), Université de Lille-Université de Lille, Droit et Santé-Université de Rouen Normandie (UNIROUEN), Epidemiologie, Systèmes d'information, Modélisation, Institut National de la Santé et de la Recherche Médicale (INSERM), Université Paul-Valéry - Montpellier 3 (UPVM)-Institut National de la Recherche Agronomique (INRA)-Centre international d'études supérieures en sciences agronomiques (Montpellier SupAgro)-École pratique des hautes études (EPHE), Service de Gynécologie-obstétrique et médecine de la reproduction - Maternité [CHU Tenon], Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU), Centre Expert en Endométriose [CHU Tenon] (GRC6 C3E), CCSD, Accord Elsevier, Institut de Recherche pour le Développement (IRD [France-Sud])-Centre National de la Recherche Scientifique (CNRS)-École pratique des hautes études (EPHE)-Université de Montpellier (UM)-Institut national d’études supérieures agronomiques de Montpellier (Montpellier SupAgro)-Institut National de la Recherche Agronomique (INRA)-Centre international d'études supérieures en sciences agronomiques (Montpellier SupAgro)-Université Paul-Valéry - Montpellier 3 (UM3), Normandie Université (NU)-Normandie Université (NU)-Université de Lille, Droit et Santé-Université de Lille, Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-École pratique des hautes études (EPHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre international d'études supérieures en sciences agronomiques (Montpellier SupAgro)-Institut National de la Recherche Agronomique (INRA)-Université Paul-Valéry - Montpellier 3 (UPVM)-Institut national d’études supérieures agronomiques de Montpellier (Montpellier SupAgro), Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro)-Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro)-Institut de Recherche pour le Développement (IRD [France-Sud]), and Sorbonne Université (SU)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)
Subjects: Adult, Infertility, medicine.medical_specialty, media_common.quotation_subject, medicine.medical_treatment, Endometriosis, Fertility, [SDV.MHEP.GEO]Life Sciences [q-bio]/Human health and pathology/Gynecology and obstetrics, Nomogram, 03 medical and health sciences, Endometriosis Infertility Index, 0302 clinical medicine, Pregnancy, medicine, Humans, Live birth, 030212 general & internal medicine, Ovarian reserve, [SDV.BDLR] Life Sciences [q-bio]/Reproductive Biology, ComputingMilieux_MISCELLANEOUS, media_common, 030219 obstetrics & reproductive medicine, Assisted reproductive technology, Obstetrics, business.industry, Area under the curve, Obstetrics and Gynecology, [SDV.BDLR]Life Sciences [q-bio]/Reproductive Biology, medicine.disease, 3. Good health, Nomograms, [SDV.MHEP.GEO] Life Sciences [q-bio]/Human health and pathology/Gynecology and obstetrics, Reproductive Medicine, Female, business, Infertility, Female
Abstract: Objective Endometriosis affects 10% of women in reproductive age and alters fertility. Its management is still debated notably the timing of surgery and ART in infertility. Several tools have been created to guide the practitioner and the couple yet many limitations persist. The objective is to create a nomogram to predict the likelihood of a live birth after surgery followed by assisted reproductive technology (ART) for patients with endometriosis-related infertility. Study design All women in a public university hospital who attempted to conceive by ART after surgery for endometriosis-related infertility from 2004 to 2016 were included. We created a model using multivariable linear regression based on a retrospective database. Result Of the 297 women included, 171 (57.6%) obtained a live birth. Age, duration of infertility, number of ICSI-IVF cycles, ovarian reserve and the revised American Fertility Society (rAFS) score were included in the nomogram. The predictive model had an area under the curve (AUC) of 0.77 (95% CI, 0.75–0.79) and was well calibrated. The external validation of the model was achieved with an AUC of 0.71 (95% CI, 0.69–0.73) and calibration was good. The staging accuracy according to AUC criteria for the nomogram compared to the currently used Endometriosis Infertility Index to predict live births were 0.77 (95% CI, 0.75–0.79) and 0.60 (95% CI: 0.57–0.63), respectively. Conclusion This simple tool appears to accurately predict the likelihood of a live birth for a patient undergoing ART after surgery for endometriosis-related infertility. It could be used to counsel patients in their choice between spontaneous versus ART conception, or oocyte donation.
Published: 2019
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28. An analysis of binary microlensing event OGLE-2015-BLG-0060

Author: Tsapras, Y., Cassan, A., Ranc, C., Bachelet, E., Street, R., Udalski, A., Hundertmark, M., Bozza, V., Beaulieu, J. P., Marquette, J. B., Euteneuer, E., Figuera Jaimes, R., Calchi Novati, S., Bramich, D. M., Dominik, M., Jaimes, R. Figuera, Horne, K., Mao, S., Menzies, J., Schmidt, R., Snodgrass, C., Steele, I. A., Wambsganss, J., Mróz, P., Szymański, M. K., Soszyński, I., Skowron, J., Pietrukowicz, P., Kozłowski, S., Poleski, R., Ulaczyk, K., PAWLAK, M., Jørgensen, U. G., Skottfelt, J., Popovas, A., Ciceri, S., Korhonen, H., Kuffmeier, M., Evans, D. F., Peixinho, N., Hinse, T. C., Burgdorf, M. J., Southworth, J., Tronsgaard, R., Kerins, E., Andersen, M. I., Rahvar, S., Wang, Y., Wertz, O., Rabus, M., Novati, S. Calchi, D'Ago, G., Scarpetta, G., Mancini, L., Abe, F., Asakura, Y., Bennett, D. P., Bhattacharya, A., Donachie, M., Evans, P., Fukui, A., Hirao, Y., Itow, Y., Kawasaki, K., Koshimoto, N., Li, M. C. A., Ling, C. H., Masuda, K., Matsubara, Y., Muraki, Y., Miyazaki, S., Nagakane, M., Ohnishi, K., Rattenbury, N., Saito, T. O., Sharan, A., Shibai, H., Sullivan, D. J., Sumi, T., Suzuki, D., Tristram, P. J., Yamada, T., Yonehara, A., Figuera Jaimes, R, Calchi Novati, S, D’Ago, G, Jaimes, R Figuera, Novati, S Calchi, Astronomische Rechen-Institut [Heidelberg] (ARI), Zentrum für Astronomie der Universität Heidelberg (ZAH), Universität Heidelberg [Heidelberg]-Universität Heidelberg [Heidelberg], M2A 2019, Laboratoire d'Astrophysique de Bordeaux [Pessac] (LAB), Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Senckenberg Institute, Geophysical Laboratory [Carnegie Institution], Carnegie Institution for Science [Washington], NSF Center for EUV Science and Technology, NSF, Ifremer (COP), Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER), CSNSM PCI, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), School of Chemical and Physical Sciences [Keele], Keele University [Keele], Okayama Astrophysical Observatory, National Astronomical Observatory of Japan (NAOJ), Department of Materials Science [Tokyo], Tokyo Institute of Technology [Tokyo] (TITECH), Laboratory for Intelligent Systems and Informatics, Department of Mechano-Informatics Graduate School of Information Science and Technology, University of Tokyo, Tokyo, Japan (ISI laboratory), University of Tokyo (UTokyo), Atmosphere and Ocean Research Institute [Kashiwa-shi] (AORI), Institut d'Astrophysique de Paris (IAP), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), NASA Goddard Space Flight Center (GSFC), Astronomical Observatory [Warsaw], Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), Space Science Department of ESA, European Space Research and Technology Centre (ESTEC), European Space Agency (ESA)-European Space Agency (ESA), Max-Planck-Institut für Sonnensystemforschung (MPS), Max-Planck-Gesellschaft, Max-Planck-Institut für Astronomie (MPIA), Ohio State University [Columbus] (OSU), Niels Bohr Institute [Copenhagen] (NBI), Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (KU)-University of Copenhagen = Københavns Universitet (KU), Kuopio Unit [FMI], Finnish Meteorological Institute (FMI), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), University of Copenhagen = Københavns Universitet (KU), Argelander Institute for Astronomy (AlfA), Rheinische Friedrich-Wilhelms-Universität Bonn, Instituto de Astrofisica de Canarias (IAC), Nagoya University, Department of Physics [Notre Dame], University of Notre Dame [Indiana] (UND), University of Auckland [Auckland], Osaka University [Osaka], Tokyo University of Science [Tokyo], Department of Chemistry, Université de Tsukuba = University of Tsukuba, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Department of Earth and Space Science [Toyonaka-shi], Osaka University, Tokyo University Sci. Dept. Sci. & Technol., The University of Tokyo (UTokyo), Science & Technology Facilities Council, University of St Andrews. St Andrews Centre for Exoplanet Science, University of St Andrews. School of Physics and Astronomy, Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Agence Spatiale Européenne = European Space Agency (ESA)-Agence Spatiale Européenne = European Space Agency (ESA), Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research (MPS), University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH), University of Copenhagen = Københavns Universitet (UCPH), and Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: GRAVITATIONAL LENS, T-EFF, Event (relativity), observational [methods], Binary number, Galaxy: Bulge, gravitational lensing: Micro, methods: Observational, techniques: Photometric, Astrophysics, gravitational lensing: micro, GALACTIC BULGE, 01 natural sciences, Galaxy: bulge, photometric [techniques], techniques: photometric, Bulge, Observatory, QB Astronomy, NETWORK, 010303 astronomy & astrophysics, QC, ComputingMilieux_MISCELLANEOUS, QB, Physics, Earth and Planetary Astrophysics (astro-ph.EP), MILKY-WAY, Astrophysics::Earth and Planetary Astrophysics, methods: observational, Astrophysics - Instrumentation and Methods for Astrophysics, [PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], bulge [Galaxy], FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Gravitational microlensing, Settore FIS/05 - Astronomia e Astrofisica, SYSTEMS, SEARCH, 0103 physical sciences, ALGORITHM, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astrophysics::Galaxy Astrophysics, 010308 nuclear & particles physics, Order (ring theory), DAS, Astronomy and Astrophysics, Light curve, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], QC Physics, Space and Planetary Science, [SDU]Sciences of the Universe [physics], DISCOVERY, astro-ph.EP, micro [gravitational lensing], Parallax, astro-ph.IM, Astrophysics - Earth and Planetary Astrophysics, PLANETS, QB799
Abstract: We present the analysis of stellar binary microlensing event OGLE-2015-BLG-0060 based on observations obtained from 13 different telescopes. Intensive coverage of the anomalous parts of the light curve was achieved by automated follow-up observations from the robotic telescopes of the Las Cumbres Observatory. We show that, for the first time, all main features of an anomalous microlensing event are well covered by follow-up data, allowing us to estimate the physical parameters of the lens. The strong detection of second-order effects in the event light curve necessitates the inclusion of longer-baseline survey data in order to constrain the parallax vector. We find that the event was most likely caused by a stellar binary-lens with masses $M_{\star1} = 0.87 \pm 0.12 M_{\odot}$ and $M_{\star2} = 0.77 \pm 0.11 M_{\odot}$. The distance to the lensing system is 6.41 $\pm 0.14$ kpc and the projected separation between the two components is 13.85 $\pm 0.16$ AU. Alternative interpretations are also considered., Comment: 13 pages, 5 figures, Published in MNRAS
Published: 2019
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29. OGLE-2015-BLG-1649Lb: A gas giant planet around a low-mass dwarf

Author: M. Hundertmark, Man Cheung Alex Li, Nicholas J. Rattenbury, Jan Skowron, R. W. Schmidt, Igor Soszyński, Daisuke Suzuki, Yasushi Muraki, Y. Kamei, Atsunori Yonehara, Arnaud Cassan, Jean-Philippe Beaulieu, Jesper Skottfelt, Keith Horne, S. Kozlowski, Heidi Korhonen, Ian A. Bond, D. M. Bramich, Akihiko Fukui, Clément Ranc, John Southworth, Michael I. Andersen, Masayuki Nagakane, Martin Donachie, Denis J. Sullivan, Etienne Bachelet, Joachim Wambsganss, Richard K. Barry, Hirosane Fujii, Iain A. Steele, Nuno Peixinho, Andrzej Udalski, Michał K. Szymański, J. W. Menzies, Aparna Bhattacharya, U. G. Jørgensen, Yiannis Tsapras, Shota Miyazaki, Martin Burgdorf, Sohrab Rahvar, Yutaka Matsubara, Tobias C. Hinse, M. Rabus, Krzysztof Ulaczyk, Paul J. Tristram, P. Mróz, Haruno Suematsu, Giuseppe D'Ago, T. Yamakawa, Chien-Hsiu Lee, Daniel F. Evans, Shude Mao, Fumio Abe, Colin Snodgrass, Valerio Bozza, P. Pietrukowicz, Radosław Poleski, Naoki Koshimoto, Martin Dominik, R. Figuera Jaimes, Yuki Hirao, Iona Kondo, Taro Matsuo, Rachel Street, Takahiro Sumi, David P. Bennett, Yoshitaka Itow, Hiroshi Shibai, P. Longa, Osaka University [Osaka], Astronomical Observatory [Warsaw], Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), Institut d'Astrophysique de Paris (IAP), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Department of Physics [Notre Dame], University of Notre Dame [Indiana] (UND), University of Auckland [Auckland], Nagoya University, Department of Physics [Osaka], Osaka University, NASA Goddard Space Flight Center (GSFC), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Max-Planck-Institut für Astronomie (MPIA), Max-Planck-Gesellschaft, Ohio State University [Columbus] (OSU), Space Science Department of ESA, European Space Research and Technology Centre (ESTEC), European Space Agency (ESA)-European Space Agency (ESA), Max-Planck-Institut für Sonnensystemforschung (MPS), Niels Bohr Institute [Copenhagen] (NBI), Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (KU)-University of Copenhagen = Københavns Universitet (KU), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), University of Copenhagen = Københavns Universitet (KU), Kuopio Unit [FMI], Finnish Meteorological Institute (FMI), Instituto de Astrofisica de Canarias (IAC), University of St Andrews. School of Physics and Astronomy, University of St Andrews. St Andrews Centre for Exoplanet Science, Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Agence Spatiale Européenne = European Space Agency (ESA)-Agence Spatiale Européenne = European Space Agency (ESA), Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research (MPS), University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH), and University of Copenhagen = Københavns Universitet (UCPH)
Subjects: Gas giant, Exoplanet astronomy, NDAS, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Gravitational microlensing, 01 natural sciences, 0103 physical sciences, QB Astronomy, Astrophysics::Solar and Stellar Astrophysics, 010306 general physics, 010303 astronomy & astrophysics, QB600, QC, Astrophysics::Galaxy Astrophysics, QB, Earth and Planetary Astrophysics (astro-ph.EP), Physics, Exoplanet astronomy (486), Astronomy, Astronomy and Astrophysics, QC Physics, Space and Planetary Science, astro-ph.EP, Astrophysics::Earth and Planetary Astrophysics, Low Mass, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Gravitational microlensing (672), QB799, Astrophysics - Earth and Planetary Astrophysics
Abstract: 著者人数: 69名 (所属. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS): 鈴木, 大介), Number of authors: 69 (Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS): Suzuki, Daisuke), Accepted: 2019-09-25, 資料番号: SA1190157000
Published: 2019
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30. Circular Pattern Matching with $k$ Mismatches

Author: Solon P. Pissis, Tomasz Waleń, Tomasz Kociumaka, Juliusz Straszyński, Wiktor Zuba, Jakub Radoszewski, Wojciech Rytter, Panagiotis Charalampopoulos, Centrum Wiskunde & Informatica, Amsterdam (CWI), The Netherlands, Department of Informatics [King's College London], King‘s College London, Department of Computer Science at Bar Ilan University, Bar-Ilan University [Israël], Institute of Informatics, University of Warsaw, Centrum Wiskunde & Informatica (CWI), Equipe de recherche européenne en algorithmique et biologie formelle et expérimentale (ERABLE), Inria Grenoble - Rhône-Alpes, Institut National de Recherche en Informatique et en Automatique (Inria)-Institut National de Recherche en Informatique et en Automatique (Inria), Bioinformatics, AIMMS, Bio Informatics (IBIVU), Institute of Informatics [Warsaw], Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), and University of Warsaw (UW)-University of Warsaw (UW)
Subjects: FOS: Computer and information sciences, 050101 languages & linguistics, General Computer Science, Computer Networks and Communications, 0102 computer and information sciences, 02 engineering and technology, 01 natural sciences, Theoretical Computer Science, Combinatorics, Approximate pattern matching, k-mismatch problem, 020204 information systems, Computer Science - Data Structures and Algorithms, 0202 electrical engineering, electronic engineering, information engineering, Data Structures and Algorithms (cs.DS), [INFO]Computer Science [cs], 0501 psychology and cognitive sciences, Pattern matching, Mathematics, Applied Mathematics, 05 social sciences, Cyclic shift, Hamming distance, Substring, Circular pattern matching, Computational Theory and Mathematics, 010201 computation theory & mathematics, 020201 artificial intelligence & image processing
Abstract: The $k$-mismatch problem consists in computing the Hamming distance between a pattern $P$ of length $m$ and every length-$m$ substring of a text $T$ of length $n$, if this distance is no more than $k$. In many real-world applications, any cyclic rotation of $P$ is a relevant pattern, and thus one is interested in computing the minimal distance of every length-$m$ substring of $T$ and any cyclic rotation of $P$. This is the circular pattern matching with $k$ mismatches ($k$-CPM) problem. A multitude of papers have been devoted to solving this problem but, to the best of our knowledge, only average-case upper bounds are known. In this paper, we present the first non-trivial worst-case upper bounds for the $k$-CPM problem. Specifically, we show an $O(nk)$-time algorithm and an $O(n+\frac{n}{m}\,k^4)$-time algorithm. The latter algorithm applies in an extended way a technique that was very recently developed for the $k$-mismatch problem [Bringmann et al., SODA 2019]. A preliminary version of this work appeared at FCT 2019. In this version we improve the time complexity of the main algorithm from $O(n+\frac{n}{m}\,k^5)$ to $O(n+\frac{n}{m}\,k^4)$., Extended version of a paper from FCT 2019
Published: 2019
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31. Laser Spectroscopy of Neutron-Rich Tin Isotopes: A Discontinuity in Charge Radii across the N=82 Shell Closure

Author: C. Gorges, Mark Bissell, Klaus Blaum, Paul-Gerhard Reinhard, L. Xie, Ziye Xu, D. L. Balabanski, Magda Kowalska, S. Sailer, L. Wehner, S. Kaufmann, Georgi Georgiev, Deyan Yordanov, W. Gins, L. V. Rodríguez, R. F. Garcia Ruiz, Stefan E. Schmidt, H. Heylen, Witold Nazarewicz, Rainer Neugart, A. Kanellakopoulos, Xiaofei Yang, Wilfried Nörtershäuser, Gerda Neyens, B. Maaß, Bradley Cheal, S. Malbrunot-Ettenauer, S. Lechner, V. Lagaki, C. Wraith, R. Sánchez, Helmholtz zentrum für Schwerionenforschung GmbH (GSI), Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Instituut voor Kern- en Stralingsfysica (K.U. LEUVEN), Catholic University of Leuven - Katholieke Universiteit Leuven (KU Leuven), Landessternwarte Königstuhl [ZAH] (LSW), Universität Heidelberg [Heidelberg], Institute of Theoretical Physics [Warsaw], Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), Instituut voor Kern-en Stralingsfysica (IKS), Institute for Tropospheric Research (IFT), and Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Physics, Multidisciplinary, General Physics and Astronomy, chemistry.chemical_element, LINE, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], 01 natural sciences, Effective nuclear charge, FORCE, Charge radius, DEPENDENCE, MOMENTS, 0103 physical sciences, Isotopes of tin, Neutron, ddc:530, Nuclear Physics - Experiment, 010306 general physics, Spectroscopy, Nuclear Experiment, ComputingMilieux_MISCELLANEOUS, Physics, Science & Technology, NUCLEI, ddc, chemistry, Pairing, Physical Sciences, Atomic physics, Tin, Nuclear density
Abstract: Physical review letters 122(19), 192502 (2019). doi:10.1103/PhysRevLett.122.192502, Published by APS, College Park, Md.
Published: 2019
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32. Optimizing egalitarian performance when colocating tasks with types for cloud data center resource management

Author: Krzysztof Rzadca, Fanny Pascual, Recherche Opérationnelle (RO), LIP6, Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institute of Informatics [Warsaw], Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), and University of Warsaw (UW)-University of Warsaw (UW)
Subjects: Theoretical computer science, Computer science, [INFO.INFO-DS]Computer Science [cs]/Data Structures and Algorithms [cs.DS], 02 engineering and technology, Scheduling (computing), 0202 electrical engineering, electronic engineering, information engineering, Resource management, scheduling, Cluster analysis, approximation algorithm, 020203 distributed computing, Job shop scheduling, co-tenancy, cloud computing, Approximation algorithm, [INFO.INFO-RO]Computer Science [cs]/Operations Research [cs.RO], workload co-location, Computational Theory and Mathematics, Hardware and Architecture, Signal Processing, Task analysis, Combinatorial optimization, heterogeneity, [INFO.INFO-DC]Computer Science [cs]/Distributed, Parallel, and Cluster Computing [cs.DC], Heuristics, complexity
Abstract: In data centers, up to dozens of tasks are colocated on a single physical machine. Machines are used more efficiently, but the performance of the tasks deteriorates, as the colocated tasks compete for shared resources. Since the tasks are heterogeneous, the resulting performance dependencies are complex. In our previous work [1] , [2] we proposed a new combinatorial optimization model that uses two parameters of a task — its size and its type — to characterize how a task influences the performance of other tasks allocated to the same machine. In this paper, we study the egalitarian optimization goal: the aim is to optimize the performance of the worst-off task. This problem generalizes the classic makespan minimization on multiple processors ($P||C_{\max }$P||Cmax). We prove that polynomially-solvable variants of $P||C_{\max }$P||Cmax are NP-hard for this generalization, and that the problem is hard to approximate when the number of types is not constant. For a constant number of types, we propose a PTAS, a fast approximation algorithm, and a series of heuristics. We simulate the algorithms on instances derived from a trace of one of Google clusters. Compared with baseline algorithms solving $P||C_{\max }$P||Cmax, our proposed algorithms aware of the types of the jobs lead to significantly better tasks’ performance. The notion of type enables us to extend standard combinatorial optimization methods to handle degradation of performance caused by colocation. Types add a layer of additional complexity. However, our results — approximation algorithms and good average-case performance — show that types can be handled efficiently.
Published: 2019
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33. Cell Wall Hydrolases in Bacteria: Insight on the Diversity of Cell Wall Amidases, Glycosidases and Peptidases Toward Peptidoglycan

Author: Vermassen, Aurore, Leroy, Sabine, Talon, Régine, Provot, Christian, Popowska, Magdalena, Desvaux, Mickael, Microbiologie Environnement Digestif Santé (MEDIS), INRA Clermont-Ferrand-Theix-Université Clermont Auvergne [2017-2020] (UCA [2017-2020]), BioFilm Control, Department of Applied Microbiology [Warsaw], Institute of Microbiology [Warsaw], Faculty of Biology [Warsaw], University of Warsaw (UW)-University of Warsaw (UW)-Faculty of Biology [Warsaw], University of Warsaw (UW)-University of Warsaw (UW), NRA (Institut National de la Recherche Agronomique), DeESSe project from the Region Auvergne, FEDER (Fonds Europeen de Developpement Regional), Polish National Center of Science 2013/09/B/NZ6/00710, Campus France PHC (Programme Hubert Curien) France-Poland POLONIUM 28298ZE, Bourse Innovation Transfert de Technologie, and Institut National de la Recherche Agronomique (INRA)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])
Subjects: cell wall binding domains, [SDV]Life Sciences [q-bio], Microbiology and Parasitology, lyse cellulaire, lcsh:QR1-502, Review, Microbiology, cell wall remodeling, Microbiologie et Parasitologie, lcsh:Microbiology, bacterial cell wall, peptidoglycan (PG) hydrolases, protein modules, bacterial division and growth, cell lysis, paroi cellulaire
Abstract: International audience; The cell wall (CW) of bacteria is an intricate arrangement of macromolecules, at least constituted of peptidoglycan (PG) but also of (lipo)teichoic acids, various polysaccharides, polyglutamate and/or proteins. During bacterial growth and division, there is a constant balance between CW degradation and biosynthesis. The CW is remodeled by bacterial hydrolases, whose activities are carefully regulated to maintain cell integrity or lead to bacterial death. Each cell wall hydrolase (CWH) has a specific role regarding the PG: (i) cell wall amidase (CWA) cleaves the amide bond between N-acetylmuramic acid and L-alanine residue at the N-terminal of the stem peptide, (ii) cell wall glycosidase (CWG) catalyses the hydrolysis of the glycosidic linkages, whereas (iii) cell wall peptidase (CWP) cleaves amide bonds between amino acids within the PG chain. After an exhaustive overview of all known conserved catalytic domains responsible for CWA, CWG, and CWP activities, this review stresses that the CWHs frequently display a modular architecture combining multiple and/or different catalytic domains, including some lytic transglycosylases as well as CW binding domains. From there, direct physiological and collateral roles of CWHs in bacterial cells are further discussed.
Published: 2019
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34. Computing the Width of Non-deterministic Automata

Author: Kuperberg, Denis, Majumdar, Anirban, Institute of Mathematics [Warsaw], Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), and University of Warsaw (UW)-University of Warsaw (UW)
Subjects: FOS: Computer and information sciences, [INFO.INFO-FL]Computer Science [cs]/Formal Languages and Automata Theory [cs.FL], Formal Languages and Automata Theory (cs.FL), Computer Science::Logic in Computer Science, Computer Science - Formal Languages and Automata Theory, Nonlinear Sciences::Cellular Automata and Lattice Gases, Computer Science::Formal Languages and Automata Theory
Abstract: International audience; We introduce a measure called width, quantifying the amount of nondetermin-ism in automata. Width generalises the notion of good-for-games (GFG) automata, that correspond to NFAs of width 1, and where an accepting run can be built on-the-fly on any accepted input. We describe an incremental determinisation construction on NFAs, which can be more efficient than the full powerset determinisation, depending on the width of the input NFA. This construction can be generalised to infinite words, and is particularly well-suited to coBüchi automata. For coBüchi automata, this procedure can be used to compute either a deterministic automaton or a GFG one, and it is algorithmically more efficient in the last case. We show this fact by proving that checking whether a coBüchi automaton is determinisable by pruning is NP-complete. On finite or infinite words, we show that computing the width of an automaton is EXPTIME-complete. This implies EXPTIME-completeness for multipebble simulation games on NFAs.
Published: 2019
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35. Evidence-Based Consensus and Systematic Review on Reducing the Time to Diagnosis of Duchenne Muscular Dystrophy

Author: Annemieke Aartsma-Rus, Madhuri Hegde, Tawfeg Ben-Omran, Filippo Buccella, Alessandra Ferlini, Pia Gallano, R. Rodney Howell, France Leturcq, Ann S. Martin, Anna Potulska-Chromik, Jonas A. Saute, Wolfgang M. Schmidt, Thomas Sejersen, Sylvie Tuffery-Giraud, Zehra Oya Uyguner, Luci A. Witcomb, Shu Yau, Stanley F. Nelson, Human Genetics, Weill Cornell Medical College in Qatar (WCMC-Q), Weill Cornell Medicine [Qatar], Department of Experimental and Diagnostic Medicine, Section of Medical Genetics, Università degli Studi di Ferrara (UniFE), Biochimie et Génétique Moléculaire, Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Hôpital Cochin [AP-HP], Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP), Department of Embryology [Warsaw], Institute of Zoology [Warsaw], Faculty of Biology [Warsaw], University of Warsaw (UW)-University of Warsaw (UW)-Faculty of Biology [Warsaw], University of Warsaw (UW)-University of Warsaw (UW), Forschungszentrum Julich, JCNS, D-52425 Julich, Germany, Karolinska Institutet [Stockholm], Laboratoire de génétique des maladies rares. Pathologie moleculaire, etudes fonctionnelles et banque de données génétiques (LGMR), IFR3, and Université Montpellier 1 (UM1)-Université Montpellier 1 (UM1)-Université de Montpellier (UM)-Institut National de la Santé et de la Recherche Médicale (INSERM)
Subjects: Male, Pediatrics, medicine.medical_specialty, Evidence-based practice, Consensus, Time Factors, Delphi Technique, Evidence-Based Medicine, Female, Humans, Muscular Dystrophy, Duchenne, Practice Guidelines as Topic, [SDV]Life Sciences [q-bio], Duchenne muscular dystrophy, MEDLINE, NO, 03 medical and health sciences, 0302 clinical medicine, medicine, LS2_6, Muscular Dystrophy, Muscular dystrophy, ComputingMilieux_MISCELLANEOUS, 030304 developmental biology, 0303 health sciences, Tempo para o tratamento, business.industry, Diagnóstico, medicine.disease, Duchenne, 3. Good health, Distrofia muscular de Duchenne, Pediatrics, Perinatology and Child Health, business, 030217 neurology & neurosurgery, Time to diagnosis
Abstract: International audience
Published: 2019
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36. The modular distribution of Stern’s sequence

Author: Andrzej Schinzel, Jean-Marc Deshouillers, Institut de Mathématiques de Bordeaux (IMB), Université Bordeaux Segalen - Bordeaux 2-Université Sciences et Technologies - Bordeaux 1-Université de Bordeaux (UB)-Institut Polytechnique de Bordeaux (Bordeaux INP)-Centre National de la Recherche Scientifique (CNRS), Institute of Mathematics [Warsaw], Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), and University of Warsaw (UW)-University of Warsaw (UW)
Subjects: Combinatorics, Stern, Distribution (number theory), business.industry, General Earth and Planetary Sciences, Modular design, business, ComputingMilieux_MISCELLANEOUS, [MATH.MATH-NT]Mathematics [math]/Number Theory [math.NT], General Environmental Science, Mathematics, Sequence (medicine)
Abstract: International audience
Published: 2019
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37. Microfluidic measurement of the dissolution rate of gypsum in water using the reactive infiltration-instability

Author: Piotr Szymczak, Olgierd Cybulski, Florian Osselin, Piotr Garstecki, Paweł Kondratiuk, Institut des Sciences de la Terre d'Orléans - UMR7327 (ISTO), Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Bureau de Recherches Géologiques et Minières (BRGM) (BRGM), Milieux Poreux - UMR7327, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Bureau de Recherches Géologiques et Minières (BRGM) (BRGM)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institute of Theoretical Physics [Warsaw], Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), and Institute of Physical Chemistry Polish Academy of Sciences
Subjects: lcsh:GE1-350, Gypsum, Materials science, 010504 meteorology & atmospheric sciences, engineering.material, Gypsum block, 010502 geochemistry & geophysics, 01 natural sciences, Instability, Volumetric flow rate, Damköhler numbers, Infiltration (hydrology), Wavelength, [SDU]Sciences of the Universe [physics], engineering, Composite material, Dissolution, lcsh:Environmental sciences, 0105 earth and related environmental sciences
Abstract: International audience; We present an original method for measuring the intrinsic dissolution rate of gypsum. We use a simple microfluidic setup, with a gypsum block inserted between two polycarbonate plates, which is dissolved by water. By changing the flow rate and the distance between the plates, we can scan a wide range of Péclet and Damköhler numbers, characterizing the relative magnitude of advection, diffusion and reaction in the system. We find the dissolution to be unstable, with a formation of a characteristic fingering pattern. The dissolution rate can then be calculated from the initial wavelength of this pattern. Alternatively, it can also be estimated from the time it takes for the gypsum chip to get completely dissolved near the inlet channel. The method presented here is general and can be used to assess the dissolution rates of other minerals.
Published: 2019
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38. Effects of climate change and horticultural use on the spread of naturalized alien garden plants in Europe

Author: Klonner, Günther, Wessely, Johannes, Gattringer, Andreas, Moser, Dietmar, Dullinger, Iwona, Hülber, Karl, Rumpf, Sabine B., Block, Svenja, Bossdorf, Oliver, Carboni, Marta, Conti, Luisa, Dawson, Wayne, Haeuser, Emily, Hermy, Martin, Münkemüller, Tamara, Parepa, Madalin, Thuiller, Wilfried, Van der Veken, Sebastiaan, Verheyen, Kris, van Kleunen, Mark, Essl, Franz, Dullinger, Stefan, Universität Wien, Eberhard Karls Universität Tübingen = Eberhard Karls University of Tuebingen, Laboratoire d'Ecologie Alpine (LECA ), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Università degli Studi Roma Tre, Department of Ecology [Warsaw], Institute of Zoology [Warsaw], Faculty of Biology [Warsaw], University of Warsaw (UW)-University of Warsaw (UW)-Faculty of Biology [Warsaw], University of Warsaw (UW)-University of Warsaw (UW), Université Catholique de Louvain = Catholic University of Louvain (UCL), Klonner, G., Wessely, J., Gattringer, A., Moser, D., Dullinger, I., Hulber, K., Rumpf, S. B., Block, S., Bossdorf, O., Carboni, M., Conti, L., Dawson, W., Haeuser, E., Hermy, M., Munkemuller, T., Parepa, M., Thuiller, W., Van der Veken, S., Verheyen, K., van Kleunen, M., Essl, F., and Dullinger, S.
Subjects: NICHE SHIFTS, DYNAMICS, range dynamics, Evolution, Plant naturalization, Biodiversity & Conservation, MODELS, biological invasions, biological invasion, Environmental Sciences & Ecology, Behavior and Systematics, INTRODUCTION HISTORY, propagule pressure, DISTURBANCE, ACCUMULATION, Science & Technology, Ecology, horticulture, Biology and Life Sciences, FRAMEWORK, PROPAGULE PRESSURE, DEBT, plant naturalization, climate change, Biodiversity Conservation, [SDV.EE.BIO]Life Sciences [q-bio]/Ecology, environment/Bioclimatology, [SDE.BE]Environmental Sciences/Biodiversity and Ecology, Life Sciences & Biomedicine, TRAITS
Abstract: International audience; Climate warming is supposed to enlarge the area climatically suitable to the naturalization of alien garden plants in temperate regions. However, the effects of a changing climate on the spread of naturalized ornamentals have not been evaluated by spatially and temporarily explicit range modelling at larger scales so far. Here, we assess how climate change and the frequency of cultivation interactively determine the spread of 15 ornamental plants over the 21st century in Europe. We coupled species distribution modelling with simulations of demography and dispersal to predict range dynamics of these species in annual steps across a 250 x 250 m raster of the study area. Models were run under four scenarios of climate warming and six levels of cultivation intensity. Cultivation frequency was implemented as size of the area used for planting a species. Although the area climatically suitable to the 15 species increases, on average, the area predicted to be occupied by them in 2090 shrinks under two of the three climate change scenarios. This contradiction obviously arises from dispersal limitations that were pronounced although we assumed that cultivation is spatially adapting to the changing climate. Cultivation frequency had a much stronger effect on species spread than climate change, and this effect was non-linear. The area occupied increased sharply from low to moderate levels of cultivation intensity, but levelled off afterwards. Our simulations suggest that climate warming will not necessarily foster the spread of alien garden plants in Europe over the next decades. However, climatically suitable areas do increase and hence an invasion debt is likely accumulating. Restricting cultivation of species can be effective in preventing species spread, irrespective of how the climate develops. However, for being successful, they depend on high levels of compliance to keep propagule pressure at a low level.
Published: 2019
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39. On the long cycle variability of the Algol OGLE-LMC-DPV-065 and its stellar, orbital and disk parameters

Author: L. Celedón, Nicola Astudillo-Defru, Igor Soszyński, Ashish Raj, Claus Tappert, José G. Fernández-Trincado, Th. Rivinius, Linda Schmidtobreick, Petr Hadrava, G. Djurašević, Neustroev, Radosław Poleski, Ronald E. Mennickent, M. Cabezas, I. Porritt, European Southern Observatory [Santiago] (ESO), European Southern Observatory (ESO), Ohio State University [Columbus] (OSU), Astronomical Observatory [Warsaw], Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), Universidad de Concepción [Chile], Univers, Transport, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UMR 6213) (UTINAM), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Franche-Comté (UFC), Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC), Instituto de Astronomia y ciencias Planetarias de Atacama (INCT), and Universidad de Atacama
Subjects: FOS: Physical sciences, Astrophysics, 01 natural sciences, 0103 physical sciences, Thick disk, Circular orbit, close, 010303 astronomy & astrophysics, ComputingMilieux_MISCELLANEOUS, Solar and Stellar Astrophysics (astro-ph.SR), Physics, 010308 nuclear & particles physics, Astronomy and Astrophysics, Radius, activity [spectroscopic - stars], Mass ratio, Orbital period, Light curve, Orbit, Stars, Astrophysics - Solar and Stellar Astrophysics, 13. Climate action, Space and Planetary Science, binaries: eclipsing [stars], circumstellar matter - fundamental parameters, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: OGLE-LMC-DPV-065 is an interacting binary whose double-hump long photometric cycle remains hitherto unexplained. We analyze photometric time series available in archive datasets spanning 124 years and present the analysis of new high-resolution spectra. A refined orbital period is found of 10\fd0316267 $\pm$ 0\fd0000056 without any evidence of variability. In spite of this constancy, small but significant changes in timings of the secondary eclipse are detected. We show that the long period continuously decreases from 350 to 218 days during 13 years, then remains almost constant for about 10 years. Our study of radial velocities indicates a circular orbit for the binary and yields a mass ratio of 0.203 $\pm$ 0.001. From the analysis of the orbital light curve we find that the system contains 13.8 and 2.81 \msun\ stars of radii 8.8 and 12.6 \rsun\ and absolute bolometric magnitudes -6.4 and -3.0, respectively. The orbit semi-major axis is 49.9 \rsun\ and the stellar temperatures are 25460 K and 9825 K. We find evidence for an optically and geometrically thick disk around the hotter star. According to our model, the disk has a radius of 25 \rsun, central and outer vertical thickness of 1.6 \rsun\ and 3.5 \rsun, and temperature of 9380 K at its outer edge. Two shock regions located at roughly opposite parts of the outer disk rim can explain the light curves asymmetries. The system is a member of the double periodic variables and its relatively high-mass and long photometric cycle make it similar in some aspects to $\beta$ Lyrae., Comment: Accepted for publication in MNRAS main journal
Published: 2019
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40. Linear Search by a Pair of Distinct-Speed Robots

Author: Tomasz Kociumaka, Jurek Czyzowicz, David Ilcinkas, Leszek Gąsieniec, Ralf Klasing, Dominik Pająk, Evangelos Bampas, School of of Electrical and Computer Engineering [Athens] (School of E.C.E), National Technical University of Athens [Athens] (NTUA), Département d'Informatique et d'Ingénierie (DII), Université du Québec en Outaouais (UQO), Department of Computer Science [Liverpool], University of Liverpool, Laboratoire Bordelais de Recherche en Informatique (LaBRI), Université de Bordeaux (UB)-Centre National de la Recherche Scientifique (CNRS)-École Nationale Supérieure d'Électronique, Informatique et Radiocommunications de Bordeaux (ENSEIRB), University of Warsaw (UW), Institute of informatics [Wrocław], See paper for details., ANR-11-BS02-0014,DISPLEXITY,Calculabilité et complexité en distribué(2011), ANR-13-JS02-0002,MACARON,Bouger et Calculer: Agents, Robots et Réseaux(2013), ANR-16-CE40-0023,DESCARTES,Abstraction modulaire pour le calcul distribué(2016), ANR-10-IDEX-0003,IDEX BORDEAUX,Initiative d'excellence de l'Université de Bordeaux(2010), Massachusetts Institute of Technology. Computer Science and Artificial Intelligence Laboratory, Pajak, Dominik S, Laboratoire d'informatique Fondamentale de Marseille (LIF), Aix Marseille Université (AMU)-École Centrale de Marseille (ECM)-Centre National de la Recherche Scientifique (CNRS), Université de Bordeaux (UB)-École Nationale Supérieure d'Électronique, Informatique et Radiocommunications de Bordeaux (ENSEIRB)-Centre National de la Recherche Scientifique (CNRS), Institute of Informatics [Warsaw], Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), University of Warsaw (UW)-University of Warsaw (UW), and Centre National de la Recherche Scientifique (CNRS)-École Centrale de Marseille (ECM)-Aix Marseille Université (AMU)
Subjects: Engineering, General Computer Science, Computer science, different speeds, [INFO.INFO-DS]Computer Science [cs]/Data Structures and Algorithms [cs.DS], 0211 other engineering and technologies, 0102 computer and information sciences, 02 engineering and technology, Bang-bang robot, linear search, 01 natural sciences, Article, Computer Science::Robotics, Position (vector), mobile robots, 0202 electrical engineering, electronic engineering, information engineering, Cartesian coordinate robot, Point (geometry), Computer vision, [INFO]Computer Science [cs], Online algorithm, Simulation, Linear search, 021103 operations research, business.industry, Applied Mathematics, Mobile robot, Computer Science Applications, 010201 computation theory & mathematics, group search, Moment (physics), Line (geometry), Robot, 020201 artificial intelligence & image processing, Artificial intelligence, [INFO.INFO-DC]Computer Science [cs]/Distributed, Parallel, and Cluster Computing [cs.DC], business
Abstract: Two mobile robots are initially placed at the same point on an infinite line. Each robot may move on the line in either direction not exceeding its maximal speed. The robots need to find a stationary target placed at an unknown location on the line. The search is completed when both robots arrive at the target point. The target is discovered at the moment when either robot arrives at its position. The robot knowing the placement of the target may communicate it to the other robot. We look for the algorithm with the shortest possible search time (i.e. the worst-case time at which both robots meet at the target) measured as a function of the target distance from the origin (i.e. the time required to travel directly from the starting point to the target at unit velocity). We consider two standard models of communication between the robots, namely wireless communication and communication by meeting. In the case of communication by meeting, a robot learns about the target while sharing the same location with a robot possessing this knowledge. We propose here an optimal search strategy for two robots including the respective lower bound argument, for the full spectrum of their maximal speeds. This extends the main result of Chrobak et al. (in: Italiano, Margaria-Steffen, Pokorný, Quisquater, Wattenhofer (eds) Current trends in theory and practice of computer science, SOFSEM, 2015) referring to the exact complexity of the problem for the case when the speed of the slower robot is at least one third of the faster one. In the wireless communication model, a message sent by one robot is instantly received by the other robot, regardless of their current positions on the line. For this model, we design a strategy which is optimal whenever the faster robot is at most \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\sqrt{17}+4\approx 8.123$$\end{document}17+4≈8.123 times faster than the slower one. We also prove that otherwise the wireless communication offers no advantage over communication by meeting.
Published: 2019
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41. Flexibility vs. robustness in cell cycle regulation of timing of M-phase entry in Xenopus laevis embryo cell-free extract

Author: Malgorzata Kloc, Jacek Z. Kubiak, Mohammed El Dika, Robert Zdanowski, Mirosław Lachowicz, Jean Pierre Tassan, Jacek Malejczyk, Mateusz Dębowski, Claude Prigent, Institute of Applied Mathematics [Warsaw] (IMSM), Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), University of Warsaw (UW)-University of Warsaw (UW), Institut de Génétique et Développement de Rennes (IGDR), Université de Rennes (UR)-Centre National de la Recherche Scientifique (CNRS)-Structure Fédérative de Recherche en Biologie et Santé de Rennes ( Biosit : Biologie - Santé - Innovation Technologique ), Methodist Hospital Research Institute, Lebanese Ministry of Education, Structure Fédérative de Recherche en Biologie et Santé de Rennes ( Biosit : Biologie - Santé - Innovation Technologique )-Centre National de la Recherche Scientifique (CNRS)-Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES), and The Methodist Hospital Research Institute, 6670 Bertner Ave, Houston, TX 77030, USA.
Subjects: 0301 basic medicine, Embryology, Embryo, Nonmammalian, kinase, Cdc25, Xenopus, environment and public health, cdk1, Dephosphorylation, Xenopus laevis, 03 medical and health sciences, Cyclin-dependent kinase, CDC2 Protein Kinase, Animals, Protein Phosphatase 2, mitosis, [SDV.GEN]Life Sciences [q-bio]/Genetics, Cyclin-dependent kinase 1, Cell-Free System, biology, phosphorylation, Cell Cycle, dynamics, Protein phosphatase 2, Models, Theoretical, cdc25, biology.organism_classification, Cell biology, enzymes and coenzymes (carbohydrates), 030104 developmental biology, Biochemistry, network, biology.protein, Phosphorylation, biological phenomena, cell phenomena, and immunity, protein, Cell Division, Developmental Biology
Abstract: International audience; During the cell cycle, cyclin dependent kinase 1 (CDK1) and protein phosphatase 2A (PP2A) play major roles in the regulation of mitosis. CDK1 phosphorylates a series of substrates triggering M-phase entry. Most of these substrates are dephosphorylated by PP2A. To allow phosphorylation of CDK1 substrates, PP2A is progressively inactivated upon M-phase entry. We have shown previously that the interplay between these two activities determines the timing of M-phase entry. Slight diminution of CDK1 activity by the RO3306 inhibitor delays M-phase entry in a dose-dependent manner in Xenopus embryo cell-free extract, while reduction of PP2A activity by OA inhibitor accelerates this process also in a dose-dependent manner. However, when a mixture of RO3306 and OA is added to the extract, an intermediate timing of M-phase entry is observed. Here we use a mathematical model to describe and understand this interplay. Simulations showing acceleration and delay in M-phase entry match previously described experimental data. CDC25 phosphatase is a major activator of CDK1 and acts through CDK1 Tyr15 and Thr14 dephosphorylation. Addition of CDC25 activity to our mathematical model was also consistent with our experimental results. To verify whether our assumption that the dynamics of CDC25 activation used in this model are the same in all experimental variants, we analyzed the dynamics of CDC25 phosphorylation, which reflect its activation. We confirm that these dynamics are indeed very similar in control extracts and when RO3306 and OA are present separately. However, when RO3306 and OA are added simultaneously to the extract, activation of CDC25 is slightly delayed. Integration of this parameter allowed us to improve our model. Furthermore, the pattern of CDK1 dephosphorylation on Tyr15 showed that the real dynamics of CDK1 activation are very similar in all experimental variants. The model presented here accurately describes, in mathematical terms, how the interplay between CDK1, PP2A and CDC25 controls the flexible timing of M-phase entry.
Published: 2016
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42. Switching of exciton character in double InGaN/GaN quantum wells

Author: Suski, T., Staszczak, G., Korona, K., Pierre Lefebvre, Eva Monroy, Drozdz, P., Grzegorz Muziol, Skierbiszewski, C., Gibasiewicz, K., Perlin, P., Institute of High Pressure Physics [Warsaw] (IHPP), Polska Akademia Nauk = Polish Academy of Sciences (PAN), Institute of Experimental Physics [Warsaw] (IFD), Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), Laboratoire Charles Coulomb (L2C), Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Nanophysique et Semiconducteurs (NPSC), PHotonique, ELectronique et Ingénierie QuantiqueS (PHELIQS), Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut de Recherche Interdisciplinaire de Grenoble (IRIG), Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut de Recherche Interdisciplinaire de Grenoble (IRIG), and Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)
Subjects: Condensed Matter::Other, [PHYS.COND.CM-MS]Physics [physics]/Condensed Matter [cond-mat]/Materials Science [cond-mat.mtrl-sci], [SPI.OPTI]Engineering Sciences [physics]/Optics / Photonic, [SPI.NANO]Engineering Sciences [physics]/Micro and nanotechnologies/Microelectronics, Condensed Matter::Mesoscopic Systems and Quantum Hall Effect
Abstract: International audience; We study the inter-well excitonic coupling in a series of In0.17Ga0.83N/GaN Double QWs (DQWs) with varying central barrier width. We observe the switching between indirect IX (inter-well) and direct DX (intra-well) excitons, for thin barriers (2 nm or less), depending on the exciton density. This density is controlled, in cw-PL, by the pumping laser power density (LPD). Above a certain threshold, we observe a sudden change of the PL blue-shift, when switching from IXs (large slope) to DXs (weak slope). In time-resolved PL, the exciton density evolves as the PL intensity decays with time, and the switching occurs from DXs to IXs, after a certain characteristic time. The decay time of IXs is of the order of hundreds of s, whereas the decay time of DXs is shorter by three orders of magnitude. The switching thresholds in both cw- and TR-PL present clear exponential dependences upon the width of the central barrier, which demonstrates the role of carrier tunneling in the overall switching processes. The described effects were studied at T10K but we found that IXs persist up to T=300K pointing out the importance of large exciton biding energy in nitride QWs.
Published: 2018

43. Well-quasi-ordering $H$-contraction-free graphs

Author: Jean-Florent Raymond, Marcin Kamiński, Théophile Trunck, Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), University of Warsaw (UW), Algorithmes, Graphes et Combinatoire (ALGCO), Laboratoire d'Informatique de Robotique et de Microélectronique de Montpellier (LIRMM), Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Modèles de calcul, Complexité, Combinatoire (MC2), Laboratoire de l'Informatique du Parallélisme (LIP), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Recherche en Informatique et en Automatique (Inria)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Recherche en Informatique et en Automatique (Inria)-Centre National de la Recherche Scientifique (CNRS), Faculty of Mathematics, Informatics, and Mechanics [Warsaw], University of Warsaw ( UW ), Algorithmes, Graphes et Combinatoire ( ALGCO ), Laboratoire d'Informatique de Robotique et de Microélectronique de Montpellier ( LIRMM ), Université de Montpellier ( UM ) -Centre National de la Recherche Scientifique ( CNRS ) -Université de Montpellier ( UM ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de l'Informatique du Parallélisme ( LIP ), École normale supérieure - Lyon ( ENS Lyon ) -Université Claude Bernard Lyon 1 ( UCBL ), Université de Lyon-Université de Lyon-Institut National de Recherche en Informatique et en Automatique ( Inria ) -Centre National de la Recherche Scientifique ( CNRS ), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM), Centre National de la Recherche Scientifique (CNRS)-Université de Lyon-Institut National de Recherche en Informatique et en Automatique (Inria)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-École normale supérieure - Lyon (ENS Lyon)-Centre National de la Recherche Scientifique (CNRS)-Université de Lyon-Institut National de Recherche en Informatique et en Automatique (Inria)-Université Claude Bernard Lyon 1 (UCBL), and Université de Lyon-École normale supérieure - Lyon (ENS Lyon)
Subjects: FOS: Computer and information sciences, Discrete Mathematics (cs.DM), Well-quasi-ordering, Induced subgraph, 0102 computer and information sciences, G.2.2, [INFO.INFO-DM]Computer Science [cs]/Discrete Mathematics [cs.DM], [ MATH.MATH-CO ] Mathematics [math]/Combinatorics [math.CO], Forbidden contractions, 01 natural sciences, Combinatorics, Edge contraction, [MATH.MATH-CO]Mathematics [math]/Combinatorics [math.CO], FOS: Mathematics, Discrete Mathematics and Combinatorics, Mathematics - Combinatorics, 0101 mathematics, Contraction (operator theory), Mathematics, Applied Mathematics, 010102 general mathematics, Graph theory, [ INFO.INFO-DM ] Computer Science [cs]/Discrete Mathematics [cs.DM], Graph, 010201 computation theory & mathematics, 06A07, Combinatorics (math.CO), Computer Science - Discrete Mathematics
Abstract: A well-quasi-order is an order which contains no infinite decreasing sequence and no infinite collection of incomparable elements. In this paper, we consider graph classes defined by excluding one graph as contraction. More precisely, we give a complete characterization of graphs H such that the class of H-contraction-free graphs is well-quasi-ordered by the contraction relation. This result is the contraction analogue on the previous dichotomy theorems of Damsaschke [Induced subgraphs and well-quasi-ordering, Journal of Graph Theory, 14(4):427-435, 1990] on the induced subgraph relation, Ding [Subgraphs and well-quasi-ordering, Journal of Graph Theory, 16(5):489-502, 1992] on the subgraph relation, and B{\l}asiok et al. [Induced minors and well-quasi-ordering, ArXiv e-prints, 1510.07135, 2015] on the induced minor relation., Comment: 18 pages
Published: 2018
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44. Rotational variation of the linear polarisation of the asteroid (3200) Phaethon as evidence for inhomogeneity in its surface properties

Author: Yu. N. Krugly, Alberto Cellino, G. Ramsay, Saran Poshyachinda, R. Cutter, V. S. Dhillon, P. T. O'Brien, Kendall Ackley, K. Ulaczyk, Ph. Bendjoya, Martin Dyer, Z. Donchev, Galin Borisov, E. Thrane, D. Vernet, J. P. Rivet, Stefano Bagnulo, Duncan K. Galloway, Don Pollacco, E. Rol, Apostolos A. Christou, Maxime Devogele, L. Abe, Tanyu Bonev, Irina Belskaya, D. Steeghs, ITA, GBR, FRA, BGR, UKR, Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astrofisico di Torino (OATo), Istituto Nazionale di Astrofisica (INAF), European Southern Observatory [Santiago] (ESO), European Southern Observatory (ESO), Armagh Observatory [Armagh], Joseph Louis LAGRANGE (LAGRANGE), Université Côte d'Azur (UCA)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institute of Astronomy, Bulgarian Academy of Sciences (BAS), V.N. Karazin Kharkiv National University (KhNU), National Astronomical Observatory - Rozhen (NAO), Department of Physics and Astronomy [Sheffield], University of Sheffield [Sheffield], University of Minnesota System, Astronomical Institute Anton Pannekoek (AI PANNEKOEK), University of Amsterdam [Amsterdam] (UvA), Astronomical Observatory [Warsaw], Faculty of Physics [Warsaw] (FUW), and University of Warsaw (UW)-University of Warsaw (UW)
Subjects: Earth and Planetary Astrophysics (astro-ph.EP), Physics, [PHYS]Physics [physics], 010504 meteorology & atmospheric sciences, FOS: Physical sciences, Library science, Astronomy and Astrophysics, 01 natural sciences, law.invention, Planetarium, Max planck institute, Telescope, Spitzer Space Telescope, Space and Planetary Science, Asteroid, Observatory, law, 0103 physical sciences, National laboratory, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], 010303 astronomy & astrophysics, ComputingMilieux_MISCELLANEOUS, 0105 earth and related environmental sciences, Phaeton, Astrophysics - Earth and Planetary Astrophysics
Abstract: Asteroid (3200) Phaethon is a Near-Earth Apollo asteroid with an unusual orbit that brings it closer to the Sun than any other known asteroid. Its last close approach to the Earth was in mid-December 2017 and the next one will be on October 2026. Previous rotationally time-resolved spectroscopy of Phaethon showed that its spectral slope is slightly bluish, in agreement with its B/F taxonomic classification, but at some rotational phases, it changes to slightly reddish. Motivated by this result we performed time-resolved imaging polarimetry of Phaethon during its recent close approach to the Earth. Phaethon has a spin period of 3.604 hours and we found a variation of the linear polarisation with rotation. This seems to be a rare case in which such variation is unambiguously found, also a consequence of its fairly large amplitude. Combining this new information with the brightness and colour variation, as well as previously reported results from Arecibo radar observations, we conclude that there is no variation of the mineralogy across the surface of Phaeton. However, the observed change in the linear polarisation may be related to differences in the thickness of the surface regolith in different areas or local topographic features., 5 pages, 2 figures, MNRAS Letters
Published: 2018
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45. The Late-type Eclipsing Binaries in the Large Magellanic Cloud: Catalog of Fundamental Physical Parameters

Author: Łukasz Wyrzykowski, Bogumił Pilecki, Jakub Ostrowski, Dariusz Graczyk, Radosław Poleski, Igor Soszyński, K. Stępień, Mónica Taormina, Paweł Pietrukowicz, Piotr Wielgórski, Ian B. Thompson, Sandro Villanova, Andrzej Udalski, Michał K. Szymański, W. Narloch, P. Mróz, Jan Skowron, Alexandre Gallenne, Zbigniew Kołaczkowski, Pierre Kervella, Jesper Storm, Piotr Konorski, Bartłomiej Zgirski, Grzegorz Pietrzyński, M. Gorski, Krzysztof Ulaczyk, Paulina Karczmarek, Wolfgang Gieren, Radosław Smolec, Szymon Kozłowski, Nicolas Nardetto, Ksenia Suchomska, Canadian Forest Service Great Lakes Forestry Centre (NRC), Natural Resources Canada (NRCan), Universidad de Concepción [Chile], Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Joseph Louis LAGRANGE (LAGRANGE), Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Astronomical Observatory of the University of Warsaw, University of Warsaw (UW), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université Côte d'Azur (UCA)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Astronomical Observatory [Warsaw], Faculty of Physics [Warsaw] (FUW), and University of Warsaw (UW)-University of Warsaw (UW)
Subjects: Physics, [PHYS]Physics [physics], 010504 meteorology & atmospheric sciences, Late type, Astronomy, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Large Magellanic Cloud, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Solar and Stellar Astrophysics (astro-ph.SR), ComputingMilieux_MISCELLANEOUS, 0105 earth and related environmental sciences
Abstract: We present a determination of precise fundamental physical parameters of twenty detached, double- lined, eclipsing binary stars in the Large Magellanic Cloud (LMC) containing G- or early K-type giant stars. Eleven are new systems, the remaining nine are systems already analyzed by our team for which we present updated parameters. The catalogue results from our long-term survey of eclipsing binaries in the Magellanic Clouds suitable for high-precision determination of distances (the Araucaria project). The V-band brightnesses of the systems range from 15.4 mag to 17.7 mag and their orbital periods range from 49 days to 773 days. Six systems have favorable geometry showing total eclipses. The absolute dimensions of all eclipsing binary components are calculated with a precision of better than 3% and all systems are suitable for a precise distance determination. The measured stellar masses are in the range 1.4 to 4.6 M_sun and comparison with the MESA isochrones gives ages between 0.1 and 2.1 Gyr. The systems show some weak age-metallicity relation. Two systems have components with very different masses: OGLE LMC-ECL-05430 and OGLE LMC-ECL-18365. Neither system can be fitted by single stellar evolution isochrone, explained by a past mass transfer scenario in the case of ECL-18365 and a gravitational capture or a hierarchical binary merger scenario in the case of ECL-05430. The longest period system OGLE LMC SC9 230659 shows a surprising apsidal motion which shifts the apparent position of the eclipses. In one spectrum of OGLE LMC-ECL-12669 we noted a peculiar dimming of one of the components by 65% well outside of the eclipses. We interpret this observation as arising from an extremely rare occultation event as a foreground Galactic object covers only one component of an extragalactic eclipsing binary., Comment: Accepted for publication in The Astrophysical Journal, 22 figures, 8 tables
Published: 2018
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46. A non-Archimedean approach to K-stability

Author: Boucksom, Sébastien, Jonsson, Mattias, Institut de Mathématiques de Jussieu (IMJ), Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Centre de Mathématiques Laurent Schwartz (CMLS), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X), Department of Ecology [Warsaw], Institute of Zoology [Warsaw], Faculty of Biology [Warsaw], University of Warsaw (UW)-University of Warsaw (UW)-Faculty of Biology [Warsaw], University of Warsaw (UW)-University of Warsaw (UW), Department of Mathematics - University of Michigan, University of Michigan [Ann Arbor], University of Michigan System-University of Michigan System, and Boucksom, Sebastien
Subjects: Mathematics - Algebraic Geometry, 32Q26, 32P05, 32U05, 14J45, 14G22, Mathematics::Algebraic Geometry, Mathematics::Complex Variables, Mathematics - Complex Variables, [MATH.MATH-AG] Mathematics [math]/Algebraic Geometry [math.AG], FOS: Mathematics, [MATH] Mathematics [math], [MATH.MATH-AG]Mathematics [math]/Algebraic Geometry [math.AG], Complex Variables (math.CV), [MATH]Mathematics [math], Algebraic Geometry (math.AG)
Abstract: We study K-stability properties of a smooth Fano variety X using non-Archi-medean geometry, specifically the Berkovich analytification of X with respect to the trivial absolute value on the ground field. More precisely, we view K-semistability and uniform K-stability as conditions on the space of plurisubharmonic (psh) metrics on the anticanonical bundle of X. Using the non-Archimedean Calabi-Yau theorem and the Legendre transform, this allows us to give a new proof that K-stability is equivalent to Ding stability. By choosing suitable psh metrics, we also recover the valuative criterion of K-stability by Fujita and Li. Finally, we study the asymptotic Fubini-Study operator, which associates a psh metric to any graded filtration (or norm) on the anticanonical ring. Our results hold for arbitrary smooth polarized varieties, and suitable adjoint/twisted notions of K-stability and Ding stability. They do not rely on the Minimal Model Program.
Published: 2018

47. Cutwidth: Obstructions and Algorithmic Aspects

Author: Michał Pilipczuk, Marcin Wrochna, Archontia C. Giannopoulou, Jean-Florent Raymond, Dimitrios M. Thilikos, Institut für Softwaretechnik und Theoretische Informatik [EECS-TUB], Fakultät Elektrotechnik und Informatik [TUB], Technische Universität Berlin ( TUB ) -Technische Universität Berlin ( TUB ), Faculty of Mathematics, Informatics, and Mechanics [Warsaw], University of Warsaw ( UW ), Algorithmes, Graphes et Combinatoire ( ALGCO ), Laboratoire d'Informatique de Robotique et de Microélectronique de Montpellier ( LIRMM ), Université de Montpellier ( UM ) -Centre National de la Recherche Scientifique ( CNRS ) -Université de Montpellier ( UM ) -Centre National de la Recherche Scientifique ( CNRS ), National and Kapodistrian University of Athens, Technische Universität Berlin (TU)-Technische Universität Berlin (TU), Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), University of Warsaw (UW), Algorithmes, Graphes et Combinatoire (ALGCO), Laboratoire d'Informatique de Robotique et de Microélectronique de Montpellier (LIRMM), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM), National and Kapodistrian University of Athens (NKUA), Department of Mathematics [Athens], and Herbstritt, Marc
Subjects: FOS: Computer and information sciences, General Computer Science, [INFO.INFO-DS]Computer Science [cs]/Data Structures and Algorithms [cs.DS], 0102 computer and information sciences, 02 engineering and technology, 05C10, 05C85, 68R10, G.2.2, [INFO.INFO-DM]Computer Science [cs]/Discrete Mathematics [cs.DM], 01 natural sciences, Combinatorics, Computer Science::Discrete Mathematics, TheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITY, Computer Science - Data Structures and Algorithms, 0202 electrical engineering, electronic engineering, information engineering, Immersion (mathematics), FOS: Mathematics, Mathematics - Combinatorics, Data Structures and Algorithms (cs.DS), Computer Science::Data Structures and Algorithms, ComputingMilieux_MISCELLANEOUS, [ INFO.INFO-DS ] Computer Science [cs]/Data Structures and Algorithms [cs.DS], Mathematics, 000 Computer science, knowledge, general works, cutwidth, Applied Mathematics, [ INFO.INFO-DM ] Computer Science [cs]/Discrete Mathematics [cs.DM], F.2.2, Graph, Computer Science Applications, Prefix, immersions, 010201 computation theory & mathematics, obstructions, fixed-parameter tractability, Theory of computation, Computer Science, Exponent, 020201 artificial intelligence & image processing, Combinatorics (math.CO), Suffix, MathematicsofComputing_DISCRETEMATHEMATICS
Abstract: Cutwidth is one of the classic layout parameters for graphs. It measures how well one can order the vertices of a graph in a linear manner, so that the maximum number of edges between any prefix and its complement suffix is minimized. As graphs of cutwidth at most k are closed under taking immersions, the results of Robertson and Seymour imply that there is a finite list of minimal immersion obstructions for admitting a cut layout of width at most k. We prove that every minimal immersion obstruction for cutwidth at most k has size at most $$2^{{O}(k^3\log k)}$$ . As an interesting algorithmic byproduct, we design a new fixed-parameter algorithm for computing the cutwidth of a graph that runs in time $$2^{{O}(k^2\log k)}\cdot n$$ , where k is the optimum width and n is the number of vertices. While being slower by a $$\log k$$ -factor in the exponent than the fastest known algorithm, given by Thilikos et al. (J Algorithms 56(1):1–24, 2005; J Algorithms 56(1):25–49, 2005), our algorithm has the advantage of being simpler and self-contained; arguably, it explains better the combinatorics of optimum-width layouts.
Published: 2018
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48. UNIFORM K-STABILITY AND ASYMPTOTICS OF ENERGY FUNCTIONALS IN KÄHLER GEOMETRY

Author: Tomoyuki Hisamoto, Sébastien Boucksom, Mattias Jonsson, Centre de Mathématiques Laurent Schwartz (CMLS), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X), Department of Mathematics, University of Michigan [Ann Arbor], University of Michigan System-University of Michigan System, Institut de Mathématiques de Jussieu (IMJ), Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Graduate School of Mathematics [Nagoya], Nagoya University, Department of Ecology [Warsaw], Institute of Zoology [Warsaw], Faculty of Biology [Warsaw], University of Warsaw (UW)-University of Warsaw (UW)-Faculty of Biology [Warsaw], University of Warsaw (UW)-University of Warsaw (UW), Department of Mathematics - University of Michigan, and Boucksom, Sebastien
Subjects: Applied Mathematics, General Mathematics, 010102 general mathematics, Mathematical analysis, [MATH.MATH-CV]Mathematics [math]/Complex Variables [math.CV], [MATH] Mathematics [math], 01 natural sciences, Stability (probability), 0103 physical sciences, [MATH.MATH-AG]Mathematics [math]/Algebraic Geometry [math.AG], 010307 mathematical physics, 0101 mathematics, [MATH]Mathematics [math], ComputingMilieux_MISCELLANEOUS, Energy (signal processing), Mathematics
Abstract: Consider a polarized complex manifold (X, L) and a ray of positive metrics on L defined by a positive metric on a test configuration for (X, L). For many common functionals in Kähler geometry, we prove that the slope at infinity along the ray is given by evaluating the non-Archimedean version of the functional (as defined in our earlier paper [BHJ15]) at the non-Archimedean metric on L defined by the test configuration. Using this asymptotic result, we show that coercivity of the Mabuchi functional implies uniform K-stability, as defined in [Der15, BHJ15]. As a partial converse, we show that uniform K-stability implies coercivity of the Mabuchi functional when restricted to Bergman metrics.
Published: 2018
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49. Switching of exciton character in double InGaN/GaN quantum wells

Author: Michał Kulczykowski, Czeslaw Skierbiszewski, Katarzyna Pieniak, Krzysztof P. Korona, P. Perlin, Grzegorz Muziol, L. Marona, Pierre Lefebvre, Michał Matuszewski, A. Khachapuridze, Julita Smalc-Koziorowska, Piotr A. Dróżdż, Tadeusz Suski, Eva Monroy, K. Gibasiewicz, G. Staszczak, Szymon Grzanka, Ewa Grzanka, Institute of High Pressure Physics [Warsaw] (IHPP), Polska Akademia Nauk = Polish Academy of Sciences (PAN), Institute of Experimental Physics [Warsaw] (IFD), Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), Laboratoire Charles Coulomb (L2C), Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Nanophysique et Semiconducteurs (NPSC), PHotonique, ELectronique et Ingénierie QuantiqueS (PHELIQS), Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut de Recherche Interdisciplinaire de Grenoble (IRIG), Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut de Recherche Interdisciplinaire de Grenoble (IRIG), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), TopGaN, Institute of Physics, Polish Academy of Sciences, and Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)
Subjects: [PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics], Photoluminescence, Materials science, Condensed matter physics, Exciton, 02 engineering and technology, Electron, 021001 nanoscience & nanotechnology, 01 natural sciences, Blueshift, 0103 physical sciences, [PHYS.COND.CM-MS]Physics [physics]/Condensed Matter [cond-mat]/Materials Science [cond-mat.mtrl-sci], [SPI.OPTI]Engineering Sciences [physics]/Optics / Photonic, Laser power scaling, [SPI.NANO]Engineering Sciences [physics]/Micro and nanotechnologies/Microelectronics, 010306 general physics, 0210 nano-technology, Ground state, Quantum well, Quantum tunnelling
Abstract: International audience; The dependence on exciton density of the interwell coupling scheme in a series of InGaN/GaN symmetrical double quantum wells (DQWs) with varying central barrier width was observed. Continuous-wave photolu-minescence (cw-PL) and time-resolved photoluminescence (TRPL), measured at low temperature (6-13 K), allowed us to examine the competition between three optical recombination channels, namely, the recombination of (i) intrawell excitons (DXs), (ii) interwell indirect excitons (IXs), and (iii) presumably coupled well excitons (CWXs), built of electron and hole wave functions that are widely spread over the entire DQW structure. We demonstrate a rather abrupt switching effect that relies on the actual exciton density in the system. In cw-PL experiments as a function of the pumping laser power, this switching is characterized by a threshold laser power density above which we observe (i) a significant change of slope of both the power-dependent blueshift and intensity of the ground-state exciton and (ii) the appearance of higher-energy optical emissions. In TRPL, as the PL intensity decays with time, both these effects are visible but in opposite direction, including the PL intensity transfer from the higher-energy state to the ground state. The observed switching is assigned to a change of the dominant excitonic recombination regime: at low pumping densities the dominant emission arises from the extremely long-lived IX, whereas above threshold the dominant emission corresponds to DXs or CWXs, depending on the barrier width. The threshold power density (or threshold time for TRPL) presents a clearly exponential dependence upon the width of the central barrier, which demonstrates the role of carrier tunneling in the overall switching process. The comparison of IXs in nitride QWs with bias electric-field induced IXs in GaAs/AlGaAs DQWs shows that the spectral blueshifts are a few times larger in the former structures. This enhancement originates from the built-in electric field in group-III nitrides, which has truly microscopic character. Moreover, it is argued that the presence of the potential fluctuations due to alloy disorder and the fluctuations of the coupling barrier width have only a secondary effect on the observed switching.
Published: 2018
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50. Efficient Computation of Sequence Mappability

Author: Panagiotis Charalampopoulos, Costas S. Iliopoulos, Tomasz Kociumaka, Solon P. Pissis, Jakub Radoszewski, Juliusz Straszyński, Interdisciplinary Center Herzliya (IDC), Department of Informatics [King's College London], King‘s College London, University of California [Berkeley] (UC Berkeley), University of California (UC), Centrum Wiskunde & Informatica (CWI), Vrije Universiteit Amsterdam [Amsterdam] (VU), Equipe de recherche européenne en algorithmique et biologie formelle et expérimentale (ERABLE), Laboratoire de Biométrie et Biologie Evolutive - UMR 5558 (LBBE), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Recherche en Informatique et en Automatique (Inria)-VetAgro Sup - Institut national d'enseignement supérieur et de recherche en alimentation, santé animale, sciences agronomiques et de l'environnement (VAS)-Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Recherche en Informatique et en Automatique (Inria)-VetAgro Sup - Institut national d'enseignement supérieur et de recherche en alimentation, santé animale, sciences agronomiques et de l'environnement (VAS)-Centre National de la Recherche Scientifique (CNRS)-Inria Lyon, Institut National de Recherche en Informatique et en Automatique (Inria), Institute of Informatics [Warsaw], Faculty of Mathematics, Informatics, and Mechanics [Warsaw] (MIMUW), University of Warsaw (UW)-University of Warsaw (UW), Bioinformatics, AIMMS, Bio Informatics (IBIVU), and Centrum Wiskunde & Informatica, Amsterdam (CWI), The Netherlands
Subjects: FOS: Computer and information sciences, k-errata tree, General Computer Science, Hamming distance, Applied Mathematics, Computer Science - Data Structures and Algorithms, [INFO]Computer Science [cs], Data Structures and Algorithms (cs.DS), F.2.2, Sequence mappability, Computer Science Applications
Abstract: In the $(k,m)$-mappability problem, for a given sequence $T$ of length $n$, the goal is to compute a table whose $i$th entry is the number of indices $j \ne i$ such that the length-$m$ substrings of $T$ starting at positions $i$ and $j$ have at most $k$ mismatches. Previous works on this problem focused on heuristics computing a rough approximation of the result or on the case of $k=1$. We present several efficient algorithms for the general case of the problem. Our main result is an algorithm that, for $k=\mathcal{O}(1)$, works in $\mathcal{O}(n)$ space and, with high probability, in $\mathcal{O}(n \cdot \min\{m^k,\log^k n\})$ time. Our algorithm requires a careful adaptation of the $k$-errata trees of Cole et al. [STOC 2004] to avoid multiple counting of pairs of substrings. Our technique can also be applied to solve the all-pairs Hamming distance problem introduced by Crochemore et al. [WABI 2017]. We further develop $\mathcal{O}(n^2)$-time algorithms to compute all $(k,m)$-mappability tables for a fixed $m$ and all $k\in \{0,\ldots,m\}$ or a fixed $k$ and all $m\in\{k,\ldots,n\}$. Finally, we show that, for $k,m = \Theta(\log n)$, the $(k,m)$-mappability problem cannot be solved in strongly subquadratic time unless the Strong Exponential Time Hypothesis fails. This is an improved and extended version of a paper that was presented at SPIRE 2018., Comment: Accepted to SPIRE 2018
Published: 2018
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