19,845 results on '"Evrard, A"'
Search Results
152. Lemierre syndrome: the forgotten disease—a case series
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Salami, Arnaud, Assouan, Camille, Nasser, Dorian, Garba, Idrissa, Mourtada, Wardatou Dine, Yapo, Assi Romaric Evrard, and Konan, Emmanuel
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- 2023
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153. Prevalence and impact of Eustachian valve on the diagnosis of patent foramen ovale in patients ventilated for an acute respiratory distress syndrome
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Sanchez, Florence, Goudelin, Marine, Evrard, Bruno, and Vignon, Philippe
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- 2023
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154. Diagnostic, prognostic and clinical value of left ventricular radial strain to identify paradoxical septal motion in ventilated patients with the acute respiratory distress syndrome: an observational prospective multicenter study
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Evrard, Bruno, Woillard, Jean-Baptiste, Legras, Annick, Bouaoud, Misylias, Gourraud, Maeva, Humeau, Antoine, Goudelin, Marine, and Vignon, Philippe
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- 2023
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155. 4D Optical fibers based on shape-memory polymers
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Strutynski, Clément, Evrard, Marianne, Désévédavy, Frédéric, Gadret, Grégory, Jules, Jean-Charles, Brachais, Claire-Hélène, Kibler, Bertrand, and Smektala, Frédéric
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- 2023
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156. Long-term immunosuppressive treatment is not associated with worse outcome in patients hospitalized in the intensive care unit for septic shock: the PACIFIC study
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Vaidie, Julien, Peju, Edwige, Jandeaux, Louise-Marie, Lesouhaitier, Mathieu, Lacherade, Jean-Claude, Guillon, Antoine, Wittebole, Xavier, Asfar, Pierre, Evrard, Bruno, Daix, Thomas, Vignon, Philippe, and François, Bruno
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- 2023
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157. Expression of the endocannabinoid system and response to cannabinoid components by the human fetal testis
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Dochez-Arnault, J., Desdoits-Lethimonier, C., Matias, I., Evrard, B., Lagarrigue, M., Toupin, M., Lardenois, A., Chalmel, F., Mazaud-Guittot, S., Dejucq-Rainsford, N., and Gely-Pernot, A.
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- 2023
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158. NBEAL2 deficiency in humans leads to low CTLA-4 expression in activated conventional T cells
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Delage, Laure, Carbone, Francesco, Riller, Quentin, Zachayus, Jean-Luc, Kerbellec, Erwan, Buzy, Armelle, Stolzenberg, Marie-Claude, Luka, Marine, de Cevins, Camille, Kalouche, Georges, Favier, Rémi, Michel, Alizée, Meynier, Sonia, Corneau, Aurélien, Evrard, Caroline, Neveux, Nathalie, Roudières, Sébastien, Pérot, Brieuc P., Fusaro, Mathieu, Lenoir, Christelle, Pellé, Olivier, Parisot, Mélanie, Bras, Marc, Héritier, Sébastien, Leverger, Guy, Korganow, Anne-Sophie, Picard, Capucine, Latour, Sylvain, Collet, Bénédicte, Fischer, Alain, Neven, Bénédicte, Magérus, Aude, Ménager, Mickaël, Pasquier, Benoit, and Rieux-Laucat, Frédéric
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- 2023
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159. A natural experiment to assess how urban interventions in lower socioeconomic areas influence health behaviors: the UrbASanté study
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Charreire, Hélène, Conti, Benoit, Bauchard, Lucile, Cissé, Ndèye Aïta, Perignon, Marlène, Rollet, Pascaline, Perrin, Coline, Blanchard, Sophie, Roda, Céline, Feuillet, Thierry, Madelin, Malika, Dupuis, Vincent, Evrard, Anne-Sophie, Hellequin, Anne-Peggy, Coll, Isabelle, Larrue, Corinne, Baudet-Michel, Sophie, Vernouillet, Gabrielle, Ntsame-Abegue, Fernande, Fabre, Isabelle, Méjean, Caroline, and Oppert, Jean-Michel
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- 2023
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160. Co-drawing of technical and high-performance thermoplastics with glasses via the molten core method
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Strutynski, Clément, Voivenel, Raphaël, Evrard, Marianne, Désévédavy, Frédéric, Gadret, Gregory, Jules, Jean-Charles, Brachais, Claire-Hélène, and Smektala, Frédéric
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- 2023
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161. Non-invasive assessment of left ventricular contractility by myocardial work index in veno-arterial membrane oxygenation patients: rationale and design of the MIX-ECMO multicentre observational study
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Bálint Károly Lakatos, Zsuzsanna Ladányi, Alexandra Fábián, Réka Ehrenberger, Tímea Turschl, Zsolt Bagyura, Bruno Evrard, David Vandroux, Marine Goudelin, Simon Lindner, Simone Britsch, Daniel Dürschmied, Endre Zima, Gergely Richárd Csikós, Zsolt Túróczi, Ádám Soltész, Endre Németh, Attila Kovács, Ferenc István Édes, and Béla Merkely
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extracorporeal membrane oxygenation ,echocardiography ,myocardial work index ,speckle-tracking echocardiography ,critical care ,Diseases of the circulatory (Cardiovascular) system ,RC666-701 - Abstract
Introduction and aimsVeno-arterial extracorporeal membrane oxygenation (VA-ECMO) is an increasingly utilized therapeutic choice in patients with cardiogenic shock, however, high complication rate often counteracts with its beneficial cardiopulmonary effects. The assessment of left ventricular (LV) function in key in the management of this population, however, the most commonly used measures of LV performance are substantially load-dependent. Non-invasive myocardial work is a novel LV functional measure which may overcome this limitation and estimate LV function independent of the significantly altered loading conditions of VA-ECMO therapy. The Usefulness of Myocardial Work IndeX in ExtraCorporeal Membrane Oxygenation Patients (MIX-ECMO) study aims to examine the prognostic role of non-invasive myocardial work in VA-ECMO-supported patients.MethodsThe MIX-ECMO is a multicentric, prospective, observational study. We aim to enroll 110 patients 48–72 h after the initiation of VA-ECMO support. The patients will undergo a detailed echocardiographic examination and a central echocardiography core laboratory will quantify conventional LV functional measures and non-invasive myocardial work parameters. The primary endpoint will be failure to wean at 30 days as a composite of cardiovascular mortality, need for long-term mechanical circulatory support or heart transplantation at 30 days, and besides that other secondary objectives will also be investigated. Detailed clinical data will also be collected to compare LV functional measures to parameters with established prognostic role and also to the Survival After Veno-arterial-ECMO (SAVE) score.ConclusionsThe MIX-ECMO study will be the first to determine if non-invasive myocardial work has added prognostic value in patients receiving VA-ECMO support.
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- 2024
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162. Clinical image: Cervicofacial rotation skin flap in PLWD patients
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C. Politis, V. Lenaerts, L. Evrard, F. Shall, and D. Gorlé
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cervicofacial skin flap ,dementia ,facial mass ,skin oncology ,Medicine ,Medicine (General) ,R5-920 - Abstract
Key Clinical Message This article outlines a surgical protocol designed for people living with dementia (PLWD). It proposes that simultaneous resection and reconstruction of skin cancer can minimizes the need for initial care. The method outlined involves primary closure via a cervicofacial rotation flap technique and the use of monofilament resorbable sutures.
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- 2024
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163. Use of risk chart algorithms for the identification of psoriatic arthritis patients at high risk for cardiovascular disease: findings derived from the project CARMA cohort after a 7.5-year follow-up period
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Jesús Tornero, Alba Erra, Santos Castañeda, Carolina Pérez-García, Raimon Sanmartí, Sara Marsal, Ingrid Moller, Esperanza Naredo, Miguel A González-Gay, Celia Erausquin, Ivan Castellví, Javier Llorca, Alejandro Muñoz, María Galindo, Enrique Raya, Lydia Abasolo, Gema Bonilla, Alfonso Corrales, Inmaculada Ureña, Carlos Rodríguez-Lozano, Carlos González-Juanatey, Cristina Fernandez Carballido, Francisco J López-Longo, Miguel Ángel González-Gay, Eduardo Collantes, José A Miranda-Filloy, Sagrario Bustabad, Indalecio Monteagudo, Jose A Piqueras, Tatiana Cobo, Joan Maymó, Carmen Barbadillo, Soledad Ojeda, Jaime Calvo Alen, Antonio Fernandez Nebro, Isabel Rodríguez, Pilar Font, Martina Steiner, Eugenio Chamizo Carmona, Beatriz González Álvarez, Santiago Munoz, Joan M Nolla, Fernando Sánchez-Alonso, Julio Sanchez, Raul Menor Almagro, Ana Pérez Gómez, Monica Ibañez, Elena Heras-Recuero, Trinidad Pérez Sandoval, Miren Uriarte-Ecenarro, Angela Pecondón, Hye Sang Park, Jessica Polo y La Borda, Zulema Plaza, Carmen García Gómez, Ivan Ferraz-Amaro, Jesús Tomás Sanchez-Costa, Olga Carmen Sánchez-González, Ana Isabel Turrión-Nieves, Ana Perez-Alcalá, José L FernándezSueiro, José A Pinto-Tasende, Eugenia Gonzálezde Rábago, María J González-Fernández, Ramón Huguet Codina, Beatriz Yoldi, Mercedes Ramentol, Gabriela Ávila, Cayetano Alegre, Fernando Gamero, José García Torón, María P Moreno-Gil, Antonio Juan-Mas, Pilar Espiño, Inmaculada Ros, Horacio Berman, Oscar Fontseré Patón, Benjamín Fernández Gutiérrez, José M Pina-Salvador, María D Fábregas, Montserrat Romera, Jesús A García-Vadillo, Rosario García de Vicuña, María A Belmonte, María V Irigoyen, Olga Martínez González, Rebeca Belmonte Gómez, Pastora Granados Bautista, Azucena Hernández Sanz, José Santos Rey, Carmen O Sánchez-González, Javier Bachiller, Antonio Zea, Francisco J Manero, Chesús Beltrán Audera, Marta Medrano, Jesús Babío Herráez, Javier del Pino, Ruth López González, María Enriqueta Peiró, José M Senabre, José C Rosas, Isabel Rotés, Estefanía Moreno, Javier Calvo, Amalia Rueda, Pilar Morales, Ana Nieto, Ana Ruibal Escribano, Sergio Ros Expósito, Ginés Sánchez Nievas, Enrique Júdez Navarro, Manuela Sianes Fernández, Silvia Martínez Pardo, Manel Pujol, Alberto Cantabrana, Esmeralda Delgado, Sergio Rodríguez Montero, Javier Rivera Redondo, Teresa González Hernández, Francisco J González-Polo, José M Moreno, Emilio Giner Serret, Laura Cebrián Méndez, María Teresa Navío, Teresa Pedraz Penalva, Encarnación Pagán, Pablo Mesadel Castillo, Ana Cruz, Ana Turrión, Desireé Ruíz, Antonio López Meseguer, Manuel J Moreno, Luis F Linares, Mercedes Morcillo, María L González-Gómez, José M Aramburu, Natalia A Rivera, Olaia Fernández Berrizbeitia, Manel Riera, Yolanda María León, Miriam Amirall, Jordi Fiter, Julia Fernández Melón, Luis Espadaler, Joaquín Belzunegui, Inmaculada Bañegil, César Díaz, Ramón Valls, María Bonet, Eva Revuelta Evrard, Javier R Godo, and José A González-Fernández
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Medicine - Abstract
Objective To assess the predictive value of four cardiovascular (CV) risk algorithms for identifying high-risk psoriatic arthritis (PsA) patients.Methods Evaluation of patients with PsA enrolled in the Spanish prospective project CARdiovascular in RheuMAtology. Baseline data of 669 PsA patients with no history of CV events at the baseline visit, who were followed in rheumatology outpatient clinics at tertiary centres for 7.5 years, were retrospectively analysed to test the performance of the Systematic Coronary Risk Assessment (SCORE), the modified version (mSCORE) European Alliance of Rheumatology Associations (EULAR) 2015/2016, the SCORE2 algorithm (the updated and improved version of SCORE) and the QRESEARCH risk estimator version 3 (QRISK3).Results Over 4790 years of follow-up, there were 34 CV events, resulting in a linearised rate of 7.10 per 1000 person-years (95% CI 4.92 to 9.92). The four CV risk scales showed strong correlations and all showed significant associations with CV events (p
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- 2024
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164. Paranormal Ruptures: Critical Approaches to Exceptional Experiences
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Renaud Evrard
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Speculative philosophy ,BD10-701 - Published
- 2024
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165. Cosmic Dragons: A Two-Component Mixture Model of COSMOS Galaxies
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William K. Black and August E. Evrard
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Astronomy ,QB1-991 ,Astrophysics ,QB460-466 - Abstract
Using the photometric population prediction method {\bf Red Dragon}, we characterize the Red Sequence (RS) and Blue Cloud (BC) of DES galaxies in the COSMOS field. Red Dragon (RD) uses a redshift-evolving, error-corrected Gaussian mixture model to detail the distribution of photometric colors, smoothly parameterizing the two populations with relative weights, mean colors, intrinsic scatters, and inter-color correlations. This resulting fit of RS and BC yields RS membership probabilities $P_{\rm RS}$ for each galaxy. Even when training on only DES main bands $griz$, RD selects the quiescent population (defined here as galaxies with $\lg {\rm sSFR \cdot yr} < -11$) with $\gtrsim 90\%$ balanced accuracy out to $z=2$; augmenting with extended photometry from VIRCAM improves this accuracy to $\sim 95\%$ out to $z=3$. We measure redshift evolution of sSFR and galactic age in several stellar mass bins, finding that the BC is consistently more star-forming (by $\gtrsim 1~{\rm dex}$) and typically younger (by $\gtrsim 1~{\rm Gyr}$) than the RS (up to $z \sim 1.4$). This characterization of both RS and BC as functions of redshift and stellar mass improves our understanding of both populations and opens the door to more precise galaxy population characterization in future deep optical and IR systems.
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- 2024
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166. Collagen molecular organization preservation in human fascia lata and periosteum after tissue engineering
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Julia Vettese, Julie Manon, Antoine Chretien, Robin Evrard, Lies Fievé, Thomas Schubert, Benoît G. Lengelé, Catherine Behets, and Olivier Cornu
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extracellular matrix ,collagen ,crosslinks ,decellularization ,sterilization ,Biotechnology ,TP248.13-248.65 - Abstract
Large bone defect regeneration remains a major challenge for orthopedic surgeons. Tissue engineering approaches are therefore emerging in order to overcome this limitation. However, these processes can alter some of essential native tissue properties such as intermolecular crosslinks of collagen triple helices, which are known for their essential role in tissue structure and function. We assessed the persistence of extracellular matrix (ECM) properties in human fascia lata (HFL) and periosteum (HP) after tissue engineering processes such as decellularization and sterilization. Harvested from cadaveric donors (N = 3), samples from each HFL and HP were decellularized following five different chemical protocols with and without detergents (D1-D4 and D5, respectively). D1 to D4 consisted of different combinations of Triton, Sodium dodecyl sulfate and Deoxyribonuclease, while D5 is routinely used in the institutional tissue bank. Decellularized HFL tissues were further gamma-irradiated (minimum 25 kGy) in order to study the impact of sterilization on the ECM. Polarized light microscopy (PLM) was used to estimate the thickness and density of collagen fibers. Tissue hydration and content of hydroxyproline, enzymatic crosslinks, and non-enzymatic crosslinks (pentosidine) were semi-quantified with Raman spectroscopy. ELISA was also used to analyze the maintenance of the decorin (DCN), an important small leucine rich proteoglycan for fibrillogenesis. Among the decellularization protocols, detergent-free treatments tended to further disorganize HFL samples, as more thin fibers (+53.7%) and less thick ones (−32.6%) were recorded, as well as less collagen enzymatic crosslinks (−25.2%, p = 0.19) and a significant decrease of DCN (p = 0.036). GAG content was significantly reduced in both tissue types after all decellularization protocols. On the other hand, HP samples were more sensitive to the D1 detergent-based treatments, with more disrupted collagen organization and greater, though not significant loss of enzymatic crosslinks (−37.4%, p = 0.137). Irradiation of D5 HFL samples, led to a further and significant loss in the content of enzymatic crosslinks (−29.4%, p = 0.037) than what was observed with the decellularization process. Overall, the results suggest that the decellularization processes did not significantly alter the matrix. However, the addition of a gamma-irradiation is deleterious to the collagen structural integrity of the tissue.
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- 2024
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167. Dark Energy Survey Year 3 results: Exploiting small-scale information with lensing shear ratios
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Sánchez, C, Prat, J, Zacharegkas, G, Pandey, S, Baxter, E, Bernstein, GM, Blazek, J, Cawthon, R, Chang, C, Krause, E, Lemos, P, Park, Y, Raveri, M, Sanchez, J, Troxel, MA, Amon, A, Fang, X, Friedrich, O, Gruen, D, Porredon, A, Secco, LF, Samuroff, S, Alarcon, A, Alves, O, Andrade-Oliveira, F, Bechtol, K, Becker, MR, Camacho, H, Campos, A, Rosell, A Carnero, Kind, M Carrasco, Chen, R, Choi, A, Crocce, M, Davis, C, De Vicente, J, DeRose, J, Di Valentino, E, Diehl, HT, Dodelson, S, Doux, C, Drlica-Wagner, A, Eckert, K, Eifler, TF, Elsner, F, Elvin-Poole, J, Everett, S, Ferté, A, Fosalba, P, Gatti, M, Giannini, G, Gruendl, RA, Harrison, I, Hartley, WG, Herner, K, Huff, EM, Huterer, D, Jarvis, M, Jain, B, Kuropatkin, N, Leget, P-F, MacCrann, N, McCullough, J, Muir, J, Myles, J, Navarro-Alsina, A, Rollins, RP, Roodman, A, Rosenfeld, R, Rykoff, ES, Sevilla-Noarbe, I, Sheldon, E, Shin, T, Troja, A, Tutusaus, I, Varga, TN, Wechsler, RH, Yanny, B, Yin, B, Zhang, Y, Zuntz, J, Abbott, TMC, Aguena, M, Allam, S, Bacon, D, Bertin, E, Bhargava, S, Brooks, D, Buckley-Geer, E, Burke, DL, Carretero, J, Costanzi, M, da Costa, LN, Pereira, MES, Desai, S, Dietrich, JP, Doel, P, Evrard, AE, Ferrero, I, and Flaugher, B
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Particle and High Energy Physics ,Astronomical Sciences ,Physical Sciences - Abstract
Using the first three years of data from the Dark Energy Survey (DES), we use ratios of small-scale galaxy-galaxy lensing measurements around the same lens sample to constrain source redshift uncertainties, intrinsic alignments and other systematics or nuisance parameters of our model. Instead of using a simple geometric approach for the ratios as has been done in the past, we use the full modeling of the galaxy-galaxy lensing measurements, including the corresponding integration over the power spectrum and the contributions from intrinsic alignments and lens magnification. We perform extensive testing of the small-scale shear-ratio (SR) modeling by studying the impact of different effects such as the inclusion of baryonic physics, nonlinear biasing, halo occupation distribution descriptions and lens magnification, among others, and using realistic N-body simulations of the DES data. We validate the robustness of our constraints in the data by using two independent lens samples with different galaxy properties, and by deriving constraints using the corresponding large-scale ratios for which the modeling is simpler. The results applied to the DES Y3 data demonstrate how the ratios provide significant improvements in constraining power for several nuisance parameters in our model, especially on source redshift calibration and intrinsic alignments. For source redshifts, SR improves the constraints from the prior by up to 38% in some redshift bins. Such improvements, and especially the constraints it provides on intrinsic alignments, translate to tighter cosmological constraints when shear ratios are combined with cosmic shear and other 2pt functions. In particular, for the DES Y3 data, SR improves S8 constraints from cosmic shear by up to 31%, and for the full combination of probes (3×2pt) by up to 10%. The shear ratios presented in this work are used as an additional likelihood for cosmic shear, 2×2pt and the full 3×2pt in the fiducial DES Y3 cosmological analysis.
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- 2022
168. The Observed Evolution of the Stellar Mass–Halo Mass Relation for Brightest Central Galaxies
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Golden-Marx, Jesse B, Miller, CJ, Zhang, Y, Ogando, RLC, Palmese, A, Abbott, TMC, Aguena, M, Allam, S, Andrade-Oliveira, F, Annis, J, Bacon, D, Bertin, E, Brooks, D, Buckley-Geer, E, Rosell, A Carnero, Kind, M Carrasco, Castander, FJ, Costanzi, M, Crocce, M, da Costa, LN, Pereira, MES, De Vicente, J, Desai, S, Diehl, HT, Doel, P, Drlica-Wagner, A, Everett, S, Evrard, AE, Ferrero, I, Flaugher, B, Fosalba, P, Frieman, J, García-Bellido, J, Gaztanaga, E, Gerdes, DW, Gruen, D, Gruendl, RA, Gschwend, J, Gutierrez, G, Hartley, WG, Hinton, SR, Hollowood, DL, Honscheid, K, Hoyle, B, James, DJ, Jeltema, T, Kim, AG, Krause, E, Kuehn, K, Kuropatkin, N, Lahav, O, Lima, M, Maia, MAG, Marshall, JL, Melchior, P, Menanteau, F, Miquel, R, Mohr, JJ, Morgan, R, Paz-Chinchón, F, Petravick, D, Pieres, A, Malagón, AA Plazas, Prat, J, Romer, AK, Sanchez, E, Santiago, B, Scarpine, V, Schubnell, M, Serrano, S, Sevilla-Noarbe, I, Smith, M, Soares-Santos, M, Suchyta, E, Tarle, G, and Varga, TN
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Astronomical Sciences ,Physical Sciences ,Astronomical and Space Sciences ,Atomic ,Molecular ,Nuclear ,Particle and Plasma Physics ,Physical Chemistry (incl. Structural) ,Astronomy & Astrophysics ,Astronomical sciences ,Particle and high energy physics ,Space sciences - Abstract
We quantify evolution in the cluster-scale stellar mass-halo mass (SMHM) relation's parameters using 2323 clusters and brightest central galaxies (BCGs) over the redshift range 0.03 ≤ z ≤ 0.60. The precision on the inferred SMHM parameters is improved by including the magnitude gap (m gap) between the BCG and fourth-brightest cluster member (M14) as a third parameter in the SMHM relation. At fixed halo mass, accounting for m gap, through a stretch parameter, reduces the SMHM relation's intrinsic scatter. To explore this redshift range, we use clusters, BCGs, and cluster members identified using the Sloan Digital Sky Survey C4 and redMaPPer cluster catalogs and the Dark Energy Survey redMaPPer catalog. Through this joint analysis, we detect no systematic differences in BCG stellar mass, m gap, and cluster mass (inferred from richness) between the data sets. We utilize the Pareto function to quantify each parameter's evolution. We confirm prior findings of negative evolution in the SMHM relation's slope (3.5σ), and detect negative evolution in the stretch parameter (4.0σ) and positive evolution in the offset parameter (5.8σ). This observed evolution, combined with the absence of BCG growth, when stellar mass is measured within 50 kpc, suggests that this evolution results from changes in the cluster's m gap. For this to occur, late-term growth must be in the intracluster light surrounding the BCG. We also compare the observed results to IllustrisTNG 300-1 cosmological hydrodynamic simulations and find modest qualitative agreement. However, the simulations lack the evolutionary features detected in the real data.
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- 2022
169. Cross-correlation of DES Y3 lensing and ACT/${\it Planck}$ thermal Sunyaev Zel'dovich Effect I: Measurements, systematics tests, and feedback model constraints
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Gatti, M., Pandey, S., Baxter, E., Hill, J. C., Moser, E., Raveri, M., Fang, X., DeRose, J., Giannini, G., Doux, C., Huang, H., Battaglia, N., Alarcon, A., Amon, A., Becker, M., Campos, A., Chang, C., Chen, R., Choi, A., Eckert, K., Elvin-Poole, J., Everett, S., Ferte, A., Harrison, I., Maccrann, N., Mccullough, J., Myles, J., Alsina, A. Navarro, Prat, J., Rollins, R. P., Sanchez, C., Shin, T., Troxel, M., Tutusaus, I., Yin, B., Abbott, T., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Bernstein, G., Bertin, E., Bolliet, B., Bond, J. R., Brooks, D., Burke, D. L., Calabrese, E., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Cawthon, R., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. da Silva, DeVicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Dunkley, J., Evrard, A. E., Ferraro, S., Ferrero, I., Flaugher, B., Fosalba, P., Frieman, J., Garcıa-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Herner, K., Hincks, A. D., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hughes, J. P., Huterer, D., Jain, B., James, D. J., Krause, E., Kuehn, K., Kuropatkin, N., Lahav, O., Lidman, C., Lima, M., Lokken, M., Madhavacheril, M. S., Maia, M. A. G., Marshall, J. L., Mcmahon, J. J., Melchior, P., Moodley, K., Mohr, J. J., Morgan, R., Nati, F., Niemack, M. D., Page, L., Palmese, A., Paz-Chinchon, F., Pieres, A., Malagon, A. A. Plazas, Rodriguez-Monroy, M., Romer, A. K., Sanchez, E., Scarpine, V., Schaan, E., Secco, L. F., Serrano, S., Sheldon, E., Sherwin, B. D., Sifon, C., Smith, M., Soares-Santos, M., Spergel, D., Suchyta, E., Tarle, G., Thomas, D., To, C., Tucker, D. L., Varga, T. N., Weller, J., Wilkinson, R. D., Wollack, E. J., and Xu, Z.
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Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We present a tomographic measurement of the cross-correlation between thermal Sunyaev-Zeldovich (tSZ) maps from ${\it Planck}$ and the Atacama Cosmology Telescope (ACT) and weak galaxy lensing shears measured during the first three years of observations of the Dark Energy Survey (DES Y3). This correlation is sensitive to the thermal energy in baryons over a wide redshift range, and is therefore a powerful probe of astrophysical feedback. We detect the correlation at a statistical significance of $21\sigma$, the highest significance to date. We examine the tSZ maps for potential contaminants, including cosmic infrared background (CIB) and radio sources, finding that CIB has a substantial impact on our measurements and must be taken into account in our analysis. We use the cross-correlation measurements to test different feedback models. In particular, we model the tSZ using several different pressure profile models calibrated against hydrodynamical simulations. Our analysis marginalises over redshift uncertainties, shear calibration biases, and intrinsic alignment effects. We also marginalise over $\Omega_{\rm m}$ and $\sigma_8$ using ${\it Planck}$ or DES priors. We find that the data prefers the model with a low amplitude of the pressure profile at small scales, compatible with a scenario with strong AGN feedback and ejection of gas from the inner part of the halos. When using a more flexible model for the shear profile, constraints are weaker, and the data cannot discriminate between different baryonic prescriptions., Comment: submitted to PRD
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- 2021
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170. Cross-correlation of DES Y3 lensing and ACT/${\it Planck}$ thermal Sunyaev Zel'dovich Effect II: Modeling and constraints on halo pressure profiles
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Pandey, S., Gatti, M., Baxter, E., Hill, J. C., Fang, X., Doux, C., Giannini, G., Raveri, M., DeRose, J., Huang, H., Moser, E., Battaglia, N., Alarcon, A., Amon, A., Becker, M., Campos, A., Chang, C., Chen, R., Choi, A., Eckert, K., Elvin-Poole, J., Everett, S., Ferte, A., Harrison, I., Maccrann, N., Mccullough, J., Myles, J., Alsina, A. Navarro, Prat, J., Rollins, R. P., Sanchez, C., Shin, T., Troxel, M., Tutusaus, I., Yin, B., Aguena, M., Allam, S., Andrade-Oliveira, F., Bernstein, G. M., Bertin, E., Bolliet, B., Bond, J. R., Brooks, D., Calabrese, E., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Cawthon, R., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Dunkley, J., Evrard, A. E., Ferraro, S., Ferrero, I., Flaugher, B., Fosalba, P., Garcia-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Herner, K., Hincks, A. D., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hughes, J. P., Huterer, D., Jain, B., James, D. J., Jeltema, T., Krause, E., Kuehn, K., Lahav, O., Lima, M., Lokken, M., Madhavacheril, M. S., Maia, M. A. G., Mcmahon, J. J., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Moodley, K., Morgan, R., Nati, F., Niemack, M. D., Page, L., Palmese, A., Paz-Chinchon, F., Pieres, A., Malagon, A. A. Plazas, Rodriguez-Monroy, M., Romer, A. K., Sanchez, E., Scarpine, V., Schaan, E., Serrano, S., Sevilla-Noarbe, I., Sheldon, E., Sherwin, B. D., Sifon, C., Smith, M., Soares-Santos, M., Spergel, D., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Varga, T. N., Weller, J., Wollack, E. J., and Xu, Z.
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Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
Hot, ionized gas leaves an imprint on the cosmic microwave background via the thermal Sunyaev Zel'dovich (tSZ) effect. The cross-correlation of gravitational lensing (which traces the projected mass) with the tSZ effect (which traces the projected gas pressure) is a powerful probe of the thermal state of ionized baryons throughout the Universe, and is sensitive to effects such as baryonic feedback. In a companion paper (Gatti et al. 2021), we present tomographic measurements and validation tests of the cross-correlation between galaxy shear measurements from the first three years of observations of the Dark Energy Survey, and tSZ measurements from a combination of Atacama Cosmology Telescope and ${\it Planck}$ observations. In this work, we use the same measurements to constrain models for the pressure profiles of halos across a wide range of halo mass and redshift. We find evidence for reduced pressure in low mass halos, consistent with predictions for the effects of feedback from active galactic nuclei. We infer the hydrostatic mass bias ($B \equiv M_{500c}/M_{\rm SZ}$) from our measurements, finding $B = 1.8\pm0.1$ when adopting the ${\it Planck}$-preferred cosmological parameters. We additionally find that our measurements are consistent with a non-zero redshift evolution of $B$, with the correct sign and sufficient magnitude to explain the mass bias necessary to reconcile cluster count measurements with the ${\it Planck}$-preferred cosmology. Our analysis introduces a model for the impact of intrinsic alignments (IA) of galaxy shapes on the shear-tSZ correlation. We show that IA can have a significant impact on these correlations at current noise levels., Comment: 22 pages, 13 figures. Comments welcome
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- 2021
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171. Characterization and performance of the Apollon Short-Focal-Area facility following its commissioning at 1 PW level
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Burdonov, K., Fazzini, A., Lelasseux, V., Albrecht, J., Antici, P., Ayoul, Y., Beluze, A., Cavanna, D., Ceccotti, T., Chabanis, M., Chaleil, A., Chen, S. N., Chen, Z., Consoli, F., Cuciuc, M., Davoine, X., Delaneau, J. P., d'Humières, E., Dubois, J-L., Evrard, C., Filippov, E., Freneaux, A., Forestier-Colleoni, P., Gremillet, L., Horny, V., Lancia, L., Lecherbourg, L., Lebas, N., Leblanc, A., Ma, W., Martin, L., Negoita, F., Paillard, J-L., Papadopoulos, D., Perez, F., Pikuz, S., Qi, G., Quéré, F., Ranc, L., Söderstrom, P. -A., Scisciò, M., Sun, S., Vallières, S., Wang, P., Yao, W., Mathieu, F., Audebert, P., and Fuchs, J.
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Physics - Plasma Physics - Abstract
We present the results of the first commissioning phase of the ``short focal length'' area (SFA) of the Apollon laser facility (located in Saclay, France), which was performed with the first available laser beam (F2), scaled to a nominal power of one petawatt. Under the conditions that were tested, this beam delivered on target pulses of 10 J average energy and 24 fs duration. Several diagnostics were fielded to assess the performance of the facility. The on-target focal spot, its spatial stability, the temporal intensity profile prior to the main pulse, as well as the resulting density gradient formed at the irradiated side of solid targets, have been thoroughly characterized, with the goal of helping users design future experiments. Emissions of energetic electrons, ions, and electromagnetic radiation were recorded, showing good laser-to-target coupling efficiency and an overall performance comparable with that of similar international facilities. This will be followed in 2022 by a further commissioning stage at the multi-petawatt level.
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- 2021
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172. Galaxy Morphological Classification Catalogue of the Dark Energy Survey Year 3 data with Convolutional Neural Networks
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Cheng, Ting-Yun, Conselice, Christopher J., Aragón-Salamanca, Alfonso, Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Bluck, A. F. L., Brooks, D., Burke, D. L., Kind, M. Carrasco, Carretero, J., Choi, A., Costanzi, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Diehl, H. T., Drlica-Wagner, A., Eckert, K., Everett, S., Evrard, A. E., Ferrero, I., Fosalba, P., Frieman, J., García-Bellido, J., Gerdes, D. W., Giannantonio, T., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Krause, E., Kuehn, K., Kuropatkin, N., Lahav, O., Maia, M. A. G., March, M., Menanteau, F., Miquel, R., Morgan, R., Paz-Chinchón, F., Pieres, A., Malagón, A. A. Plazas, Roodman, A., Sanchez, E., Scarpine, V., Serrano, S., Sevilla-Noarbe, I., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., and To, C.
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Astrophysics - Astrophysics of Galaxies - Abstract
We present in this paper one of the largest galaxy morphological classification catalogues to date, including over 20 million of galaxies, using the Dark Energy Survey (DES) Year 3 data based on Convolutional Neural Networks (CNN). Monochromatic $i$-band DES images with linear, logarithmic, and gradient scales, matched with debiased visual classifications from the Galaxy Zoo 1 (GZ1) catalogue, are used to train our CNN models. With a training set including bright galaxies ($16\le{i}<18$) at low redshift ($z<0.25$), we furthermore investigate the limit of the accuracy of our predictions applied to galaxies at fainter magnitude and at higher redshifts. Our final catalogue covers magnitudes $16\le{i}<21$, and redshifts $z<1.0$, and provides predicted probabilities to two galaxy types -- Ellipticals and Spirals (disk galaxies). Our CNN classifications reveal an accuracy of over 99\% for bright galaxies when comparing with the GZ1 classifications ($i<18$). For fainter galaxies, the visual classification carried out by three of the co-authors shows that the CNN classifier correctly categorises disky galaxies with rounder and blurred features, which humans often incorrectly visually classify as Ellipticals. As a part of the validation, we carry out one of the largest examination of non-parametric methods, including $\sim$100,000 galaxies with the same coverage of magnitude and redshift as the training set from our catalogue. We find that the Gini coefficient is the best single parameter discriminator between Ellipticals and Spirals for this data set., Comment: 23 pages, 15 figures. Accepted by MNRAS
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- 2021
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173. Velocity Dispersions of Clusters in the Dark Energy Survey Y3 redMaPPer Catalog
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Wetzell, V., Jeltema, T. E., Hegland, B., Everett, S., Giles, P. A., Wilkinson, R., Farahi, A., Costanzi, M., Hollowood, D. L., Upsdell, E., Saro, A., Myles, J., Bermeo, A., Bhargava, S., Collins, C. A., Cross, D., Eiger, O., Gardner, G., Hilton, M., Jobel, J., Kelly, P., Laubner, D., Liddle, A. R., Mann, R. G., Martinez, V., Mayers, J., McDaniel, A., Romer, A. K., Rooney, P., Sahlen, M., Stott, J., Swart, A., Turner, D. J., Viana, P. T. P., Abbott, T. M. C., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Asorey, J., Bertin, E., Burke, D. L., Calcino, J., Rosell, A. Carnero, Carollo, D., Kind, M. Carrasco, Carretero, J., Choi, A., Crocce, M., da Costa, L. N., Pereira, M. E. S., Davis, T. M., De Vicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Evrard, A. E., Ferrero, I., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Glazebrook, K., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Honscheid, K., James, D. J., Kuehn, K., Kuropatkin, N., Lahav, O., Lewis, G. F., Lidman, C., Lima, M., Maia, M. A. G., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Morgan, R., Palmese, A., Paz-Chinchón, F., Malagón, A. A. Plazas, Sanchez, E., Scarpine, V., Serrano, S., Sevilla-Noarbe, I., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Thomas, D., Tucker, B. E., Tucker, D. L., Varga, T. N., and Weller, J.
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Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We measure the velocity dispersions of clusters of galaxies selected by the redMaPPer algorithm in the first three years of data from the Dark Energy Survey (DES), allowing us to probe cluster selection and richness estimation, $\lambda$, in light of cluster dynamics. Our sample consists of 126 clusters with sufficient spectroscopy for individual velocity dispersion estimates. We examine the correlations between cluster velocity dispersion, richness, X-ray temperature and luminosity as well as central galaxy velocity offsets. The velocity dispersion-richness relation exhibits a bimodal distribution. The majority of clusters follow scaling relations between velocity dispersion, richness, and X-ray properties similar to those found for previous samples; however, there is a significant population of clusters with velocity dispersions which are high for their richness. These clusters account for roughly 22\% of the $\lambda < 70$ systems in our sample, but more than half (55\%) of $\lambda < 70$ clusters at $z>0.5$. A couple of these systems are hot and X-ray bright as expected for massive clusters with richnesses that appear to have been underestimated, but most appear to have high velocity dispersions for their X-ray properties likely due to line-of-sight structure. These results suggest that projection effects contribute significantly to redMaPPer selection, particularly at higher redshifts and lower richnesses. The redMaPPer determined richnesses for the velocity dispersion outliers are consistent with their X-ray properties, but several are X-ray undetected and deeper data is needed to understand their nature., Comment: 22 pages, accepted to MNRAS
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- 2021
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174. Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey: I. Evidence for thermal energy anisotropy using oriented stacking
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Lokken, M., Hložek, R., van Engelen, A., Madhavacheril, M., Baxter, E., DeRose, J., Doux, C., Pandey, S., Rykoff, E. S., Stein, G., To, C., Abbott, T. M. C., Adhikari, S., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Battaglia, N., Bernstein, G. M., Bertin, E., Bond, J. R., Brooks, D., Calabrese, E., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Cawthon, R., Choi, A., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. da Silva, De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Dunkley, J., Everett, S., Evrard, A. E., Ferraro, S., Flaugher, B., Fosalba, P., Frieman, J., Gallardo, P. A., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hill, J. C., Hilton, M., Hincks, A. D., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., Huang, Z., Hughes, J. P., Huterer, D., Jain, B., James, D. J., Jeltema, T., Kuehn, K., Lima, M., Maia, M. A. G., Marshall, J. L., McMahon, J., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Moodley, K., Morgan, R., Nati, F., Page, L., Ogando, R. L. C., Palmese, A., Chinchón, F. Paz, Malagón, A. A. Plazas, Pieres, A., Romer, A. K., Rozo, E., Sanchez, E., Scarpine, V., Schillaci, A., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Sifón, C., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., Tucker, D. L., Varga, T. N., Weller, J., Wechsler, R. H., Wilkinson, R. D., Wollack, E. J., and Xu, Z.
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Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
The cosmic web contains filamentary structure on a wide range of scales. On the largest scales, superclustering aligns multiple galaxy clusters along inter-cluster bridges, visible through their thermal Sunyaev-Zel'dovich signal in the Cosmic Microwave Background. We demonstrate a new, flexible method to analyze the hot gas signal from multi-scale extended structures. We use a Compton-$y$ map from the Atacama Cosmology Telescope (ACT) stacked on redMaPPer cluster positions from the optical Dark Energy Survey (DES). Cutout images from the $y$ map are oriented with large-scale structure information from DES galaxy data such that the superclustering signal is aligned before being overlaid. We find evidence for an extended quadrupole moment of the stacked $y$ signal at the 3.5$\sigma$ level, demonstrating that the large-scale thermal energy surrounding galaxy clusters is anisotropically distributed. We compare our ACT$\times$DES results with the Buzzard simulations, finding broad agreement. Using simulations, we highlight the promise of this novel technique for constraining the evolution of anisotropic, non-Gaussian structure using future combinations of microwave and optical surveys., Comment: 37 pages, 23 figures, 4 tables. Added explanatory figure, table, covariance matrix equations, discussion of CIB impact. Matches the version published in ApJ
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- 2021
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175. Dark Energy Survey Year 3 Results: Galaxy Sample for BAO Measurement
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Rosell, A. Carnero, Rodriguez-Monroy, M., Crocce, M., Elvin-Poole, J., Porredon, A., Ferrero, I., Mena-Fernandez, J., Cawthon, R., De Vicente, J., Gaztanaga, E., Ross, A. J., Sanchez, E., Sevilla-Noarbe, I., Alves, O., Andrade-Oliveira, F., Asorey, J., Avila, S., Brandao-Souza, A., Camacho, H., Chan, K. C., Ferte, A., Muir, J., Riquelme, W., Rosenfeld, R., Cid, D. Sanchez, Hartley, W. G., Weaverdyck, N., Abbott, T., Aguena, M., Sahar, A., Annis, J., Bertin, E., Brooks, D., Buckley-Geer, E., Burke, D., Calcino, J., Carollo, D., Kind, M. Carrasco, Carretero, J., Castander, F., Choi, A., Conselice, C., Costanzi, M., da Costa, L., Pereira, M. E. da Silva, Davis, T., Desai, S., Diehl, H. T., Doel, P., Drlica-Wagner, A., Eckert, K., Everett, S., Evrard, A., Flaugher, B., Fosalba, P., Frieman, J., Garcia-Bellido, J., Gerdes, D., Giannantonio, T., Glazebrook, K., Gruen, D., Gruendl, R., Gschwend, J., Gutierrez, G., Hinton, S., Hollowood, D., Honscheid, K., Hoyle, B., Huterer, D., James, D., Kim, A., Krause, E., Kuehn, K., Lahav, O., Lewis, G., Lidman, C., Lima, M., Maia, M., Malik, U., Marshall, J., Menanteau, F., Miquel, R., Mohr, J., Moller, A., Morgan, R., Ogando, R., Palmese, A., Paz-Chinchon, F., Percival, W., Pieres, A., Malagon, A. Plazas, Roodman, A., Scarpine, V., Schubnell, M., Serrano, S., Sharp, R., Sheldon, E., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M., Tarle, G., Thomas, D., To, C., Tucker, B., Tucker, D., Uddin, S., Varga, T. N., and Collaboration, DES
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Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
In this paper we present and validate the galaxy sample used for the analysis of the Baryon Acoustic Oscillation signal (BAO) in the Dark Energy Survey (DES) Y3 data. The definition is based on a colour and redshift-dependent magnitude cut optimized to select galaxies at redshifts higher than 0.5, while ensuring a high quality photometric redshift determination. The sample covers $\approx 4100$ square degrees to a depth of $i = 22.3 \ (AB)$ at $10\sigma$. It contains 7,031,993 galaxies in the redshift range from $z$= 0.6 to 1.1, with a mean effective redshift of 0.835. Photometric redshifts are estimated with the machine learning algorithm DNF, and are validated using the VIPERS PDR2 sample. We find a mean redshift bias of $z_{\mathrm{bias}} \approx 0.01$ and a mean uncertainty, in units of $1+z$, of $\sigma_{68} \approx 0.03$. We evaluate the galaxy population of the sample, showing it is mostly built upon Elliptical to Sbc types. Furthermore, we find a low level of stellar contamination of $\lesssim 4\%$. We present the method used to mitigate the effect of spurious clustering coming from observing conditions and other large-scale systematics. We apply it to the DES Y3 BAO sample and calculate sample weights that are used to get a robust estimate of the galaxy clustering signal. This paper is one of a series dedicated to the analysis of the BAO signal in the DES Y3 data. In the companion papers, Ferrero et al. (2021) and DES Collaboration (2021), we present the galaxy mock catalogues used to calibrate the analysis and the angular diameter distance constraints obtained through the fitting to the BAO scale, respectively. The galaxy sample, masks and additional material will be released in the public DES data repository upon acceptance., Comment: Accepted for publication in MNRAS. 24 pages, 24 figures
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- 2021
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176. Dark Energy Survey Year 3 Results: A 2.7% measurement of Baryon Acoustic Oscillation distance scale at redshift 0.835
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DES Collaboration, Abbott, T. M. C., Aguena, M., Allam, S., Andrade-Oliveira, F., Asorey, J., Avila, S., Bernstein, G. M., Bertin, E., Brandao-Souza, A., Brooks, D., Burke, D. L., Calcino, J., Camacho, H., Rosell, A. Carnero, Carollo, D., Kind, M. Carrasco, Carretero, J., Castander, F. J., Cawthon, R., Chan, K. C., Choi, A., Conselice, C., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. S., Davis, T. M., De Vicente, J., Desai, S., Diehl, H. T., Doel, P., Eckert, K., Elvin-Poole, J., Everett, S., Evrard, A. E., Fang, X., Ferrero, I., Ferté, A., Flaugher, B., Fosalba, P., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Glazebrook, K., Gomes, D., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Huterer, D., Jain, B., James, D. J., Jeltema, T., Kokron, N., Krause, E., Kuehn, K., Lahav, O., Lewis, G. F., Lidman, C., Lima, M., Lin, H., Maia, M. A. G., Malik, U., Martini, P., Melchior, P., Mena-Fernández, J., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Muir, J., Myles, J., Möller, A., Palmese, A., Paz-Chinchón, F., Percival, W. J., Pieres, A., Malagón, A. A. Plazas, Porredon, A., Prat, J., Rodriguez-Monroy, M., Romer, A. K., Roodman, A., Rosenfeld, R., Ross, A. J., Sanchez, E., Cid, D. Sanchez, Scarpine, V., Serrano, S., Sevilla-Noarbe, I., Sheldon, E., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Troxel, M. A., Tucker, B. E., Tucker, D. L., Tutusaus, I., Uddin, S. A., Varga, T. N., Weller, J., and Wilkinson, R. D.
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Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We present angular diameter measurements obtained by measuring the position of Baryon Acoustic Oscillations (BAO) in an optimised sample of galaxies from the first three years of Dark Energy Survey data (DES Y3). The sample consists of 7 million galaxies distributed over a footprint of 4100 deg$^2$ with $0.6 < z_{\rm photo} < 1.1$ and a typical redshift uncertainty of $0.03(1+z)$. The sample selection is the same as in the BAO measurement with the first year of DES data, but the analysis presented here uses three times the area, extends to higher redshift and makes a number of improvements, including a fully analytical BAO template, the use of covariances from both theory and simulations, and an extensive pre-unblinding protocol. We used two different statistics: angular correlation function and power spectrum, and validate our pipeline with an ensemble of over 1500 realistic simulations. Both statistics yield compatible results. We combine the likelihoods derived from angular correlations and spherical harmonics to constrain the ratio of comoving angular diameter distance $D_M$ at the effective redshift of our sample to the sound horizon scale at the drag epoch. We obtain $D_M(z_{\rm eff}=0.835)/r_{\rm d} = 18.92 \pm 0.51$, which is consistent with, but smaller than, the Planck prediction assuming flat \lcdm, at the level of $2.3 \sigma$. The analysis was performed blind and is robust to changes in a number of analysis choices. It represents the most precise BAO distance measurement from imaging data to date, and is competitive with the latest transverse ones from spectroscopic samples at $z>0.75$. When combined with DES 3x2pt + SNIa, they lead to improvements in $H_0$ and $\Omega_m$ constraints by $\sim 20\%$, Comment: 24 pages, 10 figures, matches version accepted by PRD
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- 2021
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177. Dark Energy Survey Year 3 Results: Galaxy mock catalogs for BAO analysis
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Ferrero, I., Crocce, M., Tutusaus, I., Porredon, A., Blot, L., Fosalba, P., Rosell, A. Carnero, Avila, S., Izard, A., Elvin-Poole, J., Chan, K. C., Camacho, H., Rosenfeld, R., Sanchez, E., Tallada-Crespí, P., Carretero, J., Sevilla-Noarbe, I., Gaztanaga, E., Andrade-Oliveira, F., De Vicente, J., Mena-Fernández, J., Ross, A. J., Cid, D. Sanchez, Ferté, A., Brandao-Souza, A., Fang, X., Krause, E., Gomes, D., Aguena, M., Allam, S., Annis, J., Bertin, E., Brooks, D., Kind, M. Carrasco, Castander, F. J., Cawthon, R., Choi, A., Conselice, C., Costanzi, M., da Costa, L. N., Pereira, M. E. S., Diehl, H. T., Doel, P., Drlica-Wagner, A., Everett, S., Evrard, A. E., Flaugher, B., Frieman, J., García-Bellido, J., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., Huterer, D., James, D. J., Kuehn, K., Lima, M., Maia, M. A. G., Marshall, J. L., Menanteau, F., Miquel, R., Morgan, R., Muir, J., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Percival, W. J., Malagón, A. A. Plazas, Rodriguez-Monroy, M., Scarpine, V., Schubnell, M., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Tucker, D. L., and Varga, T. N.
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Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
The calibration and validation of scientific analysis in simulations is a fundamental tool to ensure unbiased and robust results in observational cosmology. In particular, mock galaxy catalogs are a crucial resource to achieve these goals in the measurement of baryon acoustic oscillation (BAO) in the clustering of galaxies. Here we present a set of 1952 galaxy mock catalogs designed to mimic the Dark Energy Survey (DES) Year 3 BAO sample over its full photometric redshift range $0.6
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- 2021
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178. The Observed Evolution of the Stellar Mass - Halo Mass Relation for Brightest Central Galaxies
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Golden-Marx, Jesse B., Miller, C. J., Zhang, Y., Ogando, R. L. C., Palmese, A., Abbott, T. M. C., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Bacon, D., Bertin, E., Brooks, D., Buckley-Geer, E., Rosell, A. Carnero, Kind, M. Carrasco, Castander, F. J., Constanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. S., de Vicente, J., Desai, S., Diehl, H. T., Doel, P., Drlica-Wagner, A., Everett, S., Evrard, A. E., Ferrero, I., Flaugher, B., Fosalba, P., Frieman, J., Garcia-Bellido, J., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hartley, W. G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Jeltema, T., Kim, A. G., Krause, E., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. A. G., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Paz-Chinchon, F., Petravick, D., Pieres, A., Malagon, A. A. Plazas, Prat, J., Romer, A. K., Sanchez, E., Santiago, B., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., and Varga, T. N.
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Astrophysics - Astrophysics of Galaxies - Abstract
We quantify evolution in the cluster scale stellar mass - halo mass (SMHM) relation's parameters using 2323 clusters and brightest central galaxies (BCGs) over the redshift range $0.03 \le z \le 0.60$. The precision on inferred SMHM parameters is improved by including the magnitude gap ($\rm m_{gap}$) between the BCG and fourth brightest cluster member (M14) as a third parameter in the SMHM relation. At fixed halo mass, accounting for $\rm m_{gap}$, through a stretch parameter, reduces the SMHM relation's intrinsic scatter. To explore this redshift range, we use clusters, BCGs, and cluster members identified using the Sloan Digital Sky Survey C4 and redMaPPer cluster catalogs and the Dark Energy Survey redMaPPer catalog. Through this joint analysis, we detect no systematic differences in BCG stellar mass, $\rm m_{gap}$, and cluster mass (inferred from richness) between the datsets. We utilize the Pareto function to quantify each parameter's evolution. We confirm prior findings of negative evolution in the SMHM relation's slope (3.5$\sigma$) and detect negative evolution in the stretch parameter (4.0$\sigma$) and positive evolution in the offset parameter (5.8$\sigma$). This observed evolution, combined with the absence of BCG growth, when stellar mass is measured within 50kpc, suggests that this evolution results from changes in the cluster's $\rm m_{gap}$. For this to occur, late-term growth must be in the intra-cluster light surrounding the BCG. We also compare the observed results to Illustris TNG 300-1 cosmological hydrodynamic simulations and find modest qualitative agreement. However, the simulations lack the evolutionary features detected in the real data., Comment: 21 pages, 12 Figures, 3 Tables. Submitted to ApJ on July 1
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- 2021
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179. A Reduction-Based Framework for Conservative Bandits and Reinforcement Learning
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Yang, Yunchang, Wu, Tianhao, Zhong, Han, Garcelon, Evrard, Pirotta, Matteo, Lazaric, Alessandro, Wang, Liwei, and Du, Simon S.
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Computer Science - Machine Learning ,Statistics - Machine Learning - Abstract
In this paper, we present a reduction-based framework for conservative bandits and RL, in which our core technique is to calculate the necessary and sufficient budget obtained from running the baseline policy. For lower bounds, we improve the existing lower bound for conservative multi-armed bandits and obtain new lower bounds for conservative linear bandits, tabular RL and low-rank MDP, through a black-box reduction that turns a certain lower bound in the nonconservative setting into a new lower bound in the conservative setting. For upper bounds, in multi-armed bandits, linear bandits and tabular RL, our new upper bounds tighten or match existing ones with significantly simpler analyses. We also obtain a new upper bound for conservative low-rank MDP.
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- 2021
180. Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
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Zacharegkas, G., Chang, C., Prat, J., Pandey, S., Ferrero, I., Blazek, J., Jain, B., Crocce, M., DeRose, J., Palmese, A., Seitz, S., Sheldon, E., Hartley, W. G., Wechsler, R. H., Dodelson, S., Fosalba, P., Krause, E., Park, Y., Sánchez, C., Alarcon, A., Amon, A., Bechtol, K., Becker, M. R., Bernstein, G. M., Campos, A., Rosell, A. Carnero, Kind, M. Carrasco, Cawthon, R., Chen, R., Choi, A., Cordero, J., Davis, C., Diehl, H. T., Doux, C., Drlica-Wagner, A., Eckert, K., Elvin-Poole, J., Everett, S., Ferté, A., Gatti, M., Giannini, G., Gruen, D., Gruendl, R. A., Harrison, I., Herner, K., Huff, E. M., Jarvis, M., Kuropatkin, N., Leget, P. -F., MacCrann, N., McCullough, J., Myles, J., Navarro-Alsina, A., Porredon, A., Raveri, M., Rollins, R. P., Roodman, A., Ross, A. J., Rykoff, E. S., Secco, L. F., Sevilla-Noarbe, I., Shin, T., Troxel, M. A., Tutusaus, I., Varga, T. N., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., Abbott, T. M. C., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Bacon, D., Bertin, E., Brooks, D., Burke, D. L., Carretero, J., Castander, F. J., Costanzi, M., da Costa, L. N., Pereira, M. E. S., Desai, S., Dietrich, J. P., Doel, P., Evrard, A. E., Flaugher, B., Frieman, J., García-Bellido, J., Gaztanaga, E., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Kuehn, K., Lima, M., Maia, M. A. G., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Muir, J., Ogando, R. L. C., Paz-Chinchón, F., Pieres, A., Sanchez, E., Serrano, S., Smith, M., Suchyta, E., Tarle, G., Thomas, D., To, C., and Wilkinson, R. D.
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Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
Galaxy-galaxy lensing is a powerful probe of the connection between galaxies and their host dark matter halos, which is important both for galaxy evolution and cosmology. We extend the measurement and modeling of the galaxy-galaxy lensing signal in the recent Dark Energy Survey Year 3 cosmology analysis to the highly nonlinear scales ($\sim 100$ kpc). This extension enables us to study the galaxy-halo connection via a Halo Occupation Distribution (HOD) framework for the two lens samples used in the cosmology analysis: a luminous red galaxy sample (redMaGiC) and a magnitude-limited galaxy sample (MagLim). We find that redMaGiC (MagLim) galaxies typically live in dark matter halos of mass $\log_{10}(M_{h}/M_{\odot}) \approx 13.7$ which is roughly constant over redshift ($13.3-13.5$ depending on redshift). We constrain these masses to $\sim 15\%$, approximately $1.5$ times improvement over previous work. We also constrain the linear galaxy bias more than 5 times better than what is inferred by the cosmological scales only. We find the satellite fraction for redMaGiC (MagLim) to be $\sim 0.1-0.2$ ($0.1-0.3$) with no clear trend in redshift. Our constraints on these halo properties are broadly consistent with other available estimates from previous work, large-scale constraints and simulations. The framework built in this paper will be used for future HOD studies with other galaxy samples and extensions for cosmological analyses., Comment: 32 pages, 21 figures, accepted for publication in MNRAS
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- 2021
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181. Echocardiography phenotypes of right ventricular involvement in COVID-19 ARDS patients and ICU mortality: post-hoc (exploratory) analysis of repeated data from the ECHO-COVID study
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Huang, Stephen, Vieillard-Baron, Antoine, Evrard, Bruno, Prat, Gwenaël, Chew, Michelle S., Balik, Martin, and Clau-Terré, Fernando
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Medical research ,Medicine, Experimental ,Mortality -- France -- United Kingdom ,Echocardiography ,Phenotype -- Genetic aspects ,Coronaviruses -- Genetic aspects ,Acute respiratory distress syndrome -- Genetic aspects -- Patient outcomes ,Health care industry - Abstract
Purpose Exploratory study to evaluate the association of different phenotypes of right ventricular (RV) involvement and mortality in the intensive care unit (ICU) in patients with acute respiratory distress syndrome (ARDS) due to coronavirus disease 2019 (COVID-19). Methods Post-hoc analysis of longitudinal data from the multicenter ECHO-COVID observational study in ICU patients who underwent at least two echocardiography examinations. Echocardiography phenotypes were acute cor pulmonale (ACP, RV cavity dilatation with paradoxical septal motion), RV failure (RVF, RV cavity dilatation and systemic venous congestion), and RV dysfunction (tricuspid annular plane systolic excursion [less than or equal to] 16 mm). Accelerated failure time model and multistate model were used for analysis. Results Of 281 patients who underwent 948 echocardiography studies during ICU stay, 189 (67%) were found to have at least 1 type of RV involvements during one or several examinations: ACP (105/281, 37.4%), RVF (140/256, 54.7%) and/or RV dysfunction (74/255, 29%). Patients with all examinations displaying ACP had survival time shortened by 0.479 [0.284-0.803] times when compared to patients with all examinations depicting no ACP (P = 0.005). RVF showed a trend towards shortened survival time by a factor of 0.642 [0.405-1.018] (P = 0.059), whereas the impact of RV dysfunction on survival time was inconclusive (P = 0.451). Multistate analysis showed that patients might transit in and out of RV involvement, and those who exhibited ACP in their last critical care echocardiography (CCE) examination had the highest risk of mortality (hazard ratio (HR) 3.25 [2.38-4.45], P < 0.001). Conclusion RV involvement is prevalent in patients ventilated for COVID-19 ARDS. Different phenotypes of RV involvement might lead to different ICU mortality, with ACP having the worst outcome., Author(s): Stephen Huang [sup.1], Antoine Vieillard-Baron [sup.2] [sup.3], Bruno Evrard [sup.4], Gwenaël Prat [sup.5], Michelle S. Chew [sup.6], Martin Balik [sup.7], Fernando Clau-Terré [sup.8], Daniel De Backer [sup.9], Armand Mekontso [...]
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- 2023
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182. Lemierre syndrome: the forgotten disease—a case series
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Arnaud Salami, Camille Assouan, Dorian Nasser, Idrissa Garba, Wardatou Dine Mourtada, Assi Romaric Evrard Yapo, and Emmanuel Konan
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Lemierre syndrome ,Thrombophlebitis ,Anticoagulation ,Fusobacterium necrophorum ,Otorhinolaryngology ,RF1-547 - Abstract
Abstract Background The aim of this work is to share the authors’ experience and assist therapeutic decision-making in the management of Lemierre syndrome (LS). This is a retrospective descriptive study carried out in the stomatology, maxillofacial surgery, and ENT departments of the teaching hospital of Treichville (Abidjan, Côte d’Ivoire). LS cases managed from 2013 to 2023 were included in the study. Results Eight patients were enrolled (six men and two women). Internal jugular vein thrombosis was unilateral in 7 cases and bilateral in one. No germs were found in four patients. In one patient, a bacterial co-infection was responsible for the thrombosis. Surgical debridement was systematically performed in cases of necrosis. Anticoagulation was justified in three patients. No deaths were observed. Conclusion This work describes the epidemiological, clinical, therapeutic, and evolutionary aspects of LS. The management of LS should not be improvised. The choice of surgical debridement and anticoagulation depends on specific situations.
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- 2023
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183. 4D Optical fibers based on shape-memory polymers
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Clément Strutynski, Marianne Evrard, Frédéric Désévédavy, Grégory Gadret, Jean-Charles Jules, Claire-Hélène Brachais, Bertrand Kibler, and Frédéric Smektala
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Science - Abstract
Abstract Adaptative objects based on shape-memory materials are expected to significantly impact numerous technological sectors including optics and photonics. In this work, we demonstrate the manufacturing of shape-memory optical fibers from the thermal stretching of additively manufactured preforms. First, we show how standard commercially-available thermoplastics can be used to produce long continuously-structured microfilaments with shape-memory abilities. Shape recovery as well as programmability performances of such elongated objects are assessed. Next, we open the way for light-guiding multicomponent fiber architectures that are able to switch from temporary configurations back to user-defined programmed shapes. In particular, we show that distinct designs of fabricated optical fibers can maintain efficient light transmission upon completion of multiple temperature-triggered bending/straightening cycles. Such fibers are also programmed into more complex shapes including coils or near 180 ° curvatures for delivering laser light around obstacles. Finally, a shape-memory exposed-core fiber is employed in fiber evanescent wave spectroscopy experiments to optimize the performance of the sensing scheme. We strongly expect that such actuatable fibers with light-guiding abilities will trigger exciting progress of unprecedented smart devices in the areas of photonics, electronics, or robotics.
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- 2023
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184. A new scaffold-free tumoroid model provides a robust preclinical tool to investigate invasion and drug response in Renal Cell Carcinoma
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Irinka Séraudie, Catherine Pillet, Beatrice Cesana, Pauline Bazelle, Florian Jeanneret, Bertrand Evrard, Frédéric Chalmel, Assilah Bouzit, Christophe Battail, Jean-Alexandre Long, Jean Luc Descotes, Claude Cochet, and Odile Filhol
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Cytology ,QH573-671 - Abstract
Abstract Clear cell Renal Cell Carcinoma (ccRCC) is one of the most prevalent kidney cancers, which is often asymptomatic and thus discovered at a metastatic state (mRCC). mRCC are highly heterogeneous tumors composed of subclonal populations that lead to poor treatment response rate. Several recent works explored the potential of ccRCC tumoroids culture derived from patients. However, these models were produced following a scaffold-based method using collagen I or Matrigel that exhibit lot variability and whose complexity could induce treatment response modifications and phenotypic alterations. Following the observation that ccRCC tumoroids can create their own niche by secreting extracellular matrix components, we developed the first scaffold-free tumoroid model of ccRCC tumors. Tumoroids from mice as well as from human tumors were generated with high success rate (≥90%) using a magnetic suspension method and standard culture media. Immunofluorescence analysis revealed their self-organization capacities to maintain multiple tumor-resident cell types, including endothelial progenitor cells. Transcriptomic analysis showed the reproducibility of the method highlighting that the majority of gene expression patterns was conserved in tumoroids compared to their matching tumor tissue. Moreover, this model enables to evaluate drug effects and invasiveness of renal cancer cells in a 3D context, providing a robust preclinical tool for drug screening and biomarker assessment in line with alternative ex vivo methods like tumor tissue slice culture or in vivo xenograft models.
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- 2023
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185. El Niño–Southern Oscillation (ENSO)-driven hypersedimentation in the Poechos Reservoir, northern Peru
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A. Foucher, S. Morera, M. Sanchez, J. Orrillo, and O. Evrard
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Technology ,Environmental technology. Sanitary engineering ,TD1-1066 ,Geography. Anthropology. Recreation ,Environmental sciences ,GE1-350 - Abstract
Although extreme El Niño events (EENEs) have always impacted hydrological anomalies and sediment transport in South America, their intensification by global warming and their association with changes in human activities and land cover after humid periods may lead to the acceleration of sediment transfers in river systems and dam reservoirs. This situation may threaten soil and water resources in arid and semiarid regions highly dependent on water originating from large dams. In this study, we investigated the sediment sequence accumulated in the Poechos Reservoir (northern Peru) and provided a retrospective reconstruction of the interactions of El Niño–Southern Oscillation (ENSO), agricultural practices and vegetation cover changes with sediment dynamics (1978–2019). To this end, a sediment core was dated and characterized by physical and chemical analyses (e.g., scanner tomography, X-ray fluorescence, particle size analysis) to estimate the evolution of sedimentation rates and changes in sediment sources during the last 5 decades. Sediment tracing results indicated the occurrence of changes in sediment sources associated with positive and negative phases of the Eastern Pacific index with a greater contribution of the lowland dry-forest area in comparison to that of the Andean area to sediment during the El Niño events (mean contribution of 76 %; up to 90 % during the coastal El Niño events (CENEs) of 2016–2017). This source contribution was mostly controlled by the stationary rainfall occurring during the EENEs in the lowland dry-forest area characterized by a low vegetation cover. Overall, after an extreme phase of ENSO, like after the EENE 1982–1983, the normal discharges and persistent sediment supplies from the middle- and upper-catchment parts led to river aggradation and the storage of substantial amounts of sediment in alluvial plains. In the absence of a significant EENE between 1983 and 1997, the large volume of sediment stored in the alluvial plains was exported by the EENE 1997–1998 resulting in an increase in sedimentation rate of 140 % after 1997 with a significant aggradation of the deltaic zone of the reservoir. In addition to the impact of extreme climate events on sediment dynamics, the development of agriculture along the riverine system after an extreme phase of ENSO increased the availability of sediments in the main channel of the rivers, easily transported by the next EENE. This study suggests that intensification of human activities associated with a higher frequency of extreme rainfall events amplified the quantity of sediment transported by the river system, which will significantly decrease the lifespan of the reservoir, which is essential to meeting the freshwater demands of the farmers and the populations living in this arid and semiarid region.
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- 2023
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186. Research and management challenges following soil and landscape decontamination at the onset of the reopening of the Difficult-to-Return Zone, Fukushima (Japan)
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O. Evrard, T. Chalaux-Clergue, P.-A. Chaboche, Y. Wakiyama, and Y. Thiry
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Environmental sciences ,GE1-350 ,Geology ,QE1-996.5 - Abstract
Twelve years after the nuclear accident that occurred at the Fukushima Dai-ichi Nuclear Power Plant (FDNPP) in March 2011, radiocesium contamination (with a large dominance of 137Cs, with a 30-year half-life) remains a major concern in various municipalities of north-eastern Japan. The Japanese authorities completed an unprecedented soil decontamination programme in residential and cultivated areas affected by the main radioactive plume (8953 km2). They implemented a complex remediation programme scheme to remediate soils that are fundamental to life on Earth, relying on different decision rules depending on the waste type, its contamination level and its region of origin, after delineating different zones exposed to contrasted radiation rates. The central objective was not to expose local inhabitants to radioactive doses exceeding 1 mSv yr−1 in addition to the natural levels. At the onset of the full reopening of the Difficult-to-Return Zone (DTRZ) in spring 2023, the current review provides an update of a previous synthesis published in 2019 (Evrard et al., 2019). Although this ambitious soil remediation and reconstruction programme has almost been completed in the 12 municipalities of Fukushima Prefecture in which an evacuation order was imposed in at least one neighbourhood in 2011, from the 147 443 inhabitants who lived there before the accident, only 29.9 % of them had returned by 2020. Waste generated by decontamination and tsunami cleaning/demolition work is planned to have been fully transported to (interim) storage facilities by the end of 2023. The cost of the operations conducted between 2011 and 2020 for the so-called “nuclear recovery” operations (including decontamination) was estimated by the Board of Audit of Japan in 2023 as JPY 6122.3 billion (∼ EUR 44 billion). Decontamination of cropland was shown to have impacted soil fertility, and potassium fertilisation is recommended to limit the transfer of residual radiocesium to new crops. In forests that cover 71 % of the surface area of Fukushima Prefecture and that were not targeted by remediation, radiocesium is now found in the upper mineral layer of the soil in a quasi-equilibrium state. Nevertheless, 137Cs concentrations in forest products (including wood for heating and construction, wild plants, wildlife game, mushrooms) often keep exceeding the threshold values authorised in Japan, which prohibits their exploitation in the area affected by the main plume. Radionuclides from forests were shown to be exported in dissolved and particle-bound forms to downstream river systems and floodplains, although multiple monitoring records showed the continuous decrease in radiocesium concentrations in both river water and sediment across the main plume between 2011 and 2021. Fish contamination is now generally found to be below the threshold limits although reputational damage remains a major concern for local fishing communities. The remobilisation of radiocesium from sediment accumulated in reservoirs of the region is also of potential concern as it may lead to secondary contamination of fish or irrigation waters supplied to decontaminated fields. Overall, this synthesis demonstrates the need to continue monitoring post-accidental radiocesium transfer in these environments and to keep sharing data in order to refine our predictive understanding of radiocesium mobility and consolidate the tools available to model contaminant transfer in ecosystems. In forests in particular, novel countermeasures and wood uses remain to be developed and tested. Furthermore, the hydrologic connectivity between soils under different ecosystems greatly influences long-term radiocesium transport. The consequences of extreme phenomena (e.g. typhoons, forest fires) that may become more frequent in the future as a result of global change in these contaminated environments should be further anticipated.
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- 2023
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187. Long-term immunosuppressive treatment is not associated with worse outcome in patients hospitalized in the intensive care unit for septic shock: the PACIFIC study
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Julien Vaidie, Edwige Peju, Louise-Marie Jandeaux, Mathieu Lesouhaitier, Jean-Claude Lacherade, Antoine Guillon, Xavier Wittebole, Pierre Asfar, Bruno Evrard, Thomas Daix, Philippe Vignon, and Bruno François
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Septic shock ,Intensive care unit ,Immunosuppression therapy ,Organ transplantation ,Autoimmune diseases ,Mortality ,Medical emergencies. Critical care. Intensive care. First aid ,RC86-88.9 - Abstract
Abstract Background Except in a few retrospective studies mainly including patients under chemotherapy, information regarding the impact of immunosuppressive therapy on the prognosis of patients admitted to the intensive care unit (ICU) for septic shock is scarce. Accordingly, the PACIFIC study aimed to asses if immunosuppressive therapy is associated with an increased mortality in patients admitted to the ICU for septic shock. Methods This was a retrospective epidemiological multicentre study. Eight high enroller centres in septic shock randomised controlled trials (RCTs) participated in the study. Patients in the “exposed” group were selected from the screen failure logs of seven recent RCTs and excluded because of immunosuppressive treatment. The “non-exposed” patients were those included in the placebo arm of the same RCTs. A multivariate logistic regression model was used to estimate the risk of death. Results Among the 433 patients enrolled, 103 were included in the “exposed” group and 330 in the “non-exposed” group. Reason for immunosuppressive therapy included organ transplantation (n = 45 [44%]) or systemic disease (n = 58 [56%]). ICU mortality rate was 24% in the “exposed” group and 25% in the “non-exposed” group (p = 0.9). Neither in univariate nor in multivariate analysis immunosuppressive therapy was associated with a higher ICU mortality (OR: 0.95; [95% CI 0.56–1.58]: p = 0.86 and 1.13 [95% CI 0.61–2.05]: p = 0.69, respectively) or 3-month mortality (OR: 1.13; [95% CI 0.69–1.82]: p = 0.62 and OR: 1.36 [95% CI 0.78–2.37]: p = 0.28, respectively). Conclusions In this study, long-term immunosuppressive therapy excluding chemotherapy was not associated with significantly higher or lower ICU and 3-month mortality in patients admitted to the ICU for septic shock.
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- 2023
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188. Inexorable land degradation due to agriculture expansion in South American Pampa
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Foucher, Anthony, Tassano, Marcos, Chaboche, Pierre-Alexis, Chalar, Guillermo, Cabrera, Mirel, Gonzalez, Joan, Cabral, Pablo, Simon, Anne-Catherine, Agelou, Mathieu, Ramon, Rafael, Tiecher, Tales, and Evrard, Olivier
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- 2023
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189. Evaluation of amorphous and lipid-based formulation strategies to increase the in vivo cannabidiol bioavailability in piglets
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Koch, N., Jennotte, O., Bourcy, Q., Lechanteur, A., Deville, M., Charlier, C., Chiap, P., Cardot, J.M., and Evrard, B.
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- 2024
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190. Hydrocortisone plus fludrocortisone for community acquired pneumonia-related septic shock: a subgroup analysis of the APROCCHSS phase 3 randomised trial
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Djillali, ANNANE, Christian, BRUN-BUISSON, Benoit, MISSET, Jean, CHASTRE, François, BRIVET, Julien, BOHE, Carole, SCHWEBEL, Shidasp, SIAMI, Michel, SLAMA, Olivier, LEROY, Gilles, CAPELLIER, Michel, WOLFF, Mohamed, ALI BEN ALI, François, ANTONINI, Jean-François, LORIFERNE, Franck, PETITPAS, Claire, CHARPENTIER, Jean-Michel, CONSTANTIN, Gilles, D'HONNEUR, Bertrand, SOUWEINE, Xavier, FORCEVILLE, Bruno, MEGARBANE, Francois, BAUDIN, Gwenhaël, COLIN, Karim, ASEHNOUNE, Jean-Pierre, QUENOT, Bruno, FRANCOIS, Thierry, BOULAIN, Emmanuelle, MERCIER, Jean, REIGNIER, Roland, AMATHIEU, Fabrice, COOK, Alain, CARIOU, Loic, CHIMOT, Fouad, Fadel, Andrea, Polito, Bernard, Clair, Virginie, Maxime, David, Luis, Tarek, Sharshar, David, Orlikowski, Keyvan, RAZAZI, Nicolas, DE PROST, Guillaume, CARTEAUX, Maité, GARROUSTE ORGEAS, François, Philippart, Alain, Combes, Ania, Nieszkowska, Frederic, Jacobs, Dominique, Prat, Patrick, Lafforgue, Claire, ARA SOMOHANO, Clémence, MINET, Maxime, LUGOSI, Julien, Maizel, Jean Christophe, Navellou, Bruno, Mourvillier, Lila, Bouadma, Jean François, Timsit, Claude Denis, Martin, Julien, Textoris, Sandrine, Wiramus, Clément, BRUN, Benoît, RAGONNET, Ali, Ait-Hssain, Samia, Touati, Jean, Kuba, Vincent, Willems, Pierre, Lahillaire, Mohammed, Lassi, Marion, ANTONA, Alia, MEGHENEM, Marine, DEMESMAY, Eric, Boulet, Olivier, LOUTREL, Romain, DUMONT, Antoine, ROQUILLY, Pierre-Joachim, MAHE, Dominique, DEMEURE dit LATTE, Philippe, CHAMPIN, Jean François, ARNOULD, Raphaël, CINOTTI, Ronan, Le FLOCH, Marc, Clavel, Philippe, Vignon, Nicolas, Pichon, Emmanuelle, BEGOT, Anne-Laure, FEDOU, Catherine, CHAPELLAS, Antoine, GALY, Dalila, Benzekri Lefevre, Armelle, Mathonnet, Anne, Bretagnol, Isabelle, Runge, François, BARBIER, Grégoire, MULLER, Denis, GAROT, Pierre François, DEQUIN, Dominique, PERROTIN, Annick, LEGRAS, Julie, MANKIKIAN, Patrice, TALEC, Stephan, EHRMANN, Aurélie, JORET, Claire, LHOMMET, Emmanuelle, ROUVE, Laetitia, BODET-CONTENTIN, Youenn, JOUAN, Charlotte, SALMONGANDONNIERE, Laurent, MARTIN-LEFEVRE, Matthieu, HENRY-LAGARRIGUE, Aihem, YEHIA, Jean-Baptiste, LASCARROU, Christine, LEBERT, Jean-Claude, LACHERADE, Eric, LEVESQUE, Yen-Lan, NGUYEN, Fabrice, DAVIAUD, Adrien, BOUGLE, Jean Paul, MIRA, Jean Daniel, CHICHE, Frederic, PENE, Tristan, MORICHAU-BEAUCHANT, Guillaume, GERI, Pierre Henri, DESSALLES, Yannick, MONSEAU, Mélanie, SAINT-LEGER, Sandrine, BEDON-CARTE, Laetitia, Bodet-Contentin, Walid, Darwiche, Stephan, Ehrmann, Denis, Garot, Antoine, Guillon, Youenn, Jouan, Annick, Legras, Julie, Mankikian, Emmanuelle, Mercier, Marlene, Morisseau, Yonatan, Perez, Emmanuelle, Rouve, Charlotte, Salmon-Gandonniere, Julie, Helms, Hassene, Rahmani, Alexandra, Monnier, Hamid, Merdji, Raphael, Clere-Jehl, Laure, Stiel, Antoine, Studer, Pascal, Andreu, Jean-Baptiste, Roudaut, Marie, Labruyere, Marine, Jacquier, Francois, Barbier, Dalila, Benzekri, Thierry, Boulain, Sophie, Jacquier, Gregoire, Muller, Mai-Anh, Nai, Sophie, Tollec, Damien, Roux, Jonathan, Messika, Constance, Vuillard, Louis-Marie, Dumont, Laura, Federici, Noemie, Zucman, Marc, Amouretti, Djillali, Annane, Pierre, Moine, Paris, Meng, Rania, Bounab, Muriel-Sarah, Fartoukh, Michel, Djibre, Alexandre, Elabbadi, Marie-Ange, Azais, Konstantinos, Bachoumas, Arthur, Bailly, Remi, Bernardon, Gauthier, Blonz, Luc, Desmedt, Brian, Emonet, Maud, Fiancette, Matthieu, Henry, Jean-Claude, Lacherade, Jean-Baptiste, Lascarrou, Christine, Lebert, Julien, Lorber, Laurent Martin-, Lefevre, Caroline, Pouplet, Isabelle, Vinatier, Aihem, Yehia, Sarah, Benghanem, Julien, Charpentier, Clara, Vigneron, Anne-Laure, Fedou, Claire, Mancia, Emmanuelle, Begot, Thomas, Daix, Antoine, Galy, Celine, Gonzalez, Marine, Goudelin, Bruno, Evrard, Arnaud, Desachy, Julien, Vaidie, Guillaume, Gilbert, Cedric, Darreau, Benoit, Derrien, Marjorie, Saint-Martin, Patrice, Tirot, Mickael, Landais, Nicolas, Chudeau, Jean Christophe, Callahan, Dominique, Vivier, Charlene, Le Moal, Pierre-Yves, Olivier, Remy, Marnai, Francis, Schneider, Nicolas, Sedillot, Xavier, Tchenio, Adrien, Robine, Yves, Poncelin, Remi, Bruyere, Heming, Nicholas, Renault, Alain, Kuperminc, Emmanuelle, Brun-Buisson, Christian, Megarbane, Bruno, Quenot, Jean-Pierre, Siami, Shidasp, Cariou, Alain, Forceville, Xavier, Schwebel, Carole, Leone, Marc, Timsit, Jean-Francois, Misset, Benoît, Benali, Mohamed Ali, Colin, Gwenhael, Souweine, Bertrand, Asehnoune, Karim, Mercier, Emmanuelle, Chimot, Loïc, Charpentier, Claire, François, Bruno, Boulain, Thierry, Petitpas, Frank, Constantin, Jean Michel, Dhonneur, Gilles, Baudin, François, Combes, Alain, Bohé, Julien, Loriferne, Jean-François, Cook, Fabrice, Slama, Michel, Leroy, Olivier, Capellier, Gilles, Dargent, Auguste, Hissem, Tarik, Bounab, Rania, Maxime, Virginie, Moine, Pierre, Bellissant, Eric, and Annane, Djillali
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- 2024
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191. Facile synthesis of pyrite FeS2 on carbon spheres for high-efficiency Fenton-like reaction
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Ma, Chengbo, Liu, Yuexu, Wang, Jun, Evrard Deric, Nkuissi Tchikou, Li, Yang, Fan, Xiaobin, and Peng, Wenchao
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- 2024
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192. Development of a circularity design methodology for urban factories based on systemic thinking and stakeholders engagement
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Ijassi, Walid, Evrard, Damien, and Zwolinski, Peggy
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- 2024
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193. Transcriptional landscape of human keratinocyte models exposed to 60-GHz millimeter-waves
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Martin, Catherine, Evrard, Bertrand, Percevault, Frédéric, Ryder, Kate, Darde, Thomas, Lardenois, Aurélie, Zhadobov, Maxim, Sauleau, Ronan, Chalmel, Frédéric, Le Dréan, Yves, and Habauzit, Denis
- Published
- 2024
- Full Text
- View/download PDF
194. Vascular study of decellularized porcine long bones: Characterization of a tissue engineering model
- Author
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Evrard, R., Manon, J., Rafferty, C., Fieve, L., Cornu, O., Kirchgesner, T., Lecouvet, F.E., Schubert, T., and Lengele, B.
- Published
- 2024
- Full Text
- View/download PDF
195. Equivalent-oriented model for sandwich panels with ZPR accordion honeycomb
- Author
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Minfang, Chen, Yifeng, Zhong, Rong, Liu, Shiwen, Wang, and Evrard, Irakoze Alain
- Published
- 2024
- Full Text
- View/download PDF
196. VAM-based equivalent-homogenization model for 3D re-entrant auxetic honeycomb structures
- Author
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Liu, Rong, Zhong, Yifeng, Wang, Shiwen, Irakoze, Alain Evrard, and Miao, Siqi
- Published
- 2024
- Full Text
- View/download PDF
197. Comparison of methods for curvature estimation from volume fractions
- Author
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Han, Austin, Evrard, Fabien, and Desjardins, Olivier
- Published
- 2024
- Full Text
- View/download PDF
198. Carcinomas of the external auditory canal: Management and results: A multicenter REFCOR propensity score matching study
- Author
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Brenet, Esteban, Atallah, Sarah, Guerlain, Joanne, Moya-Plana, Antoine, Verillaud, Benjamin, Kania, Romain, Bakhos, David, Philouze, Pierre, Righini, Christian-Adrien, Bozorg, Alexis, Mérol, Jean-Claude, Labrousse, Marc, Vergez, Sébastien, Fakhry, Nicolas, Gallet, Patrice, Cullié, Dorian, Malard, Olivier, Mauvais, Olivier, Fath, Léa, Schultz, Philippe, Dufour, Xavier, Saroul, Nicolas, Evrard, Diane, Lesnik, Maria, Even, Caroline, Costes, Valérie, Thariat, Juliette, Taillandier de Gabory, Ludovic Le, Makeieff, Marc, Dubernard, Xavier, and Baujat, Bertrand
- Published
- 2024
- Full Text
- View/download PDF
199. « Il est urgent de contrer le développement de la médecine intégrative et de sauver la vraie médecine ». Analyse critique de dix arguments rationalistes sceptiques
- Author
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Berna, Fabrice, Lecardeur, Laurent, Verneuil, Laurence, Nizard, Julien, and Evrard, Renaud
- Published
- 2024
- Full Text
- View/download PDF
200. Dimensions auto-curatives et pré-engagement thérapeutique du « développement personnel »
- Author
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Ledeuil, Louis and Evrard, Renaud
- Published
- 2024
- Full Text
- View/download PDF
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