441 results on '"Philippe Lamy"'
Search Results
52. Supplementary information from Cellular Disposal of miR23b by RAB27-Dependent Exosome Release Is Linked to Acquisition of Metastatic Properties
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Torben Falck Ørntoft, Lars Dyrskjøt, Kenneth A. Howard, Michael Borre, Dan Theodorescu, Martin Beck, Jakob S. Pedersen, Jørgen B. Jensen, Jens P. Morth, Iver Nordentoft, Erik I. Christensen, Niels Fristrup, Khan H. Bui, Mads H. Rasmussen, Frederik Dagnaes-Hansen, Philippe Lamy, An Hendrix, Bjarke Primdal-Bengtson, Jesper B. Bramsen, Anders T. Boysen, Jens R. Laurberg, Dennis K. Jeppesen, and Marie Stampe Ostenfeld
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Supplementary materials&methods and figure legends for supplementary figures and tables.
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- 2023
53. Supplementary Table 3 from Genomic Profiling of MicroRNAs in Bladder Cancer: miR-129 Is Associated with Poor Outcome and Promotes Cell Death In vitro
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Torben F. Ørntoft, Michael Borre, Jørgen Kjems, Benedicte P. Ulhøi, Sakari Kauppinen, Karsten Zieger, Claus L. Andersen, Jens L. Jensen, Niels Fristrup, Ramshanker Ramanathan, Philippe Lamy, Asli N. Silahtaroglu, Jesper B. Bramsen, Marie S. Ostenfeld, and Lars Dyrskjøt
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Supplementary Table 3 from Genomic Profiling of MicroRNAs in Bladder Cancer: miR-129 Is Associated with Poor Outcome and Promotes Cell Death In vitro
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- 2023
54. Supplementary Figure 3 from Cellular Disposal of miR23b by RAB27-Dependent Exosome Release Is Linked to Acquisition of Metastatic Properties
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Torben Falck Ørntoft, Lars Dyrskjøt, Kenneth A. Howard, Michael Borre, Dan Theodorescu, Martin Beck, Jakob S. Pedersen, Jørgen B. Jensen, Jens P. Morth, Iver Nordentoft, Erik I. Christensen, Niels Fristrup, Khan H. Bui, Mads H. Rasmussen, Frederik Dagnaes-Hansen, Philippe Lamy, An Hendrix, Bjarke Primdal-Bengtson, Jesper B. Bramsen, Anders T. Boysen, Jens R. Laurberg, Dennis K. Jeppesen, and Marie Stampe Ostenfeld
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Analysis of RAB27A and RAB27B expression and genomic alterations in clinical samples. Effect of Rab27b knockdown on cell morphology and long-term growth kinetics.
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- 2023
55. Supplementary Table 6 from Genomic Profiling of MicroRNAs in Bladder Cancer: miR-129 Is Associated with Poor Outcome and Promotes Cell Death In vitro
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Torben F. Ørntoft, Michael Borre, Jørgen Kjems, Benedicte P. Ulhøi, Sakari Kauppinen, Karsten Zieger, Claus L. Andersen, Jens L. Jensen, Niels Fristrup, Ramshanker Ramanathan, Philippe Lamy, Asli N. Silahtaroglu, Jesper B. Bramsen, Marie S. Ostenfeld, and Lars Dyrskjøt
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Supplementary Table 6 from Genomic Profiling of MicroRNAs in Bladder Cancer: miR-129 Is Associated with Poor Outcome and Promotes Cell Death In vitro
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- 2023
56. Supplementary Figure 4 from Cellular Disposal of miR23b by RAB27-Dependent Exosome Release Is Linked to Acquisition of Metastatic Properties
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Torben Falck Ørntoft, Lars Dyrskjøt, Kenneth A. Howard, Michael Borre, Dan Theodorescu, Martin Beck, Jakob S. Pedersen, Jørgen B. Jensen, Jens P. Morth, Iver Nordentoft, Erik I. Christensen, Niels Fristrup, Khan H. Bui, Mads H. Rasmussen, Frederik Dagnaes-Hansen, Philippe Lamy, An Hendrix, Bjarke Primdal-Bengtson, Jesper B. Bramsen, Anders T. Boysen, Jens R. Laurberg, Dennis K. Jeppesen, and Marie Stampe Ostenfeld
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Effect of RAB27A, RAB27B, and NSMASE2 inhibition on cellular migration and invasion. Bioinformatic analysis of mRNA target sites, AGO2 immunoprecipitation. Analysis of genomic alterations in the miR23b locus and correlation between expression and methylation of selected miRNAs (TCGA dataset).
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- 2023
57. Supplementary Table 2 from Cellular Disposal of miR23b by RAB27-Dependent Exosome Release Is Linked to Acquisition of Metastatic Properties
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Torben Falck Ørntoft, Lars Dyrskjøt, Kenneth A. Howard, Michael Borre, Dan Theodorescu, Martin Beck, Jakob S. Pedersen, Jørgen B. Jensen, Jens P. Morth, Iver Nordentoft, Erik I. Christensen, Niels Fristrup, Khan H. Bui, Mads H. Rasmussen, Frederik Dagnaes-Hansen, Philippe Lamy, An Hendrix, Bjarke Primdal-Bengtson, Jesper B. Bramsen, Anders T. Boysen, Jens R. Laurberg, Dennis K. Jeppesen, and Marie Stampe Ostenfeld
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Lists of i) top30 exocytosed miRNAs and ii) cellular-retained miRNAs.
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- 2023
58. Data from Genomic Profiling of MicroRNAs in Bladder Cancer: miR-129 Is Associated with Poor Outcome and Promotes Cell Death In vitro
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Torben F. Ørntoft, Michael Borre, Jørgen Kjems, Benedicte P. Ulhøi, Sakari Kauppinen, Karsten Zieger, Claus L. Andersen, Jens L. Jensen, Niels Fristrup, Ramshanker Ramanathan, Philippe Lamy, Asli N. Silahtaroglu, Jesper B. Bramsen, Marie S. Ostenfeld, and Lars Dyrskjøt
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microRNAs (miRNA) are involved in cancer development and progression, acting as tumor suppressors or oncogenes. Here, we profiled the expression of 290 unique human miRNAs in 11 normal and 106 bladder tumor samples using spotted locked nucleic acid–based oligonucleotide microarrays. We identified several differentially expressed miRNAs between normal urothelium and cancer and between the different disease stages. miR-145 was found to be the most down-regulated in cancer compared with normal, and miR-21 was the most up-regulated in cancer. Furthermore, we identified miRNAs that significantly correlated to the presence of concomitant carcinoma in situ. We identified several miRNAs with prognostic potential for predicting disease progression (e.g., miR-129, miR-133b, and miR-518c*). We localized the expression of miR-145, miR-21, and miR-129 to urothelium by in situ hybridization. We then focused on miR-129 that exerted significant growth inhibition and induced cell death upon transfection with a miR-129 precursor in bladder carcinoma cell lines T24 and SW780 cells. Microarray analysis of T24 cells after transfection showed significant miR-129 target down-regulation (P = 0.0002) and pathway analysis indicated that targets were involved in cell death processes. By analyzing gene expression data from clinical tumor samples, we identified significant expression changes of target mRNA molecules related to the miRNA expression. Using luciferase assays, we documented a direct link between miR-129 and the two putative targets GALNT1 and SOX4. The findings reported here indicate that several miRNAs are differentially regulated in bladder cancer and may form a basis for clinical development of new biomarkers for bladder cancer. [Cancer Res 2009;69(11):4851–60]
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- 2023
59. Supplementary Figure 1 from Genomic Profiling of MicroRNAs in Bladder Cancer: miR-129 Is Associated with Poor Outcome and Promotes Cell Death In vitro
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Torben F. Ørntoft, Michael Borre, Jørgen Kjems, Benedicte P. Ulhøi, Sakari Kauppinen, Karsten Zieger, Claus L. Andersen, Jens L. Jensen, Niels Fristrup, Ramshanker Ramanathan, Philippe Lamy, Asli N. Silahtaroglu, Jesper B. Bramsen, Marie S. Ostenfeld, and Lars Dyrskjøt
- Abstract
Supplementary Figure 1 from Genomic Profiling of MicroRNAs in Bladder Cancer: miR-129 Is Associated with Poor Outcome and Promotes Cell Death In vitro
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- 2023
60. Supplementary Figure 2 from Cellular Disposal of miR23b by RAB27-Dependent Exosome Release Is Linked to Acquisition of Metastatic Properties
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Torben Falck Ørntoft, Lars Dyrskjøt, Kenneth A. Howard, Michael Borre, Dan Theodorescu, Martin Beck, Jakob S. Pedersen, Jørgen B. Jensen, Jens P. Morth, Iver Nordentoft, Erik I. Christensen, Niels Fristrup, Khan H. Bui, Mads H. Rasmussen, Frederik Dagnaes-Hansen, Philippe Lamy, An Hendrix, Bjarke Primdal-Bengtson, Jesper B. Bramsen, Anders T. Boysen, Jens R. Laurberg, Dennis K. Jeppesen, and Marie Stampe Ostenfeld
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Characterization of cells upon miRNA overexpression and knockdown.
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- 2023
61. Supplementary Table 3 from Cellular Disposal of miR23b by RAB27-Dependent Exosome Release Is Linked to Acquisition of Metastatic Properties
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Torben Falck Ørntoft, Lars Dyrskjøt, Kenneth A. Howard, Michael Borre, Dan Theodorescu, Martin Beck, Jakob S. Pedersen, Jørgen B. Jensen, Jens P. Morth, Iver Nordentoft, Erik I. Christensen, Niels Fristrup, Khan H. Bui, Mads H. Rasmussen, Frederik Dagnaes-Hansen, Philippe Lamy, An Hendrix, Bjarke Primdal-Bengtson, Jesper B. Bramsen, Anders T. Boysen, Jens R. Laurberg, Dennis K. Jeppesen, and Marie Stampe Ostenfeld
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Lists of A)Quantitative mass spectrometry results of RNA-binding proteins in exosomes, B) Selected miRNAs for further analysis, and C) Downregulated mRNA transcripts (selected) upon RAB27B knockdown.
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- 2023
62. Supplementary Table 1 from Cellular Disposal of miR23b by RAB27-Dependent Exosome Release Is Linked to Acquisition of Metastatic Properties
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Torben Falck Ørntoft, Lars Dyrskjøt, Kenneth A. Howard, Michael Borre, Dan Theodorescu, Martin Beck, Jakob S. Pedersen, Jørgen B. Jensen, Jens P. Morth, Iver Nordentoft, Erik I. Christensen, Niels Fristrup, Khan H. Bui, Mads H. Rasmussen, Frederik Dagnaes-Hansen, Philippe Lamy, An Hendrix, Bjarke Primdal-Bengtson, Jesper B. Bramsen, Anders T. Boysen, Jens R. Laurberg, Dennis K. Jeppesen, and Marie Stampe Ostenfeld
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miRNA profiling in exosomes and cells.
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- 2023
63. Supplementary Table 2 from Genomic Profiling of MicroRNAs in Bladder Cancer: miR-129 Is Associated with Poor Outcome and Promotes Cell Death In vitro
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Torben F. Ørntoft, Michael Borre, Jørgen Kjems, Benedicte P. Ulhøi, Sakari Kauppinen, Karsten Zieger, Claus L. Andersen, Jens L. Jensen, Niels Fristrup, Ramshanker Ramanathan, Philippe Lamy, Asli N. Silahtaroglu, Jesper B. Bramsen, Marie S. Ostenfeld, and Lars Dyrskjøt
- Abstract
Supplementary Table 2 from Genomic Profiling of MicroRNAs in Bladder Cancer: miR-129 Is Associated with Poor Outcome and Promotes Cell Death In vitro
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- 2023
64. Supplementary Table 4 from Genomic Profiling of MicroRNAs in Bladder Cancer: miR-129 Is Associated with Poor Outcome and Promotes Cell Death In vitro
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Torben F. Ørntoft, Michael Borre, Jørgen Kjems, Benedicte P. Ulhøi, Sakari Kauppinen, Karsten Zieger, Claus L. Andersen, Jens L. Jensen, Niels Fristrup, Ramshanker Ramanathan, Philippe Lamy, Asli N. Silahtaroglu, Jesper B. Bramsen, Marie S. Ostenfeld, and Lars Dyrskjøt
- Abstract
Supplementary Table 4 from Genomic Profiling of MicroRNAs in Bladder Cancer: miR-129 Is Associated with Poor Outcome and Promotes Cell Death In vitro
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- 2023
65. Immune Contexture and Differentiation Features Predict Outcome in Bladder Cancer
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Ann Taber, Frederik Prip, Philippe Lamy, Mads Agerbæk, Jørgen Bjerggaard Jensen, Torben Steiniche, and Lars Dyrskjøt
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Immune contexture ,Urology ,Programmed Cell Death 1 Receptor ,Bladder cancer ,Response ,B7-H1 Antigen ,Progression-Free Survival ,Urinary Bladder Neoplasms ,Oncology ,Humans ,Chemotherapy ,Radiology, Nuclear Medicine and imaging ,Surgery ,Biomarkers - Abstract
BACKGROUND: An improved risk assessment of patients with bladder cancer (BC) is important to optimize clinical management. OBJECTIVE: To identify whether immune cell subpopulations and cancer cell-intrinsic features are associated with outcome and response to first-line chemotherapy in BC. DESIGN, SETTING, AND PARTICIPANTS: Primary tumor tissue from 785 patients with BC (stage Ta-T4b) were stained using multiplex immunofluorescence (CD3, CD8, FOXP3, CD20, CD68, CD163, and MHC-I) and immunohistochemistry (pancytokeratin, CK5/6, GATA3, programmed death 1 [PD-1], and programmed death ligand 1 [PD-L1]). A digital image analysis quantified staining results within the carcinoma cell and stromal part of the tumor. OUTCOME MEASUREMENTS AND STATISTICAL ANALYSIS: Primary endpoints were progression-free survival, recurrence-free survival, and response to first-line chemotherapy. Optimal cutoff values for investigated markers were estimated using maximally selected rank statistics and receiver operating characteristic for each primary endpoint. Time-to-event analyses were performed using Cox regression analyses. RESULTS AND LIMITATIONS: Several immune subpopulations were independently associated with clinical outcomes. Especially, high PD-1 and PD-L1 expression was independently associated with an increased risk of recurrence and progression in non-muscle-invasive tumors, but with a lower risk of recurrence in muscle-invasive tumors. Furthermore, we observed a lower likelihood of response to first-line chemotherapy in patients with basal differentiation features. Finally, a model combining clinical risk factors with our most evident prognosticator improved prediction accuracy compared with clinical risk factors alone for progression in non-muscle-invasive BC and recurrence in muscle-invasive BC. The use of tissue microarrays and a long inclusion period are limitations to this study. CONCLUSIONS: Immune cell subpopulations and cancer cell-intrinsic features are associated with different clinical outcomes in BC. PATIENT SUMMARY: Immune cells play an important role in cancer development and treatment outcomes. Infiltration with specific immune cells and the presence of markers associated with immune evasion in the tumor predict clinical outcomes in bladder cancer.
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- 2022
66. Histoire de la commission « extrême droite » de la Ligue des droits de l’homme
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Philippe Lamy
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- 2022
67. Field cancerization impacts tumor development, T-cell exhaustion and clinical outcomes in bladder cancer
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Trine Strandgaard, Iver Nordentoft, Karin Birkenkamp-Demtröder, Liina Salminen, Frederik Prip, Julie Rasmussen, Tine Ginnerup Andreasen, Sia Viborg Lindskrog, Emil Christensen, Philippe Lamy, Michael Knudsen, Torben Steiniche, Jørgen Bjerggaard Jensen, and Lars Dyrskjøt
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Bladder field cancerization may be associated with disease outcome in patients with bladder cancer. To investigate this, we analyzed biopsies from bladder urothelium and urine samples by genomics and proteomics analyses. Samples were procured from multiple timepoints from 134 patients with early stage bladder cancer and detailed long term follow-up. We measured the field cancerization in normal-appearing bladder biopsies and found that high levels were associated with high tumor mutational burden, high neoantigen load, and high tumor-associated CD8 T-cell exhaustion. Non-synonymous mutations in known bladder cancer driver genes such asKDM6AandTP53were identified as early disease drivers in normal urothelium. High field cancerization was associated with worse outcome but not with response to BCG. The level of urinary tumor DNA (utDNA) reflected the bladder tumor burden and originated from both tumors and field cancerization. High utDNA levels after BCG were associated with worse clinical outcomes for the patients. Our results indicate that the level of field cancerization may affect clinical outcome, tumor development and immune responses. utDNA measurements have significant prognostic value and reflect the disease status of the bladder.
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- 2023
68. Genome-wide Association Study of Bladder Cancer Reveals New Biological and Translational Insights
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Stella Koutros, Lambertus A. Kiemeney, Parichoy Pal Choudhury, Roger L. Milne, Evangelina Lopez de Maturana, Yuanqing Ye, Vijai Joseph, Oscar Florez-Vargas, Lars Dyrskjøt, Jonine Figueroa, Diptavo Dutta, Graham G. Giles, Michelle A.T. Hildebrandt, Kenneth Offit, Manolis Kogevinas, Elisabete Weiderpass, Marjorie L. McCullough, Neal D. Freedman, Demetrius Albanes, Charles Kooperberg, Victoria K. Cortessis, Margaret R. Karagas, Alison Johnson, Molly R. Schwenn, Dalsu Baris, Helena Furberg, Dean F. Bajorin, Olivier Cussenot, Geraldine Cancel-Tassin, Simone Benhamou, Peter Kraft, Stefano Porru, Angela Carta, Timothy Bishop, Melissa C. Southey, Giuseppe Matullo, Tony Fletcher, Rajiv Kumar, Jack A. Taylor, Philippe Lamy, Frederik Prip, Mark Kalisz, Stephanie J. Weinstein, Jan G. Hengstler, Silvia Selinski, Mark Harland, Mark Teo, Anne E. Kiltie, Adonina Tardón, Consol Serra, Alfredo Carrato, Reina García-Closas, Josep Lloreta, Alan Schned, Petra Lenz, Elio Riboli, Paul Brennan, Anne Tjønneland, Thomas Otto, Daniel Ovsiannikov, Frank Volkert, Sita H. Vermeulen, Katja K. Aben, Tessel E. Galesloot, Constance Turman, Immaculata De Vivo, Edward Giovannucci, David J. Hunter, Chancellor Hohensee, Rebecca Hunt, Alpa V. Patel, Wen-Yi Huang, Gudmar Thorleifsson, Manuela Gago-Dominguez, Pilar Amiano, Klaus Golka, Mariana C. Stern, Wusheng Yan, Jia Liu, Shengchao Alfred Li, Shilpa Katta, Amy Hutchinson, Belynda Hicks, William A. Wheeler, Mark P. Purdue, Katherine A. McGlynn, Cari M. Kitahara, Christopher A. Haiman, Mark H. Greene, Thorunn Rafnar, Nilanjan Chatterjee, Stephen J. Chanock, Xifeng Wu, Francisco X. Real, Debra T. Silverman, Montserrat Garcia-Closas, Kari Stefansson, Ludmila Prokunina-Olsson, Núria Malats, and Nathaniel Rothman
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Genome-Wide Association Study (GWAS) ,Germline genetics ,All institutes and research themes of the Radboud University Medical Center ,Urology ,Urological cancers Radboud Institute for Health Sciences [Radboudumc 15] ,Bladder cancer ,Gene-environment interaction - Abstract
Contains fulltext : 293880.pdf (Publisher’s version ) (Closed access) BACKGROUND: Genomic regions identified by genome-wide association studies (GWAS) for bladder cancer risk provide new insights into etiology. OBJECTIVE: To identify new susceptibility variants for bladder cancer in a meta-analysis of new and existing genome-wide genotype data. DESIGN, SETTING, AND PARTICIPANTS: Data from 32 studies that includes 13,790 bladder cancer cases and 343,502 controls of European ancestry were used for meta-analysis. OUTCOME MEASUREMENTS AND STATISTICAL ANALYSES: Log-additive associations of genetic variants were assessed using logistic regression models. A fixed-effects model was used for meta-analysis of the results. Stratified analyses were conducted to evaluate effect modification by sex and smoking status. A polygenic risk score (PRS) was generated on the basis of known and novel susceptibility variants and tested for interaction with smoking. RESULTS AND LIMITATIONS: Multiple novel bladder cancer susceptibility loci (6p.22.3, 7q36.3, 8q21.13, 9p21.3, 10q22.1, 19q13.33) as well as improved signals in three known regions (4p16.3, 5p15.33, 11p15.5) were identified, bringing the number of independent markers at genome-wide significance (p
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- 2023
69. SPTAN1, APC, and FGFR3 Mutation Status and APOBEC Mutation Signatures are Predictive of Mitomycin C Response in Non-muscle-invasive Bladder Cancer
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Benedicte Parm Ulhøi, Emil Christensen, Maria Skydt Lindgren, Lars Dyrskjøt, Sia Viborg Lindskrog, Iver Nordentoft, Karin Birkenkamp-Demtröder, Jørgen Bjerggaard Jensen, and Philippe Lamy
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Oncology ,medicine.medical_specialty ,Urology ,Context (language use) ,Chemoablation ,law.invention ,Non–muscle-invasive bladder cancer ,Randomized controlled trial ,Predictive biomarkers ,law ,Internal medicine ,Mitomycin C ,medicine ,Intravesical instillations ,Biomarker discovery ,Adverse effect ,RC254-282 ,Chemoresection ,Bladder cancer ,business.industry ,Neoplasms. Tumors. Oncology. Including cancer and carcinogens ,medicine.disease ,Diseases of the genitourinary system. Urology ,Exact test ,Cohort ,Urothelial carcinoma ,RC870-923 ,business ,Biomarkers - Abstract
Take Home Message Four promising biomarkers were found to be predictive for intravesical mitomycin C in non–muscle-invasive bladder cancer patients. Prospective validation is needed., Background Currently, no biomarkers of response to mitomycin C have been identified in non–muscle-invasive bladder cancer patients. Predictive biomarkers could improve the treatment outcome and eliminate adverse events from unnecessary treatment. Objective To identify and validate predictive biomarkers of chemoresection with mitomycin C. Design, setting, and participants The intervention group of a randomised controlled trial was identified for analyses. The study was conducted between January 2018 and June 2019 in two major urological departments in Denmark. Patients had a history of Ta low-grade/high-grade disease and were included upon recurrence. The intervention group (58 patients) received chemoresection with mitomycin C. Tumour and reference germline DNA from prior tumours were analysed by whole exome sequencing. Predictive biomarkers were validated in the context of Ta low-grade tumours from the UROMOL study. Outcome measurements and statistical analysis Response to chemotherapy (intervention group from the randomised controlled trial) and recurrence-free survival (UROMOL cohort) were measured. Groups were compared using Fisher’s exact test and Wilcoxon rank sum test. Results and limitations Chemoresponse was associated with the mutation status of SPTAN1, APC, and FGFR3, and the level of APOBEC signature contribution (p = 0.035, p = 0.034, p = 0.055, and p = 0.035, respectively). The main limitations include no biopsy for biomarker discovery immediately prior to chemoresection and the unmatched validation cohort. Conclusions Mutation status of APC, SPTAN1, and FGFR3 and the level of mutational contribution from APOBEC-related signatures were identified as potential predictive biomarkers for chemoresection with mitomycin C in non–muscle-invasive bladder cancer patients. A prospective validation study is however needed. Patient summary We investigated DNA from noninvasive bladder tumours in order to predict treatment response to chemotherapy. Four biomarkers showed promising results, which should be tested in future studies.
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- 2021
70. Single nucleus and spatially resolved intra-tumor subtype heterogeneity in bladder cancer
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Sia V. Lindskrog, Sofie S. Schmøkel, Iver Nordentoft, Philippe Lamy, Michael Knudsen, Frederik Prip, Trine Strandgaard, Jørgen Bjerggaard Jensen, and Lars Dyrskjøt
- Abstract
SummaryCurrent transcriptomic classification systems for bladder cancer do not consider the level of intra-tumor subtype heterogeneity. Here we present an investigation of the extent and possible clinical impact of intra-tumor heterogeneity across early and more advanced disease stages of bladder cancer. We performed single nucleus RNA-sequencing of 48 bladder tumors and four of these tumors were additionally analyzed using spatial transcriptomics. Total bulk RNA-sequencing and spatial proteomics data were available from the same tumors for comparison, along with detailed clinical follow-up of the patients. We demonstrate that tumors display varying levels of intra-tumor subtype heterogeneity and show that a higher class 2a weight estimated from bulk RNA-sequencing data is associated with worse outcome in patients with molecular high-risk class 2a tumors. Our results indicate that discrete subtype assignments from bulk RNA-sequencing data may lack biological granularity and continuous class scores could improve clinical risk stratification of patients.HighlightsSingle nucleus RNA-sequencing of tumors from 48 bladder cancer patients.Tumors display varying levels of intra-tumor subtype heterogeneity at single nucleus and bulk tumor level.The level of subtype heterogeneity could be estimated from both single nucleus and bulk RNA-sequencing data with a high concordance between the two.High class 2a weight estimated from bulk RNA-sequencing data is associated with worse outcome in patients with molecular high-risk class 2a tumors.
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- 2022
71. Cell-free urine- and plasma DNA mutational analysis predicts neoadjuvant chemotherapy response and outcome in patients with muscle invasive bladder cancer
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Emil Christensen, Iver Nordentoft, Sara K. Elbæk, Karin Birkenkamp-Demtröder, Ann Taber, Tine G. Andreasen, Trine Strandgaard, Michael Knudsen, Philippe Lamy, Mads Agerbæk, Jørgen B. Jensen, and Lars Dyrskjøt
- Abstract
PurposeInvestigate and compare the use of plasma- and urine DNA mutation analysis for predicting neoadjuvant chemotherapy (NAC) response and long-term oncological outcome in patients with muscle invasive bladder cancer.Experimental DesignWhole exome sequencing of tumor and germline DNA was performed for 92 patients treated with NAC followed by radical cystectomy (RC). A custom NGS panel capturing approx. 50 mutations per patient was designed and utilized to track tumor-derived DNA (tdDNA) in liquid biopsies. A total of 447 plasma samples, 281 urine supernatants and 123 urine pellets collected before, during and after treatment were analyzed. Patients were enrolled from 2013-2019 with a median follow-up time of 41.3 months after RC.ResultsWe identified tdDNA before initiation of NAC in 89% of urine supernatants, 85% of urine pellets and 43% of plasma samples. tdDNA levels were higher in urine supernatants and urine pellets compared to plasma samples (pp=0.006,p=0.002). A combined measure from plasma and urine supernatant tdDNA dynamics stratified patients by outcome (p=0.003).ConclusionsAnalysis of tdDNA in plasma and urine samples both separately and combined has potential to predict treatment response and outcome.
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- 2022
72. The State of the White-Light Corona over the Minimum and Ascending Phases of Solar Cycle 25 – Comparison with Past Cycles
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Philippe Lamy and Hugo Gilardy
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Space and Planetary Science ,Astronomy and Astrophysics - Published
- 2022
73. Validation of the Alfvén Wave Solar Atmosphere Model (AWSoM) with Observations from the Low Corona to 1 au
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Nishtha Sachdeva, Bart van der Holst, Ward B. Manchester, Gabor Tóth, Yuxi Chen, Diego G. Lloveras, Alberto M. Vásquez, Philippe Lamy, Julien Wojak, Bernard V. Jackson, Hsiu-Shan Yu, and Carl J. Henney
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- 2019
- Full Text
- View/download PDF
74. Polarimetric Studies of a Fast Coronal Mass Ejection
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Marilena Mierla, Bernd Inhester, Andrei N. Zhukov, Sergei V. Shestov, Alessandro Bemporad, Philippe Lamy, and Serge Koutchmy
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Astrophysics - Solar and Stellar Astrophysics ,Space and Planetary Science ,FOS: Physical sciences ,Astronomy and Astrophysics ,Solar and Stellar Astrophysics (astro-ph.SR) - Abstract
In this work we performed a polarimetric study of a fast and wide coronal mass ejection (CME) observed on 12 July 2012 by the COR1 and COR2 instruments onboard the Solar TErrestrial RElations Observatory (STEREO) mission. The CME source region was an X1.4 flare located at approximately S15W01 on the solar disk, as observed from the Earth's perspective. The position of the CME as derived from the 3D Graduated Cylindrical Shell (GCS) reconstruction method was at around S18W00 at 2.5 solar radii and S07W00 at 5.7 solar radii, meaning that the CME was deflected towards the Equator while propagating outward in the corona. The projected speed of the leading edge of the CME also evolved from around 200 km s−1 in the lower corona to around 1000 km s−1 in the COR2 field of view. The degree of polarisation of the CME is around 65% but it can go as high as 80% in some CME regions. The CME showed deviation of the polarisation angle from the tangential in the range of 10 - 15∘ (or more). Our analysis showed that this is mostly due to the fact that the sequence of three polarised images from where the polarised parameters are derived is not taken simultaneously, but at a difference of a few seconds in time. In this interval of time, the CME moves by at least two pixels in the FOV of the instruments and this displacement results in uncertainties in the polarisation parameters (degree of polarisation, polarisation angle, etc.). We propose some steps forward to improve the derivation of the polarisation. This study is important for analysing the future data from instruments with polarisation capabilities.
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- 2022
75. Targeting natural splicing plasticity of APOBEC3B restricts its expression and mutagenic activity
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Krista A. Delviks-Frankenberry, Olusegun O. Onabajo, Seraph Han-Yin Lin, Vinay K. Pathak, Ariunaa Bayanjargal, Oscar Florez-Vargas, Joselin M. Vargas, Clara Zettelmeyer, Philippe Lamy, Lars Dyrskjøt, A. Rouf Banday, Adeola Obajemu, and Ludmila Prokunina-Olsson
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0301 basic medicine ,Gene isoform ,Spliceosome ,endocrine system ,RNA splicing ,QH301-705.5 ,Medicine (miscellaneous) ,Mutagenesis (molecular biology technique) ,General Biochemistry, Genetics and Molecular Biology ,Article ,Minor Histocompatibility Antigens ,03 medical and health sciences ,Exon ,0302 clinical medicine ,Cytidine Deaminase ,Biomarkers, Tumor ,Humans ,APOBEC3A ,Biology (General) ,Chemistry ,Alternative splicing ,Bladder cancer ,Intron ,food and beverages ,Proteins ,Exons ,Hep G2 Cells ,Phosphoproteins ,Gene expression profiling ,Progression-Free Survival ,Cell biology ,Gene Expression Regulation, Neoplastic ,Isoenzymes ,Alternative Splicing ,030104 developmental biology ,HEK293 Cells ,Urinary Bladder Neoplasms ,Mutagenesis ,030220 oncology & carcinogenesis ,Epoxy Compounds ,Macrolides ,RNA Splicing Factors ,General Agricultural and Biological Sciences ,HeLa Cells - Abstract
APOBEC3A (A3A) and APOBEC3B (A3B) enzymes drive APOBEC-mediated mutagenesis. Identification of factors affecting the activity of these enzymes could help modulate mutagenesis and associated clinical outcomes. Here, we show that canonical and alternatively spliced A3A and A3B isoforms produce corresponding mutagenic and non-mutagenic enzymes. Increased expression of the mutagenic A3B isoform predicted shorter progression-free survival in bladder cancer. We demonstrate that the production of mutagenic vs. non-mutagenic A3B protein isoforms was considerably affected by inclusion/skipping of exon 5 in A3B. Furthermore, exon 5 skipping, resulting in lower levels of mutagenic A3B enzyme, could be increased in vitro. Specifically, we showed the effects of treatment with an SF3B1 inhibitor affecting spliceosome interaction with a branch point site in intron 4, or with splice-switching oligonucleotides targeting exon 5 of A3B. Our results underscore the clinical role of A3B and implicate alternative splicing of A3B as a mechanism that could be targeted to restrict APOBEC-mediated mutagenesis., A. Rouf Banday et al. report targeting alternative splicing of APOBEC3B as a strategy to modulate APOBEC-mediated mutagenesis in cancers. Higher expression of the mutagenic APOBEC3B isoform predicted shorter progression-free survival in bladder cancer patients. Expression of this mutagenic isoform could be decreased by inducing skipping of APOBEC3B exon 5 in cells treated with SF3B1 inhibitor or splice-switching oligos.
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- 2021
76. Abstract 5600: Utility of circulating tumor DNA and transcriptomic profiling in predicting outcome in muscle invasive bladder cancer patients
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Sia Viborg Lindskrog, George Laliotis, Karin Birkenkamp-Demtröder, Iver Nordentoft, Philippe Lamy, Elshaddai Z. White, Natalia Pajak, Tine G. Andreasen, Punashi Dutta, Meenakshi Malhotra, Shruti Sharma, Mark Calhoun, Adam ElNaggar, Minetta C. Liu, Mads Agerbæk, Jørgen B. Jensen, and Lars Dyrskjøt
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Cancer Research ,Oncology - Abstract
Background: Standard treatment of localized muscle invasive bladder cancer (MIBC) is neoadjuvant chemotherapy (NAC) followed by radical cystectomy (RC); however, only 40-50% respond to NAC and approx. 50% experience relapse. Evaluation of treatment efficacy and early detection of relapse are therefore major clinical challenges. Methods: We present a clinical update of a previously described cohort of 68 patients who received NAC prior to RC (NAC cohort; Christensen et al. JCO 2019; median follow-up (FU) of 58 months) together with evaluation of a retrospectively collected cohort of 120 patients who did not receive NAC (no-NAC cohort; median FU of 71 months). Circulating tumor DNA (ctDNA) was analyzed before NAC (NAC cohort, n=63), prior to RC (NAC cohort, n=67; no-NAC cohort, n=115) and after RC (NAC cohort, n=66; no-NAC cohort, n=37) using Signatera™. RNA-seq was performed on 176 tumors. Results: Updated clinical FU for the NAC cohort showed that ctDNA-positive patients had significantly worse recurrence-free survival (RFS) compared to ctDNA-negative patients (before NAC: HR=16, 95%CI=3.6-70.5, p=0.0002; during surveillance after RC: HR=27.6, 95%CI=7.9-96.9, p Conclusion: Presence of ctDNA was associated with worse prognosis for both NAC and no-NAC treated patients. Transcriptomic analysis of primary tumors showed that anti-tumor immune responses may be associated with a particularly good outcome whereas EMT may be promoting more aggressive disease. Citation Format: Sia Viborg Lindskrog, George Laliotis, Karin Birkenkamp-Demtröder, Iver Nordentoft, Philippe Lamy, Elshaddai Z. White, Natalia Pajak, Tine G. Andreasen, Punashi Dutta, Meenakshi Malhotra, Shruti Sharma, Mark Calhoun, Adam ElNaggar, Minetta C. Liu, Mads Agerbæk, Jørgen B. Jensen, Lars Dyrskjøt. Utility of circulating tumor DNA and transcriptomic profiling in predicting outcome in muscle invasive bladder cancer patients. [abstract]. In: Proceedings of the American Association for Cancer Research Annual Meeting 2023; Part 1 (Regular and Invited Abstracts); 2023 Apr 14-19; Orlando, FL. Philadelphia (PA): AACR; Cancer Res 2023;83(7_Suppl):Abstract nr 5600.
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- 2023
77. Abstract 6075: Comprehensive genomic characterization of early-stage bladder cancer from 438 patients by whole genome- and exome sequencing
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Frederik Prip, Philippe Lamy, Iver Nordentoft, Sia Viborg Lindskrog, Trine Strandgaard, Karin Birkenkamp-Demtröder, Gregers G. Hermann, Astrid C. Petersen, Veronika Bahlinger, Marc-Oliver Grimm, Marcus Horstmann, Karin Mogensen, Roman Nawroth, Ulrika Segersten, Danijel Sikic, Kim E. M van Kessel, Tobias Maurer, Tatjana Simic, Arndt Hartmann, Ellen C. C. Zwarthoff, Per-Uno Malmström, Torben Steiniche, Jørgen Bjerggaard Jensen, Núria Malats, Francisco X. Real, and Lars Dyrskjøt
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Cancer Research ,Oncology - Abstract
Background: The genomic landscape of cancer is complex and includes mutations and copy number alterations (CNAs) that affect several cancer related pathways and drive tumor evolution. Non-muscle-invasive bladder cancers (NMIBC) are largely orphan for integrative genomic studies. Large studies are needed to delineate the genomic complexity and heterogeneity of NMIBC. Methods: A total of 438 patients with NMIBC were analyzed, 296 of which were part of the UROMOL cohort (PMID: 27321955). The median follow-up was 5 years. The progression rate was 13% (n= 56). Whole exome sequencing (WES) was performed on DNA from tumor (~150x) and matched germline samples to call somatic mutations. Additionally, shallow whole genome sequencing (sWGS; ~2x) was performed on DNA from 362 of the tumors to quantify CNAs. RNA-sequencing was available for 414 of the samples, and tumors were classified according to the UROMOL2021 transcriptomic classes. We identified significantly mutated genes by mutsigCV and significantly amplified or deleted regions by GISTIC2. Results: The median tumor mutation burden (TMB) was 3.7/Mb. TMB was not associated with progression (p=0.28). A total of 61 genes were significantly mutated in the cohort, the most frequent being FGFR3 (61%), KDM6A (44%) and KMT2D (38%). Mutations in EP300 and RHOB were significantly associated with an increased risk of progression after adjusting for grade and stage (p=0.040 and 0.044, respectively). Several mutations showed a strong transcriptomic class dependent occurrence: mutations in RB1, TP53, ERCC2 and ERBB2 were enriched in the aggressive class 2a, FGFR3 and STAG2 in class 1 and class 3, and KMT2C and KMT2D in class 3. Genome doubling was identified in 15% of the tumors. These tumors were enriched in the aggressive classes 2a and 2b and were associated with increased risk of progression (p=0.0049). In addition, we observed several significantly altered genomic regions, the most significant being deletions in 9p21.3 (CDKN2A & CDKN2B, 64%), 2q37.1 (GIGYF2 & EIF4E2, 28%) and amplification in 11q13.3 (CCND1, 9%). Class 2a tumors were enriched for genomic alterations in most of the significant regions. 9p21.3 was the only region with frequent homozygous losses (22%). High-level gains were prognostic of progression, independently of ploidy, stage and grade, for several regions, including 4p16.3 (FGFR3, p=0.00013), 17q23.2(TBX2, p=0.0004) and 8p11.23(ZNF703, p=0.011). In addition, we observed an enrichment of uniparental disomy in 4p16.3 (FGFR3, 8%). Conclusion: Here we investigated the landscape of DNA alterations in NMIBC in a large patient cohort of NMIBC samples with paired transcriptomic data and detailed clinical follow-up. We identified several novel genomic alterations; specifically, we showed that 15% of the tumors had genome doublings, and we identified a complex underlying copy number landscape of the region containing FGFR3. Citation Format: Frederik Prip, Philippe Lamy, Iver Nordentoft, Sia Viborg Lindskrog, Trine Strandgaard, Karin Birkenkamp-Demtröder, Gregers G. Hermann, Astrid C. Petersen, Veronika Bahlinger, Marc-Oliver Grimm, Marcus Horstmann, Karin Mogensen, Roman Nawroth, Ulrika Segersten, Danijel Sikic, Kim E. M van Kessel, Tobias Maurer, Tatjana Simic, Arndt Hartmann, Ellen C. C. Zwarthoff, Per-Uno Malmström, Torben Steiniche, Jørgen Bjerggaard Jensen, Núria Malats, Francisco X. Real, Lars Dyrskjøt. Comprehensive genomic characterization of early-stage bladder cancer from 438 patients by whole genome- and exome sequencing. [abstract]. In: Proceedings of the American Association for Cancer Research Annual Meeting 2023; Part 1 (Regular and Invited Abstracts); 2023 Apr 14-19; Orlando, FL. Philadelphia (PA): AACR; Cancer Res 2023;83(7_Suppl):Abstract nr 6075.
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- 2023
78. Coronal Fine Linear Rays: Are They Fast Streams From Active Regions?
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Serge Koutchmy, Philippe Lamy, Christian Viladrich, Boris Filippov, Arthur Nikoghossian, Leon Golub, M. Maksimovic, K. Issautier, N. Meyer-Vernet, M. Moncuquet, F. Pantellini, 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), Laboratoire d'Astrophysique de Marseille (LAM), and 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)
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Astrophysics::High Energy Astrophysical Phenomena ,Jets outflows and bipolar flows ,Coronal hole ,solar magnetism ,Astrophysics ,96.60.Vg ,Coronal mass ejection ,Astrophysics::Solar and Stellar Astrophysics ,Eclipse ,Physics ,solar corona ,Astronomy ,Particle emission solar wind ,96.60.Hv ,Coronal loop ,Electric and magnetic fields solar magnetism ,Helmet streamer ,Corona ,Nanoflares ,Solar wind ,astrophysical jets ,solar wind ,[SDU]Sciences of the Universe [physics] ,Physics::Space Physics ,98.58.Fd ,96.60.P - Abstract
International audience; Eclipse observations of the W-L corona show linear rays above active regions at times of solar maximum. We show that these linear rays are also observed in the field-of-view of the C2-LASCO coronagraph, in perfect correspondence with the eclipse results. A selected prominent case taken from the 2001 eclipse observation in Angola is analysed with several different methods, including the use of a synoptic map constructed using SoHO/LASCO C2 images. A clear signature of time variations near the eclipse observation is detected, suggesting that at least some parts of the beam are collimated. These observations strongly suggest high speed streams that apparently ignore the potential large scale coronal magnetic field rooted rather low in the corona. A possible origin is the neutral magnetic points located above the active region. Several mechanisms exist to explain how the plasma is accelerated in these regions to large quasi-relativistic velocities, possibly related to the occurrence of type III radio bursts. We point out a curious analogy with phenomena occurring inside coronal holes.
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- 2022
79. Elevated T-cell exhaustion and urinary tumor DNA levels are associated with BCG failure in patients with non-muscle invasive bladder cancer
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Trine Strandgaard, Sia Viborg Lindskrog, Iver Nordentoft, Emil Christensen, Karin Birkenkamp-Demtröder, Tine Ginnerup Andreasen, Philippe Lamy, Asbjørn Kjær, Daniel Ranti, Yuan-Sho Wang, Christine Bieber, Frederik Prip, Julie Rasmussen, Torben Steiniche, Nicolai Birkbak, John Sfakianos, Amir Horowitz, Jørgen Bjerggaard Jensen, and Lars Dyrskjøt
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complex mixtures - Abstract
BackgroundThe functional status of immune cells within the tumor microenvironment and tumor characteristics may explain Bacillus Calmette-Guérin (BCG)-failure in high-risk non-muscle invasive bladder cancer (NMIBC).ObjectiveTo characterize molecular correlates of BCG-failure using a multiomics approach.Design, Setting, and ParticipantsBCG-treated NMIBC patients (n=156) were included. Metachronous tumors were analyzed using RNA-sequencing (n=170) and whole exome sequencing (n=198). Urine samples were analyzed for immune-oncology related proteins (n=190), and tumor-derived DNA (tdDNA; n=192).Outcome Measurement and Statistical AnalysisPrimary endpoint was BCG-failure. Cox regression, Wilcoxon Rank Sum test, t-test or Fisher’s exact test were used.Results and LimitationsBCG caused activation of the immune system regardless of clinical response; however, immune-inhibitory proteins were observed in the urine of BCG-unresponsive patients post-treatment (CD70, PD1, CD5). BCG-failure was associated with post-BCG T-cell exhaustion (p=0.0021). Pre-BCG tumors from patients with post-BCG T-cell exhaustion were characterized by high expression of cell division and immune-related genes. A high post-BCG exhaustion prediction score in pre-BCG tumors was associated with worse post-BCG high-grade recurrence free survival (HGRFS), reflecting BCG-failure (p=0.0084). Pre-BCG tumors of class 2a and 2b were likewise associated with worse post-BCG HGRFS(p=0.0023). Post-BCG exhaustion was observed in patients with high pre-BCG neoantigen load (p=0.023) and mutations in MUC4 (p=0.0007). Finally, absence of post-BCG tdDNA clearance identified patients at high risk of recurrence (p=0.028). The retrospective design, lack of maintenance BCG, and partial overlap in analyses are limitations to the study.ConclusionsBCG failure may be caused by T-cell exhaustion. Tumor subtype and Pre-BCG tumor characteristics may identify patients at high risk of BCG-failure prior to treatment. Urinary measurements have the potential to be used as a real-time assessment of treatment response.Patient SummaryA dysfunctional immune response to BCG therapy may explain lack of response to the treatment.
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- 2022
80. Molecular correlates of cisplatin-based chemotherapy response in muscle invasive bladder cancer by integrated multi-omics analysis
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Jørgen Bjerggaard Jensen, Frederik Prip, Emil Christensen, Michael Knudsen, Philippe Lamy, Trine Line Hauge Okholm, Ann Taber, Torben Steiniche, Jakob Skou Pedersen, Sia Viborg Lindskrog, Karin Birkenkamp-Demtröder, Iver Nordentoft, Lars Dyrskjøt, and Mads Agerbæk
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0301 basic medicine ,Genome instability ,Oncology ,Cisplatin/pharmacology ,Molecular biology ,CYSTECTOMY ,medicine.medical_treatment ,Programmed Cell Death 1 Receptor ,General Physics and Astronomy ,Proteomics ,Transcriptome ,NEOADJUVANT CHEMOTHERAPY ,0302 clinical medicine ,lcsh:Science ,Neoadjuvant therapy ,Cancer ,Epigenomics ,Multidisciplinary ,Molecular medicine ,Urinary Bladder Neoplasms/drug therapy ,GEMCITABINE PLUS CISPLATIN ,ASSOCIATION ,CLONAL EVOLUTION ,BRCA2 Protein/genetics ,Neoadjuvant Therapy ,Gene Expression Regulation, Neoplastic ,Chemotherapy, Adjuvant ,030220 oncology & carcinogenesis ,DNA methylation ,Allelic Imbalance ,SURVIVAL ,SENSITIVITY ,medicine.drug ,medicine.medical_specialty ,CARCINOMA ,Urology ,Science ,SOMATIC ERCC2 MUTATIONS ,Genomics ,Context (language use) ,Article ,General Biochemistry, Genetics and Molecular Biology ,Genomic Instability ,03 medical and health sciences ,Medical research ,Drug Therapy ,Programmed Cell Death 1 Receptor/genetics ,Internal medicine ,medicine ,Biomarkers, Tumor ,Humans ,SIGNATURES ,Cisplatin ,BRCA2 Protein ,Bladder cancer ,business.industry ,General Chemistry ,DNA Methylation ,medicine.disease ,030104 developmental biology ,Urinary Bladder Neoplasms ,Gene Expression Regulation, Neoplastic/drug effects ,Mutation ,lcsh:Q ,business ,Biomarkers - Abstract
Overtreatment with cisplatin-based chemotherapy is a major issue in the management of muscle-invasive bladder cancer (MIBC), and currently none of the reported biomarkers for predicting response have been implemented in the clinic. Here we perform a comprehensive multi-omics analysis (genomics, transcriptomics, epigenomics and proteomics) of 300 MIBC patients treated with chemotherapy (neoadjuvant or first-line) to identify molecular changes associated with treatment response. DNA-based associations with response converge on genomic instability driven by a high number of chromosomal alterations, indels, signature 5 mutations and/or BRCA2 mutations. Expression data identifies the basal/squamous gene expression subtype to be associated with poor response. Immune cell infiltration and high PD-1 protein expression are associated with treatment response. Through integration of genomic and transcriptomic data, we demonstrate patient stratification to groups of low and high likelihood of cisplatin-based response. This could pave the way for future patient selection following validation in prospective clinical trials., There are currently only a few biomarkers to predict the response of muscle invasive bladder cancer to therapy. Here, the authors analyse 300 tumors using exome and RNA sequencing and find that tumors with a high degree of genomic instability and a non-basal/squamous gene expression subtype are most likely to respond to treatment.
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- 2020
81. Quelle(s) cartographie(s) pour la ville ? Expériences lyonnaises
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Philippe Lamy and Anne Pariente
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- 2022
82. Linking Small-scale Solar Wind Properties with Large-scale Coronal Source Regions through Joint Parker Solar Probe–Metis/Solar Orbiter Observations
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Daniele Telloni, Gary P. Zank, Luca Sorriso-Valvo, Raffaella D’Amicis, Olga Panasenco, Roberto Susino, Roberto Bruno, Denise Perrone, Laxman Adhikari, Haoming Liang, Masaru Nakanotani, Lingling Zhao, Lina Z. Hadid, Beatriz Sánchez-Cano, Daniel Verscharen, Marco Velli, Catia Grimani, Raffaele Marino, Francesco Carbone, Salvatore Mancuso, Ruggero Biondo, Paolo Pagano, Fabio Reale, Stuart D. Bale, Justin C. Kasper, Anthony W. Case, Thierry Dudok de Wit, Keith Goetz, Peter R. Harvey, Kelly E. Korreck, Davin Larson, Roberto Livi, Robert J. MacDowall, David M. Malaspina, Marc Pulupa, Michael L. Stevens, Phyllis Whittlesey, Marco Romoli, Vincenzo Andretta, Vania Da Deppo, Silvano Fineschi, Petr Heinzel, John D. Moses, Giampiero Naletto, Gianalfredo Nicolini, Daniele Spadaro, Marco Stangalini, Luca Teriaca, Gerardo Capobianco, Giuseppe E. Capuano, Chiara Casini, Marta Casti, Paolo Chioetto, Alain J. Corso, Yara De Leo, Michele Fabi, Federica Frassati, Fabio Frassetto, Silvio Giordano, Salvo L. Guglielmino, Giovanna Jerse, Federico Landini, Alessandro Liberatore, Enrico Magli, Giuseppe Massone, Mauro Messerotti, Maurizio Pancrazzi, Maria G. Pelizzo, Paolo Romano, Clementina Sasso, Udo Schühle, Alessandra Slemer, Thomas Straus, Michela Uslenghi, Cosimo A. Volpicelli, Luca Zangrilli, Paola Zuppella, Lucia Abbo, Frédéric Auchère, Regina Aznar Cuadrado, Arkadiusz Berlicki, Angela Ciaravella, Philippe Lamy, Alessandro Lanzafame, Marco Malvezzi, Piergiorgio Nicolosi, Giuseppe Nisticò, Hardi Peter, Sami K. Solanki, Leonard Strachan, Kanaris Tsinganos, Rita Ventura, Jean-Claude Vial, Joachim Woch, Gaetano Zimbardo, Telloni D., Zank G.P., Sorriso-Valvo L., D'amicis R., Panasenco O., Susino R., Bruno R., Perrone D., Adhikari L., Liang H., Nakanotani M., Zhao L., Hadid L.Z., Sanchez-Cano B., Verscharen D., Velli M., Grimani C., Marino R., Carbone F., Mancuso S., Biondo R., Pagano P., Reale F., Bale S.D., Kasper J.C., Case A.W., De Wit T.D., Goetz K., Harvey P.R., Korreck K.E., Larson D., Livi R., Macdowall R.J., Malaspina D.M., Pulupa M., Stevens M.L., Whittlesey P., Romoli M., Andretta V., Deppo V.D., Fineschi S., Heinzel P., Moses J.D., Naletto G., Nicolini G., Spadaro D., Stangalini M., Teriaca L., Capobianco G., Capuano G.E., Casini C., Casti M., Chioetto P., Corso A.J., Leo Y.D., Fabi M., Frassati F., Frassetto F., Giordano S., Guglielmino S.L., Jerse G., Landini F., Liberatore A., Magli E., Massone G., Messerotti M., Pancrazzi M., Pelizzo M.G., Romano P., Sasso C., Schuhle U., Slemer A., Straus T., Uslenghi M., Volpicelli C.A., Zangrilli L., Zuppella P., Abbo L., Auchere F., Cuadrado R.A., Berlicki A., Ciaravella A., Lamy P., Lanzafame A., Malvezzi M., Nicolosi P., Nistico G., Peter H., Solanki S.K., Strachan L., Tsinganos K., Ventura R., Vial J.-C., Woch J., and Zimbardo G.
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Magnetohydrodynamics (694) ,Settore FIS/05 - Astronomia E Astrofisica ,Astronomi, astrofysik och kosmologi ,Space and Planetary Science ,Solar corona (1483) ,Space plasmas (1544) ,Solar wind (1534) ,Interplanetary turbulence (830) ,Astronomy, Astrophysics and Cosmology ,Astronomy and Astrophysics ,Alfven waves (23) ,Heliosphere (711) - Abstract
The solar wind measured in situ by Parker Solar Probe in the very inner heliosphere is studied in combination with the remote-sensing observation of the coronal source region provided by the METIS coronagraph aboard Solar Orbiter. The coronal outflows observed near the ecliptic by Metis on 2021 January 17 at 16:30 UT, between 3.5 and 6.3 R ⊙ above the eastern solar limb, can be associated with the streams sampled by PSP at 0.11 and 0.26 au from the Sun, in two time intervals almost 5 days apart. The two plasma flows come from two distinct source regions, characterized by different magnetic field polarity and intensity at the coronal base. It follows that both the global and local properties of the two streams are different. Specifically, the solar wind emanating from the stronger magnetic field region has a lower bulk flux density, as expected, and is in a state of well-developed Alfvénic turbulence, with low intermittency. This is interpreted in terms of slab turbulence in the context of nearly incompressible magnetohydrodynamics. Conversely, the highly intermittent and poorly developed turbulent behavior of the solar wind from the weaker magnetic field region is presumably due to large magnetic deflections most likely attributed to the presence of switchbacks of interchange reconnection origin.
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- 2022
83. Genome-wide Meta-analysis Identifies Novel Genes Associated with Recurrence and Progression in Non-muscle-invasive Bladder Cancer
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Núria Malats, Richard T. Bryan, Philippe Lamy, Lambertus A. Kiemeney, Tessel E. Galesloot, Kar Keung Cheng, Dimitar Kolev, Sita H. Vermeulen, Neil Fleshner, Anne J. Grotenhuis, Lourdes Mengual, Katja K.H. Aben, Nicholas D. James, Samantha Conroy, Maurice P. Zeegers, Gerald W. Verhaegh, James W.F. Catto, Sia Viborg Lindskrog, Lars Dyrskjøt, Epidemiologie, RS: NUTRIM - R3 - Respiratory & Age-related Health, RS: CAPHRI - R5 - Optimising Patient Care, and Complexe Genetica
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Oncology ,Male ,medicine.medical_specialty ,Candidate gene ,Genome-wide association study ,PROGNOSIS ,Hydrolases ,Urology ,Non-muscle-invasive bladder cancer ,Vascular damage Radboud Institute for Health Sciences [Radboudumc 16] ,Single-nucleotide polymorphism ,Locus (genetics) ,Recurrence ,Internal medicine ,Urological cancers Radboud Institute for Molecular Life Sciences [Radboudumc 15] ,medicine ,SNP ,Humans ,Radiology, Nuclear Medicine and imaging ,SASH1 ,Retrospective Studies ,SLY1 ,Progression ,Proportional hazards model ,business.industry ,Hazard ratio ,Meta-analysis ,Urinary Bladder Neoplasms ,Urological cancers Radboud Institute for Health Sciences [Radboudumc 15] ,Expression quantitative trait loci ,Surgery ,Female ,Neoplasm Recurrence, Local ,business - Abstract
Background: Non-muscle-invasive bladder cancer (NMIBC) is characterized by frequent recurrences and a risk of progression in stage and grade. Increased knowledge of underlying biological mechanisms is needed.Objective: To identify single nucleotide polymorphisms (SNPs) associated with recurrence-free (RFS) and progression-free (PFS) survival in NMIBC.Design, setting, and participants: We analyzed outcome data from 3400 newly diagnosed NMIBC patients from the Netherlands, the UK, Canada, and Spain. We generated genome-wide germline SNP data using Illumina OmniExpress and Infinium Global Screening Array in combination with genotype imputation.Outcome measurements and statistical analysis: Cohort-specific genome-wide association studies (GWASs) for RFS and PFS were performed using a Cox proportional hazard model. Results were combined in a fixed-effect inverse-variance weighted meta-analysis. Candidate genes for the identified SNP associations were prioritized using functional annotation, gene-based analysis, expression quantitative trait locus analysis, and transcription factor binding site databases. Tumor expression levels of prioritized genes were tested for association with RFS and PFS in an independent NMIBC cohort.Results and limitations: This meta-analysis revealed a genome-wide significant locus for RFS on chromosome 14 (lead SNP rs12885353, hazard ratio [HR] C vs T allele 1.55, 95% confidence interval [CI] 1.33-1.82, p = 4.0 x 10(-8)), containing genes G2E3 and SCFD1. Higher expression of SCFD1 was associated with increased RFS (HR 0.70, 95% CI 0.59-0.84, p(FDR) = 0.003). Twelve other loci were suggestively associated with RFS (p < 10(-5)), pointing toward 18 additional candidate genes. For PFS, ten loci showed suggestive evidence of association, indicating 36 candidate genes. Expression levels of ten of these genes were statistically significantly associated with PFS, of which four (IFT140, UBE2I, FAHD1, and NME3) showed directional consistency with our meta-analysis results and published literature.Conclusions: In this first prognostic GWAS in NMIBC, we identified several novel candidate loci and five genes that showed convincing associations with recurrence or progression.Patient summary: In this study, we searched for inherited DNA changes that affect the outcome of non-muscle-invasive bladder cancer (NMIBC). We identified several genes that are associated with disease recurrence and progression. The roles and mechanisms of these genes in NMIBC prognosis should be investigated in future studies. (C) 2021 The Authors. Published by Elsevier B.V. on behalf of European Association of Urology.
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- 2022
84. Utility of ctDNA in predicting outcome and pathological complete response in patients with bladder cancer as a guide for selective bladder preservation strategies
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Lars Dyrskjøt, George Laliotis MD, PhD, Iver Nordentoft, Karin Birkenkamp-Demtröder, Sia Viborg Lindskrog, Philippe Lamy, Elshaddai White, Natalia Pajak, Tine Ginnerup Andreasen, Punashi Dutta, Shruti Sharma, Mark Calhoun, Adam ElNaggar, Minetta C. Liu, Mads Agerbaek, and Jørgen Bjerggaard Jensen
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Cancer Research ,Oncology - Abstract
563 Background: Muscle-invasive bladder cancer (MIBC) accounts for ~25–30% of all bladder cancer diagnoses. With neoadjuvant chemotherapy (NAC) followed by radical cystectomy (RC) as standard-of-care, the 5-year survival rate ranges from 40%–60%. Bladder-sparing protocols (BSP) have emerged as a feasible alternative to RC for MIBC treatment, however better tools are needed. In this study, we evaluated the prognostic value of circulating tumor DNA (ctDNA) in predicting recurrence in patients who achieved pathological complete response (pCR). Methods: We analyzed a previously described cohort of 68 patients (656 plasma samples; Christensen et al., JCO 2019) with MIBC who received NAC prior to cystectomy. Patients had an updated median follow-up of 58.94 months (range: 7.19-81.77) post-cystectomy. ctDNA was analyzed at baseline (before NAC; N=64), and prior to cystectomy (N=65) using a commercially available assay (Signatera, Natera, Inc.). Additionally, exploratory RNA-Seq was performed on tumors from 59 patients (samples with >5M total counts were utilized). Pathway analysis was used to compare ctDNA-positive and ctDNA-negative patients who failed to achieve pCR. Results: Of the 64 patients with ctDNA results available at baseline, 59.4% (38/64) tested ctDNA-negative, and of these 84.2% (32/38) achieved pCR. Furthermore, 40.6% (26/64) tested ctDNA-positive, and only 34.6% (9/26) achieved pCR. Likewise, prior to cystectomy, 83.9% (52/62) of patients were ctDNA-negative, and 80.7% (42/52) achieved pCR, while none of the ctDNA-positive patients achieved pCR (positive predictive value 100%; negative predictive value 80.8%). Based on both ctDNA timepoints, the probability of ctDNA-negative patients to achieve pCR was significantly higher than ctDNA-positive patients ( p
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- 2023
85. VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis
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J. Krajewski, P. Aurard, Philippe Lamy, Vishnu Reddy, Laurent Jorda, D. Molina, Josef Hanus, Josef Ďurech, P. Michel, F. Vachier, Nicolas Rambaux, J. Oey, Grzegorz Dudziński, P. Bartczak, A. Leroy, Michael Marsset, L. Dalmon, P. Beck, H. Le Coroller, Hiroko Hamanowa, Maëlle Neveu, Christophe Dumas, Hiromi Hamanowa, A. G. Sanchez, Zouhair Benkhaldoun, N. Payre, E. Podlewska-Gaca, Fabrice Cipriani, Raoul Behrend, Paolo Tanga, Aled Jones, Julie Castillo-Rogez, Miroslav Brož, P. Antonini, Tadeusz Michalowski, F. Livet, O. Labrevoir, J. M. Bosch, Emmanuel Jehin, Arthur Vigan, S. Fauvaud, A. Chapman, Marin Ferrais, Jérôme Berthier, Alexis Drouard, Mirel Birlan, J. Grice, R. Montaigut, J. His, L. Socha, Romain Fétick, Olivier Witasse, Pierre Vernazza, Thierry Fusco, Benoit Carry, F. Marchis, Doeon Kim, Toni Santana-Ros, Mikko Kaasalainen, Matti Viikinkoski, P. Sabin, M. Audejean, A. Marciniak, Myung-Jin Kim, Bin Yang, Agnieszka Kryszczyńska, François Colas, 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), Institute of Astronomy [Prague], Charles University [Prague] (CU), Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Nice, France, Department of Earth, Atmospheric and Planetary Sciences [MIT, Cambridge] (EAPS), Massachusetts Institute of Technology (MIT), Tampere University of Technology [Tampere] (TUT), Search for Extraterrestrial Intelligence Institute (SETI), Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE), 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 de Lille-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Astronomical Institute of Romanian Academy, Romanian Academy, Adam Mickiewicz University in Poznań (UAM), Institut de Recherche en Horticulture et Semences (IRHS), Université d'Angers (UA)-AGROCAMPUS OUEST, 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 National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), Université de Liège, 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)-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), California Institute of Technology (CALTECH), European Space Agency (ESA), TMT Observatory, The Open University [Milton Keynes] (OU), Department of Mathematics [Tampere], University of Maryland [College Park], University of Maryland System, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Hospices Civils de Lyon (HCL), Research on Healthcare Performance (RESHAPE - Inserm U1290 - UCBL1), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de la Santé et de la Recherche Médicale (INSERM), Universidad de Alicante, Universitat de Barcelona (UB), European Southern Observatory [Santiago] (ESO), European Southern Observatory (ESO), Observatoire de Chinon, Institut Pythéas (OSU PYTHEAS), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), Observatoire de Haute-Provence (OHP), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), Geneva Observatory, University of Geneva [Switzerland], Université Cadi Ayyad [Marrakech] (UCA), Héritages et Constructions dans le Texte et l'Image (HCTI), Institut Brestois des Sciences de l'Homme et de la Société (IBSHS), Université de Brest (UBO)-Université de Brest (UBO)-Université de Bretagne Sud (UBS)-Université de Brest (UBO), Observatoire du Bois de Bardon, Association T60, Observatoire Midi-Pyrénées, Observatoire Midi-Pyrénées (OMP), 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), Laboratory for Space Research [Hong Kong] (LSR), The University of Hong Kong (HKU), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Korea Astronomy and Space Science Institute (KASI), Okayama University, Chungbuk National University, Laboratoire d'analyse et de recherche en économie et finance internationales (Larefi), Université de Bordeaux (UB), 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), Anunaki Observatory, Sanofi-Aventis R&D, SANOFI Recherche, Planetary Science Institute [Tucson] (PSI), Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Ministerio de Economía y Competitividad (España), Belgian Science Policy Office, National Science Foundation (US), Generalitat Valenciana, Université Côte d'Azur (UCA), Université d'Angers (UA)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-INSTITUT AGRO Agrocampus Ouest, 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 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, Agence Spatiale Européenne = European Space Agency (ESA), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université de Genève = University of Geneva (UNIGE), Université de Bretagne Sud (UBS)-Université de Brest (UBO)-Institut Brestois des Sciences de l'Homme et de la Société (IBSHS), Université de Brest (UBO), 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)-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, Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Tampere University, and Computing Sciences
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asteroids ,Rotation period ,Surface (mathematics) ,Shell (structure) ,[SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] ,general [Minor planets, asteroids] ,Context (language use) ,Astrophysics ,01 natural sciences ,03 medical and health sciences ,Física Aplicada ,0103 physical sciences ,111 Mathematics ,observational [Methods] ,010303 astronomy & astrophysics ,030304 developmental biology ,Physics ,Asteroids:general ,0303 health sciences ,[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,Minor planets ,techniques: high angular resolution ,Astronomy and Astrophysics ,113 Computer and information sciences ,asteroids: general ,Bimodality ,high angular resolution [Techniques] ,Density distribution ,115 Astronomy and space science ,Space and Planetary Science ,Asteroid ,[SDU]Sciences of the Universe [physics] ,minor planets ,methods: observational ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,general [Asteroids] ,high angular resolution ,Shape analysis (digital geometry) - Abstract
Vernazza, P., et al., Until recently, the 3D shape, and therefore density (when combining the volume estimate with available mass estimates), and surface topography of the vast majority of the largest (D ≥ 100 km) main-belt asteroids have remained poorly constrained. The improved capabilities of the SPHERE/ZIMPOL instrument have opened new doors into ground-based asteroid exploration. Aims. To constrain the formation and evolution of a representative sample of large asteroids, we conducted a high-angular-resolution imaging survey of 42 large main-belt asteroids with VLT/SPHERE/ZIMPOL. Our asteroid sample comprises 39 bodies with D ≥ 100 km and in particular most D ≥ 200 km main-belt asteroids (20/23). Furthermore, it nicely reflects the compositional diversity present in the main belt as the sampled bodies belong to the following taxonomic classes: A, B, C, Ch/Cgh, E/M/X, K, P/T, S, and V. Methods. The SPHERE/ZIMPOL images were first used to reconstruct the 3D shape of all targets with both the ADAM and MPCD reconstruction methods.We subsequently performed a detailed shape analysis and constrained the density of each target using available mass estimates including our own mass estimates in the case of multiple systems. Results. The analysis of the reconstructed shapes allowed us to identify two families of objects as a function of their diameters, namely spherical and elongated bodies. A difference in rotation period appears to be the main origin of this bimodality. In addition, all but one object (216 Kleopatra) are located along the Maclaurin sequence with large volatile-rich bodies being the closest to the latter. Our results further reveal that the primaries of most multiple systems possess a rotation period of shorter than 6 h and an elongated shape (c=a ≤ 0.65). Densities in our sample range from ∼1.3 g cm-3 (87 Sylvia) to ∼4.3 g cm-3 (22 Kalliope). Furthermore, the density distribution appears to be strongly bimodal with volatile-poor (P ≥ 2.7 g cm-3) and volatile-rich (P ≤ 2.2 g cm-3) bodies. Finally, our survey along with previous observations provides evidence in support of the possibility that some C-complex bodies could be intrinsically related to IDP-like P- and D-type asteroids, representing different layers of a same body (C: core; P/D: outer shell). We therefore propose that P/ D-types and some C-types may have the same origin in the primordial trans-Neptunian disk., We warmly thank the ESO staff at Paranal and in particular Henri Boffin for providing us precious support and advice throughout the entire observing programme. P.V., A.D., M.F., L.J. and B.C. were supported by CNRS/INSU/PNP. The work of T.S-R. was carried out through grant APOSTD/2019/046 by Generalitat Valenciana (Spain). This work was supported by the MINECO (Spanish Ministry of Economy) through grant RTI2018-095076-B-C21 (MINECO/FEDER, UE). TRAPPIST project is funded by the Belgian Fund for Scientic Research (Fond National de la Recherche Scientique, FNRS) under the grant PDR T.0120.21. E.J. is a FNRS Senior Research Associate. F.M. is supported by the National Science Foundation under Grant No. 1743015.
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- 2021
86. An advanced multipole model for (216) Kleopatra triple system
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Laurent Jorda, Josef Hanus, François Colas, Alexis Drouard, J. Grice, Julie Castillo-Rogez, Patrick Michel, Philippe Lamy, Pierre Vernazza, Josef Ďurech, Miroslav Brož, Bin Yang, Matti Viikinkoski, Franck Marchis, Tadeusz Michalowski, Marin Ferrais, Fabrice Cipriani, Thierry Fusco, Nicolas Rambaux, Olivier Witasse, Przemyslaw Bartczak, Arthur Vigan, David Vokrouhlický, Emmanuel Jehin, E. Podlewska-Gaca, Toni Santana-Ros, Frédéric Vachier, M. Pajuelo, Paolo Tanga, S. Benseguane, Romain Fétick, Christophe Dumas, Grzegorz Dudziński, Mirel Birlan, Agnieszka Kryszczyńska, S. Fauvaud, Anna Marciniak, Benoit Carry, J. Berthier, Michael Marsset, Institute of Astronomy [Prague], Charles University [Prague] (CU), Search for Extraterrestrial Intelligence Institute (SETI), 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), Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE), 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 de Lille-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Department of Earth, Atmospheric and Planetary Sciences [MIT, Cambridge] (EAPS), Massachusetts Institute of Technology (MIT), Tampere University of Technology [Tampere] (TUT), Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Space Sciences, Technologies and Astrophysics Research Institute (STAR), Université de Liège, SETI Institute, Ondřejov Observatory of the Prague Astronomical Institute, Czech Academy of Sciences [Prague] (CAS), Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Observatoire du Bois de Bardon, Astronomical Institute of Romanian Academy, Romanian Academy, Thirty Meter Telescope Observatory, Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), European Space Research and Technology Centre (ESTEC), Agence Spatiale Européenne = European Space Agency (ESA), DOTA, ONERA, Université Paris Saclay [Châtillon], ONERA-Université Paris-Saclay, School of Physical Sciences [Milton Keynes], Faculty of Science, Technology, Engineering and Mathematics [Milton Keynes], The Open University [Milton Keynes] (OU)-The Open University [Milton Keynes] (OU), PLANETO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Pontificia Universidad Católica del Perú = Pontifical Catholic University of Peru (PUCP), Universidad de Alicante, Institut de Ciencies del Cosmos (ICCUB), Universitat de Barcelona (UB), European Southern Observatory [Santiago] (ESO), European Southern Observatory (ESO), Czech Science Foundation, Charles University (Czech Republic), National Science Foundation (US), National Aeronautics and Space Administration (US), Generalitat Valenciana, Ministerio de Ciencia, Innovación y Universidades (España), Fédération Wallonie-Bruxelles, and Belgian Science Policy Office
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010504 meteorology & atmospheric sciences ,fundamental parameters [Planets and satellites] ,Library science ,FOS: Physical sciences ,Astrophysics ,01 natural sciences ,methods: numerical ,Física Aplicada ,0103 physical sciences ,Celestial mechanics ,planets and satellites: fundamental parameters ,010303 astronomy & astrophysics ,0105 earth and related environmental sciences ,Physics ,Earth and Planetary Astrophysics (astro-ph.EP) ,[PHYS]Physics [physics] ,numerical [Methods] ,[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,Minor planets ,Astronomy and Astrophysics ,Astrometry ,celestial mechanics ,asteroids: individual: (216) Kleopatra ,individual: (216) Kleopatra [Asteroids] ,Space and Planetary Science ,individual: (216) Kleopatra [Minor planets, asteroids] ,minor planets ,astrometry ,TRAPPIST ,Christian ministry ,Earth and Planetary Astrophysics ,Astrophysics::Earth and Planetary Astrophysics ,Astrophysics - Earth and Planetary Astrophysics - Abstract
[Aims] To interpret adaptive-optics observations of (216) Kleopatra, we need to describe an evolution of multiple moons orbiting an extremely irregular body and include their mutual interactions. Such orbits are generally non-Keplerian and orbital elements are not constants. [Methods] Consequently, we used a modified N-body integrator, which was significantly extended to include the multipole expansion of the gravitational field up to the order ℓ = 10. Its convergence was verified against the 'brute-force' algorithm. We computed the coefficients Cℓ m, Sℓ m for Kleopatra's shape, assuming a constant bulk density. For Solar System applications, it was also necessary to implement a variable distance and geometry of observations. Our χ2 metric then accounts for the absolute astrometry, the relative astrometry (second moon with respect to the first), angular velocities, and silhouettes, constraining the pole orientation. This allowed us to derive the orbital elements of Kleopatra's two moons. [Results] Using both archival astrometric data and new VLT/SPHERE observations (ESO LP 199.C-0074), we were able to identify the true periods of the moons, P1 = (1.822359 ± 0.004156) d, P2 = (2.745820 ± 0.004820) d. They orbit very close to the 3:2 mean-motion resonance, but their osculating eccentricities are too small compared to other perturbations (multipole, mutual), meaning that regular librations of the critical argument are not present. The resulting mass of Kleopatra, m1 = (1.49 ± 0.16) × 10-12 M· or 2.97 × 1018 kg, is significantly lower than previously thought. An implication explained in the accompanying paper is that (216) Kleopatra is a critically rotating body., Broz, M. et al., This work has been supported by the Czech Science Foundation through grant 21-11058S (M. Brož, D. Vokrouhlický), 20-08218S (J. Hanuš, J. Ďurech), and by the Charles University Research program No. UNCE/SCI/023. This material is partially based upon work supported by the National Science Foundation under Grant No. 1743015. P.V., A.D., M.F. and B.C. were supported by CNRS/INSU/PNP. M.M. was supported by the National Aeronautics and Space Administration under grant No. 80NSSC18K0849 issued through the Planetary Astronomy Program. The work of TSR was carried out through grant APOSTD/2019/046 by Generalitat Valenciana (Spain). This work was supported by the MINECO (Spanish Ministry of Economy) through grant RTI2018-095076-B-C21 (MINECO/FEDER, UE). The research leading to these results has received funding from the ARC grant for Concerted Research Actions, financed by the Wallonia-Brussels Federation. TRAPPIST is a project funded by the Belgian Fonds (National) de la Recherche Scientifique (F.R.S.-FNRS) under grant FRFC 2.5.594.09.F. TRAPPIST-North is a project funded by the University of Liège, and performed in collaboration with Cadi Ayyad University of Marrakesh. E. Jehin is a FNRS Senior Research Associate.
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- 2021
87. Reply to:Reconciling differences in impact of molecular subtyping on response to cisplatin-based chemotherapy
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Jørgen Bjerggaard Jensen, Emil Christensen, Philippe Lamy, Ann Taber, Lars Dyrskjøt, and Mads Agerbæk
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Oncology ,medicine.medical_specialty ,Multidisciplinary ,business.industry ,Science ,Bladder cancer ,General Physics and Astronomy ,General Chemistry ,Neoadjuvant Therapy ,General Biochemistry, Genetics and Molecular Biology ,Subtyping ,Cancer therapeutic resistance ,Matters Arising ,Cisplatin based chemotherapy ,Chemotherapy, Adjuvant ,Internal medicine ,Cancer genomics ,medicine ,Cisplatin ,business - Published
- 2021
88. Bilobate comet morphology and internal structure controlled by shear deformation
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Carsten Güttler, F. Preusker, Dennis Bodewits, Alice Lucchetti, Philippe Lamy, J.-B. Vincent, H. U. Keller, D. Nébouy, Björn Davidsson, A. T. Auger, Matteo Massironi, Stefano Debei, Cecilia Tubiana, F. La Forgia, Stubbe F. Hviid, Hans Rickman, M. De Cecco, Luca Penasa, M. A. Barucci, L. M. Lara, Nilda Oklay, C. Matonti, Nicholas Attree, J. L. Bertaux, Olivier Groussin, Sophie Viseur, Monica Lazzarin, Maurizio Pajola, Imre Toth, Francesco Marzari, Ivano Bertini, R. Rodrigo, Jakob Deller, Sylvain Bouley, Sonia Fornasier, Holger Sierks, V. Da Deppo, J. J. Lopez-Moreno, Wing-Huen Ip, Laurent Jorda, Giampiero Naletto, G. Cremonese, Frank Scholten, Marco Fulle, Xian Shi, Stefano Mottola, P. J. Gutierrez, Detlef Koschny, Centre européen de recherche et d'enseignement des géosciences de l'environnement (CEREGE), Institut de Recherche pour le Développement (IRD)-Institut National de la Recherche Agronomique (INRA)-Aix Marseille Université (AMU)-Collège de France (CdF (institution))-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), 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), Faculty of Natural Sciences [Stirling], University of Stirling, DLR Institut für Planetenforschung, Deutsches Zentrum für Luft- und Raumfahrt [Berlin] (DLR), Géosciences Paris Sud (GEOPS), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), PLANETO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research (MPS), Max-Planck-Gesellschaft, Centro di Ateneo di Studi e Attività Spaziali 'Giuseppe Colombo' (CISAS), Università degli Studi di Padova = University of Padua (Unipd), Dipartimento di Fisica e Astronomia 'Galileo Galilei', CNR Istituto di Fotonica e Nanotecnologie [Padova] (IFN), National Research Council of Italy | Consiglio Nazionale delle Ricerche (CNR), Instituto de Astrofísica de Andalucía (IAA), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), International Space Science Institute [Bern] (ISSI), Research and Scientific Support Department, ESTEC (RSSD), European Space Research and Technology Centre (ESTEC), Agence Spatiale Européenne = European Space Agency (ESA)-Agence Spatiale Européenne = European Space Agency (ESA), Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), 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)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Department of Physics [Auburn], Auburn University (AU), INAF - Osservatorio Astronomico di Padova (OAPD), Istituto Nazionale di Astrofisica (INAF), CNR Institute for Photonics and Nanotechnologies (IFN), Department of Industrial Engineering [Padova], University of Trento [Trento], INAF - Osservatorio Astronomico di Trieste (OAT), Institute of Space Science [Taiwan], National Central University [Taiwan] (NCU), Institute of Astronomy [Taiwan] (IANCU), Institut für Geophysik und Extraterrestrische Physik [Braunschweig] (IGEP), Technische Universität Braunschweig = Technical University of Braunschweig [Braunschweig], Dipartimento di Geoscienze [Padova], Department of Physics and Astronomy [Uppsala], Uppsala University, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences [Budapest], Hungarian Academy of Sciences (MTA)-Hungarian Academy of Sciences (MTA), national funding agency of Germany (DLR), national funding agency of France (CNES), national funding agency of Italy (ASI), national funding agency of Spain (MEC), national funding agency of Sweden (SNSB), ESA Technical Directorate, Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Collège de France (CdF)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Institut National de la Recherche Agronomique (INRA), 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), IMPEC - LATMOS, Max-Planck-Institut für Sonnensystemforschung (MPS), Universita degli Studi di Padova, Consiglio Nazionale delle Ricerche [Roma] (CNR), Consejo Superior de Investigaciones Científicas [Spain] (CSIC), European Space Agency (ESA)-European Space Agency (ESA), California Institute of Technology (CALTECH)-NASA, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Technische Universität Braunschweig [Braunschweig], Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Collège de France (CdF (institution))-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut National de la Recherche Agronomique (INRA), and Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)
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Solar System ,[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,010504 meteorology & atmospheric sciences ,3d analysis ,Comet ,Geophysics ,010502 geochemistry & geophysics ,01 natural sciences ,rosetta ,Shear (geology) ,[SDU]Sciences of the Universe [physics] ,13. Climate action ,General Earth and Planetary Sciences ,Sublimation (phase transition) ,Water ice ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,Earth and Planetary Sciences (all) ,Geology ,0105 earth and related environmental sciences - Abstract
Bilobate comets—small icy bodies with two distinct lobes—are a common configuration among comets, but the factors shaping these bodies are largely unknown. Cometary nuclei, the solid centres of comets, erode by ice sublimation when they are sufficiently close to the Sun, but the importance of a comet’s internal structure on its erosion is unclear. Here we present three-dimensional analyses of images from the Rosetta mission to illuminate the process that shaped the Jupiter-family bilobate comet 67P/Churyumov–Gerasimenko over billions of years. We show that the comet’s surface and interior exhibit shear-fracture and fault networks, on spatial scales of tens to hundreds of metres. Fractures propagate up to 500 m below the surface through a mechanically homogeneous material. Through fracture network analysis and stress modelling, we show that shear deformation generates fracture networks that control mechanical surface erosion, particularly in the strongly marked neck trough of 67P/Churyumov–Gerasimenko, exposing its interior. We conclude that shear deformation shapes and structures the surface and interior of bilobate comets, particularly in the outer Solar System where water ice sublimation is negligible. The shape and internal structure of bilobate comet 67P is controlled by shear deformation inducing mechanically driven erosion along shear fracture networks, according to a 3D analysis of images from the Rosetta mission.
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- 2019
89. Abstract 1282: Elevated T cell exhaustion and immune cell infiltration is associated with BCG failure in patients with non-muscle invasive bladder cancer
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Trine Strandgaard, Iver Nordentoft, Emil Christensen, Sia Lindskrog, Philippe Lamy, Karin Birkenkamp-Demtröder, Torben Steiniche, Jørgen Bjerggaard Jensen, and Lars Dyrskjøt
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Cancer Research ,Oncology - Abstract
Introduction: Gold standard treatment in patients with high-risk non-muscle invasive bladder cancer (NMIBC) includes Bacillus Calmette-Guérin (BCG), which activates the immune cells to kill remaining cancerous cells after surgical removal of the tumors. However, 40% of patients do not have a clinical benefit of BCG. The presence of immune cells, their functional state, as well as genomic alterations in the tumor and the normal appearing urothelial tissue, defined as field effect, may have significant impact on therapeutic outcome. Materials and methods: To investigate this, we analyzed samples from 156 patients diagnosed with NMIBC, including 237 tumors, 569 urine samples, and 305 biopsies of adjacent normal appearing urothelium. Patients had a median follow-up time of 8 years. 70 patients (45%) progressed to muscle-invasive bladder cancer or experienced early high grade recurrence within two years after ended BCG treatment, defined as BCG failure. Urinary levels of 92 immune-oncology related proteins were measured in pre- and post-treatment samples using the Olink proteomics platform. Total RNA- and whole exome sequencing (WES) data was generated from tumors before and after BCG. Clonal patient-specific mutations were selected for deep-targeted sequencing of the adjacent normal appearing biopsies. The level of field effect was defined as the mean of the variant allele frequency for mutations observed in normal biopsies. Results: We found that treatment with BCG activated the immune system regardless of clinical outcome. However, patients differed in urinary protein profile after BCG depending on their clinical response. Transcriptomic analysis of tumors showed that UROMOL2021 subtypes were significantly associated with outcome and clinical response (p=0.018). Paired tumors showed a shift in subtype to an immune infiltrated subtype (class 2b) after treatment in 36% of cases. Patients with BCG failure showed signs of immune exhaustion after treatment indicated by higher expression of the T cell exhaustion marker genes CTLA4 (p=0.0067), LAG3 (p=0.00012), TIM-3 (p=0.022), KLRG1 (p=0.028), and PD-1 (p=0.047), and higher immune cell infiltration (p=0.011). Genomic features such as mutational signatures and mutational load were not predictive of clinical response. Interestingly, BCG-responsive patients had a high level of field effect before BCG (p=0.0026), suggesting that field effect could lead to increased BCG efficacy. Conclusion: BCG treatment was associated with immune system activation reflected in both urine and tissue samples. In patients with BCG failure, we observed an immune exhausted phenotype after treatment, and we observed a high level of field effect before treatment in responsive patients. Collectively, this could indicate that increased immunogenicity and prolonged immune activation are key factors in BCG treatment responsiveness. Citation Format: Trine Strandgaard, Iver Nordentoft, Emil Christensen, Sia Lindskrog, Philippe Lamy, Karin Birkenkamp-Demtröder, Torben Steiniche, Jørgen Bjerggaard Jensen, Lars Dyrskjøt. Elevated T cell exhaustion and immune cell infiltration is associated with BCG failure in patients with non-muscle invasive bladder cancer [abstract]. In: Proceedings of the American Association for Cancer Research Annual Meeting 2022; 2022 Apr 8-13. Philadelphia (PA): AACR; Cancer Res 2022;82(12_Suppl):Abstract nr 1282.
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- 2022
90. Abstract 3483: Single-nucleus RNA-sequencing of human bladder tumors delineates intra-tumor cellular and subtype heterogeneity
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Sia V. Lindskrog, Sofie S. Schmøkel, Iver Nordentoft, Philippe Lamy, Michael Knudsen, Jørgen B. Jensen, and Lars Dyrskjøt
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Cancer Research ,Oncology - Abstract
Introduction: Single cell technologies now make it possible to study tumor ecosystems at single cell resolution and may improve our biological understanding of disease aggressiveness and tumor heterogeneity. Whereas single-cell RNA-sequencing of clinical tumor biopsies requires immediate processing after tissue acquisition, single-nucleus RNA-sequencing (snRNA-seq) allows profiling of single nuclei isolated from frozen tumor tissue from patients with long-term follow-up and known clinical outcomes. Methods: We performed snRNA-seq of frozen tumors from 48 bladder cancer (BC) patients (10 Ta, 13 T1, 25 T2-4) using an optimized DroNc-seq protocol. Nuclei were isolated from frozen biopsies using IgePal lysis buffer and droplets were created using the Dolomite Bio platform followed by library generation and sequencing on an Illumina NovaSeq 6000. All epithelial nuclei were classified according to the UROMOL classes of non-muscle-invasive BC or the consensus classes of muscle-invasive BC. Bulk total RNA-sequencing (RNA-seq) was available for 44 of the tumors for comparison. Three tumors were additionally analyzed using 10x Chromium for validation and four tumors were analyzed using 10x Visium Spatial Transcriptomics. Results: After pre-processing the raw sequencing data, we obtained data from 117,653 nuclei in total and 59,201 nuclei remained after quality control filtering (1,233 nuclei per tumor and 529 expressed genes per nuclei on average). We focused our analysis on the epithelial compartment, as it constituted the bulk of the tumors (99% of all nuclei). UMAP visualization and clustering of all tumors were mainly driven by patient origin indicating a high level of inter-tumor heterogeneity. To explore intra-tumor heterogeneity and the association to disease aggressiveness, we characterized the tumors individually using hallmark BC gene signatures. Finally, we explored the composition of transcriptomic classes for each tumor and found that 52% of tumors displayed profound intra-tumor class heterogeneity with less than 70% of all nuclei belonging to a single class. The dominating transcriptomic class of single nuclei was only consistent in 44% of the tumors when compared to the overall transcriptomic class from bulk RNA-seq. This may be explained by several levels of heterogeneity and method differences, including the technical challenges of applying a bulk classifier to single nuclei data. We are currently investigating whether specific epithelial subpopulations are associated to outcome and whether signatures derived from snRNA-seq data can be recovered in bulk RNA-seq data and used as prognostic predictors. Conclusion: Our results highlight the biological complexity of bladder tumors and underline the importance of considering the extent of intra-tumor heterogeneity in the clinical management of BC patients. Citation Format: Sia V. Lindskrog, Sofie S. Schmøkel, Iver Nordentoft, Philippe Lamy, Michael Knudsen, Jørgen B. Jensen, Lars Dyrskjøt. Single-nucleus RNA-sequencing of human bladder tumors delineates intra-tumor cellular and subtype heterogeneity [abstract]. In: Proceedings of the American Association for Cancer Research Annual Meeting 2022; 2022 Apr 8-13. Philadelphia (PA): AACR; Cancer Res 2022;82(12_Suppl):Abstract nr 3483.
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- 2022
91. Abstract 1275: Treatment response and outcome prediction guided by deep targeted sequencing of urine and plasma samples in patients with muscle-invasive bladder cancer
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Emil Christensen, Iver Nordentoft, Sara K. Elbæk, Karin Birkenkamp-Demtröder, Ann Taber, Michael Knudsen, Philippe Lamy, Mads Agerbæk, Jørgen B. Jensen, and Lars Dyrskjøt
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Cancer Research ,Oncology - Abstract
Background Standard treatment in patients with localized muscle-invasive bladder cancer (MIBC) is neoadjuvant chemotherapy (NAC) followed by radical cystectomy (CX). Importantly, there is currently no clinically validated way to estimate response to NAC before CX, where a pathological assessment of tumor down-staging is used as a proxy for response. Identification and tracking of circulating tumor DNA (ctDNA) has been shown to reflect prognosis and treatment response in several cancers, including bladder cancer. Here, we aim to investigate the capability of a combined plasma, urine supernatant and urine pellet mutation analysis by deep targeted sequencing for detecting residual tumor and treatment response before CX. Methods In total, 92 patients with localized MIBC treated with NAC followed by CX were included in the study. DNA extracted from primary tumors and leukocytes were subjected to whole exome sequencing for identification of approx. 50 mutations per patient that were used to design a custom NGS panel. Urine supernatants (n=281), urine pellets (n=114) and plasma samples (n=167), collected before CX, were subjected to deep targeted sequencing employing unique molecular identifiers (UMI). Mutations were assessed using the Shearwater algorithm and samples were further assessed using Fisher’s Method and bootstrapping of random mutations. In-silico analyses identified the limit of detection to be approx. 0.1%. For 56 patients, plasma mutation data (n=288 samples) were obtained from a previously published study by our group. Results Tumor derived DNA levels in paired urine supernatants and pellets were correlated (rho=0.8), however with higher levels in pellets when adjusting for the extracted amount of DNA (p Conclusions Tumor derived DNA was more frequently observed in urine samples and at higher levels compared to plasma samples. Interestingly, we show that tumor derived DNA dynamics in urine supernatants might better reflect the local tumor environment and plasma-based tumor derived DNA better reflects outcome following surgery, i.e. disease dissemination. Citation Format: Emil Christensen, Iver Nordentoft, Sara K. Elbæk, Karin Birkenkamp-Demtröder, Ann Taber, Michael Knudsen, Philippe Lamy, Mads Agerbæk, Jørgen B. Jensen, Lars Dyrskjøt. Treatment response and outcome prediction guided by deep targeted sequencing of urine and plasma samples in patients with muscle-invasive bladder cancer [abstract]. In: Proceedings of the American Association for Cancer Research Annual Meeting 2022; 2022 Apr 8-13. Philadelphia (PA): AACR; Cancer Res 2022;82(12_Suppl):Abstract nr 1275.
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- 2022
92. Abstract 3409: Whole genome sequencing of liquid tumor biopsies (ctDNA) from men with metastatic castration resistant prostate cancer
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Simone Weiss, Philippe Lamy, Maibritt Nørgaard, Michael Knudsen, Jørgen B. Jensen, Jakob S. Pedersen, Michael Borre, and Karina D. Sørensen
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Cancer Research ,Oncology - Abstract
Background: Prostate cancer (PC) is the fifth most lethal male malignancy worldwide, as advanced metastatic castration resistant PC (mCRPC) remains incurable. Genomic biomarkers that can predict treatment response are urgently needed to facilitate personalized mCRPC treatment. Such biomarkers can be identified by whole genome sequencing (WGS) of tumor biopsies. Blood plasma can serve as a non-invasive liquid tumor biopsy as it contains cell free DNA (cfDNA), a subset of which in cancer patients is tumor-derived (circulating tumor DNA; ctDNA). The biomarker discovery potential of WGS of cfDNA in mCRPC remains largely undescribed, as most WGS studies to date have focused on tissue biopsies. Thus, we here aimed to characterize the genomic tumor landscape of mCRPC using WGS of cfDNA. Methods: We previously performed low-pass WGS (mean coverage: 0.5X) of cfDNA sampled prior to initiation of first-line mCRPC treatment from 143 mCRPC patients (mean ctDNA fraction: 0.15). From these, 10 patients with high (>0.35) ctDNA fractions who received enzalutamide as first-line mCRPC treatment were selected for deeper WGS here. Matched germline DNA from buffy coat (peripheral blood mononuclear cells) was also sequenced. Single-nucleotide variants (SNVs) were called with Mutect2 and CaVEMan, indels with Mutect2 and Pindel, copy-number variants (CNVs) with ASCAT, and structural variants (SVs) with BRASS. For the final analysis, we considered only SNVs and indels called by both tools. Results: We sequenced germline samples to a mean coverage of 25X (range: 19-28X) and cfDNA samples to a mean coverage of 32X (range: 23-43X). We identified a median of 5,241 SNVs/indels (range: 3,422-48,314) per patient and the mean tumor mutation burden was 1.7 mutations/Mb. One sample had >9 times more SNVs/indels than the median, suggesting microsatellite instability. Among the most recurrently mutated genes were LRP1B (7/10 patients), ARSB (5/10 patients), and TP53 (4/10 patients). COSMIC mutational signature analysis revealed that the clock-like signatures 1, 5, and 40 were most frequent. In contrast, the hypermutated sample was driven primarily by the defective DNA mismatch repair signatures 15, 26, and 44. CNVs affected a mean of 40.9% of the genome. Common PC CNVs were observed, including gains at chromosome 8 (MYC) in 8/10 patients and losses at chromosome 10 (PTEN) in 5/10 patients. Recurrent focal amplifications (defined as >8 copies in regions Conclusion: This study highlights that WGS of cfDNA contributes to the identification of genomic aberrations that may serve as potential biomarkers to guide personalized treatment of mCRPC in the future. Citation Format: Simone Weiss, Philippe Lamy, Maibritt Nørgaard, Michael Knudsen, Jørgen B. Jensen, Jakob S. Pedersen, Michael Borre, Karina D. Sørensen. Whole genome sequencing of liquid tumor biopsies (ctDNA) from men with metastatic castration resistant prostate cancer [abstract]. In: Proceedings of the American Association for Cancer Research Annual Meeting 2022; 2022 Apr 8-13. Philadelphia (PA): AACR; Cancer Res 2022;82(12_Suppl):Abstract nr 3409.
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- 2022
93. Response of the interplanetary hydrogen population to global changes of solar activity: a quantitative analysis based on SOHO/SWAN and SOHO/LASCO-C2 data comparison
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Philippe Lamy, Stéphane Ferron, Dimitra Koutroumpa, Lucile Conan, Hugo Gilardy, Eric Quémerais, HELIOS - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), École Supérieure des Techniques Aéronautiques et de Construction Automobile (ESTACA), Analytic and Computational Research, Inc. - Earth Sciences (ACRI-ST), and Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)
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Physics ,[PHYS]Physics [physics] ,Electron density ,education.field_of_study ,Hydrogen ,Population ,Phase (waves) ,chemistry.chemical_element ,Astrophysics ,7. Clean energy ,Solar wind ,chemistry ,13. Climate action ,[SDU]Sciences of the Universe [physics] ,Ionization ,Physics::Space Physics ,Astrophysics::Solar and Stellar Astrophysics ,education ,Interplanetary spaceflight ,Heliosphere - Abstract
For more than two decades the SOHO/SWAN instrument has been monitoring the full-sky hydrogen backscattered Lyman-α emission, and the derived three-dimensional solar wind proton flux. We present a comparison of the time series of the latitude-integrated hydrogen ionization rates (β) derived from the inversion of the SWAN full-sky maps with the integrated coronal electron density derived from the inversion of SOHO/LASCO-C2 white light images. The analysis shows a variable time lag of the SWAN β of a few Carrington rotations, correlated with the solar cycle phase (larger delay during solar maxima compared to minima). This is a direct consequence of the variation of the size of the hydrogen ionization cavity and the time it takes for hydrogen atoms to propagate in the inner heliosphere. This effect should be taken into account in studies of the interstellar neutral populations in interplanetary space.
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- 2021
94. An integrated multi-omics analysis identifies prognostic molecular subtypes of non-muscle-invasive bladder cancer
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Roman Nawroth, Richard T. Bryan, Philippe Lamy, Tobias Maurer, Margaret A. Knowles, Gregers G. Hermann, Marc-Oliver Grimm, Ann Taber, Torben Steiniche, Jørgen Bjerggaard Jensen, David J. DeGraff, Francisco X. Real, Karin Mogensen, Joshua I. Warrick, Jay D. Raman, Anshita Goel, Ulrika Segersten, Karin Birkenkamp-Demtröder, Emil Christensen, Clarice S. Groeneveld, Xiaoqi Lin, Joshua J. Meeks, Brian J. Jordan, Núria Malats, Trine Strandgaard, Sia Viborg Lindskrog, Mateo Sokac, Frederik Prip, Gottfrid Sjödahl, Ellen C. Zwarthoff, Tatjana Simic, Iver Nordentoft, Marcus Horstmann, Lasse Maretty, Douglas G. Ward, Dejan Dragicevic, Veronika Weyerer, Carolyn D. Hurst, Aurélien de Reyniès, Kim E.M. van Kessel, Per-Uno Malmström, Astrid Christine Petersen, Arndt Hartmann, Danijel Sikic, Mattias Höglund, Lars Dyrskjøt, Nicolai Juul Birkbak, and Pathology
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Cancer microenvironment ,0301 basic medicine ,Oncology ,medicine.medical_specialty ,Science ,General Physics and Astronomy ,Disease ,Biology ,Proteomics ,Article ,General Biochemistry, Genetics and Molecular Biology ,Transcriptome ,03 medical and health sciences ,0302 clinical medicine ,SDG 3 - Good Health and Well-being ,Internal medicine ,Chromosome instability ,Urologi och njurmedicin ,Cancer genomics ,medicine ,Urology and Nephrology ,Progression-free survival ,Biomarker discovery ,Cancer och onkologi ,Multidisciplinary ,Bladder cancer ,General Chemistry ,medicine.disease ,Subtyping ,Computational biology and bioinformatics ,030104 developmental biology ,Cancer and Oncology ,030220 oncology & carcinogenesis - Abstract
The molecular landscape in non-muscle-invasive bladder cancer (NMIBC) is characterized by large biological heterogeneity with variable clinical outcomes. Here, we perform an integrative multi-omics analysis of patients diagnosed with NMIBC (n = 834). Transcriptomic analysis identifies four classes (1, 2a, 2b and 3) reflecting tumor biology and disease aggressiveness. Both transcriptome-based subtyping and the level of chromosomal instability provide independent prognostic value beyond established prognostic clinicopathological parameters. High chromosomal instability, p53-pathway disruption and APOBEC-related mutations are significantly associated with transcriptomic class 2a and poor outcome. RNA-derived immune cell infiltration is associated with chromosomally unstable tumors and enriched in class 2b. Spatial proteomics analysis confirms the higher infiltration of class 2b tumors and demonstrates an association between higher immune cell infiltration and lower recurrence rates. Finally, the independent prognostic value of the transcriptomic classes is documented in 1228 validation samples using a single sample classification tool. The classifier provides a framework for biomarker discovery and for optimizing treatment and surveillance in next-generation clinical trials., Multiple molecular profiling methods are required to study urothelial non-muscle-invasive bladder cancer (NMIBC) due to its heterogeneity. Here the authors integrate multi-omics data of 834 NMIBC patients, identifying a molecular subgroup associated with multiple alterations and worse outcomes.
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- 2021
95. LASCO-C3 Observations of the K- and F-Coronae over 24 Years (1996 – 2019): Photopolarimetry and Electron Density Distribution
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Antoine Llebaria, Eric Quémerais, Philippe Lamy, Hugo Gilardy, Fabrice Ernandez, HELIOS - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), 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), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), and Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
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Physics ,Electron density ,010504 meteorology & atmospheric sciences ,Stray light ,[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] ,Polarimetry ,Astronomy and Astrophysics ,Astrophysics ,Polarizer ,Polarization (waves) ,01 natural sciences ,Corona ,law.invention ,Space and Planetary Science ,law ,Polarization ,0103 physical sciences ,Radiance ,010303 astronomy & astrophysics ,Coronagraph ,Observations ,0105 earth and related environmental sciences - Abstract
International audience; We present the polarimetric analysis of the white-light images of the corona obtained with the Large-Angle Spectrometric COronagraph LASCO-C3 onboard the Solar and Heliospheric Observatory (SOHO) from 1996 to 2019, leading to the separation of the K- and F-components and the derivation of the electron-density distribution. The analysis makes use of polarized sequences composed of three images obtained through three polarizers oriented at +60°, 0°, and -60°, complemented by a neighboring unpolarized image. However, the degradation of the 0° polarizer noticed in 1999 compelled us to reconstruct the corresponding images from those obtained with the two other polarizers and the unpolarized ones thereafter. The analysis closely follows the method developed for LASCO-C2 (Lamy et al. in Solar Phys. 295, 89, 2020) and implements the formalism of Mueller, albeit with additional difficulties notably the presence of a non-axially symmetric component of stray light. Critical corrections were derived from a SOHO roll sequence and from consistency criteria (e.g. the “tangential” direction of polarization). The quasi-uninterrupted photopolarimetric analysis of the outer corona over two complete Solar Cycles 23 and 24 was successfully achieved and our final results encompass the characterization of its polarization, of its polarized radiance, of the two-dimensional electron density, and of the K-corona. Comparison between the C3 and C2 results in the region where their fields of view overlap shows an overall agreement. The C3 results are further in agreement with those of eclipses and radio-ranging measurements to an elongation of ≈10 R⊙ but tend to diverge further out. Although the coronal polarization out to 20 R⊙ is still highly correlated with the temporal variation of the total magnetic field, this divergence probably results from the increasing polarization of the F-corona with increasing solar elongation.
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- 2021
96. Sample return of primitive matter from the outer Solar System
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Andreas Morlok, Mathieu Roskosz, Martin Rubin, Hugues Leroux, Sara S. Russell, J. Carter, Vinciane Debaille, Brigitte Zanda, Ernesto Palomba, Laurette Piani, Emmanuel Jehin, Johan Villeneuve, Vassilissa Vinogradoff, Maria Schönbächler, Joern Helbert, Yves Marrocchi, Peter Wurz, C. Cartier, Ottaviano Ruesch, Addi Bischoff, Pierre Beck, Evelyn Füri, Jérémie Lasue, A. Guilbert-Lepoutre, N. Thomas, Philippe Lamy, Laurent Jorda, Eric Quirico, Mauro Ciarniello, O. Mousis, Olivier Groussin, Henner Busemann, Ingo Leya, Rosario Brunetto, Cristian Carli, A. Delsanti, Louis Le Sergeant d'Hendecourt, T. Magna, Pierre Vernazza, Ashley J. King, Peter Hoppe, Lydie Bonal, Gregory A. Brennecka, Thorsten Kleine, C. Le Guillou, Laurent Remusat, 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), 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, Institut für Planetologie [Münster], Westfälische Wilhelms-Universität Münster = University of Münster (WWU), Lawrence Livermore National Laboratory (LLNL), 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), Institute of Geochemistry and Petrology [ETH Zürich], Department of Earth Sciences [Swiss Federal Institute of Technology - ETH Zürich] (D-ERDW), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich)- Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), Istituto di Astrofisica e Planetologia Spaziali - INAF (IAPS), Istituto Nazionale di Astrofisica (INAF), Centre de Recherches Pétrographiques et Géochimiques (CRPG), Institut national des sciences de l'Univers (INSU - CNRS)-Université de Lorraine (UL)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Géochimie, Traçage Isotopique, Minéral et élémentaire - G-Time (Bruxelles, Belgium), Physique des interactions ioniques et moléculaires (PIIM), Aix Marseille Université (AMU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Géologie de Lyon - Terre, Planètes, Environnement (LGL-TPE), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Université Jean Monnet - Saint-Étienne (UJM)-Centre National de la Recherche Scientifique (CNRS), DLR Institut für Planetenforschung, Deutsches Zentrum für Luft- und Raumfahrt [Berlin] (DLR), Max-Planck-Institut für Chemie (MPIC), Max-Planck-Gesellschaft, Space Sciences, Technologies and Astrophysics Research Institute (STAR), Université de Liège, The Natural History Museum [London] (NHM), HELIOS - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut de recherche en astrophysique et planétologie (IRAP), 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), Unité Matériaux et Transformations - UMR 8207 (UMET), Centrale Lille-Institut de Chimie du CNRS (INC)-Université de Lille-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), Physics Institute [Bern], University of Bern, Czech Geological Survey [Praha], Institut de minéralogie, de physique des matériaux et de cosmochimie (IMPMC), Muséum national d'Histoire naturelle (MNHN)-Institut de recherche pour le développement [IRD] : UR206-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), École normale supérieure - Lyon (ENS Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lille, CNRS, INRA, ENSCL, Laboratoire d'Astrophysique de Marseille [LAM], Institut de Planétologie et d'Astrophysique de Grenoble [IPAG ], Lawrence Livermore National Laboratory [LLNL], Institut d'astrophysique spatiale [IAS], Istituto di Astrofisica e Planetologia Spaziali - INAF [IAPS], Centre de Recherches Pétrographiques et Géochimiques [CRPG], Physique des interactions ioniques et moléculaires [PIIM], Laboratoire de Géologie de Lyon - Terre, Planètes, Environnement [LGL-TPE], German Aerospace Center [DLR], Max Planck Institute for Chemistry [MPIC], Space Sciences, Technologies and Astrophysics Research Institute [STAR], The Natural History Museum [London] [NHM], Laboratoire Atmosphères, Milieux, Observations Spatiales [LATMOS], Institut de recherche en astrophysique et planétologie [IRAP], Unité Matériaux et Transformations - UMR 8207 [UMET], Institut de minéralogie, de physique des matériaux et de cosmochimie [IMPMC], Institut de minéralogie et de physique des milieux condensés [IMPMC], 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), 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), Westfälische Wilhelms-Universität Münster (WWU), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Géologie de Lyon - Terre, Planètes, Environnement [Lyon] (LGL-TPE), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-École normale supérieure - Lyon (ENS Lyon), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), 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)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), and Institut de Chimie du CNRS (INC)-Université de Lille-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Centrale Lille Institut (CLIL)
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Solar System ,P/D type asteroids ,Cryogenic ,Comet ,Sample return ,010502 geochemistry & geophysics ,Primitive small body ,01 natural sciences ,Astrobiology ,Jupiter ,Sample return mission ,Neptune ,0103 physical sciences ,Comets ,010303 astronomy & astrophysics ,0105 earth and related environmental sciences ,[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,520 Astronomy ,Giant planet ,Astronomy and Astrophysics ,620 Engineering ,Planetary science ,13. Climate action ,Space and Planetary Science ,Asteroid ,[SDU]Sciences of the Universe [physics] ,Geology - Abstract
The last thirty years of cosmochemistry and planetary science have shown that one major Solar System reservoir is vastly undersampled in the available suite of extra-terrestrial materials, namely small bodies that formed in the outer Solar System (>10 AU). Because various dynamical evolutionary processes have modified their initial orbits (e.g., giant planet migration, resonances), these objects can be found today across the entire Solar System as P/D near-Earth and main-belt asteroids, Jupiter and Neptune Trojans, comets, Centaurs, and small (diameter < 200 km) trans-Neptunian objects. This reservoir is of tremendous interest, as it is recognized as the least processed since the dawn of the Solar System and thus the closest to the starting materials from which the Solar System formed. Some of the next major breakthroughs in planetary science will come from studying outer Solar System samples (volatiles and refractory constituents) in the laboratory. Yet, this can only be achieved by an L-class mission that directly collects and returns to Earth materials from this reservoir. It is thus not surprising that two White Papers advocating a sample return mission of a primitive Solar System small body (ideally a comet) were submitted to ESA in response to its Voyage 2050 call for ideas for future L-class missions in the 2035-2050 time frame. One of these two White Papers is presented in this article., Experimental Astronomy, 54 (2-3), ISSN:0922-6435, ISSN:1572-9508
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- 2021
97. First light observations of the solar wind in the outer corona with the Metis coronagraph
- Author
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F. Reale, Giuseppe Tondello, Daniele Telloni, P. Zuppella, Jean-Claude Vial, D. Moses, Luca Teriaca, Giampiero Naletto, Marco Romoli, Petr Heinzel, Federico Landini, Piergiorgio Nicolosi, Udo Schühle, Michela Uslenghi, Maurizio Pancrazzi, Silvano Fineschi, Rita Ventura, Leonard Strachan, Raffaella D'Amicis, Alessandro Liberatore, Christina Plainaki, Mauro Messerotti, Enrico Magli, Marco Stangalini, C.A. Volpicelli, Roberto Bruno, Alessandro Bemporad, Giuseppe Massone, F. Frassetto, R. Aznar Cuadrado, A. Berlicki, F. Auchere, Paolo Romano, G. Capuano, A. M. Malvezzi, Silvio Giordano, Y. De Leo, V. Da Deppo, T. Straus, Kanaris Tsinganos, Alessandra Slemer, Sami K. Solanki, Hardi Peter, V. Andretta, Cooper Downs, Daniele Spadaro, Gerardo Capobianco, A. C. Lanzafame, Gianalfredo Nicolini, Roberto Susino, Clementina Sasso, L. Zangrilli, Marco Velli, M. Casti, E. Antonucci, Angela Ciaravella, Giuseppe Nisticò, Catia Grimani, Lucia Abbo, G. Jerse, M. Fabi, Federica Frassati, Luca Poletto, Philippe Lamy, Y. M. Wang, Joachim Woch, M. G. Pelizzo, G. Zimbardo, Università degli Studi di Firenze = University of Florence [Firenze] (UNIFI), Istituto Nazionale di Astrofisica (INAF), INAF - Osservatorio Astronomico di Capodimonte (OAC), Università degli studi di Catania [Catania], INAF - Osservatorio Astrofisico di Catania (OACT), CNR Istituto di Fotonica e Nanotecnologie [Padova] (IFN), Consiglio Nazionale delle Ricerche [Roma] (CNR), Max-Planck-Institut für Sonnensystemforschung (MPS), Max-Planck-Gesellschaft, Predictive Sciences Inc., INAF - Osservatorio Astrofisico di Torino (OATo), Astronomical Institute of the Czech Academy of Sciences (ASU / CAS), Czech Academy of Sciences [Prague] (CAS), Università degli studi di Torino (UNITO), Universita degli Studi di Padova, Istituto di Astrofisica Spaziale e Fisica Cosmica - Milano (IASF-MI), Naval Research Laboratory (NRL), Catholic University of America, Università degli Studi di Urbino 'Carlo Bo', Università degli studi di Trieste, Politecnico di Torino = Polytechnic of Turin (Polito), NASA Headquarters, Institute of Electronics, Computer and Telecommunication Engineering (IEIIT-CNR), Politecnico di Torino = Polytechnic of Turin (Polito)-Consiglio Nazionale delle Ricerche [Torino] (CNR), Agenzia Spaziale Italiana (ASI), Institut d'astrophysique spatiale (IAS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Astronomical Institute [Wroclaw], University of Wrocław [Poland] (UWr), Istituto di Astrofisica e Planetologia Spaziali - INAF (IAPS), INAF - Osservatorio Astronomico di Palermo (OAPa), HELIOS - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Università di Pavia, Università della Calabria [Arcavacata di Rende] (Unical), Università degli studi di Palermo - University of Palermo, National and Kapodistrian University of Athens (NKUA), University of California [Los Angeles] (UCLA), University of California, Romoli M., Antonucci E., Andretta V., Capuano G.E., Da Deppo V., De Leo Y., Downs C., Fineschi S., Heinzel P., Landini F., Liberatore A., Naletto G., Nicolini G., Pancrazzi M., Sasso C., Spadaro D., Susino R., Telloni D., Teriaca L., Uslenghi M., Wang Y.-M., Bemporad A., Capobianco G., Casti M., Fabi M., Frassati F., Frassetto F., Giordano S., Grimani C., Jerse G., Magli E., Massone G., Messerotti M., Moses D., Pelizzo M.-G., Romano P., Schuhle U., Slemer A., Stangalini M., Straus T., Volpicelli C.A., Zangrilli L., Zuppella P., Abbo L., Auchere F., Aznar Cuadrado R., Berlicki A., Bruno R., Ciaravella A., D'amicis R., Lamy P., Lanzafame A., Malvezzi A.M., Nicolosi P., Nistico G., Peter H., Plainaki C., Poletto L., Reale F., Solanki S.K., Strachan L., Tondello G., Tsinganos K., Velli M., Ventura R., Vial J.-C., Woch J., and Zimbardo G.
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010504 meteorology & atmospheric sciences ,Astrophysics::High Energy Astrophysical Phenomena ,Solar wind ,FOS: Physical sciences ,Astrophysics ,01 natural sciences ,Wind speed ,law.invention ,symbols.namesake ,Sun: corona – solar wind – Sun: UV radiation ,law ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,010303 astronomy & astrophysics ,Coronagraph ,Solar and Stellar Astrophysics (astro-ph.SR) ,0105 earth and related environmental sciences ,Physics ,[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] ,Sun: corona ,Astronomy and Astrophysics ,Plasma ,Solar wind, Sun: corona, Sun: UV radiation ,Sun: UV radiation ,Corona ,Astrophysics - Solar and Stellar Astrophysics ,Space and Planetary Science ,Temporal resolution ,Physics::Space Physics ,symbols ,Outflow ,Doppler effect - Abstract
In this work, we present an investigation of the wind in the solar corona that has been initiated by observations of the resonantly scattered ultraviolet emission of the coronal plasma obtained with UVCS-SOHO, designed to measure the wind outflow speed by applying Doppler dimming diagnostics. Metis on Solar Orbiter complements the UVCS spectroscopic observations that were performed during solar activity cycle 23 by simultaneously imaging the polarized visible light and the H I Lyman-α corona in order to obtain high spatial and temporal resolution maps of the outward velocity of the continuously expanding solar atmosphere. The Metis observations, taken on May 15, 2020, provide the first H I Lyman-α images of the extended corona and the first instantaneous map of the speed of the coronal plasma outflows during the minimum of solar activity and allow us to identify the layer where the slow wind flow is observed. The polarized visible light (580–640 nm) and the ultraviolet H I Lyα (121.6 nm) coronal emissions, obtained with the two Metis channels, were combined in order to measure the dimming of the UV emission relative to a static corona. This effect is caused by the outward motion of the coronal plasma along the direction of incidence of the chromospheric photons on the coronal neutral hydrogen. The plasma outflow velocity was then derived as a function of the measured Doppler dimming. The static corona UV emission was simulated on the basis of the plasma electron density inferred from the polarized visible light. This study leads to the identification, in the velocity maps of the solar corona, of the high-density layer about ±10° wide, centered on the extension of a quiet equatorial streamer present at the east limb – the coronal origin of the heliospheric current sheet – where the slowest wind flows at about 160 ± 18 km s−1 from 4 R⊙ to 6 R⊙. Beyond the boundaries of the high-density layer, the wind velocity rapidly increases, marking the transition between slow and fast wind in the corona.
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- 2021
98. Evidence for differentiation of the most primitive small bodies
- Author
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Pierre Vernazza, Tadeusz Michalowski, Bin Yang, Matti Viikinkoski, Brian Warner, Agnieszka Kryszczyńska, Alexis Drouard, Alexander Storrs, Franck Marchis, J. Grice, François Colas, Patrick Michel, Laurent Jorda, Romain Fétick, Przemyslaw Bartczak, Arthur Vigan, Josef Ďurech, Marc Neveu, Frédéric Vachier, Julie Castillo-Rogez, Emmanuel Jehin, Michael Marsset, Josef Hanus, Nicolas Rambaux, Josselin Desmars, Mikko Kaasalainen, Marin Ferrais, Jérôme Berthier, Olivier Witasse, Philippe Lamy, Zouhair Benkhaldoun, E. Podlewska-Gaca, Fabrice Cipriani, Grzegorz Dudziński, Thierry Fusco, Raoul Behrend, Christophe Dumas, Anna Marciniak, Mirel Birlan, M. Pajuelo, Paolo Tanga, Benoit Carry, T. Santana-Ros, Mark A. Wieczorek, Joseph Louis LAGRANGE (LAGRANGE), 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, 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), 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), Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE), 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 de Lille-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), University of Maryland [College Park], University of Maryland System, NASA Goddard Space Flight Center (GSFC), Institute of Astronomy [Prague], Charles University [Prague], Space Sciences, Technologies and Astrophysics Research Institute (STAR), Université de Liège, Department of Earth, Atmospheric and Planetary Sciences [MIT, Cambridge] (EAPS), Massachusetts Institute of Technology (MIT), Department of Mathematics [Tampere], Tampere University of Technology [Tampere] (TUT), Astronomical Observatory [Poznan], Adam Mickiewicz University in Poznań (UAM), Geneva Observatory, University of Geneva [Switzerland], Oukaimeden Observatory, University of Cadi Ayyad (UCA), Astronomical Institute of Romanian Academy, Romanian Academy, Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), European Space Research and Technology Centre (ESTEC), European Space Agency (ESA), Institut Polytechnique des Sciences Avancées (IPSA), Thirty Meter Telescope Observatory, The Open University [Milton Keynes] (OU), University of Tampere [Finland], HELIOS - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), SETI Institute, Pontificia Universidad Católica del Perú (PUCP), Institute of Physics [Szczecin], University of Szczecin, Universidad de Alicante, Institut de Ciencies del Cosmos (ICCUB), Universitat de Barcelona (UB), Towson University [Towson, MD, United States], Center for Solar System Studies (CS3), European Southern Observatory (ESO), Czech Science Foundation, Charles University (Czech Republic), Generalitat de Catalunya, Ministerio de Ciencia, Innovación y Universidades (España), National Science Foundation (US), Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Université Nice Sophia Antipolis (1965 - 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), Charles University [Prague] (CU), Université de Genève = University of Geneva (UNIGE), Université Cadi Ayyad [Marrakech] (UCA), Agence Spatiale Européenne = European Space Agency (ESA), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Pontificia Universidad Católica del Perú = Pontifical Catholic University of Peru (PUCP), 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), Tampere University, and Computing Sciences
- Subjects
asteroids ,Solar System ,010504 meteorology & atmospheric sciences ,individual: Sylvia [Asteroids] ,individual: Sylvia [Minor planets, asteroids] ,FOS: Physical sciences ,general [Minor planets, asteroids] ,Astrophysics ,01 natural sciences ,Kuiper belt ,Jupiter ,Interplanetary dust cloud ,Neptune ,Física Aplicada ,0103 physical sciences ,111 Mathematics ,010303 astronomy & astrophysics ,0105 earth and related environmental sciences ,Physics ,Earth and Planetary Astrophysics (astro-ph.EP) ,Nodal precession ,Sylvia ,Minor planets ,Astronomy and Astrophysics ,general [Kuiper belt] ,113 Computer and information sciences ,Asteroids: general ,Meteorite ,115 Astronomy and space science ,13. Climate action ,Space and Planetary Science ,Asteroid ,[SDU]Sciences of the Universe [physics] ,Carbonaceous chondrite ,Minor plantes ,Asteroids: individual: Sylvia ,Kuiper belt: general ,general [Asteroids] ,Astrophysics - Earth and Planetary Astrophysics - Abstract
Carri, B., et al., [Context] Dynamical models of Solar System evolution have suggested that the so-called P- and D-type volatile-rich asteroids formed in the outer Solar System beyond Neptune's orbit and may be genetically related to the Jupiter Trojans, comets, and small Kuiper belt objects (KBOs). Indeed, the spectral properties of P- and D-type asteroids resemble that of anhydrous cometary dust. Aims. We aim to gain insights into the above classes of bodies by characterizing the internal structure of a large P- and D-type asteroid. [Methods] We report high-angular-resolution imaging observations of the P-type asteroid (87) Sylvia with the Very Large Telescope Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE) instrument. These images were used to reconstruct the 3D shape of Sylvia. Our images together with those obtained in the past with large ground-based telescopes were used to study the dynamics of its two satellites. We also modeled Sylvia's thermal evolution. [Results] The shape of Sylvia appears flattened and elongated (a/b 1.45; a/c 1.84). We derive a volume-equivalent diameter of 271 ± 5 km and a low density of 1378 ± 45 kg m-3. The two satellites orbit Sylvia on circular, equatorial orbits. The oblateness of Sylvia should imply a detectable nodal precession which contrasts with the fully-Keplerian dynamics of its two satellites. This reveals an inhomogeneous internal structure, suggesting that Sylvia is differentiated. [Conclusions] Sylvia's low density and differentiated interior can be explained by partial melting and mass redistribution through water percolation. The outer shell should be composed of material similar to interplanetary dust particles (IDPs) and the core should be similar to aqueously altered IDPs or carbonaceous chondrite meteorites such as the Tagish Lake meteorite. Numerical simulations of the thermal evolution of Sylvia show that for a body of such a size, partial melting was unavoidable due to the decay of long-lived radionuclides. In addition, we show that bodies as small as 130-150 km in diameter should have followed a similar thermal evolution, while smaller objects, such as comets and the KBO Arrokoth, must have remained pristine, which is in agreement with in situ observations of these bodies. NASA Lucy mission target (617) Patroclus (diameter ≈140 km) may, however, be differentiated., This work has been supported by the Czech Science Foundation through grants 20-08218S (J. Hanuš, J. Ďurech) and by the Charles University Research program No. UNCE/SCI/023. The work of TSR was carried out through grant APOSTD/2019/046 by Generalitat Valenciana (Spain). This work was supported by the MINECO (Spanish Ministry of Economy) through grant RTI2018-095076-B-C21 (MINECO/FEDER, UE). This material is partially based upon work supported by the National Science Foundation under Grant No. 1743015.
- Published
- 2021
99. Restitution of the K and F Components of the Solar Corona from LASCO-C2 Images over 24 Years [1996--2019]
- Author
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Hugo Gilardy, A. Llebaria, Philippe Lamy, Jean Loirat, Brice Boclet, 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), HELIOS - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), and Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)
- Subjects
010504 meteorology & atmospheric sciences ,K-corona ,Polarimetry ,FOS: Physical sciences ,01 natural sciences ,law.invention ,law ,0103 physical sciences ,010303 astronomy & astrophysics ,Coronagraph ,Solar and Stellar Astrophysics (astro-ph.SR) ,0105 earth and related environmental sciences ,Remote sensing ,Physics ,Sunspot ,Pixel ,[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] ,Stray light ,Astronomy and Astrophysics ,Corona ,Data set ,F-corona ,Astrophysics - Solar and Stellar Astrophysics ,Space and Planetary Science ,Radiance - Abstract
We present a photometrically accurate restitution of the K and F coronae from white-light images obtained over 24 Years [1996--2019] by the Large-Angle Spectrometric COronagraph "LASCO-C2" onboard the Solar and Heliospheric Observatory (SOHO). The procedure starts with the data set coming from the polarimetric separation of images of 512 x 512 pixels in which the F-corona and the instrumental stray light are entangled. Disentangling these components proceeds in three stages, each composed of several steps. Stage 1 establishes the distinct variations of the radiance of these components with the Sun--SOHO distance and generate a new data set of median images calculated for each Carrington rotation. Stage 2 achieves the restitution of a set of 36 stray light images reflecting its temporal variation and the periodic rolls of SOHO which started in 2003. Stage 3 achieves the restitution of the F-corona and a time series of daily images is generated. These results allowed us processing the whole set of routine LASCO-C2 images of 1024 x 1024 pixels (approximately 626000 images) and producing calibrated, high resolution images of the K-corona. We extend our past conclusions that the temporal variation of the integrated radiance of the K-corona tracks the solar activity over two solar cycles 23 and 24 and that it is highly correlated with the temporal variation of the total magnetic field. The behaviours of the integrated radiance during the last few years of the declining phases of solar cycles 23 and 24 are remarkably similar, reaching the same floor level and leading to a duration of 11.0 year for the latter cycle, in agreement with the sunspot determination., 1. Added two new Sections 3.5 and 4.2 discussing uncertainties, with new Figures (21 and 23); results unchanged. 2. Added a comparison with the results of Hayes et al. (2001) in Fig. 24
- Published
- 2020
100. Pervasive chromosomal instability and karyotype order in tumour evolution
- Author
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Lars Dyrskjøt, Andrew Rowan, Priscilla K. Brastianos, Stuart Horswell, Wei-Ting Lu, Gareth A. Wilson, Mickael Escudero, Francesc Castro-Giner, David Allan Moore, Thanos P. Mourikis, Iver Nordentoft, Dhruva Biswas, Katja Harbst, Ian Tomlinson, Fabrice Andre, Lucy R. Yates, Kerstin Haase, Neeltje Steeghs, Michelle Dietzen, Thomas B.K. Watkins, Raymond J. Cho, Hang Xu, Nicholas McGranahan, Boris C. Bastian, Zoltan Szallasi, Fanny Jaulin, Kevin Litchfield, Peter Savas, Marina Petkovic, Franco Caramia, Jonas Demeulemeester, Philippe Lamy, Lavinia Spain, Stefan C. Dentro, Sergi Elizalde, Emilia L. Lim, Lewis Au, Maise Al Bakir, Eva Grönroos, Sally M. Dewhurst, Sherene Loi, Charles Swanton, George D. Cresswell, Mariam Jamal-Hanjani, Samra Turajlic, Göran Jönsson, Nicolai Juul Birkbak, Cecile Vicier, Samuel F. Bakhoum, Vivianne C. G. Tjan-Heijnen, Peter Van Loo, Nicholas M. Luscombe, Peter J. Campbell, Rachel Rosenthal, Roland F. Schwarz, Interne Geneeskunde, MUMC+: MA Medische Oncologie (9), and RS: GROW - R3 - Innovative Cancer Diagnostics & Therapy
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Male ,0301 basic medicine ,Loss of Heterozygosity ,Chromosomes, Human, Pair 11/genetics ,SCNA ,Chromosomal Instability/genetics ,Loss of heterozygosity ,0302 clinical medicine ,Neoplasms ,Chromosome instability ,Pair 11 ,Neoplasm Metastasis ,Neoplasm Metastasis/genetics ,Oncogene Proteins ,Multidisciplinary ,Karyotype ,Neoplasms/genetics ,CANCER ,Clone Cells/metabolism ,Oncogene Proteins/genetics ,030220 oncology & carcinogenesis ,Pair 8 ,Female ,Ploidy ,Human ,Chromosomes, Human, Pair 8 ,EXPRESSION ,GENES ,DNA Copy Number Variations ,Evolution ,General Science & Technology ,Locus (genetics) ,Human leukocyte antigen ,DNA Copy Number Variations/genetics ,Biology ,Chromosomes ,Article ,Evolution, Molecular ,03 medical and health sciences ,Chromosomal Instability ,Cyclin E ,Genetics ,Humans ,IDENTIFICATION ,Loss of Heterozygosity/genetics ,Chromosomes, Human, Pair 11 ,Human Genome ,Molecular ,Chromosome ,Chromosomes, Human, Pair 8/genetics ,Clone Cells ,MODEL ,030104 developmental biology ,Mutagenesis ,METASTASIS ,Cancer research ,PATTERNS ,Cyclin E/genetics - Abstract
Chromosomal instability in cancer consists of dynamic changes to the number and structure of chromosomes(1,2). The resulting diversity in somatic copy number alterations (SCNAs) may provide the variation necessary for tumour evolution(1,3,4). Here we use multi-sample phasing and SCNA analysis of 1,421 samples from 394 tumours across 22 tumour types to show that continuous chromosomal instability results in pervasive SCNA heterogeneity. Parallel evolutionary events, which cause disruption in the same genes (such asBCL9, MCL1,ARNT(also known asHIF1B),TERTandMYC) within separate subclones, were present in 37% of tumours. Most recurrent losses probably occurred before whole-genome doubling, that was found as a clonal event in 49% of tumours. However, loss of heterozygosity at the human leukocyte antigen (HLA) locus and loss of chromosome 8p to a single haploid copy recurred at substantial subclonal frequencies, even in tumours with whole-genome doubling, indicating ongoing karyotype remodelling. Focal amplifications that affected chromosomes 1q21 (which encompassesBCL9, MCL1andARNT), 5p15.33 (TERT), 11q13.3 (CCND1), 19q12 (CCNE1) and 8q24.1 (MYC) were frequently subclonal yet appeared to be clonal within single samples. Analysis of an independent series of 1,024 metastatic samples revealed that 13 focal SCNAs were enriched in metastatic samples, including gains in chromosome 8q24.1 (encompassingMYC) in clear cell renal cell carcinoma and chromosome 11q13.3 (encompassingCCND1) in HER2(+)breast cancer. Chromosomal instability may enable the continuous selection of SCNAs, which are established as ordered events that often occur in parallel, throughout tumour evolution.Chromosomal instability enables the continuous selection of somatic copy number alterations, which are established as ordered events that often occur in parallel, throughout tumour evolution and metastasis.
- Published
- 2020
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