Zobrazeno 1 - 10
of 292
pro vyhledávání: '"Plaszczynski, Stéphane"'
The analysis of social networks, in particular those describing face-to-face interactions between individuals, is complex due to the intertwining of the topological and temporal aspects. We revisit them both, using public data recorded by the sociopa
Externí odkaz:
http://arxiv.org/abs/2402.03333
We compare face-to-face interaction data recorded by wearable sensors in various sociological environments. The interactions among individuals display a clear environment-dependent diversity in agreement with previous analyses. The contact durations
Externí odkaz:
http://arxiv.org/abs/2212.06673
Autor:
Plaszczynski, Stephane, Grammaticos, Basile, Pallud, Johan, Campagne, Jean-Eric, Badoual, Mathilde
Diffuse low grade gliomas are invasive and incurable brain tumours that inevitably transform into higher grade ones. A classical treatment to delay this transition is radiotherapy (RT). Following RT, the tumour gradually shrinks during a period of ty
Externí odkaz:
http://arxiv.org/abs/2206.07401
Diffuse low grade gliomas are slowly growing tumors that always recur after treatment. In this paper, we revisit the modeling of the tumor radius evolution before and after the radiotherapy process and propose a novel model that is simple, yet biolog
Externí odkaz:
http://arxiv.org/abs/2107.02534
Autor:
LSST Dark Energy Science Collaboration, Abolfathi, Bela, Armstrong, Robert, Awan, Humna, Babuji, Yadu N., Bauer, Franz Erik, Beckett, George, Biswas, Rahul, Bogart, Joanne R., Boutigny, Dominique, Chard, Kyle, Chiang, James, Cohen-Tanugi, Johann, Connolly, Andrew J., Daniel, Scott F., Digel, Seth W., Drlica-Wagner, Alex, Dubois, Richard, Gawiser, Eric, Glanzman, Thomas, Habib, Salman, Hearin, Andrew P., Heitmann, Katrin, Hernandez, Fabio, Hložek, Renée, Hollowed, Joseph, Jarvis, Mike, Jha, Saurabh W., Kalmbach, J. Bryce, Kelly, Heather M., Kovacs, Eve, Korytov, Danila, Krughoff, K. Simon, Lage, Craig S., Lanusse, François, Larsen, Patricia, Li, Nan, Longley, Emily Phillips, Lupton, Robert H., Mandelbaum, Rachel, Mao, Yao-Yuan, Marshall, Phil, Meyers, Joshua E., Park, Ji Won, Peloton, Julien, Perrefort, Daniel, Perry, James, Plaszczynski, Stéphane, Pope, Adrian, Rykoff, Eli S., Sánchez, F. Javier, Schmidt, Samuel J., Uram, Thomas D., Villarreal, Antonia, Walter, Christopher W., Wiesner, Matthew P., Wood-Vasey, W. Michael
In preparation for cosmological analyses of the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST), the LSST Dark Energy Science Collaboration (LSST DESC) has created a 300 deg$^2$ simulated survey as part of an effort called Data Chall
Externí odkaz:
http://arxiv.org/abs/2101.04855
Autor:
LSST Dark Energy Science Collaboration, Abolfathi, Bela, Alonso, David, Armstrong, Robert, Aubourg, Éric, Awan, Humna, Babuji, Yadu N., Bauer, Franz Erik, Bean, Rachel, Beckett, George, Biswas, Rahul, Bogart, Joanne R., Boutigny, Dominique, Chard, Kyle, Chiang, James, Claver, Chuck F., Cohen-Tanugi, Johann, Combet, Céline, Connolly, Andrew J., Daniel, Scott F., Digel, Seth W., Drlica-Wagner, Alex, Dubois, Richard, Gangler, Emmanuel, Gawiser, Eric, Glanzman, Thomas, Gris, Phillipe, Habib, Salman, Hearin, Andrew P., Heitmann, Katrin, Hernandez, Fabio, Hložek, Renée, Hollowed, Joseph, Ishak, Mustapha, Ivezić, Željko, Jarvis, Mike, Jha, Saurabh W., Kahn, Steven M., Kalmbach, J. Bryce, Kelly, Heather M., Kovacs, Eve, Korytov, Danila, Krughoff, K. Simon, Lage, Craig S., Lanusse, François, Larsen, Patricia, Guillou, Laurent Le, Li, Nan, Longley, Emily Phillips, Lupton, Robert H., Mandelbaum, Rachel, Mao, Yao-Yuan, Marshall, Phil, Meyers, Joshua E., Moniez, Marc, Morrison, Christopher B., Nomerotski, Andrei, O'Connor, Paul, Park, HyeYun, Park, Ji Won, Peloton, Julien, Perrefort, Daniel, Perry, James, Plaszczynski, Stéphane, Pope, Adrian, Rasmussen, Andrew, Reil, Kevin, Roodman, Aaron J., Rykoff, Eli S., Sánchez, F. Javier, Schmidt, Samuel J., Scolnic, Daniel, Stubbs, Christopher W., Tyson, J. Anthony, Uram, Thomas D., Villarreal, Antonia, Walter, Christopher W., Wiesner, Matthew P., Wood-Vasey, W. Michael, Zuntz, Joe
We describe the simulated sky survey underlying the second data challenge (DC2) carried out in preparation for analysis of the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) by the LSST Dark Energy Science Collaboration (LSST DESC).
Externí odkaz:
http://arxiv.org/abs/2010.05926
Autor:
Möller, Anais, Peloton, Julien, Ishida, Emille E. O., Arnault, Chris, Bachelet, Etienne, Blaineau, Tristan, Boutigny, Dominique, Chauhan, Abhishek, Gangler, Emmanuel, Hernandez, Fabio, Hrivnac, Julius, Leoni, Marco, Leroy, Nicolas, Moniez, Marc, Pateyron, Sacha, Ramparison, Adrien, Turpin, Damien, Ansari, Réza, Allam Jr., Tarek, Bajat, Armelle, Biswas, Biswajit, Boucaud, Alexandre, Bregeon, Johan, Campagne, Jean-Eric, Cohen-Tanugi, Johann, Coleiro, Alexis, Dornic, Damien, Fouchez, Dominique, Godet, Olivier, Gris, Philippe, Karpov, Sergey, Gomez-Moran, Ada Nebot, Neveu, Jérémy, Plaszczynski, Stephane, Savchenko, Volodymyr, Webb, Natalie
Fink is a broker designed to enable science with large time-domain alert streams such as the one from the upcoming Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST). It exhibits traditional astronomy broker features such as automatised
Externí odkaz:
http://arxiv.org/abs/2009.10185
Publikováno v:
A&A 633, A26 (2020)
We revisit the case of fast Monte-Carlo simulations of galaxy positions for a non-gaussian field. More precisely we address the question of generating a 3D field with a given one-point function (as a log-normal one, but not only) and some power-spect
Externí odkaz:
http://arxiv.org/abs/1906.09042
Autor:
Ansari, Reza, Choyer, Adeline, Habibi, Farhang, Magneville, Christophe, Moniez, Marc, Plaszczynski, Stéphane, Renault, Cécile, Ricol, Jean-Stéphane, Souchard, Julien
Publikováno v:
A&A 623, A76 (2019)
Imaging billions of galaxies every few nights during ten years, LSST should be a major contributor to precision cosmology in the 2020 decade. High precision photometric data will be available in six bands, from near-infrared to near-ultraviolet. The
Externí odkaz:
http://arxiv.org/abs/1902.03004
Autor:
Chisari, Nora Elisa, Alonso, David, Krause, Elisabeth, Leonard, C. Danielle, Bull, Philip, Neveu, Jérémy, Villarreal, Antonia, Singh, Sukhdeep, McClintock, Thomas, Ellison, John, Du, Zilong, Zuntz, Joe, Mead, Alexander, Joudaki, Shahab, Lorenz, Christiane S., Troester, Tilman, Sanchez, Javier, Lanusse, Francois, Ishak, Mustapha, Hlozek, Renée, Blazek, Jonathan, Campagne, Jean-Eric, Almoubayyed, Husni, Eifler, Tim, Kirby, Matthew, Kirkby, David, Plaszczynski, Stéphane, Slosar, Anze, Vrastil, Michal, Wagoner, Erika L.
The Core Cosmology Library (CCL) provides routines to compute basic cosmological observables to a high degree of accuracy, which have been verified with an extensive suite of validation tests. Predictions are provided for many cosmological quantities
Externí odkaz:
http://arxiv.org/abs/1812.05995