Zobrazeno 1 - 10
of 1 970
pro vyhledávání: '"Limousin, P."'
Autor:
Schneider, Benjamin, Prigozhin, Gregory, Foster, Richard F., Bautz, Marshall W., Fu, Hope, Grant, Catherine E., Heine, Sarah, Juneau, Jill, LaMarr, Beverly, Limousin, Olivier, Lourie, Nathan, Malonis, Andrew, Miller, Eric D.
The advent of back-illuminated complementary metal-oxide-semiconductor (CMOS) sensors and their well-known advantages over charge-coupled devices (CCDs) make them an attractive technology for future X-ray missions. However, numerous challenges remain
Externí odkaz:
http://arxiv.org/abs/2409.05954
Autor:
Limousin, M., Niemiec, A., Beauchesne, B., Diego, J., Jauzac, M., Sharon, K., Acebron, A., Lagattuta, D., Mahler, G., Williams, L., Richard, J., Jullo, E., Furtak, L., Faisst, A., Frye, B., Hibon, P., Natarajan, P., Rich, M.
Parametric strong lensing studies of galaxy clusters often display "misleading features". This is the case in the galaxy cluster Abell 370. Using strong lensing techniques, it has been described parametrically by a four dark matter clumps model and g
Externí odkaz:
http://arxiv.org/abs/2409.04584
Autor:
Patel, Nency R., Jauzac, Mathilde, Niemiec, Anna, Lagattuta, David, Mahler, Guillaume, Beauchesne, Benjamin, Edge, Alastair, Ebeling, Harald, Limousin, Marceau
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 533, Issue 4, October 2024, Pages 4500-4514
We present a combined strong and weak gravitational-lensing analysis of the massive galaxy cluster MACS J1423.8+2404 ($z=0.545$, MACS J1423 hereafter), one of the most dynamically relaxed and massive cool-core clusters discovered in the MAssive Clust
Externí odkaz:
http://arxiv.org/abs/2405.04577
Autor:
Furtak, Lukas J., Zitrin, Adi, Richard, Johan P., Eckert, Dominique, Sayers, Jack, Ebeling, Harald, Fujimoto, Seiji, Laporte, Nicolas, Lagattuta, David, Limousin, Marceau, Mahler, Guillaume, Meena, Ashish K., Andrade-Santos, Felipe, Frye, Brenda L., Jauzac, Mathilde, Koekemoer, Anton M., Kohno, Kotaro, Espada, Daniel, Lu, Harry, Massey, Richard, Niemiec, Anna
MACS J0600.1-2008 (MACS0600) is an X-ray luminous, massive galaxy cluster at $z_{\mathrm{d}}=0.43$, studied previously by the REionization LensIng Cluster Survey (RELICS) and ALMA Lensing Cluster Survey (ALCS) projects which revealed a complex, bimod
Externí odkaz:
http://arxiv.org/abs/2404.03286
Autor:
Collier, Hannah, Limousin, Olivier, Xiao, Hualin, Claret, Arnaud, Schuller, Frederic, Dresing, Nina, Valkila, Saku, Lara, Francisco Espinosa, Fedeli, Annamaria, Foucambert, Simon, Krucker, Säm
The Spectrometer/Telescope for Imaging X-rays (STIX) is a hard X-ray imaging spectrometer on board the ESA and NASA heliospheric mission Solar Orbiter. STIX has been operational for three years and has observed X-ray emission from ~35,000 solar flare
Externí odkaz:
http://arxiv.org/abs/2402.03816
Autor:
Ferro, Lisa, Virgilli, Enrico, Moita, Miguel, Frontera, Filippo, Rosati, Piero, Guidorzi, Cristiano, Ferrari, Claudio, Lolli, Riccardo, Caroli, Ezio, Auricchio, Natalia, Stephen, John B., Del Sordo, Stefano, Gargano, Carmelo, Squerzanti, Stefano, Pucci, Mauro, Limousin, Olivier, Meuris, Aline, Laurent, Philippe, Allaire, Hugo
Publikováno v:
Proceedings Volume 12181, Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray; 121812K (2022)
Hard X-/soft Gamma-ray astronomy (> 100 keV) is a crucial field for the study of important astrophysical phenomena such as the 511 keV positron annihilation line in the Galactic center region and its origin, gamma-ray bursts, soft gamma-ray repeaters
Externí odkaz:
http://arxiv.org/abs/2309.11187
Autor:
Jean-Baptiste Ducloyer, Alexandra Poinas, Léa Duchesne, Pascal Caillet, Corinne Lejus-Bourdeau, Guylène Le Meur, Michel Weber, Catherine Ivan, Nadège Limousin, Thomas Desmidt, Patrick Pladys, Pierre-Jean Pisella, Anne Bernard, Hubert Lardy, Philippe Gohier, Ludovic Martin, Frédéric Mouriaux, Pierre Lebranchu, Raoul Kanav Khanna, E3CAPS group
Publikováno v:
BMC Medical Education, Vol 24, Iss 1, Pp 1-10 (2024)
Abstract Introduction Training novice ophthalmology residents on the EyeSi® simulator increases cataract surgery safety. However, there is no consensus regarding how much training residents should perform before their first time on patients. We eval
Externí odkaz:
https://doaj.org/article/394aab4aa07f4761b5f5bad2443d9060
Autor:
Niemiec, Anna, Jauzac, Mathilde, Eckert, Dominique, Lagattuta, David, Sharon, Keren, Koekemoer, Anton M., Umetsu, Keiichi, Acebron, Ana, Diego, Jose M., Harvey, David, Jullo, Eric, Kokorev, Vasily, Limousin, Marceau, Mahler, Guillaume, Natarajan, Priyamvada, Nonino, Mario, Remolina, Juan D., Steinhardt, Charles, Tam, Sut-Ieng, Zitrin, Adi
The HST treasury program BUFFALO provides extended wide-field imaging of the six Hubble Frontier Fields galaxy clusters. Here we present the combined strong and weak-lensing analysis of Abell 370, a massive cluster at z=0.375. From the reconstructed
Externí odkaz:
http://arxiv.org/abs/2307.03778
Autor:
Diego, Jose M., Li, Sung Kei, Meena, Ashish K., Niemiec, Anna, Acebron, Ana, Jauzac, Mathilde, Struble, Mitchell F., Amruth, Alfred, Broadhurst, Tom J., Cerny, Catherine, Ebeling, Harald, Filippenko, Alexei V., Jullo, Eric, Kelly, Patrick, Koekemoer, Anton M., Lagatutta, David, Lim, Jeremy, Limousin, Marceau, Mahler, Guillaume, Patel, Nency, Remolina, Juan, Richard, Johan, Sharon, Keren, Steinhardt, Charles, Umetsu, Keichii, Williams, Liliya, Zitrin, Adi, Palencia, J. M., Ji, Liang Dai. Lingyuan, Pascale, Massimo
We present a constraint on the abundance of supergiant (SG) stars at redshift z approx. 1, based on recent observations of a strongly lensed arc at this redshift. First we derive a free-form model of MACS J0416.1-2403 using data from the BUFFALO prog
Externí odkaz:
http://arxiv.org/abs/2304.09222
Autor:
Xiao, Hualin, Maloney, Shane, Krucker, Säm, Dickson, Ewan, Massa, Paolo, Lastufka, Erica, Battaglia, Andrea Francesco, Etesi, Laszlo, Hochmuth, Nicky, Schuller, Frederic, Ryan, Daniel F., Limousin, Olivier, Collier, Hannah, Warmuth, Alexander, Piana, Michele
Publikováno v:
A&A 673, A142 (2023)
The Spectrometer and Telescope for Imaging X-rays (STIX) on board Solar Orbiter observes solar X-ray emission in the range of 4 – 150 keV and produces spectra and images of solar flares over a wide range of flare magnitudes. During nominal operatio
Externí odkaz:
http://arxiv.org/abs/2302.00497