Zobrazeno 1 - 10
of 256
pro vyhledávání: '"Boehm, Céline"'
Autor:
Jalan, Priyanka, Negi, Vibhore, Surdej, Jean, Boehm, Céline, Delchambre, Ludovic, Brok, Jakob Sebastian den, Dobie, Dougal, Drake, Andrew, Ducourant, Christine, Djorgovski, S. George, Galluccio, Laurent, Graham, Matthew J., Klüter, Jonas, Krone-Martins, Alberto, LeCampion, Jean-François, Mahabal, Ashish A., Mignard, François, Murphy, Tara, Nierenberg, Anna, Scarano, Sergio, Simon, Joseph, Slezak, Eric, Sluse, Dominique, Spíndola-Duarte, Carolina, Stern, Daniel, Teixera, Ramachrisna, Wambsganss, Joachim
Gravitational lensing is proven to be one of the most efficient tools for studying the Universe. The spectral confirmation of such sources requires extensive calibration. This paper discusses the spectral extraction technique for the case of multiple
Externí odkaz:
http://arxiv.org/abs/2312.08217
Autor:
Allingham, Joseph F. V., Bœhm, Céline, Eckert, Dominique, Jauzac, Mathilde, Lagattuta, David J., Mahler, Guillaume, Hilton, Matt, Lewis, Geraint F., Ettori, Stefano
Publikováno v:
MNRAS, 528, 1711 (2024)
Whilst X-rays and Sunyaev-Zel'dovich observations allow to study the properties of the intra-cluster medium (ICM) of galaxy clusters, their gravitational potential may be constrained using strong gravitational lensing. Although being physically relat
Externí odkaz:
http://arxiv.org/abs/2309.07076
Autor:
Kawata, Daisuke, Kawahara, Hajime, Gouda, Naoteru, Secrest, Nathan J., Kano, Ryouhei, Kataza, Hirokazu, Isobe, Naoki, Ohsawa, Ryou, Usui, Fumihiko, Yamada, Yoshiyuki, Graham, Alister W., Pettitt, Alex R., Asada, Hideki, Baba, Junichi, Bekki, Kenji, Dorland, Bryan N., Fujii, Michiko, Fukui, Akihiko, Hattori, Kohei, Hirano, Teruyuki, Kamizuka, Takafumi, Kashima, Shingo, Kawanaka, Norita, Kawashima, Yui, Klioner, Sergei A., Kodama, Takanori, Koshimoto, Naoki, Kotani, Takayuki, Kuzuhara, Masayuki, Levine, Stephen E., Majewski, Steven R., Masuda, Kento, Matsunaga, Noriyuki, Miyakawa, Kohei, Miyoshi, Makoko, Morihana, Kumiko, Nishi, Ryoichi, Notsu, Yuta, Omiya, Masashi, Sanders, Jason, Tanikawa, Ataru, Tsujimoto, Masahiro, Yano, Taihei, Aizawa, Masataka, Arimatsu, Ko, Biermann, Michael, Boehm, Celine, Chiba, Masashi, Debattista, Victor P., Gerhard, Ortwin, Hirabayashi, Masayuki, Hobbs, David, Ikenoue, Bungo, Izumiura, Hideyuki, Jordi, Carme, Kohara, Naoki, Löffler, Wolfgang, Luri, Xavier, Mase, Ichiro, Miglio, Andrea, Mitsuda, Kazuhisa, Newswander, Trent, Nishiyama, Shogo, Obuchi, Yoshiyuki, Ootsubo, Takafumi, Ouchi, Masami, Ozaki, Masanobu, Perryman, Michael, Prusti, Timo, Ramos, Pau, Read, Justin I., Rich, R. Michael, Schönrich, Ralph, Shikauchi, Minori, Shimizu, Risa, Suematsu, Yoshinori, Tada, Shotaro, Takahashi, Aoi, Tatekawa, Takayuki, Tatsumi, Daisuke, Tsujimoto, Takuji, Tsuzuki, Toshihiro, Urakawa, Seitaro, Uraguchi, Fumihiro, Utsunomiya, Shin, Van Eylen, Vincent, van Leeuwen, Floor, Wada, Takehiko, Walton, Nicholas A.
Japan Astrometry Satellite Mission for INfrared Exploration (JASMINE) is a planned M-class science space mission by the Institute of Space and Astronautical Science, the Japan Aerospace Exploration Agency. JASMINE has two main science goals. One is t
Externí odkaz:
http://arxiv.org/abs/2307.05666
A growing number of Milky Way globular clusters have been identified to possess a noticeable degree of solid-body rotation. For several clusters, the combination of stellar proper motions and radial velocities allows for 3-dimensional spin axes to be
Externí odkaz:
http://arxiv.org/abs/2306.11276
There have been many efforts in the last three decades to embed the empirical MOND program into a robust theoretical framework. While many such theories can explain the profile of galactic rotation curves, they usually cannot explain the evolution 15
Externí odkaz:
http://arxiv.org/abs/2304.05134
Autor:
Mosbech, Markus R., Jenkins, Alexander C., Bose, Sownak, Boehm, Celine, Sakellariadou, Mairi, Wong, Yvonne Y. Y.
We show that gravitational waves have the potential to unravel the microphysical properties of dark matter due to the dependence of the binary black hole merger rate on cosmic structure formation, which is itself highly dependent on the dark matter s
Externí odkaz:
http://arxiv.org/abs/2207.14126
A change in the mass of the Galaxy with time will leave its imprint on the motions of the stars, with stars having radially outward (mass loss) or inward (mass accretion) bulk motions. Here we test the feasibility of using the mean radial motion of s
Externí odkaz:
http://arxiv.org/abs/2207.11739
Autor:
Allingham, Joseph F. V., Jauzac, Mathilde, Lagattuta, David J., Mahler, Guillaume, Bœhm, Céline, Lewis, Geraint F., Eckert, Dominique, Edge, Alastair, Ettori, Stefano
Publikováno v:
MNRAS, 522, 1118-1137 (2023)
We present the strong lensing analysis of two galaxy clusters: MACS J0242.5-2132 (MACS J0242, $z=0.313$) and MACS J0949.8+1708 (MACS J0949, $z=0.383$). Their total matter distributions are constrained thanks to the powerful combination of observation
Externí odkaz:
http://arxiv.org/abs/2207.10520
Similarly to warm dark matter which features a cut-off in the matter power spectrum due to free-streaming, many interacting dark matter models predict a suppression of the matter power spectrum on small length scales through collisional damping. Fore
Externí odkaz:
http://arxiv.org/abs/2207.03107
For several decades, astronomers have measured the electromagnetic emission in the universe from the lowest to the highest energies with incredible precision. The lowest end of the spectrum, corresponding to radio waves, is fairly well studied and un
Externí odkaz:
http://arxiv.org/abs/2204.13711