Zobrazeno 1 - 10
of 66
pro vyhledávání: '"Maughan, Ben"'
Autor:
Sereno, Mauro, Maurogordato, Sophie, Cappi, Alberto, Barrena, Rafael, Benoist, Christophe, Haines, Christopher P., Radovich, Mario, Nonino, Mario, Ettori, Stefano, Ferragamo, Antonio, Gavazzi, Raphael, Huot, Sophie, Pizzuti, Lorenzo, Pratt, Gabriel W., Streblyanska, Alina, Zarattini, Stefano, Castignani, Gianluca, Eckert, Dominique, Gastaldello, Fabio, Kay, Scott T., Lovisari, Lorenzo, Maughan, Ben J., Pointecouteau, Etienne, Rasia, Elena, Rossetti, Mariachiara, Sayers, Jack
The Cluster HEritage project with XMM-Newton - Mass Assembly and Thermodynamics at the Endpoint of structure formation (CHEX-MATE) is a programme to study a minimally biased sample of 118 galaxy clusters detected by Planck through the Sunyaev-Zeldovi
Externí odkaz:
http://arxiv.org/abs/2410.18165
Autor:
Potter, Cicely, Tümer, Ayşegül, Wang, Qian H. S., Wik, Daniel R., Maughan, Ben J., Schellenberger, Gerrit
Galaxy clusters are the most recently formed and most massive, gravitationally bound structures in the universe. The number of galaxy clusters formed is highly dependent on cosmological parameters, such as the dark matter density, $\sigma_8$, and $\O
Externí odkaz:
http://arxiv.org/abs/2309.11743
Autor:
Kim, Junhan, Sayers, Jack, Sereno, Mauro, Bartalucci, Iacopo, Chappuis, Loris, De Grandi, Sabrina, De Luca, Federico, De Petris, Marco, Donahue, Megan E., Eckert, Dominique, Ettori, Stefano, Gaspari, Massimo, Gastaldello, Fabio, Gavazzi, Raphael, Gavidia, Adriana, Ghizzardi, Simona, Iqbal, Asif, Kay, Scott, Lovisari, Lorenzo, Maughan, Ben J., Mazzotta, Pasquale, Okabe, Nobuhiro, Pointecouteau, Etienne, Pratt, Gabriel W., Rossetti, Mariachiara, Umetsu, Keiichi
Publikováno v:
A&A 686, A97 (2024)
Galaxy clusters are the products of structure formation through myriad physical processes that affect their growth and evolution throughout cosmic history. As a result, the matter distribution within galaxy clusters, or their shape, is influenced by
Externí odkaz:
http://arxiv.org/abs/2307.04794
Autor:
Bhargava, Sunayana, Garrel, Christian, Koulouridis, Elias, Pierre, Marguerite, Valtchanov, Ivan, Cerardi, Nicolas, Maughan, Ben J., Aguena, Michel, Benoist, Christophe, Baguley, Cale, Ramos-Ceja, Miriam E., Adami, Christophe, Chiappetti, Lucio, Vignali, Cristian, Willis, Jon P.
Publikováno v:
A&A 673, A92 (2023)
X-ray observations of galaxy clusters are impacted by the presence of active galactic nuclei (AGNs) in a manner that is challenging to quantify, leading to biases in the detection and measurement of cluster properties for both astrophysics and cosmol
Externí odkaz:
http://arxiv.org/abs/2301.11196
Autor:
Oppizzi, Filippo, De Luca, Federico, Bourdin, Hervé, Mazzotta, Pasquale, Ettori, Stefano, Gastaldello, Fabio, Kay, Scott, Lovisari, Lorenzo, Maughan, Ben J., Pointecouteau, Etienne, Pratt, Gabriel W., Rossetti, Mariachiara, Sayers, Jack, Sereno, Mauro
Pressure profiles are sensitive probes of the thermodynamic conditions and the internal structure of galaxy clusters. The intra-cluster gas resides in hydrostatic equilibrium within the Dark Matter gravitational potential. However, this equilibrium m
Externí odkaz:
http://arxiv.org/abs/2209.09601
Autor:
Campitiello, Maria Giulia, Ettori, Stefano, Lovisari, Lorenzo, Bartalucci, Iacopo, Eckert, Dominique, Rasia, Elena, Rossetti, Mariachiara, Gastaldello, Fabio, Pratt, Gabriel W., Maughan, Ben, Pointecouteau, Etienne, Sereno, Mauro, Biffi, Veronica, Borgani, Stefano, De Luca, Federico, De Petris, Marco, Gaspari, Massimo, Ghizzardi, Simona, Mazzotta, Pasquale, Molendi, Silvano
Publikováno v:
A&A 665, A117 (2022)
In this work, we performed an analysis of the X-ray morphology of the 118 CHEX-MATE (Cluster HEritage project with XMM-Newton - Mass Assembly and Thermodynamics at the Endpoint of structure formation) galaxy clusters, with the aim to provide a classi
Externí odkaz:
http://arxiv.org/abs/2205.11326
Autor:
Logan, Crispin H. A., Maughan, Ben J., Diaferio, Antonaldo, Duffy, Ryan T., Geller, Margaret J., Rines, Kenneth, Sohn, Jubee
Publikováno v:
A&A 665, A124 (2022)
Clusters of galaxies are powerful probes with which to study cosmology and astrophysics. However, for many applications an accurate measurement of a cluster's mass is essential. A systematic underestimate of hydrostatic masses from X-ray observations
Externí odkaz:
http://arxiv.org/abs/2202.08569
Autor:
Lovisari, Lorenzo, Maughan, Ben J.
X-ray observations of the hot intra-cluster medium (ICM) in galaxy groups and clusters provide quantities such as their gas mass, X-ray luminosity, and temperature. The analysis of the scaling relations between these observable properties gives consi
Externí odkaz:
http://arxiv.org/abs/2202.07673
Autor:
Akino, Daichi, Eckert, Dominique, Okabe, Nobuhiro, Sereno, Mauro, Umetsu, Keiichi, Oguri, Masamune, Gastaldello, Fabio, Chiu, I-Non, Ettori, Stefano, Evrard, August E., Farahi, Arya, Maughan, Ben, Pierre, Marguerite, Ricci, Marina, Valtchanov, Ivan, Mccarthy, Ian, Mcgee, Sean, Miyazaki, Satoshi, Nishizawa, Atsushi J., Tanaka, Masayuki
We present our determination of the baryon budget for an X-ray-selected XXL sample of 136 galaxy groups and clusters spanning nearly two orders of magnitude in mass ($M_{500}\sim 10^{13}-10^{15}M_\odot$) and the redshift range $0< z < 1$. Our joint a
Externí odkaz:
http://arxiv.org/abs/2111.10080
Autor:
Sereno, Mauro, Umetsu, Keiichi, Ettori, Stefano, Eckert, Dominique, Gastaldello, Fabio, Giles, Paul, Lieu, Maggie, Maughan, Ben, Okabe, Nobuhiro, Birkinshaw, Mark, Chiu, I-Non, Fujita, Yutaka, Miyazaki, Satoshi, Rapetti, David, Koulouridis, Elias, Pierre, Marguerite
Scaling relations trace the formation and evolution of galaxy clusters. We exploited multi-wavelength surveys -- the XXL survey at \emph{XMM-Newton} in the X-ray band, and the Hyper Suprime-Cam Subaru Strategic Program for optical weak lensing -- to
Externí odkaz:
http://arxiv.org/abs/1912.02827