Zobrazeno 1 - 10
of 179
pro vyhledávání: '"CLUSTERS: INTRACLUSTER MEDIUM [GALAXIES]"'
Publikováno v:
Towler, I, Kay, S T & Altamura, E 2023, ' Gas clumping and its effect on hydrostatic bias in the MACSIS simulations ', Monthly Notices of the Royal Astronomical Society, vol. 520, no. 4, pp. 5845–5857 . https://doi.org/10.1093/mnras/stad453
We use the MACSIS hydrodynamical simulations to estimate the extent of gas clumping in the intracluster medium of massive galaxy clusters and how it affects the hydrostatic mass bias. By comparing the clumping to the azimuthal scatter in the emission
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e05562546fd268f755ec549e076f2b81
https://doi.org/10.1093/mnras/stad453
https://doi.org/10.1093/mnras/stad453
Autor:
D J Turner, P A Giles, A K Romer, R Wilkinson, E W Upsdell, M Klein, P T P Viana, M Hilton, S Bhargava, C A Collins, R G Mann, M Sahlén, J P Stott
Publikováno v:
Turner, D J, Giles, P A, Romer, A K, Wilkinson, R, Upsdell, E W, Klein, M, Viana, P T P, Hilton, M, Bhargava, S, Collins, C A, Mann, R G, Sahlén, M & Stott, J P 2022, ' The XMM Cluster Survey: An independent demonstration of the fidelity of the eFEDS galaxy cluster data products and implications for future studies ', Monthly Notices of the Royal Astronomical Society, vol. 517, no. 1, pp. 657-674 . https://doi.org/10.1093/mnras/stac2463
We present the first comparison between properties of clusters of galaxies detected by the eROSITA Final Equatorial-Depth Survey (eFEDS) and the XMM Cluster Survey (XCS). We have compared, in an ensemble fashion, properties from the eFEDS X-ray clust
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::01f95d98c5f0be819d4baccf12a95201
https://doi.org/10.1093/mnras/stac2463
https://doi.org/10.1093/mnras/stac2463
Autor:
Daichi Akino, Dominique Eckert, Nobuhiro Okabe, Mauro Sereno, Keiichi Umetsu, Masamune Oguri, Fabio Gastaldello, I-Non Chiu, Stefano Ettori, August E Evrard, Arya Farahi, Ben Maughan, Marguerite Pierre, Marina Ricci, Ivan Valtchanov, Ian McCarthy, Sean McGee, Satoshi Miyazaki, Atsushi J Nishizawa, Masayuki Tanaka
Publikováno v:
Publ.Astron.Soc.Jap.
Publ.Astron.Soc.Jap., 2022, 74 (1), pp.175-208-208. ⟨10.1093/pasj/psab115⟩
Akino, D, Eckert, D, Okabe, N, Sereno, M, Umetsu, K, Oguri, M, Gastaldello, F, Chiu, I-N, Ettori, S, Evrard, A E, Farahi, A, Maughan, B, Pierre, M, Ricci, M, Valtchanov, I, Mccarthy, I, Mcgee, S, Miyazaki, S, Nishizawa, A J & Tanak, M 2022, ' HSC-XXL : Baryon budget of the 136 XXL Groups and Clusters ', Publications of the Astronomical Society of japan, vol. 74, no. 1, pp. 175–208 . https://doi.org/10.1093/pasj/psab115
Publ.Astron.Soc.Jap., 2022, 74 (1), pp.175-208-208. ⟨10.1093/pasj/psab115⟩
Akino, D, Eckert, D, Okabe, N, Sereno, M, Umetsu, K, Oguri, M, Gastaldello, F, Chiu, I-N, Ettori, S, Evrard, A E, Farahi, A, Maughan, B, Pierre, M, Ricci, M, Valtchanov, I, Mccarthy, I, Mcgee, S, Miyazaki, S, Nishizawa, A J & Tanak, M 2022, ' HSC-XXL : Baryon budget of the 136 XXL Groups and Clusters ', Publications of the Astronomical Society of japan, vol. 74, no. 1, pp. 175–208 . https://doi.org/10.1093/pasj/psab115
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a62d1144ac2f8b8d39dafc1da6aecb88
https://doi.org/10.1093/pasj/psab115
https://doi.org/10.1093/pasj/psab115
Autor:
S. Mascia, L. Pentericci, A. Calabrò, T. Treu, P. Santini, L. Yang, L. Napolitano, G. Roberts-Borsani, P. Bergamini, C. Grillo, P. Rosati, B. Vulcani, M. Castellano, K. Boyett, A. Fontana, K. Glazebrook, A. Henry, C. Mason, E. Merlin, T. Morishita, T. Nanayakkara, D. Paris, N. Roy, H. Williams, X. Wang, G. Brammer, M. Bradač, W. Chen, P. L. Kelly, A. M. Koekemoer, M. Trenti, R. A. Windhorst
Publikováno v:
Mascia, S, Pentericci, L, Calabro, A, Treu, T, Santini, P, Yang, L, Napolitano, L, Roberts-Borsani, G, Bergamini, P, Grillo, C, Rosati, P, Vulcani, B, Castellano, M, Boyett, K, Fontana, A, Glazebrook, K, Henry, A, Mason, C, Merlin, E, Morishita, T, Nanayakkara, T, Paris, D, Roy, N, Williams, H, Wang, X, Brammer, G, Bradac, M, Chen, W, Kelly, P L, Koekemoer, A M, Trenti, M & Windhorst, R A 2023, ' Closing in on the sources of cosmic reionization : First results from the GLASS-JWST program ', Astronomy & Astrophysics, vol. 672, A155 . https://doi.org/10.1051/0004-6361/202345866
The escape fraction of Lyman-continuum (LyC) photons ($f_{esc}$) is a key parameter for determining the sources of cosmic reionization at $z\geq 6$. At these redshifts, owing to the opacity of the intergalactic medium, the LyC emission cannot be meas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5546ecf571e515a6d71aeb38842e4b06
Autor:
Weiguang Cui, Romeel Dave, Alexander Knebe, Elena Rasia, Meghan Gray, Frazer Pearce, Chris Power, Gustavo Yepes, Dhayaa Anbajagane, Daniel Ceverino, Ana Contreras-Santos, Daniel de Andres, Marco De Petris, Stefano Ettori, Roan Haggar, Qingyang Li, Yang Wang, Xiaohu Yang, Stefano Borgani, Klaus Dolag, Ying Zu, Ulrike Kuchner, Rodrigo Cañas, Antonio Ferragamo, Giulia Gianfagna
Publikováno v:
Cui, W, Dave, R, Knebe, A, Rasia, E, Gray, M, Pearce, F, Power, C, Yepes, G, Anbajagane, D, Ceverino, D, Contreras-Santos, A, Andres, D D, Petris, M D, Ettori, S, Haggar, R, Li, Q, Wang, Y, Yang, X, Borgani, S, Dolag, K, Zu, Y, Kuchner, U, Cañas, R, Ferragamo, A & Gianfagna, G 2022, ' The Three Hundred project: The gizmo-simba run ', Monthly Notices of the Royal Astronomical Society, vol. 514, no. 1, pp. 977-996 . https://doi.org/10.1093/mnras/stac1402
Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM
We introduce gizmo-simba, a new suite of galaxy c
We introduce gizmo-simba, a new suite of galaxy c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5724c2eacac0a8096cd45fae83a89c39
https://doi.org/10.1093/mnras/stac1402
https://doi.org/10.1093/mnras/stac1402
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 494, 4, pp. 5207-5229
Monthly Notices of the Royal Astronomical Society, 494, 5207-5229
Musoke, G, Young, A J, Molnar, S M & Birkinshaw, M 2020, ' Numerical simulations of colliding jets in an external wind : application to 3C 75 ', Monthly Notices of the Royal Astronomical Society, vol. 494, no. 4, staa1071, pp. 5207-5229 . https://doi.org/10.1093/mnras/staa1071
Monthly Notices of the Royal Astronomical Society, 494(4), 5207-5229. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 494, 5207-5229
Musoke, G, Young, A J, Molnar, S M & Birkinshaw, M 2020, ' Numerical simulations of colliding jets in an external wind : application to 3C 75 ', Monthly Notices of the Royal Astronomical Society, vol. 494, no. 4, staa1071, pp. 5207-5229 . https://doi.org/10.1093/mnras/staa1071
Monthly Notices of the Royal Astronomical Society, 494(4), 5207-5229. Oxford University Press
The radio galaxy 3C 75 is remarkable because it contains a pair of radio-loud active galaxies, each of which produces a two-sided jet, with the jet beams appearing to collide and merge to the west of the galaxies. Motivated by 3C 75, we have conducte
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ffd21a7eed372f2cf3bfc52b71e5d4bd
https://doi.org/10.1093/mnras/staa1071
https://doi.org/10.1093/mnras/staa1071
Autor:
Weiguang Cui, Qingyang Li, E. Rasia, Romeel Davé, Marco De Petris, Frazer R. Pearce, Gustavo Yepes, John A. Peacock, Xiaohu Yang, Alexander Knebe
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Li, Q, Cui, W, Yang, X, Rasia, E, Dave, R, Petris, M D, Knebe, A, Peacock, J A, Pearce, F & Yepes, G 2020, ' The Three Hundred Project: the stellar and gas profiles ', Monthly Notices of the Royal Astronomical Society, vol. 495, no. 3, pp. 2930-2948 . https://doi.org/10.1093/mnras/staa1385
Li, Q, Cui, W, Yang, X, Rasia, E, Dave, R, Petris, M D, Knebe, A, Peacock, J A, Pearce, F & Yepes, G 2020, ' The Three Hundred Project: the stellar and gas profiles ', Monthly Notices of the Royal Astronomical Society, vol. 495, no. 3, pp. 2930-2948 . https://doi.org/10.1093/mnras/staa1385
Using the catalogues of galaxy clusters from The Three Hundred project, modelled with both hydrodynamic simulations, (Gadget-X and Gadget-MUSIC), and semi-analytic models (SAMs), we study the scatter and self-similarity of the profiles and distributi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6cf168713747e6e3593068100e0d5ce6
https://doi.org/10.1093/mnras/staa1385
https://doi.org/10.1093/mnras/staa1385
Autor:
Vacca, Valentina, Shimwell, Timothy, Perley, Richard A, Govoni, Federica, Murgia, Matteo, Feretti, Luigina, Giovannini, Gabriele, Loi, Francesca, Carretti, Ettore, Cova, Filippo, Gastaldello, Fabio, Girardi, Marisa, Enßlin, Torsten, Akamatsu, Hiroki, Bonafede, Annalisa, Bonnassieux, Etienne, Boschin, Walter, Botteon, Andrea, Brunetti, Gianfranco, Brüggen, Marcus, Finoguenov, Alexis, Hoang, Duy, Iacobelli, Marco, Orrú, Emanuela, Paladino, Rosita, Röttgering, Huub, van , Weeren, Reinout, Vitello, Fabio, Wittor, Denis
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 511(3), 3389-3407
The galaxy cluster Abell 523 (A523) hosts an extended diffuse synchrotron source historically classified as a radio halo. Its radio power at 1.4 GHz makes it one of the most significant outliers in the scaling relations between observables derived fr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8761d715b89bd40614637354a3978052
https://hdl.handle.net/11368/3024301
https://hdl.handle.net/11368/3024301
Autor:
P. Tozzi, R. Gilli, A. Liu, S. Borgani, M. Lepore, L. Di Mascolo, A. Saro, L. Pentericci, C. Carilli, G. Miley, T. Mroczkowski, M. Pannella, E. Rasia, P. Rosati, C. S. Anderson, A. Calabró, E. Churazov, H. Dannerbauer, C. Feruglio, F. Fiore, R. Gobat, S. Jin, M. Nonino, C. Norman, H. J. A. Röttgering
Publikováno v:
Tozzi, P, Gilli, R, Liu, A, Borgani, S, Lepore, M, Di Mascolo, L, Saro, A, Pentericci, L, Carilli, C, Miley, G, Mroczkowski, T, Pannella, M, Rasia, E, Rosati, P, Anderson, C S, Calabro, A, Churazov, E, Dannerbauer, H, Feruglio, C, Fiore, F, Gobat, R, Jin, S, Nonino, M, Norman, C & Rottgering, H J A 2022, ' The 700 ks Chandra Spiderweb Field : II. Evidence for inverse-Compton and thermal diffuse emission in the Spiderweb galaxy ', Astronomy and Astrophysics, vol. 667, A134 . https://doi.org/10.1051/0004-6361/202244337
Astronomy & Astrophysics, 667:A134
Astronomy & Astrophysics, 667:A134
We present the X-ray imaging and spectral analysis of the diffuse emission around the Spiderweb galaxy at z=2.16 and of its nuclear emission, based on a deep (700 ks) Chandra observation. We characterize the nuclear emission and computed the contamin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7e2bd7312d99dca95a1e5d2361305799
https://orbit.dtu.dk/en/publications/f9a76617-8bd6-4b67-8926-3e105772dbaf
https://orbit.dtu.dk/en/publications/f9a76617-8bd6-4b67-8926-3e105772dbaf
Autor:
D Anbajagane, C Chang, B Jain, S Adhikari, E J Baxter, B A Benson, L E Bleem, S Bocquet, M S Calzadilla, J E Carlstrom, C L Chang, R Chown, T M Crawford, A T Crites, W Cui, T de Haan, L Di Mascolo, M A Dobbs, W B Everett, E M George, S Grandis, N W Halverson, G P Holder, W L Holzapfel, J D Hrubes, A T Lee, D Luong-Van, M A McDonald, J J McMahon, S S Meyer, M Millea, L M Mocanu, J J Mohr, T Natoli, Y Omori, S Padin, C Pryke, C L Reichardt, J E Ruhl, A Saro, K K Schaffer, E Shirokoff, Z Staniszewski, A A Stark, J D Vieira, R Williamson
Publikováno v:
Anbajagane, D, Chang, C, Jain, B, Adhikari, S, Baxter, E J, Benson, B A, Bleem, L E, Bocquet, S, Calzadilla, M S, Carlstrom, J E, Chang, C L, Chown, R, Crawford, T M, Crites, A T, Cui, W, Haan, T D, Mascolo, L D, Dobbs, M A, Everett, W B, George, E M, Grandis, S, Halverson, N W, Holder, G P, Holzapfel, W L, Hrubes, J D, Lee, A T, Luong-Van, D, McDonald, M A, McMahon, J J, Meyer, S S, Millea, M, Mocanu, L M, Mohr, J J, Natoli, T, Omori, Y, Padin, S, Pryke, C, Reichardt, C L, Ruhl, J E, Saro, A, Schaffer, K K, Shirokoff, E, Staniszweski, Z, Stark, A A, Vieira, J D & Williamson, R 2022, ' Shocks in the Stacked Sunyaev-Zel'dovich Profiles of Clusters II: Measurements from SPT-SZ + Planck Compton-y Map ', Monthly Notices of the Royal Astronomical Society, vol. 514, no. 2, pp. 1645-1663 . https://doi.org/10.1093/mnras/stac1376
We search for the signature of cosmological shocks in stacked gas pressure profiles of galaxy clusters using data from the South Pole Telescope (SPT). Specifically, we stack the latest Compton-y maps from the 2500 deg^2 SPT-SZ survey on the locations
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::48c4777292960680957f576ac778838e
http://arxiv.org/abs/2111.04778
http://arxiv.org/abs/2111.04778