Results 111 to 120 of about 49,283 (254)
The Bigfoot: A Footprint of a Coma Cluster Progenitor at z = 3.98
The Astrophysical Journal LettersProtoclusters, galaxy clusters’ high-redshift progenitors, hold the key to understanding the formation and evolution of clusters and their member galaxies. However, their cosmological distances and spatial extensions (tens of Mpc) have inhibited complete Hanwen Sun, Tao Wang, Emanuele Daddi, Qiaoyang Hao, Ke Xu, David Elbaz, Luwenjia Zhou, Houjun Mo, Huiyuan Wang, Longyue Chen, Yangyao Chen, Shuowen Jin, Yipeng Lyu, Nikolaj Sillassen, Kai Wang, Tiancheng Yang +15 moredoaj +1 more sourceObservations of Galaxy Clustering at High Redshift
, 1998 This paper reviews the current status of measurements of galaxy clustering at high redshifts (z > 0.3). The focus is on the inherent limitations in the observation and interpretation of the ``evolution of clustering''. It is likely that results from the first attempts to characterize galaxy clustering beyond the ``local'' universe have been ...openaire +2 more sourcesDeep Chandra Observations of the z = 1.16 Relaxed, Cool-core Galaxy Cluster SPT-CL J2215-3537
The Astrophysical JournalGalaxy clusters serve as a unique and valuable laboratory for probing cosmological models and understanding astrophysics at the high-mass limit of structure formation.Haley R. Stueber, Adam B. Mantz, Steven W. Allen, Anthony M. Flores, R. Glenn Morris, Abigail Y. Pan, Taweewat Somboonpanyakul, Lindsey E. Bleem, Michael Calzadilla, Benjamin Floyd, Julie Hlavacek-Larrondo, Michael McDonald, Arnab Sarkar +12 moredoaj +1 more sourceGalaxy stellar mass functions of different morphological types in
clusters, and their evolution between z=0.8 and z=0
, 2010 We present the galaxy stellar mass function (MF) and its evolution in
clusters from z~0.8 to the current epoch, based on the WIde-field Nearby
Galaxy-cluster Survey (WINGS) (0 ...Alan Dressler, Alessandro Omizzolo, Alessia Moretti, Alfonso Aragón-Salamanca, Andreon, Antonio Cava, Aragon-Salamanca, Baldry, Baldry, Baldry, Balogh, Barger, Bekki, Bekki, Bell, Bell, Benedetta Vulcani, Bernardi, Bianca M. Poggianti, Blanton, Bolzonella, Bolzonella, Borch, Boselli, Brinchmann, Brunner, Bundy, Bundy, Byrd, Capak, Cava, Conselice, Daniela Bettoni, De Propris, Desai, Dressler, Dressler, Drory, Ebeling, Ebeling, Ebeling, Fasano, Fasano, Fasano, Feulner, Finn, Font, Fontana, Fontana, Franceschini, Fritz, Gehrels, Giovanni Fasano, Gonzalez, Gregory Rudnick, Gunn, Gwyn, Halliday, Holden, Huertas-Company, Icke, Ilbert, Jacopo Fritz, Jesús Varela, Kauffmann, Kodama, Kovac, Kroupa, Larson, Lotz, Makino, Mauro D'Onofrio, McCarthy, Mihos, Milvang-Jensen, Moore, Noeske, Ocvirk, Ocvirk, Oesch, Ostriker, Pannella, Pelló, Poggianti, Poggianti, Poggianti, Poggianti, Postman, Pozzetti, Pozzetti, Pérez-González, Rudnick, Rudnick, Rudnick, Salpeter, Schechter, Smith, Sánchez-Blázquez, Tasca, Tiziano Valentinuzzi, Toft, Valentinuzzi, Valentinuzzi, van der Wel, van der Wel, Varela, Vazdekis, Vergani, von der Linden, Vulcani, White +110 morecore +1 more sourceActive Galactic Nucleus Properties of ∼1 Million Member Galaxies of Galaxy Groups and Clusters at z < 1.4 Based on the Subaru Hyper Suprime-Cam Survey
The Astrophysical JournalHerein, we present the statistical properties of active galactic nuclei (AGNs) for approximately 1 million member galaxies of galaxy groups and clusters with 0.1 < cluster redshift ( z _cl ) < 1.4 selected using the Subaru Hyper Suprime-Cam, the so ...Yoshiki Toba, Aoi Hashiguchi, Naomi Ota, Masamune Oguri, Nobuhiro Okabe, Yoshihiro Ueda, Masatoshi Imanishi, Atsushi J. Nishizawa, Tomotsugu Goto, Bau-Ching Hsieh, Marie Kondo, Shuhei Koyama, Kianhong Lee, Ikuyuki Mitsuishi, Tohru Nagao, Taira Oogi, Koki Sakuta, Malte Schramm, Anri Yanagawa, Anje Yoshimoto +19 moredoaj +1 more sourceThe Future Landscape of High-Redshift Galaxy Cluster Science
, 2019 We describe the opportunities for galaxy cluster science in the high- redshift regime where massive, virialized halos first formed and where star formation and AGN activity peaked. New observing facilities from radio to X-ray wavelengths, combining high spatial/spectral resolution with large collecting areas, are poised to uncover this population.Mantz, Adam, Allen, Steven W., Battaglia, Nicholas, Benson, Bradford, Canning, Rebecca, Ettori, Stefano, Evrard, August, von der Linden, Anja, McDonald, Michael, Abidi, Muntazir, Ahmed, Zeeshan, Amin, Mustafa A., Ansarinejad, Behzad, Armstrong, Robert, Avestruz, Camille, Baccigalupi, Carlo, Bandura, Kevin, Barkhouse, Wayne, Basu, Kaustuv moni, Bavdhankar, Chetan Bender, Amy N., de Bernardis, Paolo, Bischoff, Colin, Biviano, Andrea, Bleem, Lindsey, Bocquet, Sebastian, Bond, J. Richard, Borgani, Stefano, Borrill, Julian, Boutigny, Dominique, Frye, Brenda, Bruggen, Marcus, Cai, Zheng, Carlstrom, John E., Castander, Francisco J., Challinor, Anthony, Clowe, Douglas, Cohn, J. D., Comparat, Johan, Cooray, Asantha, Coulton, William, Cyr-Racine, Francis-Yan, Daddi, Emanuele, Delabrouille, Jacques, Dell'antonio, Ian, Demarteau, Marcel, Donahue, Megan, Dunkley, Joanna, Escoffier, Stephanie, Essinger-Hileman, Tom, Fabbian, Giulio, Fabjan, Dunja, Farahi, Arya, Foreman, Simon, Fraisse, Aurelien A., Garcia, Luz Angela, GASPARI M, Gerbino, Martina, Gitti, Myriam, Gluscevic, Vera, Gonzalez, Anthony, Górski, Krzysztof M., Gruen, Daniel, Gudmundsson, Jon E., Gupta, Nikhel, de Haan, Tijmen, Hernquist, Lars, Hirata, Christopher M., Hlozek, Renee, Jeltema, Tesla, Cohen-Tanugi, Johann, Johnson, Bradley, Kadota, Kenji, Kamionkowski, Marc, Khatri, Rishi, Kisner, Theodore, Kneib, Jean-Paul, Knox, Lloyd, Kovetz, Ely D., Krause, Elisabeth, Lattanzi, Massimiliano, Lau, Erwin T., Liguori, Michele, Lovisari, Lorenze, Macorra, Axel de la, Masi, Silvia, Masui, Kiyoshi, Maughan, Benjamin, Maurogordato, Sophie, McMahon, Jeff, McNamara, Brian, Melchior, Peter, Mertens, James, Meyers, Joel, Mirbabayi, Mehrdad, More, Surhud, Motloch, Pavel, Moustakas, John, Mroczkowski, Tony, Mukherjee, Suvodip, Nagai, Daisuke +199 more +9 more sources
