Results 111 to 120 of about 15,250,094 (223)
Weak Lensing by High‐Redshift Clusters of Galaxies. I. Cluster Mass Reconstruction
The Astrophysical Journal, 2000 43 pages, 15 figures, uses aastex, submitted to ApJ 4 color plates produced here as jpg's, larger versions of the jpgs can be found at http://www.mpa-garching.mpg.de ...Clowe, D., Luppino, G., Kaiser, N., Gioia, I. +3 moreopenaire +2 more sourcesA 100 Mpc2 Structure Traced by Hyperluminous Galaxies around a Massive z = 2.85 Protocluster
The Astrophysical JournalWe present wide-field mapping at 850 μ m and 450 μ m of the z = 2.85 protocluster in the HS 1549+19 field using the Submillimetre Common-User Bolometer Array 2. Spectroscopic follow-up of 18 bright sources selected at 850 μ m, using the Northern Extended George C.P. Wang, Scott C. Chapman, Nikolaus Sulzenauer, Frank Bertoldi, Christopher C. Hayward, Ryley Hill, Satoshi Kikuta, Yuichi Matsuda, Douglas Rennehan, Douglas Scott, Ian Smail, Charles C. Steidel +11 moredoaj +1 more sourceA high redshift sample of x-ray selected galaxy clusters [PDF]
, 1998 This thesis describes the creation of a X-ray selected galaxy cluster catalogue — the Southern Serendipitous High-redshift Archival ROSAT Cluster (SHARC) catalogue — and the use of the high-redshift subsample in constraining models of structure formation.Burke, Douglas Johncore JWST’s First Glimpse of a z > 2 Forming Cluster Reveals a Top-heavy Stellar Mass Function
The Astrophysical Journal LettersClusters and their progenitors (protoclusters) at z ∼ 2 − 4, the peak epoch of star formation, are ideal laboratories to study the formation process of both the clusters themselves and their member galaxies.Hanwen Sun, Tao Wang, Ke Xu, Emanuele Daddi, Qing Gu, Tadayuki Kodama, Anita Zanella, David Elbaz, Ichi Tanaka, Raphael Gobat, Qi Guo, Jiaxin Han, Shiying Lu, Luwenjia Zhou +13 moredoaj +1 more sourceEuclid preparation
Astronomy & AstrophysicsWe present our methodology for identifying known clusters as counterparts to objects in the Euclid Catalogue of Galaxy Clusters (ECGC). Euclid is expected to detect a large number of optically selected galaxy clusters over the approximately 14 000 square Melin J.-B., Stanford S. A., Widmer A., Tarrío P., Bartlett J. G., Sadibekova T., Pratt G. W., Arnaud M., Pacaud F., Reiprich T. H., Biviano A., Bardelli S., Borgani S., Corasaniti P.-S., Ettori S., Finoguenov A., Ghaffari Z., Giles P. A., Girardi M., Golden-Marx J. B., Gonzalez A. H., Klein M., Lesci G. F., Maturi M., Maughan B. J., Moscardini L., Pierre M., Radovich M., Rosati P., Sorce J. G., Tsaprazi E., Altieri B., Amara A., Andreon S., Auricchio N., Baccigalupi C., Baldi M., Branchini E., Brescia M., Camera S., Cañas-Herrera G., Capobianco V., Carbone C., Carretero J., Castellano M., Castignani G., Cavuoti S., Chambers K. C., Cimatti A., Colodro-Conde C., Congedo G., Conselice C. J., Conversi L., Copin Y., Courbin F., Courtois H. M., Da Silva A., Degaudenzi H., De Lucia G., Dole H., Douspis M., Dubath F., Duncan C. A. J., Dupac X., Dusini S., Escoffier S., Fabricius M., Farina M., Farrens S., Faustini F., Ferriol S., Finelli F., Fosalba P., Frailis M., Franceschi E., Fumana M., Galeotta S., George K., Gillis B., Giocoli C., Gracia-Carpio J., Grazian A., Grupp F., Haugan S. V. H., Holmes W., Hormuth F., Hornstrup A., Jahnke K., Jhabvala M., Keihänen E., Kermiche S., Kiessling A., Kilbinger M., Kubik B., Kümmel M., Kunz M., Kurki-Suonio H., Le Brun A. M. C., Ligori S., Lilje P. B., Lindholm V., Lloro I., Mainetti G., Maino D., Maiorano E., Mansutti O., Marggraf O., Martinelli M., Martinet N., Marulli F., Massey R. J., Maurogordato S., Medinaceli E., Mei S., Melchior M., Mellier Y., Meneghetti M., Merlin E., Meylan G., Mora A., Moresco M., Munari E., Nakajima R., Neissner C., Niemi S.-M., Padilla C., Paltani S., Pasian F., Pedersen K., Pettorino V., Polenta G., Poncet M., Popa L. A., Pozzetti L., Raison F., Rebolo R., Renzi A., Rhodes J., Riccio G., Romelli E., Roncarelli M., Rossetti E., Saglia R., Sakr Z., Sánchez A. G., Sapone D., Sartoris B., Schneider P., Schrabback T., Secroun A., Sefusatti E., Seidel G., Seiffert M., Serrano S., Simon P., Sirignano C., Sirri G., Stanco L., Steinwagner J., Tallada-Crespí P., Tavagnacco D., Taylor A. N., Tereno I., Tessore N., Toft S., Toledo-Moreo R., Torradeflot F., Tutusaus I., Valenziano L., Valiviita J., Vassallo T., Verdoes Kleijn G., Veropalumbo A., Wang Y., Weller J., Zamorani G., Zerbi F. M., Zucca E., Allevato V., Ballardini M., Bolzonella M., Bozzo E., Burigana C., Cabanac R., Cappi A., Di Ferdinando D., Escartin Vigo J. A., Gabarra L., Martín-Fleitas J., Matthew S., Mauri N., Metcalf R. B., Pezzotta A., Pöntinen M., Porciani C., Risso I., Scottez V., Sereno M., Tenti M., Viel M., Wiesmann M., Akrami Y., Alvi S., Andika I. T., Anselmi S., Archidiacono M., Atrio-Barandela F., Benoist C., Bergamini P., Bertacca D., Bethermin M., Blanchard A., Blot L., Böhringer H., Brown M. L., Bruton S., Calabro A., Camacho Quevedo B., Caro F., Carvalho C. S., Castro T., Cogato F., Conseil S., Cooray A. R., Costanzi M., Cucciati O., Davini S., Desprez G., Díaz-Sánchez A., Diaz J. J., Di Domizio S., Diego J. M., Dimauro P., Enia A., Fang Y., Ferrari A. G., Fontana A., Franco A., Ganga K., García-Bellido J., Gasparetto T., Gautard V., Gavazzi R., Gaztanaga E., Giacomini F., Gianotti F., Gozaliasl G., Guidi M., Gutierrez C. M., Hall A., Hemmati S., Hernández-Monteagudo C., Hildebrandt H., Hjorth J., Kajava J. J. E., Kang Y., Kansal V., Karagiannis D., Kiiveri K., Kirkpatrick C. C., Kruk S., Le Graet J., Legrand L., Lembo M., Lepori F., Leroy G., Lesgourgues J., Leuzzi L., Liaudat T. I., Liu S. J., Loureiro A., Macias-Perez J., Maggio G., Magliocchetti M., Mamon G. A., Mannucci F., Maoli R., Martins C. J. A. P., Maurin L., Miluzio M., Monaco P., Montoro A., Moretti C., Morgante G., Murray C., Naidoo K., Navarro-Alsina A., Nesseris S., Passalacqua F., Paterson K., Pisani A., Potter D., Quai S., Rocci P.-F., Rodighiero G., Sacquegna S., Sahlén M., Sanders D. B., Sarpa E., Schneider A., Schultheis M., Sciotti D., Sellentin E., Smith L. C., Tanidis K., Tao C., Testera G., Teyssier R., Tosi S., Troja A., Tucci M., Valieri C., Venhola A., Vergani D., Verza G., Vielzeuf P., Walton N. A. +316 moredoaj +1 more sourceThe 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 sourceTesting the Standard Cosmological Model [PDF]
, 2011 This thesis exploits the wealth of information contained in the existing cosmological surveys, and demonstrates how the use of tools such as two-point statistics permit the extraction of such information.SAWANGWIT, UTANEcore The Hot and Energetic Universe:The evolution of galaxy groups and clusters [PDF]
, 2013 Major astrophysical questions related to the formation and evolution of structures, and more specifically of galaxy groups and clusters, will still be open in the coming decade and beyond: what is the interplay of galaxy, supermassive black hole, and ...Bourdin, H., Maughan, B., Molendi, S., Mohr, J., von der Linden, A., Borgani, S., Sanders, J., Biffi, V., Dolag, K., H. Reiprich, T., Clerc, N., Smith, R., Springel, V., Arnaud, M., Brueggen, M., Finoguenov, A., Hoekstra, H., Hildebrandt, H., Marrone, D., Pointecouteau, E., Rasia, E., Boehringer, H., Romer, K., Schwope, A., Mazzotta, P., de Plaa, J., Nevalainen, J., Pierre, M., Borm, K., W. Pratt, G., Kaastra, J., Schrabback, T., Allen, S., Fassbender, R., Schindler, S., Ramos-Ceja, M., Lovisari, L., Ohashi, T., Pacaud, F., Adami, C., Elbaz, D., Bulbul, E., Ota, N., H. Croston, J., -Y. Zhang, Y., Brunetti, G., Ettori, S., Lamer, G. +47 morecore
