Down-sizing in galaxy formation at z ∼ 1 in the Subaru/XMM-Newton deep survey (SXDS)

Monthly Notices of the Royal Astronomical Society

Volumn 350, Issue 3, 2004, Pages 1005-1014

  Kodama, Tadayuki ^a   Yamada, Toru ^a   Akiyama, Masayuki ^a   Aoki, Kentaro ^a   Doi, Mamoru ^b   Furusawa, Hisanori ^a   Fuse, Tetsuharu ^a   Imanishi, Masatoshi ^a   Ishida, Cathy ^a   Iye, Masanori ^a   Kajisawa, Masaru ^a   Karoji, Hiroshi ^a   Kobayashi, Naoto ^b   Komiyama, Yutaka ^a   Kosugi, George ^a   Maeda, Yoshitomo ^c   Miyazaki, Satoshi ^a   Mizumoto, Yoshihiko ^a   Morokuma, Tomoki ^b   Nkata, Fumiaki ^d   Noumaru, Junichi ^a   Ogasawara, Ryusuke ^a   Ouchi, Masami ^b   Sasaki, Toshiyuki ^a   Sekiguchi, Kazuhiro ^a   Shimasaku, Kazuhiro ^b   Simpson, Chris ^d   Takata, Tadafumi ^a   Tanaka, Ichi ^e   Ueda, Yoshihiro ^c   Yasuda, Naoki ^b   Yoshida, Michitoshi ^a   more..

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^b UNIVERSITY OF TOKYO   (Japan)

^c JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

^d DURHAM UNIVERSITY   (United Kingdom)

^e TOHOKU UNIVERSITY   (Japan)

Author keywords

Galaxies: clusters: general; Galaxies: evolution; Galaxies: formation; Galaxies: stellar content

Indexed keywords

COLOR; STARS; SURVEYS;

DEEP SURVEY; GALAXIES: CLUSTERS: GENERAL; GALAXY EVOLUTION; GALAXY FORMATIONS; GALAXY:STELLAR CONTENT; HIGHEST DENSITY REGIONS; MASSIVE SYSTEMS; STARS FORMATION; WIDE-FIELD; XMM-NEWTON;

GALAXIES;

EID: 2642526750     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07711.x     Document Type: Article

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