The SVBABU/XMM-Newton deep survey (SXDS). V. Optically faint variable object survey

Astrophysical Journal

Volumn 676, Issue 1, 2008, Pages 163-183

  Morokuma, Tomoki ^a,b   Doi, Mamoru ^b   Yasuda, Naoki ^b   Akiyama, Masayuki ^a   Sekiguchi, Kazuhiro ^a   Furusawa, Hisanori ^a   Ueda, Yoshihiro ^c   Totani, Tomonori ^c   Oda, Takeshi ^c,d   Nagao, Tohru ^a,d   Kashikawa, Nobunari ^a   Murayama, Takashi ^e   Ouchi, Masami ^f,g   Watson, Mike G ^h   Richmond, Michael W ⁱ   Lidman, Christopher ^j   Perlmutter, Saul ^k   Spadafora, Anthony L ^k   Aldering, Greg ^k   Wang, Lifan ^k,l   Hook, Isobel M ^m   Knop, Rob A ^m   more..

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^b UNIVERSITY OF TOKYO   (Japan)

^c KYOTO UNIVERSITY   (Japan)

^d Kyoto University ^*

^e TOHOKU UNIVERSITY   (Japan)

^f STScI   (United States)

^g UNIVERSITY OF LEICESTER   (United Kingdom)

^h ROCHESTER INSTITUTE OF TECHNOLOGY   (United States)

ⁱ EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^j LAWRENCE BERKELEY NATIONAL LABORATORY   (United States)

^k TEXAS A AND M UNIVERSITY   (United States)

^l UNIVERSITY OF OXFORD   (United Kingdom)

^m VANDERBILT UNIVERSITY   (United States)

more..

Author keywords

Galaxies: active; Stars: variables: other; Supernovae: general; Surveys

Indexed keywords

EID: 42149144578     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/527467     Document Type: Review

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