The distant type Ia supernova rate

Astrophysical Journal

Volumn 577, Issue 1 I, 2002, Pages 120-132

  Pain, R ^a   Fabbro, S ^a,b   Sullivan, M ^c   Ellis, R S ^d,e   Aldering, G ^f   Astier, P ^a   Deustua, S E ^f   Fruchter, A S ^g   Goldhaber, G ^f,h   Goobar, A ⁱ   Groom, D E ^f   Hardin, D ^a   Hook, I M ^j   Howell, D A ^f   Irwin, M J ^d   Kim, A G ^f   Kim, M Y ^f   Knop, R A ^f   Lee, J C ^f,k   Lidman, C ^l   McMahon, R G ⁿ   Nugent, P E ^f   Panagia, N ^g   Pennypacker, C R ^f,m   Perlmutter, S ^f,h   Ruiz Lapuente, P ⁿ   Schahmaneche, K ^a   Schaefer, B ^o,p   Walton, N A ^d   more..

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b INSTITUTO SUPERIOR TÉCNICO   (Portugal)

^c DURHAM UNIVERSITY   (United Kingdom)

^d UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^f LAWRENCE BERKELEY NATIONAL LABORATORY   (United States)

^g AURA for the European Space Agency   (United States)

^h UNIVERSITY OF CALIFORNIA   (United States)

ⁱ STOCKHOLM UNIVERSITY   (Sweden)

^j UNIVERSITY OF OXFORD   (United Kingdom)

^k MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^l EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^m UNIVERSITY OF CALIFORNIA   (United States)

ⁿ UNIVERSITY OF BARCELONA   (Spain)

^o YALE UNIVERSITY   (United States)

^p UNIVERSITY OF TEXAS AT AUSTIN   (United States)

more..

Author keywords

Galaxies: evolution; Galaxies: high redshift; Supernovae: general

Indexed keywords

EID: 0038569322     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/342129     Document Type: Review

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