Rest-frame R-band light curve of A z ∼ 1.3 supernova obtained with keck laser adaptive optics

Astronomical Journal

Volumn 133, Issue 6, 2007, Pages 2709-2715

  Melbourne, J ^a   Dawson, K S ^b   Koo, D C ^a   Max, C ^a,c   Larkin, J E ^d   Wright, S A ^d   Steinbring, E ^e   Barczys, M ^d   Aldering, G ^b   Barbary, K ^b,f   Dor, M ^g   Fadeyev, V ^b   Goldhaber, G ^b,f   Hattori, T ^h   Ihara, Y ^g   Kashikawa, N ^h   Konishi, K ^g   Kowalski, M ^b   Kuznetsova, N ^b   Lidman, C ⁱ   Morokuma, T ^g   Perlmutter, S ^b,f   Rubin, D ^b,f   Schlegel, D J ^b   Spadafora, A L ^b   Takanashl, N ^g   Yasuda, N ^g   more..

^a University of California Santa Cruz   (United States)

^b LAWRENCE BERKELEY NATIONAL LABORATORY   (United States)

^c LAWRENCE LIVERMORE NATIONAL LABORATORY   (United States)

^d UNIVERSITY OF CALIFORNIA   (United States)

^e NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g UNIVERSITY OF TOKYO   (Japan)

^h NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

ⁱ EUROPEAN SOUTHERN OBSERVATORY   (Chile)

Author keywords

Galaxies: high redshitt; Instrumentation: adaptive optics; Supernovae: general; Techniques: high angular resolution

Indexed keywords

EID: 34250667986     PISSN: 00046256     EISSN: None     Source Type: Journal    
DOI: 10.1086/517492     Document Type: Article

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