Implications for the hubble constant from the first seven supernovae at z ≥ 0.35

Astrophysical Journal

Volumn 476, Issue 2 PART II, 1997, Pages

  Kim, A G ^a,b   Gabi, S ^a,c   Goldhaber, G ^a,b   Groom, D E ^a   Hook, I M ^b   Kim, M Y ^a   Lee, J C ^a   Pennypacker, C R ^a,c   Perlmutter, S ^a,b   Small, I A ^a,b   Goobar, A ^d   Pain, R ^e   Ellis, R S ^f   McMahon, R G ^f   Boyle, B J ^g,h   Bunclark, P S ^g   Carter, D ^g   Irwin, M J ^g   Glazebrook, K ^h   Newberg, H J M ⁱ   Fllippenko, A V ^b   Matheson, T ^b   Dopita, M ^j   Couch, W J ^k   more..

^a LAWRENCE BERKELEY NATIONAL LABORATORY   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c UNIVERSITY OF CALIFORNIA   (United States)

^d STOCKHOLM UNIVERSITY   (Sweden)

^e UNIVERSITÉ PARIS DESCARTES   (France)

^f UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^g ROYAL GREENWICH OBSERVATORY   (United Kingdom)

^h ANGLO AUSTRALIAN OBSERVATORY   (Australia)

ⁱ FERMI NATIONAL ACCELERATOR LABORATORY   (United States)

^j AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^k UNIVERSITY OF NEW SOUTH WALES   (Australia)

more..

Author keywords

Distance scale; Supernovae: general

Indexed keywords

EID: 0003161292     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/310507     Document Type: Article

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