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dc.contributor.authorRiess, Adam
dc.contributor.authorKirshner, Robert
dc.contributor.authorSchmidt, Brian
dc.contributor.authorJha, Saurabh
dc.contributor.authorChallis, Peter
dc.contributor.authorGarnavich, Peter
dc.contributor.authorEsin, Ann
dc.contributor.authorCarpenter, Chris
dc.contributor.authorGrashius, Randy
dc.contributor.authorSchild, Rudolph
dc.date.accessioned2019-09-27T13:17:08Z
dc.date.issued1999
dc.identifier.citationRiess, Adam G., Robert P. Kirshner, Brian P. Schmidt, Saurabh Jha, Peter Challis, Peter M. Garnavich, Ann A. Esin, et al. 1999. “BVRI light curves for 22 type Ia supernovae.” The Astronomical Journal 117 (2): 707–24. https://doi.org/10.1086/300738.
dc.identifier.issn0004-6256
dc.identifier.issn1538-3881
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:41417334*
dc.description.abstractWe present 1210 Johnson/Cousins B, V, R, and I photometric observations of 22 recent Type Ia supernovae (SNe Ia): SNe 1993ac, 1993ae, 1994M, 1994S, 1994T, 1994Q, 1994ae, 1995D, 1995E, 1995al, 1995ac, 1995ak, 1995bd, 1996C, 1996X, 1996Z, 1996ab, 1996ai, 1996bk, 1996bl, 1996bo, and 1996bv. Most of the photometry was obtained at the Fred Lawrence Whipple Observatory of the Harvard-Smithsonian Center for Astrophysics in a cooperative observing plan aimed at improving the database for SNe Ia. The redshifts of the sample range from cz = 1200 to 37,000 km s(-1) with a mean of ct = 7000 km s(-1).
dc.language.isoen_US
dc.publisherAmerican Astronomical Society
dash.licenseLAA
dc.titleBVRI light curves for 22 type Ia supernovae
dc.typeJournal Article
dc.description.versionAccepted Manuscript
dc.relation.journalThe Astronomical Journal
dash.depositing.authorKirshner, Robert P.::0f07c3b6230f5e5a42326bcba12a1795::600
dc.date.available2019-09-27T13:17:08Z
dash.workflow.comments1Science Serial ID 94356
dc.identifier.doi10.1086/300738
dash.source.volume117;2
dash.source.page707


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