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Hubble Space Telescope and Ground-based Observations of Type Ia Supernovae at Redshift 0.5: Cosmological Implications

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dc.contributor.authorClocchiatti, Alejandro
dc.contributor.authorSchmidt, Brian
dc.contributor.authorFilippenko, Alexei
dc.contributor.authorChallis, Peter M
dc.contributor.authorCovarrubias, Ricardo
dc.contributor.authorGarnavich, Peter M
dc.contributor.authorGermany, Lisa
dc.contributor.authorGilliland, Ron
dc.contributor.authorLeibundgut, Bruno
dc.contributor.authorLeonard, D C
dc.contributor.authorMatheson, Thomas
dc.contributor.authorPhillips, Mark M
dc.contributor.authorPrieto, Jose Luis
dc.contributor.authorSchommer, Robert
dc.contributor.authorStubbs, Christopher
dc.contributor.authorTonry, John
dc.contributor.authorSchmidt, Brian
dc.date.accessioned2015-12-08T22:13:54Z
dc.date.issued2006
dc.date.updated2015-12-08T07:46:36Z
dc.description.abstractWe present observations of the Type I Supernovae (SNe) 1999M, 1999N, 1999Q, 1999S, and 1999U, at redshiftz z ≈ 0.5. They were discovered in early 1999 with the 4.0 m Blanco telescope at Cerro Tololo Inter-American Observatory by the High-z Supernova Sea
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/30001
dc.publisherIOP Publishing
dc.rightshttp://www.sherpa.ac.uk/romeo/issn/0004-637X/ Author can archive publisher's version/PDF. Publisher's version/PDF may be used on any website or authors' institutional repository (Sherpa/Romeo as of 26/9/2018)
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Cosmology: observations; Distance scale; Galaxies: distances and redshifts; Supernovae: general
dc.titleHubble Space Telescope and Ground-based Observations of Type Ia Supernovae at Redshift 0.5: Cosmological Implications
dc.typeJournal article
dcterms.accessRightsOpen Access
local.bibliographicCitation.lastpage21
local.bibliographicCitation.startpage1
local.contributor.affiliationClocchiatti, Alejandro, Pontifica Universidad Catolica (Astronomy)
local.contributor.affiliationSchmidt, Brian, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationFilippenko, Alexei, University of California
local.contributor.affiliationChallis, Peter M, Harvard-Smithsonian Center for Astrophysics
local.contributor.affiliationCovarrubias, Ricardo, University of Washington
local.contributor.affiliationGarnavich, Peter M, University of Notre Dame
local.contributor.affiliationGermany, Lisa, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationGilliland, Ron, Space Telescope Science Institute
local.contributor.affiliationLeibundgut, Bruno, European Southern Observatory
local.contributor.affiliationLeonard, D C, California Institute of Technology
local.contributor.affiliationMatheson, Thomas, National Optical Astronomy Observatory
local.contributor.affiliationPhillips, Mark M, Observatories of the Carnegie Institution of Washington
local.contributor.affiliationPrieto, Jose Luis, Ohio State University
local.contributor.affiliationSchommer, Robert, Cerro Tololo Inter-American Observatory
local.contributor.affiliationStubbs, Christopher, Harvard University
local.contributor.affiliationTonry, John, University of Hawaii
local.contributor.authoruidGermany, Lisa, u931535
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4114753xPUB70
local.identifier.citationvolume642
local.identifier.doi10.1086/498491
local.identifier.essn1538-4357
local.identifier.scopusID2-s2.0-33745319302
local.type.statusPublished Version

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