The Hubble space telescope cluster supernova survey. VI. the volumetric type Ia supernova rate in high-redshift galaxy clusters

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dc.contributor.authorBarbary, K.en
dc.contributor.authorAldering, G.en
dc.contributor.authorAmanullah, R.en
dc.contributor.authorBrodwin, M.en
dc.contributor.authorConnolly, N.en
dc.contributor.authorDawson, K. S.en
dc.contributor.authorDoi, M.en
dc.contributor.authorEisenhardt, P.en
dc.contributor.authorFaccioli, L.en
dc.contributor.authorFadeyev, V.en
dc.contributor.authorFakhouri, H. K.en
dc.contributor.authorFruchter, A. S.en
dc.contributor.authorGilbank, D. G.en
dc.contributor.authorGladders, M. D.en
dc.contributor.authorGoldhaber, G.en
dc.contributor.authorGoobar, A.en
dc.contributor.authorHattori, T.en
dc.contributor.authorHsiao, E.en
dc.contributor.authorHuang, X.en
dc.contributor.authorIhara, Y.en
dc.contributor.authorKashikawa, N.en
dc.contributor.authorKoester, B.en
dc.contributor.authorKonishi, K.en
dc.contributor.authorKowalski, M.en
dc.contributor.authorLidman, C.en
dc.contributor.authorLubin, L.en
dc.contributor.authorMeyers, J.en
dc.contributor.authorMorokuma, T.en
dc.contributor.authorOda, T.en
dc.contributor.authorPanagia, N.en
dc.contributor.authorPerlmutter, S.en
dc.contributor.authorPostman, M.en
dc.contributor.authorRipoche, P.en
dc.contributor.authorRosati, P.en
dc.contributor.authorRubin, D.en
dc.contributor.authorSchlegel, D. J.en
dc.contributor.authorSpadafora, A. L.en
dc.contributor.authorStanford, S. A.en
dc.contributor.authorStrovink, M.en
dc.contributor.authorSuzuki, N.en
dc.contributor.authorTakanashi, N.en
dc.contributor.authorTokita, K.en
dc.contributor.authorYasuda, N.en
dc.date.accessioned2025-06-11T06:35:15Z
dc.date.available2025-06-11T06:35:15Z
dc.date.issued2012-01-20en
dc.description.abstractWe present a measurement of the volumetric Type Ia supernova (SN Ia) rate out to z ≃ 1.6 from the Hubble Space Telescope Cluster Supernova Survey. In observations spanning 189 orbits with the Advanced Camera for Surveys we discovered 29 SNe, of which approximately 20 are SNe Ia. Twelve of these SNe Ia are located in the foregrounds and backgrounds of the clusters targeted in the survey. Using these new data, we derive the volumetric SN Ia rate in four broad redshift bins, finding results consistent with previous measurements at z ≳ 1 and strengthening the case for an SN Ia rate that is ≳ 0.6 × 10-4 h 3 70yr-1Mpc-3 at z 1 and flattening out at higher redshift. We provide SN candidates and efficiency calculations in a form that makes it easy to rebin and combine these results with other measurements for increased statistics. Finally, we compare the assumptions about host-galaxy dust extinction used in different high-redshift rate measurements, finding that different assumptions may induce significant systematic differences between measurements.en
dc.description.statusPeer-revieweden
dc.identifier.issn0004-637Xen
dc.identifier.scopus84855784211en
dc.identifier.urihttp://www.scopus.com/inward/record.url?scp=84855784211&partnerID=8YFLogxKen
dc.identifier.urihttps://hdl.handle.net/1885/733758329
dc.language.isoenen
dc.sourceAstrophysical Journalen
dc.subjectcosmology: observationsen
dc.subjectsupernovae: generalen
dc.subjectwhite dwarfsen
dc.titleThe Hubble space telescope cluster supernova survey. VI. the volumetric type Ia supernova rate in high-redshift galaxy clustersen
dc.typeJournal articleen
dspace.entity.typePublicationen
local.contributor.affiliationBarbary, K.; University of California at Berkeleyen
local.contributor.affiliationAldering, G.; Lawrence Berkeley National Laboratoryen
local.contributor.affiliationAmanullah, R.; University of California at Berkeleyen
local.contributor.affiliationBrodwin, M.; Harvard-Smithsonian Center for Astrophysicsen
local.contributor.affiliationConnolly, N.; Hamilton Collegeen
local.contributor.affiliationDawson, K. S.; Lawrence Berkeley National Laboratoryen
local.contributor.affiliationDoi, M.; The University of Tokyoen
local.contributor.affiliationEisenhardt, P.; Jet Propulsion Laboratory, California Institute of Technologyen
local.contributor.affiliationFaccioli, L.; Lawrence Berkeley National Laboratoryen
local.contributor.affiliationFadeyev, V.; University of California at Santa Cruzen
local.contributor.affiliationFakhouri, H. K.; University of California at Berkeleyen
local.contributor.affiliationFruchter, A. S.; Space Telescope Science Instituteen
local.contributor.affiliationGilbank, D. G.; University of Waterlooen
local.contributor.affiliationGladders, M. D.; The University of Chicagoen
local.contributor.affiliationGoldhaber, G.; University of California at Berkeleyen
local.contributor.affiliationGoobar, A.; Oskar Klein Centreen
local.contributor.affiliationHattori, T.; National Institutes of Natural Sciences - National Astronomical Observatory of Japanen
local.contributor.affiliationHsiao, E.; Lawrence Berkeley National Laboratoryen
local.contributor.affiliationHuang, X.; University of California at Berkeleyen
local.contributor.affiliationIhara, Y.; The University of Tokyoen
local.contributor.affiliationKashikawa, N.; The University of Tokyoen
local.contributor.affiliationKoester, B.; The University of Chicagoen
local.contributor.affiliationKonishi, K.; The University of Tokyoen
local.contributor.affiliationKowalski, M.; University of Bonnen
local.contributor.affiliationLidman, C.; Australian Astronomical Observatoryen
local.contributor.affiliationLubin, L.; University of California at Davisen
local.contributor.affiliationMeyers, J.; University of California at Berkeleyen
local.contributor.affiliationMorokuma, T.; The University of Tokyoen
local.contributor.affiliationOda, T.; Kyoto Universityen
local.contributor.affiliationPanagia, N.; Space Telescope Science Instituteen
local.contributor.affiliationPerlmutter, S.; University of California at Berkeleyen
local.contributor.affiliationPostman, M.; Space Telescope Science Instituteen
local.contributor.affiliationRipoche, P.; Lawrence Berkeley National Laboratoryen
local.contributor.affiliationRosati, P.; European Southern Observatoryen
local.contributor.affiliationRubin, D.; University of California at Berkeleyen
local.contributor.affiliationSchlegel, D. J.; Lawrence Berkeley National Laboratoryen
local.contributor.affiliationSpadafora, A. L.; Lawrence Berkeley National Laboratoryen
local.contributor.affiliationStanford, S. A.; University of California at Davisen
local.contributor.affiliationStrovink, M.; University of California at Berkeleyen
local.contributor.affiliationSuzuki, N.; Lawrence Berkeley National Laboratoryen
local.contributor.affiliationTakanashi, N.; The University of Tokyoen
local.contributor.affiliationTokita, K.; The University of Tokyoen
local.contributor.affiliationYasuda, N.; The University of Tokyoen
local.identifier.citationvolume745en
local.identifier.doi10.1088/0004-637X/745/1/31en
local.identifier.pure69bf6ea9-1acd-46e6-84fb-2e0bd26a3a28en
local.identifier.urlhttps://www.scopus.com/pages/publications/84855784211en
local.type.statusPublisheden

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