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dc.contributor.authorPierel, JDRen
dc.contributor.authorRodney, Sen
dc.contributor.authorAvelino, Aen
dc.contributor.authorBianco, Fen
dc.contributor.authorFilippenko, AVen
dc.contributor.authorFoley, RJen
dc.contributor.authorFriedman, Aen
dc.contributor.authorHicken, Men
dc.contributor.authorHounsell, Ren
dc.contributor.authorJha, SWen
dc.contributor.authorKessler, Ren
dc.contributor.authorKirshner, RPen
dc.contributor.authorMandel, Kaiseyen
dc.contributor.authorNarayan, Gen
dc.contributor.authorScolnic, Den
dc.contributor.authorStrolger, Len
dc.date.accessioned2019-07-02T23:30:27Z
dc.date.available2019-07-02T23:30:27Z
dc.date.issued2018-11-01en
dc.identifier.issn0004-6280
dc.identifier.urihttps://www.repository.cam.ac.uk/handle/1810/294279
dc.description.abstractEmpirical models of supernova (SN) spectral energy distributions (SEDs) are widely used for SN survey simulations and photometric classifications. The existing library of SED models has excellent optical templates but limited, poorly constrained coverage of ultraviolet (UV) and infrared (IR) wavelengths. However, both regimes are critical for the design and operation of future SN surveys, particularly at IR wavelengths that will be accessible with the James Webb Space Telescope (JWST) and the Wide-Field Infrared Survey Telescope (WFIRST). We create a public repository of improved empirical SED templates using a sampling of Type Ia and core-collapse (CC) photometric light curves to extend the Type Ia parameterized SALT2 model and a set of SN Ib, SN Ic, and SN II SED templates into the UV and near-IR. We apply this new repository of extrapolated SN SED models to examine how future surveys can discriminate between CC and Type Ia SNe at UV and IR wavelengths, and present an open-source software package written in Python, SNSEDextend, that enables a user to generate their own extrapolated SEDs.
dc.publisherIOP Publishing
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleExtending Supernova Spectral Templates for Next-generation Space Telescope Observationsen
dc.typeArticle
prism.endingPage114504
prism.issueIdentifier993en
prism.publicationDate2018en
prism.publicationNamePublications of the Astronomical Society of the Pacificen
prism.startingPage114504
prism.volume130en
dc.identifier.doi10.17863/CAM.41378
dcterms.dateAccepted2018-08-20en
rioxxterms.versionofrecord10.1088/1538-3873/aadb7aen
rioxxterms.versionVoR
rioxxterms.licenseref.urihttp://www.rioxx.net/licenses/all-rights-reserveden
rioxxterms.licenseref.startdate2018-11-01en
dc.contributor.orcidPierel, JDR [0000-0002-2361-7201]
dc.contributor.orcidMandel, Kaisey [0000-0001-9846-4417]
dc.identifier.eissn1538-3873
rioxxterms.typeJournal Article/Reviewen
cam.issuedOnline2018-10-12en


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Attribution 4.0 International
Except where otherwise noted, this item's licence is described as Attribution 4.0 International