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<ri:Resource created="2017-11-08T14:15:49Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Swift-UVOT obs. analysis of 29 SNe Ia</title><shortName>J/ApJ/836/232</shortName><identifier>ivo://CDS.VizieR/J/ApJ/836/232</identifier><altIdentifier>doi:10.26093/cds/vizier.18360232</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Brown P.J.</name></creator><creator><name>Landez N.J.</name></creator><creator><name>Milne P.A.</name></creator><creator><name>Stritzinger M.D.</name></creator><date role="Updated">2017-12-13T19:44:59Z</date><date role="Created">2017-11-08T14:15:49Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>supernovae</subject><subject>ultraviolet-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>The intrinsic colors of Type Ia supernovae (SNe Ia) are important to understanding their use as cosmological standard candles. Understanding the effects of reddening and redshift on the observed colors are complicated and dependent on the intrinsic spectrum, the filter curves, and the wavelength dependence of reddening. We present ultraviolet and optical data of a growing sample of SNe Ia observed with the Ultraviolet/Optical Telescope on the Swift spacecraft and use this sample to re-examine the near-UV (NUV) colors of SNe Ia. We find that a small amount of reddening (E(B-V)=0.2mag) could account for the difference between groups designated as NUV-blue and NUV-red, and a moderate amount of reddening (E(B-V)=0.5mag) could account for the whole NUV-optical differences. The reddening scenario, however, is inconsistent with the mid-UV colors and color evolution. The effect of redshift alone only accounts for part of the variation. Using a spectral template of SN2011fe, we can forward model the effects of redshift and reddening and directly compare those with the observed colors. We find that some SNe are consistent with reddened versions of SN2011fe, but most SNe Ia are much redder in the uvw1-v color than SN2011fe reddened to the same b-v color. The absolute magnitudes show that two out of five NUV-blue SNe Ia are blue because their near-UV luminosity is high, and the other three are optically fainter. We also show that SN 2011fe is not a "normal" SN Ia in the UV, but has colors placing it at the blue extreme of our sample.</description><source format="bibcode">2017ApJ...836..232B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/836/232</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/527">J/AJ/131/527 : UBVRI light curves of 44 type Ia supernovae (Jha+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/659/122">J/ApJ/659/122 : Improved distances to type Ia supernovae (Jha+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/689/377">J/ApJ/689/377 : PAIRITEL SNe Ia as NIR standard candles (Wood-Vasey+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/4517">J/AJ/137/4517 : UVOT light curves of supernovae (Brown+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/185/32">J/ApJS/185/32 : First-year SDSS-II SN results (Kessler+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/721/1608">J/ApJ/721/1608 : Absolute UV magnitudes of type Ia SNe (Brown+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/139/120">J/AJ/139/120 : Low-redshift Type-Ia supernovae (Folatelli+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/731/120">J/ApJ/731/120 : Intrinsic SN Ia light curves (Mandel+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/753/22">J/ApJ/753/22 : Swift/UVOT observations of SN 2011fe (Brown+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/554/A27">J/A+A/554/A27 : 2011fe spectrophotometric time series (Pereira+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/568/A22">J/A+A/568/A22 : Joint analysis of the SDSS-II and SNLS SNe Ia (Betoule+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/212/18">J/ApJS/212/18 : An atlas of UV-to-MIR galaxy SEDs (Brown+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/796/L18">J/ApJ/796/L18 : Type Ia supernova 2011de UVOT photometry (Brown, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/438/1391">J/MNRAS/438/1391 : Host galaxies of Type Ia SN from PTF (Pan+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/102">J/AJ/152/102 : Flux conversion factors for Swift/UVOT filters (Brown+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/826/56">J/ApJ/826/56 : HST/WFC3 obs. of Cepheids in SN Ia host gal. 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