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DO THE PHOTOMETRIC COLORS OF TYPE II-P SUPERNOVAE ALLOW ACCURATE DETERMINATION OF HOST GALAXY EXTINCTION?

dc.creatorKrisciunas, Kevin
dc.creatorHamuy, Mario
dc.creatorSuntzeff, Nicholas B.
dc.creatorEspinoza, Juan
dc.creatorGonzalez, David
dc.creatorGonzalez, Luis
dc.creatorGonzalez, Sergio
dc.creatorKoviak, Kathleen
dc.creatorKrzeminski, Wojtek
dc.creatorMorrell, Nidia
dc.creatorPhillips, Mark M.
dc.creatorRoth, Miguel
dc.creatorThomas-Osip, Joanna
dc.date.accessioned2019-10-15T19:13:07Z
dc.date.available2019-10-15T19:13:07Z
dc.date.issued2009
dc.identifier.issn0004-6256
dc.identifier.issn1538-3881
dc.identifier.urihttps://hdl.handle.net/1969.1/184777
dc.format.extent7en
dc.publisherThe Astronomical Journal
dc.relation.ispartof1foldr Import 2019-10-08 Batch 14en
dc.relation.uri10.1088/0004-6256/137/1/34en
dc.titleDO THE PHOTOMETRIC COLORS OF TYPE II-P SUPERNOVAE ALLOW ACCURATE DETERMINATION OF HOST GALAXY EXTINCTION?en


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