The infrared light curve of SN 2011fe in M101 and the distance to M101

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dc.contributor.authorMatheson, T.
dc.contributor.authorJoyce, R.R.
dc.contributor.authorAllen, L.E.
dc.contributor.authorSaha, A.
dc.contributor.authorSilva, D.R.
dc.contributor.authorWood-Vasey, W.M.
dc.contributor.authorAdams, J.J.
dc.contributor.authorAnderson, R.E.
dc.contributor.authorBeck, T.L.
dc.contributor.authorBentz, M.C.
dc.contributor.authorBershady, M.A.
dc.contributor.authorBinkert, W.S.
dc.contributor.authorButler, K.
dc.contributor.authorCamarata, M.A.
dc.contributor.authorEigenbrot, A.
dc.contributor.authorEverett, M.
dc.contributor.authorGallagher, J.S.
dc.contributor.authorGarnavich, P.M.
dc.contributor.authorGlikman, E.
dc.contributor.authorHarbeck, D.
dc.contributor.authorHargis, J.R.
dc.contributor.authorHerbst, H.
dc.contributor.authorHorch, E.P.
dc.contributor.authorHowell, S.B.
dc.contributor.authorJha, S.
dc.contributor.authorKaczmarek, J.F.
dc.contributor.authorKnezek, P.
dc.contributor.authorManne-Nicholas, E.
dc.contributor.authorMathieu, R.D.
dc.contributor.authorMeixner, M.
dc.contributor.authorMilliman, K.
dc.contributor.authorPower, J.
dc.contributor.authorRajagopal, J.
dc.contributor.authorReetz, K.
dc.contributor.authorRhode, K.L.
dc.contributor.authorSchechtman-Rook, A.
dc.contributor.authorSchwamb, M.E.
dc.contributor.authorSchweiker, H.
dc.contributor.authorSimmons, B.
dc.contributor.authorSimon, J.D.
dc.contributor.authorSummers, D.
dc.contributor.authorYoung, M.D.
dc.contributor.authorWeyant, A.
dc.contributor.authorWilcots, E.M.
dc.contributor.authorWill, G.
dc.contributor.authorWilliams, D.
dc.date.accessioned2014-10-30T19:04:25Z
dc.date.available2014-10-30T19:04:25Z
dc.date.issued2012
dc.description.abstractWe present near-infrared light curves of supernova (SN) 2011fe in M101, including 34 epochs in H band starting 14 days before maximum brightness in the B band. The light curve data were obtained with the WIYN High-Resolution Infrared Camera. When the data are calibrated using templates of other Type Ia SNe, we derive an apparent H-band magnitude at the epoch of B-band maximum of 10.85 ± 0.04. This implies a distance modulus for M101 that ranges from 28.86 to 29.17 mag, depending on which absolute calibration for Type Ia SNe is used.
dc.identifier.citationMatheson, T., Joyce, R. R., Allen, L. E., Saha, A., Silva, D. R., Wood-Vasey, W. M., . . . Williams, D. (2012). The infrared light curve of SN 2011fe in M101 and the distance to M101. Astrophysical Journal, 754(1), 19. http://dx.doi.org/10.1088/0004-637X/754/1/19
dc.identifier.urihttps://hdl.handle.net/2022/19078
dc.language.isoen_US
dc.publisherThe American Astronomical Society
dc.relation.isversionofhttps://doi.org/10.1088/0004-637X/754/1/19
dc.rights© 2012 The American Astronomical Society.
dc.subjectgalaxies: distances and redshifts
dc.subjectgalaxies: individual (M101)
dc.subjectsupernovae: individual (SN 2011fe)
dc.titleThe infrared light curve of SN 2011fe in M101 and the distance to M101
dc.typeArticle

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