The Infrared Light Curve of SN 2011fe in M101 and the Distance to M101
arXiv:1205.3828 · doi:10.1088/0004-637X/754/1/19
Abstract
We present near infra-red light curves of supernova (SN) 2011fe in M101, including 34 epochs in H band starting fourteen days before maximum brightness in the B-band. The light curve data were obtained with the WIYN High-Resolution Infrared Camera (WHIRC). 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 \pm 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.
arXiv comment9 pages, 3 figures, emulateapj style, accepted for publication in The Astrophysical Journal
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