Figure 1 from Early Observations and Analysis of the Type Ia SN 2014J in M82

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Early Observations and Analysis of the Type Ia SN 2014J in M82

Authors: G. H. Marion, D. J. Sand, E. Y. Hsiao, D. P. K. Banerjee, S. Valenti, M. D. Stritzinger, J. Vinkó, V. Joshi, V. Venkataraman, N. M. Ashok, R. Amanullah, R. P. Binzel, J. J. Bochanski, G. L. Bryngelson, C. R. Burns, D. Drozdov, S. K. Fieber-Beyer, M. L. Graham, D. A. Howell, J. Johansson, R. P. Kirshner, P. A. Milne, J. Parrent, J. M. Silverman, R. J. Vervack, Jr., and J. C. Wheeler

Marion et al. 2015 The Astrophysical Journal 798 39.

Provider: AAS Journals

Caption: Figure 1.

Photometry of SN 2014J from −11d to +29d. The observations were made at Mt. Abu (JHK_s) and by the LCOGT (UBVRI). The LC properties and the significant extinction of SN 2014J are discussed in Section 3. Photometric uncertainties are plotted, although there may be residual systematics due to M82 host galaxy contamination. Note that the NIR bands have not reached their secondary peaks at the final observation date in this sample.

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