Not Color‐Blind: Using Multiband Photometry to Classify Supernovae

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Not Color Blind: Using Multiband Photometry to Classify Supernovae

Large numbers of supernovae (SNe) have been discovered in recent years, and many more will be found in the near future. Once discovered, further study of a SN and its possible use as an astronomical tool (e.g., as a distance estimator) require knowledge of the SN type. Current classification methods rely almost solely on the analysis of SN spectra to determine their type. However, spectroscopy ...

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Using Multi-Band Photometry to Classify Supernovae

1 School of Physics & Astronomy, Tel-Aviv University, Tel-Aviv 69978, Israel (dovip, avishay, dani)@wise.tau.ac.il 2 Department of Astronomy, 601 Campbell Hall, University of California, Berkeley, CA 94720-3411 [email protected] 3 Five College Astronomy Department, University of Massachusetts, Amherst, MA 01003-9305 [email protected] 4 Harvard-Smithsonian Center for Astrophy...

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ژورنال

عنوان ژورنال: Publications of the Astronomical Society of the Pacific

سال: 2002

ISSN: 0004-6280,1538-3873

DOI: 10.1086/341741