Early Time Bolometric Light curves of Type-II Supernovae Observed by Swift

Details Early Time Bolometric Light curves of Type-II Supernovae Observed by Swift Early Time Bolometric Light curves of Type-II Supernovae Observed by Swift

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21924232p&link_type=abstract

American Astronomical Society, AAS Meeting #219, #242.32

Astronomy and Astrophysics

Astronomy

Scientific paper

We present early time ( 0-50 days) bolometric light curves of UV-bright Core Collapse Supernovae observed with the Swift UV/Optical Telescope. We generate pseudo-bolometric light curves from Swift UV and optical data and examine these by subtype as well as the observed and interpolated UV and IR flux contributions by epoch and bolometric corrections at early times from UV data.

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