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

Published online by Cambridge University Press:  05 September 2012

T. A. Pritchard  and
P. W. A. Roming
T. A. Pritchard
Affiliation:
Dept. of Astronomy & Astrophysics, The Pennsylvania State University, 525 Davey Lab, University Park, PA 16802, USA email: tapritchard@astro.psu.edu
P. W. A. Roming
Affiliation:
Dept. of Astronomy & Astrophysics, The Pennsylvania State University, 525 Davey Lab, University Park, PA 16802, USA email: tapritchard@astro.psu.edu Southwest Research Institute, Department of Space Science 6220 Culebra Rd, San Antonio, Texas, 78238USA email: proming@swri.edu
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Abstract

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We present early time (~0-50 days) bolometric light curves of UV-bright Core Collapse Supernovae observed with the Swift UV/Optical Telescope. We also 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.

Keywords

supernovae:generalultraviolet: generalcatalogs
Type
Poster Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S279: Death of Massive Stars: Supernovae and Gamma-Ray Bursts , April 2011 , pp. 383 - 384
Copyright
Copyright © International Astronomical Union 2012

References

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