Photometry of the Type Ib/c SN2013ge Virtual Observatory Resource

Authors

1. Drout M.R.
2. Milisavljevic D.
3. Parrent J.
4. Margutti R.
5. Kamble A.,Soderberg A.M.
6. Challis P.
7. Chornock R.
8. Fong W.
9. Frank S.
10. Gehrels N.,Graham M.L.
11. Hsiao E.
12. Itagaki K.
13. Kasliwal M.
14. Kirshner R.P.
15. Macomb D.,Marion G.H.
16. Norris J.
17. Phillips M.M.

Published by

CDS

Abstract

We present extensive multiwavelength (radio to X-ray) observations of the Type Ib/c supernova (SN Ib/c) SN 2013ge from -13 to +457 days relative to maximum light, including a series of optical spectra and Swift UV-optical photometry beginning 2-4 days post-explosion. This data set makes SN 2013ge one of the best-observed normal SNe Ib/c at early times - when the light curve is particularly sensitive to the progenitor configuration and mixing of radioactive elements - and reveals two distinct light curve components in the UV bands.

Keywords

1. supernovae
2. photometry

Bibliographic source Bibcode

2016ApJ...821...57D

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/821/57

IVOA Identifier IVOID

ivo://CDS.VizieR/J/ApJ/821/57

Document Object Identifer DOI

doi:10.26093/cds/vizier.18210057

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http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/821/57

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