Photometry of the Type Ib/c SN2013ge

DOI

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.

Identifier
DOI http://doi.org/10.26093/cds/vizier.18210057
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJ/821/57
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/821/57
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/821/57
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJ/821/57
Provenance
Creator Drout M.R.; Milisavljevic D.; Parrent J.; Margutti R.; Kamble A.,Soderberg A.M.; Challis P.; Chornock R.; Fong W.; Frank S.; Gehrels N.,Graham M.L.; Hsiao E.; Itagaki K.; Kasliwal M.; Kirshner R.P.; Macomb D.,Marion G.H.; Norris J.; Phillips M.M.
Publisher CDS
Publication Year 2016
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy