@inproceedings{754e06b92d3d45519e57a0b919bc852c,
title = "Swift/UVOT observations of type Ib/c supernovae",
abstract = "Swift is an ideal observatory for studying Type Ib/c supernovae. It is able to respond rapidly to newly discovered supernovae and it is able to obtain unique near-ultraviolet photometry and spectra. To date Swift has observed 11 SNe Ib/c with long-term follow-up on two of them. SN2006aj, which is associated with GRB 060218, was observed starting a few minutes after the explosion, making it the earliest detection of a SN. SN2006jc was followed from near maximum light until it faded into its host galaxy Mg II emission lines are seen in the UV spectrum, which are intepreted as evidence for circumstellar interaction.",
keywords = "Gamma-ray bursts, Supernova",
author = "Holland, {Stephen T.} and Stefan Immler and Brown, {Peter J.} and Roming, {Peter W.A.} and {Vanden Berk}, Dan and Milne, {Peter A.}",
year = "2007",
doi = "10.1063/1.2803596",
language = "English (US)",
isbn = "0735404488",
series = "AIP Conference Proceedings",
pages = "391--393",
booktitle = "SUPERNOVA 1987A",
note = "SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters ; Conference date: 19-02-2007 Through 23-02-2007",
}