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Title:
Detection of X-Ray Emission from SN 2005kd with Swift
Authors:
Immler, S.; Pooley, D.; Brown, P. J.
Publication:
The Astronomer's Telegram, #981
Publication Date:
01/2007
Origin:
ATEL
Keywords:
Optical, Ultra-Violet, X-ray, Novae, Supernovae
Bibliographic Code:
2007ATel..981....1I

Abstract

Swift Ultraviolet/Optical Telescope (UVOT) and X-Ray Telescope (XRT) started observing the type IIn SN 2005kd (IAUC #8630) on 2007-01-24.04 UT. The following UVOT magnitudes were measured: UVW1 [181-321nm] = 18.6 (2,422 s exposure time), UVM2 [166-268 nm] = 19.7 (2,994 s), and UVW2 [112-264 nm] = 19.7 (3,214 s). The magnitudes have not been corrected for extinction. Due to the location of the SN within a dense spiral arm, errors are estimated to be 0.4 mag.
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Database: Astronomy
Physics
arXiv e-prints