Possible Detection of SN 2007pk in X-Rays with Swift

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Title:		Possible Detection of SN 2007pk in X-Rays with Swift
Authors:		Immler, S.; Pooley, D.; Brown, P. J.; Li, W.; Filippenko, A. V. ;
Publication:		The Astronomer's Telegram, #1284
Publication Date:		11/2007
Origin:		ATEL
Keywords:		Optical, Ultra-Violet, X-ray, Novae, Supernovae
Bibliographic Code:		2007ATel.1284....1I

Abstract

Swift Ultraviolet/Optical Telescope (UVOT) and X-Ray Telescope (XRT) observed the type-IIn SN 2007pk (CBET #1129, ATel #1271) on 2007-11-13.09, 2007-11-14.04, 2007-11-15.44, and 2007-11-16.04 UT. A bright X-ray source is detected at the position of the SN within a 10 image pixel (23.5-arcsec) aperture centered on the SN, which includes the nucleus of the host galaxy NGC 579 (8-arcsec offset from the SN) in the merged 7.3 ks Swift XRT observations.

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