Detection of X-Ray Emission from SN 2005ip with Swift

Details Detection of X-Ray Emission from SN 2005ip with Swift Detection of X-Ray Emission from SN 2005ip with Swift

Feb 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1004....1i&link_type=abstract

The Astronomer's Telegram, #1004

Astronomy and Astrophysics

Astronomy

6

Optical, Ultra-Violet, X-Ray, Novae, Supernovae

Scientific paper

Swift Ultraviolet/Optical Telescope (UVOT) and X-Ray Telescope (XRT) started observing the type II SN 2005ip in NGC 2906 (CBET #275, IAUC #8628) on 2007-02-14.08 UT. The following UVOT magnitudes were measured for SN 2005ip: V = 18.5 (747 s exposure time), B = 18.7 (747 s), U = 18.1 (747 s), UVW1 [181-321nm] = 17.7 (1516 s), UVM2 [166-268 nm] = 18.4 (356 s), and UVW2 [112-264 nm] = 18.4 (3000 s). Statistical and systematic errors are approximately 0.1 mag each.

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