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

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

Jan 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel..981....1i&link_type=abstract

The Astronomer's Telegram, #981

Astronomy and Astrophysics

Astronomy

1

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

Scientific paper

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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