Swift observations of SN2011hs

Details Swift observations of SN2011hs Swift observations of SN2011hs

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3768....1m&link_type=abstract

The Astronomer's Telegram, #3768

Astronomy and Astrophysics

Astronomy

Ultra-Violet, X-Ray, Supernovae

Scientific paper

The spectral properties of SN2011hs show a good match to the energetic type-IIb 'hypernova' 2003bg approximately 15 days before maximum light (Milisavljevic CBET 2902). A Swift-ToO was executed to observe the field of SN2011hs starting from 2011-11-15T16:28:36 UT. No X-ray source is detected at the optical position of the transient (RA=22:57:11.77 dec=-43:23:4.8) with a 3 sigma upper limit of 2.3d-3 cts/s in the 0.3-10 keV energy band (total exposure= 9.3 ks).

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