Swift observations of SN2011it

Details Swift observations of SN2011it Swift observations of SN2011it

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3804....1m&link_type=abstract

The Astronomer's Telegram, #3804

Astronomy and Astrophysics

Astronomy

Ultra-Violet, X-Ray, Supernovae

Scientific paper

SN2011it has been recently classified as a broad-line type-Ic supernova (Tomasella, CBET 2938). A Swift-ToO was executed to observe the field of SN2011it starting from 2011-12-08T00:22:48 UT, with the primary aim to constrain the off-axis X-ray emission from the SN. No X-ray source is detected at the optical position of the transient with a 3 sigma upper limit of 2.4d-3 cts/s in the 0.3-10 keV energy band (total exposure= 8.3 ks).

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