Continued Swift monitoring campaign of SN2011fe

Details Continued Swift monitoring campaign of SN2011fe Continued Swift monitoring campaign of SN2011fe

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3642....1m&link_type=abstract

The Astronomer's Telegram, #3642

Astronomy and Astrophysics

Astronomy

1

Ultra-Violet, X-Ray, Supernovae

Scientific paper

Swift has continued to monitor the evolution of the type Ia SN2011fe since its discovery (Atel #3581) providing the best sampled UV light-curve of a type Ia SN at very early times, ever. Compared to the first epoch of Swift-UVOT observations (Atel #3590) the SN has brightened of ~4.5 mag, ~5 mag and ~6 mag in the uvm2, uvw2 and uvw1 filter, respectively. Assuming August 23rd to be the date of the SN explosion, SN2011fe reached an observed peak magnitude of ~10.9 in the uvw1 band at day 16th.

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