Continued Swift/UVOT Monitoring of PTF11kly / SN2011fe

Details Continued Swift/UVOT Monitoring of PTF11kly / SN2011fe Continued Swift/UVOT Monitoring of PTF11kly / SN2011fe

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3594....1c&link_type=abstract

The Astronomer's Telegram, #3594

Astronomy and Astrophysics

Astronomy

Optical, Ultra-Violet, Supernovae, Transient

Scientific paper

The UV-Optical Telescope on Swift has continued to monitor the field of PTF11kly / SN2011fe (ATEL #3581). In an orbit beginning at 00:01:40 UT on 2011 August 26, we report the following preliminary AB magnitudes: V: 13.83 & 0.03 B: 13.99 ± 0.03 U: 15.26 ± 0.03 UVW1: 17.33 ± 0.05 UVM2: 18.92 ± 0.08 UVW2: 18.48 ± 0.07 Compared with the first epoch of UVOT imaging (ATEL #3590), the supernova has brightened significantly in all filters.

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