Swift UVOT detection of SN2011ek

Details Swift UVOT detection of SN2011ek Swift UVOT detection of SN2011ek

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3541....1x&link_type=abstract

The Astronomer's Telegram, #3541

Astronomy and Astrophysics

Astronomy

Ultra-Violet, X-Ray, Supernovae

Scientific paper

The Swift satellite began observing SN2011ek (CBETs #2783 and #2785) on August 9th, 2011. The UVOT data show a relatively bright source coincident with the location of the supernova. Including possible contamination from the host galaxy, we measure the following preliminary magnitudes: UT(midtime) Filter Mag(AB) MagErr 0.7223 V 15.22 0.04 0.7120 B 15.82 0.03 0.7101 U 17.43 0.07 0.7072 UVW1 19.62 0.14 0.7297 UVM2 >22.31 N/A 0.7167 UVW2 21.43 0.22 There is no source detected by the XRT at this position, roughly corresponding to a 3sigma upper limit of 4x10-13 erg/cm2/s.

Affiliated with

Also associated with

No associations

Rating

Swift UVOT detection of SN2011ek does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Swift UVOT detection of SN2011ek, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Swift UVOT detection of SN2011ek will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1021868