Optical follow-up of SN2011ek

Details Optical follow-up of SN2011ek Optical follow-up of SN2011ek

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3550....1n&link_type=abstract

The Astronomer's Telegram, #3550

Physics

Optical

Scientific paper

Prompted by ATel #3541 and CBET #2783, we observed the Supernova with the remote controlled TACOR 23.5cm telescope on top of the Department of Physics of La Sapienza University, Rome Italy, equipped with an Apogee U2 camera and R (Cousins) filter. A comparison sequence was taken from GSC2.3 catalogue. The source was at R=14.58 ± 0.05 on August 11 00:30 UT (JD 2,455,784.521); it is therefore brighter than the discovery report (CBET #2783) as expected for a SN still in the rising phase.

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