PTF observations of SN2012aw (PTF12bvh) and explosion date constraints

Details PTF observations of SN2012aw (PTF12bvh) and explosion date constraints PTF observations of SN2012aw (PTF12bvh) and explosion date constraints

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012atel.3996....1p&link_type=abstract

The Astronomer's Telegram, #3996

Astronomy and Astrophysics

Astronomy

Optical, Supernovae

Scientific paper

The PTF (ATEL #1964, #3253; http://www.astro.caltech.edu/ptf/ ; Law et al. 2009, PASP, 121, 1395; Rau et al. 2009, PASP, 121, 1334) reports observations of SN2012aw (Fagotti 2012, CBET #3054), which we designate internally as PTF12bvh. The SN is well detected on two images taken on March 17.18 at an R band magnitude of ~14.1 (calibrated relative to USNO-B1), with an uncertain systematic offset due to strong light contamination by the planet Mars.

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