Daily Photometry Of SN 2011fe, The Youngest Type Ia Supernova, From u Through K-band

Details Daily Photometry Of SN 2011fe, The Youngest Type Ia Supernova, From u Through K-band Daily Photometry Of SN 2011fe, The Youngest Type Ia Supernova, From u Through K-band

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21924223b&link_type=abstract

American Astronomical Society, AAS Meeting #219, #242.23

Astronomy and Astrophysics

Astronomy

Scientific paper

SN 2011fe is the youngest SNIa ever discovered, identified in the PTF images only hours after explosion. The LCOGT network followed this SN with daily cadence in optical (ugri) bands, with high cadence observations in g and i, while UKIRT collected daily cadence near infrared data. Here we analyze daily photometry, including a bolometric lightcurve, of SN 2011fe starting a day after explosion through 15 days after maximum.

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