Bounds to the gamma--ray flux emitted by SN 2011fe before the maximum of light as obtained by INTEGRAL/SPI

Details Bounds to the gamma--ray flux emitted by SN 2011fe before the maximum of light as obtained by INTEGRAL/SPI Bounds to the gamma--ray flux emitted by SN 2011fe before the maximum of light as obtained by INTEGRAL/SPI

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3683....1i&link_type=abstract

The Astronomer's Telegram, #3683

Astronomy and Astrophysics

Astronomy

1

Gamma Ray, Supernovae

Scientific paper

SN2011fe (RA = 14:03:05.81, Dec = +54:16:25.4; J2000) is a Type Ia supernovae that was discovered in M101 on August 24th 2011, about one day after the explosion by the Palomar Transient Factory (Nugent et al, ATEL #3581). The optical maximum was reached around September 10th-11th. The prospected gamma-ray emission maximum in radioactive decay lines should be around 70-100 days after the explosion.

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