AGILE monitoring of the strongly variable gamma-ray emission from the Crab Nebula

Details AGILE monitoring of the strongly variable gamma-ray emission from the Crab Nebula AGILE monitoring of the strongly variable gamma-ray emission from the Crab Nebula

Apr 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3286....1s&link_type=abstract

The Astronomer's Telegram, #3286

Astronomy and Astrophysics

Astronomy

2

Gamma Ray, Neutron Star, Supernova Remnant, Transient, Pulsar

Scientific paper

Strongly variable gamma-ray emission above 100 MeV continues to be detected by AGILE from a source positionally consistent with the Crab Nebula. After a telemetry gap that AGILE experienced on April 14, 2011 (in partial coincidence with the strong gamma-ray flare reported by Fermi-LAT in ATel # 3284) the AGILE-GRID detected the following gamma-ray flux above 100 MeV (pulsar plus nebula): MJD=55666.44-55667.44, 2011-04-15 10:40 UT - 2011-04-16 10:38 UT, F = (19.6 ± 3.7) 10^{-6} ph/cm2/sec.

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