Fermi Large Area Telescope Gamma-Ray Detection of the Radio Galaxy M87
The Fermi LAT Collaboration: A.A. Abdo, et al., D.E. Harris, F., Massaro, L. Stawarz

TL;DR
The Fermi-LAT telescope detected gamma-ray emission from the radio galaxy M87, marking it as the third such galaxy observed in high-energy gamma rays, with the emission consistent with a synchrotron self-Compton model and no significant variability.
Contribution
This paper reports the first detection of gamma-ray emission from M87 by Fermi-LAT, expanding the class of radio galaxies observed in high-energy gamma rays and analyzing its spectral properties.
Findings
Gamma-ray emission from M87 is consistent with SSC models.
No significant gamma-ray variability was observed over ten months.
The gamma-ray flux is comparable to previous upper limits from EGRET.
Abstract
We report the Fermi-LAT discovery of high-energy (MeV/GeV) gamma-ray emission positionally consistent with the center of the radio galaxy M87, at a source significance of over 10 sigma in ten-months of all-sky survey data. Following the detections of Cen A and Per A, this makes M87 the third radio galaxy seen with the LAT. The faint point-like gamma-ray source has a >100 MeV flux of 2.45 (+/- 0.63) x 10^-8 ph cm^-2 s^-1 (photon index = 2.26 +/- 0.13) with no significant variability detected within the LAT observation. This flux is comparable with the previous EGRET upper limit (< 2.18 x 10^-8 ph cm^-2 s^-1, 2 sigma), thus there is no evidence for a significant MeV/GeV flare on decade timescales. Contemporaneous Chandra and VLBA data indicate low activity in the unresolved X-ray and radio core relative to previous observations, suggesting M87 is in a quiescent overall level over the…
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