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VERITAS OBSERVATIONS OF DAY-SCALE FLARING OF M 87 IN 2010 APRIL
Journal article   Open access   Peer reviewed

VERITAS OBSERVATIONS OF DAY-SCALE FLARING OF M 87 IN 2010 APRIL

E Aliu, T Arlen, A Cannon, A Cesarini, L Ciupik, E COLLINS-HUGHES, M. P Connolly, W Cui, R Dickherber, C Duke, …
The Astrophysical journal, Vol.746(2), 141
2012
DOI: 10.1088/0004-637X/746/2/141
url
https://doi.org/10.1088/0004-637X/746/2/141View
Published (Version of record) Open Access

Abstract

VERITAS has been monitoring the very-high-energy (VHE; > 100 GeV) gamma-ray activity of the radio galaxy M 87 since 2007. During 2008, flaring activity on a timescale of a few days was observed with a peak flux of (0.70  ±  0.16) × 10−11 cm−2 s−1 at energies above 350 GeV. In 2010 April, VERITAS detected a flare from M 87 with peak flux of (2.71  ±  0.68) × 10−11 cm−2 s−1 for E > 350 GeV. The source was observed for six consecutive nights during the flare, resulting in a total of 21 hr of good-quality data. The most rapid flux variation occurred on the trailing edge of the flare with an exponential flux decay time of 0.90+0.22−0.15 days. The shortest detected exponential rise time is three times as long, at 2.87+1.65−0.99 days. The quality of the data sample is such that spectral analysis can be performed for three periods: rising flux, peak flux, and falling flux. The spectra obtained are consistent with power-law forms. The spectral index at the peak of the flare is equal to 2.19  ±  0.07. There is some indication that the spectrum is softer in the falling phase of the flare than the peak phase, with a confidence level corresponding to 3.6 standard deviations. We discuss the implications of these results for the acceleration and cooling rates of VHE electrons in M 87 and the constraints they provide on the physical size of the emitting region.
Astronomy Earth, ocean, space Exact sciences and technology

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