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Detailed Multifrequency Study of a Rapid VHE Flare of Mrk501 in May 2009

机译:2009年5月MRK501快速VHE耀斑的详细多频研究

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We present observations of the gamma-ray blazar Markarian 501 between April 17 and May 5, 2009, with the Whipple 10-m telescope, VERITAS, the Fermi Large Area Telescope (LAT), Swift and RXTE as part of a 4.5-month multi-wavelength campaign. The presentation will focus on the strong very high energy (VHE) gamma-ray activity detected on May 1st with Whipple and VERITAS, when the measured flux (E > 400 GeV) reached five times the flux of the Crab Nebula, coincident with an increase in the optical polarization by a factor of 5, and a rotation of the polarization angle by 15 degrees. We also show that, during this 3-week period, the largest flux and spectral variability is seen at the highest energies of the broadband spectral energy distribution.
机译:我们在4月17日至5月5日至2009年5月5日之间展示了伽马射线布拉泽标记501,惠普斯10米望远镜,Veritas,费米大面积望远镜(LAT),Swift和RXTE,作为4.5个月多的一部分 - 波长活动。当测量的助焊剂(E> 400 GEV)达到螃蟹星云的助焊剂的五倍时,展示将重点关注于5月1日检测到的强烈的非常高能量(VHE)γ射线活动。在光学偏振中倍数5,偏振角旋转15度。我们还表明,在这3周的时间内,在宽带光谱能量分布的最高能量处看到最大的磁通和光谱变异性。

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