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

机译:2009年5月对Mrk501的快速VHE耀斑进行的详细多频研究

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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:我们提供了2009年4月17日至5月5日之间的伽玛射线Blazar Markarian 501观测资料,其中包括Whipple 10米望远镜,VERITAS,费米大面积望远镜(LAT),Swift和RXTE,作为4.5个月多次观测的一部分-波长运动。本演讲将重点介绍5月1日用Whipple和VERITAS检测到的强甚高能量(VHE)伽马射线活动,当时测得的通量(E> 400 GeV)达到蟹状星云通量的五倍,同时增加偏振角为5倍,偏振角旋转15度。我们还表明,在这三周的时间内,在宽带频谱能量分布的最高能量处看到了最大的通量和频谱变化。

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