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

A. PICHEL FOR THE VERITAS COLLABORATION, D. PANEQUE FOR THE FERMI/LAT COLLABORATION

Beijing

Conferencia; 32th International Cosmic Ray Conference; 2011

ICRC

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 multiwavelength 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.