Detailed multifrequency study of a rapid VHE flare of mrk501 in May 2009

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...

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Publicado: 2011
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Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_NIS23770_v8_n_p173_Pichel
http://hdl.handle.net/20.500.12110/paper_NIS23770_v8_n_p173_Pichel
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spelling paper:paper_NIS23770_v8_n_p173_Pichel2023-06-08T16:40:03Z Detailed multifrequency study of a rapid VHE flare of mrk501 in May 2009 Blazars Gamma rays Whipple telescope Cosmic rays Gamma rays Blazars Large area telescopes Multi frequency Multi-wavelength campaigns Polarization angle Spectral energy distribution Spectral variability Very high energies Telescopes 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. 2011 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_NIS23770_v8_n_p173_Pichel http://hdl.handle.net/20.500.12110/paper_NIS23770_v8_n_p173_Pichel
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Blazars
Gamma rays
Whipple telescope
Cosmic rays
Gamma rays
Blazars
Large area telescopes
Multi frequency
Multi-wavelength campaigns
Polarization angle
Spectral energy distribution
Spectral variability
Very high energies
Telescopes
spellingShingle Blazars
Gamma rays
Whipple telescope
Cosmic rays
Gamma rays
Blazars
Large area telescopes
Multi frequency
Multi-wavelength campaigns
Polarization angle
Spectral energy distribution
Spectral variability
Very high energies
Telescopes
Detailed multifrequency study of a rapid VHE flare of mrk501 in May 2009
topic_facet Blazars
Gamma rays
Whipple telescope
Cosmic rays
Gamma rays
Blazars
Large area telescopes
Multi frequency
Multi-wavelength campaigns
Polarization angle
Spectral energy distribution
Spectral variability
Very high energies
Telescopes
description 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.
title Detailed multifrequency study of a rapid VHE flare of mrk501 in May 2009
title_short Detailed multifrequency study of a rapid VHE flare of mrk501 in May 2009
title_full Detailed multifrequency study of a rapid VHE flare of mrk501 in May 2009
title_fullStr Detailed multifrequency study of a rapid VHE flare of mrk501 in May 2009
title_full_unstemmed Detailed multifrequency study of a rapid VHE flare of mrk501 in May 2009
title_sort detailed multifrequency study of a rapid vhe flare of mrk501 in may 2009
publishDate 2011
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_NIS23770_v8_n_p173_Pichel
http://hdl.handle.net/20.500.12110/paper_NIS23770_v8_n_p173_Pichel
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