Multiwavelength observations of mrk 501 in 2008

The well-studied VHE (E > 100 GeV) blazar Mrk 501 was observed between March and May 2008 as part of an extensive multiwavelength observation campaign including radio, optical, X-ray and VHE gamma-ray instruments. Mrk 501 was in a low state of activity during the campaign, with a low VHE flux of...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Kranich, D., Paneque, D., Cesarini, A., Falcone, A., Giroletti, M., Hoversten, E., Hovatta, T., Kovalev, Y.Y., Lähteenmäki, A., Nieppola, E., Pagani, C., Pichel, A., Satalecka, K., Scargle, J., Steele, D., Tavecchio, F., Tescaro, D., Tornikoski, M., Villata, M.
Formato: CONF
Materias:
Blazar
Mrk 501
SSC model
Gamma rays
Crab Nebula flux
Energy dependent
High-energy electron
Multiwavelength observations
Spectral energy distribution
SSC models
Cosmic rays
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_NIS23286_v_n_p_Kranich
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id todo:paper_NIS23286_v_n_p_Kranich
record_format dspace
spelling todo:paper_NIS23286_v_n_p_Kranich2023-10-03T16:46:21Z Multiwavelength observations of mrk 501 in 2008 Kranich, D. Paneque, D. Cesarini, A. Falcone, A. Giroletti, M. Hoversten, E. Hovatta, T. Kovalev, Y.Y. Lähteenmäki, A. Nieppola, E. Pagani, C. Pichel, A. Satalecka, K. Scargle, J. Steele, D. Tavecchio, F. Tescaro, D. Tornikoski, M. Villata, M. Blazar Mrk 501 SSC model Gamma rays Blazar Crab Nebula flux Energy dependent High-energy electron Mrk 501 Multiwavelength observations Spectral energy distribution SSC models Cosmic rays The well-studied VHE (E > 100 GeV) blazar Mrk 501 was observed between March and May 2008 as part of an extensive multiwavelength observation campaign including radio, optical, X-ray and VHE gamma-ray instruments. Mrk 501 was in a low state of activity during the campaign, with a low VHE flux of about 20% the Crab Nebula flux. Nevertheless, significant flux variations could be observed in X-rays as well as -rays. Overall Mrk 501 showed increased variability when going from radio to -ray energies. The broadband spectral energy distribution during the two different emission states of the campaign was well described by a homogeneous one-zone synchrotron self-Compton model. The high emission state was satisfactorily modeled by increasing the amount of high energy electrons with respect to the low emission state. This parameterization is consistent with the energy-dependent variability trend observed during the campaign. CONF info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_NIS23286_v_n_p_Kranich
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Blazar
Mrk 501
SSC model
Gamma rays
Blazar
Crab Nebula flux
Energy dependent
High-energy electron
Mrk 501
Multiwavelength observations
Spectral energy distribution
SSC models
Cosmic rays
spellingShingle Blazar
Mrk 501
SSC model
Gamma rays
Blazar
Crab Nebula flux
Energy dependent
High-energy electron
Mrk 501
Multiwavelength observations
Spectral energy distribution
SSC models
Cosmic rays
Kranich, D.
Paneque, D.
Cesarini, A.
Falcone, A.
Giroletti, M.
Hoversten, E.
Hovatta, T.
Kovalev, Y.Y.
Lähteenmäki, A.
Nieppola, E.
Pagani, C.
Pichel, A.
Satalecka, K.
Scargle, J.
Steele, D.
Tavecchio, F.
Tescaro, D.
Tornikoski, M.
Villata, M.
Multiwavelength observations of mrk 501 in 2008
topic_facet Blazar
Mrk 501
SSC model
Gamma rays
Blazar
Crab Nebula flux
Energy dependent
High-energy electron
Mrk 501
Multiwavelength observations
Spectral energy distribution
SSC models
Cosmic rays
description The well-studied VHE (E > 100 GeV) blazar Mrk 501 was observed between March and May 2008 as part of an extensive multiwavelength observation campaign including radio, optical, X-ray and VHE gamma-ray instruments. Mrk 501 was in a low state of activity during the campaign, with a low VHE flux of about 20% the Crab Nebula flux. Nevertheless, significant flux variations could be observed in X-rays as well as -rays. Overall Mrk 501 showed increased variability when going from radio to -ray energies. The broadband spectral energy distribution during the two different emission states of the campaign was well described by a homogeneous one-zone synchrotron self-Compton model. The high emission state was satisfactorily modeled by increasing the amount of high energy electrons with respect to the low emission state. This parameterization is consistent with the energy-dependent variability trend observed during the campaign.
format CONF
author Kranich, D.
Paneque, D.
Cesarini, A.
Falcone, A.
Giroletti, M.
Hoversten, E.
Hovatta, T.
Kovalev, Y.Y.
Lähteenmäki, A.
Nieppola, E.
Pagani, C.
Pichel, A.
Satalecka, K.
Scargle, J.
Steele, D.
Tavecchio, F.
Tescaro, D.
Tornikoski, M.
Villata, M.
author_facet Kranich, D.
Paneque, D.
Cesarini, A.
Falcone, A.
Giroletti, M.
Hoversten, E.
Hovatta, T.
Kovalev, Y.Y.
Lähteenmäki, A.
Nieppola, E.
Pagani, C.
Pichel, A.
Satalecka, K.
Scargle, J.
Steele, D.
Tavecchio, F.
Tescaro, D.
Tornikoski, M.
Villata, M.
author_sort Kranich, D.
title Multiwavelength observations of mrk 501 in 2008
title_short Multiwavelength observations of mrk 501 in 2008
title_full Multiwavelength observations of mrk 501 in 2008
title_fullStr Multiwavelength observations of mrk 501 in 2008
title_full_unstemmed Multiwavelength observations of mrk 501 in 2008
title_sort multiwavelength observations of mrk 501 in 2008
url http://hdl.handle.net/20.500.12110/paper_NIS23286_v_n_p_Kranich
work_keys_str_mv AT kranichd multiwavelengthobservationsofmrk501in2008
AT panequed multiwavelengthobservationsofmrk501in2008
AT cesarinia multiwavelengthobservationsofmrk501in2008
AT falconea multiwavelengthobservationsofmrk501in2008
AT girolettim multiwavelengthobservationsofmrk501in2008
AT hoverstene multiwavelengthobservationsofmrk501in2008
AT hovattat multiwavelengthobservationsofmrk501in2008
AT kovalevyy multiwavelengthobservationsofmrk501in2008
AT lahteenmakia multiwavelengthobservationsofmrk501in2008
AT nieppolae multiwavelengthobservationsofmrk501in2008
AT paganic multiwavelengthobservationsofmrk501in2008
AT pichela multiwavelengthobservationsofmrk501in2008
AT sataleckak multiwavelengthobservationsofmrk501in2008
AT scarglej multiwavelengthobservationsofmrk501in2008
AT steeled multiwavelengthobservationsofmrk501in2008
AT tavecchiof multiwavelengthobservationsofmrk501in2008
AT tescarod multiwavelengthobservationsofmrk501in2008
AT tornikoskim multiwavelengthobservationsofmrk501in2008
AT villatam multiwavelengthobservationsofmrk501in2008
_version_ 1782030722187395072

Ejemplares similares