Multiwavelength observations and modeling of 1ES 1959+650 in a low flux state
We report on the VERITAS observations of the high-frequency peaked BL Lac object 1ES 1959+650 in the period 2007-2011. This source is detected at TeV energies by VERITAS at 16.4 standard deviation (σ) significance in 7.6 hr of observation in a low flux state. A multiwavelength spectral energy distri...
Guardado en:
Autores principales: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
---|---|
Formato: | JOUR |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v775_n1_p_Aliu |
Aporte de: |
id |
todo:paper_0004637X_v775_n1_p_Aliu |
---|---|
record_format |
dspace |
spelling |
todo:paper_0004637X_v775_n1_p_Aliu2023-10-03T14:02:33Z Multiwavelength observations and modeling of 1ES 1959+650 in a low flux state Aliu, E. Archambault, S. Arlen, T. Aune, T. Beilicke, M. Benbow, W. Bird, R. Böttcher, M. Bouvier, A. Bugaev, V. Byrum, K. Cesarini, A. Ciupik, L. Collins-Hughes, E. Connolly, M.P. Cui, W. Dickherber, R. Duke, C. Dumm, J. Errando, M. Falcone, A. Federici, S. Feng, Q. Finley, J.P. Finnegan, G. Fortson, L. Furniss, A. Galante, N. Gall, D. Gillanders, G.H. Griffin, S. Grube, J. Gyuk, G. Hanna, D. Holder, J. Hughes, G. Humensky, T.B. Kaaret, P. Kertzman, M. Khassen, Y. Kieda, D. Krawczynski, H. Krennrich, F. Lang, M.J. Madhavan, A.S. Maier, G. Majumdar, P. McArthur, S. McCann, A. Moriarty, P. Mukherjee, R. Nelson, T. O'Faoláin De Bhróithe, A. Ong, R.A. Orr, M. Otte, A.N. Park, N. Perkins, J.S. Pichel, A. Pohl, M. Popkow, A. Prokoph, H. Quinn, J. Ragan, K. Reyes, L.C. Reynolds, P.T. Roache, E. Saxon, D.B. Schroedter, M. Sembroski, G.H. Skole, C. Smith, A.W. Staszak, D. Telezhinsky, I. Theiling, M. Tyler, J. Varlotta, A. Vassiliev, V.V. Wakely, S.P. Weekes, T.C. Weinstein, A. Welsing, R. Williams, D.A. Zitzer, B. BL Lacertae objects: general galaxies: active gamma rays: galaxies We report on the VERITAS observations of the high-frequency peaked BL Lac object 1ES 1959+650 in the period 2007-2011. This source is detected at TeV energies by VERITAS at 16.4 standard deviation (σ) significance in 7.6 hr of observation in a low flux state. A multiwavelength spectral energy distribution (SED) is constructed from contemporaneous data from VERITAS, Fermi-LAT, RXTE PCA, and Swift UVOT. Swift XRT data is not included in the SED due to a lack of simultaneous observations with VERITAS. In contrast to the orphan γ-ray flare exhibited by this source in 2002, the X-ray flux of the source is found to vary by an order of magnitude, while other energy regimes exhibit less variable emission. A quasi-equilibrium synchrotron self-Compton model with an additional external radiation field is used to describe three SEDs corresponding to the lowest, highest, and average X-ray states. The variation in the X-ray spectrum is modeled by changing the electron injection spectral index, with minor adjustments of the kinetic luminosity in electrons. This scenario produces small-scale flux variability of the order of ≲ 2 in the high energy (E > 1 MeV) and very high energy (E > 100 GeV) γ-ray regimes, which is corroborated by the Fermi-LAT, VERITAS, and Whipple 10 m telescope light curves. © 2013. The American Astronomical Society. All rights reserved.. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_0004637X_v775_n1_p_Aliu |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
BL Lacertae objects: general galaxies: active gamma rays: galaxies |
spellingShingle |
BL Lacertae objects: general galaxies: active gamma rays: galaxies Aliu, E. Archambault, S. Arlen, T. Aune, T. Beilicke, M. Benbow, W. Bird, R. Böttcher, M. Bouvier, A. Bugaev, V. Byrum, K. Cesarini, A. Ciupik, L. Collins-Hughes, E. Connolly, M.P. Cui, W. Dickherber, R. Duke, C. Dumm, J. Errando, M. Falcone, A. Federici, S. Feng, Q. Finley, J.P. Finnegan, G. Fortson, L. Furniss, A. Galante, N. Gall, D. Gillanders, G.H. Griffin, S. Grube, J. Gyuk, G. Hanna, D. Holder, J. Hughes, G. Humensky, T.B. Kaaret, P. Kertzman, M. Khassen, Y. Kieda, D. Krawczynski, H. Krennrich, F. Lang, M.J. Madhavan, A.S. Maier, G. Majumdar, P. McArthur, S. McCann, A. Moriarty, P. Mukherjee, R. Nelson, T. O'Faoláin De Bhróithe, A. Ong, R.A. Orr, M. Otte, A.N. Park, N. Perkins, J.S. Pichel, A. Pohl, M. Popkow, A. Prokoph, H. Quinn, J. Ragan, K. Reyes, L.C. Reynolds, P.T. Roache, E. Saxon, D.B. Schroedter, M. Sembroski, G.H. Skole, C. Smith, A.W. Staszak, D. Telezhinsky, I. Theiling, M. Tyler, J. Varlotta, A. Vassiliev, V.V. Wakely, S.P. Weekes, T.C. Weinstein, A. Welsing, R. Williams, D.A. Zitzer, B. Multiwavelength observations and modeling of 1ES 1959+650 in a low flux state |
topic_facet |
BL Lacertae objects: general galaxies: active gamma rays: galaxies |
description |
We report on the VERITAS observations of the high-frequency peaked BL Lac object 1ES 1959+650 in the period 2007-2011. This source is detected at TeV energies by VERITAS at 16.4 standard deviation (σ) significance in 7.6 hr of observation in a low flux state. A multiwavelength spectral energy distribution (SED) is constructed from contemporaneous data from VERITAS, Fermi-LAT, RXTE PCA, and Swift UVOT. Swift XRT data is not included in the SED due to a lack of simultaneous observations with VERITAS. In contrast to the orphan γ-ray flare exhibited by this source in 2002, the X-ray flux of the source is found to vary by an order of magnitude, while other energy regimes exhibit less variable emission. A quasi-equilibrium synchrotron self-Compton model with an additional external radiation field is used to describe three SEDs corresponding to the lowest, highest, and average X-ray states. The variation in the X-ray spectrum is modeled by changing the electron injection spectral index, with minor adjustments of the kinetic luminosity in electrons. This scenario produces small-scale flux variability of the order of ≲ 2 in the high energy (E > 1 MeV) and very high energy (E > 100 GeV) γ-ray regimes, which is corroborated by the Fermi-LAT, VERITAS, and Whipple 10 m telescope light curves. © 2013. The American Astronomical Society. All rights reserved.. |
format |
JOUR |
author |
Aliu, E. Archambault, S. Arlen, T. Aune, T. Beilicke, M. Benbow, W. Bird, R. Böttcher, M. Bouvier, A. Bugaev, V. Byrum, K. Cesarini, A. Ciupik, L. Collins-Hughes, E. Connolly, M.P. Cui, W. Dickherber, R. Duke, C. Dumm, J. Errando, M. Falcone, A. Federici, S. Feng, Q. Finley, J.P. Finnegan, G. Fortson, L. Furniss, A. Galante, N. Gall, D. Gillanders, G.H. Griffin, S. Grube, J. Gyuk, G. Hanna, D. Holder, J. Hughes, G. Humensky, T.B. Kaaret, P. Kertzman, M. Khassen, Y. Kieda, D. Krawczynski, H. Krennrich, F. Lang, M.J. Madhavan, A.S. Maier, G. Majumdar, P. McArthur, S. McCann, A. Moriarty, P. Mukherjee, R. Nelson, T. O'Faoláin De Bhróithe, A. Ong, R.A. Orr, M. Otte, A.N. Park, N. Perkins, J.S. Pichel, A. Pohl, M. Popkow, A. Prokoph, H. Quinn, J. Ragan, K. Reyes, L.C. Reynolds, P.T. Roache, E. Saxon, D.B. Schroedter, M. Sembroski, G.H. Skole, C. Smith, A.W. Staszak, D. Telezhinsky, I. Theiling, M. Tyler, J. Varlotta, A. Vassiliev, V.V. Wakely, S.P. Weekes, T.C. Weinstein, A. Welsing, R. Williams, D.A. Zitzer, B. |
author_facet |
Aliu, E. Archambault, S. Arlen, T. Aune, T. Beilicke, M. Benbow, W. Bird, R. Böttcher, M. Bouvier, A. Bugaev, V. Byrum, K. Cesarini, A. Ciupik, L. Collins-Hughes, E. Connolly, M.P. Cui, W. Dickherber, R. Duke, C. Dumm, J. Errando, M. Falcone, A. Federici, S. Feng, Q. Finley, J.P. Finnegan, G. Fortson, L. Furniss, A. Galante, N. Gall, D. Gillanders, G.H. Griffin, S. Grube, J. Gyuk, G. Hanna, D. Holder, J. Hughes, G. Humensky, T.B. Kaaret, P. Kertzman, M. Khassen, Y. Kieda, D. Krawczynski, H. Krennrich, F. Lang, M.J. Madhavan, A.S. Maier, G. Majumdar, P. McArthur, S. McCann, A. Moriarty, P. Mukherjee, R. Nelson, T. O'Faoláin De Bhróithe, A. Ong, R.A. Orr, M. Otte, A.N. Park, N. Perkins, J.S. Pichel, A. Pohl, M. Popkow, A. Prokoph, H. Quinn, J. Ragan, K. Reyes, L.C. Reynolds, P.T. Roache, E. Saxon, D.B. Schroedter, M. Sembroski, G.H. Skole, C. Smith, A.W. Staszak, D. Telezhinsky, I. Theiling, M. Tyler, J. Varlotta, A. Vassiliev, V.V. Wakely, S.P. Weekes, T.C. Weinstein, A. Welsing, R. Williams, D.A. Zitzer, B. |
author_sort |
Aliu, E. |
title |
Multiwavelength observations and modeling of 1ES 1959+650 in a low flux state |
title_short |
Multiwavelength observations and modeling of 1ES 1959+650 in a low flux state |
title_full |
Multiwavelength observations and modeling of 1ES 1959+650 in a low flux state |
title_fullStr |
Multiwavelength observations and modeling of 1ES 1959+650 in a low flux state |
title_full_unstemmed |
Multiwavelength observations and modeling of 1ES 1959+650 in a low flux state |
title_sort |
multiwavelength observations and modeling of 1es 1959+650 in a low flux state |
url |
http://hdl.handle.net/20.500.12110/paper_0004637X_v775_n1_p_Aliu |
work_keys_str_mv |
AT aliue multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT archambaults multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT arlent multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT aunet multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT beilickem multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT benboww multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT birdr multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT bottcherm multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT bouviera multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT bugaevv multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT byrumk multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT cesarinia multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT ciupikl multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT collinshughese multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT connollymp multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT cuiw multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT dickherberr multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT dukec multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT dummj multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT errandom multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT falconea multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT federicis multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT fengq multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT finleyjp multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT finnegang multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT fortsonl multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT furnissa multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT galanten multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT galld multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT gillandersgh multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT griffins multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT grubej multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT gyukg multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT hannad multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT holderj multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT hughesg multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT humenskytb multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT kaaretp multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT kertzmanm multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT khasseny multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT kiedad multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT krawczynskih multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT krennrichf multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT langmj multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT madhavanas multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT maierg multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT majumdarp multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT mcarthurs multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT mccanna multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT moriartyp multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT mukherjeer multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT nelsont multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT ofaolaindebhroithea multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT ongra multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT orrm multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT ottean multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT parkn multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT perkinsjs multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT pichela multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT pohlm multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT popkowa multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT prokophh multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT quinnj multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT ragank multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT reyeslc multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT reynoldspt multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT roachee multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT saxondb multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT schroedterm multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT sembroskigh multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT skolec multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT smithaw multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT staszakd multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT telezhinskyi multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT theilingm multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT tylerj multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT varlottaa multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT vassilievvv multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT wakelysp multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT weekestc multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT weinsteina multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT welsingr multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT williamsda multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate AT zitzerb multiwavelengthobservationsandmodelingof1es1959650inalowfluxstate |
_version_ |
1807318446807973888 |