Veritas 2008-2009 monitoring of the variable gamma-ray source M87
M87 is a nearby radio galaxy that is detected at energies ranging from radio to very high energy (VHE) gamma rays. Its proximity and its jet, misaligned from our line of sight, enable detailed morphological studies and extensive modeling at radio, optical, and X-ray energies. Flaring activity was ob...
Guardado en:
Autores principales: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
---|---|
Formato: | JOUR |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v716_n1_p819_Acciari |
Aporte de: |
id |
todo:paper_0004637X_v716_n1_p819_Acciari |
---|---|
record_format |
dspace |
spelling |
todo:paper_0004637X_v716_n1_p819_Acciari2023-10-03T14:02:12Z Veritas 2008-2009 monitoring of the variable gamma-ray source M87 Acciari, V.A. Aliu, E. Arlen, T. Aune, T. Beilicke, M. Benbow, W. Boltuch, D. Bradbury, S.M. Buckley, J.H. Bugaev, V. Byrum, K. Cannon, A. Cesarini, A. Chow, Y.C. Ciupik, L. Cogan, P. Cui, W. Dickherber, R. Duke, C. Finley, J.P. Finnegan, G. Fortin, P. Fortson, L. Furniss, A. Galante, N. Gall, D. Gillanders, G.H. Godambe, S. Grube, J. Guenette, R. Gyuk, G. Hanna, D. Holder, J. Hui, C.M. Humensky, T.B. Imran, A. Kaaret, P. Karlsson, N. Kertzman, M. Kieda, D. Konopelko, A. Krawczynski, H. Krennrich, F. Lang, M.J. Lebohec, S. Maier, G. McArthur, S. McCann, A. McCutcheon, M. Millis, J. Moriarty, P. Ong, R.A. Otte, A.N. Pandel, D. Perkins, J.S. Pichel, A. Pohl, M. Quinn, J. Ragan, K. Reyes, L.C. Reynolds, P.T. Roache, E. Rose, H.J. Rovero, A.C. Schroedter, M. Sembroski, G.H. Senturk, G.D. Smith, A.W. Steele, D. Swordy, S.P. Theiling, M. Thibadeau, S. Varlotta, A. Vincent, S. Wagner, R.G. Wakely, S.P. Ward, J.E. Weekes, T.C. Weinstein, A. Weisgarber, T. Williams, D.A. Wissel, S. Wood, M. Zitzer, B. Harris, D.E. Massaro, F. Gamma rays: galaxies M87 is a nearby radio galaxy that is detected at energies ranging from radio to very high energy (VHE) gamma rays. Its proximity and its jet, misaligned from our line of sight, enable detailed morphological studies and extensive modeling at radio, optical, and X-ray energies. Flaring activity was observed at all energies, and multi-wavelength correlations would help clarify the origin of the VHE emission. In this paper, we describe a detailed temporal and spectral analysis of the VERITAS VHE gamma-ray observations of M87 in 2008 and 2009. In the 2008 observing season, VERITAS detected an excess with a statistical significance of 7.2 standard deviations (σ) from M87 during a joint multi-wavelength monitoring campaign conducted by three major VHE experiments along with the Chandra X-ray Observatory. In 2008 February, VERITAS observed a VHE flare from M87 occurring over a 4 day timespan. The peak nightly flux above 250GeV was (1.14 0.26) × 10 -11 cm -2 s -1 , which corresponded to 7.7% of the Crab Nebula flux. M87 was marginally detected before this 4 day flare period, and was not detected afterward. Spectral analysis of the VERITAS observations showed no significant change in the photon index between the flare and pre-flare states. Shortly after the VHE flare seen by VERITAS, the Chandra X-ray Observatory detected the flux from the core of M87 at a historical maximum, while the flux from the nearby knot HST-1 remained quiescent. Acciari etal. presented the 2008 contemporaneous VHE gamma-ray, Chandra X-ray, and Very Long Baseline Array radio observations which suggest the core as the most likely source of VHE emission, in contrast to the 2005 VHE flare that was simultaneous with an X-ray flare in the HST-1 knot. In 2009, VERITAS continued its monitoring of M87 and marginally detected a 4.2σ excess corresponding to a flux of 1% of the Crab Nebula. No VHE flaring activity was observed in 2009. © 2010. 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_v716_n1_p819_Acciari |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Gamma rays: galaxies |
spellingShingle |
Gamma rays: galaxies Acciari, V.A. Aliu, E. Arlen, T. Aune, T. Beilicke, M. Benbow, W. Boltuch, D. Bradbury, S.M. Buckley, J.H. Bugaev, V. Byrum, K. Cannon, A. Cesarini, A. Chow, Y.C. Ciupik, L. Cogan, P. Cui, W. Dickherber, R. Duke, C. Finley, J.P. Finnegan, G. Fortin, P. Fortson, L. Furniss, A. Galante, N. Gall, D. Gillanders, G.H. Godambe, S. Grube, J. Guenette, R. Gyuk, G. Hanna, D. Holder, J. Hui, C.M. Humensky, T.B. Imran, A. Kaaret, P. Karlsson, N. Kertzman, M. Kieda, D. Konopelko, A. Krawczynski, H. Krennrich, F. Lang, M.J. Lebohec, S. Maier, G. McArthur, S. McCann, A. McCutcheon, M. Millis, J. Moriarty, P. Ong, R.A. Otte, A.N. Pandel, D. Perkins, J.S. Pichel, A. Pohl, M. Quinn, J. Ragan, K. Reyes, L.C. Reynolds, P.T. Roache, E. Rose, H.J. Rovero, A.C. Schroedter, M. Sembroski, G.H. Senturk, G.D. Smith, A.W. Steele, D. Swordy, S.P. Theiling, M. Thibadeau, S. Varlotta, A. Vincent, S. Wagner, R.G. Wakely, S.P. Ward, J.E. Weekes, T.C. Weinstein, A. Weisgarber, T. Williams, D.A. Wissel, S. Wood, M. Zitzer, B. Harris, D.E. Massaro, F. Veritas 2008-2009 monitoring of the variable gamma-ray source M87 |
topic_facet |
Gamma rays: galaxies |
description |
M87 is a nearby radio galaxy that is detected at energies ranging from radio to very high energy (VHE) gamma rays. Its proximity and its jet, misaligned from our line of sight, enable detailed morphological studies and extensive modeling at radio, optical, and X-ray energies. Flaring activity was observed at all energies, and multi-wavelength correlations would help clarify the origin of the VHE emission. In this paper, we describe a detailed temporal and spectral analysis of the VERITAS VHE gamma-ray observations of M87 in 2008 and 2009. In the 2008 observing season, VERITAS detected an excess with a statistical significance of 7.2 standard deviations (σ) from M87 during a joint multi-wavelength monitoring campaign conducted by three major VHE experiments along with the Chandra X-ray Observatory. In 2008 February, VERITAS observed a VHE flare from M87 occurring over a 4 day timespan. The peak nightly flux above 250GeV was (1.14 0.26) × 10 -11 cm -2 s -1 , which corresponded to 7.7% of the Crab Nebula flux. M87 was marginally detected before this 4 day flare period, and was not detected afterward. Spectral analysis of the VERITAS observations showed no significant change in the photon index between the flare and pre-flare states. Shortly after the VHE flare seen by VERITAS, the Chandra X-ray Observatory detected the flux from the core of M87 at a historical maximum, while the flux from the nearby knot HST-1 remained quiescent. Acciari etal. presented the 2008 contemporaneous VHE gamma-ray, Chandra X-ray, and Very Long Baseline Array radio observations which suggest the core as the most likely source of VHE emission, in contrast to the 2005 VHE flare that was simultaneous with an X-ray flare in the HST-1 knot. In 2009, VERITAS continued its monitoring of M87 and marginally detected a 4.2σ excess corresponding to a flux of 1% of the Crab Nebula. No VHE flaring activity was observed in 2009. © 2010. The American Astronomical Society. All rights reserved. |
format |
JOUR |
author |
Acciari, V.A. Aliu, E. Arlen, T. Aune, T. Beilicke, M. Benbow, W. Boltuch, D. Bradbury, S.M. Buckley, J.H. Bugaev, V. Byrum, K. Cannon, A. Cesarini, A. Chow, Y.C. Ciupik, L. Cogan, P. Cui, W. Dickherber, R. Duke, C. Finley, J.P. Finnegan, G. Fortin, P. Fortson, L. Furniss, A. Galante, N. Gall, D. Gillanders, G.H. Godambe, S. Grube, J. Guenette, R. Gyuk, G. Hanna, D. Holder, J. Hui, C.M. Humensky, T.B. Imran, A. Kaaret, P. Karlsson, N. Kertzman, M. Kieda, D. Konopelko, A. Krawczynski, H. Krennrich, F. Lang, M.J. Lebohec, S. Maier, G. McArthur, S. McCann, A. McCutcheon, M. Millis, J. Moriarty, P. Ong, R.A. Otte, A.N. Pandel, D. Perkins, J.S. Pichel, A. Pohl, M. Quinn, J. Ragan, K. Reyes, L.C. Reynolds, P.T. Roache, E. Rose, H.J. Rovero, A.C. Schroedter, M. Sembroski, G.H. Senturk, G.D. Smith, A.W. Steele, D. Swordy, S.P. Theiling, M. Thibadeau, S. Varlotta, A. Vincent, S. Wagner, R.G. Wakely, S.P. Ward, J.E. Weekes, T.C. Weinstein, A. Weisgarber, T. Williams, D.A. Wissel, S. Wood, M. Zitzer, B. Harris, D.E. Massaro, F. |
author_facet |
Acciari, V.A. Aliu, E. Arlen, T. Aune, T. Beilicke, M. Benbow, W. Boltuch, D. Bradbury, S.M. Buckley, J.H. Bugaev, V. Byrum, K. Cannon, A. Cesarini, A. Chow, Y.C. Ciupik, L. Cogan, P. Cui, W. Dickherber, R. Duke, C. Finley, J.P. Finnegan, G. Fortin, P. Fortson, L. Furniss, A. Galante, N. Gall, D. Gillanders, G.H. Godambe, S. Grube, J. Guenette, R. Gyuk, G. Hanna, D. Holder, J. Hui, C.M. Humensky, T.B. Imran, A. Kaaret, P. Karlsson, N. Kertzman, M. Kieda, D. Konopelko, A. Krawczynski, H. Krennrich, F. Lang, M.J. Lebohec, S. Maier, G. McArthur, S. McCann, A. McCutcheon, M. Millis, J. Moriarty, P. Ong, R.A. Otte, A.N. Pandel, D. Perkins, J.S. Pichel, A. Pohl, M. Quinn, J. Ragan, K. Reyes, L.C. Reynolds, P.T. Roache, E. Rose, H.J. Rovero, A.C. Schroedter, M. Sembroski, G.H. Senturk, G.D. Smith, A.W. Steele, D. Swordy, S.P. Theiling, M. Thibadeau, S. Varlotta, A. Vincent, S. Wagner, R.G. Wakely, S.P. Ward, J.E. Weekes, T.C. Weinstein, A. Weisgarber, T. Williams, D.A. Wissel, S. Wood, M. Zitzer, B. Harris, D.E. Massaro, F. |
author_sort |
Acciari, V.A. |
title |
Veritas 2008-2009 monitoring of the variable gamma-ray source M87 |
title_short |
Veritas 2008-2009 monitoring of the variable gamma-ray source M87 |
title_full |
Veritas 2008-2009 monitoring of the variable gamma-ray source M87 |
title_fullStr |
Veritas 2008-2009 monitoring of the variable gamma-ray source M87 |
title_full_unstemmed |
Veritas 2008-2009 monitoring of the variable gamma-ray source M87 |
title_sort |
veritas 2008-2009 monitoring of the variable gamma-ray source m87 |
url |
http://hdl.handle.net/20.500.12110/paper_0004637X_v716_n1_p819_Acciari |
work_keys_str_mv |
AT acciariva veritas20082009monitoringofthevariablegammaraysourcem87 AT aliue veritas20082009monitoringofthevariablegammaraysourcem87 AT arlent veritas20082009monitoringofthevariablegammaraysourcem87 AT aunet veritas20082009monitoringofthevariablegammaraysourcem87 AT beilickem veritas20082009monitoringofthevariablegammaraysourcem87 AT benboww veritas20082009monitoringofthevariablegammaraysourcem87 AT boltuchd veritas20082009monitoringofthevariablegammaraysourcem87 AT bradburysm veritas20082009monitoringofthevariablegammaraysourcem87 AT buckleyjh veritas20082009monitoringofthevariablegammaraysourcem87 AT bugaevv veritas20082009monitoringofthevariablegammaraysourcem87 AT byrumk veritas20082009monitoringofthevariablegammaraysourcem87 AT cannona veritas20082009monitoringofthevariablegammaraysourcem87 AT cesarinia veritas20082009monitoringofthevariablegammaraysourcem87 AT chowyc veritas20082009monitoringofthevariablegammaraysourcem87 AT ciupikl veritas20082009monitoringofthevariablegammaraysourcem87 AT coganp veritas20082009monitoringofthevariablegammaraysourcem87 AT cuiw veritas20082009monitoringofthevariablegammaraysourcem87 AT dickherberr veritas20082009monitoringofthevariablegammaraysourcem87 AT dukec veritas20082009monitoringofthevariablegammaraysourcem87 AT finleyjp veritas20082009monitoringofthevariablegammaraysourcem87 AT finnegang veritas20082009monitoringofthevariablegammaraysourcem87 AT fortinp veritas20082009monitoringofthevariablegammaraysourcem87 AT fortsonl veritas20082009monitoringofthevariablegammaraysourcem87 AT furnissa veritas20082009monitoringofthevariablegammaraysourcem87 AT galanten veritas20082009monitoringofthevariablegammaraysourcem87 AT galld veritas20082009monitoringofthevariablegammaraysourcem87 AT gillandersgh veritas20082009monitoringofthevariablegammaraysourcem87 AT godambes veritas20082009monitoringofthevariablegammaraysourcem87 AT grubej veritas20082009monitoringofthevariablegammaraysourcem87 AT guenetter veritas20082009monitoringofthevariablegammaraysourcem87 AT gyukg veritas20082009monitoringofthevariablegammaraysourcem87 AT hannad veritas20082009monitoringofthevariablegammaraysourcem87 AT holderj veritas20082009monitoringofthevariablegammaraysourcem87 AT huicm veritas20082009monitoringofthevariablegammaraysourcem87 AT humenskytb veritas20082009monitoringofthevariablegammaraysourcem87 AT imrana veritas20082009monitoringofthevariablegammaraysourcem87 AT kaaretp veritas20082009monitoringofthevariablegammaraysourcem87 AT karlssonn veritas20082009monitoringofthevariablegammaraysourcem87 AT kertzmanm veritas20082009monitoringofthevariablegammaraysourcem87 AT kiedad veritas20082009monitoringofthevariablegammaraysourcem87 AT konopelkoa veritas20082009monitoringofthevariablegammaraysourcem87 AT krawczynskih veritas20082009monitoringofthevariablegammaraysourcem87 AT krennrichf veritas20082009monitoringofthevariablegammaraysourcem87 AT langmj veritas20082009monitoringofthevariablegammaraysourcem87 AT lebohecs veritas20082009monitoringofthevariablegammaraysourcem87 AT maierg veritas20082009monitoringofthevariablegammaraysourcem87 AT mcarthurs veritas20082009monitoringofthevariablegammaraysourcem87 AT mccanna veritas20082009monitoringofthevariablegammaraysourcem87 AT mccutcheonm veritas20082009monitoringofthevariablegammaraysourcem87 AT millisj veritas20082009monitoringofthevariablegammaraysourcem87 AT moriartyp veritas20082009monitoringofthevariablegammaraysourcem87 AT ongra veritas20082009monitoringofthevariablegammaraysourcem87 AT ottean veritas20082009monitoringofthevariablegammaraysourcem87 AT pandeld veritas20082009monitoringofthevariablegammaraysourcem87 AT perkinsjs veritas20082009monitoringofthevariablegammaraysourcem87 AT pichela veritas20082009monitoringofthevariablegammaraysourcem87 AT pohlm veritas20082009monitoringofthevariablegammaraysourcem87 AT quinnj veritas20082009monitoringofthevariablegammaraysourcem87 AT ragank veritas20082009monitoringofthevariablegammaraysourcem87 AT reyeslc veritas20082009monitoringofthevariablegammaraysourcem87 AT reynoldspt veritas20082009monitoringofthevariablegammaraysourcem87 AT roachee veritas20082009monitoringofthevariablegammaraysourcem87 AT rosehj veritas20082009monitoringofthevariablegammaraysourcem87 AT roveroac veritas20082009monitoringofthevariablegammaraysourcem87 AT schroedterm veritas20082009monitoringofthevariablegammaraysourcem87 AT sembroskigh veritas20082009monitoringofthevariablegammaraysourcem87 AT senturkgd veritas20082009monitoringofthevariablegammaraysourcem87 AT smithaw veritas20082009monitoringofthevariablegammaraysourcem87 AT steeled veritas20082009monitoringofthevariablegammaraysourcem87 AT swordysp veritas20082009monitoringofthevariablegammaraysourcem87 AT theilingm veritas20082009monitoringofthevariablegammaraysourcem87 AT thibadeaus veritas20082009monitoringofthevariablegammaraysourcem87 AT varlottaa veritas20082009monitoringofthevariablegammaraysourcem87 AT vincents veritas20082009monitoringofthevariablegammaraysourcem87 AT wagnerrg veritas20082009monitoringofthevariablegammaraysourcem87 AT wakelysp veritas20082009monitoringofthevariablegammaraysourcem87 AT wardje veritas20082009monitoringofthevariablegammaraysourcem87 AT weekestc veritas20082009monitoringofthevariablegammaraysourcem87 AT weinsteina veritas20082009monitoringofthevariablegammaraysourcem87 AT weisgarbert veritas20082009monitoringofthevariablegammaraysourcem87 AT williamsda veritas20082009monitoringofthevariablegammaraysourcem87 AT wissels veritas20082009monitoringofthevariablegammaraysourcem87 AT woodm veritas20082009monitoringofthevariablegammaraysourcem87 AT zitzerb veritas20082009monitoringofthevariablegammaraysourcem87 AT harrisde veritas20082009monitoringofthevariablegammaraysourcem87 AT massarof veritas20082009monitoringofthevariablegammaraysourcem87 |
_version_ |
1782025960558690304 |