Observation of Markarian 421 in TeV gamma rays over a 14-year time span

V. A. Acciari; T. Arlen; T. Aune; W. Benbow; R. Bird; A. Bouvier; S. M. Bradbury; J. H. Buckley; V. Bugaev; I. De La Calle Perez; D. A. Carter-Lewis; A. Cesarini; L. Ciupik; E. Collins-Hughes; M. P. Connolly; W. Cui; C. Duke; J. Dumm; A. Falcone; S. Federici; D. J. Fegan; S. J. Fegan; J. P. Finley; G. Finnegan; L. Fortson; J. Gaidos; N. Galante; D. Gall; K. Gibbs; G. H. Gillanders; S. Griffin; J. Grube; G. Gyuk; D. Hanna; D. Horan; T. B. Humensky; P. Kaaret; M. Kertzman; Y. Khassen; D. Kieda; H. Krawczynski; F. Krennrich; M. J. Lang; J. E. McEnery; A. S. Madhavan; P. Moriarty; T. Nelson; A. O'Faoláin De Bhróithe; R. A. Ong; M. Orr; A. N. Otte; J. S. Perkins; D. Petry; A. Pichel; M. Pohl; J. Quinn; K. Ragan; T. Reynolds; E. Roache; A. Rovero; M. Schroedter; G. H. Sembroski; A. Smith; I. Telezhinsky; M. Theiling; J. Toner; J. Tyler; A. Varlotta; M. Vivier; S. P. Wakely; J. E. Ward; T. C. Weekes; A. Weinstein; R. Welsing; D. A. Williams; S. Wissel

doi:10.1016/j.astropartphys.2013.10.004

Observation of Markarian 421 in TeV gamma rays over a 14-year time span

V. A. Acciari
, T. Arlen
, T. Aune
, W. Benbow
, R. Bird
, A. Bouvier
, S. M. Bradbury
, J. H. Buckley
, V. Bugaev
, I. De La Calle Perez
, D. A. Carter-Lewis
, A. Cesarini
, L. Ciupik
, E. Collins-Hughes
, M. P. Connolly
, W. Cui
, C. Duke
, J. Dumm
, A. Falcone
, S. Federici

D. J. Fegan, S. J. Fegan, J. P. Finley, G. Finnegan, L. Fortson, J. Gaidos, N. Galante, D. Gall, K. Gibbs, G. H. Gillanders, S. Griffin, J. Grube, G. Gyuk, D. Hanna, D. Horan, T. B. Humensky, P. Kaaret, M. Kertzman, Y. Khassen, D. Kieda, H. Krawczynski, F. Krennrich, M. J. Lang, J. E. McEnery, A. S. Madhavan, P. Moriarty, T. Nelson, A. O'Faoláin De Bhróithe, R. A. Ong, M. Orr, A. N. Otte, J. S. Perkins, D. Petry, A. Pichel, M. Pohl, J. Quinn, K. Ragan, T. Reynolds, E. Roache, A. Rovero, M. Schroedter, G. H. Sembroski, A. Smith, I. Telezhinsky, M. Theiling, J. Toner, J. Tyler, A. Varlotta, M. Vivier, S. P. Wakely, J. E. Ward, T. C. Weekes, A. Weinstein, R. Welsing, D. A. Williams, S. Wissel

Galway-Mayo Institute of Technology
Center for Astrophysics | Harvard & Smithsonian
University of California, Los Angeles
University of California at Santa Cruz
University College Dublin
University of Leeds
Washington University in St. Louis
ESAC campus
Iowa State University
IDA Business Park
Adler Planetarium
Purdue University
Grinnell College
University of Minnesota
Pennsylvania State University
University of Potsdam
c/o DESY
University of Utah
University of Iowa
McGill University
Barnard College
DePauw University
NASA Goddard Space Flight Center
University of Maryland
College of Computing
Biochemical and Environmental Engineering
European Southern Observatory
Instituto de Astronomía y Física del Espacio
Cork Institute of Technology
Valeo Vision Systems
The Bartol Research Institute
University of Chicago

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

Résumé

The variability of the blazar Markarian 421 in TeV gamma rays over a 14-year time period has been explored with the Whipple 10 m telescope. It is shown that the dynamic range of its flux variations is large and similar to that in X-rays. A correlation between the X-ray and TeV energy bands is observed during some bright flares and when the complete data sets are binned on long timescales. The main database consists of 878.4 h of observation with the Whipple telescope, spread over 783 nights. The peak energy response of the telescope was 400 GeV with 20% uncertainty. This is the largest database of any TeV-emitting active galactic nucleus (AGN) and hence was used to explore the variability profile of Markarian 421. The time-averaged flux from Markarian 421 over this period was 0.446±0.008 Crab flux units. The flux exceeded 10 Crab flux units on three separate occasions. For the 2000-2001 season the average flux reached 1.86 Crab units, while in the 1996-1997 season the average flux was only 0.23 Crab units.

langue originale	Anglais
Pages (de - à)	1-10
Nombre de pages	10
journal	Astroparticle Physics
Volume	54
Les DOIs	https://doi.org/10.1016/j.astropartphys.2013.10.004
état	Publié - 1 févr. 2014

Accès au document

10.1016/j.astropartphys.2013.10.004

Autres fichiers et liens

Lien vers la publication dans Scopus

Contient cette citation

Acciari, V. A., Arlen, T., Aune, T., Benbow, W., Bird, R., Bouvier, A., Bradbury, S. M., Buckley, J. H., Bugaev, V., De La Calle Perez, I., Carter-Lewis, D. A., Cesarini, A., Ciupik, L., Collins-Hughes, E., Connolly, M. P., Cui, W., Duke, C., Dumm, J., Falcone, A., ... Wissel, S. (2014). Observation of Markarian 421 in TeV gamma rays over a 14-year time span. Astroparticle Physics, 54, 1-10. https://doi.org/10.1016/j.astropartphys.2013.10.004

@article{9d2d02b643f845ef9a6db10953123995,

title = "Observation of Markarian 421 in TeV gamma rays over a 14-year time span",

abstract = "The variability of the blazar Markarian 421 in TeV gamma rays over a 14-year time period has been explored with the Whipple 10 m telescope. It is shown that the dynamic range of its flux variations is large and similar to that in X-rays. A correlation between the X-ray and TeV energy bands is observed during some bright flares and when the complete data sets are binned on long timescales. The main database consists of 878.4 h of observation with the Whipple telescope, spread over 783 nights. The peak energy response of the telescope was 400 GeV with 20\% uncertainty. This is the largest database of any TeV-emitting active galactic nucleus (AGN) and hence was used to explore the variability profile of Markarian 421. The time-averaged flux from Markarian 421 over this period was 0.446±0.008 Crab flux units. The flux exceeded 10 Crab flux units on three separate occasions. For the 2000-2001 season the average flux reached 1.86 Crab units, while in the 1996-1997 season the average flux was only 0.23 Crab units.",

keywords = "AGN, Markarian 421, TeV gamma rays",

author = "Acciari, \{V. A.\} and T. Arlen and T. Aune and W. Benbow and R. Bird and A. Bouvier and Bradbury, \{S. M.\} and Buckley, \{J. H.\} and V. Bugaev and \{De La Calle Perez\}, I. and Carter-Lewis, \{D. A.\} and A. Cesarini and L. Ciupik and E. Collins-Hughes and Connolly, \{M. P.\} and W. Cui and C. Duke and J. Dumm and A. Falcone and S. Federici and Fegan, \{D. J.\} and Fegan, \{S. J.\} and Finley, \{J. P.\} and G. Finnegan and L. Fortson and J. Gaidos and N. Galante and D. Gall and K. Gibbs and Gillanders, \{G. H.\} and S. Griffin and J. Grube and G. Gyuk and D. Hanna and D. Horan and Humensky, \{T. B.\} and P. Kaaret and M. Kertzman and Y. Khassen and D. Kieda and H. Krawczynski and F. Krennrich and Lang, \{M. J.\} and McEnery, \{J. E.\} and Madhavan, \{A. S.\} and P. Moriarty and T. Nelson and \{O'Faol{\'a}in De Bhr{\'o}ithe\}, A. and Ong, \{R. A.\} and M. Orr and Otte, \{A. N.\} and Perkins, \{J. S.\} and D. Petry and A. Pichel and M. Pohl and J. Quinn and K. Ragan and T. Reynolds and E. Roache and A. Rovero and M. Schroedter and Sembroski, \{G. H.\} and A. Smith and I. Telezhinsky and M. Theiling and J. Toner and J. Tyler and A. Varlotta and M. Vivier and Wakely, \{S. P.\} and Ward, \{J. E.\} and Weekes, \{T. C.\} and A. Weinstein and R. Welsing and Williams, \{D. A.\} and S. Wissel",

year = "2014",

month = feb,

day = "1",

doi = "10.1016/j.astropartphys.2013.10.004",

language = "English",

volume = "54",

pages = "1--10",

journal = "Astroparticle Physics",

issn = "0927-6505",

}

Acciari, VA, Arlen, T, Aune, T, Benbow, W, Bird, R, Bouvier, A, Bradbury, SM, Buckley, JH, Bugaev, V, De La Calle Perez, I, Carter-Lewis, DA, Cesarini, A, Ciupik, L, Collins-Hughes, E, Connolly, MP, Cui, W, Duke, C, Dumm, J, Falcone, A, Federici, S, Fegan, DJ, Fegan, SJ, Finley, JP, Finnegan, G, Fortson, L, Gaidos, J, Galante, N, Gall, D, Gibbs, K, Gillanders, GH, Griffin, S, Grube, J, Gyuk, G, Hanna, D, Horan, D, Humensky, TB, Kaaret, P, Kertzman, M, Khassen, Y, Kieda, D, Krawczynski, H, Krennrich, F, Lang, MJ, McEnery, JE, Madhavan, AS, Moriarty, P, Nelson, T, O'Faoláin De Bhróithe, A, Ong, RA, Orr, M, Otte, AN, Perkins, JS, Petry, D, Pichel, A, Pohl, M, Quinn, J, Ragan, K, Reynolds, T, Roache, E, Rovero, A, Schroedter, M, Sembroski, GH, Smith, A, Telezhinsky, I, Theiling, M, Toner, J, Tyler, J, Varlotta, A, Vivier, M, Wakely, SP, Ward, JE, Weekes, TC, Weinstein, A, Welsing, R, Williams, DA & Wissel, S 2014, 'Observation of Markarian 421 in TeV gamma rays over a 14-year time span', Astroparticle Physics, VOL. 54, p. 1-10. https://doi.org/10.1016/j.astropartphys.2013.10.004

TY - JOUR

T1 - Observation of Markarian 421 in TeV gamma rays over a 14-year time span

AU - Acciari, V. A.

AU - Arlen, T.

AU - Aune, T.

AU - Benbow, W.

AU - Bird, R.

AU - Bouvier, A.

AU - Bradbury, S. M.

AU - Buckley, J. H.

AU - Bugaev, V.

AU - De La Calle Perez, I.

AU - Carter-Lewis, D. A.

AU - Cesarini, A.

AU - Ciupik, L.

AU - Collins-Hughes, E.

AU - Connolly, M. P.

AU - Cui, W.

AU - Duke, C.

AU - Dumm, J.

AU - Falcone, A.

AU - Federici, S.

AU - Fegan, D. J.

AU - Fegan, S. J.

AU - Finley, J. P.

AU - Finnegan, G.

AU - Fortson, L.

AU - Gaidos, J.

AU - Galante, N.

AU - Gall, D.

AU - Gibbs, K.

AU - Gillanders, G. H.

AU - Griffin, S.

AU - Grube, J.

AU - Gyuk, G.

AU - Hanna, D.

AU - Horan, D.

AU - Humensky, T. B.

AU - Kaaret, P.

AU - Kertzman, M.

AU - Khassen, Y.

AU - Kieda, D.

AU - Krawczynski, H.

AU - Krennrich, F.

AU - Lang, M. J.

AU - McEnery, J. E.

AU - Madhavan, A. S.

AU - Moriarty, P.

AU - Nelson, T.

AU - O'Faoláin De Bhróithe, A.

AU - Ong, R. A.

AU - Orr, M.

AU - Otte, A. N.

AU - Perkins, J. S.

AU - Petry, D.

AU - Pichel, A.

AU - Pohl, M.

AU - Quinn, J.

AU - Ragan, K.

AU - Reynolds, T.

AU - Roache, E.

AU - Rovero, A.

AU - Schroedter, M.

AU - Sembroski, G. H.

AU - Smith, A.

AU - Telezhinsky, I.

AU - Theiling, M.

AU - Toner, J.

AU - Tyler, J.

AU - Varlotta, A.

AU - Vivier, M.

AU - Wakely, S. P.

AU - Ward, J. E.

AU - Weekes, T. C.

AU - Weinstein, A.

AU - Welsing, R.

AU - Williams, D. A.

AU - Wissel, S.

PY - 2014/2/1

Y1 - 2014/2/1

N2 - The variability of the blazar Markarian 421 in TeV gamma rays over a 14-year time period has been explored with the Whipple 10 m telescope. It is shown that the dynamic range of its flux variations is large and similar to that in X-rays. A correlation between the X-ray and TeV energy bands is observed during some bright flares and when the complete data sets are binned on long timescales. The main database consists of 878.4 h of observation with the Whipple telescope, spread over 783 nights. The peak energy response of the telescope was 400 GeV with 20% uncertainty. This is the largest database of any TeV-emitting active galactic nucleus (AGN) and hence was used to explore the variability profile of Markarian 421. The time-averaged flux from Markarian 421 over this period was 0.446±0.008 Crab flux units. The flux exceeded 10 Crab flux units on three separate occasions. For the 2000-2001 season the average flux reached 1.86 Crab units, while in the 1996-1997 season the average flux was only 0.23 Crab units.

AB - The variability of the blazar Markarian 421 in TeV gamma rays over a 14-year time period has been explored with the Whipple 10 m telescope. It is shown that the dynamic range of its flux variations is large and similar to that in X-rays. A correlation between the X-ray and TeV energy bands is observed during some bright flares and when the complete data sets are binned on long timescales. The main database consists of 878.4 h of observation with the Whipple telescope, spread over 783 nights. The peak energy response of the telescope was 400 GeV with 20% uncertainty. This is the largest database of any TeV-emitting active galactic nucleus (AGN) and hence was used to explore the variability profile of Markarian 421. The time-averaged flux from Markarian 421 over this period was 0.446±0.008 Crab flux units. The flux exceeded 10 Crab flux units on three separate occasions. For the 2000-2001 season the average flux reached 1.86 Crab units, while in the 1996-1997 season the average flux was only 0.23 Crab units.

KW - AGN

KW - Markarian 421

KW - TeV gamma rays

UR - https://www.scopus.com/pages/publications/84889816469

U2 - 10.1016/j.astropartphys.2013.10.004

DO - 10.1016/j.astropartphys.2013.10.004

M3 - Article

AN - SCOPUS:84889816469

SN - 0927-6505

VL - 54

SP - 1

EP - 10

JO - Astroparticle Physics

JF - Astroparticle Physics

ER -

Observation of Markarian 421 in TeV gamma rays over a 14-year time span

Résumé

Accès au document

Autres fichiers et liens

Empreinte digitale

Contient cette citation