A. Abramowski
HESS and Fermi-LAT discovery of γ-rays from the blazar 1ES 1312−423
Abramowski, A.; Acero, F.; Aharonian, F.; Akhperjanian, A.G.; Angüner, E.; Anton, G.; Balenderan, S.; Balzer, A.; Barnacka, A.; Becherini, Y.; Becker Tjus, J.; Bernlöhr, K.; Birsin, E.; Bissaldi, E.; Biteau, J.; Boisson, C.; Bolmont, J.; Bordas, P.; Brucker, J.; Brun, F.; Brun, P.; Bulik, T.; Carrigan, S.; Casanova, S.; Cerruti, M.; Chadwick, P.M.; Chalme-Calvet, R.; Chaves, R.C.G.; Cheesebrough, A.; Chrétien, M.; Colafrancesco, S.; Cologna, G.; Conrad, J.; Couturier, C.; Dalton, M.; Daniel, M.K.; Davids, I.D.; Degrange, B.; Deil, C.; deWilt, P.; Dickinson, H.J.; Djannati-Ataï, A.; Domainko, W.; Drury, L. O'C.; Dubus, G.; Dutson, K.; Dyks, J.; Dyrda, M.; Edwards, T.; Egberts, K.; Eger, P.; Espigat, P.; Farnier, C.; Fegan, S.; Feinstein, F.; Fernandes, M.V.; Fernandez, D.; Fiasson, A.; Fontaine, G.; Förster, A.; Füßling, M.; Gajdus, M.; Gallant, Y.A.; Garrigoux, T.; Gast, H.; Giebels, B.; Glicenstein, J.F.; Göring, D.; Grondin, M.-H.; Grudzińska, M.; Häffner, S.; Hague, J.D.; Hahn, J.;...
Authors
F. Acero
F. Aharonian
A.G. Akhperjanian
E. Angüner
G. Anton
S. Balenderan
A. Balzer
A. Barnacka
Y. Becherini
J. Becker Tjus
K. Bernlöhr
E. Birsin
E. Bissaldi
J. Biteau
C. Boisson
J. Bolmont
P. Bordas
J. Brucker
F. Brun
P. Brun
T. Bulik
S. Carrigan
S. Casanova
M. Cerruti
Professor Paula Chadwick p.m.chadwick@durham.ac.uk
Head Of Department
R. Chalme-Calvet
R.C.G. Chaves
A. Cheesebrough
M. Chrétien
S. Colafrancesco
G. Cologna
J. Conrad
C. Couturier
M. Dalton
M.K. Daniel
I.D. Davids
B. Degrange
C. Deil
P. deWilt
H.J. Dickinson
A. Djannati-Ataï
W. Domainko
L. O'C. Drury
G. Dubus
K. Dutson
J. Dyks
M. Dyrda
T. Edwards
K. Egberts
P. Eger
P. Espigat
C. Farnier
S. Fegan
F. Feinstein
M.V. Fernandes
D. Fernandez
A. Fiasson
G. Fontaine
A. Förster
M. Füßling
M. Gajdus
Y.A. Gallant
T. Garrigoux
H. Gast
B. Giebels
J.F. Glicenstein
D. Göring
M.-H. Grondin
M. Grudzińska
S. Häffner
J.D. Hague
J. Hahn
J. Harris
G. Heinzelmann
G. Henri
G. Hermann
O. Hervet
A. Hillert
J.A. Hinton
W. Hofmann
P. Hofverberg
M. Holler
D. Horns
A. Jacholkowska
C. Jahn
M. Jamrozy
M. Janiak
F. Jankowsky
I. Jung
M.A. Kastendieck
K. Katarzyński
U. Katz
S. Kaufmann
B. Khélifi
M. Kieffer
S. Klepser
D. Klochkov
W. Kluźniak
T. Kneiske
D. Kolitzus
Nu Komin
K. Kosack
S. Krakau
F. Krayzel
P.P. Krüger
H. Laffon
G. Lamanna
J. Lefaucheur
M. Lemoine-Goumard
J-P. Lenain
D. Lennarz
T. Lohse
A. Lopatin
C-C. Lu
V. Marandon
A. Marcowith
G. Maurin
N. Maxted
M. Mayer
T.J.L. McComb
M.C. Medina
J. Méhault
U. Menzler
M. Meyer
R. Moderski
M. Mohamed
E. Moulin
T. Murach
C.L. Naumann
M. de Naurois
D. Nedbal
J. Niemiec
Professor Sam Nolan s.j.nolan@durham.ac.uk
Director Of Dcad
L. Oakes
S. Ohm
E. de Oña Wilhelmi
B. Opitz
M. Ostrowski
I. Oya
M. Panter
R.D. Parsons
M. Paz Arribas
N.W. Pekeur
G. Pelletier
J. Perez
P.-O. Petrucci
B. Peyaud
S. Pita
H. Poon
G. Pühlhofer
M. Punch
A. Quirrenbach
S. Raab
M. Raue
A. Reimer
O. Reimer
M. Renaud
R. de los Reyes
F. Rieger
L. Rob
S. Rosier-Lees
G. Rowell
B. Rudak
C.B. Rulten
V. Sahakian
D.A. Sanchez
A. Santangelo
R. Schlickeiser
F. Schüssler
A. Schulz
U. Schwanke
S. Schwarzburg
S. Schwemmer
H. Sol
G. Spengler
F. Spieß
Ł Stawarz
R. Steenkamp
C. Stegmann
F. Stinzing
K. Stycz
I. Sushch
A. Szostek
J.-P. Tavernet
R. Terrier
M. Tluczykont
C. Trichard
K. Valerius
C. van Eldik
G. Vasileiadis
C. Venter
A. Viana
P. Vincent
H.J. Völk
F. Volpe
M. Vorster
S.J. Wagner
P. Wagner
Professor Martin Ward martin.ward@durham.ac.uk
External Examiner (PGR)
M. Weidinger
R. White
A. Wierzcholska
P. Willmann
A. Wörnlein
D. Wouters
M. Zacharias
A. Zajczyk
A.A. Zdziarski
A. Zech
H.-S. Zechlin
J.S. Perkins
R. Ojha
J. Stevens
P.G. Edwards
M. Kadler
Abstract
A deep observation campaign carried out by the High Energy Stereoscopic System (HESS) on Centaurus A enabled the discovery of γ-rays from the blazar 1ES 1312−423, 2° away from the radio galaxy. With a differential flux at 1 TeV of ϕ(1 TeV) = (1.9 ± 0.6stat ± 0.4sys) × 10−13 cm−2 s−1 TeV−1 corresponding to 0.5 per cent of the Crab nebula differential flux and a spectral index Γ = 2.9 ± 0.5stat ± 0.2sys, 1ES 1312−423 is one of the faintest sources ever detected in the very high energy (E > 100 GeV) extragalactic sky. A careful analysis using three and a half years of Fermi Large Area Telescope (Fermi-LAT) data allows the discovery at high energies (E > 100 MeV) of a hard spectrum (Γ = 1.4 ± 0.4stat ± 0.2sys) source coincident with 1ES 1312−423. Radio, optical, UV and X-ray observations complete the spectral energy distribution of this blazar, now covering 16 decades in energy. The emission is successfully fitted with a synchrotron self-Compton model for the non-thermal component, combined with a blackbody spectrum for the optical emission from the host galaxy.
Citation
Abramowski, A., Acero, F., Aharonian, F., Akhperjanian, A., Angüner, E., Anton, G., …Kadler, M. (2013). HESS and Fermi-LAT discovery of γ-rays from the blazar 1ES 1312−423. Monthly Notices of the Royal Astronomical Society, 434(3), 1889-1901. https://doi.org/10.1093/mnras/stt1081
Journal Article Type | Article |
---|---|
Publication Date | Sep 21, 2013 |
Deposit Date | Feb 5, 2014 |
Publicly Available Date | Jun 18, 2014 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 434 |
Issue | 3 |
Pages | 1889-1901 |
DOI | https://doi.org/10.1093/mnras/stt1081 |
Keywords | Radiation mechanisms: non-thermal, Galaxies: active, BL Lacertae objects: individual: 1ES 1312–423, Galaxies: jets, Gamma-rays: galaxies |
Public URL | https://durham-repository.worktribe.com/output/1462383 |
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Copyright Statement
This article has been accepted for publication in Monthly notices of the Royal Astronomical Society ©: 2013 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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