Issue |
A&A
Volume 571, November 2014
|
|
---|---|---|
Article Number | A39 | |
Number of page(s) | 10 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361/201424142 | |
Published online | 04 November 2014 |
Long-term monitoring of PKS 2155−304 with ATOM and H.E.S.S.: investigation of optical/γ-ray correlations in different spectral states
1
Universität Hamburg, Institut für Experimentalphysik,
Luruper Chaussee 149,
22761
Hamburg,
Germany
2
Max-Planck-Institut für Kernphysik, PO Box 103980, 69029
Heidelberg,
Germany
3 Dublin Institute for Advanced Studies, 31 Fitzwilliam Place,
Dublin 2, Ireland
4 National Academy of Sciences of the Republic of Armenia,
Marshall Baghramian Avenue, 24, 0019 Yerevan, Republic of Armenia
5
Yerevan Physics Institute, 2 Alikhanian Brothers St., 375036
Yerevan,
Armenia
6
Institut fürPhysik, Humboldt-Universität zu Berlin,
Newtonstr. 15, 12489
Berlin,
Germany
7 University of Namibia, Department of Physics, 13301 Private
Bag, Windhoek, Namibia
8
University of Durham, Department of Physics,
South Road, Durham
DH1 3LE,
UK
9
GRAPPA, Anton Pannekoek Institute for Astronomy, University of
Amsterdam, Science Park
904, 1098 XH
Amsterdam, The
Netherlands
10
Obserwatorium Astronomiczne, Uniwersytet Jagielloński, ul. Orla
171, 30-244
Kraków,
Poland
11
now at Harvard-Smithsonian Center for Astrophysics, 60 Garden St,
MS-20, Cambridge,
MA
02138,
USA
12
Department of Physics and Electrical Engineering, Linnaeus
University, 351
95
Växjö,
Sweden
13
Institut für Theoretische Physik, Lehrstuhl IV: Weltraum und
Astrophysik, Ruhr-Universität Bochum, 44780
Bochum,
Germany
14
GRAPPA, Anton Pannekoek Institute for Astronomy and Institute of
High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH
Amsterdam, The
Netherlands
15
Institut für Astro- und Teilchenphysik,
Leopold-Franzens-Universität Innsbruck, 6020
Innsbruck,
Austria
16
Laboratoire Leprince-Ringuet, École Polytechnique,
CNRS/IN2P3, 91128
Palaiseau,
France
17
now at Santa Cruz Institute for Particle Physics, Department of
Physics, University of California at Santa Cruz, Santa Cruz, CA
95064,
USA
18
Centre for Space Research, North-West University,
Potchefstroom
2520, South
Africa
19
LUTH, Observatoire de Paris, CNRS, Université Paris
Diderot, 5 place Jules
Janssen, 92190
Meudon,
France
20 LPNHE, Université Pierre et Marie Curie Paris 6, Université
Denis Diderot Paris 7, CNRS/IN2P3, 4 place Jussieu, 75252, Paris Cedex 5, France
21
Institut für Astronomie und Astrophysik, Universität
Tübingen, Sand 1,
72076
Tübingen,
Germany
22
Laboratoire Univers et Particules de Montpellier, Université
Montpellier 2, CNRS/IN2P3, CC 72,
place Eugène Bataillon, 34095
Montpellier Cedex 5,
France
23
DSM/Irfu, CEA Saclay, 91191
Gif-Sur-Yvette Cedex,
France
24
Astronomical Observatory, The University of Warsaw,
Al. Ujazdowskie 4, 00-478
Warsaw,
Poland
25
Instytut Fizyki Ja¸drowej PAN, ul. Radzikowskiego
152, 31-342
Kraków,
Poland
26 School of Physics, University of the Witwatersrand, 1 Jan
Smuts Avenue, Braamfontein, Johannesburg, 2050 South Africa
27
Landessternwarte, Universität Heidelberg,
Königstuhl, 69117
Heidelberg,
Germany
28
Oskar Klein Centre, Department of Physics, Stockholm University,
Albanova University Center, 10691
Stockholm,
Sweden
29
Université Bordeaux 1, CNRS/IN2P3, Centre d’Études Nucléaires de Bordeaux
Gradignan, 33175
Gradignan,
France
30
School of Chemistry & Physics, University of
Adelaide, Adelaide
5005,
Australia
31
APC, AstroParticule et Cosmologie, Université Paris Diderot,
CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10 rue Alice Domon et Léonie
Duquet, 75205
Paris Cedex 13,
France
32
Univ. Grenoble Alpes, IPAG and CNRS, 38000
Grenoble,
France
33
Department of Physics and Astronomy, The University of Leicester,
University Road, Leicester, LE1
7RH, UK
34
Nicolaus Copernicus Astronomical Center, ul. Bartycka
18, 00-716
Warsaw,
Poland
35
Institut für Physik und Astronomie, Universität
Potsdam, Karl-Liebknecht-Strasse
24/25, 14476
Potsdam,
Germany
36
Laboratoire d’Annecy-le-Vieux de Physique des Particules,
Université de Savoie, CNRS/IN2P3, 74941
Annecy-le-Vieux,
France
37
DESY, 15738
Zeuthen,
Germany
38
Universität Erlangen-Nürnberg, Physikalisches
Institut, Erwin-Rommel-Str.
1, 91058
Erlangen,
Germany
39
Centre for Astronomy, Faculty of Physics, Astronomy and
Informatics, Nicolaus Copernicus University, Grudziadzka 5, 87-100
Torun,
Poland
40
Department of Physics, University of the Free State,
PO Box 339, 9300
Bloemfontein, South
Africa
41 Charles University, Faculty of Mathematics and
Physics,Institute of Particle and Nuclear Physics, V Holešovičkách 2, 180 00 Prague 8,
Czech Republic
42
GRAPPA, Institute of High-Energy Physics, University of
Amsterdam, Science Park
904, 1098 XH
Amsterdam, The
Netherlands
Received: 5 May 2014
Accepted: 10 July 2014
In this paper we report on the analysis of all the available optical and very high-energy γ-ray (>200 GeV) data for the BL Lac object PKS 2155−304, collected simultaneously with the ATOM and H.E.S.S. telescopes from 2007 until 2009. This study also includes X-ray (RXTE, Swift) and high-energy γ-ray (Fermi-LAT) data. During the period analysed, the source was transitioning from its flaring to quiescent optical states, and was characterized by only moderate flux changes at different wavelengths on the timescales of days and months. A flattening of the optical continuum with an increasing optical flux can be noted in the collected dataset, but only occasionally and only at higher flux levels. We did not find any universal relation between the very high-energy γ-ray and optical flux changes on the timescales from days and weeks up to several years. On the other hand, we noted that at higher flux levels the source can follow two distinct tracks in the optical flux–colour diagrams, which seem to be related to distinct γ-ray states of the blazar. The obtained results therefore indicate a complex scaling between the optical and γ-ray emission of PKS 2155−304, with different correlation patterns holding at different epochs, and a γ-ray flux depending on the combination of an optical flux and colour rather than a flux alone.
Key words: radiation mechanisms: non-thermal / galaxies: active / black hole physics / BL Lacertae objects: individual: PKS 2155-304 / galaxies: jets / gamma rays: galaxies
© ESO, 2014
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