Issue |
A&A
Volume 515, June 2010
|
|
---|---|---|
Article Number | A76 | |
Number of page(s) | 5 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361/200913607 | |
Published online | 11 June 2010 |
Simultaneous multi-frequency observation of the unknown redshift blazar PG 1553+113 in March-April 2008
1
IFAE, Edifici Cn., Campus UAB, 08193 Bellaterra, Spain e-mail: nijil.mankuzhiyil@uniud.it
2
ETH Zurich, 8093 Switzerland
3
INAF National Institute for Astrophysics, 00136 Rome, Italy
4
Universidad Complutense, 28040 Madrid, Spain
5
Technische Universität Dortmund, 44221 Dortmund, Germany
6
Universitat Autònoma de Barcelona, 08193 Bellaterra, Spain
7
Università di Padova and INFN, 35131 Padova, Italy
8
Inst. de Astrofísica de Canarias, 38200 La Laguna, Tenerife, Spain
9
University of Łódź, 90236 Lodz, Poland
10
Tuorla Observatory, University of Turku, 21500 Piikkiö, Finland
11
Deutsches Elektronen-Synchrotron (DESY), 15738 Zeuthen, Germany
12
Max-Planck-Institut für Physik, 80805 München, Germany
13
Università di Siena, and INFN Pisa, 53100 Siena, Italy
14
Universitat de Barcelona (ICC/IEEC), 08028 Barcelona, Spain
15
Universität Würzburg, 97074 Würzburg, Germany
16
Depto. de Astrofisica, Universidad, 38206 La Laguna, Tenerife, Spain
17
Università di Udine, and INFN Trieste, 33100 Udine, Italy
18
Supported by INFN Padova
19
Institut de Ciències de l'Espai (IEEC-CSIC), 08193 Bellaterra, Spain
20
Now at: Max-Planck-Institut für Kernphysik, 69029 Heidelberg, Germany
21
Now at: Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
22
Inst. de Astrofísica de Andalucía (CSIC), 18080 Granada, Spain
23
Croatian MAGIC Consortium, Institute R. Boskovic, University of Rijeka and University of Split, 10000 Zagreb, Croatia
24
University of California, Davis, CA-95616-8677, USA
25
Deceased
26
Inst. for Nucl. Research and Nucl. Energy, 1784 Sofia, Bulgaria
27
INAF/Osservatorio Astronomico and INFN, 34143 Trieste, Italy
28
ICREA, 08010 Barcelona, Spain
29
Università di Pisa, and INFN Pisa, 56126 Pisa, Italy
30
INAF, Trieste Astronomical Observatory, 34143 Trieste, Italy
31
Now at: Scuola Normale Superiore, 56126 Pisa, Italy
32
INAF/IASF-Bologna, 40129 Bologna, Italy
33
INAF/IASF-Roma, 00133 Roma, Italy
34
INAF, Astronomical Obs. Brera, 23807 Merate, Italy
35
Abastumani Astrophysical Observatory, 383762 Abastumani, Georgia
36
INAF, Astronomical Obs. Torino, 10025 Torino, Italy
37
University of Perugia, 06123 Perugia, Italy
38
University of Insubria, 22100 Como, Italy
39
INAF, IASF-Milano, 20133 Milano, Italy
Received:
4
November
2009
Accepted:
3
March
2010
The blazar PG 1553+113 is a well known TeV γ-ray emitter. In this paper we determine its spectral energy distribution through simultaneous multi-frequency data to study its emission processes. An extensive campaign was carried out between March and April 2008, where optical, X-ray, high-energy (HE) γ-ray, and very-high-energy (VHE) γ-ray data were obtained with the KVA, Abastumani, REM, RossiXTE/ASM, AGILE and MAGIC telescopes, respectively. We combine the data to derive the source's spectral energy distribution and interpret its double-peaked shape within the framework of a synchrotron self-Compton model.
Key words: BL Lacertae objects: individual: PG 1553+113 / X-rays: galaxies / gamma rays: galaxies / galaxies: active
© ESO, 2010
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