The blazar PG 1553+113 is a well known TeV gamma-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) gamma-ray, and very-high-energy (VHE) gamma-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.

J., A., H., A., L. A., A., P., A., M., B., C., B., et al. (2010). Simultaneous multi-frequency observation of the unknown redshift blazar PG 1553+113 in March-April 2008. ASTRONOMY & ASTROPHYSICS, 515(9) [10.1051/0004-6361/200913607].

Simultaneous multi-frequency observation of the unknown redshift blazar PG 1553+113 in March-April 2008

BONNOLI, GIACOMO;PAOLETTI, RICCARDO;STAMERRA, ANTONIO;
2010-01-01

Abstract

The blazar PG 1553+113 is a well known TeV gamma-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) gamma-ray, and very-high-energy (VHE) gamma-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.
2010
J., A., H., A., L. A., A., P., A., M., B., C., B., et al. (2010). Simultaneous multi-frequency observation of the unknown redshift blazar PG 1553+113 in March-April 2008. ASTRONOMY & ASTROPHYSICS, 515(9) [10.1051/0004-6361/200913607].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11365/39321
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