The BL Lac objects OQ 530 and S5 0716+714. Simultaneous observations in the X-rays, radio, optical and TeV bands
G. Tagliaferri, M. Ravasio, G. Ghisellini, P. Giommi, E. Massaro, R., Nesci, G. Tosti, M.F. Aller, H.D. Aller, A. Celotti, L. Maraschi, F., Tavecchio, A. Wolter

TL;DR
This study presents simultaneous multi-wavelength observations of two BL Lac objects, revealing their X-ray spectra are best described by a double power-law model consistent with synchrotron and inverse Compton emission, and interprets their spectral states within a unified blazar model.
Contribution
First simultaneous multi-band observations of OQ 530 and S5 0716+714, demonstrating spectral features and variability consistent with a homogeneous synchrotron and inverse Compton model.
Findings
X-ray spectra are better fitted by a double power-law model.
Spectral breaks at 0.3 and 1.5 keV indicate synchrotron and inverse Compton components.
Variability observed in S5 0716+714 supports the emission scenario.
Abstract
We present the results of the BeppoSAX observations of two BL Lacs, OQ 530 and S5 0716+714, as part of a ToO program for the simultaneous observation at radio, optical, X-ray and TeV energies. Both sources are detected in the LECS and MECS, with S5 0716+714 visible also in the PDS band, up to about 60 keV. The X-ray spectra of both sources are better fitted by a double power-law model, with a steep soft X-ray component flattening at harder energies, with breaks at 0.3 and 1.5 keV, respectively. The concave shape of the spectra in both objects is consistent with soft X-rays being produced by the synchrotron and harder X-rays by the inverse Compton processes. Also the X-ray variability properties confirm this scenario, in particular for S5 0716+714 our observation shows variations by about a factor 3 over one hour below 3 keV and no variability above. Their simultaneous broad band energy…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Particle Accelerators and Free-Electron Lasers · Particle accelerators and beam dynamics
