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Swift multi-wavelength observations of the high-redshift Blazar S5 0836+710 (4C 71.07)

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2016 Publication Year

2020-06-01T16:42:52Z Acceptance in OA@INAF

Swift multi-wavelength observations of the high-redshift Blazar S5 0836+710 (4C 71.07)

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VERCELLONE, STEFANO; ROMANO, Patrizia; RAITERI, Claudia Maria; Acosta Pulido, Jose; VILLATA, Massimo; et al.

Authors

http://hdl.handle.net/20.500.12386/25882 Handle

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CONTROL ID: 2476654

TITLE: Swift multi-wavelength observations of the high-redshift Blazar S5 0836+710 (4C 71.07) ABSTRACT BODY:

Abstract (2,250 Maximum Characters): We present the preliminary results of a year-long Swift monitoring campaign of the high-redshift (z=2.172) flat-spectrum radio quasar (FSRQ) S5 0836+710 (4C 71.07). The campaign, based on one observation per month, 5 ks each observation, for 12 months, allowed us to investigate the synchrotron and nuclear emission contributions to the optical-UV frequency range of its spectral energy distribution and the X-ray spectral variations along a baseline of a year. We obtained a high-accuracy determination of UVOT magnitudes, an X-ray photon index with an uncertainty of the order of 5%, and well-sampled light curves both in the optical-UV and X-ray energy bands to study their possible modulations and correlations. Our study allowed us to exploit the unique Swift capabilities in terms of both simultaneous energy coverage and schedule flexibility. The Swift monitoring campaign was supported by observations by the GLAST-AGILE Support Program (GASP) of the Whole Earth Blazar Telescope (WEBT) Collaboration, which provided radio, near-infrared, and optical photometric data as well as optical polarimetry. Moreover, a spectroscopic monitoring was obtained at the William Herschel Telescope (WHT) and the Nordic Optical Telescope (NOT). All these observations will allow us to obtain a comprehensive picture of the jet as well as of the nuclear source emission.

AUTHORS/INSTITUTIONS: S. Vercellone, P. Romano, INAF-IASF Palermo, Palermo, ITALY|C.M. Raiteri, M. Villata, M.I. Carnerero Martin, INAF-OATO, Torino, ITALY|J. Acosta Pulido, M.I. Carnerero Martin, IAC, Tenerife, SPAIN| CURRENT SESSION TYPE: Oral

CURRENT SCIENTIFIC CATEGORY: 01. Active Galactic Nuclei and Blazars CONTACT (ADDRESS 1 ONLY): Via Ugo La Malfa 153

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