The High-redshift Blazar S5 0836+71: A Broadband Study
Abstract
A broadband study of the high-redshift blazar S5 0836+71 (z = 2.172) is presented. Multi-frequency light curves show multiple episodes of X-ray and γ-ray flares, while optical-UV fluxes show little variations. During the GeV outburst, the highest γ-ray flux measured is (5.22 ± 1.10) × 10-6 ph c{{m}-2} {{s}-1} in the range of 0.1-300 GeV, which corresponds to an isotropic γ-ray luminosity of (1.62 ± 0.44) × 1050 erg s-1, thereby making this one of the most luminous γ-ray flares ever observed from any blazar. A fast γ-ray flux rising time of ∼3 hr is also noticed, which is probably the first measurement of hour-scale variability detected from a high-redshift (z \gt 2) blazar. The various activity states of S5 0836+71 are reproduced under the assumption of the single-zone leptonic emission model. In all states, the emission region is located inside the broad-line region, and the optical-UV radiation is dominated by the accretion disk emission. The modeling parameters suggest the enhancement in bulk Lorentz factor as a primary cause of the γ-ray flare. The high X-ray activity with a less variable γ-ray counterpart can be due to the emission region being located relatively closer to the black hole where the dominating energy density of the disk emission results in higher X-ray flux due to inverse-Compton scattering of disk photons.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- May 2015
- DOI:
- 10.1088/0004-637X/804/1/74
- arXiv:
- arXiv:1502.07227
- Bibcode:
- 2015ApJ...804...74P
- Keywords:
-
- galaxies: active;
- galaxies: jets;
- galaxies: high-redshift;
- quasars: individual: S5 0836+71;
- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- 41 pages, 9 figures, 6 tables, to appear in The Astrophysical Journal. arXiv admin note: text overlap with arXiv:1501.07363