Radio to gamma-ray variability study of blazar S5 0716+714

Rani, B.; Krichbaum, T. P.; Fuhrmann, L.; Böttcher, M.; Lott, B.; Aller, H. D.; Aller, M. F.; Angelakis, E.; Bach, U.; Bastieri, D.; Falcone, A. D.; Fukazawa, Y.; Gabanyi, K. E.; Gupta, A. C.; Gurwell, M.; Itoh, R.; Kawabata, K. S.; Krips, M.; Lähteenmäki, A. A.; Liu, X.; Marchili, N.; Max-Moerbeck, W.; Nestoras, I.; Nieppola, E.; Quintana-Lacaci, G.; Readhead, A. C.  S.; Richards, J. L.; Sasada, M.; Sievers, A.; Sokolovsky, K.; Stroh, M.; Tammi, J.; Tornikoski, M.; Uemura, M.; Ungerechts, H.; Urano, T.; Zensus, J. A.

doi:10.1051/0004-6361/201321058

Title: Radio to gamma-ray variability study of blazar S5 0716+714

Journal Article · Wed Mar 13 00:00:00 EDT 2013 · Astronomy and Astrophysics

DOI:https://doi.org/10.1051/0004-6361/201321058· OSTI ID:1356594

Rani, B.; Krichbaum, T. P.; Fuhrmann, L.; Böttcher, M.; Lott, B.; Aller, H. D.; Aller, M. F.; Angelakis, E.; Bach, U.; Bastieri, D.; Falcone, A. D.; Fukazawa, Y.; Gabanyi, K. E.; Gupta, A. C.; Gurwell, M.; Itoh, R.; Kawabata, K. S.; Krips, M.; Lähteenmäki, A. A.; Liu, X. more »

In this paper, we present the results of a series of radio, optical, X-ray, and γ-ray observations of the BL Lac object S50716+714 carried out between April 2007 and January 2011. The multifrequency observations were obtained using several ground- and space-based facilities. The intense optical monitoring of the source reveals faster repetitive variations superimposed on a long-term variability trend on a time scale of ~350 days. Episodes of fast variability recur on time scales of ~60-70 days. The intense and simultaneous activity at optical and γ-ray frequencies favors the synchrotron self-Compton mechanism for the production of the high-energy emission. Two major low-peaking radio flares were observed during this high optical/γ-ray activity period. The radio flares are characterized by a rising and a decaying stage and agrees with the formation of a shock and its evolution. We found that the evolution of the radio flares requires a geometrical variation in addition to intrinsic variations of the source. Different estimates yield robust and self-consistent lower limits of δ ≥ 20 and equipartition magnetic field B_eq ≥ 0.36 G. Causality arguments constrain the size of emission region θ ≤ 0.004 mas. We found a significant correlation between flux variations at radio frequencies with those at optical and γ-rays. Theoptical/GeV flux variations lead the radio variability by ~65 days. The longer time delays between low-peaking radio outbursts and optical flares imply that optical flares are the precursors of radio ones. An orphan X-ray flare challenges the simple, one-zone emission models, rendering them too simple. Finally, here we also describe the spectral energy distribution modeling of the source from simultaneous data taken through different activity periods.

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Research Organization:: SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)

Sponsoring Organization:: USDOE

Contributing Organization:: Fermi-LAT Collaboration

Grant/Contract Number:: AC02-76SF00515

OSTI ID:: 1356594

Journal Information:: Astronomy and Astrophysics, Vol. 552; ISSN 0004-6361

Publisher:: EDP SciencesCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 75 works

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Multiwavelength picture of the blazar S5 0716+714 during its brightest outburst Manganaro, Marina; Pedaletti, Giovanna; Doert, Marlene arXiv https://doi.org/10.48550/arxiv.1704.03238	text	January 2017
Interferometric Monitoring of Gamma-ray Bright AGNs: S5 0716+714 Lee, Jee Won; Lee, Sang-Sung; Hodgson, Jeffrey A. arXiv https://doi.org/10.48550/arxiv.1705.06835	text	January 2017
Multiwavelength Photometric and Spectropolarimetric Analysis of the FSRQ 3C 279 Patiño-Álvarez, V. M.; Fernandes, S.; Chavushyan, V. arXiv https://doi.org/10.48550/arxiv.1806.01693	text	January 2018
Multiwavelength Cross-Correlations and Flaring Activity in Bright Blazars Liodakis, I.; Romani, R. W.; Filippenko, A. V. arXiv https://doi.org/10.48550/arxiv.1808.05625	text	January 2018
Ejection of Double knots from the radio core of PKS 1510--089 during the strong gamma-ray flares in 2015 Park, Jongho; Lee, Sang-Sung; Kim, Jae-Young arXiv https://doi.org/10.48550/arxiv.1904.11118	text	January 2019
Optical variability modeling of newly identified blazar candidates behind Magellanic Clouds Żywucka, Natalia; Tarnopolski, Mariusz; Böttcher, Markus arXiv https://doi.org/10.48550/arxiv.1912.03530	text	January 2019
H.E.S.S. Monitoring of PKS 2155-304 in 2015 and 2016 Wierzcholska, Alicja; Zacharias, Michael; Jankowsky, Felix arXiv https://doi.org/10.48550/arxiv.1908.01232	text	January 2019

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