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Title: S5 0716+714: GeV variability study

Journal Article · · Advances in Space Research
 [1];  [2];  [3];  [2];  [2]
  1. Max-Planck-Institut fur Radioastronomie (MPIfR) (Germany); Aryabhatta Research Institute of Observational Sciences (ARIES), Manora Peak (India)
  2. Max-Planck-Institut fur Radioastronomie (MPIfR) (Germany)
  3. Universite Bordeaux 1, CNRS/IN2p3, Centre d Etudes Nucleaires de Bordeaux Gradignan (France)

The GeV observations by Fermi-LAT give us the opportunity to characterize the high-energy emission (100 MeV–300 GeV) variability properties of the BL Lac object S5 0716+714. In this study, we performed flux and spectral analysis of more than 3 year long (August 2008 to April 2012) Fermi-LAT data of the source. During this period, the source exhibits two different modes of flux variability with characteristic timescales of ~75 and ~140 days, respectively. In addition, we also notice that the flux variations are characterized by a weak spectral hardening. The GeV spectrum of the source shows a clear deviation from a simple power law, and is better explained by a broken power law. Similar to other bright Fermi blazars, the break energy does not vary with the source flux during the different activity states. Finally, we discuss several possible scenarios to explain the observed spectral break.

Research Organization:
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Contributing Organization:
Fermi-LAT Collaboration
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1356588
Journal Information:
Advances in Space Research, Vol. 51, Issue 12; ISSN 0273-1177
Publisher:
ElsevierCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 11 works
Citation information provided by
Web of Science

References (21)

FERMI /LARGE AREA TELESCOPE BRIGHT GAMMA-RAY SOURCE LIST journal June 2009
SPECTRAL PROPERTIES OF BRIGHT FERMI -DETECTED BLAZARS IN THE GAMMA-RAY BAND journal January 2010
THE SECOND CATALOG OF ACTIVE GALACTIC NUCLEI DETECTED BY THE FERMI LARGE AREA TELESCOPE journal December 2011
Discovery of very high Energy γ-Rays from the Blazar s5 0716+714 journal October 2009
AGILE detection of variable γ -ray activity from the blazar S5 0716+714 in September–October 2007 journal September 2008
Disentangling the synchrotron and inverse Compton variability in the X-ray emission of the intermediate BL Lacertae object S5 0716+71 journal September 2006
ON THE BREAK IN THE FERMI -LARGE AREA TELESCOPE SPECTRUM OF 3C 454.3 journal April 2010
Simultaneous X-ray and optical observations of S5 0716+714 after the outburst of March 2004 journal August 2006
Multiwavelength intraday variability of the BL Lacertae S5 0716+714: Multiwavelength variability of the BL Lac S5 0716+714 journal August 2012
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EGRET observations of the BL Lacertae objects 0716+714 and 0521-365 journal March 1995
An adaptive-binning method for generating constant-uncertainty/constant-significance light curves with Fermi -LAT data journal July 2012
Does the Blazar Gamma‐Ray Spectrum Harden with Increasing Flux? Analysis of 9 Years of EGRET Data journal March 2007
Detection of the host galaxy of S5 0716+714 journal July 2008
GeV BREAKS IN BLAZARS AS A RESULT OF GAMMA-RAY ABSORPTION WITHIN THE BROAD-LINE REGION journal June 2010
Optical and radio behaviour of the BL Lacertae object 0716+714 journal April 2003
Quasi-Periodic Oscillations of ∼15 Minutes in the Optical Light Curve of the bl lac s5 0716+714 journal July 2010
Nearly Periodic Fluctuations in the Long-Term X-Ray Light Curves of the Blazars ao 0235+164 and 1es 2321+419 journal April 2009
Modelling the very high energy flare of 3C 279 using one-zone leptonic model: Modelling the VHE flare of 3C 279 journal November 2011
Flicker of extragalactic radio sources at two frequencies journal September 1985
FERMI LARGE AREA TELESCOPE DETECTION OF BRIGHT γ-RAY OUTBURSTS FROM THE PECULIAR QUASAR 4C +21.35 journal April 2011

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The Connection Between the Radio jet and the Gamma-Ray Emission in the Radio Galaxy 3c 120 journal July 2015

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