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Title: FERMI LARGE AREA TELESCOPE OBSERVATIONS OF MARKARIAN 421: THE MISSING PIECE OF ITS SPECTRAL ENERGY DISTRIBUTION

Journal Article · · Astrophysical Journal
 [1]; ; ; ; ; ; ; ;  [2]; ; ; ;  [3];  [4];  [5];  [6];  [7];  [8];  [9];  [10]
  1. National Research Council Research Associate, National Academy of Sciences, Washington, DC 20001 (United States)
  2. W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305 (United States)
  3. Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, I-56127 Pisa (Italy)
  4. Laboratoire AIM, CEA-IRFU/CNRS/Universite Paris Diderot, Service d'Astrophysique, CEA Saclay, 91191 Gif sur Yvette (France)
  5. Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, I-34127 Trieste (Italy)
  6. Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I-35131 Padova (Italy)
  7. Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I-06123 Perugia (Italy)
  8. Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064 (United States)
  9. Dipartimento di Fisica 'M. Merlin' dell'Universita e del Politecnico di Bari, I-70126 Bari (Italy)
  10. Laboratoire Leprince-Ringuet, Ecole polytechnique, CNRS/IN2P3, Palaiseau (France)

We report on the {gamma}-ray activity of the high-synchrotron-peaked BL Lacertae object Markarian 421 (Mrk 421) during the first 1.5 years of Fermi operation, from 2008 August 5 to 2010 March 12. We find that the Large Area Telescope (LAT) {gamma}-ray spectrum above 0.3 GeV can be well described by a power-law function with photon index {Gamma} = 1.78 {+-} 0.02 and average photon flux F(> 0.3 GeV) = (7.23 {+-} 0.16) x 10{sup -8} ph cm{sup -2} s{sup -1}. Over this time period, the Fermi-LAT spectrum above 0.3 GeV was evaluated on seven-day-long time intervals, showing significant variations in the photon flux (up to a factor {approx}3 from the minimum to the maximum flux) but mild spectral variations. The variability amplitude at X-ray frequencies measured by RXTE/ASM and Swift/BAT is substantially larger than that in {gamma}-rays measured by Fermi-LAT, and these two energy ranges are not significantly correlated. We also present the first results from the 4.5 month long multifrequency campaign on Mrk 421, which included the VLBA, Swift, RXTE, MAGIC, the F-GAMMA, GASP-WEBT, and other collaborations and instruments that provided excellent temporal and energy coverage of the source throughout the entire campaign (2009 January 19 to 2009 June 1). During this campaign, Mrk 421 showed a low activity at all wavebands. The extensive multi-instrument (radio to TeV) data set provides an unprecedented, complete look at the quiescent spectral energy distribution (SED) for this source. The broadband SED was reproduced with a leptonic (one-zone synchrotron self-Compton) and a hadronic model (synchrotron proton blazar). Both frameworks are able to describe the average SED reasonably well, implying comparable jet powers but very different characteristics for the blazar emission site.

OSTI ID:
21578244
Journal Information:
Astrophysical Journal, Vol. 736, Issue 2; Other Information: DOI: 10.1088/0004-637X/736/2/131; ISSN 0004-637X
Country of Publication:
United States
Language:
English

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VLBA monitoring of Mrk 421 at 15 GHz and 24 GHz during 2011 journal September 2012
Discovery of high and very high-energy emission from the BL Lacertae object SHBL J001355.9–185406 journal June 2013
The TeV blazar Markarian 421 at the highest spatial resolution journal November 2013
The 2009 multiwavelength campaign on Mrk 421: Variability and correlation studies journal April 2015
Unprecedented study of the broadband emission of Mrk 421 during flaring activity in March 2010 journal May 2015
The F-GAMMA programme: multi-frequency study of active galactic nuclei in the Fermi era : Programme description and the first 2.5 years of monitoring⋆ journal November 2016
Long-term multi-wavelength variability and correlation study of Markarian 421 from 2007 to 2009 journal September 2016
The TANAMI Multiwavelength Program: Dynamic spectral energy distributions of southern blazars journal June 2016
Very high energy outburst of Markarian 501 in May 2009 journal October 2016
Multiband variability studies and novel broadband SED modeling of Mrk 501 in 2009 journal July 2017
Long-term optical monitoring of TeV emitting blazars: I. Data analysis⋆ journal December 2018
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A hadronic origin for ultra-high-frequency-peaked BL Lac objects journal February 2015
Photohadronic origin of $\boldsymbol {\gamma }$-ray BL Lac emission: implications for IceCube neutrinos journal March 2015
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Swift Observations of Mrk 421 in Selected Epochs. I. The Spectral and Flux Variability in 2005–2008 journal February 2018
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Stable Radio Core of the Blazar Mrk 501 during High-energy Active State in 2012 journal October 2019
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THE SWIFT /BAT HARD X-RAY TRANSIENT MONITOR journal October 2013
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Discovery of high and very high-energy emission from the BL Lacertae object SHBL J001355.9–185406 text January 2013
Very high energy outburst of Markarian 501 in May 2009 text January 2016
Multiband variability studies and novel broadband SED modeling of Mrk 501 in 2009 text January 2017
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MAGIC detection of very high energy γ-ray emission from the low-luminosity blazar 1ES 1741+196 journal February 2017
Long-term multi-wavelength variability and correlation study of Markarian 421 from 2007 to 2009 text January 2016
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New Hard-TeV Extreme Blazars Detected with the MAGIC Telescopes text January 2020
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Unprecedented study of the broadband emission of Mrk 421 during flaring activity in March 2010 text January 2014
The Origin of the Extragalactic Gamma-Ray Background and Implications for Dark-Matter Annihilation text January 2015
The 2009 multiwavelength campaign on Mrk 421: Variability and correlation studies text January 2015
The F-GAMMA program: Multi-frequency study of Active Galactic Nuclei in the Fermi era. Program description and the first 2.5 years of monitoring text January 2016
Multiband variability studies and novel broadband SED modeling of Mrk 501 in 2009 text January 2016
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The correlation between the total magnetic flux and the total jet power text January 2018
Possible Accretion Disk Origin of the Emission Variability of a Blazar Jet text January 2018
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