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Title: MAGIC detection of short-term variability of the high-peaked BL Lac object 1ES 0806+524

Journal Article · · Monthly Notices of the Royal Astronomical Society
DOI:https://doi.org/10.1093/mnras/stv895· OSTI ID:1356435
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The high-frequency-peaked BL Lac (HBL) 1ES 0806+524 (z = 0.138) was discovered in very high energy (VHE) γ-rays in 2008. Until now, the broad-band spectrum of 1ES 0806+524 has been only poorly characterized, in particular at high energies. In this paper, we analysed multiwavelength observations from γ-rays to radio performed from 2011 January to March, which were triggered by the high activity detected at optical frequencies. These observations constitute the most precise determination of the broad-band emission of 1ES 0806+524 to date. The stereoscopic Major Atmospheric Gamma-Ray Imaging Cherenkov (MAGIC) observations yielded a γ-ray signal above 250 GeV of (3.7 ± 0.7) per cent of the Crab Nebula flux with a statistical significance of 9.9σ. The multiwavelength observations showed significant variability in essentially all energy bands, including a VHE γ-ray flare that lasted less than one night, which provided unprecedented evidence for short-term variability in 1ES 0806+524. The spectrum of this flare is well described by a power law with a photon index of 2.97 ± 0.29 between ~150 GeV and 1 TeV and an integral flux of (9.3 ± 1.9) per cent of the Crab nebula flux above 250 GeV. The spectrum during the non-flaring VHE activity is compatible with the only available VHE observation performed in 2008 with VERITAS when the source was in a low optical state. Lastly, the broad-band spectral energy distribution can be described with a one-zone synchrotron self-Compton model with parameters typical for HBLs, indicating that 1ES 0806+524 is not substantially different from the HBLs previously detected.

Research Organization:
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Contributing Organization:
Fermi-LAT Collaboration; MAGIC Collaboration
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1356435
Journal Information:
Monthly Notices of the Royal Astronomical Society, Vol. 451, Issue 1; ISSN 0035-8711
Publisher:
Royal Astronomical SocietyCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 18 works
Citation information provided by
Web of Science

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Gamma-ray Excess from a Stacked Sample of High- and Intermediate-frequency Peaked Blazars Observed with the MAGIC Telescope text January 2011
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Systematic search for VHE gamma-ray emission from X-ray bright high-frequency BL Lac objects text January 2007
Host galaxy subtraction of TeV candidate BL Lacertae objects text January 2007
Implementation of the Random Forest Method for the Imaging Atmospheric Cherenkov Telescope MAGIC text January 2007
Simultaneous multiwavelength observations of the blazar 1ES1959+650 at a low TeV flux text January 2008
Infrared to X-ray observations of PKS 2155-304 in a low state text January 2008
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Very-High-Energy Gamma Rays from a Distant Quasar: How Transparent Is the Universe? text January 2008
Improving the performance of the single-dish Cherenkov telescope MAGIC through the use of signal timing text January 2008
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TeV candidate BL Lac objects text January 2001
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Cited By (14)

Insights into the emission of the blazar 1ES 1011+496 through unprecedented broadband observations during 2011 and 2012 journal June 2016
Optical polarization of high-energy BL Lacertae objects journal December 2016
Empirical multi-wavelength prediction method for very high energy gamma-ray emitting BL Lacertae objects journal December 2017
Long-term optical monitoring of TeV emitting blazars: I. Data analysis⋆ journal December 2018
Investigating the peculiar emission from the new VHE gamma-ray source H1722+119 journal March 2016
Optical Variability Modeling of Newly Identified Blazar Candidates behind Magellanic Clouds journal January 2020
On the Jet Properties of γ -Ray-loud Active Galactic Nuclei journal April 2018
Multi-TeV Flaring from High-energy Blazars: An Evidence of the Photohadronic Process journal October 2019
Insights into the emission of the blazar 1ES 1011+496 through unprecedented broadband observations during 2011 and 2012 text January 2016
Investigating the peculiar emission from the new VHE gamma-ray source H1722+119 text January 2016
Investigating the peculiar emission from the new VHE gamma-ray source H1722+119 text January 2016
Optical polarization of high-energy BL Lac objects text January 2016
Multi-TeV flaring from high energy blazars: An evidence of the photohadronic process text January 2019
Optical variability modeling of newly identified blazar candidates behind Magellanic Clouds text January 2019

Figures / Tables (11)


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