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Title: Multiwavelength Observations of the Blazar VER J0521+211 during an Elevated TeV Gamma-Ray State

Journal Article · · The Astrophysical Journal
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We report on a long-lasting, elevated gamma-ray flux state from VER J0521+211 observed by VERITAS, MAGIC, and Fermi-LAT in 2013 and 2014. The peak integral flux above 200 GeV measured with the nightly binned light curve is (8.8 ± 0.4) × 10–7 photons m–2 s–1, or ~37% of the Crab Nebula flux. Multiwavelength observations from X-ray, UV, and optical instruments are also presented. A moderate correlation between the X-ray and TeV gamma-ray fluxes was observed, and the X-ray spectrum appeared harder when the flux was higher. Using the gamma-ray spectrum and four models of the extragalactic background light (EBL), a conservative 95% confidence upper limit on the redshift of the source was found to be z ≤ 0.31. Unlike the gamma-ray and X-ray bands, the optical flux did not increase significantly during the studied period compared to the archival low-state flux. The spectral variability from optical to X-ray bands suggests that the synchrotron peak of the spectral energy distribution (SED) may become broader during flaring states, which can be adequately described with a one-zone synchrotron self-Compton model varying the high-energy end of the underlying particle spectrum. The synchrotron peak frequency of the SED and the radio morphology of the jet from the MOJAVE program are consistent with the source being an intermediate-frequency-peaked BL Lac object.

Research Organization:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
Sponsoring Organization:
USDOE Office of Science (SC), Basic Energy Sciences (BES). Scientific User Facilities (SUF)
Contributing Organization:
MAGIC Collaboration; VERITAS Collaboration
Grant/Contract Number:
AC02-05CH11231
OSTI ID:
1983269
Journal Information:
The Astrophysical Journal, Journal Name: The Astrophysical Journal Journal Issue: 2 Vol. 932; ISSN 0004-637X
Publisher:
IOP PublishingCopyright Statement
Country of Publication:
United States
Language:
English

References (56)

The Swift Ultra-Violet/Optical Telescope journal October 2005
The Swift X-Ray Telescope journal October 2005
The major upgrade of the MAGIC telescopes, Part II: A performance study using observations of the Crab Nebula journal January 2016
SciPy 1.0: fundamental algorithms for scientific computing in Python journal February 2020
On characterizing the variability properties of X-ray light curves from active galaxies journal November 2003
The large-scale structure of FR-II radio sources journal July 1998
A unifying view of the spectral energy distributions of blazars journal September 1998
Time-dependent modelling of the Markarian 501 X-ray and TeV gamma-ray data taken during 1997 March and April journal November 2002
Astropy: A community Python package for astronomy journal September 2013
Unprecedented study of the broadband emission of Mrk 421 during flaring activity in March 2010 journal May 2015
An innovative blazar classification based on radio jet kinematics journal July 2016
Multi-wavelength characterization of the blazar S5 0716+714 during an unprecedented outburst phase journal November 2018
A fast, very-high-energy γ -ray flare from BL Lacertae during a period of multi-wavelength activity in June 2015 journal March 2019
Correlation between the TeV and X-ray emission in high-energy peaked BL Lac objects journal March 2005
The Leiden/Argentine/Bonn (LAB) Survey of Galactic HI: Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections journal September 2005
Extragalactic optical-infrared background radiation, its time evolution and the cosmic photon-photon opacity journal June 2008
Unified Schemes for Radio-Loud Active Galactic Nuclei journal June 1995
Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds journal June 1998
Constraints on the Physical Parameters of TeV Blazars journal December 1998
The Swift Gamma‐Ray Burst Mission journal August 2004
Break in the Very High Energy Spectrum of PG 1553+113: New Upper Limit on Its Redshift? journal January 2007
THE FIRST SWIFT ULTRAVIOLET/OPTICAL TELESCOPE GRB AFTERGLOW CATALOG journal December 2008
THE LARGE AREA TELESCOPE ON THE FERMI GAMMA-RAY SPACE TELESCOPE MISSION journal May 2009
Stability of Relativistic Force-Free jets journal May 2009
Modeling the Extragalactic Background Light from Stars and dust journal February 2010
Spectral Energy Distribution of Markarian 501: Quiescent State Versus Extreme Outburst journal February 2011
Measuring Reddening with Sloan Digital sky Survey Stellar Spectra and Recalibrating sfd journal August 2011
RAPID TeV GAMMA-RAY FLARING OF BL LACERTAE journal December 2012
Spectroscopy of the Largest ever γ-Ray-Selected bl lac Sample journal January 2013
Studies in Astronomical time Series Analysis. vi. Bayesian Block Representations journal February 2013
DISCOVERY OF A NEW TeV GAMMA-RAY SOURCE: VER J0521+211 journal September 2013
The 1% Concordance Hubble Constant journal October 2014
FERMI LARGE AREA TELESCOPE THIRD SOURCE CATALOG journal June 2015
A METHOD FOR SETTING UPPER LIMITS TO THE EXTRAGALACTIC BACKGROUND LIGHT WITH FERMI -LAT AND TeV OBSERVATIONS OF BLAZARS journal April 2010
Magic Discovery of very high Energy Emission from the fsrq pks 1222+21 journal February 2011
Deep Broadband Observations of the Distant Gamma-Ray Blazar pks 1424+240 journal March 2014
Calibration of X-ray absorption in our Galaxy journal March 2013
Temporal correlation between the optical and γ-ray flux variations in the blazar 3C 454.3 journal April 2019
Photohadronic neutrinos from transients in astrophysical sources journal November 1998
Matplotlib: A 2D Graphics Environment journal January 2007
The NumPy Array: A Structure for Efficient Numerical Computation journal March 2011
Photometric calibration of the Swift ultraviolet/optical telescope: Photometric calibration of the Swift UVOT journal December 2007
Superorbital variability of X-ray and radio emission of Cyg X-1 - II. Dependence of the orbital modulation and spectral hardness on the superorbital phase journal September 2008
Extragalactic background light inferred from AEGIS galaxy-SED-type fractions: EBL from AEGIS galaxy-SED-type fractions journal October 2010
Semi-analytic modelling of the extragalactic background light and consequences for extragalactic gamma-ray spectra: Modelling of the EBL and gamma-ray spectra journal April 2012
In-flight calibration of the Swift XRT Point Spread Function conference August 2005
Magnetic Fields in Blazar Pc-Scale jets — Possible Connection to spin Rates of Black Holes? journal September 2008
The Origin of Ultra-High-Energy Cosmic Rays journal September 1984
seaborn: statistical data visualization journal April 2021
MULTIWAVELENGTH STUDY OF QUIESCENT STATES OF Mrk 421 WITH UNPRECEDENTED HARD X-RAY COVERAGE PROVIDED BY NuSTAR IN 2013 journal March 2016
The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package journal August 2018
On the Redshift of TeV BL Lac Objects journal March 2017
Multiwavelength Observations of the Blazar BL Lacertae: A New Fast TeV Gamma-Ray Flare journal March 2018
MOJAVE. XVII. Jet Kinematics and Parent Population Properties of Relativistically Beamed Radio-loud Blazars journal March 2019
A Decade of Multiwavelength Observations of the TeV Blazar 1ES 1215+303: Extreme Shift of the Synchrotron Peak Frequency and Long-term Optical–Gamma-Ray Flux Increase journal March 2020
MOJAVE. XV. VLBA 15 GHz Total Intensity and Polarization Maps of 437 Parsec-scale AGN Jets from 1996 to 2017 journal January 2018