The Astrophysical Journal (Jan 2023)

VERITAS Discovery of Very High Energy Gamma-Ray Emission from S3 1227+25 and Multiwavelength Observations

  • A. Acharyya,
  • C. B. Adams,
  • A. Archer,
  • P. Bangale,
  • W. Benbow,
  • A. Brill,
  • J. L. Christiansen,
  • A. J. Chromey,
  • M. Errando,
  • A. Falcone,
  • Q. Feng,
  • J. P. Finley,
  • G. M. Foote,
  • L. Fortson,
  • A. Furniss,
  • G. Gallagher,
  • W. Hanlon,
  • D. Hanna,
  • O. Hervet,
  • C. E. Hinrichs,
  • J. Hoang,
  • J. Holder,
  • W. Jin,
  • M. N. Johnson,
  • P. Kaaret,
  • M. Kertzman,
  • D. Kieda,
  • T. K. Kleiner,
  • N. Korzoun,
  • F. Krennrich,
  • M. J. Lang,
  • M. Lundy,
  • G. Maier,
  • C. E McGrath,
  • M. J. Millard,
  • J. Millis,
  • C. L. Mooney,
  • P. Moriarty,
  • R. Mukherjee,
  • S. O’Brien,
  • R. A. Ong,
  • M. Pohl,
  • E. Pueschel,
  • J. Quinn,
  • K. Ragan,
  • P. T. Reynolds,
  • D. Ribeiro,
  • E. Roache,
  • I. Sadeh,
  • A. C. Sadun,
  • L. Saha,
  • M. Santander,
  • G. H. Sembroski,
  • R. Shang,
  • M. Splettstoesser,
  • A. K. Talluri,
  • J. V. Tucci,
  • V. V. Vassiliev,
  • D. A. Williams,
  • S. L. Wong,
  • The VERITAS Collaboration,
  • Talvikki Hovatta,
  • Svetlana G. Jorstad,
  • Sebastian Kiehlmann,
  • Anne Lähteenmäki,
  • Ioannis Liodakis,
  • Alan P. Marscher,
  • Walter Max-Moerbeck,
  • Anthony C. S. Readhead,
  • Rodrigo Reeves,
  • Paul S. Smith,
  • Merja Tornikoski

DOI
https://doi.org/10.3847/1538-4357/acd2d0
Journal volume & issue
Vol. 950, no. 2
p. 152

Abstract

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We report the detection of very high energy gamma-ray emission from the blazar S3 1227+25 (VER J1230+253) with the Very Energetic Radiation Imaging Telescope Array System (VERITAS). VERITAS observations of the source were triggered by the detection of a hard-spectrum GeV flare on 2015 May 15 with the Fermi-Large Area Telescope (LAT). A combined 5 hr VERITAS exposure on May 16 and 18 resulted in a strong 13 σ detection with a differential photon spectral index, Γ = 3.8 ± 0.4, and a flux level at 9% of the Crab Nebula above 120 GeV. This also triggered target-of-opportunity observations with Swift, optical photometry, polarimetry, and radio measurements, also presented in this work, in addition to the VERITAS and Fermi-LAT data. A temporal analysis of the gamma-ray flux during this period finds evidence of a shortest variability timescale of τ _obs = 6.2 ± 0.9 hr, indicating emission from compact regions within the jet, and the combined gamma-ray spectrum shows no strong evidence of a spectral cutoff. An investigation into correlations between the multiwavelength observations found evidence of optical and gamma-ray correlations, suggesting a single-zone model of emission. Finally, the multiwavelength spectral energy distribution is well described by a simple one-zone leptonic synchrotron self-Compton radiation model.

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