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Deep broadband observations of the distant gamma-ray blazar pks 1424+240
Journal article   Open access

Deep broadband observations of the distant gamma-ray blazar pks 1424+240

S Archambault, T Aune, B Behera, M Beilicke, W Benbow, K Berger, R Bird, J Biteau, V Bugaev, K Byrum, …
The Astrophysical Journal
28 Mar 2014
url
https://doi.org/10.1088/2041-8205/785/1/l16View
Published, Version of Record (VoR)Open Access (License Unspecified) Open

Abstract

absorption bl lacertae objects: individual (pks 1424+240)-cosmic background radiation energy cosmic-ray extragalactic background light gamma rays: galaxies large-area telescope radiation redshift space-telescope mission spectra tev blazars universe
We present deep VERITAS observations of the blazar PKS 1424+240, along with contemporaneous Fermi Large Area Telescope, Swift X-ray Telescope, and Swift UV Optical Telescope data between 2009 February 19 and 2013 June 8. This blazar resides at a redshift of z >= 0.6035, displaying a significantly attenuated gamma-ray flux above 100 GeV due to photon absorption via pair-production with the extragalactic background light. We present more than 100 hr of VERITAS observations over three years, a multiwavelength light curve, and the contemporaneous spectral energy distributions. The source shows a higher flux of (2.1 +/- 0.3) x 10(-7) photons m(-2) s(-1) above 120 GeV in 2009 and 2011 as compared to the flux measured in 2013, corresponding to (1.02 +/- 0.08) x 10-7 photons m(-2) s(-1) above 120 GeV. The measured differential very high energy (VHE; E >= 100 GeV) spectral indices are Gamma = 3.8 +/- 0.3, 4.3 +/- 0.6 and 4.5 +/- 0.2 in 2009, 2011, and 2013, respectively. No significant spectral change across the observation epochs is detected. We find no evidence for variability at gamma-ray opacities of greater than tau = 2, where it is postulated that any variability would be small and occur on timescales longer than a year if hadronic cosmic-ray interactions with extragalactic photon fields provide a secondary VHE photon flux. The data cannot rule out such variability due to low statistics.

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