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VERITAS and multiwavelength observations of the BL Lacertae object 1ES 1741+196
Journal article   Open access

VERITAS and multiwavelength observations of the BL Lacertae object 1ES 1741+196

A. U. Abeysekara, S. Archambault, A. Archer, W. Benbow, R. Bird, J. Biteau, M. Buchovecky, J. H. Buckley, V. Bugaev, K. Byrum, …
Monthly notices of the Royal Astronomical Society, v 459(3), pp 2550-2557
01 Jul 2016
url
https://doi.org/10.1093/mnras/stw664View
Published, Version of Record (VoR)Maybe Open Access (Publisher Bronze) Open

Abstract

Astronomy & Astrophysics Physical Sciences Science & Technology
We present results from multiwavelength observations of the BL Lacertae object 1ES 1741 + 196, including results in the very high energy gamma-ray regime using the Very Energetic Radiation Imaging Telescope Array System (VERITAS). The VERITAS time-averaged spectrum, measured above 180 GeV, is well modelled by a power law with a spectral index of 2.7 +/- 0.7(stat) +/- 0.2(syst). The integral flux above 180 GeV is (3.9 +/- 0.8(stat) +/- 1.0(syst)) x 10(-8) m(-2) s(-1), corresponding to 1.6 per cent of the Crab nebula flux on average. The multiwavelength spectral energy distribution of the source suggests that 1ES 1741+196 is an extreme-high-frequency-peaked BL Lacertae object. The observations analysed in this paper extend over a period of six years, during which time no strong flares were observed in any band. This analysis is therefore one of the few characterizations of a blazar in a non-flaring state.

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Web of Science research areas
Astronomy & Astrophysics
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