A survey of Active Galaxies with the HAWC Gamma-ray Observatory
Abstract
The High Altitude Water Cherenkov Gamma-Ray Observatory has been accumulating a progressively deeper exposure of the TeV sky since its inauguration in March 2015. Located at geographical latitude $+19^\circ$N, HAWC has been able to perform a deep and unbiased survey of two thirds of the sky. We analyzed three years of HAWC data searching for long term persistent emission from a redshift limited ($z\leq 0.3$) sample of active galactic nuclei drawn from the {\it Fermi}-LAT 3FHL catalog. The HAWC dataset confirms the high significance detection of the two nearest BL Lac objects, \mbox{Mrk 421} and \mbox{Mrk 501}, and sets limits for the rest of the sample, down to integrated photon fluxes of order $N(>0.5~{\rm TeV})\lesssim 10^{-12}\,\rm cm^{-2}s^{-1}$. We present and discuss some of the results of this survey, focusing on individual objects of particular interest.
- Publication:
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arXiv e-prints
- Pub Date:
- August 2019
- DOI:
- arXiv:
- arXiv:1908.06831
- Bibcode:
- 2019arXiv190806831C
- Keywords:
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- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- Contribution to the International Cosmic Ray Conference ICRC 2019. 8 pages, 3 figures. A couple of errors in Table 1 have been corrected