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3HWC: The Third HAWC Catalog of Very-High-Energy Gamma-ray Sources

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arxiv 2007.08582 v3 pith:Y4N6N6WK submitted 2020-07-16 astro-ph.HE astro-ph.IM

A. Albert , R. Alfaro , C. Alvarez , J.R. Angeles Camacho , J.C. Arteaga-Velázquez , K.P. Arunbabu , D. Avila Rojas , H.A. Ayala Solares
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classification astro-ph.HEastro-ph.IM
keywords catalogsourcesgamma-raydetectedhawccirccounterpartpotential
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We present a new catalog of TeV gamma-ray sources using 1523 days of data from the High Altitude Water Cherenkov (HAWC) observatory. The catalog represents the most sensitive survey of the Northern gamma-ray sky at energies above several TeV, with three times the exposure compared to the previous HAWC catalog, 2HWC. We report 65 sources detected at $\geq$ 5 sigma significance, along with the positions and spectral fits for each source. The catalog contains eight sources that have no counterpart in the 2HWC catalog, but are within $1^\circ$ of previously detected TeV emitters, and twenty sources that are more than $1^\circ$ away from any previously detected TeV source. Of these twenty new sources, fourteen have a potential counterpart in the fourth \textit{Fermi} Large Area Telescope catalog of gamma-ray sources. We also explore potential associations of 3HWC sources with pulsars in the ATNF pulsar catalog and supernova remnants in the Galactic supernova remnant catalog.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. GeV-TeV Connections in Galaxies: Evolutionary Signatures from Pulsars in Globular Clusters

    astro-ph.HE 2025-08 unverdicted novelty 5.0 of 10

    Globular cluster pulsar winds may make a significant contribution to GeV and TeV gamma-ray emission from massive quiescent galaxies, with strength tied to each galaxy's evolutionary history.

  2. The spectral shapes of Galactic gamma-ray source

    astro-ph.HE 2025-02 conditional novelty 5.0 of 10

    Summing the catalogued spectra of Galactic gamma-ray sources yields a smooth total spectrum, with a break around 30 TeV, built from individual sources of very different shapes.

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