Search for very-high-energy emission from Gamma-ray Bursts using the first 18 months of data from the HAWC Gamma-ray Observatory

Article, Preprint English OPEN
The HAWC Collaboration; Alfaro, R.; Alvarez, C.; Álvarez, J.; Arceo, R.; Arteaga-Velázquez, J.; Rojas, D.; Solares, H.; Barber, A.; Bautista-Elivar, N.; Becerril, A.; Belmont-Moreno, E.; BenZvi, S.; Bernal, A.; Braun, J.; Brisbois, C.; Caballero-Mora, K.; Capistrán, T.; Carramiñana, A.; Casanova, S.; Castillo, M.; Cotti, U.; Cotzomi, J.; de León, S.; de la Fuente, E.; De León, C.; DeYoung, T.; Hernandez, R.; Dingus, B.; DuVernois, M.; ... view all 105 authors
(2017)
  • Identifiers: doi: 10.3847/1538-4357/aa756f
  • Subject: Astrophysics - High Energy Astrophysical Phenomena | HAWC - Abteilung Hinton
    arxiv: Astrophysics::High Energy Astrophysical Phenomena

The High Altitude Water Cherenkov (HAWC) Gamma-ray Observatory is an extensive air shower detector operating in central Mexico, which has recently completed its first two years of full operations. If for a burst like GRB 130427A at a redshift of 0.34 and a high-energy c... View more
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