BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:A TeV follow-up survey of active galactic nuclei with the HAWC gam
 ma-ray observatory
DTSTART;VALUE=DATE-TIME:20190527T210000Z
DTEND;VALUE=DATE-TIME:20190527T212000Z
DTSTAMP;VALUE=DATE-TIME:20260615T140625Z
UID:indico-contribution-47@cern.ch
DESCRIPTION:Speakers: Dr. CARRAMINANA\, Alberto (INAOE)\nActive galactic n
 uclei (AGN)\, the most common type of GeV gamma-ray sources\, have a prepo
 nderant role as extragalactic particle accelerators. Unfortunately our vis
 ion of them is limited to the nearby Universe by the process of photon-pho
 ton attenuation of very high-energy gamma-rays\, which limits the observab
 le distance for a given photon energy coverage. The HAWC gamma-ray observa
 tory\, an extensive air shower array in continuous operation in Mexico sin
 ce 2015\, has surveyed 2/3 of the sky at TeV energies with the sensitivity
  to detect the Crab Nebula in single transits. We present a three year fol
 low-up study of a redshift limited sample of AGN previously detected at Ge
 V energies\, performed with a sensitivity down to integrated photon fluxes
  N(> 0.5TeV) ~ 1e-12 cm-2 s-1.\n\nhttps://indico.nucleares.unam.mx/event/1
 448/session/7/contribution/47
LOCATION:Edificio Carolino\, Benemérita Universidad Autónoma de Puebla S
 ala de Proyecciones
URL:https://indico.nucleares.unam.mx/event/1448/session/7/contribution/47
END:VEVENT
END:VCALENDAR