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Very-high-energy gamma rays from a distant quasar: How transparent is the universe?

Albert J.
•
Aliu E.
•
Anderhub H.
altro
Zapatero J.
2008
  • journal article

Periodico
SCIENCE
Abstract
The atmospheric Cherenkov gamma- ray telescope MAGIC, designed for a low- energy threshold, has detected very- high- energy gamma rays from a giant flare of the distant Quasi- Stellar Radio Source ( in short: radio quasar) 3C 279, at a distance of more than 5 billion light- years ( a redshift of 0.536). No quasar has been observed previously in very- high- energy gamma radiation, and this is also the most distant object detected emitting gamma rays above 50 gigaelectron volts. Because high- energy gamma rays may be stopped by interacting with the diffuse background light in the universe, the observations by MAGIC imply a low amount for such light, consistent with that known from galaxy counts.
DOI
10.1126/science.1157087
WOS
WOS:000257121200032
Archivio
http://hdl.handle.net/11390/878828
info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-46449098817
Diritti
closed access
Scopus© citazioni
434
Data di acquisizione
Jun 2, 2022
Vedi dettagli
Web of Science© citazioni
384
Data di acquisizione
Mar 24, 2024
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