Astrophysics with MILAGRO
19946 pages
Part of Proceedings, 2nd Compton Symposium on Gamma Ray Astronomy : College Park, Maryland, September 20-22, 1994, 726-730
Published in:
- AIP Conf.Proc. 304 (1994) 726-730
Contribution to:
- Published: May 12, 2008
DOI:
Experiments:
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Abstract: (AIP)
This paper describes how data from a new type of air shower detector, MILAGRO, can shed light on a variety of interesting problems in astrophysics. MILAGRO has the capability to make observations of VHE/UHE emission from the recently discovered TeV gamma‐ray source Markarian 421, an Active Galactic Nucleus (AGN). An observation of the attenuation of this signal in the range of 1–20 TeV can be used to make the first measurement of the intergalactic infrared radiation. We will also describe how MILAGRO can improve the existing limits on the density of Primordial Black Holes (PBH) by three orders of magnitude. In addition, MILAGRO will have a large aperture and continuous operation which gives it the capability to search for VHE gamma ray bursts.- Active galaxies
- Astrophysics
- Attenuation
- Black holes
- Cosmic gamma ray sources
- gamma ray: burst
- gamma ray: VHE
- black hole: primordial
- density: primordial
- radiation: infrared
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