Evidence of TeV gamma-ray emission from the nearby starburst galaxy NGC 253
arXiv:astro-ph/0304295 · doi:10.1051/0004-6361:20030247
Abstract
TeV gamma-rays were recently detected from the nearby normal spiral galaxy NGC 253 (Itoh et al., 2002). Observations to detect the Cherenkov light images initiated by gamma-rays from the direction of NGC 253 were carried out in 2000 and 2001 over a total period of 150 hours. The orientation of images in gamma-ray--like events is not consistent with emission from a point source, and the emission region corresponds to a size greater than 10 kpc in radius. Here, detailed descriptions of the analysis procedures and techniques are given.
16 pages, 27 figures, aa.cls
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Cited by in corpus (12)
- Teraelectronvolt Astronomy
- Detection of Gamma Rays From a Starburst Galaxy
- Detection of Sub-TeV Gamma-Rays from the Galactic Center Direction by CANGAROO-II
- Astrophysical Origins of Ultrahigh Energy Cosmic Rays
- High energy gamma-ray emission from the starburst nucleus of NGC 253
- Detection of Gamma-rays around 1TeV from RX J0852.0-4622 by CANGAROO-II
- A Search for TeV Gamma-ray Emission from the PSR B1259-63/SS2883 Binary System with the CANGAROO-II 10-m Telescope
- A search for very high energy gamma-ray emission from the starburst galaxy NGC 253 with H.E.S.S
- Evidence of TeV gamma-ray emission from the nearby starburst galaxy NGC 253
- Erratum: Detection of diffuse TeV gamma-ray emission from the nearby starburst galaxy NGC 253
- Constraints on Cold Dark Matter in the Gamma-ray Halo of NGC 253
- Search for TeV gamma-rays from SN 1987A in 2001