paper

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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