Observations of H1426+428 from 1999 to 2002 with The Whipple Observatory 10 m Telescope
| dc.creator | Horan, D. | |
| dc.date | 2003-05-29 | |
| dc.date.accessioned | 2026-07-07T02:08:38Z | |
| dc.date.available | 2026-07-07T02:08:38Z | |
| dc.description | The BL Lacertae object H1426+428 is the most distant, confirmed source of TeV gamma rays. At a redshift of 0.129, its detection at TeV energies has important implications for estimating the density of the extragalactic infra-red background radiation. H1426+428 was observed extensively during the 2001/2002 observing season with the Whipple 10 m gamma-ray telescope. The results of these observations are presented here and are combined with the results of previous observations made between 1999 and 2001 at Whipple. | |
| dc.description | 4 pages to be published in the Proceedings of the 28th International Cosmic Ray Conference (Tsukuba, Japan 2003) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0305579 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0305579 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6128 | |
| dc.subject | Astrophysics | |
| dc.title | Observations of H1426+428 from 1999 to 2002 with The Whipple Observatory 10 m Telescope | |
| dc.type | text |