Issue |
A&A
Volume 391, Number 3, September I 2002
|
|
---|---|---|
Page(s) | L25 - L28 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361:20021034 | |
Published online | 09 August 2002 |
Letter to the Editor
Detection of the BL Lac object 1ES 1426+428 in the Very High Energy gamma-ray band by the CAT Telescope from 1998–2000
1
Physique Corpuscul aire et Cosmologie, IN2P3/CNRS, Collège de France et Université Paris VII, 75231 Paris Cedex 05, France
2
Laboratoire Leprince-Ringuet, IN2P3/CNRS, École Polytechnique, 91128 Palaiseau, France
3
Centre d'Études Spatiales des Rayonnements, INSU/CNRS, Université Paul Sabatier, 31028 Toulouse, France
4
Groupe de Physique Fondamentale, Université de Perpignan, 66860 Perpignan, France
5
Service d'Astrophysique, CEA/DSM/DAPNIA, Centre d'Études de Saclay, 91191 Gif-sur-Yvette, France
6
Laboratoire de Physique Nucléaire et de Hautes Énergies, IN2P3/CNRS, Universités Paris VI/VII, 75252 Paris Cedex 05, France
7
Institute of Particle and Nuclear Physics, Charles University, 11636 Prague, Czech Republic
Corresponding author: A. Djannati-Ataï, djannati@in2p3.fr
Received:
18
June
2002
Accepted:
12
July
2002
The BL Lac Object 1ES 1426+428, at a red-shift of
, has been monitored by the Cat
telescope from February 1998 to June 2000. The accumulation of 26 h of observations shows a γ-ray signal of 321 events above
at 5.2 standard deviations,
determined using data analysis cuts adapted to a weak, steep-spectrum
source.
The source emission has an average flux of
,
and a very steep spectrum, with a differential spectral index of
which can be refined to
using a higher flux data subset.
If, as expected from its broad-band properties, the Very High Energy
emission is hard at the source, these observations support a strong
absorption effect of γ-rays by the Intergalactic Infrared field.
Key words: galaxies: active / galaxies: nuclei / BL Lacertæ objects: individual: 1ES 1426+428 / gamma-rays: observations
© ESO, 2002
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