Canonical Name: | SN 1006 |
TeVCat Name: | TeV J1502-419 |
Other Names: | |
Source Type: | Shell |
R.A.: | 15 02 50 (hh mm ss) |
Dec.: | -41 56 30 (dd mm ss) |
Gal Long: | 327.57 (deg) |
Gal Lat: | 14.56 (deg) |
Distance: | 2.18 kpc |
Flux: | (Crab Units) |
Energy Threshold: | GeV |
Spectral Index: | |
Extended: | No |
Discovery Date: | 1998-04 |
Discovered By: | CANGAROO |
TeVCat SubCat: | Other Sources |
Source Notes:
This source has upper limits from HESS below the
quoted detection flux of CANGAROO and has, since then,
been announced at a lower flux level by H.E.S.S.
(see separate entry in the
Default catalogue).
Seen by: CANGAROO
-
The First X-Ray Proper-Motion Measurements of the Forward Shock in the Northeastern Limb of SN 1006
Katsuda, S. et al., ArXiv e-prints p (2009) [LINK]
-
Reanalysis of Data Taken by the CANGAROO 3.8 Meter Imaging Atmospheric Cherenkov Telescope: PSR B1706-44, SN 1006, and Vela
Yoshikoshi, T. et al., ArXiv e-prints p (2009) [LINK]
-
Upper limits to the SN1006 multi-TeV gamma-ray flux from HESS observations
Aharonian, F. et al., A&A 437 p135-139 (2005) [LINK]
-
Discovery of TeV Gamma Rays from SN 1006: Further Evidence for the Supernova Remnant Origin of Cosmic Rays
Tanimori, T. et al., ApJ 497 pL25+ (1998) [LINK]
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