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Observation Date (UT) Observation Lat

Canonical Name:M 82
TeVCat Name:TeV J0955+696
Other Names:NGC 3034
Source Type:Starburst
R.A.:09 55 52.7 (hh mm ss)
Dec.:+69 40 46 (dd mm ss)
Gal Long: 141.41 (deg)
Gal Lat: 40.57 (deg)
Distance: 3900 kpc
Flux:0.009 (Crab Units)
Energy Threshold:700 GeV
Spectral Index:2.5
Extended:No
Discovery Date:2009-07
Discovered By: VERITAS
TeVCat SubCat:Default Catalog

Source Notes:

This detection was announced by VERITAS at the 31st ICRC in Lodz with details following in VERITAS Collaboration (2009)..

Source position and its uncertainty:
- The position provided in TeVCat comes from NED:
- From Jackson et al. (2007):
- R.A. (J2000): 09h 55m 52.725s
- Dec. (J2000): +69d 40m 45.78s

Flux and Spectral Properties:
From VERITAS Collaboration (2009):
- "At a flux of 0.9% of that observed from the Crab Nebula, M 82 is
among the weakest VHE sources ever detected."
- "The observed differential VHE gamma-ray spectrum is best fitted
using a power-law function with a photon index of:"
... 2.5 +/- 0.6 (stat) +/- 0.2 (syst)
- "The measured gamma-ray flux is:"
... 3.7 +/- 0.8 (stat) +/- 0.7 (syst) x10e-13 cm-2 s-1 above 700 GeV
- "no flux variations are observed"
- "The luminosity of M 82 above 700 GeV inferred from the gamma-ray
flux is 2 x 10e32 W, or about 2 x 10e6 times smaller than its far
infrared luminosity (Sanders et al., 2003)"

Distance:
From Sakai & Madore (1999):
- "M82 lies at a distance of 3.9 +/- 0.3 (random) +/- 0.3 (syst) Mpc"
- this corresponds to a redshift of z = 0.00068 (H0 = 67.8 km/sec/Mpc, Omega_m = 0.308, Omega_v = 0.692) (from NED)
- and to a distance of approximately 12 million light years from Earth



Seen by: VERITAS
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