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Observation Date (UT) Observation Lat

Canonical Name:NGC 253
TeVCat Name:TeV J0047-253
Other Names:
Source Type:Starburst
R.A.:00 47 32.54 (hh mm ss)
Dec.:-25 17 25.4 (dd mm ss)
Gal Long: 97.29 (deg)
Gal Lat: -87.97 (deg)
Distance: 2500 kpc
Flux:0.0021 (Crab Units)
Energy Threshold:220 GeV
Spectral Index:
Extended:No
Discovery Date:2009-07
Discovered By: H.E.S.S.
TeVCat SubCat:Default Catalog

Source Notes:

This source's detection was announced at the 2009 ICRC in Lodz.
The detection was published in Science Express and subsequently in Science.

Source position and its uncertainty:
The source position in TeVCat was updated on 180614 to that from H.E.S.S. Collaboration (2018).
From H.E.S.S. Collaboration (2018):
- R.A. (J2000): 00 47 32.54 +/- 11.2s
- Dec. (J2000): -25 17 25.4 +/- 10.3''
From Abramowski et al. (2012):
- R.A. (J2000): 00 47 34.3 +/- 1.4s (=21'')
- Dec. (J2000): -25 17 22.6 +/- 0.3' (=18'')
From Acero et al. (2009):
- R.A. (J2000): 00 47 33.6 +/- 30s
- Dec. (J2000): -25 18 08 +/- 27''

Spectral Information:
From H.E.S.S. Collaboration (2018):
- "The VHE gamma-ray energy spectrum is best fit by a power-law
distribution with a flux normalisation of
(1.34 +/- 0.14 stat +/- 0.27 sys) x 10-13 cm-2 s-1 TeV-1 at 1 TeV
about 40 % above, but compatible with the value obtained in
Abramowski et al. (2012). The spectral index:
2.39 +/- 0.14 stat +/- 0.25 sys
is slightly softer than but consistent with the previous measurement
within systematic errors."

From Abramowski et al. (2012):
- Spectral index: 2.14 +/- 0.18 +/- 0.30

Flux:
From Abramowski et al. (2012):
- (0.21 +/- 0.05)% of the Crab Nebula flux above 190 GeV

Source Extent:
From H.E.S.S. Collaboration (2018):
- "With the PSF being understood better, a possible extension of the
gamma-ray source is constrained to <= 1.4' at the 3 sigma level
compared to the previous limit of <= 2.4'."


Seen by: H.E.S.S.
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