Back to Main Page
Observation Date (UT) Observation Lat

Canonical Name:Crab Pulsar
TeVCat Name:TeV J0534+220p
Other Names:
Source Type:PSR
R.A.:05 34 31.9 (hh mm ss)
Dec.:+22 00 52.2 (dd mm ss)
Gal Long: 184.56 (deg)
Gal Lat: -5.78 (deg)
Distance: 2 kpc
Flux:0.01 (Crab Units)
Energy Threshold:150 GeV
Spectral Index:3.8
Extended:No
Discovery Date:2008-11
Discovered By: MAGIC
TeVCat SubCat:Default Catalog

Source Notes:

The Crab Pulsar was listed under the Crab TeVCat entry until 141027

Source position:
The source position is taken from SIMBAD:
- R.A. (J2000): 05 34 31.9
- Dec. (J2000): +22 00 52.2

Spectral Information:
From de Ona Wilhelmi (2015) via Lemoine-Goumard (2015):
- "... the MAGIC collaboration is now seeing significant pulsed
emission (from the Crab) above 1 TeV as can be seen Figure in 5 in
de Ona Wilhelmi (2015)."
From VERITAS Collaboration (2015):
- "In this work, we show an updated energy spectrum that extends
beyond 400 GeV and up to 1 TeV. The results agree well with the
originally published VERITAS measurement. However, the accumulated
statistics were not sufficient to reconstruct a spectral point at 1 TeV."
From VERITAS Collaboration (2011):
- spectral index: 3.8 +/- 0.5(stat) +/- 0.2(syst)

Flux:
From VERITAS Collaboration (2011):
- flux: approximately 1% that of the nebula

Emission components:
- Saito et al. reported on the discovery of VHE Bridge emission
from the Crab Pulsar at the 2014 Fermi Symposium
- in addition to the pulsed component, steady gamma-ray emission is
also detected from the nebula, e.g., Weekes et al. (1989),
Konopelko et al. (1996)


Seen by: MAGIC, VERITAS
Want a reference added? Send a bibtex entry to the TeVCat Team
Try TevCat 2.0 Beta!