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Observation Date (UT) Observation Lat

Canonical Name:CTA 1
TeVCat Name:TeV J0006+729
Other Names:SNR G119.5+10.2,
VER J0006+729
Source Type:PWN
R.A.:00 06 26 (hh mm ss)
Dec.:+72 59 01.0 (dd mm ss)
Gal Long: 119.60 (deg)
Gal Lat: 10.40 (deg)
Distance: 1.4 kpc
Flux:0.04 (Crab Units)
Energy Threshold:1000 GeV
Spectral Index:2.2
Extended:Yes
Size (X):0.30 (deg)
Size (Y):0.24 (deg)
Discovery Date:2011-10
Discovered By: VERITAS
TeVCat SubCat:Default Catalog

Source Notes:

Source Position:
From Aliu et al. (2012):
- R.A. (J2000): 00h 06m 26s +/- 0.09 deg
- Dec. (J2000): +72d 59' 01.0" +/- 0.04deg
- Systematic uncertainty: 50"

Spectral Information:
From Aliu et al. (2012):
- Spectral index: 2.2 +/- 0.2(stat) +/- 0.3(syst)

Source Morphology:
From Aliu et al. (2012):
- semi-major axis: 0.30deg
- semi-minor axis: 0.24deg

Source Classification:
From Martin et al. (2016):
- "We estimate the molecular mass around CTA 1 using data from Planck
and the Harvard CO survey. We observe that the molecular mass in the
vicinity of the complex is not enough to explain the TeV emission
observed by VERITAS, even under favorable assumptions for the
cosmic-ray acceleration properties of the supernova remnant. This
supports the idea that the TeV emission comes from the PWN. "
From Acero et al. (2013):
- This LAT emission from this source below 10 GeV is likely from a
pulsar


Seen by: VERITAS
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