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Observation Date (UT) Observation Lat

Canonical Name:BL Lacertae
TeVCat Name:TeV J2202+422
Other Names:1ES 2200+420,
Source Type:IBL
R.A.:22 02 43.3 (hh mm ss)
Dec.:+42 16 40 (dd mm ss)
Gal Long: 92.59 (deg)
Gal Lat: -10.44 (deg)
Distance: z=0.069
Flux:0.03 (Crab Units)
Energy Threshold:200 GeV
Spectral Index:3.6
Extended:No
Discovery Date:2001-04
Discovered By: Crimea
TeVCat SubCat:Default Catalog

Source Notes:

Source position and its uncertainty:
From Arlen et al. (2013):
- R.A. (J2000): 22h 02m 37s
- Dec. (J2000): +42d 15' 25''
- statistical uncertainty of approx. 0.01 deg in each direction
From Albert et al. (2007):
- This is the position that is reported in TeVCat.
- R.A. (J2000): 22h 02m 43.3s
- Dec. (J2000): 42d 16' 40"
- "The small offset and the extension of the image are comparable
to the telescope PSF (0.1deg) and the telescope pointing error (1.5')"

Spectral Properties:
From Abeysekara et al. (2018):
- This is the spectrum during a flare that reached 180% of the Crab at its peak and averaged
0.95 Crab Units over its whole duration (above 200 GeV).
- A log-parabola model was found to fit the VERITAS data better than a power law.
- dN/dE = F0 (E/E0) ^(-alpha - b log10(E/E0))
- spectral index (alpha): 2.4 +/- 0.1
- b: 1.8 +/- 0.3
- F0: 2.22 +/- 0.07 x10e-5 m-2 s-1 TeV-1
- E0: 200 GeV
From Arlen et al. (2013):
- This is the spectrum during a flare that reached 125% of the Crab flux at these energies:
- dN/dE = F0 (E/E0)^-alpha
- spectral index (alpha): 3.6 +/- 0.4
- F0: 0.58 +/- 0.07 x10e-9 cm-2 s-1 TeV-1
- E0: 300 GeV
From Albert et al. (2007):
- This is the spectrum during a low-flux state corresponding to 3% of the Crab flux at these energies:
- dN/dE = F0 (E/E0)^-alpha
- spectral index (alpha): 3.6 +/- 0.5
- F0: 1.9 +/- 0.5 x10e-11 cm-2 s-1 TeV-1
- EO: 300 GeV

Classification:
Initially, this source was classified as an LBL in TeVCat. It has
been updated (121113) to an IBL based on its classification in
the Fermi 2nd AGN Catalog (Ackermann et al. 2012)


Seen by: Crimea, MAGIC, VERITAS
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