Canonical Name: | TXS 0210+515 |
TeVCat Name: | TeV J0214+517 |
Other Names: | RX J0214.2+5144 RGB J0214+517
|
Source Type: | HBL |
R.A.: | 02 14 17.9 (hh mm ss) |
Dec.: | +51 44 52 (dd mm ss) |
Gal Long: | 135.74 (deg) |
Gal Lat: | -9.05 (deg) |
Distance: | z=0.049 |
Flux: | (Crab Units) |
Energy Threshold: | 300 GeV |
Spectral Index: | 1.9 |
Extended: | No |
Discovery Date: | 2019-01 |
Discovered By: | MAGIC |
TeVCat SubCat: | Default Catalog |
Source Notes:
This source was moved to the Default Catalogue on 191118.
This detection was announced at the
eXtreme 19 Conference by
Fallah Ramazani et al. (2019).
Source Position:
The source position reported in TeVCat is taken from
NED:
R.A. (J2000): 02h 14m 17.9344s
Dec. (J2000): +51d 44' 51.947''
Spectral Properties:
From
MAGIC Collaboration (2019):
The data were fit with a simple power-law spectrum of the form:
- dN/dE = F0 x (E/E0)^-A
- F0: 0.10 +/- 0.03 x10e-12 cm-2 s-1
- A: 2.0 +/- 0.3
- E0: 1574 GeV
The integral flux above 200 GeV is 1.6 +/- 0.5 x10e-12 cm-2 s-1
From
Fallah Ramazani et al. (2019):
- spectral index at VHE (observed): 1.90 +/- 0.29
- flux (>300 GeV): 5.1 +/- 2.0 x10e-12 ph cm-2 s-1
Distance:
From
Marcha et al. (1996):
- "Optical spectroscopy of the 200-mJy sample was obtained at the
Multiple Mirror Telescope on Mt Hopkins, on the nights of 1992 May 8-9
and November 2-3."
- a redshift of z=0.049 +/- 0.002 was measured
Seen by: MAGIC
-
Detectability of large correlation length inflationary magnetic field with Cherenkov telescopes
Korochkin, Alexander et al., arXiv e-prints parXiv:2111.10311 (2021) [LINK]
-
New hard-TeV extreme blazars detected with the MAGIC telescopes
MAGIC Collaboration et al., arXiv e-prints parXiv:1911.06680 (2019) [LINK]
-
Long-term optical monitoring of TeV emitting blazars. I. Data analysis
Nilsson, K. et al., A&A 620 pA185 (2018) [LINK]
-
All the MAGIC of extreme blazars
Fallah Ramanzani, V. et al. for the MAGIC Collaboration, Proc. eXtreme 19 [LINK]
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the TeVCat Team