Canonical Name: | MAGIC J0223+403 |
TeVCat Name: | TeV J0223+430 |
Other Names: | |
Source Type: | UNID |
R.A.: | 02 23 12 (hh mm ss) |
Dec.: | +43 00 42 (dd mm ss) |
Gal Long: | 140.25 (deg) |
Gal Lat: | -16.75 (deg) |
Distance: | |
Flux: | 0.022 (Crab Units) |
Energy Threshold: | 150 GeV |
Spectral Index: | 3.1 |
Extended: | No |
Discovery Date: | 2009-02 |
Discovered By: | MAGIC |
TeVCat SubCat: | Default Catalog |
Source Notes:
Source position and its uncertainty:
From
Aliu et al. (2009):
- RA (J2000): 02 23 12
- Dec (J2000): +43 00 42
- positional uncertainty 0.048deg (private communication MAGIC Collaboration)
Source Association:
From
Aliu et al. (2009):
- both 3C66A and 3C66B were considered as candidates
for the origin of the gamma-ray emission. The excess measured
is closer to 3C66B than to 3C66A:
"The origin of the emission from 3C66A can be statistically
excluded with a probability of 95.6%. Adding linearly the
systematic uncertainty of the pointing of the data set (2')
i.e., shifting the excess position by 2′ toward the catalog
position of 3C66A, the exclusion probability is 85.4%."
Seen by: MAGIC
-
Proper Motion of the Sub-Parsec Scale Jet in the Radio Galaxy 3C 66B
Sudou, H. and Iguchi, S., ArXiv e-prints p (2011) [LINK]
-
A Very Close Binary Black Hole in a Giant Elliptical Galaxy 3C 66B and its Black Hole Merger
Iguchi, S. et al., ApJ 724 pL166-L170 (2010) [LINK]
-
3C 66B as a TeV radio galaxy
Tavecchio, F. and Ghisellini, G., MNRAS 394 pL131-L135 (2009) [LINK]
-
Discovery of a Very High Energy Gamma-Ray Signal from the 3C 66A/B Region
MAGIC Collaboration, ApJ 692, L29 (2009) [LINK]
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