Table A.5.
X-ray properties of Turin-SyCAT sources (first five rows; full table available at the CDS)
ID | SyCAT | WISE | ROSAT | Counts | ϑrw | 3PBC | 3PBC counterpart | 3PBC class | FHX | ϑ3w | BAT105 | BAT105 | ϑbw | IBIS name | IBIS class | ϑiw |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
name | name | name | (arcsec) | name | name | class | erg s−1 cm−2 | (arcsec) | name | class | (arcsec) | name | class | (arcsec) | ||
(1) | (2) | (3) | (4) | (5, 6) | (7) | (8) | (9) | (10) | (11, 12) | (13) | (14) | (15) | (16) | (17) | (18) | (19) |
1 | SY1 J0002+0322 | J000226.41+032107.0 | J000226.6+032105 | 0.226±0.0267 | 3.22 | J0002.5+0322 | NGC 7811 | Sy1 | 1.39E-11±1.80E-12 | 0.69 | J0002.5+0323 | Sy1.5 | 48.13 | |||
2 | SY2 J0004+7020 | J0004.0+7018 | 2MASX | AG? | 1.10±0.13e−11 | 0.26 | J0005.0+7021 | Sy1.9 | 0.18 | J00040+7020 | Sy2 | 0.4 | ||||
J00040192+7019185 | ||||||||||||||||
3 | SY1 J0006+2013 | J000619.53+201210.6 | J0006.3+2012 | Mrk 335 | Sy1 | 1.76E-11±1.40E-12 | 0.12 | J0006.2+2012 | Sy1.2 | 148.93 | ||||||
4 | SY2 J0025+6821 | J002532.37+682144.9 | 3PBC J0025.5+6822 | IGR J00256+6821 | Sy2 | 1.79E-11±1.40E-12 | 0.515 | J0025.8+6818 | Sy2 | 158.70 | IGR J00256+6821 | AGN,Sy2 | 0.49 | |||
5 | SY1 J0025-1859 | J002542.34-190010.1 | J002542.6-190009 | 0.299±0.032 | 3.65 | 3PBC J0025.6-1859 | 2MASX J00254238-1900106 | Sy1 | 1.05E-11±1.60E-12 | 0.30 |
Column description: (1) Catalog ID; (2) SyCAT name; (3) WISE name; (4) ROSAT name; (5, 6) X-ray counts from the ROSAT catalog and its 1σ uncertainty in parentheses; (7) angular separation between ROSAT and WISE positions in arcseconds; (8) 3PBC name; (9) counterpart listed in the 3PBC; (10) 3PBC classification; (11, 12) FHX and its 1σ uncertainty in parentheses (in units of erg s−1 cm−2); (13) angular separation between 3PBC and WISE positions in arcseconds; (14) BAT105 name; (15) BAT105 classification; (16) angular separation between BAT105 and WISE positions in arcseconds; (17) INTEGRAL name from IBIS4CAT; (18) INTEGRAL classification from IBIS4CAT; (19) angular separation between IBIS4CAT and WISE positions in arcseconds.
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