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Table 3:

Sample of 15 sources extracted from the list of 398 extragalactic radio sources detected during EC025A and EC025B experiments (211 out of 218 detected during EC025A, and 187 out of 229 detected during EC025B). The complete list is available at the CDS.

IERS name
Name from catalog Catalog V z Type $\alpha$ $\delta$ Flux $\alpha_{SX}$ Exp.
            h min s $^{\circ}$ $^\prime$ $^{\prime\prime}$ S X    
0946+091 09480+08421I FIRST 17.49 1.971 QUA 9 48 53.6070 8 55 14.410 16 3 -1.28 B
0949+241 GB6J095207+235248 CLASS 16.78 0.970 QUA 9 52 6.3897 23 52 45.250 30 18 -0.39 A
0948+658 095232+653800 NVSS 18.00   BL 9 52 32.2300 65 38 0.300 34 30 -0.08 B
0950-084 J095301-084034 CRATES 17.20   BL 9 53 2.7200 -8 40 18.400 62 48 -0.20 A
0950+326 GB6J095328+322552 CLASS 17.74 1.574 QUA 9 53 27.9563 32 25 51.530 71 133 0.48 A
0952+338 GB6J095537+333522 CLASS 17.44 2.500 QUA 9 55 37.9383 33 35 3.937 66 46 -0.28 A
0956+216 095930+212319 NVSS 17.40 0.365 BL 9 59 30.0400 21 23 19.200 18 15 -0.18 B
0957+136 GB6J100035+132440 CLASS 17.15 1.352 QUA 10 0 33.8516 13 24 10.896 50 21 -0.67 A
0957+561* GB6J100121+555357 CLASS 16.98 1.413 QUA 10 1 20.6911 55 53 55.611 24 11 -0.60 A
0959+684 GB6J100308+681313 CLASS 15.92 0.773 QUA 10 3 6.7676 68 13 16.811 57 31 -0.47 A
1002+483 10060+47544F FIRST 17.65 2.370 QUA 10 5 15.9610 48 5 33.210 50 18 -0.80 B
1001+621 GB6J100516+615443 CLASS 17.81 2.740 QUA 10 5 17.6044 61 54 17.281 36 13 -0.79 A
1007+716 GB6J101132+712434 CLASS 17.60 1.192 QUA 10 11 32.6159 71 24 41.616 466 42 -1.86 A
1009+334 GB6J101211+330936 CLASS 17.99 2.260 QUA 10 12 11.4526 33 9 26.414 70 47 -0.31 A
1009+067 GB6J101213+063051 CLASS 16.80 0.727 BL 10 12 13.3477 6 30 57.175 83 62 -0.23 A

Notes. The apparent optical magnitude from Véron-Cetty & Véron (2006) is denoted V, the redshift z, and the type of the object is ``BL'' for BL Lac objects and ``QUA'' for quasars. The right ascension $\alpha$ and declination $\delta$ are extracted from the catalog specified in the third column. The mean correlated flux densities are given in mJy, the derived S/X spectral index is denoted $\alpha_{SX}$, and the name of the experiment is given in the last column (``A'' for EC025A and ``B'' for EC025B).
IERS name of gravitational lenses is marked with an asterisk. These sources will be omitted from subsequent steps of the project.
The catalogs from which the coordinates were extracted are: CLASS (Myers et al. 2003; position accuracy $\sim$35 mas), CRATES (Healey et al. 2007; position accuracy ranging from $\sim$50 mas to $1^{\prime\prime}$), FIRST (Becker et al. 1995; position accuracy ranging from $\sim$50 mas to $1^{\prime\prime}$), NVSS (Condon et al. 1998; position accuracy $\sim$ $1^{\prime\prime}$), and AHA (Andrei, A. H. 2007, private communication of improved positions for QSOs as extracted from the input catalog for Gaia; position accuracy better than $1^{\prime\prime}$). For the last catalog, the name of the source written in the table is extracted from Véron-Cetty & Véron (2006).


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