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Table 7

Multi-wavelength data for the VLBI-detected sources.

ID Opt. ID R c 3.6 μm z spec z phot Morph. Fit Model FX(0.5–2 keV) Flag log LX(0.5–2 keV) HR1
mag mag 10-16   erg/s/cm2 erg/s
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)

L0009 –99
L0025 –99
L0034 –99
L0049 –99
L0051 –99
L0055 –99
L0066 –99
L0077 –99
L0119 166 492 25.20 1.70 2 1 110 –99
L0130 42 435 20.43 0.4239 0.34 2 1 131 –99
L0140 55 191 24.44 4.20 1 1 126 –99
L0149 28 661 20.09 3.2687 0.29 2 1 131 –99
L0171 34 378 24.67 0.97 1 1 123 –99
L0194 0
L0199 –1
L0227 89 171 19.14 18.69 1.439 0.27 0 3 129 –99
L0231 117 241 23.24 0.87 2 1 108 –99
L0251 –1
L0256 45 485 20.90 0.5396 0.60 3 1 101 –99
L0352 55 842 21.04 0.593 0.91 2 2 129 –99
L0386 –1
L0397 69 623 21.68 18.95 0.69 2 4 120 –99
L0411 187 543 25.87 21.54 1.82 1 4 123 0 < 42.95
L0412 124 257 24.86 21.39 2.12 1 4 122 0 < 43.14
L0420 46 934 24.83 1.13 1 1 131 –99
L0423 114 988 24.74 19.72 1.34 2 4 107 0 < 42.57
L0449 47 368 20.19 0.55 2 1 109 –99
L0477 53 986 18.94 17.83 0.3177 0.40 2 4 107 –99
L0484 48 731 21.69 0.59 3 1 114 –99
L0506 –1
L0535 206 628 21.69 18.89 0.58 2 4 2 6.8 42.11 –0.69
L0536 206 644 24.19 20.47 1.73 1 2 114 25.5 44.02 –0.5
L0578 206 598 22.85 18.99 0.99 1.00 1 4 5 48.9 43.61 0.03
L0593 97 588 24.77 19.55 1.04 3 4 113 0 < 42.25
L0607 49 780 22.51 19.27 1.16 3 4 119 –99
L0648 88 715 26.02 2.07 1 4 130 0 < 43.12
L0703 206 690 24.24 20.18 0.462 1.53 1 4 114 42.6 42.65 –0.62
L0708 –1
L0724 167 757 25.51 20.13 1.51 3 4 113 0 < 42.72
L0846 59 617 21.51 19.14 0.58 2 4 108 –99
L0860 40 969 19.82 0.3826 0.52 2 1 102 –99
L0876 110 535 20.29 19.12 0.54 2 4 102 0 < 41.47
L0890 206 578 21.25 18.33 0.71 0.58 2 4 2 30.0 42.99 –0.53
L0911 206 453 22.93 19.29 1.013 1.11 2 2 1 4.3 42.58 –0.63
L0927 –99
L0933 126 512 21.25 0.493 0.53 2 4 113 0 < 41.37
L0953 170 521 16.40 0.0731 0.29 2 4 101 –99
L0973 206 457 22.11 19.74 0.762 0.68 0 4 5 122.7 43.69 –0.59
L0977 206 416 23.88 18.59 1.45 1.30 1 4 18 18.9 43.67 –0.35
L0997 45 980 22.89 0.96 1 4 102 –99
L1034 66 996 24.07 19.72 1.33 1 4 115 0 < 42.56
L1052 85 797 20.03 18.85 0.41 2 4 107 0 < 41.17
L1092 92 439 22.18 19.09 0.62 2 4 108 0 < 41.63
L1115 206 406 20.84 18.41 0.711 0.73 2 4 124 77.1 43.40 –0.65
L1148 –1
L1165 117 627 21.37 20.75 0.33 2 4 123 0 < 40.91
L1200 84 577 25.61 21.32 2.55 1 4 121 0 < 43.38
L1225 78 963 23.09 19.37 0.91 2 1 108 0 < 42.09
L1235 151 191 21.53 0.73 2 4 102 –99
L1286 175 609 25.29 21.27 1.91 1 4 128 0 < 43.02
L1302 206 717 26.04 21.54 1.49 1 4 124 31.5 43.92 –0.28
L1306 114 090 25.13 2.23 1 4 128 0 < 43.21
L1364 0
L1374 128 598 19.11 17.55 0.33 4 3 123 –99
L1404 –99

Notes.Column 1: source ID used in this paper; Col. 2: ID from Fotopoulou et al. (2012), −99: outside imaged area, –1: uncatalogued/blended counterpart, 0: no visible counterpart; Col. 3: Rc AB magnitude; Col. 4: 3.6   μm AB magnitude from the SWIRE survey; Col. 5: spectroscopic redshift, where available; Col. 6: best photometric redshift; Col. 7: morphology flag, 0: point-like, 1 – unresolved, 2 – early type or bulge-dominated, 3 – unclassified, 4 – spiral; Col. 8: quality of the fit, 1: too few bands, 2: blended photometry, 3: doubful because of a lack of X-ray information, 4: a good fit; Col. 9: model type used in the best fit for photometric redshift; Col. 10: X-ray flux in the 0.5–2 keV band; Col. 11: X-ray luminosity in the 0.5–2 keV band, −99: outside imaged area, 0: imaged, but undetected; Col. 12: a “<” indicates that the X-ray luminosity is an upper limit; Col. 13: hardness ratio calculated between the 0.5–2 keV and 2.0–4.5 keV bands.

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