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Table 5

Radio properties for the 811 X-ray selected + 11 X-ray undetected SDSS type 1 AGN falling in the FIRST field.

SRCID Frf@2500 Å α ox Frf@4400 Å Frf@5 GHz @5 GHz up.lim Class. 4400 Å X
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)

X-ray detected AGN
192021 0.0258 ± 0.0007 −1.2251 ± 0.0292 0.0732 ± 0.0018 undet. 0.6451 ± 0.1754 undet. 24.983 ± 6.828 NC undet. 8.812 ± 2.405 undet. 0.0002 ± 0.0001
192103 0.0529 ± 0.0015 −1.1479 ± 0.0122 134.9836 ± 7.8384 2550.286 ± 164.680 RL 0.0148 ± 0.0013
192335 0.0309 ± 0.0009 −1.3782 ± 0.2267 0.0616 ± 0.0015 undet. 0.6504 ± 0.1721 undet. 21.022 ± 5.594 NC undet. 10.556 ± 2.806 undet. 0.0007 ± 0.0005
5632 0.0903 ± 0.0025 −1.5908 ± 0.0452 undet. 0.8725 ± 0.0546 undet. 9.665 ± 0.663 ndRI undet. 0.0008 ± 0.0002
[...]

X-ray undetected AGN
01Xund 0.0007 ± 0.0001 −0.9594 ± 0.1594 0.0281 ± 0.0007 0.8359 ± 0.1700 1236.742 ± 253.902 RL 29.700 ± 6.085  >0.0068
02Xund 0.0048 ± 0.0001 −1.1943 ± 0.1626 1.6489 ± 0.2886 345.411 ± 61.235 RL  >0.0104
03Xund 0.0712 ± 0.0020 −1.6124 ± 0.1583 0.4992 ± 0.1278 7.015 ± 1.807 dRI  >0.0020
04Xund 0.0416 ± 0.0012 −1.0559 ± 0.1490 2.8774 ± 0.3212 69.226 ± 7.971 RL  >0.0008
[...]

Notes. The complete table is published in its entirety at the CDS. A portion is shown here for guidance regarding its form and content. In the first part, we list the X-ray detected AGN; in the second part, we report basic data for the 11 sources in the parent sample undetected in the X-ray (see text).Column (1): unique source identification number in the 2XMMi catalogue; for the X-ray undetected sources, arbitrary ID number (as in Table 3). Column (2): monochromatic optical continuum flux at 2500 Å, recovered as described in Sects. 3 and 4 (in units of mJy). Column (3): X-ray-to-optical spectral index, αox ≡ log (F2 kev/F2500 Å)/log (ν2 kev/ν2500 Å). Column (4): monochromatic optical continuum flux at 4400 Å, recovered as described in Sects. 3 and 4.2 (in units of mJy); “–”: source without Hβ line in their spectra. Column (5): monochromatic radio flux at 5 GHz (rest frame; in units of mJy), recovered from the integrated flux density at 1.5 GHz assuming a power-law spectrum Fν ∝ να with index α = 0.5, as described in Sect. 4; undet.: source not detected by FIRST. Column (6): for sources not detected by FIRST, monochromatic radio flux limit at 5 GHz (rest frame; in units of mJy), calculated from the flux limit at 1.5 GHz of the FIRST survey, F1.5 GHz = 1 mJy, assuming the same spectral shape (Fν ∝ να with index α = 0.5). Column (7): radio-UV radioloudness parameter, defined as the ratio between the radio flux at 5 GHz and the optical flux at 2500 Å, both rest frame; undet.: source not detected by FIRST. Column (8): for sources not detected by FIRST, limit to the radio-UV radioloudness parameter, calculated from the limit to the radio flux at 5 GHz and the optical flux at 2500 Å, both rest frame. Column (9): radio classification: RL = radioloud; dRI = detected radiointermediate; ndRI = nondetected with 1 < ℛup.lim ≤ 10; RQ = radioquiet; NC = nonclassified. Column (10): radio-optical radioloudness parameter, defined as the ratio between the radio flux at 5 GHz and the optical flux at 4400 Å, both rest frame; undet.: source with Hβ line in its spectrum but not detected by FIRST; “–”: source (detected or not detected by FIRST) without Hβ line in its spectrum. Column (11): for sources not detected by FIRST, limit to the radio-optical radioloudness parameter, calculated from the limit to the radio flux at 5 GHz and the optical flux at 4400 Å, both rest frame; “–”: source without Hβ line in its spectrum. Column (12): radio-X-ray radioloudness parameter, defined as the ratio between the radio luminosity at 5 GHz and the X-ray luminosity in the 2−10 keV energy range; undet.: source not detected by FIRST. Column (13): limit to the radio-X-ray radioloudness parameter, calculated from the limit to the radio luminosity at 5 GHz and the X-ray luminosity in the 2−10 keV energy range. Note that for the X-ray detected AGN not detected by FIRST (first part), it is an upper limit, while for sources in the second part, radio-detected and X-ray undetected, it is a lower limit.

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