Table 3
Results for the 14 sources for which it was possible to carry out a spectral analysis.
| Name | NH | cts | S/N | F(0.5–2 keV) | L(0.5–2 keV) | F [O III] | L [O III] | F [O III] /FsX | F [O III] /FsX | ||
| 1020 | [10-14 erg cm2 s-1] | 1041 | 10-14 | 1041 | ext | nuc | |||||
| [cm-2] | pha(po) | pha(mek) | pha(xstar) | [erg s-1] | [erg cm2 s-1] | [erg s-1] | |||||
|
|
|||||||||||
| 3C 33 | 3.23 | 44 | 6.5 | 0.904 | 0.829 | 1.78 | 1.48 | 5.92 | 4.91 | 3.3 | 2.3 |
| 3C 63 | 2.47 | 31 | 5.4 | 1.77 | 1.72 | 1.89 | 15.8 | ||||
| 3C 98 | 10.2 | 25 | 4.7 | 0.592 | 0.587 | 0.805 | 0.171 | ||||
| 3C 171* | 5.65 | 134 | 11.3 | 1.15 | 1.52 | 1.34 | 30.4 | 3.09 | 51.8 | 2.3 | 3.1 |
| 3C 180 | 13.6 | 6 | 2.3 | <0.664 | <0.736 | <0.846 | <11.8 | 1.80 | 698 | >2.1 | |
| 3C 234 | 1.76 | 13 | 3.6 | 0.670 | 0.651 | 0.715 | 6.75 | 4.13 | 39.1 | 5.8 | 2.5 |
| 3C 305* | 1.31 | 89 | 9.3 | 4.38 | 3.98 | 4.87 | 1.92 | 11.1 | 4.36 | 2.3 | 2.3 |
| 3C 379.1 | 5.43 | 3 | 1.7 | <0.266 | <0.280 | <0.317 | <6.24 | 0.332 | 6.54 | >1.04 | |
| 3C 403* | 12.2 | 51 | 7.0 | 0.494 | 0.467 | 0.641 | 0.520 | 4.79 | 3.89 | 7.5 | 2.0 |
| 3C 433* | 7.77 | 83 | 8.7 | 1.01 | 0.971 | 1.27 | 3.25 | ||||
| 3C 445* | 4.49 | 92 | 9.2 | 0.884 | 0.816 | 1.03 | 0.756 | 3.60 | 2.64 | 3.5 | 3.8 |
| 3C 452 | 9.64 | 12 | 2.3 | <0.06 | <0.0594 | <0.0736 | <0.117 | 0.467 | 0.738 | >6.3 | 1.5 |
| 3C 456 | 3.70 | 11 | 3.2 | 0.597 | 0.606 | 0.670 | 14.4 | ||||
| 3C 459 | 5.24 | 13 | 3.6 | 0.739 | 0.754e | 0.858 | 11.9 | ||||
Notes. We mark with a star symbol the 5 sources with a sufficiently high number of counts for which we perform in addition a spectral fit. We converted the observed number counts in a flux value adopting three different models: a power-law, mekal, or Xstar, absorbed by the Galactic NH column density. We report the unabsorbed soft X-ray fluxes for all 3 models and the luminosity for the Xstar model in the soft X-ray band (0.5–2 keV). We also give the [O III] flux and luminosity in the same regions used for the extraction of the X-ray spectra.
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