Table 6
Optical/X-ray photometry.
| Epoch | log f2500 | log f2 keV | log ℓ2500 | log ℓ2 keV | α ox | Δαox |
|
|
|
||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | ||
|
|
|||||||||||
| Dec. 2004 | –25.46 | –30.46 | 29.49 | 24.49 | –1.92 | –0.52 | 25.28 | –1.68 | –0.28 | ||
| Jun. 2008 | –25.39 | –30.17 | 29.56 | 24.77 | –1.84 | –0.43 | 25.31 | –1.63 | –0.22 | ||
| Dec. 2008 | –25.40 | –29.80 | 29.55 | 25.15 | –1.69 | –0.28 | 25.57 | –1.53 | –0.12 | ||
| 2009 Long Look | –25.30 | –30.46 | 29.64 | 24.49 | –1.98 | –0.56 | 25.26 | –1.62 | –0.20 | ||
Notes. Column (1): epoch of observation. Column (2): 2500 Å rest frame flux density corrected for Galactic extinction. Column (3): 2 keV rest frame flux density corrected for Galactic absorption. Column (4): 2500 Å rest frame luminosity density corrected for Galactic extinction. Column (5): 2 keV rest frame luminosity density corrected for Galactic absorption. Column (6): observed optical-to-X-ray spectral index. Column (7): difference between the observed αox and the one expected on the basis of the ℓ2500 luminosity. Column (8): 2 keV rest frame luminosity density corrected for Galactic and intrinsic absorption. Column (9): optical-to-X-ray spectral index corrected for the intrinsic X-ray absorption. Column (10): difference between the corrected and the one expected on the basis of the ℓ2500 luminosity. Flux densities are in [erg s-1 cm-2 Hz-1], luminosity densities are in [erg s-1 Hz-1].
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