Table A.8.
Results of the optical/UV SED fitting (Sect. 6).
BAT ID | Swift ID | kTmax | E(B − V)HG | Fuvo | Flag |
---|---|---|---|---|---|
3 | SWIFTJ0002.5+0323 |
![]() |
![]() |
![]() |
- |
6 | SWIFTJ0006.2+2012 |
![]() |
< 0.014 |
![]() |
- |
16 | SWIFTJ0029.2+1319 |
![]() |
![]() |
![]() |
- |
19 | SWIFTJ0034.5-7904 | 2.7 | < 0.001 |
![]() |
t |
34 | SWIFTJ0051.6+2928 |
![]() |
![]() |
![]() |
- |
36 | SWIFTJ0051.9+1724 |
![]() |
< 0.012 |
![]() |
- |
39 | SWIFTJ0054.9+2524 |
![]() |
![]() |
![]() |
- |
43 | SWIFTJ0059.4+3150 |
![]() |
< 0.007 |
![]() |
- |
45 | SWIFTJ0101.5-0308 |
![]() |
![]() |
![]() |
- |
51 | SWIFTJ0105.7-1414 |
![]() |
0.000 |
![]() |
e |
Notes. We have listed the best-fit values of the disk temperature (kTmax in eV), the extinction due to the host galaxy E(B − V)HG, and the total, intrinsic optical/UV flux (from 10−7–0.1 keV) with errors. The last column shows, in the form of flags, if the disk temperature was fixed to its median value of 2.7 eV (t) and if the host galaxy extinction was fixed to zero (e) during the fitting. Flux units: 10−11 erg cm−2 s−1. The table in its entirety is available at the CDS.
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