Table 1.
Sample.
Name | z | αEUV | log LUV | NH | Γ | log LX | Δ log LX | Telescope | log LR | log RUV |
---|---|---|---|---|---|---|---|---|---|---|
[erg s−1 | × 1020 cm−2 | [erg s−1 | [erg s−1 | [erg s−1 | ||||||
Hz−1] | Hz−1] | Hz−1] | Hz−1] | |||||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
1857+566 | 1.6 | 2.87 | 31.10 | ≤45.5 | 1.70![]() |
27.95 ± 1.12 | 0.81 | Swift | 34.91 | 3.81 |
1229−021 | 1.05 | 2.65 | 31.14 | 13.14![]() |
1.80![]() |
27.77 ± 0.02 | 0.59 | Chandra | 34.90 | 3.76 |
1022+194 | 0.83 | 2.55 | 30.59 | 2.55![]() |
27.13 ± 0.08 | 0.37 | ROSAT | 34.39 | 3.80 | |
1040+123 | 1.03 | 2.20 | 30.82 | ≤3.99 | 1.60![]() |
27.65 ± 0.03 | 0.73 | Chandra | 35.11 | 4.30 |
0743−673 | 1.51 | 2.20 | 31.79 | ≤59.0 | 1.69![]() |
28.87 ± 0.44 | 1.20 | Swift | 35.13 | 3.34 |
1317+520 | 1.06 | 2.18 | 31.32 | ≤1.22 | 1.70![]() |
27.54 ± 0.02 | 0.23 | Chandra | 34.42 | 3.10 |
1137+660 | 0.65 | 2.0 | 31.18 | 5.24![]() |
2.04![]() |
27.74 ± 0.11 | 0.54 | Chandra | 33.54 | 2.36 |
1354+195 | 0.72 | 1.95 | 31.18 | 4.83![]() |
1.88![]() |
27.85 ± 0.02 | 0.65 | Chandra | 34.58 | 3.40 |
1340+289 | 0.91 | 1.9 | 30.91 | ≤14.7 | 1.78![]() |
28.21 ± 0.46 | 1.21 | Swift | 33.92 | 3.01 |
2340−036 | 0.90 | 1.88 | 31.33 | ≤12.5 | 1.68![]() |
28.17 ± 0.39 | 0.85 | Swift | 33.91 | 2.58 |
1241+176 | 1.27 | 1.79 | 31.68 | ≤37.9 | 1.51![]() |
27.87 ± 0.53 | 0.28 | Swift | 34.32 | 2.64 |
1340+606 | 0.96 | 1.78 | 30.80 | ≤6.25 | 1.84![]() |
27.26 ± 0.03 | 0.34 | Chandra | 32.86 | 2.06 |
0024+224 | 1.12 | 1.77 | 31.55 | 27.83 | 0.35 | ROSAT | 34.60 | 3.06 | ||
0232−042 | 1.45 | 1.75 | 31.72 | ≤0.82 | 1.87![]() |
28.13 ± 0.03 | 0.52 | XMM-Newton | 34.68 | 2.97 |
0637−752 | 0.65 | 1.75 | 31.06 | ≤0.01 | 1.79![]() |
28.16 ± 0.06 | 1.04 | Chandra | 33.67 | 2.61 |
Notes. Column (1): Source name. Column (2): Redshift. Column (3): EUV spectral index. Column (4): Optical-UV spectral luminosity at 2500 Å. Column (5): Intrinsic hydrogen column density. Column (6): Power-law photon index. Column (7): X-ray spectral luminosity at 2 keV. Column (8): Excess of X-ray luminosity in RLAGNs with an EUV deficit to that in RQAGNs. Column (9): X-ray telescope. Column (10): Radio spectral luminosity at 5 GHz. Column (11): Radio loudness defined as RUV = LR/LUV.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.