Table 3.
Estimates of warm corona radius Rcor from TITAN-NOAR normalization NSE (Eq. (6)), in terms of gravitational radii, for sources of known distances (D).
Source | ObsID | NSE = S/D2 | Rcor | Source | ObsID | NSE = S/D2 | Rcor |
---|---|---|---|---|---|---|---|
D | [×10−7] | [Rg] | D | [×10−7] | [Rg] | ||
112600401 | 2.20±0.17 | 121.76 ± 4.58 | 112170101 | 1.77 ±0.18 | 11.14 ±0.57 | ||
148000201 | 0.97±0.45 | 80.62 ± 18.58 | NGC 7469 | 112170301 | 3.99 ±0.31 | 16.75 ± 0.65 | |
1H0419-577 | 148000301 | 1.08±0.23 | 85.26 ± 9.24 | 57.30 Mpc | 207090101 | 2.20 ±0.16 | 12.45 ± 0.46 |
148000401 | 24.80±15.0 | 408.55, ± 126.03 | 207090201 | 2.10 ±0.08 | 12.15 ± 0.24 | ||
459.83 Mpc | 148000501 | 4.46±1.48 | 173.26 ± 28.75 | PG0804+761 | 605110101 | 1.47 ±0.23 | 95.72 ± 7.60 |
148000601 | 0.82±0.32 | 74.28 ± 14.34 | 442.45 Mpc | 605110201 | 1.26 ±0.15 | 88.49 ± 5.27 | |
604720301 | 1.92±0.09 | 113.77 ± 2.79 | PG0844+349 | 103660201 | 1.25 ± 0.10 | 77.75 ± 2.99 | |
604720401 | 3.79±0.34 | 159.71 ± 7.10 | 390.00 Mpc | 554710101 | 0.18 ± 0.02 | 29.29 ± 1.98 | |
ESO198-G24 | 067190101 | 0.22 ± 0.08 | 16.67 ± 3.18 | 201940101 | 0.88 ±0.02 | 130.86 ± 1.73 | |
200.89 Mpc | 112910101 | 0.26 ± 0.38 | 18.12 ± 13.37 | PG1116+215 | 201940201 | 0.76 ±0.19 | 121.17 ± 15.20 |
305370101 | 0.50 ± 0.05 | 25.31 ± 1.35 | 554380101 | 1.30 ± 0.25 | 159.22 ± 15.48 | ||
HE1029-1401 | 110950101 | 1.06± 0.35 | 70.79 ± 11.71 | 781.54 Mpc | 554380201 | 0.66 ±0.11 | 112.85 ± 9.35 |
384.82 Mpc | 203770101 | 2.51± 0.06 | 108.68 ± 1.28 | 554380301 | 0.52 ±0.10 | 100.25 ± 9.54 | |
IRASF12397+3333 | 202180201 | 1.32±0.12 | 31.75 ± 1.47 | PG1351+640 | 205390301 | 0.26 ±0.03 | 35.30 ± 2.41 |
155.0 Mpc | 202180301 | 1.76±0.49 | 36.68 ± 5.07 | 391.23 Mpc | 556230201 | 0.03 ±0.01 | 11.62 ± 1.58 |
MRK 279 | 302480401 | 1.64 ±0.08 | 30.96 ±0.77 | ||||
135.49 Mpc | 302480501 | 1.45 ±0.06 | 29.06 ± 0.58 | PG1402+261 | 400200101 | 0.64 ±0.05 | 103.89 ± 3.76 |
302480601 | 1.53 ±0.11 | 29.90 ± 1.04 | 728.43 Mpc | 400200201 | 0.15 ±0.06 | 49.99 ± 10.02 | |
MRK 335 | 510010701 | 2.72 ±1.39 | 25.28 ± 6.46 | 5010101 | 1.87 ± 0.09 | 85.87 ± 2.00 | |
85.90 Mpc | 600540501 | 68.5 ±8.01 | 126.84 ± 7.42 | PG1440+356 | 5010201 | 2.01 ±0.17 | 88.96 ± 3.69 |
600540601 | 1.36 ±0.55 | 17.88 ± 3.59 | 351.87 Mpc | 5010301 | 0.98 ± 0.05 | 62.04 ± 1.70 | |
107660201 | 1.84 ±0.17 | 85.10 ± 3.94 | |||||
0130720101 | 6.92±0.52 | 26.69 ± 0.46 | |||||
0601390201 | 5.06±0.42 | 42.15 ± 1.76 | Q0056-363 | 102040701 | 0.50 ±0.10 | 91.38 ± 9.25 | |
0601390301 | 6.36±0.56 | 47.26 ± 2.10 | 722.24 Mpc | 205680101 | 0.47 ±0.03 | 87.98 ± 3.22 | |
0601390401 | 6.63±0.51 | 48.24 ± 1.85 | 401930101 | 0.48 ± 0.04 | 88.99 ± 4.06 | ||
Mrk 509 | 0601390501 | 5.01±0.16 | 60.41 ± 3.51 | 109070101 | 4.03 ±0.22 | 69.57 ± 1.90 | |
0601390601 | 14.02±0.85 | 70.09 ± 2.12 | 506440101 | 3.08 ±0.09 | 60.8 ± 0.91 | ||
105 Mpc | 0601390701 | 8.31±1.45 | 54.03 ± 4.73 | RE1034+396 | 561580201 | 6.17 ±0.33 | 86.05 ± 2.31 |
0601390801 | 6.09±0.51 | 46.25 ± 1.95 | 655310101 | 6.21 ±0.33 | 86.36 ±2.06 | ||
0601390901 | 4.93±0.21 | 41.63 ± 0.91 | 194.16 Mpc | 655310201 | 5.15 ±0.18 | 78.62 ±1.40 | |
06013901001 | 9.38±0.72 | 57.38 ± 2.21 | 675440101 | 10.5 ±1.99 | 112.25 ± 10.64 | ||
06013901101 | 5.92±0.42 | 45.60 ± 1.95 | 675440201 | 5.59 ±0.26 | 81.87 ± 1.93 | ||
675440301 | 5.91 ±0.16 | 84.20 ± 1.16 | |||||
MRK 590 | 109130301 | 0.14 ±0.10 | 5.79 ± 2.13 | ||||
87.10 Mpc | 201020201 | 0.40 ±0.10 | 9.79 ± 1.26 | ||||
103862101 | 1.14 ±0.76 | 17.12 ±5.69 | |||||
059830101 | 2.55 ±0.14 | 17.38 ± 0.41 | UGC393 | 400070201 | 2.17 ±0.36 | 23.64 ± 1.96 | |
109970101 | 1.31 ±0.49 | 12.48 ± 2.31 | 400070301 | 0.74 ±0.13 | 13.82 ± 1.25 | ||
NGC 4593 | 740920201 | 1.10 ±0.50 | 11.43 ± 2.31 | 90.00 Mpc | 400070401 | 1.52±0.24 | 19.77 ± 1.55 |
740920301 | 1.05 ±0.43 | 11.15 ± 2.27 | 502091001 | 1.00 ±0.15 | 16.06 ±1.22 | ||
61.00 Mpc | 740920401 | 0.38 ±0.24 | 6.67 ± 2.13 | ||||
740920501 | 1.36 ±0.19 | 12.69 ± 0.87 | |||||
740920601 | 1.20 ±0.17 | 11.94 ± 0.86 |
Notes. Two sources- HB890405-123 and LBQS1228+1116 are not included here due to the unavailability of black hole mass measurements. Details on distance measurement (D) are given in Sect. 5.4.
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