Open Access

Table A.1.

Literature low-z measurements collected by L19.

Source z log L2 − 10 Ecut Flag References
NGC 5506 0.006 42.68 1 (a),(b)
NGC 7213 0.006 42.07 < 140 1 (a),(b)
MCG-6-30-15 0.008 43.39 < 110 1 (a),(b)
MCG 5-23-16 0.009 43.2 1 (a),(b)
SWIFT J2127.4+5654 0.014 43.0 1 (a),(b)
NGC 5548 0.018 43.3 1 (a),(b)
Mrk 335 0.026 42.51 < 174 1 (a),(b)
1H0707-495 0.041 43.06 < 63 1 (a),(b)
Fairall 9 0.047 43.98 < 242 1 (a),(b)
Cyg A 0.056 44.24 < 110 1 (a),(b)
3C 382 0.058 44.37 1 (a),(b)
IGR J0033+6122 0.105 45.28 < 52 2 (c),(a),(b)
3C 111 0.049 44.81 2 (c),(a),(b)
IGR J07597-3842 0.04 43.89 2 (c),(a),(b)
NGC 3783 0.01 43.42 2 (c),(a),(b)
NGC 4151 0.003 42.96 2 (c),(a),(b)
IGR J16558-5203 0.054 44.12 2 (c),(a),(b)
1H2251-179 0.064 44.62 2 (c),(a),(b)
MCG-02-58-022 0.047 44.29 < 510 2 (c),(a),(b)
MCG+08-11-011 0.021 44.03 1 (d),(b)
Mrk 6 0.019 43.21 1 (d),(b)
IGR J12415-5750 0.024 43.24 1 (d),(b)
IC4329A 0.016 43.97 1 (d),(b)
GRS 1734-292 0.021 43.64 1 (d),(b)
3C 390.3 0.056 44.37 1 (d),(b)
NGC 6814 0.005 42.18 1 (d),(b)
4C 74.24 0.104 44.38 1 (d),(b)
S5 2116+81 0.086 44.42 < 93 1 (d),(b)
PG 1114+445 0.144 44.6 < 22 2 (e),(a),(b)
NGC 4051 0.002 40.68 < 381 2 (e),(a),(b)
PG 1202+281 0.165 44.39 < 64 2 (e),(a),(b)
NGC 4138 0.003 41.21 < 75 2 (e),(a),(b)
Mrk 766 0.013 42.38 2 (e),(a),(b)
NGC 4258 0.002 40.82 < 284 2 (e),(a),(b)
Mrk 50 0.023 43.19 < 334 2 (e),(a),(b)
NGC 4593 0.009 42.82 < 517 2 (e),(a),(b)
Mrk 1383 0.087 44.17 < 134 2 (e),(a),(b)
NGC 3998 0.0035 41.51 1 (f),(b)
NGC 4579 0.0056 41.9 1 (f),(b)
ESO 103-035 0.013 42.96 1 (g),(b)
IGR 2124 0.02 43.68 1 (g),(b)
B2202-209 0.532 45.22 1 (h),(b)
GRS 1734-292 0.021 43.72 1 (i),(b)

Notes. Col. (1): Source name; Col. (2): Redshift; Col. (3): Logarithm of the 2−10 keV luminosity (erg s−1); Col. (4): High-energy cutoff (keV); Col. (5): Telescope flag, 1=NuSTAR, 2=non-focusing; Col. (6): References.

References. (a) Fabian et al. (2015), (b) L19, (c) Malizia et al. (2014), (d) Molina et al. (2019), (e) Vasudevan et al. (2013), (f) Younes et al. (2019), (g) Buisson et al. (2018), (h) Kammoun et al. (2017), (i) Tortosa et al. (2017).

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