Open Access

Table 1.

Key properties of galaxies in the LLAGN sample.

ID RA Dec z Dist log LX Ref.
[Mpc] [erg/s]
NGC1052 40.269 −8.2558 0.00496 19.19 41.20 2
NGC2273 102.536 60.8457 0.00613 29.76 40.89 1
NGC2685 133.894 58.7343 0.00295 13.26 39.00 2
NGC2655 133.909 78.2234 0.00467 23.82 41.20 2
NGC2768 137.906 60.0373 0.00451 22.07 39.73 1
NGC2787 139.826 69.2033 0.00232 7.41 39.20 1
NGC2841 140.511 50.9766 0.00211 14.51 38.94 1
NGC3031 148.888 69.0652 −0.00013 3.59 39.15 1
NGC3079 150.491 55.6799 0.00368 19.01 40.05 1
NGC3147 154.223 73.4007 0.00934 42.72 41.92 1
NGC3185 154.410 21.6883 0.00410 24.98 39.40 2
NGC3190 154.526 21.8326 0.00437 23.98 40.07 1
NGC3193 154.603 21.8940 0.00460 33.01 38.76 1
NGC3414 162.817 27.9750 0.00490 25.92 40.48 1
NGC3516 166.697 72.5685 0.00883 38.01 42.49 1
NGC3718 173.145 53.0679 0.00331 16.98 41.22 1
NGC3898 177.313 56.0843 0.00385 21.97 38.93 1
NGC3945 178.306 60.6755 0.00427 21.57 39.80 1
NGC3953 178.454 52.3266 0.00350 18.93 38.04 1
NGC3982 179.117 55.1252 0.00371 21.55 40.78 5
NGC4013 179.630 43.9468 0.00277 19.71 38.80 1
... ... ... ... ... ... ...

Notes. The full version is available at the CDS. Distances are given in Mpc. X-ray luminosities are rest-frame and absorption-corrected, expressed in erg s−1. The table includes references for the X-ray luminosities: 1 for Williams et al. (2022), 2 for González-Martín et al. (2009), 3 for Osorio-Clavijo et al. (2023), 4 for Yun et al. (2022), 5 for Kammoun et al. (2020), 6 for Cappi et al. (2006), and 7 for Masini et al. (2022).

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