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Table 2

X-ray luminositiesb and Hα equivalent radii b.

Galaxy Cont. Da log(Lsoft) b log(Lhard)b Reqc σReq c
Filter (Mpc) (erg/s) (erg/s) (pc) (pc) (pc)
(1) (2) (3) (4) (5) (6) (7) (8)
IC 1459 FR680P15 29.24 40.6 40.5 245.52 0.17
NGC 315 F555W 68.11 42.0 41.8 398.66 0.02
F814W* 68.11 42.0 41.8 528.32 0.22
NGC 2639 F547M* 45.45 42.2 40.1 212.37 0.18
F814W 45.45 42.2 40.1 185.79 0.12
NGC 2681 F814W 17.22 38.6 41.0 209.75 0.07 48.27
NGC 2787 F702W 7.48 38.9 38.8 43.50 0.03 29.11
NGC 2841 F435W* 11.97 39.4 39.2 167.91 0.02
F814W 11.97 39.4 39.2 142.97 0.25 16.36d
NGC 3226 F814W 23.55 40.7 40.8 100.49 0.02 29.53d
NGC 3245 F702W 20.89 38.8 40.8 117.78 0.21 158.90
NGC 3379 F547M 10.57 38.0 39.9
NGC 3607 F814W 22.80 38.6 40.5 283.65 0.31 27.17d
NGC 3623 F547M 7.28 39.1 39.4 86.33 0.08 35.52
NGC 3627 F606W 10.28 39.2 41.2 0.08 109.45
NGC 3998 F791W 21.98 42.7 40.6 237.93 0.08 233.01
NGC 4036 f547M 24.55 39.0 40.9 199.21 0.06 116.29
NGC 4111 F702W 15.00 40.9 40.4 132.19 0.03 308.69
NGC 4278 F814W 16.07 39.6 41.0 67.00 0.08 118.34
NGC 4314 F606W 9.68 39.6 39.1 165.01 0.04
NGC 4374 F547M 18.37 39.5 41.3 401.75 0.03
F814W* 18.37 39.5 41.3 340.93 0.06 197.53
NGC 4438 F675W 16.83 40.1 40.8 255.57 0.02 153.53
NGC 4486 F547M 16.07 40.9 40.8 224.74 0.08 81.99
NGC 4552 F814W 15.35 39.5 39.3 216.95 0.15 217.22
NGC 4579 F791W 16.83 40.9 41.2 145.98 0.03 174.22
F547M 16.83 40.9 41.2 45.09 0.01
NGC 4594 F791W 9.77 39.6 39.9 93.35 0.09 107.34
NGC 4636 F814W 14.66 39.0 40.9 54.75
NGC 4676A F555W* 88.00 39.7 39.9 598.38 0.10
F814W 88.00 39.7 39.9 769.16 0.06
NGC 4676B F555W* 88.00 40.0 40.1 1001.37 0.06
F814W 88.00 40.0 40.1 843.25 0.05
NGC 4696 F702W 35.48 41.6 40.0 205.77 0.15
NGC 4736 F555W* 5.20 38.8 38.6 146.49 0.03
F814W 5.20 38.8 38.6 252.39 0.01 226.27
NGC 5005 F791W 21.28 40.7 41.6 248.99 0.03 393.56
NGC 5055 F547M 7.14 38.6 39.6 76.04 0.06 62.92
NGC 5846 F702W 24.89 40.2 40.8 156.31 0.08 88.26
NGC 5866 F814W 15.35 40.1 38.1

Notes.  dThe resulting radius is smaller than 2 pixels.

(a)

Distances from Table 1 in González-Martín et al. (2009a).

(b)

These luminosities have been corrected from intrinsic absorption; LX (2–10 keV) has also been corrected for Compton thickness. Lhard and Lsoft hold for the logarithm of the (2–10) keV (from Gonzalez-Martín et al. 2009b) and (0.3–2) keV (from Gonzalez-Martín et al. 2009a).

(c)

Req is the equivalent radius corresponding to a level 3 times higher that the dispersion of the background. corresponds to the isophotal level at 2.9 × 10-9 erg s-1 cm-2 arcsec-2.

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