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Table 1

General properties of the sample galaxies.

Name RA Dec Dist.1 N Gal m B Morph. Optical X-ray Jet Ref.2
(J2000) (J2000) (Mpc) (1020 cm-2) type class. class.
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)

NGC 315 00 57 48.88 +00 21 08.8 59.60 5.88 12.20 E L1.9 AGN Y (1)
NGC 1052 02 41 04.80 +08 15 20.8 19.48 3.07 11.44 E L1.9 AGN Y (2)
NGC 1961 05 42 04.6 +69 22 42 56.20 8.28 11.01 SAB(rs)c L2 AGN Y (3)
NGC 2681 08 53 32.73 +51 18 49.3 15.25 2.45 11.15 S0-a(s) L1.9 AGN* N (1)
NGC 2787 09 19 18.56 +69 12 12.0 10.24 4.32 11.60 S0-a(sr) L1.9 AGN N (1)
NGC 2841 09 22 02.63 +50 58 35.5 16.62 1.45 10.06 Sb(r) L2 AGN N (1)
NGC 32263 10 23 27.01 +19 53 54.7 29.84 2.14 12.34 E L1.9 AGN N (1)
NGC 3608 11 16 58.96 +18 08 54.9 24.27 1.49 11.57 E L2/S2: Non-AGN* N (1)
NGC 3718 11 32 34.8 +53 04 05 17.00 1.08 11.19 SB(s)a L1.9 AGN Y (1)
NGC 4261 12 19 23.22 +05 49 30.8 31.32 1.55 11.35 E L2 AGN Y (4)
NGC 4278 12 20 06.83 +29 16 50.7 15.83 1.77 11.04 E L1.9 AGN Y (5)
NGC 4374 12 25 03.74 +12 53 13.1 17.18 2.60 10.11 E L2 AGN* Y (6)
NGC 4494 12 31 24.03 +25 46 29.9 13.84 1.52 10.68 E L2:: AGN N (1)
NGC 4636 12 42 49.87 +02 41 16.0 16.24 1.81 10.43 E L1.9 Non-AGN* Y (7)
NGC 4736 12 50 53.06 +41 07 13.6 5.02 1.44 8.71 Sab(r) L2 AGN N (1)
NGC 5195 13 29 59.6 +47 15 58 7.91 1.56 10.38 IA L2: AGN N (8)
NGC 5813 15 01 11.26 +01 42 07.1 30.15 4.21 11.48 E L2: Non-AGN* Y (9)
NGC 5982 15 38 39.8 +59 21 21 41.22 1.82 12.05 E L2:: AGN N (10)

Notes. (Col. 1) Name, (Col. 2) right ascension, (Col. 3) declination, (Col. 4) distance, (Col. 5) galactic absorption, (Col. 6) aparent magnitude in the Johnson filter B from Ho et al. (1997), (Col. 7) galaxy morphological type from González-Martín et al. (2009a), (Col. 8) optical classification from Ho et al. (1997), (Col. 9) X-ray classification from González-Martín et al. (2009b), where the * represent Compton-thick candidates from González-Martín et al. (2009a), (Col. 10) evidence of radio jet, and (Col. 11) references for radio data.

(1)

All distances are taken from the NED and correspond to the average redshift-independent distance estimates.

(3)

We rejected the long-term variability analysis (i.e., comparison of spectra at different epochs) of NGC 3226 because XMM-Newton data may be contaminated by emission from NGC 3227 (see HG13), while we have mantained the UV and short-term analyses (i.e., light curves).

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