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Table 1:

List of observed Seyfert galaxies - basic data.
Object Alternative RA Dec Hubble Redshift z Velocity cz $D_{\rm L}$ Ang.scale
  name [h m s] [d m s] type   [km s-1] [Mpc] [pc/ $\hbox{$^{\prime\prime}$ }$]
Mrk 34 MCG +10-15-104 10 34 08.6 +60 01 52 Spiral 0.0505 $15~140\pm90$ 218 956
Mrk 622 UGC 04229 08 07 41.0 +39 00 15 S0 0.0232 $6964\pm11$ 99.6 461
Mrk 1066 UGC 02456 02 59 58.6 +36 49 14 (R)SB(s)0+ 0.0120 $3605\pm22$ 47.3 224
NGC 262 Mrk 348 00 48 47.1 +31 57 25 SA(s)0/a 0.0150 $4507\pm4$ 58.2 274
NGC 449 Mrk 1 01 16 07.2 +33 05 22 (R')S? 0.0159 $4780\pm2$ 62.3 293
NGC 2273 Mrk 620 06 50 08.6 +60 50 45 SB(r)a: 0.0061 $1840\pm4$ 25.8 124
NGC 2992 MCG -02-25-014 09 45 42.0 -14 19 35 Sa pec 0.0077 $2311\pm4$ 36.6 175
NGC 3081 IC 2529 09 59 29.5 -22 49 35 (R1)SAB(r)0/a 0.0080 $2391\pm3$ 37.7 180
NGC 4388 UGC 07520 12 25 46.7 +12 39 44 SA(s)b: sp 0.0084 $2524\pm1$ 16.7(*) 81(*)
NGC 5728 MCG -03-37-005 14 42 23.9 -17 15 11 (R1)SAB(r)a 0.0094 $2804\pm20$ 41.9 199
NGC 5929 UGC 09851 15 26 06.1 +41 40 14 Sab: pec 0.0083 $2492\pm8$ 35.7 170
Adopted from the NASA/IPAC Extragalactic Database (NED). The cosmological scales assume $H_0 = 73~{\rm km~s}^{-1}~{\rm Mpc}^{-1}$, $\Omega_{\rm M} = 0.27$, $\Omega_\Lambda = 0.73$. $D_{\rm L}$: luminosity distance; Ang.scale: angular scale. (*) Values from Yasuda et al. (1997), with NGC 4388 considered inside the Virgo cluster.

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