Table 1
Galaxy sample characteristics.
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) |
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| Galaxy | α | δ | Morphological | ρ E | M B | (m − M) | AGN | age(Gyr) | [Z/H] | age(Gyr) | [Z/H] | N GCs | S N |
| (J2000) | (J2000) | type | [Mpc-3] | SB+06 | SB+06+ | Yamada06+ | Yamada06+ | ||||||
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| NGC 3377 | 10 47 42.4 | +13 59 08 | E5/E6 | 0.49 | −19.2 | 30.25 | yes* | 8.90 | –0.10 | – | – | 266 ± 66 | 2.4 ± 0.6 |
| NGC 4278 | 12 20 06.8 | +29 16 51 | E1/E2 | 1.25 | −21.2 | 31.03 | LINER | 11.64 | 0.079 | – | – | – | – |
| NGC 4365 | 12 24 28.2 | +07 19 03 | E3 | 2.93 | −20.96 | 31.55 | – | 12.60 | 0.139 | 14 | 0.16 | 3246 ± 598 | 3.86 ± 0.71 |
| NGC 4374 | 12 25 03.7 | +12 53 13 | E1 | 3.99 | −21.2 | 31.32 | Sy2 | 10.40 | 0.099 | – | – | 4301 ± 1201 | 5.20 ± 1.45 |
| NGC 4382 | 12 25 24.2 | +18 11 27 | S0+(s)pec | 2.04 | −21.3 | 31.33 | – | – | – | – | – | 1110 ± 181 | 1.29 ± 0.21 |
| NGC 4406 | 12 26 11.7 | +12 56 46 | S0/E3 | 1.41 | −20.60 | 31.17 | – | – | – | – | – | 2660 ± 129 | 2.57 ± 0.12 |
| NGC 4473 | 12 29 48.9 | +13 25 46 | E5 | 2.17 | −20.3 | 30.98 | – | – | – | 12.3 | 0.09 | 376 ± 97 | 1.98 ± 0.51 |
| NGC 4486 | 12 30 49.4 | +12 23 28 | E0/E1+pec | 4.17 | −21.79 | 31.03 | LINER | – | – | – | – | 14660 ± 891 | 12.59 ± 0.77 |
| NGC 4526 | 12 34 03.0 | +07 41 57 | SAB00(s) | 2.97 | −20.0 | 31.14 | - | – | – | – | – | 388 ± 117 | 1.09 ± 0.33 |
| NGC 4552 | 12 35 39.8 | +12 33 23 | E0/E1 | 2.97 | −20.6 | 30.93 | Sy2 | 8.89 | 0.121 | – | – | 984 ± 198 | 2.82 ± 0.57 |
| NGC 4570 | 12 36 53.6 | +07 14 46 | S0 sp | 2.66 | −19.5 | 30.91 | – | – | – | – | – | 139 ± 23 | 1.09 ± 0.18 |
| NGC 4621 | 12 42 02.3 | +11 38 49 | E5 | 2.60 | −20.6 | 31.31 | – | 11.40 | 0.115 | 13.3 | 0.23 | 803 ± 355 | 2.70 ± 1.19 |
| NGC 4649 | 12 43 40.0 | +11 33 10 | E2 | 3.49 | −21.47 | 31.13 | yes* | – | – | – | – | 4745 ± 1099 | 5.16 ± 1.20 |
| NGC 4660 | 12 44 32.1 | +11 11 25 | E | 3.37 | −19.2 | 30.54 | – | – | – | – | – | 205 ± 28 | 2.97 ± 0.41 |
Notes. (1) galaxy; (2), (3) equatorial coordinates; (4) morphological type (from Emsellem et al. 2007; Cappellari et al. 2007 and NED); (5) environmental density (ρE) (from Tully 1988); (6) integrated magnitude (HYPERLEDA); (7) distance modulus (Tonry et al. 2001 and NED); (8) AGN class (Véron-Cetty & Véron 2006) –
there is evidence for a black hole, although the classification of the AGN is missing (Kormendy et al. 1998; Gebhardt et al. 2003); (9–12) ages and metallicities estimates (from the spectral synthesis analysis of Sánchez-Blázquez et al. 2006 and Hβ vs. [MgFe] estimation of Yamada et al. 2006 respectively). The last two columns refer to the (13) estimated number of GCs (NGCs) and the (14) specific frequency (SN) from Peng et al. (2008) for the ACSVCS galaxies and Kundu & Whitmore (2001) for NGC 3377.
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