Table 1.
Galaxy properties.
| Galaxy | RA | Dec | D | log M* | reff | σ | NH | Ngal |
|---|---|---|---|---|---|---|---|---|
| [Mpc] | [M⊙] | [kpc] | [km s−1] | [1020 cm−2] | (< 0.2 Mpc) | |||
| MRK 1216† | 08 28 47.11 | −06 56 24.44 | 94 ± 2 |
 |
3.0 ± 0.1 | 308 ± 7 | 4.58 | 0 |
| NGC 472† | 01 20 28.70 | +32 42 32.68 | 74 ± 1 |
 |
2.4 ± 0.1 | 217 ± 8 | 6.52 | 1 |
| PGC 32873† | 10 56 16.06 | +42 19 59.30 | 112 ± 2 |
 |
2.3 ± 0.1 | 304 ± 8 | 1.21 | 1 |
| PGC 70520† | 23 07 20.19 | +36 21 45.14 | 72 ± 1 |
 |
1.6 ± 0.1 | 248 ± 8 | 10.30 | 0 |
| J091842.83+031557.1★ | 9 18 42.83 | +03 15 57.10 | 239.5 |
 |
1.2 | 221 ± 8 | 3.16 | 0 |
| J092318.89+025538.3★ | 09 23 18.88 | +02 55 38.30 | 395.5 |
 |
1.8 | 227 ± 12 | 3.92 | 0 |
| J093634.60+034428.4★ | 09 36 34.59 | +03 44 28.40 | 202.6 |
 |
2.1 | 256 ± 5 | 3.13 | 0 |
Notes. † The D distances, M* stellar masses, reff effective radii, and σ central stellar velocity dispersions are adopted from Yıldırım et al. (2017); M* is obtained from dynamical models, reff is measured along the major axis of the best-fitting ellipse containing half of the light, and σ is given within the best-fitting circular aperture. ★ D, M*, and σ are adopted from SDSS spectroscopic catalogs. NH is the weighted H I + H II galactic hydrogen column density along the given sightline (Willingale et al. 2013). Ngal shows the number of neighboring galaxies within 0.2 Mpc distance determined from a cone search.
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