Table 1.
Observational and physical properties of the 25 galaxies.
| Galaxy | ID | Vrad | LB | Telescope/survey | Integration time | Depth μlim | FOV | |
|---|---|---|---|---|---|---|---|---|
| [km s−1] | [log L⊙] | [hours] | [mag arcsec−2 ] | degrees2 | ||||
| CIG 11 | UGC 139 | 3906 | 10.03 | VST | 4.8 | 29.7 | 4.936 | |
| CIG 33 | NGC 237 | 4090 | 9.95 | VST | 4.8 | 29.7 | 4.987 | |
| CIG 59 | UGC 1167 | 4193 | 9.56 | VST | 4.8 | 29.7 | 6.040 | |
| CIG 94 | UGC 1706 | 4694 | 9.74 | INT | 4.8 | 29.8 | 0.451 | |
| CIG 96 | NGC 864 | 1562 | 9.57 | VST | 5.9 | 29.7 | 6.041 | |
| CIG 100 | UGC 1863 | 6546 | 9.86 | HSC-SSP | – | 29.5 | 0.155 | |
| CIG 154 | UGC 3171 | 4530 | 10.06 | VST | 4.8 | 29.5 | 6.006 | |
| CIG 279 | NGC 2644 | 2196 | 9.03 | VST | 4.8 | 29.5 | 6.046 | |
| CIG 329 | NGC 2862 | 4473 | 9.27 | INT | 3.5 | 29.8 | 0.318 | |
| CIG 335 | NGC 2870 | 3568 | 10.17 | INT | 6.2 | 30.0 | 0.340 | |
| CIG 340 | IC 2487 | 4710 | 9.61 | INT | 5.7 | 30.3 | 0.418 | |
| CIG 512 | UGC 6903 | 2234 | 8.65 | HSC-SSP | – | 29.6 | 0.155 | |
| CIG 568 | UGC 8170 | 11094 | 10.02 | VST | 6.8 | 30.4 | 0.598 | |
| CIG 613 | UGC 9048 | 11121 | 10.72 | INT | 4.1 | 30.0 | 0.307 | |
| CIG 616 | UGC 9088 | 6668 | 9.65 | INT | 3.8 | 30.0 | 0.308 | |
| CIG 626 | NGC 5584 | 1934 | 9.43 | HSC-SSP | – | 29.8 | 0.155 | |
| CIG 744 | UGC 10437 | 3088 | 9.16 | HSC-SSP | – | 29.6 | 0.155 | |
| CIG 772 | IC 1231 | 5643 | 10.34 | INT | 4.7 | 30.1 | 0.309 | |
| CIG 800 | NGC 6347 | 6636 | 10.08 | INT | 4.2 | 29.9 | 0.307 | |
| CIG 838 | IC 1269 | 6558 | 10.74 | INT | 3.6 | 29.6 | 0.315 | |
| CIG 947 | NGC 7217 | 952 | 10.52 | JRT | 10.3 | 29.0 | 0.142 | |
| CIG 971 | UGC 12082 | 802 | 8.48 | JRT | 3.0 | 28.5 | 0.118 | |
| CIG 1002 | NGC 7451 | 6638 | 9.96 | VST | 10.0 | 29.9 | 7.297 | |
| CIG 1004 | NGC 7479 | 2443 | 9.70 | JRT | 3.7 | 28.5 | 0.127 | |
| CIG 1047 | UGC 12857 | 2465 | 9.45 | VST | 6.2 | 29.6 | 6.456 |
Notes. The first two columns show the CIG name and the main ID of each galaxy. The third and fourth columns show the radial velocity and the absolute luminosity in the B band of the galaxy, obtained from the last revision of the AMIGA parameters in Jones et al. (2018). The fifth column shows the telescope used to acquire the images (see Sect. 2.1). The sixth and seventh columns show the total integration time in hours and the surface brightness limits [3σ, 10″ × 10″] of the image in mag arcsec−2, respectively, computed as explained in Román et al. (2020). The eighth column shows the FOV of the whole image in degrees2.
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