Table 3.
Observation log.
| KIG | Exp. time | Date | Filter | FWHM | ZP |
|---|---|---|---|---|---|
| [s] | SDSS | [arcsec] | mag | ||
| 264 | 1800 | 9 | g | 1 2 |
22.83 ± 0.03 |
| 660 | 10 | r | 1 1 |
23.18 ± 0.05 | |
| 378 | 600 | 15 | g | 1 3 |
21.81 ± 0.02 |
| 540 | 15 | r | 1 0 |
21.94 ± 0.02 | |
| 412 | 1500 | 11 | g | 1 3 |
23.01 ± 0.03 |
| 2340 | 13 | r | 1 0 |
21.64 ± 0.04 | |
| 481 | 2100 | 13 | g | 2 0 |
22.62 ± 0.04 |
| 1080 | 13 | r | 2 0 |
22.44 ± 0.02 | |
| 490 | 1500 | 14 | g | 1 3 |
22.98 ± 0.05 |
| 1260 | 14 | r | 1 0 |
22.27 ± 0.01 | |
| 517 | 2700 | 9, 15 | g | 1 2 |
22.27 ± 0.12 |
| 2340 | 9, 15 | r | 1 0 |
21.64 ± 0.09 | |
| 578 | 2400 | 15 | g | 1 2 |
22.56 ± 0.11 |
| 1440 | 15 | r | 1 2 |
22.15 ± 0.01 | |
| 595 | 3000 | 11 | g | 1 0 |
22.65 ± 0.05 |
| 1800 | 11 | r | 1 1 |
22.46 ± 0.06 | |
| 599 | 1800 | 9 | g | 1 6 |
22.69 ± 0.06 |
| 1650 | 9 | r | 1 1 |
22.46 ± 0.06 | |
| 620 | 2400 | 13 | g | 2 0 |
22.44 ± 0.02 |
| 1440 | 13 | r | 1 8 |
22.09 ± 0.01 | |
| 636 | 2400 | 15 | g | 1 1 |
22.50 ± 0.04 |
| 1440 | 15 | r | 1 4 |
22.17 ± 0.02 | |
| 637 | 1800 | 14 | g | 1 2 |
22.78 ± 0.01 |
| 1440 | 14 | r | 1 4 |
22.11 ± 0.01 | |
| 644 | 1800 | 10 | g | 1 3 |
22.85 ± 0.03 |
| 1800 | 10 | r | 1 3 |
21.92 ± 0.02 | |
| 670 | 2100 | 13 | g | 1 8 |
22.62 ± 0.04 |
| 1800 | 13 | r | 1 6 |
22.45 ± 0.01 | |
| 685 | 2400 | 14 | g | 0 9 |
22.27 ± 0.03 |
| 1440 | 14 | r | 1 2 |
22.12 ± 0.04 | |
| 705 | 1510 | 9 | g | 1 3 |
22.50 ± 0.05 |
| 1200 | 9 | r | 1 0 |
21.87 ± 0.02 | |
| 722 | 1800 | 13 | g | 2 6 |
22.74 ± 0.07 |
| 900 | 14 | r | 0 8 |
22.65 ± 0.04 | |
| 732 | 3150 | 11 | g | 1 5 |
22.41 ± 0.02 |
| 1800 | 11 | r | 1 3 |
21.80 ± 0.01 | |
| 733 | 3000 | 15 | g | 1 2 |
22.24 ± 0.06 |
| 1800 | 15 | r | 1 1 |
21.68 ± 0.04 | |
| 841 | 1500 | 10 | g | 1.″0 | 23.04 ± 0.01 |
| 1800 | 10 | r | 1 1 |
21.92 ± 0.03 |
Notes. We report the total exposure time in Col. 2. Galaxies were observed in April 2018: the observing date is given in Col. 3. The filter and average Gaussian FWHM of stars nearby the galaxy, measured on the co-added images using the IRAF task IMEXAMINE, are reported in Cols. 4 and 5 respectively (see Sect. 3). The adopted ZP are provided in Col. 6.
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