Table 3.
Observation log.
KIG | Exp. time | Date | Filter | FWHM | ZP |
---|---|---|---|---|---|
[s] | SDSS | [arcsec] | mag | ||
264 | 1800 | 9 | g | 1![]() |
22.83 ± 0.03 |
660 | 10 | r | 1![]() |
23.18 ± 0.05 | |
378 | 600 | 15 | g | 1![]() |
21.81 ± 0.02 |
540 | 15 | r | 1![]() |
21.94 ± 0.02 | |
412 | 1500 | 11 | g | 1![]() |
23.01 ± 0.03 |
2340 | 13 | r | 1![]() |
21.64 ± 0.04 | |
481 | 2100 | 13 | g | 2![]() |
22.62 ± 0.04 |
1080 | 13 | r | 2![]() |
22.44 ± 0.02 | |
490 | 1500 | 14 | g | 1![]() |
22.98 ± 0.05 |
1260 | 14 | r | 1![]() |
22.27 ± 0.01 | |
517 | 2700 | 9, 15 | g | 1![]() |
22.27 ± 0.12 |
2340 | 9, 15 | r | 1![]() |
21.64 ± 0.09 | |
578 | 2400 | 15 | g | 1![]() |
22.56 ± 0.11 |
1440 | 15 | r | 1![]() |
22.15 ± 0.01 | |
595 | 3000 | 11 | g | 1![]() |
22.65 ± 0.05 |
1800 | 11 | r | 1![]() |
22.46 ± 0.06 | |
599 | 1800 | 9 | g | 1![]() |
22.69 ± 0.06 |
1650 | 9 | r | 1![]() |
22.46 ± 0.06 | |
620 | 2400 | 13 | g | 2![]() |
22.44 ± 0.02 |
1440 | 13 | r | 1![]() |
22.09 ± 0.01 | |
636 | 2400 | 15 | g | 1![]() |
22.50 ± 0.04 |
1440 | 15 | r | 1![]() |
22.17 ± 0.02 | |
637 | 1800 | 14 | g | 1![]() |
22.78 ± 0.01 |
1440 | 14 | r | 1![]() |
22.11 ± 0.01 | |
644 | 1800 | 10 | g | 1![]() |
22.85 ± 0.03 |
1800 | 10 | r | 1![]() |
21.92 ± 0.02 | |
670 | 2100 | 13 | g | 1![]() |
22.62 ± 0.04 |
1800 | 13 | r | 1![]() |
22.45 ± 0.01 | |
685 | 2400 | 14 | g | 0![]() |
22.27 ± 0.03 |
1440 | 14 | r | 1![]() |
22.12 ± 0.04 | |
705 | 1510 | 9 | g | 1![]() |
22.50 ± 0.05 |
1200 | 9 | r | 1![]() |
21.87 ± 0.02 | |
722 | 1800 | 13 | g | 2![]() |
22.74 ± 0.07 |
900 | 14 | r | 0![]() |
22.65 ± 0.04 | |
732 | 3150 | 11 | g | 1![]() |
22.41 ± 0.02 |
1800 | 11 | r | 1![]() |
21.80 ± 0.01 | |
733 | 3000 | 15 | g | 1![]() |
22.24 ± 0.06 |
1800 | 15 | r | 1![]() |
21.68 ± 0.04 | |
841 | 1500 | 10 | g | 1.″0 | 23.04 ± 0.01 |
1800 | 10 | r | 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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