Table A.2.
List of 4FGL associated sources observing information.
| 4FGL Source Name | Obs. Date | R mag | Exp. time | E(B-V) | SNR | Airmass | Seeing |
|---|---|---|---|---|---|---|---|
| yyyy-mm-dd | s | " | |||||
| J0128.2+4400 | 2023-01-26 | 20.2 | 5400 | 0.0651 | 2 | 1.37 | 1.2 |
| J0138.6+2923 | 2022-11-20 | 19.8 | 5400 | 0.0425 | 8 | 1.07 | 3 |
| J0304.5+3349 | 2022-11-19 | 18.9 | 3600 | 0.3007 | 10 | 1.01 | 1.3 |
| J0328.9+3514 | 2023-01-25 | 17.3 | 1800 | 0.2200 | 66 | 1.17 | 1.3 |
| J0429.8+2843 | 2022-11-19 | 20.8 | 7200 | 0.7408 | 8 | 1.13 | 1.6 |
| J0436.2−0038 | 2023-01-26 | 18.4 | 3600 | 0.0375 | 15 | 1.36 | 1.2 |
| J0539.7−0521c | 2023-01-25 | 18.7 | 3600 | 0.1784 | 30 | 1.26 | 1.22 |
| J0614.8+6136 | 2023-01-24 | 19.9 | 5400 | 0.1909 | 12 | 1.19 | 1.3 |
| J0704.7+4508 | 2023-01-26 | 18.2 | 2400 | 0.0881 | 25 | 1.28 | 1.2 |
| J0713.0+5738 | 2023-01-25 | 19.0 | 2400 | 0.0461 | 7 | 1.15 | 1.8 |
| J0733.0+4915 | 2023-01-24 | 19.6 | 3600 | 0.0747 | 10 | 1.44 | 1.6 |
| J0746.5−0710 | 2023-01-25 | 18.9 | 2400 | 0.0957 | 6 | 1.54 | 1.8 |
| J1054.5+2211 | 2023-01-24 | 17.2 | 3600 | 0.0138 | 93 | 1.08 | 1.6 |
| J1229.1+5521 | 2023-01-26 | 17.9 | 2400 | 0.0110 | 72 | 1.12 | 1.2 |
| J1517.0+2639 | 2023-06-22 | 19.5 | 3600 | 0.0297 | 4 | 1.01 | 0.7 |
| J1556.6+1417 | 2023-06-23 | 20.2 | 2400 | 0.0388 | 7 | 1.06 | 0.7 |
| J1754.7+3444 | 2023-06-23 | 19.6 | 1800 | 0.0321 | 10 | 1.02 | 0.7 |
| J1959.0+3844 | 2023-06-22, 23 | 20.2 | 3000 | 0.5232 | 5 | 1.09, 1.07 | 0.5, 0.6 |
| J2000.0+4214 | 2023-06-22 | 19.4 | 5400 | 0.3741 | 20 | 1.20 | 0.6 |
| J2120.7+4428 | 2023-06-22 | 21.7 | 3600 | 0.5558 | 3 | 1.13 | 0.8 |
| J2139.1+3724 | 2022-11-20 | 20.1 | 5400 | 0.0496 | 7 | 1.07 | 2 |
| J2317.0+3756 | 2022-11-19 | 19.9 | 3600 | 0.1340 | 4 | 1.11 | 1.6 |
Notes. Column information are as follows: (1) 4FGL source name; (2) date of observation (yyyy-mm-dd); (3) apparent R-band magnitude; (4) exposure time in seconds; (5) reddening E(B - V) in mag; (6) mean signal-to-noise ratio of the spectrum; (7) airmass and (8) mean seeing of the exposure in arcsec.
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