Table 4.
Log of observatories and instrumentations used to obtain our ground-based photometry.
| Observatory | Telescope (†) | Detector | Filters | Reference | Table |
|---|---|---|---|---|---|
| SLO,G2 (a) | 60 | CCD: FLI ML3041 | U, B, V, RC, IC | 1 | A.1 |
| SLO,G1 (b) | 18 | CCD: SBIG ST-10 MXE | B, V, RC, IC | 1 | A.1 |
| ANS Collab. (c) | 30, 40 | CCD: SBIG ST-8, MG4-9000 | B, V, RC, IC | 2,3 | A.2 |
| AOKS (d) | 35.6 | CCD: G2-1600 | B, V, RC, IC | 4 | A.1 |
| SAI (e) | 125 | InSb photometer | J, H, K, L | 5 | 2 |
| SAI | 40,16,50 | photographic plate | mpg | 6,7,8 | A.3 |
| SO (f) | 30,40 | photographic plate | mpg, mpv | 6,7,8 | A.3 |
Notes.
Sonneberg Observatory archive: http://www.4pisysteme.de/observatory/observatory_4_2_en.html.
(†)Diameter of the primary mirror in cm.
References. 1 – Sekeráš et al. (2019), 2 – Munari (2012), 3 – Munari & Moretti (2012), 4 – Kudzej et al. (2019), 5 – Shenavrin et al. (2011), 6 – Bacher et al. (2005), 7 – Sokolovsky et al. (2016), 8 – http://scan.sai.msu.ru/vast/.
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