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Table 1.

Details about the telescopes and instruments used.

Telescope C1 C2 F G H I
2.0 m RC 2.0 m RC 1.3 m RC 1.0 m RC 60 cm RC 50 cm Cassegrain
CCD model VersArray:1300B iKon-L 2k × 4k UKATC SI 1100 Cryo Andor iKon-L Apogee Alta
UV, AR, BI 936 BEX2-DD U42
Chip size 1340 × 1300 px 2048 × 2048 px 2048 × 4096 px 4096 × 4096 px 2048 × 2048 px 2048 × 2048 px
Pixel size 20 × 20 μm 13.5 × 13.5 μm 13 × 13 μm 15 × 15 μm 13.5 × 13.5 μm 13 × 13 μm
Scale px−1 px−1 px−1 px−1 px−1 px−1
Field 17′ × 17′ 10′ × 20′
Gain 1.0 e ADU−1 1.0/1.1 e ADU−1 0.74 e ADU−1 0.57 e ADU−1 1.1 e ADU−1 1.28 e ADU−1
Read out noise 2.0 e rms 6.7/6.9 e rms 4.2 e rms 4.19 e rms 6.9 e rms 8.3 e rms
Binning used 1 × 1 1 × 1 1 × 1 2 × 2 1 × 1 2 × 2
Typical seeing 15 to 25 15 to 25 1″ to 3″ 1″ to 3″ 15 to 3″ 2″ to 3″

Notes. Configuration C1: 2.0 m RC telescope at Rozhen NAO, Bulgaria. Configuration C2: 2.0 m RC telescope + FoReRo-2 focal reducer at Rozhen NAO. The gain and read-out noise are reported for the blue and red channels, respectively. Telescope F: 1.3 m JC Bhattacharya telescope (JCBT), Kavalur, India. Telescope G: 1.0 m RC telescope, Turkey. Telescope H: 60 cm RC robotic telescope, Turkey. Telescope I: 50 cm Cassegrain telescope, Krakow, Poland.

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