GMOS r’ band light curve of source compared to a reference star

International Gemini Observatory/NOIRLab/NSF/AURA

GMOS r’ band light curve of source compared to a reference star

Top, GMOS r’ band light curve of source compared to a reference star in images (shown in Figure 2). Three observations were carried out in five days, on 2008 May 11, 12 and 15, in the Gemini queue mode. Average seeing conditions for the three nights were 0.63, 0.58 and 0.70 arcsecond.

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