Fig. 3
Gunn z′-band light curve of S106IR over a time span of 5 days (top panel). We note the rather large short-term variations on some of the nights; the period of hours is much shorter than the main period of variability of 5 days. The measurements of a comparison star in the field of very similar brightness in z′, 2MASS J20273205+3723571, is shown for reference.
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