Fig. 11

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Proper motion measurements for tile e1084. Top: histogram in Ks band for stellar sources in both the first and latest Ks band epochs observed for e1084. About 60% of the sources have counterparts in Gaia DR3. This number dropped to ≲40% for Ks > 16.0 mag. Bottom: Naive PM measurements based on the differences of the RA/Dec between the latest and the first epochs. The grid pattern is an artefact of the binning algorithm used for plotting, and is not a real feature. Only stellar sources with Ks < 16.0 have been used and the timespan is ~4.2 yr (1530 days). The mean values are PMRA cos Dec = −6.40 ± 5.46 mas yr−1 and PMDec = −1.53 ± 5.02 mas yr−1.

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