Positions of the 20 brightest stars (in I band) from the KMTC01 pyDIA reduction that overlap the Keck OSIRIS image (solid rectangle). The star positions are in the original reference-frame pixel coordinates. The pixels are approximately ﹩{0.4}^{{\prime} ^{\prime} }﹩. For ease of comparison to the Keck images, the stars are color coded according to K _pseudo ≡ I − (V − I) by K _pseudo < (13, 13.5, 14, 14.5, 15, 15.5) → (black, red, green, cyan, blue, magenta). The source position (X, Y)_source=(153.074, 150.317) is shown by a cross.