Extended Data Figure 1 : Galactic bulge luminosity function used for simulations.

From: No large population of unbound or wide-orbit Jupiter-mass planets

Extended Data Figure 1

a, Deep luminosity function (LF) for subfield BLG513.12, which was observed both by the OGLE-IV survey and by the Hubble Space Telescope (HST)38. Both luminosity functions overlap in the range 16 mag < I < 18 mag. This deep luminosity function was used as a template to generate artificial microlensing events in analysed fields, after shifting to match the centroid of the red clump giant stars in a given field. b, Comparison between the observed luminosity function for subfield BLG512.32 and the simulated luminosity function.