Extended Data Table 1: Best-fitting parameters for ultrashort microlensing event candidates

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

Table 1
  1. Is is the source brightness and fs = Fs/(Fs + Fb) is the blending parameter. We also show 1σ confidence intervals for tE. The inclusion of the finite source effect does not improve χ2 much (typically Δχ2 = 0.0–3.3). Equatorial coordinates are given for the epoch J2000. RA, right ascension; Decl., declination.