================================================================================ Limits on planetary-mass primordial black holes from the OGLE high-cadence survey of the Magellanic Clouds P. Mróz, A. Udalski, M.K. Szymański, I. Soszyński, P. Pietrukowicz, S. Kozłowski, R. Poleski, J. Skowron, K. Ulaczyk, M. Gromadzki, K. Rybicki, P. Iwanek, M. Wrona, and M.J. Mróz ================================================================================ pmroz@astrouw.edu.pl The directory structure is as follows: ReadMe.txt - this file limits.txt - 95% upper limits on compact objects as constituents of dark matter phot/ - calibrated I-band photometry of individual events phot.tar.gz - gzipped phot/ directory eff/ - event detection efficiencies in individual fields eff.tar.gz - gzipped eff/ directory Format of the photometry files: -------------------------------------------------------------------------------- Bytes Format Units Description -------------------------------------------------------------------------------- 1- 13 F13.5 HJD Heliocentric Julian Date 15- 20 F6.3 mag I magnitude 22- 26 F5.3 mag Magnitude error -------------------------------------------------------------------------------- The I-band photometry is calibrated to the standard system. Format of the detection efficiency files: -------------------------------------------------------------------------------- Bytes Format Units Description -------------------------------------------------------------------------------- 1- 5 F13.5 - Minimal log(t_E) 7- 11 F6.3 - Maximal log(t_E) 13- 19 F7.5 - Detection efficiency for log(rho) = -3.0 21- 27 F7.5 - Detection efficiency for log(rho) = -2.0 29- 35 F7.5 - Detection efficiency for log(rho) = -1.0 37- 43 F7.5 - Detection efficiency for log(rho) = 0.0 45- 51 F7.5 - Detection efficiency for log(rho) = 0.2 53- 59 F7.5 - Detection efficiency for log(rho) = 0.4 61- 67 F7.5 - Detection efficiency for log(rho) = 0.6 69- 75 F7.5 - Detection efficiency for log(rho) = 0.8 77- 83 F7.5 - Detection efficiency for log(rho) = 1.0 --------------------------------------------------------------------------------