Index of /ogle/ogle4/galactic_disk_microlensing
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Microlensing optical depth and event rate
in the OGLE-IV Galactic plane fields
P. Mroz, A. Udalski, M. K. Szymanski, I. Soszynski, P. Pietrukowicz,
S. Kozlowski, J. Skowron, R. Poleski, K. Ulaczyk, M. Gromadzki,
K. Rybicki, P. Iwanek, and M. Wrona
========================================================================
pmroz@astro.caltech.edu
The directory structure is as follows:
README - this file
table_A1.txt - electronic version of Table A1 (basic information
about analyzed fields)
table_B1.txt - electronic version of Table B1 (best-fitting
parameters of the analyzed microlensing events)
table_B2.txt - electronic version of Table B2 (possible microlensing
events)
table_C1.txt - electronic version of Table C1 (surface density
of stars in the OGLE GVS fields)
data/ - calibrated I-band photometry of individual events
data.tar.gz - gzipped phot/ directory
data_c/ - calibrated I-band photometry of possible microlensing
events
data_c.tar.gz - gzipped phot_c/ directory
eff21/ - event detection efficiencies in individual fields
(for sources brighter than I=21)
eff21.tar.gz - gzipped eff21/ directory
eff20/ - event detection efficiencies in individual fields
(for sources brighter than I=20)
eff20.tar.gz - gzipped eff21/ directory
Format of the photometry files:
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Bytes Format Units Description
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1- 13 F13.5 HJD Heliocentric Julian Date
15- 20 F6.3 mag I magnitude
22- 26 F5.3 mag Magnitude error
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The I-band photometry is calibrated to the standard system.
The uncertainties were corrected using the Skowron et al. (2016)'s
method.
Format of the detection efficiency files:
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Bytes Format Units Description
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1- 5 F5.3 --- Minimal log(t_E)
7- 11 F5.3 --- Maximal log(t_E)
13- 20 F8.6 --- Detection efficiency
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