Index of /ogle/ogle3/OIII-CVS/gd/wd
=======================================================================
Large Variety of New Pulsating Stars
in the OGLE-III Galactic Disk Fields
P. Pietrukowicz, W.A. Dziembowski, P. Mroz, I. Soszynski, A. Udalski,
R. Poleski, M.K. Szymanski, M. Kubiak, G. Pietrzynski,
L. Wyrzykowski, K. Ulaczyk, S. Kozlowski, and J. Skowron
=======================================================================
pietruk@astrouw.edu.pl
This directory contains details on the pulsating white dwarf
identified in the OGLE-III Galactic disk fields.
The directory structure is as follows:
README - this file
ident.dat - identification of the star
wd.dat - parameters of the star
phot/I/ - I-band photometry
phot/V/ - V-band photometry
phot.tar.gz - gzipped phot/ directory
fcharts/ - finding chart
pap.pdf - PDF version of the paper Pietrukowicz et al. (2013),
Acta Astron., 63, 379, (arXiv:1311.5894) describing
this result
Format of the file ident.dat:
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Bytes Format Units Description
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1- 15 A15 --- Star's ID in the form OGLE-GD-WD-NNNN
18- 25 A8 --- OGLE-III field
27- 32 I6 --- OGLE-III database number
35- 36 I2 h Right ascension, equinox J2000.0 (hours)
38- 39 I2 m Right ascension, equinox J2000.0 (minutes)
41- 45 F5.2 s Right ascension, equinox J2000.0 (seconds)
47 A1 --- Declination, equinox J2000.0 (sign)
48- 49 I2 deg Declination, equinox J2000.0 (degrees)
51- 52 I2 arcmin Declination, equinox J2000.0 (arc minutes)
54- 57 F4.1 arcsec Declination, equinox J2000.0 (arc seconds)
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Format of the file wd.dat:
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Bytes Format Units Description
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1- 15 A15 --- Star's ID in the form OGLE-GD-WD-NNNN
18- 23 F6.3 mag Intensity mean V-band magnitude
25- 30 F6.3 mag Mean V-I color
32- 37 F6.3 mag Intensity mean I-band magnitude
40- 49 F10.8 days Period
51- 60 F10.8 days Uncertainty of the period
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Finding chart is a gzipped Postscript image. The name of the file is in
the form: OGLE-GD-WD-NNNN.ps.gz. The finding chart is 60"x60" subframes
of the I-band reference frames centered on the star. White cross marks the
star. North is up and East to the left.
Any presentation of the scientific analysis or usage of the data from the
OGLE catalog of variable stars should include appropriate references
to OGLE papers.