==========================================================================
J/AcA/52/129 DIA OGLE2 candidate variable stars catalog (Wozniak+, 2002)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
catalog.dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/AcA/52/129
==========================================================================
drwxr-xr-x 8 cats root 196 Apr 4 2023 [Up]
drwxr-xr-x 2 cats root 260 Jan 13 2023 [TAR file]
-rw-r--r-- 1 cats archive 464 Dec 19 2022 .message
-rw-r--r-- 1 cats archive 7262 Nov 28 2007 ReadMe
-rw-r--r-- 1 cats archive 1031 Sep 19 2007 +footg5.gif
-rw-r--r-- 1 cats archive 3377 Mar 5 2008 +footg8.gif
-r--r--r-- 1 cats archive 9057160 Nov 25 2003 catalog.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :J/AcA/52/129 DIA OGLE2 candidate variable stars catalog (Wozniak+, 2002)
================================================================================
Difference image analysis of the OGLE-II Bulge data.
III. Catalog of 200000 candidate variable stars.
Wozniak P.R., Udalski A., Szymanski M., Kubiak M., Pietrzynski G.,
Soszinski I., Zebrun K.
<Acta Astron., 52, 129 (2002)>
=2002AcA....52..129W
================================================================================
ADC_Keywords: Surveys ; Stars, variable ; Photometry
Keywords: Galaxy: center - catalogs - stars: variable: general
Abstract:
We present the first edition of a catalog of variable stars from
OGLE-II Galactic bulge data covering 3 years: 1997-1999. Typically
200-300 I band data points are available in 49 fields between -11 and
+11 degrees in galactic longitude, totaling roughly 11 square degrees
in sky coverage. Photometry was obtained using the Difference Image
Analysis (DIA) software and tied to the OGLE data base with the DoPhot
package. The present version of the catalog comprises 221801 light
curves. In this preliminary work the level of contamination by
spurious detections is still about 10%. Parts of the catalog have only
crude calibration, insufficient for distance determinations. The next,
fully calibrated, edition will include the data collected in year
2000. The data is accessible via ftp, at
ftp://bulge.princeton.edu/ogle/ogle2/bulge_dia_variables