/ftp/cats/aliases/O/OGLE_23_



==========================================================================
J/AcA/53/27   VI photometry of MM1 and MM7 OGLE fields   (Pigulski+, 2003)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	tables.dat idata/* vdata/*
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/AcA/53/27
==========================================================================

drwxr-xr-x 5 cats root 101 Jan 29 2012 [Up] drwxr-xr-x 4 cats root 4096 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 479 Dec 19 2022 .message -rw-r--r-- 1 cats archive 7660 Nov 28 2007 ReadMe -rw-r--r-- 1 cats archive 1009 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2947 Mar 5 2008 +footg8.gif drwxr-xr-x 2 cats archive 77824 Jun 1 2006 idata -r--r--r-- 1 cats archive 251441 Jun 1 2006 tables.dat [txt] [txt.gz] [fits] [fits.gz] [html] drwxr-xr-x 2 cats archive 53248 Oct 20 2003 vdata
Beginning of ReadMe : J/AcA/53/27 VI photometry of MM1 and MM7 OGLE fields (Pigulski+, 2003) ================================================================================ Reanalysis of the OGLE-I observations with the image substraction method. I. Galactic Bar fields MM1-A, MM1-B, MM7-A, and MM7-B. Pigulski A., Kolaczkowski Z., Kopacki G. <Acta Astron., 53, 27 (2003)> =2003AcA....53...27P ================================================================================ ADC_Keywords: Stars, variable ; Photometry Keywords: stars: variables: general - delta Sct - stars: variables: RR Lyr - catalogs Abstract: As a result of the reanalysis of the OGLE-I observations by means of the image subtraction method, we present the first part of a catalog, consisting of data for variable stars in four Galactic fields observed by OGLE-I, viz. MM1-A, MM1-B, MM7-A, and MM7-B. In total, 2016 variable stars have been found. This increased the number of known variable stars in these fields more than twofold. We comment on the detectability of the variable stars in previous studies.