/ftp/cats/aliases/O/OGLE_BUL-SC_1_



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J/A+A/478/659     OGLE Be stars in Galactic Bulge               (Sabogal+, 2008)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table4.dat table5.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/478/659
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drwxr-xr-x 12 cats archive 215 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 482 Dec 19 2022 .message -r--r--r-- 1 cats archive 4668 Mar 5 2008 ReadMe -rw-r--r-- 1 cats archive 1030 Feb 23 2008 +footg5.gif -rw-r--r-- 1 cats archive 3380 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 518673 Jan 17 2008 table4.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 6272 Jan 22 2008 table5.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/478/659 OGLE Be stars in Galactic Bulge (Sabogal+, 2008) ================================================================================ A catalogue of Be stars in the direction of the Galactic Bulge. Sabogal B.E., Mennickent R.E., Pietrzynski G., Garca J.A., Gieren W., Kolaczkowski Z. <Astron. Astrophys. 478, 659 (2008)> =2008A&A...478..659S ================================================================================ ADC_Keywords: Stars, nearby ; Stars, Be ; Photometry Keywords: stars: emission-line, Be - Galaxy: bulge - catalogs Abstract: We report the first systematic search for Be star candidates in the direction of the Galactic Bulge. We present the full catalogue, give a brief description of the stellar variability seen, and show some light curve examples. We searched for stars matching specific criteria of magnitude, color and variability in the I band. Our search was conducted on the 48 OGLE II fields of the Galactic Bulge. Description: This search has resulted in 29053 Be star candidates listed in Table 4. 198 of these stars show periodic light variations and are listed in Table 5. Nearly 1500 stars in this final sample are almost certainly Be stars, providing an ideal sample for spectroscopic multi-object follow-up studies.