/ftp/cats/J_other/OEJV/./149



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J/other/OEJV/149        New Miras in Galactic Bulge           (Hummerich+ 2012)
The following files can be converted to FITS (extension .fit or fit.gz)
	table1.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/other/OEJV/149
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Beginning of ReadMe : J/other/OEJV/149 New Miras in Galactic Bulge (Hummerich+ 2012) ================================================================================ New Mira variables from the MACHO Galactic Bulge Fields Hummerich S., Bernhard K. <Open European J. Var. stars 149; BAV Mitteilungen Nr. 227 (2012)> =2012OEJV..149....1H ================================================================================ ADC_Keywords: Stars, variable Abstract: 500 new Mira variables in the direction of the Galactic Bulge are presented, which were found in the MACHO database. Description: 500 previously unrecorded Mira variables were found during an inspection of R-band lightcurves from the MACHO Galactic Bulge fields (http://macho.anu.edu.au/). This research continues the search for new Miras in the MACHO database (Bernhard, 2011PZP....11...12B). The MACHO 1.3m telescope is situated at Mount Stromlo in Australia and uses B and R filters in combination with eight 2048*2048 CCD cameras. Calculation of MACHO R magnitudes was done from the given instrumental R magnitudes using the formula given in Alcock et al. (1999PASP..111.1539A). Astrometric positions and near-infrared color indices were derived from the 2MASS catalog (Skrutskie et al. 2006, VII/233). Only objects with an amplitude >2mag (Rc) were taken into consideration. In addition, all lightcurves have been inspected visually; objects with significant changes in amplitude, mean magnitude and / or period suggesting semi-regularity have been rejected. Each object was checked against the Strasbourg CDS Vizier service and the International Variable Star Index (VSX) for pre-existence as a Mira-type star in variability catalogues. Summary data for all new Mira variables are listed in Table 1. (:) denotes uncertain value. Lightcurves, folded lightcurves and further details are available via AAVSO-VSX (http://www.aavso.org/vsx/).