AGAPEROS: variable stars in the LMC Bar (Melchior+, 2000)

Computer Science

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Stars: Variable, Magellanic Clouds, Photometry

Scientific paper

The 91-92 EROS-1 data set has been used to select Long Timescale and Long Period Variables (LT&LPV). We choose to perform a selection of variable objects as comprehensive as possible, independent of periodicity and of their position on the colour magnitude diagram, and produce a catalogue of 632 variable objects. Table 2 provides the parameters of the variable objects detected in this paper. They are sorted in order of increasing right ascension. The columns contains the name of the variable including the RA,DEC (J2000.0) coordinates, the number of the chip and (x,y) position, the blending flags (PhiC/Phi0)B, (PhiC/Phi0)R in both colours, the BEROS and REROS magnitude, the number of star NstarB, NstarR found in the superpixel, the magnitude BEROSDAO and REROSDAO estimated with DAOPHOT, and when available the cross-identifications with previous catalogue. (1 data file).

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