CCD RV light curve of M15 RR Lyrae (Arellano Ferro+, 2006)

Details CCD RV light curve of M15 RR Lyrae (Arellano Ferro+, 2006) CCD RV light curve of M15 RR Lyrae (Arellano Ferro+, 2006)

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ycatp008004201a&link_type=abstract

VizieR On-line Data Catalog: J/other/RMxAA/42.75. Originally published in: 2006RMxAA..42...75A

Other

Clusters: Globular, Stars: Variable, Photometry: Ccd

Scientific paper

V and R images were obtained in 2000 and 2001, using the 1.5m telescope of San Pedro Martit Observatory (SPM), in Baja California, Mexico. A total of 129 and 127 images in the V and R filters, respectively, were obtained during both seasons and distributed in two fields of the cluster. The instrumental magnitudes were obtained using the PSF function, calculated for each frame from relatively isolated and well exposed stars, in the field of the cluster. The transformation to the standard system was performed differentially, relative to a group of standard stars in the observed fields of M15. The accuracy of the photometry is estimated as +/-0.031 and +/-0.019 for the V and R filters respectively.
(3 data files).

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