Warsaw Variability Surveys

Abstract

Four large/medium size photometric surveys are being conducted by Warsaw astronomers: Warsaw-LCO survey of globular clusters, OGLE, DIRECT and ASAS. In this contribution we provide short description of these projects and discuses briefly some results obtained for pulsating variables.

6 pages, LaTex, 2 encapsulated Postscript figures. To be published in IAU Coll 176 "The Impact of Large Scale Surveys on Pulsating Stars research", eds. L. Szabados & D. Kurtz (ASP Conf. Ser.); corrected erroneous WWW address

References in corpus (8)

• DIRECT Distances to Nearby Galaxies Using Detached Eclipsing Binaries and Cepheids. I. Variables in the Field M31B
• RR Lyrae Variables in the Globular Cluster M55. The First Evidence for Non Radial Pulsations in RR Lyr Stars
• DIRECT Distances to Nearby Galaxies Using Detached Eclipsing Binaries and Cepheids. II. Variables in the Field M31A
• Search for Variable Stars in the Globular Cluster M3
• DIRECT Distances to Nearby Galaxies Using Detached Eclipsing Binaries and Cepheids. III. Variables in the Field M31C
• DIRECT Distances to Nearby Galaxies Using Detached Eclipsing Binaries and Cepheids. IV. Variables in the Field M31D
• CCD PHOTOMETRY OF VARIABLE STARS IN THE GLOBULAR CLUSTER RU 106
• CCD Photometry of Faint Variable Stars in the Globular Cluster NGC 6752