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A Synoptic Variability Survey of M3

Published online by Cambridge University Press:  12 April 2016

Andrew Szentgyorgyi ,
Krzysztof Z. Stanek ,
Dimitar Sasselov ,
Janusz Kaluzny  and
Aleksander Schwarzenberg-Czerny
Andrew Szentgyorgyi
Affiliation:
Optical and Infrared Division, Harvard-Smithsonian Center for Astrophysics, 60 Garden St, Cambridge, MA, 02138, USA
Krzysztof Z. Stanek
Affiliation:
Optical and Infrared Division, Harvard-Smithsonian Center for Astrophysics, 60 Garden St, Cambridge, MA, 02138, USA
Dimitar Sasselov
Affiliation:
Optical and Infrared Division, Harvard-Smithsonian Center for Astrophysics, 60 Garden St, Cambridge, MA, 02138, USA
Janusz Kaluzny
Affiliation:
Nicolaus Copernicus Astronomical Center, Bartycka 18, 00-716 Warsaw, Poland
Aleksander Schwarzenberg-Czerny
Affiliation:
Nicolaus Copernicus Astronomical Center, Bartycka 18, 00-716 Warsaw, Poland

Abstract

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We present preliminary results from a synoptic photometric variability survey of the galactic globular cluster M3. These data consist of between 9 and 13 nights of data, the sampling allows a minimum detectable period of 10 minutes and is complete to MV ~ 21.

Type
Part 3. Cepheids, RR Lyrae Stars, Distance Scales
Information
International Astronomical Union Colloquium , Volume 176: The Impact of Large-Scale Surveys on Pulsating Star Research , 2000 , pp. 161 - 164
Copyright
Copyright © Astronomical Society of the Pacific 2000

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