Construction of the Database for Pulsating Variable Stars

Details Construction of the Database for Pulsating Variable Stars Construction of the Database for Pulsating Variable Stars

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012cha%26a..36...27c&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 36, Issue 1, p. 27-38.

Astronomy and Astrophysics

Astrophysics

Scientific paper

A database for pulsating variable stars is constructed to favor the study of variable stars in China. The database includes about 230,000 variable stars in the Galactic bulge, LMC and SMC observed in an about 10 yr period by the MACHO(MAssive Compact Halo Objects) and OGLE(Optical Gravitational Lensing Experiment) projects. The software used for the construction is LAMP, i.e., Linux+Apache+MySQL+PHP. A web page is provided for searching the photometric data and light curves in the database through the right ascension and declination of an object. Because of the flexibility of this database, more up-to-date data of variable stars can be incorporated into the database conveniently.

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