The analysis of MONS simulation data on α Cen A+B

Details The analysis of MONS simulation data on α Cen A+B The analysis of MONS simulation data on α Cen A+B

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.485..313r&link_type=abstract

In: Proceedings of the First Eddington Workshop on Stellar Structure and Habitable Planet Finding, 11 - 15 June 2001, Córdoba, S

Physics

Methods: Data Analysis, Solar-Like Stars: Oscillations

Scientific paper

A realistic simulation of the stellar system α Cen A+B as it would be seen by MONS satellite has been generated in the "MONS Time-series simulation and analysis Team". The simulation apparently includes all properties known of the stars, instrumental noise sources and sensitivity properties expected. We have been working with this data series without any previous knowledge of the information included in it or on how it has been generated, with the exception of its length, one month, and its sampling time, 80 seconds. It has been tried to extract as many information as possible about: frequencies, damping time, amplitudes, rotation, background noise level, mode identification etc.

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