The analysis of Eddington asteroseismology data

Details The analysis of Eddington asteroseismology data The analysis of Eddington asteroseismology data

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.485..200k&link_type=abstract

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

Computer Science

Stars: Photometry, Low-Amplitude Oscillations

Scientific paper

The primary science goal for Eddington is to detect stellar oscillations and terrestrial-sized planets. The oscillations will be used to perform asteroseismology on a large sample of stars of different ages, masses and chemical composition. In order to do this we need high precision photometric time series observations. To achieve high precision, we need to understand the different noise and error sources and verify our ability to measure stellar oscillations at the required level of sensitivity. This paper describes some key aspects of the analysis of the Eddington asteroseismology, data, focusing on the known noise sources. In the last section an alternative design for Eddington is discussed.

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