Colour-correlated noise: can it improve the S/N of the Eddington data?

Details Colour-correlated noise: can it improve the S/N of the Eddington data? Colour-correlated noise: can it improve the S/N of the Eddington data?

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004esasp.538..335k&link_type=abstract

In: Second Eddington Workshop: Stellar structure and habitable planet finding, 9 - 11 April 2003, Palermo, Italy. Edited by F. F

Physics

Instrumentation: Noise Properties, Sun: Background Noise Spectrum

Scientific paper

In this paper we use the SoHO/VIRGO three colour time series data to investigate how colour correlated stellar signal and noise may be used to improve the S/N of the Eddington time series. We conclude that one may implement a two-colour system on Eddington in order to reduce the amount of noise at low frequencies. We propose a blue and a red broad band filter having the following passbands: blue: 350-650 nm and red: 550-850 nm.

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