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Cross-Correlation and Maximum Likelihood Analysis: A New Approach to Combine Cross-Correlation Functions

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arxiv astro-ph/0303426 v1 pith:7THHUCRN submitted 2003-03-18 astro-ph

classification astro-ph
keywords analysisapproachcombinationcross-correlationcombinefunctionsschemealready
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This paper presents a new approach to combine cross-correlation functions. The combination is based on a maximum-likelihood approach and uses a non-linear combination scheme. It can be effective for radial-velocity analysis of multi-order spectra, or for analysis of multiple exposures of the same object. Simulations are presented to show the potential of the suggested combination scheme. The technique has already been used to detect a very faint companion of HD41004.

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    astro-ph.GA 2025-06 conditional novelty 4.0 of 10

    Analytic Milky Way potentials reproduce N-body satellite orbits to within 5% for masses up to 10^8 Msun and radii above 30 kpc, but only within the first 1 to 2 Gyr.

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