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Stellar Radial Velocities of High Precision: Techniques and Results
International Astronomical Union Colloquium, 1984AbstractRelative radial velocities can now be determined with internal errors as small as ~ 10 m s−l. A variety of techniques for achieving this level of precision are either presently running, or will soon be on-line. These could be used on several astronomical frontiers; the most demanding application is the search for extra-solar planetary systems ...
Bruce Campbell, G.A.H. Walker
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FM stars: a Fourier view of pulsating binary stars, a new technique for measuring radial velocities photometrically [PDF]
Some pulsating stars are good clocks. When they are found in binary stars, the frequencies of their luminosity variations are modulated by the Doppler effect caused by orbital motion. For each pulsation frequency this manifests itself as a multiplet separated by the orbital frequency in the Fourier transform of the light curve of the star.
Hiromoto Shibahashi, D W Kurtz
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The radial velocity estimation based on digital spotlight technique
2015 IEEE 5th Asia-Pacific Conference on Synthetic Aperture Radar (APSAR), 2015For synthetic aperture radar(SAR) imaging of ship targets, it's difficult to generate high quality images because their motion characteristics are blind in most cases. Aiming at this problem, this paper presents a processing scheme for estimating the radial velocity based on the digital spotlight processing.
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