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      Externally Dispersed Interferometry for Precision Radial Velocimetry

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          Abstract

          Externally Dispersed Interferometry (EDI) is the series combination of a fixed-delay field-widened Michelson interferometer with a dispersive spectrograph. This combination boosts the spectrograph performance for both Doppler velocimetry and high resolution spectroscopy. The interferometer creates a periodic spectral comb that multiplies against the input spectrum to create moire fringes, which are recorded in combination with the regular spectrum. The moire pattern shifts in phase in response to a Doppler shift. Moire patterns are broader than the underlying spectral features and more easily survive spectrograph blurring and common distortions. Thus, the EDI technique allows lower resolution spectrographs having relaxed optical tolerances (and therefore higher throughput) to return high precision velocity measurements, which otherwise would be imprecise for the spectrograph alone.

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          Spatial heterodyne spectroscopy for the exploration of diffuse interstellar emission lines at far-ultraviolet wavelengths

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            An Externally Dispersed Interferometer for Sensitive Doppler Extrasolar Planet Searches

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              An Externally Dispersed Interferometer Prototype for Sensitive Radial Velocimetry: Theory and Demonstration on Sunlight

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                Author and article information

                Journal
                10 October 2007
                Article
                0710.2130
                251b5f25-3091-4da3-b5e3-9458c30fe07b
                History
                Custom metadata
                7 Pages, White paper submitted to the AAAC Exoplanet Task Force
                astro-ph

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