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Astronomical spectrograph calibration with broad-spectrum frequency combs

Published

Author(s)

Danielle Braje, Matthew S. Kirchner, Tara M. Fortier, Scott A. Diddams, Leo W. Hollberg, Steve Osterman

Abstract

Broad-band frequency combs are filtered to spectrographically resolvable frequency-mode spacing, and the limitations of using cavities for spectral filtering are considered. Data and theory are used to show implications to spectrographic calibration of high-resolution, astronomical spectrometers.
Citation
European Physical Journal D
Volume
48

Keywords

Fabry-Perot cavity, frequency comb, spectrograph calibration

Citation

Braje, D. , Kirchner, M. , Fortier, T. , Diddams, S. , Hollberg, L. and Osterman, S. (2008), Astronomical spectrograph calibration with broad-spectrum frequency combs, European Physical Journal D, [online], https://tsapps.nist.gov/publication/get_pdf.cfm?pub_id=842428 (Accessed February 29, 2024)
Created May 29, 2008, Updated February 19, 2017