Paper
21 March 1997 Interferometric spectrometer for liquid mirror survey telescopes
Author Affiliations +
Proceedings Volume 2871, Optical Telescopes of Today and Tomorrow; (1997) https://doi.org/10.1117/12.269028
Event: Optical Telescopes of Today and Tomorrow, 1996, Landskrona/Hven, Sweden
Abstract
A new application for the technique of holographic Fourier transform spectroscopy [Stroke and Funkhauser, Phys. Lett. 16, 272 (1965)] is presented. We propose placing a Michelson interferometer in the focal plane of a zenith-looking liquid mirror telescope [Borra et al., this conference]. A wedge whose apex runs perpendicular to the star drift direction is introduced between the two arms creating a variation in the star's apparent intensity due to interference as it drifts across the focal plane. The record of this intensity variation is the interferogram of the star, i.e. the Fourier transform of its spectrum. Imaging the mirrors of the Michelson onto a CCD array thus allows simultaneous spectral measurements of numerous sources. We present calculations indicating that a limiting magnitude of 18.6 may be reached with a spectral sampling of 4 A covering from 5000 A to 9000 A by summing 100 nights of observations.
© (1997) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Kjetil Dohlen "Interferometric spectrometer for liquid mirror survey telescopes", Proc. SPIE 2871, Optical Telescopes of Today and Tomorrow, (21 March 1997); https://doi.org/10.1117/12.269028
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Cited by 3 scholarly publications.
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KEYWORDS
Signal to noise ratio

Stars

Mirrors

Spectroscopy

Telescopes

Charge-coupled devices

Fourier transforms

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