Paper
9 September 2019 Self-nulling spectrograph for star glare rejection
Author Affiliations +
Abstract
We introduce a notional nulling interferometer for extinction of glare from single star exoplanetary systems. The principle of double dispersion telescopy correlates an incident angular position with a unique wavelength. In such telescopes, a secondary spectrograph is used to disambiguate overlapping wavelengths from the primary disperser. A single rejection band can be created in the secondary spectrograph based on the resulting wavelength modulation. Two optical paths are directed from the slit situated between the primary and secondary dispersers. Angles of incidence and path lengths are slightly offset between the pair of post-slit wave trains. By this configuration, a half wave path difference is established at the position and diameter of the host star, causing phase cancellation at a unique spectral band. Having a single rejection band avoids repetitive banding endemic to conventional interferometric telescopy. There is a tradeoff with chromatic aberration in the images of the exoplanets.
© (2019) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Thomas D. Ditto "Self-nulling spectrograph for star glare rejection", Proc. SPIE 11117, Techniques and Instrumentation for Detection of Exoplanets IX, 111171P (9 September 2019); https://doi.org/10.1117/12.2525524
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KEYWORDS
Stars

Interferometers

Telescopes

Exoplanets

Mirrors

Spectrographs

Interferometry

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