Paper
28 July 2008 The development and applications of a ground-based fiber nulling coronagraph
Author Affiliations +
Abstract
A rotating nulling coronagraph has been built for use on ground-based telescopes. The system is based on the concept of sub-aperturing the pupil of the telescope with two elliptical apertures and combining the resulting two input beams on a single-mode fiber. By a relative π phase shift of the beams, the starlight can be nulled and a relatively faint companion star can be detected. Rotation of the aperture mask on the telescope pupil results in a signal similar to that expected from a space-borne telescope system such as the proposed TPF/Darwin interferometer. The design of the nulling coronagraph and the ancillary systems that are needed, such as the fringe tracker, are described and the potential for observations on telescopes such as the Palomar 200" is discussed. Results of a nulling experiment using a single mode fiber as a beam combiner for broadband light between 1.50 μm and 1.80 μm are shown.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Stefan Martin, Eugene Serabyn, Kurt Liewer, Frank Loya, Bertrand Mennesson, Charles Hanot, and Dimitri Mawet "The development and applications of a ground-based fiber nulling coronagraph", Proc. SPIE 7013, Optical and Infrared Interferometry, 70131Y (28 July 2008); https://doi.org/10.1117/12.789484
Lens.org Logo
CITATIONS
Cited by 12 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Nulling interferometry

Telescopes

Space telescopes

Mirrors

Stars

Coronagraphy

Sensors

RELATED CONTENT

METIS: the mid-infrared E-ELT imager and spectrograph
Proceedings of SPIE (July 28 2014)
SHARK NIR from K band to a key instrument,...
Proceedings of SPIE (July 27 2016)
Keck Interferometer
Proceedings of SPIE (July 24 1998)
Near-infrared AO coronagraph design for giant telescopes
Proceedings of SPIE (January 30 2003)

Back to Top