Published December 13, 2020 | Version Published
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Wavefront control experiments with a single mode fiber at the High-Contrast Spectroscopy Testbed for Segmented Telescopes (HCST)

Abstract

Achieving high levels of contrast over broad bandwidths with segmented aperture telescopes is a key requirement to maximize the scientific yield for future exoplanet imaging missions and ground-based extremely large telescopes. The High-Contrast Spectroscopy Testbed for Segmented Telescopes (HCST) in the Exoplanet Technology Laboratory (ET Lab) at Caltech is designed to proof test new technologies aimed at tackling some of the most pressing and challenging goals of exoplanet science, namely the imaging and spectroscopic characterization of small planets across a wide range of stellar host types, including temperature Earth-size planets. Here we report on the status of a key milestone: Demonstration of 20% bandwidth nulling experiments using single mode fibers wavefront control.

Additional Information

© 2020 Society of Photo-Optical Instrumentation Engineers (SPIE). This work was partially supported by the National Science Foundation AST-ATI Grant 1710210.

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Additional details

Identifiers

Eprint ID
107342
Resolver ID
CaltechAUTHORS:20210106-103901413

Funding

NSF
AST-1710210

Dates

Created
2021-01-06
Created from EPrint's datestamp field
Updated
2021-11-16
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
Astronomy Department
Series Name
Proceedings of SPIE
Series Volume or Issue Number
11443