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Studies of the Effects of Control Bandwidth and Dark-Hole Size on the HCIT Contrast Performance In this presentation, we compare model predictions with HCIT experiments. These were done for Coronagraph Milestone 3 model validation.
Document ID
20170007041
Acquisition Source
Jet Propulsion Laboratory
Document Type
Presentation
External Source(s)
hdl:2014/45748
Authors
Sidick, Erkin (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Shaklan, Stuart (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Balasubramanian, Kunjithapatha (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Cady, Eric J. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 1, 2017
Publication Date
August 9, 2015
Subject Category
Instrumentation And Photography
Astronomy
Meeting Information
Meeting: Spie Optics + Photonics Exhibit 2015
Location: San Diego, CA
Country: United States
Start Date: August 9, 2015
End Date: August 13, 2015
Sponsors: International Society for Optical Engineering
Distribution Limits
Public
Copyright
Other
Keywords
adaptive optics
exoplanets
high-contrast imaging
space telescopes
coronagraphy

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