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A Phase-Shifting Zernike Wavefront Sensor for the Palomar P3K Adaptive Optics SystemA phase-shifting Zernike wavefront sensor has distinct advantages over other types of wavefront sensors. Chief among them are: 1) improved sensitivity to low-order aberrations and 2) efficient use of photons (hence reduced sensitivity to photon noise). We are in the process of deploying a phase-shifting Zernike wavefront sensor to be used with the realtime adaptive optics system for Palomar. Here we present the current state of the Zernike wavefront sensor to be integrated into the high-order adaptive optics system at Mount Palomar's Hale Telescope.
Document ID
20130003213
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
External Source(s)
Authors
Wallace, J. Kent
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Crawford, Sam
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Loya, Frank
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Moore, James
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 27, 2013
Publication Date
July 1, 2012
Subject Category
Space Sciences (General)
Meeting Information
Meeting: SPIE Astronomical Telescopes+Instrumentation
Location: Amsterdam
Country: Netherlands
Start Date: July 1, 2012
End Date: July 6, 2012
Sponsors: International Society for Optical Engineering
Distribution Limits
Public
Copyright
Other
Keywords
adaptive optics
wavefront sensing

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