Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

Keck Adaptive Optics: Error Budget

Not Accessible

Your library or personal account may give you access

Abstract

The optics error budgets for the W.M. Keck Observatory natural guide star (NGS) and laser guide star (LGS) adaptive optics (AO) facilities' are presented. The purpose of generating this error budget2 is three-fold: (1) to summarize the error sources which will contribute to the degradation of images on a science instrument fed by the AO facilities, (2) to compare the predicted performance with the requirements, and (3) to provide a tool for evaluating potential engineering, and observing, trade-offs.

© 1996 Optical Society of America

PDF Article
More Like This
W.M. Keck Observatory Adaptive Optics Facility

P. Wizinowich, D. S. Acton, A. Gleckler, T. Gregory, P. Stomski, K. Avicola, J. Brase, H. Friedman, D. Gavel, and C. Max
AMB.1 Adaptive Optics (AO) 1996

Keck Observatory Adaptive Optics Program

Peter L. Wizinowich and Anthony D. Gleckler
MB1 Adaptive Optics (AO) 1995

Keck Adaptive Optics: Optical Bench Subsystem

T. Gregory, P. Wizinowich, D. S. Acton, A. Gleckler, P. Stomski, S. Radau, J. Maute, and M. Sirota
AMB.2 Adaptive Optics (AO) 1996

Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All rights reserved, including rights for text and data mining and training of artificial technologies or similar technologies.