Share Email Print

Proceedings Paper

Status of point spread function determination for Keck adaptive optics
Format Member Price Non-Member Price
PDF $17.00 $21.00

Paper Abstract

There is great interest in the adaptive optics (AO) science community to overcome the limitations imposed by incomplete knowledge of the point spread function (PSF). To address this limitation a program has been initiated at the W. M. Keck Observatory (WMKO) to demonstrate PSF determination for observations obtained with Keck AO science instruments. This paper aims to give a broad view of the progress achieved in this area. The concept and the implementation are briefly described. The results from on-sky on-axis NGS AO measurements using the NIRC2 science instrument are presented. On-sky performance of the technique is illustrated by comparing the reconstructed PSFs to NIRC2 PSFs. Accuracy of the reconstructed PSFs in terms of Strehl ratio and FWHM are discussed. Science cases for the first phase of science verification have been identified. More technical details of the program are presented elsewhere in the conference.

Paper Details

Date Published: 21 July 2014
PDF: 11 pages
Proc. SPIE 9148, Adaptive Optics Systems IV, 91480S (21 July 2014); doi: 10.1117/12.2056696
Show Author Affiliations
S. Ragland, W. M. Keck Observatory (United States)
L. Jolissaint, Univ. of Applied Sciences Western Switzerland (Switzerland)
P. Wizinowich, W. M. Keck Observatory (United States)
C. Neyman, W. M. Keck Observatory (United States)

Published in SPIE Proceedings Vol. 9148:
Adaptive Optics Systems IV
Enrico Marchetti; Laird M. Close; Jean-Pierre Véran, Editor(s)

© SPIE. Terms of Use
Back to Top
Sign in to read the full article
Create a free SPIE account to get access to
premium articles and original research
Forgot your username?