The Adaptive Optics Point Spread Function from Keck and Gemini
Abstract
From analyzing adaptive optics (AO) images of stars obtained at Keck (10 m telescope) and Gemini North (8 m telescope) Observatories, we verify that in general, the AO point spread function (PSF) can be modeled as a Lorentzian or a Lorentzian plus an Airy. However, an additional Gaussian component in the Gemini PSF is associated with an observed degraded AO performance.
Document Details
- Document Type
- Technical Report
- Publication Date
- Sep 01, 2009
- Accession Number
- ADA531760
Entities
People
- Al Conrad
- Benoit Carry
- Jack Drummond
- Julian Christou
- William J. Merline
Organizations
- Air Force Research Laboratory