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<title>StarFinder: an IDL GUI-based code to analyze crowded fields with isoplanatic correcting PSF fitting</title>

2000/04/07 by E. Diolaiti, Emiliano Diolaiti, O. Bendinelli +6 · 5 citations
Mathematics · Physics and Astronomy · #Adaptive optics #Adaptive optics and wavefront sensing #Artificial intelligence #Code (set theory) #Computational science #Computer graphics (images) #Computer science #Field (mathematics) #Galaxies: Formation, Evolution, Phenomena #Geometry #Graphical user interface #Mathematics #Optics #Physics #Point (geometry) #Point spread function #Programming language #Source code #Stellar, planetary, and galactic studies #Strehl ratio #astro-ph

paper · pdf · doi:10.1117/12.390377

9 pages, to to be published on "Proceeedings of Adaptive Optical Systems Technology",Proc.of SPIE,Vol.4007,2000. In press

arxiv created 2000/04/07 · openalex publication_date 2000/07/07 · arxiv updated 2015/06/24 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

StarFinder is a new code for the deep analysis of stellar fields, designed for well-sampled images with high and low Strehl ratio. It is organized in the form of a self-contained IDL widget-based application, with a 'user-friendly' graphic interface. We give here a general description of the code along with some applications to real data with space-invariant Point Spread Function (PSF). We present also some methods to handle anisoplanatic effects in wide-field Adaptive Optics (AO)observations.

Citations

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