[c]StarFinder: A code for stellar field analysis[/c][/b]
Abstract: StarFinder is an IDL code for the deep analysis of stellar fields, designed for Adaptive Optics well-sampled images with high and low Strehl ratio. The Point Spread Function is extracted directly from the frame, to take into account the actual structure of the instrumental response and the atmospheric effects. The code is written in IDL language and organized in the form of a self-contained widget-based application, provided with a series of tools for data visualization and analysis. A description of the method and some applications to Adaptive Optics data are presented.
Credit: Diolaiti, Emiliano; Bendinelli, Orazio; Bonaccini, Domenico; Close, Laird M.; Currie, Doug G.; Parmeggiani, Gianluigi
Site: http://cfao.ucolick.org/software/starfinder.php
https://ui.adsabs.harvard.edu/abs/2000ASPC..216..623D
Bibcode: 2000ascl.soft11001D
Preferred citation method: https://ui.adsabs.harvard.edu/abs/2000SPIE.4007..879D
ID: ascl:0011.001
StarFinder: A code for stellar field analysis
StarFinder: A code for stellar field analysis
Last edited by Ada Coda on Thu Aug 08, 2019 8:43 pm, edited 1 time in total.
Reason: Updated code entry.
Reason: Updated code entry.
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