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Starfinder: a code for crowded stellar fields analysis

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arxiv astro-ph/9911354 v1 pith:VHMZ3DO6 submitted 1999-11-18 astro-ph

E.Diolaiti , O.Bendinelli , D.Bonaccini , L.Close , D.Currie , G.Parmeggiani This is my paper · ORCID
classification astro-ph
keywords analysiscodefieldsstarfinderstellaradaptiveanisoplanaticapplications
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Starfinder is an IDL code for the deep analysis of stellar fields, designed for well-sampled images with high and low Strehl factor. An important feature is represented by the possibility to measure the anisoplanatic effect in wide-field Adaptive Optics observations and exploit this knowledge to improve the analysis of the observed field. A description of the method and applications to real AO data are presented.

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Cited by 1 Pith paper

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  1. Discovery of a Dense Association of Stars in the Vicinity of the Supermassive Black Hole Sgr A*

    astro-ph.GA 2024-11 conditional novelty 6.0 of 10

    New proper motion measurements reveal a co-moving group of 28 stars near IRS 1W in the Galactic Center, possibly a tidally stripped cluster remnant around an intermediate-mass black hole or a disk projection.

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