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Analysis of isoplanatic high resolution stellar fields by the StarFinder code

Open access
Diolaiti, E., Bendinelli, O., Bonaccini, D., Close, L., Currie, D., Parmeggiani, G.·2000·Astronomy and Astrophysics Supplement Series

Abstract

We describe a new code for the deep analysis of stellar fields, designed for Adaptive Optics (AO) Nyquist-sampled images with high and low Strehl ratio. The Point Spread Function (PSF) is extracted directly from the image 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 AO data are presented.

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Metadata

Authors
Diolaiti, E., Bendinelli, O., Bonaccini, D., Close, L., Currie, D., & Parmeggiani, G.
Venue
Astronomy and Astrophysics Supplement Series
Publisher
EDP Sciences
Published
2000-12
Volume
147
Issue
2
Pages
335-346
ISSN
  • 0365-0138 (ISSN-L)
  • 1286-4846
OpenAlex
W2130468066
Cited by
400
References
0
FWCI
3.79
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Analysis of isoplanatic high resolution stellar fields by the StarFinder code. https://app.cochat.ai/papers/10.1051/aas:2000305
The paper
Diolaiti, E., Bendinelli, O., Bonaccini, D., Close, L., Currie, D., & Parmeggiani, G. (2000). Analysis of isoplanatic high resolution stellar fields by the StarFinder code. Astronomy and Astrophysics Supplement Series. https://doi.org/10.1051/aas%3A2000305

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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.