StarFinder: An IDL GUI based code to analyze crowded fields with isoplanatic correcting PSF fitting

E. Diolaiti; O. Bendinelli; D. Bonaccini; L. M. Close; D. G. Currie; G. Parmeggiani

StarFinder: An IDL GUI based code to analyze crowded fields with isoplanatic correcting PSF fitting

E. Diolaiti, O. Bendinelli, D. Bonaccini, L. M. Close, D. G. Currie, G. Parmeggiani

Research output: Contribution to journal › Conference article › peer-review

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.

Original language	English (US)
Pages (from-to)	II/-
Journal	Proceedings of SPIE - The International Society for Optical Engineering
Volume	4007
State	Published - 2000
Externally published	Yes
Event	Adaptive Optical Systems Technology - Munich, Ger Duration: Mar 29 2000 → Mar 31 2000

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Cite this

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title = "StarFinder: An IDL GUI based code to analyze crowded fields with isoplanatic correcting PSF fitting",

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.",

author = "E. Diolaiti and O. Bendinelli and D. Bonaccini and Close, {L. M.} and Currie, {D. G.} and G. Parmeggiani",

year = "2000",

language = "English (US)",

volume = "4007",

pages = "II/--",

journal = "Proceedings of SPIE - The International Society for Optical Engineering",

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publisher = "SPIE",

note = "Adaptive Optical Systems Technology ; Conference date: 29-03-2000 Through 31-03-2000",

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TY - JOUR

T1 - StarFinder

T2 - Adaptive Optical Systems Technology

AU - Diolaiti, E.

AU - Bendinelli, O.

AU - Bonaccini, D.

AU - Close, L. M.

AU - Currie, D. G.

AU - Parmeggiani, G.

PY - 2000

Y1 - 2000

N2 - 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.

AB - 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.

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UR - http://www.scopus.com/inward/citedby.url?scp=0033699097&partnerID=8YFLogxK

M3 - Conference article

AN - SCOPUS:0033699097

SN - 0277-786X

VL - 4007

SP - II/-

JO - Proceedings of SPIE - The International Society for Optical Engineering

JF - Proceedings of SPIE - The International Society for Optical Engineering

Y2 - 29 March 2000 through 31 March 2000

ER -

StarFinder: An IDL GUI based code to analyze crowded fields with isoplanatic correcting PSF fitting

Abstract

ASJC Scopus subject areas

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