A deconvolution method for accurate astrometry and photometry on adaptive optics images of stellar fields

Proceedings of SPIE - The International Society for Optical Engineering

Volumn 3353, Issue , 1998, Pages 426-437

  Véran, Jean Pierre ^a   Rigaut, François J ^b  

^a NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

Author keywords

Adaptive optics; Astrometry; Deconvolution; Galactic Center; Photometry; Stellar fields

Indexed keywords

ADAPTIVE OPTICS; ARCTIC ENGINEERING; CONVOLUTION; CURVE FITTING; OPTICAL SYSTEMS; OPTICAL TRANSFER FUNCTION; PHOTOLITHOGRAPHY; PHOTOMETERS;

ADAPTIVE OPTICS IMAGES; ASTROMETRY; DECONVOLUTION METHODS; FOURIER DOMAINS; GALACTIC CENTER; LEVENBERG-MARQUARDT METHODS; OBJECTIVE FUNCTIONS; PHOTOMETRIC DATUM; POINT-SPREAD FUNCTIONS; REGULARIZED LEAST SQUARES; STELLAR FIELDS; SUPER RESOLUTIONS;

PHOTOMETRY;

EID: 37949008986     PISSN: 0277786X     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1117/12.321740     Document Type: Conference Paper

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