Simulation of moving exoplanets detection using the VLT instrument SPHERE/IRDIS

Proceedings of SPIE - The International Society for Optical Engineering

Volumn 7015, Issue , 2008, Pages

  Smith, I ^a   Carbillet, M ^a   Ferrari, A ^a   Mouillet, D ^b   Boccaletti, A ^c   Dohlen, K ^d  

^a UNIVERSITÉ DE NICE SOPHIA ANTIPOLIS   (France)

^b OBSERVATOIRE DE GRENOBLE   (France)

^c UNIVERSITÉ PARIS DIDEROT   (France)

^d OBSERVATOIRE DE MARSEILLE   (France)

Author keywords

Adaptive optics; Coronagraphy; Detection; Exoplanets; Simulation; SPHERE

Indexed keywords

ANALYTICAL PROPERTIES; CORONAGRAPHY; DATA MODELS; DATA SETS; DETECTION; DIRECT IMAGING; ESTIMATION ALGORITHM; EXOPLANET; EXOPLANETS; EXTREME ADAPTIVE OPTICS; FALSE ALARMS; GAUSSIAN DATA; HIGH CONTRAST; INITIAL POSITION; INTENSITY RATIO; LOW SIGNAL-TO-NOISE RATIO; PLANET FINDERS; QUASI-STATIC; SIMULATION; STATIONARITY; THRESHOLDING; TIME EVOLUTIONS; VLT INSTRUMENTS;

ADAPTIVE OPTICS; ALARM SYSTEMS; ESTIMATION; SIGNAL TO NOISE RATIO; SIMULATORS; SPHERES; UNCERTAINTY ANALYSIS;

DATA PROCESSING;

EID: 66949147614     PISSN: 0277786X     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1117/12.789413     Document Type: Conference Paper

References (9)

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