Comparison of coronagraphs for high-contrast imaging in the context of extremely large telescopes

Astronomy and Astrophysics

Volumn 492, Issue 1, 2008, Pages 289-300

  Martinez, P ^a,b,f   Boccaletti, A ^b,f   Kasper, M ^a   Cavarroc, C ^c   Yaitskova, N ^a   Fusco, T ^d,f   Verinaud C ^e  

^a EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^b UNIVERSITÉ PARIS DIDEROT   (France)

^c DIF   (France)

^d ONERA   (France)

^e LABORATOIRE D ASTROPHYSIQUE   (France)

^f PHASE ^*

Author keywords

Instrumentation: adaptive optics; Instrumentation: high angular resolution; Techniques: high angular resolution; Telescopes

Indexed keywords

ABERRATIONS; CALIBRATION; GEOMETRICAL OPTICS; INSTRUMENTS; OPTICAL INSTRUMENTS; OPTICAL PROPERTIES; TELESCOPES;

ANGULAR SEPARATIONS; BASELINE DESIGNS; CALIBRATION UNITS; CENTRAL OBSCURATIONS; CONTRAST IMAGING; CORONAGRAPHIC TELESCOPES; CRITICAL PARAMETERS; DETECTION PROCESSES; ERROR SOURCES; EXTREME ADAPTIVE OPTICS; EXTREMELY LARGE TELESCOPES; INSTRUMENTATION: ADAPTIVE OPTICS; INSTRUMENTATION: HIGH ANGULAR RESOLUTION; LYOT CORONAGRAPHS; PHASE ABERRATIONS; POINTING ERRORS; SECONDARY SUPPORTS; SIMPLE MODELS; STATIC PHASE; STREHL RATIOS; TECHNIQUES: HIGH ANGULAR RESOLUTION;

OPTICAL TELESCOPES;

EID: 57249111605     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810650     Document Type: Article

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