High angular resolution in 2010-2020: A comparison between possible post-VLT/VLTI instruments

Proceedings of SPIE - The International Society for Optical Engineering

Volumn 4838, Issue 1, 2002, Pages 134-143

  Arnold, L ^a   Lagrange, A M ^b   Mourard, D ^c   Riaud, P ^a,d   Ferrari, M ^e   Gillet, S ^a   Kern, P ^b   Koechlin, L ^f   Labeyrie, A ^a   Lardiere O ^a   Malbet, F ^b   Perrin, G ^d   Roussel, G ^g   Tallon, M ^h  

^a OBSERVATOIRE DE HAUTE PROVENCE   (France)

^b LABORATOIRE D ASTROPHYSIQUE   (France)

^c UNIVERSITÉ CÔTE D'AZUR   (France)

^d OBSERVATOIRE DE PARIS   (France)

^e AIX MARSEILLE UNIVERSITÉ   (France)

^f IRAP   (France)

^g ONERA   (France)

^h CENTRE DE RECHERCHE ASTROPHYSIQUE DE LYON   (France)

Author keywords

Coronagraphy; ELT; Extremely large telescope; High angular resolution; High dynamics imaging; Hypertelescope; Interferometric array; Prospective; Science performance

Indexed keywords

ADAPTIVE OPTICS; IMAGING TECHNIQUES; INTERFEROMETERS; OPTICAL RESOLVING POWER;

INTERFEROMETRIC ARRAYS;

TELESCOPES;

EID: 0038739126     PISSN: 0277786X     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1117/12.458939     Document Type: Conference Paper

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