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Volumn 448, Issue 2, 2006, Pages 801-808

The four-quadrant phase-mask coronagraph: White light laboratory results with an achromatic device

Author keywords

Instrumentation: adaptive optics; Methods: observational; Stars: planetary systems; Techniques: high angular resolution

Indexed keywords

ADAPTIVE OPTICS; ASTROPHYSICS; ATTENUATION; BIREFRINGENCE; ERROR ANALYSIS;

EID: 33644954100     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20054158     Document Type: Article
Times cited : (40)

References (21)
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    • Chabrier, G., Allard, F., Baraffe, I., Barman, T., & Hauschildt, P. H. 2004, in Extrasolar Planets: Today and Tomorrow, ed. J.P. Beaulieu, A. Lecavelier des Etangs, & C. Terquem, Proc. ASP Conf., 321, 131
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    • Chabrier, G.1    Allard, F.2    Baraffe, I.3    Barman, T.4    Hauschildt, P.H.5
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    • Mieremet, A.L.1    Braat, J.J.2    Bokhove, H.3    Ravel, K.4
  • 19
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    • Adaptive Optical System Technologies, ed. D. Bonaccini, & R. K. Tyson
    • Roussel, G., Lacombe, F., Puget, P., et al. 1998, in Adaptive Optical System Technologies, ed. D. Bonaccini, & R. K. Tyson, Proc. SPIE, 3353, 508
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    • Roussel, G.1    Lacombe, F.2    Puget, P.3
  • 20
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    • New Frontiers in Stellar Interferometry, ed. W. Traub
    • Serabyn, E., Booth, A. J., Colavita, M. M., et al. 2004, in New Frontiers in Stellar Interferometry, ed. W. Traub, Proc. SPIE, 5491, 806
    • (2004) Proc. SPIE , vol.5491 , pp. 806
    • Serabyn, E.1    Booth, A.J.2    Colavita, M.M.3


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.