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Volumn 438, Issue 2, 2005, Pages 757-767

Accounting for the anisoplanatic point spread function in deep wide-field adaptive optics images

Author keywords

Galaxies: fundamental parameters; Galaxies: statistics; Infrared galaxies; Instrumentation: adaptive optics

Indexed keywords

GALAXIES: FUNDAMENTAL PARAMETERS; GALAXIES: STATISTICS; INFRARED GALAXIES; INSTRUMENTATION: ADAPTIVE OPTICS;

EID: 23244459925     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20052890     Document Type: Article
Times cited : (20)

References (29)
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    • (2005) Proc. ESO Workshop
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  • 3
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    • After the dark ages: When galaxies were young (the universe at 2 < z < 5)
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    • Dickinson, M.1
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    • 23244455961 scopus 로고    scopus 로고
    • Science with Adaptive Optics, ed. M. Kasper, & W. Brandner
    • Tristram, K., & Prieto, A. 2005, in Science with Adaptive Optics, ESO workshop, ed. M. Kasper, & W. Brandner
    • (2005) ESO Workshop
    • Tristram, K.1    Prieto, A.2
  • 29
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    • Astronomical Site Evaluation in the Visible and Radio Range, ed. J. Vernin, Z. Benkhaldoun, & C. Muñoz-Tuñón
    • Weiß, A., Hippler, S., Kasper, M., Wooder, N., & Quartel, J. 2002b, in Astronomical Site Evaluation in the Visible and Radio Range, ed. J. Vernin, Z. Benkhaldoun, & C. Muñoz-Tuñón, ASP Conf. Proc., 266, 86
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    • Weiß, A.1    Hippler, S.2    Kasper, M.3    Wooder, N.4    Quartel, J.5


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.