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Volumn 5489, Issue PART 1, 2004, Pages 391-406

OWL phase a status report

Author keywords

Extremely Large Telescopes; OWL; Science objectives; Segments fabrication; Wavefront control

Indexed keywords

ADAPTIVE OPTICS; ARRAYS; COMPUTATIONAL FLUID DYNAMICS; COMPUTER SIMULATION; GLASS CERAMICS; INFRARED DEVICES; INVESTMENTS; SENSORS; SILICON CARBIDE; WAVEFRONTS;

EID: 10444266685     PISSN: 0277786X     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1117/12.556015     Document Type: Conference Paper
Times cited : (25)

References (22)
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  • 4
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  • 7
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    • Dierickx, P.1
  • 8
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    • OWL optical design, active optics and error budget
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  • 11
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    • APE: A breadboard to evaluate new phasing technologies for a future European Giant optical telescope
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  • 12
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    • Simulations of(MC)AO for a 100-m telescope
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  • 13
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    • MAD status report
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  • 15
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    • SLODAR: Measuring optical turbulence altitude with a Shack-Hartmann wavefront sensor
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  • 16
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    • OWL site survey: First seeing measurements with ADIMM
    • June
    • Z. Benkhaldoun, A. Abahamid, Y. El Azhari and E. Siher, OWL Site Survey: first seeing measurements with ADIMM. SPIE 5489-10, June 2004.
    • (2004) SPIE , vol.5489 , Issue.10
    • Benkhaldoun, Z.1    Abahamid, A.2    El Azhari, Y.3    Siher, E.4
  • 17
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    • Correlation between TOMS aerosol index and astronomical extinction
    • June
    • E. Siher, S. Ortolani, M. Sarazin, Z. Benkhaldoun; Correlation between TOMS aerosol index and astronomical extinction; SPIE 5489-13, June 2004.
    • (2004) SPIE , vol.5489 , Issue.13
    • Siher, E.1    Ortolani, S.2    Sarazin, M.3    Benkhaldoun, Z.4
  • 18
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    • Site Selection for OWL using past, present and future climate information
    • June
    • E. Graham, M. Sarazin, M. Beniston, C. Collet, M. Hayoz, M. Neun, S. Goyette; Site Selection for OWL using past, present and future climate information; SPIE 5489-12, June 2004.
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    • Graham, E.1    Sarazin, M.2    Beniston, M.3    Collet, C.4    Hayoz, M.5    Neun, M.6    Goyette, S.7
  • 19
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    • Science and technology drivers for future giant telescopes
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  • 20
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.