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Volumn 5491, Issue PART 3, 2004, Pages 1649-1660

Baseline monitoring for astrometric interferometry

Author keywords

Astrometry; Baseline; Interferometry; Narrow angle astrometry; Pivot point

Indexed keywords

ASTROMETRY; BASELINE; NARROW-ANGLE ASTROMETRY; PIVOT POINT;

EID: 11144302500     PISSN: 0277786X     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1117/12.552320     Document Type: Conference Paper
Times cited : (6)

References (5)
  • 1
    • 0001570471 scopus 로고
    • Potential of long-baseline infrared interferometry for narrow-angle astrometry
    • M. Shao and M. M. Colavita, "Potential of long-baseline infrared interferometry for narrow-angle astrometry," A&A, 262, 353-358, 1992.
    • (1992) A&A , vol.262 , pp. 353-358
    • Shao, M.1    Colavita, M.M.2
  • 2
    • 0000991624 scopus 로고
    • The Mark II stellar interferometer
    • M. Shao, M. M. Colavita, et al., "The Mark II Stellar Interferometer," A&A, 193, 357-371, 1988.
    • (1988) A&A , vol.193 , pp. 357-371
    • Shao, M.1    Colavita, M.M.2
  • 3
    • 0028750797 scopus 로고
    • The USNO astrometric interferometer
    • J. B. Breckinridge, ed., Proc SPIE
    • D. J. Hutter, "The USNO Astrometric Interferometer," Amplitude and Intensity Spatial Interferometry II, J. B. Breckinridge, ed., Proc SPIE, 2200, 81-88, 1994.
    • (1994) Amplitude and Intensity Spatial Interferometry II , vol.2200 , pp. 81-88
    • Hutter, D.J.1
  • 4
    • 0038995698 scopus 로고
    • Wide angle astrometry with the Mark II stellar interferometer
    • M. Shao, M. M. Colavita, et al., "Wide Angle Astrometry with the Mark II Stellar Interferometer," AJ, 100, 1701-1711, 1990.
    • (1990) AJ , vol.100 , pp. 1701-1711
    • Shao, M.1    Colavita, M.M.2
  • 5
    • 0032682178 scopus 로고    scopus 로고
    • The palomar testbed interferometer
    • M. M. Colavita, T. K. Wallace, et al., "The Palomar Testbed Interferometer," ApJ, 510, 505-521, 1999.
    • (1999) ApJ , vol.510 , pp. 505-521
    • Colavita, M.M.1    Wallace, T.K.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.