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Volumn 281, Issue 5384, 1998, Pages 1825-1829

Overview and initial results of the very long baseline interferometry space observatory programme

(53)  Hirabayashi, H a   Hirosawa, H a   Kobayashi, H a   Murata, Y a   Edwards, P G a   Fomalont, E B a   Fujisawa, K a   Ichikawa, T a   Kii, T a   Lovell, J E J a   Moellenbrock, G A a   Okayasu, R a   Inoue, M b   Kawaguchi, N b   Kameno, S b   Shibata, K M b   Asaki, Y b   Bushimata, T b   Enome, S b   Horiuchi, S b   more..


Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; ASTRONOMY; DATA ANALYSIS; GAMMA RADIATION; INTERFEROMETRY; NOISE; PRIORITY JOURNAL; TELECOMMUNICATION;

EID: 0032544294     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.281.5384.1825     Document Type: Article
Times cited : (191)

References (38)
  • 2
    • 3543147958 scopus 로고    scopus 로고
    • note
    • -7 degrees) is about the angle spanned by a strand of hair at a distance of 20 km from the observer.
  • 4
  • 6
    • 0026169479 scopus 로고
    • L. R. D'Addario, IEEE Trans. Instrum. Meas. 40, 584 (1991); N. Kawaguchi et al., in VLBI Technology: Progress and Future Observational Possibilities, T. Sasao, S. Manabe, O. Kameya, M. Inoue, Eds. (Terra Scientific, Tokyo, 1994), pp. 26-33.
    • (1991) IEEE Trans. Instrum. Meas. , vol.40 , pp. 584
    • D'Addario, L.R.1
  • 7
    • 0002320459 scopus 로고
    • T. Sasao, S. Manabe, O. Kameya, M. Inoue, Eds. Terra Scientific, Tokyo
    • L. R. D'Addario, IEEE Trans. Instrum. Meas. 40, 584 (1991); N. Kawaguchi et al., in VLBI Technology: Progress and Future Observational Possibilities, T. Sasao, S. Manabe, O. Kameya, M. Inoue, Eds. (Terra Scientific, Tokyo, 1994), pp. 26-33.
    • (1994) VLBI Technology: Progress and Future Observational Possibilities , pp. 26-33
    • Kawaguchi, N.1
  • 8
    • 3543122016 scopus 로고    scopus 로고
    • note
    • The Usuda tracking station is funded and operated by the Institute of Space and Astronautical Science. The other four tracking stations are funded by NASA, with the Green Bank tracking station being operated by NRAO and the remainder by the Jet Propulsion Laboratory.
  • 9
    • 3543104538 scopus 로고    scopus 로고
    • Americal Astronautical Society/Goddard Space Flight Center, Greenbelt, MD, 11 to 15 May (Univelt, San Diego, CA, in press)
    • T.-H. You, J. Ellis, N. Mottinger, AAS/GSFC International Symposium on Space Flight Dynamics, Americal Astronautical Society/Goddard Space Flight Center, Greenbelt, MD, 11 to 15 May 1998 (Univelt, San Diego, CA, in press).
    • (1998) AAS/GSFC International Symposium on Space Flight Dynamics
    • You, T.-H.1    Ellis, J.2    Mottinger, N.3
  • 11
    • 3543090580 scopus 로고    scopus 로고
    • note
    • -1 (where 1 Mpc = 3.26 million light-years) and a cosmological deceleration constant of 0.5.
  • 13
    • 3543091724 scopus 로고    scopus 로고
    • note
    • -1/2, and φ is the angle between the line of sight and the radio jet axis.
  • 19
    • 3543110471 scopus 로고    scopus 로고
    • in preparation
    • E. B. Fomalont et al., in preparation.
    • Fomalont, E.B.1
  • 29
    • 3543112815 scopus 로고    scopus 로고
    • in preparation
    • L. I. Gurvits et al., in preparation.
    • Gurvits, L.I.1
  • 32
    • 0001339410 scopus 로고
    • T. J. Pearson and A. C. S. Readhead, Astrophys. J. 328, 114 (1988); A. L. Fey, A. W. Clegg, E. B. Fomalont, Astrophys. J. Suppl. Ser. 105, 299 (1996).
    • (1988) Astrophys. J. , vol.328 , pp. 114
    • Pearson, T.J.1    Readhead, A.C.S.2
  • 35
    • 0000838102 scopus 로고
    • R. P. Linfield et al., Astrophys. J. 336, 1105 (1989); R. P. Linfield et al., ibid. 358, 350 (1990).
    • (1989) Astrophys. J. , vol.336 , pp. 1105
    • Linfield, R.P.1
  • 36
    • 4243729776 scopus 로고
    • R. P. Linfield et al., Astrophys. J. 336, 1105 (1989); R. P. Linfield et al., ibid. 358, 350 (1990).
    • (1990) Astrophys. J. , vol.358 , pp. 350
    • Linfield, R.P.1
  • 38
    • 3543074239 scopus 로고    scopus 로고
    • note
    • We thank the many individuals, organizations, and institutions that have made this mission possible and have contributed toward its success. In particular, the support of M. Oda and T. Nishimura in the early stages of the mission is gratefully acknowledged.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.