• Cooper, B. F. C. (1970), Correlators with two-bit quantization, Astron. J. Phys., 23, 521527.
  • Kiuchi, H., and T. Kondo (1996), The wavefront clock technique applied to the current VLBI systems, Publ. Astron. Soc. Jpn., 48, 137146.
  • Kiuchi, H., J. Amagai, S. Hama, and M. Imae (1997), K-4 VLBI data-acquisition system, Publ. Astron. Soc. Jpn., 49, 699708.
  • Kiuchi, H., M. Imae, T. Kondo, M. Sekido, S. Hama, T. Hoshino, H. Uose, and T. Yamamoto (2000), Real-time VLBI system using ATM network, IEEE Trans. Geosci. Remote Sens., 38, 12901297.
  • Koyama, Y., N. Kurihara, T. Kondo, M. Sekido, Y. Takahashi, H. Kiuchi, and K. Heki (1998), Automated geodetic very long baseline interferometry observation and data analysis system, Earth Planets Space, 50, 709722.
  • Koyama, Y., J. Nakajima, M. Sekido, and T. Kondo (2000), Geodetic VLBI experiments using giga-bit VLBI system, in IVS CRL TDC News 17, pp. 1517, Int. VLBI Serv. for Geod. and Astrometry, Greenbelt, Md.
  • Rogers, A. E. E. (1970), Very-long-baseline interferometry with large effective bandwidth for phase-delay measurements, Radio Sci., 5, 12391247.
  • Rogers, A. E. E., and J. M. Moran (1981), Coherence limits for very-long-baseline interferometry, IEEE Trans. Instrum. Meas., 30, 283286.
  • Rogers, A. E. E., et al. (1983), Very-long-baseline radio interferometry: The Mark-III system for geodesy, astrometry, and aperture synthesis, Science, 219, 5154.
  • Rogers, A. E. E., A. T. Moffet, D. C. Backer, and J. M. Moran (1984), Coherence limits in VLBI observation at 3-millimeter wavelength, Radio Sci., 19, 15521560.
  • Whitney, A. R. (2000), How do VLBI correlators work? paper presented at 2000 General Meeting, Int. VLBI Serv. for Geod. and Astrometry, Kötzting, Germany.
  • Whitney, A. R., et al. (2004), Mark 4 VLBI correlator: Architecture and algorithms, Radio Sci., 39, RS1007, doi:10.1029/2002RS002820.