Key Stone Project

KSP VLBI Data / Flux Densitiy of Observed Radio Sources

Flux densities evaluated from the correlated amplitudes obtained from the KSP Correlator at Koganei can be viewed in this page. Both X-band and S-band results are displayed together. The KASHIM11-MIURA baseline is used before May 5, 1999, and KASHIM11-TATEYAMA baseline after that date. See a paper submitted to the Radio Science for details.

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Last Update: June 2, 2000

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