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- W169492781 abstract "Abstract : We implement a new parabolic antenna for VLBI experiments in Kashima Space Communication Center, CRL. The receivers for 330M, 610M, 1.5G, 2.2G, 5G, 8.3G, 10G, 15G, 22G, and 43GHz (with a receiver for 49GHz also under preparation) enable us to carry out not only VLBI but also various other tasks. CRL is now making a system for observing milli-second pulsars such as PSR1937 + 21, which are well-known for their extreme stability. We plan to obtain very precise timings of pulses by compensating the dispersion in frequency domain with high-speed and wideband sampling. We also plan to survey other highly stable pulsars using the VLBI backend. This report outlines the status quo of pulsar observation in CRL, and VLBI of pulsars." @default.
- W169492781 created "2016-06-24" @default.
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- W169492781 date "1989-11-30" @default.
- W169492781 modified "2023-10-14" @default.
- W169492781 title "Observation Plan of High-stable Pulsars in CRL" @default.
- W169492781 hasPublicationYear "1989" @default.
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