WebbAfter the two telescopes were phased as a twofold larger single telescope, the mean signal-to-noise ratio (S/N) of the 6.7 GHz methanol masers observed by the phased … WebbThis paper presents new results of a water maser survey of late-type stellar objects at 22.235GHz with the Kashima 34-m radio telescope. We have detected 179 out of 643 observed sources, including 32 new detections.
A broadband VLBI system using transportable stations for geodesy …
Webb120 Sekido and Kawai Table 1 Antenna performance parameters of the Kashima 34-m telescope. Receiver Pol. Frequency SEFD [Jy] L-band RHCP/LHCP 1405-1440MHz, 1600-1720MHz ∼ 500 S-band RHCP/LHCP 2210-2350MHz ∼ 250 X-band RHCP/LHCP 8180-9080MHz ∼ 370 Wideband V-Linear Pol. 6.4-15GHz ∼ 1000 – 2000 K-band … WebbPDF The Kashima 34-m radio telescope has been continuously operated and maintained by the National Institute of Information and Communications Technology (NICT) as a facility of the Kashima Space Technology Center (KSTC) in Japan. This brief report summarizes the status of this telescope, the staff, and activities during 2012. quick repair for outlook
Development of the Phase-up Technology of the Radio Telescopes …
WebbTechnology (NICT) Kashima 34 m, Gifu 11 m (only the first epoch) telescopes. VERA only was used for the annual parallax measurement, while VERA along with NRO, and … Webb29 maj 2012 · Kashima 34 m antenna is located at south of Ibaraki prefecture which are near Tokyo. This antenna is one of first astronomical VLBI station in Japan. The antenna is operated by the National Institute of Information and Communications Technology (NICT). Kashima is famous for a home town of Japanese professional football team, Kashima … WebbIn addition, Mizusawa VLBI Observatory collaborates with other antennas and universities: the Yamaguchi 32-m antenna, Takahagi and Hitachi 32-m antennas, Gifu University’s … shipwreck in the little mermaid