1-Gbps VLBI, The First Detection of Fringes |
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Authors: | J Nakajima Y Koyama M Sekido N Kurihara T Kondo M Kimura N Kawaguchi |
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Institution: | (1) Communications Research Laboratory, Kashima Space Research Center, 893 Hirai, Kashima-city Ibaraki, 314-0012, Japan;(2) Communications Research Laboratory, Kashima Space Research Center, 893 Hirai, Kashima-city Ibaraki, 314-0012, Japan;(3) Department of Astronomy, University of Tokyo, Tokyo, 113-003, Japan;(4) National Astronomical Observatory Osawa Mitaka, Tokyo, 181-8588, Japan |
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Abstract: | We report on the detection of VLBI fringes from quasars by a new VLBI system operating at 1 Gbps (1024 Mbits-per-second). Newly developed 1024 Msps (mega sample-per-second) AD samplers and 1024 Mbps recorders were used for the observations. A correlator with external buffers was used for the 1024 Mbps correlation processing of the tapes data.Our new VLBI system enabled 1024 Mbps VLBI, and this allowed the sampling of a 512 MHz bandwidth from a radio telescope receiver. This is the highest sampling speed ever used for VLBI, and the widest bandwidth used for VLBI observation. Initial sensitivity as evaluated by SNR comparison with earlier VLBI systems produced results to matched the expanded bandwidth. In our first observations, simultaneous optical fibre linked real-time VLBI observations were made to check the validity of data and precisely detemine the clock offsets among the radio telescopes. |
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Keywords: | fringe detection high sensitivity quasar VLBI |
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