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A VLBI (Very Long Baseline Interferometer) observation of pulsar B0329+54 was carried out with the CVN (Chinese VLBI Network) in February 2015. It is the first time for the CVN to observe the pulsar B0329+54 in the S/X dual frequency bands. The observation was performed in the phase referencing mode. The observational data, including 16 channels of 16MHz bandwidth, were collected by the CDAS (Chinese...
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