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Timing Observations of PSR B1937+21 at CRL
2004
Symposium - International astronomical union
Preserved Fulltext
Pulsar parameters of PSR B1937+21 acquired from observations at the Kashima 34-m antenna over five years are consistent with published reports. The frequency stability is 2 × 10−14over the data span of 6.5 years using Kashima data combined with Parkes data.
doi:10.1017/s0074180900181598
fatcat:tqchei7wv5bvxctqnbnrupakta