Timing Observations of PSR B1937+21 at CRL

Y. Hanado, Y. Shibuya, F. Nakagawa, M. Sekido, M. Hosokawa, M. Imae
2004 Symposium - International astronomical union  
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