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Timing Observations of PSR B1937+21 at CRL
Published online by Cambridge University Press: 19 July 2016
Abstract
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 × 10−14 over the data span of 6.5 years using Kashima data combined with Parkes data.
- Type
- Part 10: Radio Pulsar Timing
- Information
- Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 437 - 438
- Copyright
- Copyright © Astronomical Society of the Pacific 2004