Timing Observations of PSR B1937+21 at CRL
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.
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Veröffentlicht in: | Symposium - International Astronomical Union 2004, Vol.218, p.437-438 |
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Hauptverfasser: | , , , , , |
Format: | Artikel |
Sprache: | eng |
Online-Zugang: | Volltext |
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Zusammenfassung: | 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. |
---|---|
ISSN: | 0074-1809 |
DOI: | 10.1017/S0074180900181598 |