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We have re-analyzed the stability of pulse arrival times from pulsars and white dwarfs using several analysis tools for measuring the noise characteristics of sampled time and frequency data.
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Parker, T., data received 13 May 2009 from Tom Parker at NIST, who did the comparison from data available in Circular T www.bipm.org/jsp/en/TimeFtp.jsp?TypePub=publication#TAIPubFormPubli2 and on the BIPM website www.bipm.org/en/scientific/tai/ ; See Parker, T.E., Metrologia
2010
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Parker, T., email communication on 9 February 2010. At NIST they are able to calibrate the Cs 5071A clocks against the NIST-F1 standard to an accuracy better than 1 × 10 − 15 1\times 10^{-15} hence the accuracy evaluation for the particular cesium standard used here was estimated to be 2 × 10 − 15 2\times 10^{-15} . This is much better than the accuracy quoted by the manufacturer, without such calibration, usually around 5 × 10 − 13 5\times 10^{-13}
2010
Closest in time.
2010
Closest in time.