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  1. SAFe Program
  2. SP-1480

Prepare SDP/SRC for pulsars in relativistic binary systems

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      PSRCHIVE correctly predicts the pulse phase of highly accelerated pulsars by utilising Tempo2’s 2D polynomial phase-predictors

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      PSRCHIVE correctly predicts the pulse phase of highly accelerated pulsars by utilising Tempo2’s 2D polynomial phase-predictors
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      Given: pulsar ephemeris is installed into PSRFITS archive

      When: PSRCHIVE applies timing corrections to the times of arrival, based on that ephemeris

      Then: the pulse phase is predicted correctly, i.e. the pulse phase does not systematically drift as a function of frequency/time by more than X%. 

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        • Given: pulsar ephemeris is installed into PSRFITS archive • When: PSRCHIVE applies timing corrections to the times of arrival, based on that ephemeris • Then: the pulse phase is predicted correctly, i.e. the pulse phase does not systematically drift as a function of frequency/time by more than X%. 
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    • PI22 - UNCOVERED

    Description

      Update PSRCHIVE and DSPSR to utilise the two-dimensional polynomial phase-predictors of TEMPO2 for correctly predicting the pulse phase of highly accelerated pulsars in highly relativistic binary systems.

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              A.Noutsos Noutsos, Aristeidis
              A.Griffin Griffin, Anthony
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                  Structure Helper Panel