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The invariant interval

The high S/N pulsars the invariant interval can be used to mitigate the effects of polarisation calibration errors.

PSRCHIVE

To convert an observation to the invariant interval use:

 pam -I 

Notes:

  • Always take the invariant interval before frequency and/or time scrunching.
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Page last modified on June 21, 2007, at 10:35 AM