Precision Pulsar Timing

Details Precision Pulsar Timing Precision Pulsar Timing

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atnf.prop..560b&link_type=abstract

ATNF proposal P140, Semester: October, 2006

Mathematics

Logic

Stellar, Galactic, Parkes

Scientific paper

It is the aim of this proposal to investigate the theoretical limits of pulsar timing. This term, we are reducing the number of sources from 13 to 3 and increasing our integration times. By maintaining our monthly observations we will be sensitive to long-term variations, and an intensive month-long campaign will help determine if millisecond pulsars can be integrated down to ~10ns errors with the Parkes radio telescope. Such errors would permit very stringent limits on a cosmological background of gravitational waves with existing instrumentation prior to the construction of the SKA.

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