Timing Observations of PSR B1534+12

Details Timing Observations of PSR B1534+12 Timing Observations of PSR B1534+12

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...199.1705s&link_type=abstract

American Astronomical Society, 199th AAS Meeting, #17.05; Bulletin of the American Astronomical Society, Vol. 33, p.1335

Astronomy and Astrophysics

Astronomy

Scientific paper

We present radio timing observations of the double-neutron-star binary PSR B1534+12. The total time span of the data is now more than 11 years. Five "post-Keplerian" relativistic orbital parameters are measured, resulting in high-precision tests of the predictions of general relativity. The addition of four years of high-quality coherently dedispersed data from the upgraded Arecibo telescope has resulted in a measurement of the orbital period derivative three times more precise than that achieved before the upgrade was completed. This yields a refined estimate of the distance to the pulsar using kinematic corrections to the observed orbital period derivative.

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