Timing analysis of Geminga with a phase cross-correlation method

Details Timing analysis of Geminga with a phase cross-correlation method Timing analysis of Geminga with a phase cross-correlation method

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cha%26a..22...35z&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 22, Issue 1, p. 35-40.

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

Taking advantage of the stability of the spin and frequency variations of Geminga, we have made a phase-correlation analysis of egret data from four widely sepataed observing periods. The results are similar to those obtained from period folding over a much longer data set, thus demonstrating the effectiveness of the phase-correlation method in the derivation of the timing parameters of stable γ-ray pulsars.

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