Searching for pulsed emission from XTE J0929–314 at high radio frequencies

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Table 2:

Parameters for the pulsar candidate with the highest *S/N* shown in Fig. 1.
Signal to noise ratio, S/N	5.87
Dispersion Measure, DM (pc cm^-3)	5.51
Orbital period, $P_{\rm orb}$ (s)	2614.74575
Projected semi-major axis, $a~\sin i$ (lt-ms)	6.290(9)
Spin frequency, $\nu_{\rm S}$ (Hz)	185.105259
Ascending node passage, T₀ (MJD)	52 405.48676(1)

Source LaTeX | All tables | In the text

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