Table 3.
Timing solution for PSR J1803−3002C found by DRACULA.
| Pulsar | J1803−3002C |
|---|---|
| RA (J2000) | 18h03m35 221(4) |
| Dec (J2000) |
 (1) |
| Spin frequency, f (s−1) | 171.22104938954(5) |
| 1st spin frequency derivative, ḟ (Hz s−1) | −2.044(1) × 10−14 |
| Reference epoch (MJD) | 59 206.206359 |
| Start of timing data (MJD) | 58 699.375 |
| End of timing data (MJD) | 59 625.230 |
| Dispersion measure (pc cm−3) | 193.88 |
| Number of ToAs | 59 |
| Weighted rms residual (μs) | 103.325 |
| Derived parameters | |
| Spin period, P (s) | 0.00584040340(2) |
| 1st spin period derivative, Ṗ (s s−1) | 6.973(4) × 10−19 |
| Surface magnetic field, B0, (G) | 2.04 × 109 |
| Characteristic age, τc (Myr) | 133 |
Notes. The timing solution is derived from the timing of the observed ToA with DRACULA closest to the position of the pulsar found by SEEKAT. The time units are TDB, the adopted terrestrial time standard is TT(TAI), and the Solar System ephemeris used is JPL DE421 (Folkner et al. 2009). The numbers in parentheses represent 1σ uncertainties in the last digit.
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