Table B.1
Measured timing model parameters for PSRs J0030+0451, J0613–0200, J0751 + 1807 and J0900–3144. Here the epoch of spin frequency, sky position and DM are all set to MJD 55000. The definitions of the proper motion terms are: 
, 
, 
, 
. The components in the red-noise model used in the Bayesian analysis to obtain the timing solution are shown in the last row, where RN, DM, SV stand for achromatic red noise, chromatic red noise for DM variation, and scattering variation, respectively. All of the above apply to all tables in this section.
| Pulsar Jname | J0030+0451 | J0613–0200 | J0751+1807 | J0900–3144 |
|---|---|---|---|---|
| Right ascension, α (J2000) | — | 06:13:43.975688(1) | 07:51:09.155329(6) | 09:00:43.953105(8) |
| Declination, δ (J2000) | — | −02:00:47.22541(4) | 18:07:38.4858(5) | −31:44:30.8950(1) |
| Ecliptic longitude λ (deg) | 8.910356334(10) | — | — | — |
| Ecliptic latitude β (deg) | 1.4456958(4) | — | — | — |
| Spin frequency, v (Hz) | 205.530695938456(2) | 326.6005620234831(4) | 287.457853995106(1) | 90.011841919354(1) |
Spin frequency derivative,  (s−2) |
−4.2977(1) × 10−16 | −1.023017(8) × 10−15 | −6.43455(6) × 10−16 | −3.96012(7) × 10−16 |
| DM (cm−3 pc) | 4.331(1) | 38.7759(7) | 30.2457(8) | 75.691(2) |
| DM1 (cm−3 pc yr−1) | 0.0002(1) | −8(2) × 10−5 | −0.00046(7) | 0.0009(5) |
| DM2 (cm−3 pc yr−2) | −2(2) × 10−5 | −1.8(6) × 10−5 | 10(20) × 10−6 | −0.00019(9) |
| Proper motion in α, µα (mas yr−1) | — | 1.837(2) | −2.70(1) | −1.03(2) |
| Proper motion in δ, µδ (mas yr−1) | — | −10.359(6) | −13.27(7) | 1.99(2) |
| Proper motion in λ, µλ (mas yr−1) | −5.523(5) | — | — | — |
| Proper motion in β, µβ (mas yr−1) | 3.1(2) | — | — | — |
| Parallax, ϖ (mas) | 3.09(6) | 1.00(5) | 0.85(4) | — |
| Binary model | — | T2 | T2 | T2 |
| Orbital period, Pb (d) | — | 1.198512575192(8) | 0.263144270793(3) | 18.7376360584(1) |
| Projected semi-major axis, x (s) | — | 1.09144411(2) | 0.3966135(1) | 17.24880996(4) |
| Epoch of ascending node (MJD), Tasc | — | 53113.79635421(1) | 51800.21586830(2) | 52678.63028838(3) |
 component of the eccentricity, κ |
— | 4.05(4)×10−6 | 2.9(1) × 10−6 | 9.884(5)×10−6 |
 component of the eccentricity, η |
— | 3.50(4)×10−6 | 3(1)×10−7 | 3.484(4)×10−6 |
| Orbital period derivative, Ṗb | — | 3.5(2)×10−14 | −3.50(5) × 10−14 | — |
Derivative of x,  |
— | — | 2(2)×10−16 | — |
| 3rd harmonic of Shapiro delay, h3 (s) | — | 2.6(2)×10−7 | 1.9(2)×10−7 | — |
| 4th harmonic of Shapiro delay, h4 (s) | — | — | 4(23)×10−9 | — |
| Ratio of harmonics amplitude, ζ | — | 0.69(4) | — | — |
| Noise model | RN | RN, DM | DM | RN, DM |
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