Pulsar name .......................................... | J1721-2457 | J1745-0952 | J1810-2005 | J1918-0642 |
Fit and data-set | ||||
MJD range ............................................ | 52 076-54 799 | 52 076-54 776 | 50 757-54 796 | 52 094-54 814 |
Number of TOAs .................................. | 120 | 113 | 491 | 152 |
Rms timing residual (![]() |
31.9 | 20.8 | 270.7 | 2.6 |
Weighted fit ......................................... | Y | Y | Y | Y |
Reduced ![]() |
1.05 | 1.02 | 1.01 | 1.04 |
Measured quantities | ||||
Right ascension, ![]() |
17![]() ![]() ![]() |
17![]() ![]() ![]() |
18![]() ![]() ![]() |
19![]() ![]() ![]() |
Declination, ![]() |
-24°57![]() ![]() |
-09$^$52![]() ![]() |
-20$^$05![]() ![]() |
-06$^$42![]() ![]() |
Pulse frequency, ![]() |
285.989343507338(15) | 51.609431233273(5) | 30.467142155106(7) | 130.7895141841235(6) |
First derivative of pulse frequency, ![]() |
-
![]() |
-
![]() |
-
![]() |
-
![]() |
Dispersion measure, DM (cm-3pc) ...... | 48.34(3) | 64.27(9) | 241.0(3) | 26.554(10) |
Proper motion in RA,
![]() |
1.8(1.8) | -21.2(1.1) | 0(2) | -7.20(10) |
Proper motion in Dec,
![]() |
-14(25) | 11(5) | 17(37) | -5.7(3) |
Binary ..................................................... | - | ELL1 | ELL1 | ELL1 |
Orbital period, ![]() |
4.943453386(12) | 15.01201911(4) | 10.9131777486(12) | |
Projected semi-major axis of orbit, x (lt-s) | 2.378599(5) | 11.977880(18) | 8.3504716(4) | |
TASC (MJD) ........................................... | 53198.621445(3) | 53195.528458(4) | 53402.53135510(8) | |
EPS1 (
![]() |
0.000009(3) | 0.000009(3) | -0.00001244(9) | |
EPS2 (
![]() |
-0.000004(4) | -0.000017(3) | -0.00001555(9) | |
Set quantities | ||||
Epoch of frequency determination (MJD) | 53400.0 | 53200.0 | 53200.0 | 53400.0 |
Epoch of position determination (MJD)... | 53400.0 | 53200.0 | 53200.0 | 53400.0 |
Epoch of DM determination (MJD) ......... | 53400.0 | 53200.0 | 53200.0 | 53400.0 |
Derived quantities | ||||
Orbital eccentricity,
![]() |
- |
![]() |
![]() |
![]() |
Omega, ![]() ![]() ![]() |
- | 114(28) | 152(12) | 218.6(4) |
Characteristic age, (Gyr) ........................ | 10.0 | 3.3 | 3.5 | 4.7 |
Surface magnetic field strength, (108G).. | 1.4 | 13.5 | 22.4 | 4.4 |
Distanceb, (kpc) ...................................... | 1.3(2) | 1.8(3) | 4.0(4) | 1.23(13) |
Spin period (ms) ..................................... | 3.49663 | 19.3763 | 32.8222 | 7.64587 |
Spin period derivative ............................ |
![]() |
![]() |
![]() |
![]() |
Mass function, (![]() |
- | 0.000591270(4) | 0.00818737(4) | 0.0052494438(8) |
Minimum companion mass, (![]() |
- | 0.11 | 0.28 | 0.24 |
Total proper motion,
![]() |
15(25) | 24(2) | 17(37) | 9.2(2) |
Transverse velocity, ![]() |
<140c | 200(50) | <400c | 54(7) |
Assumptions | ||||
Clock correction procedure ................... | TT(TAI) | |||
Solar system ephemeris model .............. | DE405 | |||
Model version number ........................... | 5.00 |
Notes. Figures in parentheses are the nominal 1
TEMPO2
uncertainties in the least-significant digits quoted.
(a) Before combining the data sets from the
different observatories, the errors on the TOAs were scaled with a
constant factor to have each individual data set return a reduced
.
(b) The DM distances are estimated from the Cordes & Lazio (2002) model. (c) Velocity limits from Eq. (1).
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