Table 2.1
(continued)
B1820−11
357.76199(5)
200.6720(12)
47260.5438(4)
0.794608(7)
99.1719(11)
7.4E−5(130) –
–
–
–
J1829+2456
1.176027941(16)
7.238(2)
52848.579775(3)
0.1391412(19)
229.92(2)
0.2919(16)
–
–
–
–
B1855+09
12.3271713831(3)
9.2307819(9)
46432.781(3)
2.170E−5(4)
276.47(7)
–
–
–
0.9987(6)
0.27(3)
J1903+0327
95.174118753(14)
105.5934643(5) 55015.58158859(4)
0.436678409(3) 141.6524786(6) 0.0002400(2) –
–
0.9760(15) 1.03(3)
J1906+0746
0.16599304683(11) 1.4199620(18) 54288.9298810(2)
0.0853028(6)
76.3320(6)
7.5841(5)
−0.56E−12(3)
0.000470(5)
–
–
J1909−3744 b
1.533449474406(13) 1.89799118(4) 53631.39(4)
1.14E−7(10)
156(8)
–
5.03E−13(6)
–
–
0.2067(19)
J1910−5959A a
0.83711347691(3)
1.2060418(7)
51919.206480057(55) –
–
–
–
–
0.9997(3)
0.180(18)
J1913+1102
0.206252330(6)
1.754623(8)
56241.029660(5)
0.08954(1)
264.279(9)
5.632(18)
–
–
–
–
B1913+16
0.322997448918(3) 2.341782(3)
52144.90097849(3)
0.6171340(4)
292.54450(8)
4.226585(4)
−2.423E−12(1) 4.307E−06(4) –
–
J1930−1852
45.0600007(5)
86.890277(7)
56526.642330(3)
0.39886340(17) 292.07706(2)
0.00078(4)
–
–
–
–
J1946+3417
27.01994783(5)
13.8690718(5) 56819.4529124(10)
0.134495389(17) 223.364186(14) 0.001363(9) –
–
–
–
J1950+2414
22.1913727(10)
14.2199738(11) 55846.0226219(15)
0.07981158(12) 274.4155(3)
0.0020(3)
–
–
–
–
J1957+2516
0.2381447210(7)
0.283349(6)
–
2.8E−5(26)
45(52)
–
12E−12(2)
–
–
–
B1957+20 b
0.3819666069(8)
0.0892253(6)
48196.0635242(6)
0.00000(4)
–
–
1.47E−11(8)
–
–
–
J2019+2425
76.51163479(2)
38.7676297(8) 50054.6439021(40000) 0.00011109(4)
159.03(2)
–
−3E−11(6)
–
–
–
J2032+4127
16835(835)
13580(6490)
58061(9)
0.964(30)
34(18)
–
–
–
–
15.0(28)
J2051−0827
0.09911025490(4)
0.0450720(3)
–
5.1E−5(10)
36(11)
–
−5.9E−12(3)
–
–
–
J2129−0429 b
0.6352274131(3)
1.855(42)
–
–
–
–
–
–
–
0.44(4)
B2127+11C a
0.33528204828(5)
2.51845(6)
50000.0643452(3)
0.681395(2)
345.3069(5)
4.4644(1)
−3.96E−12(5)
0.00478(4)
–
–
J2129−5721
6.6254930923(13)
3.50056678(14) –
1.219E−5(8)
197.1(4)
–
7.9E−13(36)
–
–
–
J2215+5135
0.172502105(8)
0.468141(13)
–
1.1E−5(29)
68(92)
–
−439E−12(2)
–
–
0.23
J2222−0137
2.44576469(13)
10.8480239(6) 56001.38381(8)
3.80967E−4(30) 119.900(11)
0.1033(29)
0.20E−12(9)
–
0.99659(30) 1.293(25)
B2303+46
12.33954454(17)
32.6878(3)
47452.560747(17)
0.658369(9)
35.0776(7)
0.0099(2)
–
–
–
–
J2339−0533
0.19309840181(4)
0.611656(4)
–
0.0002102(5)
177(3)
–
−2.226E−20(19) –
0.87
0.32
Left to right: pulsar name, orbital period, projected semimajor axis, epoch of periastron, eccentricity, longitude of periastron, periastron advance, orbital decay, time-dilation and gravitational red-shift
parameter, sine of the inclination of the orbit (equal, in general relativity, to the shape parameter of the Shapiro delay) and mass of the companion star (equal, in general relativity, to the range parameter
of the Shapiro delay). Note that for the globular cluster pulsars (denoted by a
), some of the parameters can be severely affected by the cluster potential well and not be directly related to relativistic gravity.
More in general pulsars with positive derivative of the orbital period are certainly affected by non-relativistic effects (mass losses, or kinematic effects due to the influence of the Galactic potential and/or
proper motion of the pulsar); pulsars with positive ˙
Pb
are hence marked with b
. Data extracted from PSRcat v1.57. http://www.atnf.csiro.au/research/pulsar/psrcat/ [1]
(continued)
B1820−11
357.76199(5)
200.6720(12)
47260.5438(4)
0.794608(7)
99.1719(11)
7.4E−5(130) –
–
–
–
J1829+2456
1.176027941(16)
7.238(2)
52848.579775(3)
0.1391412(19)
229.92(2)
0.2919(16)
–
–
–
–
B1855+09
12.3271713831(3)
9.2307819(9)
46432.781(3)
2.170E−5(4)
276.47(7)
–
–
–
0.9987(6)
0.27(3)
J1903+0327
95.174118753(14)
105.5934643(5) 55015.58158859(4)
0.436678409(3) 141.6524786(6) 0.0002400(2) –
–
0.9760(15) 1.03(3)
J1906+0746
0.16599304683(11) 1.4199620(18) 54288.9298810(2)
0.0853028(6)
76.3320(6)
7.5841(5)
−0.56E−12(3)
0.000470(5)
–
–
J1909−3744 b
1.533449474406(13) 1.89799118(4) 53631.39(4)
1.14E−7(10)
156(8)
–
5.03E−13(6)
–
–
0.2067(19)
J1910−5959A a
0.83711347691(3)
1.2060418(7)
51919.206480057(55) –
–
–
–
–
0.9997(3)
0.180(18)
J1913+1102
0.206252330(6)
1.754623(8)
56241.029660(5)
0.08954(1)
264.279(9)
5.632(18)
–
–
–
–
B1913+16
0.322997448918(3) 2.341782(3)
52144.90097849(3)
0.6171340(4)
292.54450(8)
4.226585(4)
−2.423E−12(1) 4.307E−06(4) –
–
J1930−1852
45.0600007(5)
86.890277(7)
56526.642330(3)
0.39886340(17) 292.07706(2)
0.00078(4)
–
–
–
–
J1946+3417
27.01994783(5)
13.8690718(5) 56819.4529124(10)
0.134495389(17) 223.364186(14) 0.001363(9) –
–
–
–
J1950+2414
22.1913727(10)
14.2199738(11) 55846.0226219(15)
0.07981158(12) 274.4155(3)
0.0020(3)
–
–
–
–
J1957+2516
0.2381447210(7)
0.283349(6)
–
2.8E−5(26)
45(52)
–
12E−12(2)
–
–
–
B1957+20 b
0.3819666069(8)
0.0892253(6)
48196.0635242(6)
0.00000(4)
–
–
1.47E−11(8)
–
–
–
J2019+2425
76.51163479(2)
38.7676297(8) 50054.6439021(40000) 0.00011109(4)
159.03(2)
–
−3E−11(6)
–
–
–
J2032+4127
16835(835)
13580(6490)
58061(9)
0.964(30)
34(18)
–
–
–
–
15.0(28)
J2051−0827
0.09911025490(4)
0.0450720(3)
–
5.1E−5(10)
36(11)
–
−5.9E−12(3)
–
–
–
J2129−0429 b
0.6352274131(3)
1.855(42)
–
–
–
–
–
–
–
0.44(4)
B2127+11C a
0.33528204828(5)
2.51845(6)
50000.0643452(3)
0.681395(2)
345.3069(5)
4.4644(1)
−3.96E−12(5)
0.00478(4)
–
–
J2129−5721
6.6254930923(13)
3.50056678(14) –
1.219E−5(8)
197.1(4)
–
7.9E−13(36)
–
–
–
J2215+5135
0.172502105(8)
0.468141(13)
–
1.1E−5(29)
68(92)
–
−439E−12(2)
–
–
0.23
J2222−0137
2.44576469(13)
10.8480239(6) 56001.38381(8)
3.80967E−4(30) 119.900(11)
0.1033(29)
0.20E−12(9)
–
0.99659(30) 1.293(25)
B2303+46
12.33954454(17)
32.6878(3)
47452.560747(17)
0.658369(9)
35.0776(7)
0.0099(2)
–
–
–
–
J2339−0533
0.19309840181(4)
0.611656(4)
–
0.0002102(5)
177(3)
–
−2.226E−20(19) –
0.87
0.32
Left to right: pulsar name, orbital period, projected semimajor axis, epoch of periastron, eccentricity, longitude of periastron, periastron advance, orbital decay, time-dilation and gravitational red-shift
parameter, sine of the inclination of the orbit (equal, in general relativity, to the shape parameter of the Shapiro delay) and mass of the companion star (equal, in general relativity, to the range parameter
of the Shapiro delay). Note that for the globular cluster pulsars (denoted by a
), some of the parameters can be severely affected by the cluster potential well and not be directly related to relativistic gravity.
More in general pulsars with positive derivative of the orbital period are certainly affected by non-relativistic effects (mass losses, or kinematic effects due to the influence of the Galactic potential and/or
proper motion of the pulsar); pulsars with positive ˙
Pb
are hence marked with b
. Data extracted from PSRcat v1.57. http://www.atnf.csiro.au/research/pulsar/psrcat/ [1]