Table 1
Main properties of the MSPs in this study.
| Pulsar | l | b | P | Ṗ obs | d | Ṗ int | Ė int | h | L γ | η |
| (°) | (°) | (ms) | (10-20) | (kpc) | (10-20) | (1033 erg s-1) | (10-11 erg cm-2 s-1) | (1033 erg s-1) | % | |
|
|
||||||||||
| J0034−0534 | 111.49 | −68.07 | 1.877 | 0.49762(9) | 0.54(11)† | 0.489(12) | 29.2(7) | 1.80(10) | 0.6(3) | 2(1) |
| J0340+4130 | 153.78 | −11.02 | 3.299 | 0.70486(15) | 1.73(30)† | 0.661(5) | 7.27(6) | 2.22(13) | 8(3) | 110(40) |
| J0610−2100 | 227.75 | −18.18 | 3.861 | 1.23317(4) | 3.5(10)† | 0.01(34) | 0.1(23) | 1.15(11) | 17(10) | – |
| J0614−3329 | 240.50 | −21.83 | 3.149 | 1.74169(8) | 1.9(4)† | 1.7616(15) | 22.279(19) | 11.10(24) | 48(22) | 220(100) |
| J0740+6620 | 149.73 | 29.60 | 2.886 | 1.23(6) | 0.68(10)† | 0.73(16) | 12.0(26) | 0.36(23)∥ | 0.2(1) | 2(1) |
| J0751+1807 | 202.73 | 21.09 | 3.479 | 0.778802(9) | 1.51(35) | 0.53(6) | 5.0(5) | 1.30(10) | 4(2) | 70(40) |
| J0931−1902 | 251.00 | 23.05 | 4.638 | 0.3612(17) | 1.88(51)† | 0.37(3) | 1.5(1) | 0.67(22)∥ | 2.8(18) | 200(130) |
| J1024−0719 | 251.70 | 40.52 | 5.162 | 1.855242(27) | 1.13(18) | −3.1(8) | −8.9(23) | 0.36(5) | 0.5(2) | – |
| J1231−1411 | 295.53 | 48.39 | 3.684 | 2.26235(11) | 0.44(5)† | 0.77(17) | 6.1(14) | 10.30(21) | 2.4(5) | 39(18) |
| J1455−3330 | 330.72 | 22.56 | 7.987 | 2.43072(5) | 1.01(22) | 2.330(28) | 1.806(22) | 0.42(15)∥ | 0.5(3) | 28(16) |
| J1614−2230 | 352.64 | 20.19 | 3.151 | 0.962464(11) | 0.77(5) | 0.34(5) | 4.3(6) | 2.33(15) | 1.6(2) | 38(10) |
| J1730−2304 | 3.14 | 6.02 | 8.123 | 2.018340(28) | 0.84(19) | 1.15(29) | 0.84(22) | 1.0(5)∥ | 1.1(10) | 130(130) |
| J1741+1351 | 37.89 | 21.64 | 3.747 | 3.02163(6) | 1.08(5)⋆ | 2.909(7) | 21.82(5) | 0.57(11) | 0.8(2) | 4(1) |
| J1811−2405 | 7.07 | −2.56 | 2.661 | 1.33708(7) | 1.8(5)† | 1.20(11) | 25.1(23) | 1.4(8) | 5(4) | 20(17) |
| J1823−3021A | 2.79 | −7.91 | 5.440 | 337.61901(32) | 7.6(4)‡ | 336.42(28) | 825.0(7) | 1.59(17) | 110(20) | 13(2) |
| J2017+0603 | 48.62 | −16.03 | 2.896 | 0.79936(7) | 0.9(4) | 0.8122(15) | 13.199(24) | 3.49(17) | 3(3) | 23(20) |
| J2043+1711 | 61.92 | −15.31 | 2.380 | 0.52480(21) | 1.76(32)† | 0.393(32) | 11.5(9) | 3.02(14) | 11(4) | 100(40) |
| J2214+3000 | 86.86 | −21.67 | 3.119 | 1.47269(9) | 0.60(31) | 1.30(10) | 16.9(13) | 3.30(12) | 1.5(15) | 9(9) |
| J2302+4442 | 103.40 | −14.00 | 5.192 | 1.38689(17) | 1.19(23)† | 1.386(10) | 3.908(29) | 3.81(14) | 6.5(25) | 170(70) |
Notes. The columns give the pulsar names, Galactic coordinates, rotational periods, apparent spin-down rates, distances, corrected spin-down rates and spin-down powers, and the >100 MeV γ-ray energy fluxes, luminosities and efficiencies. Numbers in parentheses are 1σ uncertainties in the last digit(s) quoted. Distance values marked with a † symbol are derived from the pulsar DM, with uncertainties as described in the text. The distance for PSR J1741+1351 (marked with a ⋆) comes from Espinoza et al. (2013), while that for PSR J1823−3021A (marked with a ‡ symbol) is from Kuulkers et al. (2003). Other distance values are from timing parallax measurements obtained in this study (see Sect. 2.3). The >100 MeV γ-ray energy fluxes are taken from the 3FGL catalog (Acero et al. 2015), except for PSR J1811−2405 (Ng et al. 2014), and the values marked with a ∥ for which the fluxes were determined here (see Sect. 3).
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