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Table 1

Main properties of the MSPs in this study.

Pulsar l b P obs d 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) %

J00340534 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)
J06102100 227.75 18.18 3.861 1.23317(4) 3.5(10) 0.01(34) 0.1(23) 1.15(11) 17(10)
J06143329 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)
J09311902 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)
J10240719 251.70 40.52 5.162 1.855242(27) 1.13(18) 3.1(8) 8.9(23) 0.36(5) 0.5(2)
J12311411 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)
J14553330 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)
J16142230 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)
J17302304 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)
J18112405 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)
J18233021A 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 J18233021A (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 J18112405 (Ng et al. 2014), and the values marked with a for which the fluxes were determined here (see Sect. 3).

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