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Table 2.

Pulsar geometry as derived from fitting the gamma-ray light curves.

Pulsar αTPC ζTPC αOG ζOG
(deg) (deg) (deg) (deg)
J0002+6216* 47 67 81 67
J0007+7303 2 2 9 79
J0106+4855* 65 89 90 89
J0357+3205 3 0 3 80
J0359+5414 3 0 89 19
J0554+3107 3 1 9 77
J0622+3749 9 69 6 80
J0631+0646*
J0633+0632 74 85 90 88
J1836+5925 28 85 5 77
J1838−0537 10 69 13 78
J1846+0919 2 2 5 73
J1906+0722 30 67 74 17
J1907+0602* 45 66 82 59
J1932+1916 3 0 90 20
J1954+2836 62 77 8 80
J1957+5033 2 2 6 73
J1958+2846 33 69 31 78
J2017+3625 51 71 15 80
J2021+4026 62 26 29 89
J2028+3332 28 69 40 87
J2030+4415 72 89 72 87
J2032+4127* 88 77 85 84
J2055+2539 14 69 66 25
J2111+4606 13 69 11 79
J2139+4716 21 66 19 80
J2238+5903 90 84 89 87

Notes. Column 1: name of the pulsar (pulsars with know radio emission are denoted with *). Columns 2 and 3: best-fit values for the angles α and ζ for the TPC model. Columns 4 and 5: same as Cols. 2 and 3, but for the OG model. Unless otherwise stated, the error was considered to be ±10.

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