Open Access

Table 2.

Best fit values for the geometry of each pulsar according to the analysis of their gamma-ray light curves.

PSR α (in °) ζ (in °) ϕs
J0248+6021 30 42 −0.07
J0631+1036* 40 36 0.01
J0659+1414* 45 32 −0.23
J0742–2822* 140 136 0.16
J0835–4510* 65 58 −0.1
J0908–4913* 95 92 −0.08
J1016–5857 40 64 −0.02
J1019–5749 30 42 0.07
J1028–5819 75 64 −0.01
J1048–5832* 60 68 −0.12
J1057–5226* 25 44 −0.01
J1119–6127* 60 40 −0.06
J1357–6429* 20 34 −0.09
J1420–6048* 45 56 −0.08
J1509–5850 40 24 −0.06
J1648–4611* 60 42 −0.05
J1702–4128* 155 148 −0.05
J1709–4429* 40 56 −0.1
J1718–3825* 30 38 −0.06
J1730–3350 20 36 −0.05
J1747–2958 45 68 −0.07
J1801–2451* 85 72 −0.12
J1835–1106* 30 36 0.03
J1907+0602 45 68 −0.04
J1952+3252 60 84 −0.06
J2021+3651 60 80 −0.09
J2030+3641 20 42 −0.07
J2032+4127 85 72 −0.08
J2043+2740 45 68 −0.06
J2229+6114 35 44 −0.03
J2240+5832* 60 80 −0.09

Notes. Pulsars flagged with superscript * are those that have radio polarization RVM fits (see Table 1) using the α and ζ values given above (except for PSR J1057−5226, as discussed in Sect. 4.3).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.