Table 5.
Parameters of the functions describing the eclipse ingress and egress phases.
| Pulsar | Ingress | Egress | ||||
|---|---|---|---|---|---|---|
| μi | τi (ϕ−1) | Φstart | μe | τe (ϕ−1) | Φend | |
| *J1513−2550 | 0.37(9) | > 0.01 | 0.23 | 0.21(1) | 0.019(2) | 0.31(1) |
| J1555−2908 | 0.37(9) | > 0.01 | 0.21 | 0.242(4) | 0.0191(9) | 0.37(2) |
| J1628−3205 | 0.224(8) | 0.024(2) | 0.102(4) | 0.290(1) | 0.0355(6) | 0.471(2) |
| J1705−1903 | 0.440(3) | 0.0461(7) | 0.092(2) | 0.072(6) | 0.041(1) | 0.381(3) |
| J1731−1847 | 0.20(7) | 0.01(1) | 0.134(7) | 0.3430(5) | 0.0123(2) | 0.42(2) |
| J1959+2048 | 0.260(3) | 0.0078(6) | 0.21(1) | 0.205(3) | 0.0231(8) | 0.345(7) |
| J2051−0827 | 0.346(1) | 0.0356(3) | 0.1509(7) | 0.119(2) | 0.0440(5) | 0.361(1) |
| J2055+3829 | 0.2342(9) | 0.0179(2) | 0.127(2) | 0.236(1) | 0.0227(3) | 0.3713(5) |
| J2115+5448 | 0.36(9) | > 0.01 | 0.20 | 0.236(1) | 0.0258(4) | 0.352(1) |
| J2256−1024 | 0.273(3) | 0.0114(6) | 0.205(1) | 0.211(1) | 0.0200(2) | 0.3297(5) |
Notes. The parameters are determined from the fit presented in Sect. 3.3. The terms μ and ϕ are orbital phases and therefore have no unit. The three ‘abrupt’ eclipsers (starred names) have no proper ingress phase; hence, the beginning of the eclipse is taken at the last TOA above the S/N threshold before the superior conjunction, and the τi is only an upper limit.
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.