Table 6
α and ζ best-fit solution resulting from the γ-ray only fit of the 41 RL pulsars.
| α PC | α SG | α OG | α OPC | α others | ζ PC | ζ SG | ζ OG | ζ OPC | ζ others | |
| ° | ° | ° | ° | ° | ° | ° | ° | ° | ° | |
|
|
||||||||||
| J0205+6449 |
|
|
|
|
|
|
|
|
85.7 − 90 2 | |
| J0248+6021 |
|
|
|
|
|
|
|
|
||
| J0534+2200 |
|
|
|
|
|
|
|
|
60.10 − 64.35 2 | |
| J0631+1036 |
|
|
|
|
|
|
|
|
||
| J0659+1414 |
|
|
|
|
|
|
|
|
||
| J0729−1448 |
|
|
|
|
|
|
|
|
||
| J0742−2822 |
|
|
|
|
|
|
|
|
||
| J0835−4510 |
|
|
|
|
431/703 |
|
|
|
|
62.95 − 64.27 2 |
| J0908−4913 |
|
|
|
|
|
|
|
|
||
| J0940−5428 |
|
|
|
|
|
|
|
|
||
| J1016−5857 |
|
|
|
|
|
|
|
|
||
| J1019−5749 |
|
|
|
|
|
|
|
|
||
| J1028−5819 |
|
|
|
|
|
|
|
|
||
| J1048−5832 |
|
|
|
|
|
|
|
|
||
| J1057−5226 |
|
|
|
|
|
|
|
|
||
| J1105−6107 |
|
|
|
|
|
|
|
|
||
| J1112−6103 |
|
|
|
|
|
|
|
|
||
| J1119−6127 |
|
|
|
|
|
|
|
|
||
| J1124−5916 |
|
|
|
|
|
|
|
|
68.0 − 82.0 2 | |
| J1357−6429 |
|
|
|
|
|
|
|
|
||
| J1410−6132 |
|
|
|
|
|
|
|
|
||
| J1420−6048 |
|
|
|
|
|
|
|
|
||
| J1509−5850 |
|
|
|
|
|
|
|
|
||
| J1513−5908 |
|
|
|
|
|
|
|
|
||
| J1648−4611 |
|
|
|
|
|
|
|
|
||
| J1702−4128 |
|
|
|
|
|
|
|
|
||
| J1709−4429 |
|
|
|
|
|
|
|
|
49.0 − 57.8 2 | |
| J1718−3825 |
|
|
|
|
|
|
|
|
||
| J1730−3350 |
|
|
|
|
|
|
|
|
||
| J1741−2054 |
|
|
|
|
|
|
|
|
||
| J1747−2958 |
|
|
|
|
|
|
|
|
||
| J1801−2451 |
|
|
|
|
|
|
|
|
||
| J1833−1034 |
|
|
|
|
|
|
|
|
85.1 − 85.6 2 | |
| J1835−1106 |
|
|
|
|
|
|
|
|
||
| J1952+3252 |
|
|
|
|
|
|
|
|
||
| J2021+3651 |
|
|
|
|
|
|
|
|
76.0 − 82.0 2 | |
| J2030+3641 |
|
|
|
|
|
|
|
|
||
| J2032+4127 |
|
|
|
|
|
|
|
|
||
| J2043+2740 |
|
|
|
|
|
|
|
|
||
| J2229+6114 |
|
|
|
|
|
|
|
|
38.0 − 54.0 2 | |
| J2240+5832 |
|
|
|
|
|
|
|
|
||
Notes. The central and last columns list independent α and ζ estimates, found in the literature, respectively. Superscript and subscript refer to upper and lower errors, respectively. The errors bigger than 1 correspond to the 3σ statistical error. The solutions compatible, within the errors, with the solutions obtained by fitting jointly radio and γ-ray light curves and listed in Table 3 are highlighted in grey cells.
Reference.
α = ζ + 6.5 found by Johnston et al. (2005) with ζ ~ 63.5 from Ng & Romani (2008).
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.