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Table 1.
Radio-loud γ-ray MSPs from the first sample.
| Name | P (ms) | i (deg) | Companion |
|---|---|---|---|
| J0218+4232 | 2.32 | 85.1 | He WD |
| J0437−4715 | 5.76 | 42.42 | He WD |
| J0737−3039A | 22.7 | 89.35 | NS |
| J0740+6620 | 2.89 | 87.56 | He WD |
| J0955−6150 | 1.99 | 83.2 | |
| J1012−4235 | 3.1 | 87.97 | He WD |
| J1125−6014 | 2.63 | 77.6 | He WD |
| J1600−3053 | 3.6 | 68.6 | He WD |
| J1614−2230 | 3.15 | 89.18 | CO WD |
| J1713+0747 | 4.57 | 72.0 | He WD |
| J1741+1351a | 3.75 | 73 | He WD |
| J1857+0943 | 5.36 | 88.0 | He WD |
| J1909−3744 | 2.95 | 86.69 | He WD |
| J2043+1711 | 2.38 | 83.2 | He WD |
Notes. For each pulsar, measured spin period P, orbital inclination angle i from Shapiro delay and companion type (WD for white dwarf, He for helium, and CO for carbon-oxygen) are provided.
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