Table B.1.
Resulting emission height behavior of individual pulsars.
| Pulsar | Group | Slope | Pulsar | Group | Slope | Pulsar | Group | Slope |
| J0034–0721 | 1 | − | J1156–5707 | 1 | − | J1707–4729 | −1 | − |
| J0108–1431 | 1 | + | J1157–6224 | 1 | − | J1709–1640 | 0 | + |
| J0151–0635 | 1 | + | J1253–5820 | 1 | + | J1709–4429 | 1 | + |
| J0304+1932 | 0 | − | J1302–6350 | −1 | + | J1715–3903 | 1 | + |
| J0401–7608 | −1 | + | J1305–6203 | 1 | − | J1715–4034 | −1 | − |
| J0452–1759 | 0 | − | J1306–6617 | −1 | + | J1716–4005 | −1 | − |
| J0536–7543 | −1 | + | J1320–5359 | 1 | − | J1717–3425 | −1 | + |
| J0543+2329 | 1 | − | J1326–5859 | −1 | + | J1718–3825 | 1 | + |
| J0601–0527 | −1 | − | J1326–6700 | 0 | + | J1720–2933 | 0 | + |
| J0614+2229 | 1 | − | J1327–6222 | −1 | − | J1722–3632 | 1 | − |
| J0624–0424 | −1 | − | J1327–6301 | 1 | − | J1722–3712 | 1 | + |
| J0630–2834 | 1 | + | J1328–4357 | 0 | − | J1723–3659 | 1 | − |
| J0631+1036 | 1 | + | J1338–6204 | 1 | + | J1727–2739 | −1 | − |
| J0659+1414 | 1 | − | J1352–6803 | 1 | + | J1731–4744 | 0 | + |
| J0729–1448 | 1 | + | J1356–5521 | −1 | + | J1733–3716 | 1 | + |
| J0729–1836 | 1 | + | J1357–62 | −1 | − | J1735–0724 | −1 | − |
| J0738–4042 | 1 | + | J1357–6429 | 1 | − | J1739–3023 | 1 | − |
| J0742–2822 | 1 | − | J1359–6038 | −1 | + | J1741–2733 | −1 | − |
| J0745–5353 | −1 | + | J1401–6357 | 0 | + | J1741–3016 | 1 | − |
| J0758–1528 | 0 | + | J1412–6145 | −1 | + | J1741–3927 | −1 | − |
| J0809–4753 | 1 | − | J1420–6048 | 1 | + | J1743–3150 | 1 | + |
| J0820–1350 | 0 | − | J1455–59 | 1 | − | J1748–1300 | 1 | + |
| J0820–4114 | 1 | − | J1456–6843 | −1 | + | J1749–3002 | 1 | + |
| J0835–4510 | 1 | − | J1513–5908 | −1 | + | J1750–3157 | 1 | + |
| J0842–4851 | −1 | − | J1524–5625 | −1 | − | J1751–3323 | −1 | + |
| J0855–4644 | 1 | + | J1524–5706 | −1 | + | J1757–2421 | 0 | + |
| J0857–4424 | 1 | − | J1530–5327 | −1 | + | J1801–2451 | −1 | + |
| J0901–4624 | 1 | − | J1531–5610 | −1 | − | J1803–2137 | −1 | + |
| J0904–7459 | 1 | + | J1534–5405 | −1 | − | J1807–0847 | 1 | − |
| J0905–5127 | 1 | − | J1535–4114 | 1 | − | J1809–1917 | 0 | + |
| J0907–5157 | −1 | + | J1536–5433 | 0 | + | J1816–2650 | 1 | + |
| J0908–1739 | 1 | − | J1539–5626 | −1 | + | J1817–3618 | 1 | − |
| J0924–5814 | 1 | − | J1548–5607 | −1 | + | J1822–2256 | 0 | + |
| J0940–5428 | 0 | − | J1559–4438 | −1 | + | J1823–3106 | 1 | − |
| J0942–5552 | 1 | + | J1603–5657 | 0 | + | J1826–1334 | −1 | + |
| J0954–5430 | 0 | − | J1605–5257 | 1 | + | J1830–1059 | 1 | − |
| J0959–4809 | 1 | + | J1611–5209 | 0 | − | J1833–0827 | −1 | − |
| J1015–5719 | 1 | + | J1637–4553 | 1 | − | J1834–0426 | 1 | + |
| J1016–5857 | −1 | − | J1637–4642 | 1 | − | J1835–1106 | 1 | − |
| J1034–3224 | 1 | + | J1643–4505 | −1 | + | J1841–0345 | 1 | − |
| J1038–5831 | −1 | − | J1648–4611 | 1 | − | J1842–0905 | 1 | − |
| J1047–6709 | −1 | + | J1649–4653 | −1 | − | J1845–0434 | 1 | + |
| J1048–5832 | 0 | + | J1651–4246 | −1 | − | J1845–0743 | 1 | + |
| J1049–5833 | 1 | + | J1651–5222 | 1 | + | J1852–0635 | −1 | − |
| J1056–6258 | 1 | − | J1652–2404 | 1 | − | J1853–0004 | 0 | − |
| J1105–6107 | 1 | − | J1653–3838 | −1 | + | J1900–2600 | 1 | + |
| J1110–5637 | −1 | − | J1700–3312 | 1 | + | J1910+0358 | −1 | − |
| J1114–6100 | 1 | + | J1701–3726 | 1 | + | J1913–0440 | 1 | − |
| J1115–6052 | 1 | − | J1701–4533 | 1 | + | J1932+2220 | 1 | − |
| J1119–6127 | 1 | − | J1702–4128 | −1 | + | J1941–2602 | 1 | + |
| J1123–6259 | 1 | + | J1702–4310 | 1 | − | J2048–1616 | −1 | + |
| J1136–5525 | −1 | + | J1703–3241 | 0 | + | J2346–0609 | 0 | − |
| J1146–6030 | 0 | − | J1705–3950 | 1 | + |
Notes. The table lists the classification based on the groups as classified by Δϕ0 (column 2) and the correlation between emission height and observing frequency, with the slope indicating the trend: positive for increasing height with frequency and negative for decreasing (column 3).
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