Table 1
Pulsars for which the absolute alignment was not achieved with the refolding using the same ephemeris (see text for details).
| PSR Name | Extra DM shift/causes for misalignment |
|
|
|
| B0114+58 | S |
| B0525+21 | F4, S, g |
| B1633+24 | F4, rms = 1.3, DM = −0.11, Δφ = 0.043 |
| B1818−04 | S |
| B1839+09 | rms = 1.4, DM = −0.13, Δφ = 0.051 |
| B1848+13 | DM = −0.04, Δφ = 0.017 |
| B1907+10 | F3, S |
| B1915+13 | S |
| B2148+63 | S |
Notes. The extra DM shift (in cm-3 pc) and corresponding phase shift (Δφ) needed to align the profiles are indicated, or possibly other reasons for the observed shift, e.g., S for scattering, which notably alters the shape of the profile, g in case a glitch occurred during the range of the ephemeris, number of spin-frequency derivatives fitted to obtain a good ephemeris (i.e. F#), or final rms (in ms) of the best timing solution.
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