The details of the timing results and discussion of these four millisecond pulsars are presented in "Four Highly Dispersed Millisecond Pulsars Discovered in the Arecibo PALFA Galactic Plane Survey" by F. Crawford et al., Astrophysical Journal, 757, 90 (2012).
The ephemeris files are in TEMPO format.
All profiles are at a frequency of 1.4 GHz.
| Pulsar | P (ms) | DM | Ephemeris File | Pulse Profile | Poln Profile | Residuals (Date) | Residuals (Orb Phase) | Notes |
| J1844+0115 | 4.19 | 148 | binary | |||||
| J1850+0124 | 3.56 | 119 | binary | |||||
| J1900+0308 | 4.91 | 250 | binary | |||||
| J1944+2236 | 3.62 | 185 | N/A | isolated | ||||
Below: A histogram of DM/P for known Galactic MSPs (unshaded) and newly discovered PALFA MSPs (shaded), including the four MSPs presented on this page. Both data sets are complete up to mid-2012.