Geminga ephemeris obtaited with Fermi-LAT data. Timing noise is modeled with a set of cubic splines defined in intervals of ∼100 days and smoothly joined at their edges (C3 continuous, jumps only in F2). In tempo2, this requires to increase the number of glitch parameters defined in initialise.C, that defaults to 40. PINT does not have this limitation.
The procedure is described here (appendix A).
Please contact me if you plan to use this for a publication.
| START | 54685 | 2008-08-06 | ||
| FINISH | 60586 | 2024-10-02 |