...
- These methods used for this pipeline will be documented in Kerr et al. (2014, in prep). Once this paper is available, please cite it for any uses of this work.
- Each row of the table corresponds to one pulsar timed using the LAT data. Both the full par file and the TOAs are available via links in the first column.
- The Whitened Residuals show the residuals for the full timing model. Unlike previous timing solutions, whitening is achieved by estimating the time-domain realization of the timing noise, then subtracting this signal by linear interpolation (the "SIFUNC" terms in the ephemeris).
- The Unwhitened Residuals show the residuals to a model without any red noise terms. For most pulsars, only the first frequency derivative is included in this model. For the Crab, this includes up to F2.
- Horizontal dashed lines on the plots indicate the epoch of glitches.
- The Phaseogram shows a 2-D plot of the LAT photons vs pulse phase and time.
- The Pulse Profile plot shows the full LAT profile along with the analytic template (solid blue, with the individual components in dashed blue lines). The residuals between the model and the data are in red.
- The Position plot shows the timing position with uncertainty, along with the published multiwavelength location (e.g. X-ray counterpart), when available. The LAT timing position uncertainty includes the effects of timing noise.
...