A curved Crab spin-down baseline reduces errors in 37 later records under a fixed early fit
A smooth baseline is needed to measure a lasting change in the Crab pulsar's rate of slowing. We compare a straight baseline with a curved baseline that assumes a constant braking index. Both models use the same early data and four fitted parameters. We fit data from 2015 to 2022 and test 37 later timing records through 8 July 2025. The curved model reduces the root mean squared error from 13.43 to 8.49 units of 10^-15 Hz/s. This is a 36.8 percent reduction. All eight sensitivity checks also favor the curved model. The fitted lasting shift changes from -440.21 to -430.38 units with equal record weights. The result shows that baseline curvature matters for this continuation and shift estimate. The test is retrospective. One stress test perturbed the early data and fitted both models again. Its 95 percent gain range included zero. Timing noise and early-fit uncertainty limit the physical interpretation. The package contains numerical data, source hashes, code, predictions, figures, and reproduction steps.
Crab pulsar · spin-down · braking index · glitch recovery · public data · prediction test · timing noise · reproducible analysis
References
7- usesdoi:10.1093/mnras/265.4.1003
This paper describes the origin of the Jodrell Bank Crab timing data. The data team requests this citation. We use the public monthly ephemeris and preserve its source URL and hash.
- usesdoi:10.3847/1538-4357/adbca6
We use the early fit intervals, glitch epoch, and fixed exponential factor for a later-data comparison. We fit each baseline and recovery again.
- doi:10.1093/mnras/stu2118
This paper gives prior work on the Crab pulsar's rotation and lasting changes after glitches.
- doi:10.1051/0004-6361/201526490
This paper gives prior use of constant braking laws for Crab timing episodes. The present contribution is the specified later-data comparison.
- doi:10.1093/mnras/staf1415
This paper uses published persistent shifts for model comparisons. It gives context for checking the baseline dependence of those shifts.
- usesdoi:10.1038/s41592-019-0686-2
We use SciPy for numerical fitting. The package records the software version.
- usesdoi:10.1109/MCSE.2007.55
We use Matplotlib to make the figures. The package records the software version.
Cited by
1 publicationPublic catalog entries on Sciscape.
- usesA local frequency balance test flags five of eight listed Crab glitches in the 2010–2026 monthly record
We use this publication’s numeric extraction for a separate check on all 482 frequencies, derivatives, and quoted errors. We do not reuse its fitted models.