Published ephemeris pairs reduce measured sector mean timing offsets below one minute in three TESS hot Jupiters
We tested the three largest normalized timing offsets in an earlier SCI audit. We fit 68 transits in 12 public TESS light curves from 2018 to 2026. We measured HAT-P-16 b, KELT-18 b, and WASP-20 b. Latest sector mean offsets from saved archive composite pairs were -13.88, -76.01, and -12.76 minutes. Published time and period pairs reduced them to -0.37, +0.88, and +0.95 minutes. Two composite rows mixed reference times from fixed-period fits with newer periods. The mixed pairs add constant prediction shifts of 13.51 and 13.71 minutes. The third row used an older period that differed by 4.59 seconds per orbit. Earlier sectors predicted each latest sector within 0.38 minute. The new contribution is a source audit, 68 transit times, and prediction tests with the latest sectors withheld. The sample covers three selected planets. It does not exclude smaller physical timing changes. The package includes original data, code, provenance, error checks, and figures.
TESS · transit timing · ephemeris · NASA Exoplanet Archive · HAT-P-16 b · KELT-18 b · WASP-20 b · catalog validation · reproducible research
References
13- usesTESS 2-minute transit times of 153 bright hot Jupiters missed the NASA Exoplanet Archive default ephemeris predictions by more than 3 sigma for 33 planets (sectors 21-107) sci:sha256:1895bf428f65ddb5d621f1e1b67e6fe70b4074599f4ced66ffdc1cf0a99b69fe
Its quality-approved table defines the three targets. We fit the public light curves again.
- usesdoi:10.26133/NEA13
The saved composite table supplies the predictions under test.
- usesdoi:10.26133/NEA12
The saved Planetary Systems table supplies complete published ephemeris pairs.
- doi:10.3847/PSJ/ade3c2
This paper describes the archive data and services.
- usesdoi:10.1002/asna.20224012
Its fixed-period fits supply two reference times in the tested composite pairs.
- supportsdoi:10.1093/mnras/stae854
Later TESS data support its paired time and period for HAT-P-16 b.
- supportsdoi:10.3847/1538-4365/ac545b
Later TESS data support its paired time and period for KELT-18 b.
- supportsdoi:10.3847/1538-4365/ac9da4
Later TESS data support its paired time and period for WASP-20 b.
- usesdoi:10.3847/1538-3881/aa6d5d
The archive attributes the older KELT-18 b comparison parameters to this discovery paper.
- doi:10.48550/arXiv.2509.21551
Its version 1 reports a HAT-P-16 curvature that remains compatible with the TESS-only data here.
- usesdoi:10.1117/1.JATIS.1.1.014003
The TESS mission supplies the observations.
- usesdoi:10.1117/12.2233418
SPOC supplies the processed light curves.
- usesdoi:10.1086/683602
The batman software supplies transit templates and exposure integration.
Cited by
1 publicationPublic catalog entries on Sciscape.
- Local fits to TESS sector 104 place one TOI-1130 c transit 2.2 to 2.7 minutes after the 2024 forecast
This source audit shows that inconsistent period and reference time pairs can cause large apparent timing offsets. We instead test one direct forecast table.