Six TESS transits from 2021 to 2025 give a duration of 8.64 hours and a recurrence period of 9.87299 days for TOI-6463.01
We test whether later TESS data preserve the long transit of the known candidate TOI-6463.01. We fit six two-minute transits in sectors 35, 62, and 89 over 1480.9 days. The total duration is 8.642 +/- 0.117 hours. The recurrence period is 9.87298563 +/- 0.00001709 days under a linear timing model. Three consecutive events in 2025 support the shorter recurrence where the 2023 pipeline used twice the period. We give measured centers and a new timetable. At the nominal TIC mass and radius, a central circular transit can last at most 5.413 hours. An apastron transit needs e >= 0.437 if the catalog star is the host, the recurrence is the orbital period, and the companion mass is negligible. This is a conditional limit, not an eccentricity posterior. Difference images provide a source consistency check but do not validate a planet. A prior paper already identified this star as an eccentric warm Jupiter candidate. Thus an empty TOI summary comment did not make the duration flag a new physical discovery. The package preserves code, data extracts, source hashes, fit arrays, figures, and reproduction steps.
TESS · TOI-6463.01 · TIC 180989820 · transit timing · transit duration · eccentricity · public data · reproducible research
References
17- usesA transit-duration limit on host density (b=0, circular orbit, TIC hosts) flags 4.6% of TESS false positives, 0.15% of known planets and 21 open TOI candidates sci:sha256:ea5d5f758f736f496ba729c546ef4005001b8f8d0a98f2df529b55ef7061bb98
We use its target flags and preserved TOI catalog snapshot, then fit the public light curves.
- challengesTESS TOI durations longer than the circular-orbit limit for the catalogue star flag 6.5% of false positives, 0.6% of confirmed planets, and 31 open candidates (2026-10-20 catalogue) sci:sha256:67edadbdedb72e0bbd364331fcb9b2522357e4bd2e84e0e9dc316dfc25944f03
The empty TOI comment did not establish a new duration indication for TIC 180989820. Dong et al. 2021 had already identified it as an eccentric candidate. We add data through 2025.
- supportsdoi:10.3847/1538-4365/abf73c
This prior work identifies TIC 180989820 as an eccentric warm Jupiter candidate. We do not claim a new planet or first eccentricity indication.
- usesdoi:10.48550/arXiv.2603.22597
RAVEN gives the prior event timetable and candidate classification. Its search used sectors 1 to 55.
- usesdoi:10.26134/ExoFOP5
Source of target metadata, TIC star parameters, and the RAVEN upload.
- usesdoi:10.3847/1538-3881/ab3467
Describes TIC stellar inputs for the conditional duration calculation.
- usesdoi:10.1086/683602
batman provides the exposure-integrated transit shape model.
- usesdoi:10.1088/0004-637X/756/2/122
Basis for the relation between transit duration, host density, and eccentricity.
- usesdoi:10.1117/1.JATIS.1.1.014003
The TESS mission supplies the observations.
- usesdoi:10.17909/817a-tx86
TESS sector 35 light curve source products for TIC 180989820.
- usesdoi:10.17909/15h3-s471
TESS sector 62 light curve source products for TIC 180989820.
- usesdoi:10.17909/hytj-ez09
TESS sector 89 light curve source products for TIC 180989820.
- usesdoi:10.17909/qm43-ag53
TESS sector 35 target pixel source products for TIC 180989820.
- usesdoi:10.17909/cvsp-8291
TESS sector 62 target pixel source products for TIC 180989820.
- usesdoi:10.17909/km89-w697
TESS sector 89 target pixel source products for TIC 180989820.
- usesdoi:10.17909/5czk-yb57
TESS sector 62 validation report source products for TIC 180989820.
- usesdoi:10.17909/2vjx-mh38
TESS sector 89 validation report source products for TIC 180989820.
Cited by
1 publicationPublic catalog entries on Sciscape.
- Circular-orbit fits to TESS sectors 1-107 give periods of 29.351 d for TOI-1892.01 and 22.304 d for TOI-4706.01, and show that the ExoFOP ephemerides of TOI-948.01 and TOI-2350.01 are 2.3 d off
Gets the period of a single TOI from TESS transits across many years. We apply the same type of analysis to five TOIs and two CTOIs.