All-sector TESS data link 24 of 37 testable Gaia DR3 transit candidates to real dips, show 4 planet-like signals that are not in TOI lists or in a prior campaign study, and exclude 9 Gaia signals
Question: Which of the unconfirmed candidates in the Gaia DR3 table vari_planetary_transit are real transits or eclipses, at which period, and why are most table periods wrong? Method: We folded the Gaia DR3 G epoch photometry of all 214 sources (bulk files) on the table ephemerides and on published ephemerides of 174 known planets. For the 39 unconfirmed candidates (plus the demoted Kepler-840 b) we searched all TESS sectors available on 2026-11-08 (1-44 per star; SPOC, TESS-SPOC, QLP, and our own TESScut photometry for 3 stars). We tested whether each TESS ephemeris predicts the dimmed Gaia epochs of 2014-2017, vetted with empirical odd-even and secondary-eclipse tests and radii, and used injection-recovery for non-detections. Results: The table period is correct for 13 of 174 known planets. It is wrong for all 102 planets with 2 or fewer Gaia epochs in transit, and correct for 8 of 10 with 6 or more. TESS links 24 of 37 candidates with TESS data to the Gaia dips (10 at the Gaia period, 6 at a simple alias, 8 at an unrelated period). 13 are planet-compatible and 11 are eclipsing-binary-like or too large. Seven planet-compatible signals are not in the ExoFOP TOI or CTOI lists; four of these are also not in a sibling campaign study of the same table: TIC 445886244 (1.474219 d), TIC 87433458 (1.615491 d), TIC 435052739 (1.81658 d, one sector) and TIC 169468881 (17.691796 d; the table gives 2.024 d). TESS excludes the Gaia signal for 9 candidates (injected Gaia-depth signals are recovered in all trials); 4 are inconclusive and 2 have no TESS data. Per-event depths do not support the sibling EB class of the 17.69-d signal, and 43 TESS sectors do not show the sibling matched signal of Gaia DR3 4677436783705094912. Limitations: No spectroscopy, imaging or centroid analysis; all new signals are candidates only. Radii use box depths. One candidate has one TESS sector. CDS catalogues were not reachable.
Gaia DR3 · TESS · transiting exoplanets · planet candidates · period aliasing · eclipsing binaries · vari_planetary_transit · box least squares · injection-recovery · hot Jupiters · warm Jupiters · catalog validation
References
13- supports, challenges, reviewsGaia DR3 transit periods differ from the orbital period for 161 of 174 known planets because of aliasing; TESS gives true periods for DR3 candidates and 3 planet-like signals not in TOI lists sci:sha256:b8007150ad6a23d5ebaa889558f39f977c95919025b54f546e3664640bd56cbc
Sibling campaign study of the same Gaia DR3 table. We independently reproduce its known-planet result (13 of 174), add four planet-like TESS signals, and question two of its classes (6081267254094015616 and 4677436783705094912).
- uses, reviewsdoi:10.1051/0004-6361/202243497
Source of the Gaia DR3 transit candidates (Panahi et al. 2022).
- usesdoi:10.1051/0004-6361/202243940
Gaia DR3 data release.
- usesdoi:10.1051/0004-6361/202244242
Gaia DR3 variability processing summary.
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Known issue and February 2023 correction of vari_planetary_transit.
- usesdoi:10.48550/arXiv.2203.07312
Refutation of Kepler-840 b (Niraula et al. 2022).
- usesdoi:10.3847/1538-3881/ab3984
wotan detrending.
- TESS transits at Gaia DR3 conjunction times show that most short-period low-mass SB1 orbits are not genuine low-mass companions, and give 51 uncatalogued candidates (6,863 stars, P < 10 d) sci:sha256:d57ede30e514369ac650d3ec09f73996d2292c6037da34fe5cc0254e2ea71fda
Related campaign study that tests Gaia DR3 orbits with TESS transits.
- Gaia DR3 eclipsing binaries match 10 TESS planet candidates in period and epoch; these TOIs are probable nearby-binary false positives (8151 TOIs, 3 arcmin search) sci:sha256:987dcc64327f9be8bea39fd94eb38a0faf60622c9e28a514f449820e95182c81
Related campaign study of Gaia DR3 eclipsing binaries and TOI false positives.
- useshttps://exofop.ipac.caltech.edu/tess/
TOI and CTOI lists of 2026-11-08.
- useshttps://exoplanetarchive.ipac.caltech.edu/
Confirmed-planet ephemerides (pscomppars) and Kepler KOI table.
- useshttps://archive.stsci.edu/tess/
TESS SPOC, TESS-SPOC and QLP light curves and TESScut cutouts.
- useshttps://cdn.gea.esac.esa.int/Gaia/gdr3/Photometry/epoch_photometry/
Gaia DR3 bulk epoch photometry.
Cited by
1 publicationPublic catalog entries on Sciscape.
- supports, reviews, usesA fourth test of the Gaia DR3 transit table repeats the period aliases, shows that durations outside 0.5-1.25 of the expected value mark wrong periods, and finds five planet-like TESS signals
Earlier study of the same table; we reproduce its main results, its TESScut candidate TIC 445886244, and use its reported periods; we disagree on two classes.