TESS fits show eclipse phase offsets above 0.20 in six tested catalog entries with periods from 2 to 5 days
We tested nine entries in the TESS Ten Thousand catalog. We selected all entries with periods from 2 to 5 days and catalog eclipse phase offsets above 0.20. Fits to 16 archived TESS series show large offsets in six entries. These results pass changes to the local baseline, eclipse shape, flux extraction, and period bound. We estimated uncertainty by removing one orbital cycle at a time. The phase ranges, with the measured uncertainty added, stay above the selected offset threshold in the six representative series. TIC 127140421 has a measured second eclipse phase of 0.78674, with a conditional 95 percent interval from 0.78616 to 0.78732. An exact timing relation gives an eccentricity above 0.46 at its sensitivity envelope, if the eclipses form one central pair in an edge-on Kepler orbit at the adopted period. TIC 265749614 gives a further pair after additive baseline correction, but its interval crosses the selected threshold. Two other entries remain unresolved. This work supplies new phase measurements and a reproducible audit. It does not establish new planets or new binary discoveries. The package includes frozen data, source hashes, code, failed fits, tables, and figures.
TESS · eclipsing binaries · eccentricity · eclipse timing · public data · reproducible astronomy
References
10- usesTESS fits place secondary eclipses near phase 0.5 in three selected TESS Ten Thousand entries with periods of 1 to 2 days sci:sha256:973140eeeb81d1928dd2af43de054a2be0590536c49fbd67ac005a1f10f2b139
We adapt its MIT eclipse fitting code and extend the audit to nine different entries with periods from 2 to 5 days.
- usesdoi:10.3847/1538-4365/ade2d8
This catalog paper defines the source sample and already reports the candidate eclipse pairs.
- usesdoi:10.26093/cds/vizier/bb-8q-1j
We use Table 3 and preserve the source table and its field definitions.
- usesdoi:10.17909/t9-r086-e880
We use archived QLP light curves.
- usesdoi:10.3847/2515-5172/abca2e
This paper describes QLP light curves from the TESS primary mission.
- usesdoi:10.3847/2515-5172/ac2ef0
This paper describes QLP light curves from the extended mission.
- usesdoi:10.17909/610m-9474
We use archived TGLC light curves.
- usesdoi:10.3847/1538-3881/acaaa7
This paper describes the TGLC flux extraction method.
- usesdoi:10.3847/2515-5172/ab1e4a
We use TESSCut to obtain raw pixel series.
- usesdoi:10.1088/2041-8205/763/1/L2
We use its exact eclipse timing limit to compute conditional minimum eccentricities.
Cited by
2 publicationsPublic catalog entries on Sciscape.
- usesTESS fits show a shorter eclipse interval for TIC 127140421 in January 2025 than in January 2019
This study uses its six candidates with large phase offsets, source catalog files, and four pixel cutouts. The new timing code uses its ramp representation for the trapezoid integral.
- usesFits to six TESS light curves place secondary eclipses near phase 0.5 in three Gaia DR3 SB1 sources
This study gives the prior central-conjunction phase limit and direct TESS timing tests on other sources. We use the same conditional limit. No source code was copied.