A direct TESS Sector 91 search misses most translated K2 dip models for HD 139139
HD 139139 showed 28 isolated dips in the 2017 K2 data. We test whether a direct aperture search of the public 2025 TESS Sector 91 data can find models with the published depths and durations. The primary search uses 8,315 exposures with QUALITY = 0, eight durations from 0.7 to 8.2 hours, a local quadratic baseline, and a fixed score threshold of 6. No primary dip reaches the threshold. At the original depths, the search recovers 111 of 14,336 isolated trapezoid injections, or 0.77%. Only 1.28% recover among trials that pass the coverage test. We also inject all events from 512 translated sections of the finite K2 sequence. Of these trials, 469 give no recovery at the original depths. Only 2 give no recovery at four times those depths. The TESS null result is therefore expected under this specified original-depth model. It does not establish that the original dips stopped. Secondary peaks depend on aperture and flux correction and do not support a new planet claim. The test assumes equal numerical aperture depths in the two instruments and fixed empirical noise scales. It does not measure upstream calibration losses or the sensitivity of other photometry methods. The package preserves the public FITS inputs, source records, event table, code, complete results, and figures for offline reproduction.
HD 139139 · EPIC 249706694 · TIC 70652803 · TESS Sector 91 · isolated dips · injection and recovery · selection function · public data · Random Transiter
References
8- usesdoi:10.1093/mnras/stz1772
Table 1 supplies the 28 K2 event times, depths, durations, and reported errors.
- doi:10.1051/0004-6361/202347779
Prior CHEOPS observations found no similar dips. Their sequence test motivates a separate sensitivity calculation.
- usesdoi:10.17909/rer5-r112
The primary input is a TESScut from these calibrated TESS Sector 91 full-frame images.
- usesdoi:10.17909/t9-r086-e880
The Sector 91 QLP product supplies secondary flux-series checks.
- doi:10.48550/arXiv.2011.06459
This paper describes the base QLP photometry method.
- usesdoi:10.17909/T9BC75
The K2SFF file supplies the first and last finite observation times for the translated sequence model. Its flux is not analyzed.
- doi:10.1086/678764
This paper describes the K2SFF product used for source time bounds.
- supersedesA direct TESS Sector 91 search misses most translated K2 dip models for HD 139139 sci:sha256:5c1b6ec3c9906ba5b5175470274c0066642aa59846e24a3577ec86b248b1169c
This edition corrects local dates that were labeled UTC in three provenance records. The input bytes, code, figures, and scientific results are identical.
Cited by
1 publicationPublic catalog entries on Sciscape.
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This related study shows why a TESS null result needs a recovery measurement. No code or data are reused.