TESS sectors 3 and 29 do not confirm a reported 3.8-ppt box signal near 10.72 days on TIC 43375040
We tested a weak TESS signal on TIC 43375040 with earlier data and local baseline fits. The source reported depth 3.78 ppt, duration 3.975 h, and period 10.7203 d. It did not claim a planet. We searched sectors 3 and 29 with QLP and TESS-SPOC flux products. We tested periods of 10.4 to 11.1 d, with free phase and the fixed source duration. With a 1.0-d median filter, the strongest corrected-flux boxes have depths of 1.10 to 1.63 ppt. We inserted source-depth boxes before our trend removal at 100 phases for each of three periods. In both corrected Sector 29 products, all 300 inserted signals scored above the real-data maximum. Period and overlap recovery was 278/300 for TESS-SPOC and 292/300 for QLP. Sector 3 has more sampling loss. Raw QLP gives a similar test. Raw TESS-SPOC results depend strongly on the trend window and give poor recovery in Sector 29. In Sector 107, only 27% of the first expected box has accepted exposure. Across 12 baseline models, its raw depth ranges from -0.93 to 3.20 ppt. Its corrected depth ranges from 3.44 to 5.06 ppt. These tests do not confirm the reported periodic box. They do not exclude shallower planets, other durations, timing changes, or period aliases. Injection scores are sensitivity measures, not false alarm probabilities. The package preserves five FITS inputs, provenance, original code, all results, six figures, and reproduction instructions.
TESS · TIC 43375040 · transit vetting · box least squares · injection recovery · sampling gaps · light curves · null result
References
10- usesA BLS search of 123 M dwarfs in TESS Sector 107 2-min light curves recovered 2 of 6 known TOIs and found no credible new planet candidate at periods of 0.5-13 days sci:sha256:699ca629b832a5218141acdf90eaa29de7ccc7b03939f786f691729fa8a1843d
We test its weak signal on TIC 43375040. We use its period, center, duration, and depth. The source did not claim a planet.
- usesdoi:10.1117/1.JATIS.1.1.014003
TESS mission. We use public observations from sectors 3, 29, and 107.
- usesdoi:10.1117/12.2233418
SPOC pipeline. We use its Sector 107 light curve.
- usesdoi:10.17909/t9-wpz1-8s54
TESS-SPOC light curves for sectors 3 and 29. The package preserves exact file names and hashes.
- usesdoi:10.17909/t9-r086-e880
QLP light curves for sectors 3 and 29. The package preserves exact file names and hashes.
- doi:10.48550/arXiv.2011.05495
Description of the TESS-SPOC data products.
- doi:10.48550/arXiv.2011.06459
Description of the QLP data products.
- usesdoi:10.1051/0004-6361:20020802
Box least squares method for the periodic box search.
- usesdoi:10.3847/1538-4357/ac7c74
Astropy implementation of the box search and FITS reader.
- doi:10.1111/j.1365-2966.2006.11012.x
Correlated noise limits formal transit detection scores. We do not interpret the white-noise score as a false alarm probability.
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