The best periodic box retains 29.3% of ideal signal-to-noise for 14 TOI-4504 c times with fixed cycles, equal eight-hour transits, and white noise
We test the loss of expected signal-to-noise when a periodic box template is applied to 14 published transit centers of TOI-4504 c. Cycle labels stay fixed. The model has equal eight-hour box transits, equal depths, a known baseline, and equal white noise in complete independent event records. Period, phase, and template width are free. We prove that a global maximum occurs in a finite set of box contact intersections. We check that set with exact integer arithmetic. The best periodic template retains 0.2931265613 of the expected signal-to-noise of a filter that knows all centers. Its width is 29.78912 hours and it overlaps eight of the 14 events. A fixed eight-hour template retains 0.2494194805. Allowing independent center shifts within three times each printed timing error plus rounding raises the best ratio to 0.2957859789. Changing the assumed transit duration from four to twelve hours gives ratios from 0.222270 to 0.340435. A separate seven-event test for planet d gives 0.797821. Source checks, exact witnesses, independent numerical checks, code, provenance, figures, and reproduction instructions are included. This is a controlled timing benchmark. It does not measure detection efficiency in TESS data or test a new planet.
TOI-4504 · transit timing variations · periodic transit search · box template · exact optimization · signal-to-noise · reproducible benchmark
References
6- usesNo fixed period fits 14 published TOI-4504 c transit times within 48 hours sci:sha256:91255e799106ca92c096bb28d1c61a251d1845a26f5e97a0be4c02991d5d50cb
We use its preserved timing table, article HTML, and MIT source table checker. We answer a different question: the maximum normalized expected signal-to-noise of a periodic box with free width.
- usesdoi:10.48550/arXiv.2603.05720
Version 1 Table 2 supplies all 14 independent c centers, seven d centers, cycle labels, and printed timing errors. The exact source HTML is preserved.
- doi:10.3847/2041-8213/ad9a53
- doi:10.1111/j.1745-3933.2011.01111.x
- doi:10.1051/0004-6361:20020802
- doi:10.1088/0004-637X/765/2/132
Cited by
1 publicationPublic catalog entries on Sciscape.
- usesLater measured transits reduce the best periodic box signal for two of 80 selected Kepler planets in an equal white noise model
We use its finite contact proof and unchanged Python reference code. We adapt the solver to C++ integer arithmetic and compare early and full Kepler event sets.