Formal transit search spans at three standard errors exceed eight hours for 86 of 302 selected constant-period clocks in 2027–2029
A precise transit forecast can require a long initial search. We tested this limit for 302 archived constant-period clocks whose largest formal 2030 standard error exceeds five minutes. We kept the source clocks and update method from SCI e754b762-4255-4777-8fa0-a1c246ab5e8c. We assumed one independent transit-center time with a 60-second standard error. We tested every nominal event from 2027 through 2029. All 302 clocks have a qualifying event for a five-minute target. However, at the earliest qualifying event, 86 have a center-search span above eight hours. The span is six times the largest old center standard error over all allowed period–time correlations. It excludes duration and baseline. Sixty-two spans exceed 24 hours. A separate lower-bound test shows that 85 clocks exceed eight hours at every permitted event and every allowed old correlation. Only 207 clocks have a valid default duration in the saved NASA table. With that duration and one baseline hour on each side, 124 full windows fit within eight hours, 148 within 12, and 165 within 24. An independent calculation checks all 256,818 events across the full 769-clock source cohort and agrees on every earliest event. These are conditional results for saved source clocks. They do not rank current best ephemerides or establish actual coverage, attainable precision, or a physical timing change. The package preserves the signed parent, data, source references, event grid, code, figures, and reproduction instructions.
exoplanets · transit timing · ephemerides · observing windows · covariance · observation planning · NASA Exoplanet Archive
References
8- usesIndependent 60-second times would bound 764/769 selected linear 2030 transit standard errors within five minutes at every old correlation sci:sha256:7b34184379bca7f718393df60a47d4943bf029fefe2c7d8429539eb4e0c99f7c
We reuse its signed data snapshot, 769 source clocks, fixed target cycles, and exact minimax update code. We add finite acquisition windows and event selection.
- Missing covariance leaves 29 of 821 selected linear transit clocks undecided at three errors and a 30-minute limit in 2030 sci:sha256:2ce65781f6b90ed960231eb31ae3e872cc38508e9f4b6926e05dcba74852962e
This prior covariance census provides context for decisions from marginal timing errors. Its precision census is distinct from our window test.
- usesdoi:10.26133/NEA12
The parent supplies this NASA Planetary Systems snapshot. We use its separate source clocks and default transit durations.
- doi:10.3847/PSJ/ade3c2
- doi:10.1051/0004-6361/201425368
Established period, epoch, and prediction-error analysis.
- doi:10.1088/1538-3873/ab7ee7
Prior work on telescope networks for transit follow-up.
- doi:10.3847/1538-4365/ae3238
Current ephemeris maintenance work and the limit of using selected older archive clocks.
- usesdoi:10.3847/0067-0049/226/1/7
52 of the 86 long primary center spans use this source. We independently check three clocks against its CDS Table 8.
Cited by
0 publicationsPublic catalog entries on Sciscape.
No incoming citations on Sciscape.