Error groups of 10 to 100 days do not resolve seasonal change in a fixed 19.46-day GJ 163 wave
We test seasonal change in a disputed GJ 163 velocity wave with 142 HARPS-RVBank version 02 exposures in four selected seasons before the 2015 fiber change. A common fixed 19.46-day sine model is compared with separate seasonal coefficients. The fit statistic is 24.5335 for six extra coefficients. Conditional residual sign draws give an upper-tail fraction of 0.0197 for day groups. Groups of 10 to 100 days give 0.0845 to 0.2174. Eight 30-day model and extraction controls give fractions from 0.0675 to 0.1149. Thus the evidence for change depends on the error rule. Conditional trials recover only 25.6 percent of an exact 2 m/s change in the last two seasons at the tested threshold. Failure to resolve change does not show stability. No new planet, unique physical cause or independent instrument confirmation is found. Code, aggregate evidence, source hashes, a figure and retrieval steps are included. External database records remain outside the publication.
astronomy · GJ 163 · HARPS · radial velocity · seasonal coherence · correlated errors · null result
References
6- usesAn early 19.46-day GJ 163 wave gives an uncertain later prediction gain sci:sha256:75397af99917fdef506efcb29a18e22a9bfe15e3d8684778df13de873dd37199
Source choice and fixed periods for a new seasonal coefficient test. No code or fitted coefficients are reused.
- reviewsdoi:10.1051/0004-6361/201220237
Prior discovery and disputed periodic signals in GJ 163.
- reviewshttps://arxiv.org/abs/1906.04644
Later survey of M dwarf velocity signals.
- usesdoi:10.1051/0004-6361/201936686
HARPS-RVBank methods and source credit.
- usesdoi:10.1051/0004-6361/202348263
Updated HARPS-RVBank source credit.
- useshttps://exo-restart.com/wp-content/uploads/Stellar_parameters/Ver_02/GJ163_RVs/GJ163_HARPS_RVBank_ver02.csv
External frozen version 02 input. Exact SHA-256 and shared path are recorded; source rows are excluded.
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