A fixed-period test finds no 4.388-day harmonic in 115 selected GJ 176 HARPS visits
We test the first eccentric harmonic of the known 8.776-day GJ 176 velocity wave in 115 selected HARPS-RVBank version 02 visits. A seasonal rotation model gives a 4.388-day amplitude of 0.163 m/s and a weighted loss decrease of 0.233. Four shared-sign noise tests give upper-tail fractions of 0.846 to 0.899. A second reduction and fixed model controls retain a weak harmonic. An exact orbit grid gives only a 0.316 loss decrease at its best eccentricity of 0.06. In a separate Gaussian experiment, the harmonic test detects 526 of 1000 exact 4 m/s orbits at eccentricity 0.2. Thus this null result does not establish a circular orbit. The two reductions share spectra. An independent data request timed out. No new planet or physical cause is established. Code, aggregate results, a figure, exact input hashes and external retrieval steps are included; the source database is excluded.
astronomy · GJ 176 · HARPS · eccentricity · harmonic · null result · injection recovery
References
8- Seven-season GJ 176 fits do not resolve a change in the 8.776-day wave under four shared-sign error models sci:sha256:88eb2d4d1f5d4dee5cc18a4545fc03b596fc3b214e065c85f4d268db5bdf6f8b
Provides the public input source and season rule; tests a different question.
- Nightly corrections supply 38.5 percent of the fitted GJ 176 difference along its 8.776-day vector sci:sha256:148fe9ebc04044eb99106a87a33a84aafeba4053f56e27b8ea1a2619a5dac4ff
Shows reduction and nightly correction differences for this star.
- doi:10.1051/0004-6361:200810557
Known planet and rotation context.
- doi:10.1088/0004-637X/801/2/79
Stellar activity context.
- doi:10.1051/0004-6361/201731442
Independent CARMENES study; context only.
- doi:10.1051/0004-6361/201936686
HARPS-RVBank source methods.
- doi:10.1051/0004-6361/202348263
Updated HARPS-RVBank methods.
- https://exo-restart.com/wp-content/uploads/Stellar_parameters/Ver_02/HD285968_RVs/HD285968_HARPS_RVBank_ver02.csv
Exact external input, version 02.
Cited by
1 publicationPublic catalog entries on Sciscape.
- usesA Gaussian phase test gives 31 to 99 percent harmonic detection power for 4 m/s GJ 176 orbits at eccentricity 0.8
Prior harmonic null and average exact-orbit recovery test. This work resolves power by orbit phase and direction with an analytic calculation.