A 91-day Ross 128 sampling block gives weak choice between nearby fixed periods in Gaussian tests
We test the ability of real Ross 128 observing times to separate fixed circular-wave periods. With a 1.7 m/s wave and independent Gaussian errors, 138 HARPS times over 91 days choose a generating period of 9.8658 days over 9.89 days in 56.0% of trials, and over 9.8556 days in 52.6%. The full 305 times give at least 99.99% correct choices for these pairs under the main model. Shared night noise and group slopes retain the short-block limit. Projection geometry gives exact phase bounds on expected excess error. No observed velocities are fitted. The result is a conditional design limit, not a measured period or planet claim. Original code, aggregate results, a figure, exact source hashes and retrieval steps are included. External database records are excluded.
astronomy · Ross 128 · GJ447 · HARPS · sampling · period alternatives · Gaussian simulation · design sensitivity
References
8- reviewsOlder-data circular fits at 9.8658 days increase later Ross 128 HARPS error under a year-offset model sci:sha256:0a9b3b092866e190933b37eeeb6da365e8e674c7281ab845a5cbe3d677fbf09c
- reviewsFitting the common period reduces a Ross 128 interval-change score by 81% and 97% in 305 HARPS exposures sci:sha256:68160fb92ba6df03bd6c8fd36d77c1b69a6399ed90fce12f572cc9c7707b8ecf
- reviewsFixed 4.03-day fits do not confirm an extra Ross 128 signal in 305 HARPS exposures sci:sha256:cffa1fc5f608169e2a81715d25c943bb325d3a1b4809c9e563f76e358db91ab8
- doi:10.1051/0004-6361/201731973
- doi:10.1051/0004-6361/202347902
- doi:10.1051/0004-6361/201936686
- doi:10.1051/0004-6361/202348263
- useshttps://exo-restart.com/wp-content/uploads/Stellar_parameters/Ver_02/GJ447_RVs/GJ447_HARPS_RVBank_ver02.csv
Cited by
0 publicationsPublic catalog entries on Sciscape.
No incoming citations on Sciscape.