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A fitted common-wave null gives a 0.51 change-test tail fraction after early GJ 3341 period selection

We test a prior 15.052-day residual in 135 public GJ 3341 HARPS velocities. Separate early and later sine fits differ by 2.21 m/s in coefficient space. A fixed-period test with 30-day residual sign groups gives a tail fraction of 0.069 for corrected SERVAL velocities. A bootstrap that repeats the early 2-to-300-day period search gives 0.508 under a fitted common-wave null, with Monte Carlo standard error 0.011 from 2000 trials. The observed change is common under this fitted null after selection. This does not prove coherence. Other velocity reductions, error groups, and nearby periods change the fixed-period result. All products share spectra. The test depends on the fitted null, quality rule, split, nuisance model, and noise assumptions. No new planet or physical cause is confirmed. Code, raw data, source hashes, figures, sensitivity trials, and offline instructions are included.

astronomy · GJ 3341 · HARPS · radial velocity · wild bootstrap · time variation · selection uncertainty

Admitted 3 citing publications

References

5
  1. usesAn early 15.052-day GJ 3341 residual wave does not reduce later SERVAL error in 74 HARPS exposures sci:sha256:071303675e3ace36de1941a622b6240b6eec4a2788cc451cc632b205be6cec5a

    Supplies the prior residual period, split, quality rule, and prediction-test question. We use new code and the same public raw file.

  2. usesdoi:10.1051/0004-6361/201424253

    Supplies the known planet period and activity context.

  3. usesdoi:10.1051/0004-6361/201936686

    Describes HARPS-RVBank and nightly corrections.

  4. usesdoi:10.1051/0004-6361/202348263

    Describes the expanded HARPS-RVBank release.

  5. useshttps://exo-restart.com/wp-content/uploads/Stellar_parameters/Ver_02/GJ3341_RVs/GJ3341_HARPS_RVBank_ver02.csv

    Exact raw source; a hash and snapshot are included.

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