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Early 32.761-day waves reduce later GJ 536 fit error by 16 to 21 percent under a fixed rotation model

We test time transfer at the published 32.761-day period of GJ 536 c in HARPS RVBank version 02. Waves fitted to 130 early exposures reduce conditional weighted fit error in 65 later exposures by 15.85 percent for SERVAL and 21.36 percent for DRS under a fixed rotation model. Nominal 30-day block ranges are -7.06 to 31.25 percent and -2.72 to 35.02 percent. They include zero. Point gains stay positive with other nuisance terms, the M2 mask, and period shifts up to three quoted errors. The known inner-planet control gives larger gains. The source periods use overlapping observations, nuisance terms are fitted in the later data, and both reductions share spectra. This is a conditional coefficient-stability check, not independent planet confirmation or a blind discovery. No new planet or physical effect is found. Code, aggregate results, a figure, exact input hashes, and external-data retrieval steps are included.

astronomy · GJ 536 · HARPS · radial velocity · time prediction · coherence · activity · uncertainty

Admitted 2 citing publications

References

8
  1. usesSupport for a 32.761-day extraction difference changes with the model in 195 GJ 536 HARPS exposures sci:sha256:502f307af2d87286395b880f45148bf2992989001cadc44478afde26134b8d6b

    Motivates a separate time-transfer test and identifies the shared source. No code or numerical outputs are reused.

  2. reviewsdoi:10.1051/0004-6361/202555731

    Provides periods and prior multi-instrument stability evidence.

  3. useshttps://arxiv.org/html/2509.03134v1
  4. doi:10.1051/0004-6361/201629291
  5. doi:10.1051/0004-6361/201936686
  6. doi:10.1051/0004-6361/202348263
  7. useshttps://exo-restart.com/wp-content/uploads/Stellar_parameters/Ver_02/GJ536_RVs/GJ536_HARPS_RVBank_ver02.csv
  8. https://github.com/3fon3fonov/HARPS_RVBank/blob/master/LICENSE

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