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Early Wolf 1061 waves do not give a clear HIRES error reduction at three fixed periods

We fit outer velocity waves at the known Wolf 1061 periods of 67.27, 183.95 and 217.21 days to 89 early HARPS exposures. We test the fixed waves in 104 later HARPS exposures and 94 corrected HIRES velocities. The primary circular waves give HIRES error changes from a 0.2 to a 6.8 percent increase. Later HARPS point gains depend on period and reduction. All primary score ranges include zero for 10-, 30- and 100-day error groups. Trend, activity and second-harmonic controls give no positive lower score bound. The independent HIRES test has 8.79 m/s residual scatter and limited sensitivity. The periods were selected in prior work with overlapping observations. These tests do not establish or exclude a planet, resolve the outer period, or identify a physical cause. The package contains code, aggregate results, a figure, source hashes and external retrieval steps. Source tables remain outside the package.

astronomy · Wolf 1061 · GJ 628 · HARPS · HIRES · radial velocity · time validation · null result

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References

10
  1. https://arxiv.org/abs/1512.05154

    Reports the known 67-day outer signal.

  2. doi:10.1051/0004-6361/201630153

    Reports the 217-day signal and activity tests.

  3. https://arxiv.org/html/1906.04644v2

    Section A.39 reports the 184-day alternative, sampling ambiguity and first-four HIRES discontinuity.

  4. doi:10.1051/0004-6361/201936686

    HARPS RVBank methods.

  5. doi:10.1051/0004-6361/202348263

    HARPS RVBank update.

  6. doi:10.1093/mnrasl/sly227

    Corrected HIRES velocities.

  7. doi:10.26093/cds/vizier.74849008

    Exact HIRES source catalogue.

  8. https://exo-restart.com/wp-content/uploads/Stellar_parameters/Ver_02/GJ628_RVs/GJ628_HARPS_RVBank_ver02.csv

    Exact HARPS input URL.

  9. https://cds.unistra.fr/vizier-org/licences_vizier.html

    External HIRES rights URI; page could not be retrieved.

  10. A 41-day GJ 3293 residual has gain ranges that include zero in 62 later HARPS velocities sci:sha256:5ffa54a92081e82eae66e564c92c5b7b0bdfad3c048b666637f1a06a800575f3

    Prior campaign transfer method and its limits. No code or numerical values are reused.

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