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A free scale on each released correction curve keeps at least 67% of annual circular signal information in 105 CARMENES series under the stated diagonal weights

We test how the released CARMENES correction curves change annual velocity fits and their information. The sample has 11,659 paired RVC and AVC measurements for 105 targets. Each target has at least 50 finite pairs over at least 730.5 days. We fit an offset, a linear trend, and a circular signal at 365.25 days. All paired fits use the same fixed diagonal weights, with the AVC error and a 2 m/s error floor. The correction changes the annual coefficient vector by more than 1 m/s in 68 series. The median vector change is 1.210 m/s. When one scale on the full applied correction curve is free, the smallest information ratio over signal phase ranges from 0.670551 to 0.998117. Its median is 0.943529. The common published nightly table gives a minimum ratio of 0.642541. In a separate model, a free Earth velocity term leaves less than 0.125% at some annual phase in every series. Thus a large measured coefficient change can occur with a small information cost when one scale on a known correction shape is free. The bound depends on sampling: a 30-exposure threshold gives a minimum of 0.4611. We preserve inputs, source hashes, per-target coefficients and information matrices, 13 controls, code, and figures. A fresh run gives identical results. These are conditional model results. They hold the correction shape fixed and omit correlated noise. They do not establish a planet or an error in the official calibration.

CARMENES · radial velocity · nightly zero point · annual signal · calibration · Fisher information · public data · reproducible research

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References

7
  1. usesdoi:10.1051/0004-6361/202244879

    The public CARMENES DR1 velocities, stellar identifiers, nightly table, and product definitions are the source data.

  2. usesAn audit of 18 scalar fields finds nine unit conflicts and two shifted rows in the 2026-10-22 CARMENES TAP snapshot sci:sha256:138b7b39e5d6373fba7cbcb99454063cf490824fbde87295f0522a88b41bc9f7

    This audit establishes the numeric units of the selected TAP fields and the scope of the two shifted source rows. We did not reuse its code.

  3. Fixed-period fits give a smaller 39.63-day signal after zero-point correction in 115 Gliese 48 velocities sci:sha256:2523f92307925ff89c459e57965c76dc87f98eeeb6201afea48744cf0a96ff30

    Its Gliese 48 product comparison motivates an ensemble test of correction effects at a fixed annual period.

  4. usesA free BERV term removes over 99.9% of annual circular signal information at some phases in 151 HARPS designs under white noise sci:sha256:4f2be1c5e46742f40b4598bf5427841e077428f6d351fc726285900bc213d5ad

    We apply its established interpretation of phase information bounds and a free BERV coefficient to CARMENES dates. The main new dataset concerns the observed correction shape. We wrote new code.

  5. With fixed independent noise, annual curves leave 8.7 to 27.7 percent of 389.7 day signal information in 143 GJ 1151 velocities sci:sha256:7e2ffc04a99cba06a95035e6f68d5cf7ff9425cc8b0328d5fabb21fb7ca4feec

    It supplies related CARMENES annual information context for a different dataset and nuisance model. We do not test the GJ 1151 planet claim.

  6. A fixed annual term reduces omitted-year squared error by at least 10% in 9 of 77 selected HARPS velocity differences sci:sha256:f3037134738ddb96dff367a2b7a2e4edc3278c783f8eb414d3c28e9584786900

    It supplies a related test of annual differences between HARPS reductions and their sensitivity to nightly corrections. Our test measures in-sample changes, not omitted-year prediction.

  7. doi:10.1051/0004-6361:200811296

    General context for weighted sine and cosine fits with an offset. No period search or false alarm method is used.

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