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2023 Barnard's Star date means give a positive 4.1244-day band term at the 2021–2022 phase under independent Gaussian errors

We test whether a known blue minus red velocity feature in Barnard's Star repeats between observing seasons. We use 112 published MAROON-X velocity pairs to form 103 daily groups in BJD. All four published periods stay fixed. A fit to 2021 and 2022 sets the direction of the 4.1244-day sine and cosine pair. Its signed projection in 23 date means from 2023 is 0.449 m/s. A separate 95% Student t interval is 0.139 to 0.760 m/s. This interval assumes independent Gaussian date errors and relative variances from the quoted channel errors. The model uses separate run lines and one unknown variance scale in 2023. Constant and quadratic run trends give 0.452 and 0.463 m/s. The interval includes zero under two fixed damped cosine noise models with a 10-day decay time. Thus the evidence for a repeated band term depends on the error model. The test is retrospective. The period and feature were already selected with these observations. This is not a new independent detection, and the physical cause is not identified. We also give four model-based simultaneous 95% upper bounds on band amplitude. For b, c, d, and e, these are 0.477, 0.690, 0.450, and 0.412 m/s under the primary model. The package preserves source files, code, provenance, results, figures, and reproduction instructions.

Barnard's Star · MAROON-X · radial velocity · wavelength dependence · time split · conditional inference

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References

5
  1. usesdoi:10.3847/2041-8213/adb8d5

    Table 4 supplies the paired velocities. Table 3 supplies fixed periods and context amplitudes.

  2. Linear run fits give a 0.36 m/s channel difference at 4.1244 days in 112 Barnard's Star velocity pairs sci:sha256:1b1ebba0e713f6ff12035cf68382cef4baa61193f29073e219c94933f9a80e20

    [Legacy relation: reproduces] Our all-112-epoch linear fit reproduces its combined 4.1244-day band difference. We add seasonal phase tests and simultaneous bounds.

  3. Quadratic run fits to 112 Barnard's Star epochs give a 0.356 m/s channel difference at 4.1244 days sci:sha256:d0bfd601542d60c099cdad0057a9fcc3aaaece94f001492c4534a33b7abf7f86

    This earlier quadratic study also reports the same combined feature and extensive controls. Our contribution is the seasonal extension.

  4. Three fixed HARPS curves show no detected blue to red velocity difference in 25 ESPRESSO nights of HD 32564 under independent nightly errors sci:sha256:448fb9367d48c9f2d1a4bb65ec90a0df7a4a094f35ab0542b75cc58e5d70f867

    This study gives a paired band test for a different star with coefficients on fixed curves.

  5. Six fixed noise models give conditional 95% CARMENES amplitude bounds of 0.720–1.444 m/s for Barnard's star at eccentricity 0.306 on a finite 58.59–58.88-day orbit grid sci:sha256:b12513edcdb07eec8743e1f817d48399bb036020afa45592ade925a668fba6ec

    This earlier CARMENES study gives conservative coefficient-ellipse amplitude bounds under fixed covariance models for a different Barnard candidate. Our observations and tested periods differ.

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