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A first harmonic does not improve later SERVAL predictions for GJ 3341 at a fixed 14.207-day period

We test whether a first harmonic of the known GJ 3341 b signal improves prediction from 61 early HARPS visits to 74 later visits. At a fixed 14.207-day period, corrected SERVAL mean square error rises by 0.616 percent. A 10-day block resampling gives a central 95 percent gain range from -26.28 to +6.89 percent. Corrected DRS gives a small gain and uncorrected SERVAL gives a loss. The products share spectra. In 5000 exact-orbit injections with eccentricity 0.31, amplitude 3.036 m/s and independent Gaussian errors, 36.38 percent give a gain at most the observed value. Thus the null forecast result cannot reject the reported eccentric orbit. Period controls change the sign of the small gain. No new planet, eccentricity constraint or independent telescope confirmation is reported. Code, exact input, hashes, controls, prediction rows, simulations and offline steps are included.

astronomy · GJ 3341 · HARPS · radial velocity · eccentricity · harmonic · prediction · null result

Admitted 1 citing publication

References

8
  1. usesAn early 15.052-day GJ 3341 residual wave does not reduce later SERVAL error in 74 HARPS exposures sci:sha256:071303675e3ace36de1941a622b6240b6eec4a2788cc451cc632b205be6cec5a

    Provides the sample rule and time split. It tests a different extra period.

  2. usesA bounded planet-period error gives less than 0.938 m/s of the early GJ 3341 residual sci:sha256:c3c027b931e792a62b2afdb9bee75afb79c86e4113438f89f32b907796acc0f2

    Provides the fixed planet-period context and prior harmonic nuisance model. No code is reused.

  3. reviewsA fitted common-wave null gives a 0.51 change-test tail fraction after early GJ 3341 period selection sci:sha256:f92ee6f46a242c0473cfcf25329e4b99160129edac49aa122e08dc67f39e89da

    Earlier change test for the separate residual wave.

  4. usesdoi:10.1051/0004-6361/201424253

    Reported planet period, amplitude and eccentricity motivate the test.

  5. usesdoi:10.1051/0004-6361/201936686

    Describes HARPS-RVBank reductions and instrument corrections.

  6. usesdoi:10.1051/0004-6361/202348263

    Describes the HARPS-RVBank update.

  7. reviewsdoi:10.1051/0004-6361/202346570

    Separate HARPS analysis recovers the known planet; it is not independent telescope evidence for orbit shape.

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

    Exact public input. Hash, shared path and snapshot are included.

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