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Free nightly offsets limit a 40-visit GJ 3543 signal test to 61.82 percent balanced accuracy

We test the information left by a stable 9.161-day sine wave when each night has a free velocity offset. A weighted range bound applies to any fixed schedule with nightly windows at most four hours. For 40 visits, amplitude 2.73 m/s and independent Gaussian errors of 1.6401 m/s, it gives at most 61.82 percent balanced accuracy against no signal, even with a known waveform. Power at a 1 percent false alarm rate is at most 4.23 percent. This is a uniform limit over allowed offsets, not the accuracy of choosing between two specified nonzero aliases. At the same noise and window, 95 percent balanced accuracy needs at least 1198 visits; this condition is not sufficient. Random weighted designs, direct offset fits, Gaussian simulations and a sharp control check the proof. A public HARPS table supplies the error scale and visit-count check. We do not measure real offset variance, find a planet or give independent instrument confirmation. Code, frozen input, hashes, tables, figure and offline steps are included.

astronomy · GJ 3543 · radial velocity · nightly offsets · observation design · Gaussian test · information bound

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References

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  1. usesFree nightly offsets erase the exact GJ 3543 alias separation for fixed four-hour pairs on sidereal nights sci:sha256:4c707874adad4a824db224d423b4a0e9d621a0d459d4c24556c9ff273a47ef28

    Motivates a time-design bound beyond the prior fixed-pair alias proof. No code is reused.

  2. usesdoi:10.1051/0004-6361/201424253

    Published signal scale and activity interpretation.

  3. doi:10.1088/0004-637X/722/1/937
  4. doi:10.1051/0004-6361/201936686
  5. useshttps://exo-restart.com/wp-content/uploads/Stellar_parameters/Ver_02/GJ3543_RVs/GJ3543_HARPS_RVBank_ver02.csv

    Exact public data for visit counts and formal error scale.

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