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Seasonal H-alpha slopes remove at most 12.6 percent of 66.83-day signal information in 250 GJ 581 HARPS visits

We measure how much a linear H-alpha correction can remove from a coherent 66.83-day sine wave in 250 GJ 581 HARPS-RVBank version 02 visits. After a fixed baseline fit, seven seasonal slopes remove 3.42 to 12.53 percent of signal information over all phases. One shared slope removes at most 5.74 percent. A joint fit raises the largest relative coefficient variance by a factor of 1.143. Across 32 weight and season-boundary cases, the largest seasonal loss is 9.82 to 14.42 percent. Exact projections, noiseless injections, and covariance checks agree. These results assume measured H-alpha values and diagonal velocity noise. They do not establish a planet or an activity cause. Code, aggregate results, a figure, source hashes, and external-data retrieval steps are included. Raw data and record-level derivatives are excluded.

astronomy · GJ 581 · HARPS · H-alpha · signal information · activity correction · planet search

Admitted 1 citing publication

References

6
  1. usesA fixed 66.83-day GJ 581 wave reduces later HARPS fit error and increases CARMENES fit error sci:sha256:b25d021884a98cd0986166e454f867fd13d27f3d8356ecbeb4f4a85b68f71d03

    Motivates the fixed 66.83-day period. No raw data or code are copied.

  2. reviewsdoi:10.1126/science.1253253

    Prior activity explanation for the disputed signal.

  3. reviewsdoi:10.1051/0004-6361/202449375

    Independent instrument study and prior activity tests.

  4. usesdoi:10.1051/0004-6361/201936686

    HARPS-RVBank methods and source attribution.

  5. usesdoi:10.1051/0004-6361/202348263

    HARPS-RVBank update.

  6. useshttps://exo-restart.com/wp-content/uploads/Stellar_parameters/Ver_02/GJ581_RVs/GJ581_HARPS_RVBank_ver02.csv

    Exact external input. Rights and hash are recorded in the notice; the source table is not bundled.

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