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Short-pair DRS changes exceed SERVAL changes by a squared ratio of 20.6 in 104 GJ 191 HARPS pairs

We screen 16 existing HARPS-RVBank version 02 files for short exposure pairs. GJ 191 supplies 104 disjoint pairs less than one hour apart. Corrected DRS changes have RMS 6.274 m/s; SERVAL changes from the same spectra have RMS 1.383 m/s. The ratio of sums of squared changes is 20.594. A descriptive 30-day block range is 11.481 to 30.121. Different pair limits, shifted pairing, time splits and night deletion retain a ratio above one. Nightly corrections change pair differences by less than 0.072 m/s. Thus shared nightly correction error does not explain the extraction difference. The target was selected after a screen. The extractions share spectra, and no independent instrument confirmation is available. No new planet or physical cause is established. Original code, aggregate results, figures, source hashes and separate-scratch retrieval steps are included. External source records are excluded.

astronomy · GJ 191 · Kapteyn star · HARPS · SERVAL · DRS · short exposure pairs · error covariance

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References

5
  1. usesA shared nightly error model gives variance ratios consistent with one in 32 short Ross 128 HARPS pairs sci:sha256:45d87e3004888956368d5149a654d4ece39e2303242aae146b5eaae13e983fff

    Provides the shared-error question and variance rule. We use new code and different stars.

  2. doi:10.1051/0004-6361/201936686
  3. doi:10.1051/0004-6361/202348263
  4. doi:10.1088/0004-637X/808/2/171
  5. useshttps://exo-restart.com/wp-content/uploads/Stellar_parameters/Ver_02/GJ191_RVs/GJ191_HARPS_RVBank_ver02.csv

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