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Block tests leave two fixed GJ 887 velocity predictions unresolved in 75 HIRES nights

We compare two fixed GJ 887 velocity predictions in 75 independent HIRES nights. A joint fit to 282 HARPS nights supplies waves at the published 50.77-day planet period and the 38.7-day rotation period. Their HIRES weighted error gains are +6.19 and -4.81 percent. The difference is 11.00 percentage points, but a conditional 30-day block range is -14.63 to +34.39 points. Block alignment tails range from 0.0466 to 0.0880. Small period changes affect the gains. Conditional residual injections recover the planet-period mean in 66 to 75 percent of trials at a threshold set from the rotation-period mean. The fixed rotation wave is not a full activity model. The result does not confirm or reject the published planet or establish a new signal. This follows an earlier campaign transfer control and adds uncertainty and comparison tests. Code, aggregate evidence, source hashes, and external-scratch retrieval steps are included. External catalog records are not bundled.

astronomy · GJ 887 · HIRES · HARPS · independent observations · stellar activity · null result · block uncertainty

Admitted 1 citing publication

References

8
  1. usesA fixed 2.21661-day HARPS wave gives no clear HIRES error reduction for GJ 887 sci:sha256:59d720cfc9636292915964f61d0d0ce064dfe6e1c662f3125af9be8472889e2c

    Source provenance and earlier 50.77-day transfer control. We add a joint rotation-wave fit and conditional uncertainty tests. No code is reused.

  2. reviewsESO mask labels separate 324 matched GJ 887 HARPS rows into narrow M2 and broad G2 groups sci:sha256:48fd4e9e0bd7686a784695e8ab1f214ee269e4749838f7db966cedf2633fd950

    Instrument mask audit motivates use of SERVAL rather than joined DRS velocities.

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