Order 75 has a fitted amplitude of 58.5 m/s at 365.25 days relative to a fixed reference in 345 GJ 411 CARMENES spectra
We test public CARMENES DR1 order velocities for GJ 411. We select 345 spectra from 2016 to 2020. Each order is compared with a fixed weighted reference from all 42 populated orders. A velocity shared by all orders cancels from each difference. Physical order 75, array index 43, has a fitted semi-amplitude of 58.52 m/s at a fixed period of 365.25 days. The fit includes a constant and linear trend. Fits that omit one observing year give 53.76 to 62.44 m/s. A residual sign test uses the largest fit gain over all 42 orders. With 90-day blocks, 9 of 49,999 draws reach the observed gain. The tail probability is 0.00020 under this approximate block model. It assumes independent blocks with errors symmetric under a shared sign change. The test does not cover all period or model choices. In two band differences, the 215.7-day candidate test has a 30-day block probability of 0.07508. With annual and half-year terms, this probability is 0.30860. The result does not confirm or reject the planet candidate. Earlier work reported annual changes in GJ 411 activity indices. We locate a large order difference and release fixed-weight diagnostics. We do not identify its cause or measure an error of this size in the final scalar stellar velocity. The package contains derived data, code, figures, source records, and reproduction instructions. A fresh source download gives the same results. Separate QR fits check the results from the derived data.
GJ 411 · Lalande 21185 · CARMENES DR1 · radial velocity · spectral orders · annual variation · chromatic diagnostics · fixed weights · block bootstrap · reproducible data
References
6- usesdoi:10.1051/0004-6361/202244879
We use the public CARMENES DR1 order velocities and quality fields for GJ 411 through the GAVO TAP service.
- usesdoi:10.1051/0004-6361/201731483
We use the SERVAL order field definitions and their documented m/s units.
- usesdoi:10.1051/0004-6361/202038820
We compare our differences with the published chromatic index on matched observation dates. This paper already reported annual changes in activity indices.
- usesdoi:10.3847/1538-3881/ac5c47
We use the reported 215.7-day candidate period and control periods. Our differential tests cannot confirm or reject a common planet velocity.
- doi:10.48550/arXiv.2603.03643
This study reports long-term changes in GJ 411 SOPHIE activity indices. It gives context for the limits of activity tests.
- usesAn audit of 18 scalar fields finds nine unit conflicts and two shifted rows in the 2026-10-22 CARMENES TAP snapshot sci:sha256:138b7b39e5d6373fba7cbcb99454063cf490824fbde87295f0522a88b41bc9f7
Its scalar-field unit audit informed our unit checks. We add an order-array scale check and measure order differences; the audit did not test these arrays.
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