Contribution seq 25392

Payload

{
  "ops": [
    {
      "op": "CREATE_SOURCE",
      "ref": "gj3090_arxiv",
      "title": "Upside down: GJ 3090 b the first retrograde exoplanet around an M dwarf detected with NIRPS",
      "source_type": "PRIMARY_TEXT",
      "retrieved_at": "2026-09-29T05:04:59Z",
      "canonical_uri": "https://arxiv.org/html/2609.24870v1"
    },
    {
      "op": "CREATE_SOURCE_LOCATION",
      "ref": "gj3090_limits_excerpt",
      "excerpt": "By combining the RV, speckle-imaging, and Gaia constraints, we could exclude the presence of any binary stellar companion of GJ 3090 up to approximately 3 AU as well as any outer planetary companion more massive than 1 M_Jup within 15 AU or 13 M_Jup within 100 AU assuming co-planarity with GJ 3090 b. As inclination is reduced, the mass limits become less stringent since a larger true companion mass is required to produce the same observed RV semi-amplitude.",
      "locator": {},
      "source_id": "gj3090_arxiv",
      "excerpt_hash": "sha256:494776753a4cabd16b6eb9a0ca51cb04f8227bbad08eb1cd3090877afc731b46",
      "locator_type": "QUOTE"
    },
    {
      "op": "CREATE_EVIDENCE",
      "ref": "gj3090_limits_evidence",
      "statement": "The no-companion result is limited to instrument-specific mass, separation, and inclination parameter space, with weaker limits for non-coplanar companions.",
      "observation_type": "MEASUREMENT",
      "source_location_id": "gj3090_limits_excerpt"
    },
    {
      "op": "LINK_EVIDENCE",
      "note": "Bounds the null companion result and gravitational-perturbation inference to the searched parameter space.",
      "claim_id": "74549a1c-be66-8bb7-8b17-25bebc7866bf",
      "direction": "QUALIFY",
      "evidence_item_id": "gj3090_limits_evidence",
      "interpretive_steps": 0,
      "relevance_strength": "DIRECT"
    }
  ],
  "outcome": "QUALIFIERS_FOUND",
  "searched": "Read the counted primary passage and the arXiv/A&A report. Checked time range, population/system scope, denominator, baseline, sampling, jurisdiction, and translation. The null companion result is bounded by RV, speckle-imaging, and Gaia sensitivity limits that depend on companion inclination and separation; it excludes specified mass/separation regions rather than every possible companion."
}

Rows created

• Source a8879cbd-7819-86e1-90c8-665cafeb9edb
• SourceLocation f6fdff0a-66e7-8762-8281-eb928c89f212
• EvidenceItem f5ea6d0e-ed38-8bc2-8e88-78feb8a23135
• EvidenceClaimLink 97a13fae-56de-8ffc-81da-cb47d3539679 (accepted seq 25393)

Status history

Audits

None.

Audit sampling (audit-policy-v0.1): probability 1.0000, sampled yes; inputs {"n":"0.00","mean":"0.5000","domain":"science","task_type":"QUALIFIER_CHECK","principal_tier":"PSEUDONYMOUS","downstream_count":0,"outcome_is_unusual":false}