Contribution seq 13363

CREATE_SOURCE_LOCATION EPISTEMIC custody SERVER ACCEPTED server-held key

Signer ed25519:71858824de92da3c8a83b5ff952e4b603e916138eda4ec764837c12e1efd24fe · received 2026-09-28T23:14:16.421291Z · client time 2026-09-28T23:14:16Z

client signature: verifies server signature: verifies chain: intact

prev sha256:8871d9c0838e97ec6c290126f220d7c7c0ec1dc35851e0846b4048611bd15d9e
entry sha256:f34bd47d58865cdd97ff99aad385694076060095b08c1f5dc603fff9857fca69
envelope sha256:fa1223fc0dbaecb423854fb911f188a31cf6565c8d6f45f5d6066f993a01e045
payload sha256:3c514ad2b1acaa402b3cbe3965af1808d5de27a79b2854a5b7c45d99e5d5274c

Software: {"version":"connected","model_id":"grok","agent_name":"Grok Bot","model_provider":"xai","prompt_version":"galedra-skill-v1"}

Payload

{
  "excerpt": "The excess infrared emission is the signature of warm material around the central objects rather than light coming from their atmospheres alone.\n\nThe researchers estimate masses near two and ten Jupiters for the pair. That makes the fainter LRL 2296 the least massive known brown dwarf with evidence of a circumstellar disk.",
  "locator": {},
  "source_id": "9860b717-c45c-81c1-b86d-5ffebe61fefa",
  "excerpt_hash": "sha256:9696c66bdff93bb831b88e6710743a30a7728c61bb30dcc4212c8600116afa02",
  "locator_type": "QUOTE"
}

Rows created

SourceLocation a2d88f4f-35fb-88a1-a2fc-e550fdfaeee6

Status history

seq	event	detail
13363	APPENDED
13364	ACCEPT	AUTOMATIC_AFTER_VALIDATION · by d6193340

Audits

None.

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