Contribution seq 13354

CREATE_SOURCE_LOCATION EPISTEMIC custody SERVER ACCEPTED server-held key

Signer ed25519:71858824de92da3c8a83b5ff952e4b603e916138eda4ec764837c12e1efd24fe · received 2026-09-28T23:14:11.831366Z · client time 2026-09-28T23:14:11Z

client signature: verifies server signature: verifies chain: intact

prev sha256:270be208f1ad3b213615f4a7680e4d347475ece138dbfe29cef5f85fdac0cbed
entry sha256:a6a9e10b75edd0e931b77d1f8ef9236abf96fad14cb4c7d421916e02f1e813e6
envelope sha256:1be33cb731d9e2690a40653dbaa40a10d62c27f3d57763200d8dfa04495ef1e5
payload sha256:163a710e2817c394c3a310e72ed6fe380c588fc9fe4477ce6c28c8e60e01aff5

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

Payload

{
  "excerpt": "The object is one of nine new brown dwarfs confirmed by the James Webb Space Telescope in a deeper survey of IC 348, a star-forming region about 1,000 light-years away in Perseus. The Astrophysical Journal Letters study extends the population of spectroscopically classified brown dwarfs down to an estimated two Jupiter masses.",
  "locator": {},
  "source_id": "9860b717-c45c-81c1-b86d-5ffebe61fefa",
  "excerpt_hash": "sha256:ee9a272106f40c1fb6aa10c4b2d7ec817d0ce2f33fc254c2be0e894a9011cf82",
  "locator_type": "QUOTE"
}

Rows created

SourceLocation d2bf1e35-097f-886c-9d93-aa6ffece7345

Status history

seq	event	detail
13354	APPENDED
13355	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}