Contribution seq 15999

CREATE_SOURCE_LOCATION EPISTEMIC custody SERVER ACCEPTED server-held key

Signer ed25519:71858824de92da3c8a83b5ff952e4b603e916138eda4ec764837c12e1efd24fe · received 2026-09-29T00:37:05.186480Z · client time 2026-09-29T00:37:05Z

client signature: verifies server signature: verifies chain: intact

prev sha256:2171edf3092becf0bbac4865644b123f3525854e809f95b73a794b9f1de2c768
entry sha256:5027fcec57d9fdd1c09e25698072b612dd4d833528fd44a429208649aad1d069
envelope sha256:541e60a85326a72b4050315def53616b37e7bd3bcc9ce8d1082bbaa9dd24711d
payload sha256:b5bc70ad47b44eda10549ffb428c306ca623e37c4a6891ff585f305b384b66f5

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

Payload

{
  "excerpt": "Here we report a detection of very-high-energy γ-ray emission from five nearby GMCs using a stacking analysis of 4.5 years of observations with the Large High Altitude Air Shower Observatory (LHAASO). The spectral energy distributions derived for the GMCs are consistent with the expected γ-ray flux produced via CRs interacting with the interstellar medium over 1–100 TeV.",
  "locator": {},
  "source_id": "698613c2-242a-83af-a541-c12ac25acb4c",
  "excerpt_hash": "sha256:62275b45a09c44978fb055246b33f4b9019e73cfa1985280d7272d9656763aaf",
  "locator_type": "QUOTE"
}

Rows created

SourceLocation ed32e01d-2769-8d9e-b2ae-d41dc4a41f4f

Status history

seq	event	detail
15999	APPENDED
16000	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}