{"as_of":"2026-08-17T04:55:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:03e72c6e040fd479aee28c0f45ab5277875980e2c648a0e6300a8fa0f0d55444","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T19:10:39.502517Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-16T13:42:56.174853Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2302.04130","last_updated":"2023-07-06T07:38:50Z","snapshot_observed_at":"2026-08-16T15:56:47.811418Z","submitted_at":"2023-02-08T15:27:05Z","title":"High-energy neutrino emission associated with gravitational-wave signals: effects of cocoon photons and constraints on late-time emission","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.04130","snapshot_observed_at":"2026-08-15T19:10:39.502517Z","title":"Matsui, S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.17581","last_updated":"2025-06-21T04:25:17Z","snapshot_observed_at":"2026-08-15T22:07:15.499268Z","submitted_at":"2025-06-21T04:25:17Z","title":"Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-15T19:10:39.502517Z"},"links":{"cited_paper":"/paper/2302.04130","citing_paper":"/paper/2506.17581"},"observation_digest":"sha256:3079f8d3cfb2065fed55b19e3043211cd00e85e8a73730086e25f045b15a6bd8","observation_id":"fbe07b3d-101a-4fce-9d08-1548114d30cb","resolution":{"observed_at":"2026-08-15T19:10:39.502517Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.04130","last_updated":"2023-07-06T07:38:50Z","snapshot_observed_at":"2026-08-16T15:56:47.811418Z","submitted_at":"2023-02-08T15:27:05Z","title":"High-energy neutrino emission associated with gravitational-wave signals: effects of cocoon photons and constraints on late-time emission","version":2},"cited_work":{"arxiv_id":"2302.04130","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.04130","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Matsui, S","venue":null,"work_id":"eb456fe9-6faa-40fc-afcf-63a91796efb6","year":2023},"citing_paper":{"arxiv_id":"2601.11203","last_updated":"2026-04-03T05:44:30Z","snapshot_observed_at":"2026-07-06T22:41:53.823272Z","submitted_at":"2026-01-16T11:26:42Z","title":"Little Red Dots as Hidden Neutrino Sources","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-05-16T13:42:07.307781Z"},"links":{"cited_paper":"/paper/2302.04130","citing_paper":"/paper/2601.11203"},"observation_digest":"sha256:14e1412fb6efa908f778a163dc4b1bb96bd785d8df97efede9629444b2c1ecf2","observation_id":"f88cd2e8-06fc-4cb7-82df-48995d60649d","resolution":{"observed_at":"2026-05-16T13:42:56.177057Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2302.04130/citation-record","integrity":"/paper/2302.04130/integrity","json":"/paper/2302.04130/citation-record.json","paper":"/paper/2302.04130"},"outbound":[],"paper":{"arxiv_id":"2302.04130","last_updated":"2023-07-06T07:38:50Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-16T15:56:47.811418Z","submitted_at":"2023-02-08T15:27:05Z","title":"High-energy neutrino emission associated with gravitational-wave signals: effects of cocoon photons and constraints on late-time emission"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2302.04130."}