{"as_of":"2026-08-08T15:22:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ef227691a3f39fa5d53ceb5ad52220e54271fcdaefd9a04a6a970ea688ce94bb","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T00:15:14.178689Z","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":"2026-07-01T12:45:44.485226Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2503.07531","last_updated":"2025-06-24T16:40:53Z","snapshot_observed_at":"2026-08-07T17:16:07.614207Z","submitted_at":"2025-03-10T16:58:20Z","title":"Predicted Neutrino Signal Features of Core-Collapse Supernovae","version":2},"cited_work":{"arxiv_id":"2503.07531","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.07531","snapshot_observed_at":"2026-07-01T12:45:44.485226Z","title":null,"venue":null,"work_id":"0cc9ad90-302a-459f-8a7d-632b5497cc8e","year":2025},"citing_paper":{"arxiv_id":"2605.01099","last_updated":"2026-08-05T20:26:40Z","snapshot_observed_at":"2026-08-08T15:15:25.106609Z","submitted_at":"2026-05-01T21:08:36Z","title":"Three-flavor supernova neutrino simulation using a hybrid quantum-classical algorithm with qutrits","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-09T18:25:40.957080Z"},"links":{"cited_paper":"/paper/2503.07531","citing_paper":"/paper/2605.01099"},"observation_digest":"sha256:ff52ffa06dc4b4cce5eb713d36ea692e26e24e2bad97fca9bbcd3145686bbdd3","observation_id":"dbc49e01-dced-467e-8d13-f9fb8e8bad27","resolution":{"observed_at":"2026-05-11T16:16:06.914671Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.07531","last_updated":"2025-06-24T16:40:53Z","snapshot_observed_at":"2026-08-07T17:16:07.614207Z","submitted_at":"2025-03-10T16:58:20Z","title":"Predicted Neutrino Signal Features of Core-Collapse Supernovae","version":2},"cited_work":{"arxiv_id":"2503.07531","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.07531","snapshot_observed_at":"2026-07-01T12:45:44.485226Z","title":null,"venue":null,"work_id":"0cc9ad90-302a-459f-8a7d-632b5497cc8e","year":2025},"citing_paper":{"arxiv_id":"2606.30756","last_updated":"2026-06-29T18:00:51Z","snapshot_observed_at":"2026-07-07T00:04:34.491408Z","submitted_at":"2026-06-29T18:00:51Z","title":"Parameterizing the Standing Accretion Shock Instability for Inference with Galactic Supernova Neutrino Signals at IceCube","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-07-01T01:47:53.424100Z"},"links":{"cited_paper":"/paper/2503.07531","citing_paper":"/paper/2606.30756"},"observation_digest":"sha256:d8569c09c21782ba8101d31a11b5e3442d75cdd314b0ababcb2018e4893648cb","observation_id":"912529a9-37a5-48cd-89fd-6f4634122781","resolution":{"observed_at":"2026-07-01T12:45:44.486636Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.07531","last_updated":"2025-06-24T16:40:53Z","snapshot_observed_at":"2026-08-07T17:16:07.614207Z","submitted_at":"2025-03-10T16:58:20Z","title":"Predicted Neutrino Signal Features of Core-Collapse Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.07531","snapshot_observed_at":"2026-08-01T23:35:21.835487Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.15392","last_updated":"2026-07-16T18:43:32Z","snapshot_observed_at":"2026-08-06T08:46:15.300374Z","submitted_at":"2026-07-16T18:43:32Z","title":"Solar-System Abundances of $p$-Nuclides Probe Collective Neutrino Oscillations in Supernovae","version":1},"reference_index":107,"source":"pdf_text","source_observed_at":"2026-08-01T23:35:21.835487Z"},"links":{"cited_paper":"/paper/2503.07531","citing_paper":"/paper/2607.15392"},"observation_digest":"sha256:83416574859d3c4b376bb34e0b06a1861f1865543e811b50eac49b97225f33d9","observation_id":"6dc49aa3-0fea-4b2f-96cb-cd851bc12f45","resolution":{"observed_at":"2026-08-01T23:35:21.835487Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.07531","last_updated":"2025-06-24T16:40:53Z","snapshot_observed_at":"2026-08-07T17:16:07.614207Z","submitted_at":"2025-03-10T16:58:20Z","title":"Predicted Neutrino Signal Features of Core-Collapse Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.07531","snapshot_observed_at":"2026-08-07T00:15:14.178689Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.02747","last_updated":"2026-08-03T18:00:20Z","snapshot_observed_at":"2026-08-08T11:33:03.473485Z","submitted_at":"2026-08-03T18:00:20Z","title":"A \"Neutrino Fog\" For Gravitational Waves: The Stochastic Gravitational Wave Background from Supernova Neutrino Memory","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-07T00:15:14.178689Z"},"links":{"cited_paper":"/paper/2503.07531","citing_paper":"/paper/2608.02747"},"observation_digest":"sha256:e81b9fb8f81983b6b125fc1065a35eca79b1b3dcf035cd38bcde8de55cbc2bb2","observation_id":"7f3749a3-05e2-40d9-9fca-dfea0f880a4a","resolution":{"observed_at":"2026-08-07T00:15:14.178689Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2503.07531/citation-record","integrity":"/paper/2503.07531/integrity","json":"/paper/2503.07531/citation-record.json","paper":"/paper/2503.07531"},"outbound":[],"paper":{"arxiv_id":"2503.07531","last_updated":"2025-06-24T16:40:53Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-07T17:16:07.614207Z","submitted_at":"2025-03-10T16:58:20Z","title":"Predicted Neutrino Signal Features of Core-Collapse Supernovae"},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2503.07531."}