{"as_of":"2026-08-08T05:50:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:5094732552676999051653b73c53b59bd2adf96b04da86dca10e8383d5aab581","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":9,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":9,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T22:12:03.199086Z","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":"2026-05-20T15:53:33.506659Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2501.15256","last_updated":"2025-03-04T05:03:37Z","snapshot_observed_at":"2026-07-06T20:26:07.715114Z","submitted_at":"2025-01-25T16:04:00Z","title":"Three-dimensional core-collapse supernova models with phenomenological treatment of neutrino flavor conversions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15256","snapshot_observed_at":"2026-08-07T22:12:03.199086Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.09260","last_updated":"2025-05-08T06:54:55Z","snapshot_observed_at":"2026-08-07T22:05:09.898623Z","submitted_at":"2025-02-13T12:18:57Z","title":"Spectral diversity in collisional neutrino-flavor conversion: flavor equipartition or swap","version":3},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-07T22:12:03.199086Z"},"links":{"cited_paper":"/paper/2501.15256","citing_paper":"/paper/2502.09260"},"observation_digest":"sha256:405451fd5fb86c8678a1615756666974f00a605ae993f2a0654ec490e4a8f933","observation_id":"f97ca351-936b-412a-a010-6073724fb857","resolution":{"observed_at":"2026-08-07T22:12:03.199086Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15256","last_updated":"2025-03-04T05:03:37Z","snapshot_observed_at":"2026-07-06T20:26:07.715114Z","submitted_at":"2025-01-25T16:04:00Z","title":"Three-dimensional core-collapse supernova models with phenomenological treatment of neutrino flavor conversions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15256","snapshot_observed_at":"2026-08-07T14:58:55.560887Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.16961","last_updated":"2025-07-18T18:00:34Z","snapshot_observed_at":"2026-08-07T14:50:13.266770Z","submitted_at":"2025-05-22T17:44:06Z","title":"Predicting the outcome of collisional neutrino flavor conversion","version":3},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-07T14:58:55.560887Z"},"links":{"cited_paper":"/paper/2501.15256","citing_paper":"/paper/2505.16961"},"observation_digest":"sha256:2bd96da15911046e26e58f2a37e22f73ad54b4323b5dcf9cffecf16de76f1024","observation_id":"0fadd55a-d5af-4d00-b5fb-fce6fd1fc481","resolution":{"observed_at":"2026-08-07T14:58:55.560887Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15256","last_updated":"2025-03-04T05:03:37Z","snapshot_observed_at":"2026-07-06T20:26:07.715114Z","submitted_at":"2025-01-25T16:04:00Z","title":"Three-dimensional core-collapse supernova models with phenomenological treatment of neutrino flavor conversions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15256","snapshot_observed_at":"2026-08-07T11:16:08.135268Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.03271","last_updated":"2025-06-03T18:01:04Z","snapshot_observed_at":"2026-08-07T11:04:59.384951Z","submitted_at":"2025-06-03T18:01:04Z","title":"Local-equilibrium theory of neutrino oscillations","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-07T11:16:08.135268Z"},"links":{"cited_paper":"/paper/2501.15256","citing_paper":"/paper/2506.03271"},"observation_digest":"sha256:8088338bfcef3076767d7a40642c7b7fd4c4fdb12603bf75ad550746690c4186","observation_id":"fd2111df-dbdd-4ca3-a3c0-44084a3d3976","resolution":{"observed_at":"2026-08-07T11:16:08.135268Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15256","last_updated":"2025-03-04T05:03:37Z","snapshot_observed_at":"2026-07-06T20:26:07.715114Z","submitted_at":"2025-01-25T16:04:00Z","title":"Three-dimensional core-collapse supernova models with phenomenological treatment of neutrino flavor conversions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15256","snapshot_observed_at":"2026-08-07T05:49:20.750063Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.07017","last_updated":"2025-07-25T07:27:58Z","snapshot_observed_at":"2026-08-07T05:41:31.263588Z","submitted_at":"2025-06-08T06:47:31Z","title":"Comparative Testing of Subgrid Models for Fast Neutrino Flavor Conversions in Core-collapse Supernova Simulations","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-07T05:49:20.750063Z"},"links":{"cited_paper":"/paper/2501.15256","citing_paper":"/paper/2506.07017"},"observation_digest":"sha256:d8b0ce4315adb23a4c2912106bd0436057b3c6269fcae92084045992e9b7c5f5","observation_id":"4fa51310-8248-4b75-ba19-cd7d9bedc588","resolution":{"observed_at":"2026-08-07T05:49:20.750063Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15256","last_updated":"2025-03-04T05:03:37Z","snapshot_observed_at":"2026-07-06T20:26:07.715114Z","submitted_at":"2025-01-25T16:04:00Z","title":"Three-dimensional core-collapse supernova models with phenomenological treatment of neutrino flavor conversions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15256","snapshot_observed_at":"2026-08-06T16:29:11.631155Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.13429","last_updated":"2025-09-03T15:30:02Z","snapshot_observed_at":"2026-08-08T04:08:18.291014Z","submitted_at":"2025-07-17T18:00:00Z","title":"Electron-neutrino lepton number crossings: Variations with the supernova core physics","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T16:29:11.631155Z"},"links":{"cited_paper":"/paper/2501.15256","citing_paper":"/paper/2507.13429"},"observation_digest":"sha256:58159a025ba36384c36b6a39a69d22ae2294cfb5f54800057c7e5f8700ad89a2","observation_id":"66d0eb99-8e7c-422c-84cb-118a90299d08","resolution":{"observed_at":"2026-08-06T16:29:11.631155Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15256","last_updated":"2025-03-04T05:03:37Z","snapshot_observed_at":"2026-07-06T20:26:07.715114Z","submitted_at":"2025-01-25T16:04:00Z","title":"Three-dimensional core-collapse supernova models with phenomenological treatment of neutrino flavor conversions","version":2},"cited_work":{"arxiv_id":"2501.15256","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2501.15256","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"3d8e18df-8503-4e30-8532-092c5f522ca1","year":2025},"citing_paper":{"arxiv_id":"2604.25687","last_updated":"2026-04-28T14:18:05Z","snapshot_observed_at":"2026-07-06T23:11:30.068819Z","submitted_at":"2026-04-28T14:18:05Z","title":"Collective neutrino-antineutrino pair oscillations","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-05-07T15:58:06.378902Z"},"links":{"cited_paper":"/paper/2501.15256","citing_paper":"/paper/2604.25687"},"observation_digest":"sha256:d3db5ca66ce614d6310f21e3bf5614e1cb6878930bc943e274c5bcf8bccc9395","observation_id":"eee23fc2-bf6c-4980-887c-261c0986bc40","resolution":{"observed_at":"2026-05-12T00:01:13.787611Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15256","last_updated":"2025-03-04T05:03:37Z","snapshot_observed_at":"2026-07-06T20:26:07.715114Z","submitted_at":"2025-01-25T16:04:00Z","title":"Three-dimensional core-collapse supernova models with phenomenological treatment of neutrino flavor conversions","version":2},"cited_work":{"arxiv_id":"2501.15256","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2501.15256","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"3d8e18df-8503-4e30-8532-092c5f522ca1","year":2025},"citing_paper":{"arxiv_id":"2605.16504","last_updated":"2026-05-15T18:01:01Z","snapshot_observed_at":"2026-07-06T23:27:38.955917Z","submitted_at":"2026-05-15T18:01:01Z","title":"Neutrino Flavor Conversion Shapes the Rate of Failed Core-collapse Supernovae","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-05-20T15:53:30.768047Z"},"links":{"cited_paper":"/paper/2501.15256","citing_paper":"/paper/2605.16504"},"observation_digest":"sha256:8ff01fe62bb5c0f6d9615e5db7967bf3962ab11893cb662837ca83e155cd59b3","observation_id":"0e551a82-6aaa-446a-b45f-7d811c5af3dd","resolution":{"observed_at":"2026-05-20T15:53:33.508096Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15256","last_updated":"2025-03-04T05:03:37Z","snapshot_observed_at":"2026-07-06T20:26:07.715114Z","submitted_at":"2025-01-25T16:04:00Z","title":"Three-dimensional core-collapse supernova models with phenomenological treatment of neutrino flavor conversions","version":2},"cited_work":{"arxiv_id":"2501.15256","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2501.15256","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"3d8e18df-8503-4e30-8532-092c5f522ca1","year":2025},"citing_paper":{"arxiv_id":"2605.18972","last_updated":"2026-05-18T18:00:49Z","snapshot_observed_at":"2026-08-02T13:27:27.446236Z","submitted_at":"2026-05-18T18:00:49Z","title":"Flavor Conversion Enhances or Suppresses Supernova Explodability Independent of the Progenitor Mass","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-05-20T08:10:13.936279Z"},"links":{"cited_paper":"/paper/2501.15256","citing_paper":"/paper/2605.18972"},"observation_digest":"sha256:72f254476e1cc2918b4a4ba9a8f5c5a48933306c25354b67bc98e7ed00cb32ec","observation_id":"12d5e407-55d0-4398-a468-d5dc1f168f46","resolution":{"observed_at":"2026-05-20T08:13:08.455277Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15256","last_updated":"2025-03-04T05:03:37Z","snapshot_observed_at":"2026-07-06T20:26:07.715114Z","submitted_at":"2025-01-25T16:04:00Z","title":"Three-dimensional core-collapse supernova models with phenomenological treatment of neutrino flavor conversions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15256","snapshot_observed_at":"2026-08-01T23:35:17.381736Z","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":71,"source":"pdf_text","source_observed_at":"2026-08-01T23:35:17.381736Z"},"links":{"cited_paper":"/paper/2501.15256","citing_paper":"/paper/2607.15392"},"observation_digest":"sha256:a33249ded972787c2efcbda9f395ce974b83cbedf350b21cbbfd769fdb5e4d42","observation_id":"f8b3c23c-b066-4204-bd3c-da26a1666b48","resolution":{"observed_at":"2026-08-01T23:35:17.381736Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2501.15256/citation-record","integrity":"/paper/2501.15256/integrity","json":"/paper/2501.15256/citation-record.json","paper":"/paper/2501.15256"},"outbound":[],"paper":{"arxiv_id":"2501.15256","last_updated":"2025-03-04T05:03:37Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T20:26:07.715114Z","submitted_at":"2025-01-25T16:04:00Z","title":"Three-dimensional core-collapse supernova models with phenomenological treatment of neutrino flavor conversions"},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2501.15256."}