{"as_of":"2026-08-18T23:42:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2cd3a5f47951b092153fda21335187b7d8a982f56bde660eacd7bbe901f58e7b","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":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-18T06:34:40.430872+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T00:12:18.420238Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-10T02:16:42.221889Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2305.02078","last_updated":"2024-03-11T13:44:49Z","snapshot_observed_at":"2026-08-16T16:44:55.888598Z","submitted_at":"2023-05-03T12:32:18Z","title":"EMPRESS. XIII. Chemical Enrichments of Young Galaxies Near and Far at z ~ 0 and 4-10: Fe/O, Ar/O, S/O, and N/O Measurements with Chemical Evolution Model Comparisons","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.02078","snapshot_observed_at":"2026-08-11T21:08:52.289829Z","title":"EMPRESS. XIII. Chemical Enrichment of Young Galaxies Near and Far at z ∼ 0 and 4–10: Fe/O, Ar/O, S/O, and N/O Measurements with a Comparison of Chemical Evolution Models","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.04983","last_updated":"2024-12-06T12:07:44Z","snapshot_observed_at":"2026-08-17T16:57:03.528586Z","submitted_at":"2024-12-06T12:07:44Z","title":"Red, hot, and very metal poor: extreme properties of a massive accreting black hole in the first 500 Myr","version":1},"reference_index":126,"source":"pdf_text","source_observed_at":"2026-08-11T21:08:52.289829Z"},"links":{"cited_paper":"/paper/2305.02078","citing_paper":"/paper/2412.04983"},"observation_digest":"sha256:311c45c025c1a88ca5f65f2a90651fd7afcf39e90ca9f027dd26eea66419725b","observation_id":"e01a2528-215f-49e4-89b5-57e5e29a09df","resolution":{"observed_at":"2026-08-11T21:08:52.289829Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.02078","last_updated":"2024-03-11T13:44:49Z","snapshot_observed_at":"2026-08-16T16:44:55.888598Z","submitted_at":"2023-05-03T12:32:18Z","title":"EMPRESS. XIII. Chemical Enrichments of Young Galaxies Near and Far at z ~ 0 and 4-10: Fe/O, Ar/O, S/O, and N/O Measurements with Chemical Evolution Model Comparisons","version":4},"cited_work":{"arxiv_id":"2305.02078","doi":null,"metadata_source":"pith","pith_arxiv_id":"2305.02078","snapshot_observed_at":"2026-07-10T02:16:42.221889Z","title":"EMPRESS. XIII. Chemical Enrichments of Young Galaxies Near and Far at z ~ 0 and 4-10: Fe/O, Ar/O, S/O, and N/O Measurements with Chemical Evolution Model Comparisons","venue":"astro-ph.GA","work_id":"d33d0f84-a396-4f44-9f0a-501759ed2de1","year":2023},"citing_paper":{"arxiv_id":"2607.08749","last_updated":"2026-07-09T17:49:55Z","snapshot_observed_at":"2026-08-08T08:47:40.626689Z","submitted_at":"2026-07-09T17:49:55Z","title":"Deep Spectroscopic Follow-Up of Maisie's Galaxy -- A Typical Galaxy in the Early Universe","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2305.02078","citing_paper":"/paper/2607.08749"},"observation_digest":"sha256:a334909411bfcc0568daf6595fe66e307f9554e94b5ef2f59f40fd3e8d1ed66a","observation_id":"028d978e-8acb-4686-9b71-36b1e1b83b0f","resolution":{"observed_at":"2026-07-10T02:16:42.223226Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.02078","last_updated":"2024-03-11T13:44:49Z","snapshot_observed_at":"2026-08-16T16:44:55.888598Z","submitted_at":"2023-05-03T12:32:18Z","title":"EMPRESS. XIII. Chemical Enrichments of Young Galaxies Near and Far at z ~ 0 and 4-10: Fe/O, Ar/O, S/O, and N/O Measurements with Chemical Evolution Model Comparisons","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.02078","snapshot_observed_at":"2026-08-02T01:14:15.566364Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14758","last_updated":"2026-07-16T09:43:20Z","snapshot_observed_at":"2026-08-17T05:03:07.756786Z","submitted_at":"2026-07-16T09:43:20Z","title":"The Mysterious Case of Iron in XMPs: Anomalous High log(Fe/O) Observed in Extremely Metal-Poor Galaxies HSCJ1631+4426 and SDSSJ0811+4730","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-02T01:14:15.566364Z"},"links":{"cited_paper":"/paper/2305.02078","citing_paper":"/paper/2607.14758"},"observation_digest":"sha256:26f0f767bfd6f830552298423e0e18f533be9a50e439f6afe4140b2fa9424cde","observation_id":"b0d984ef-6056-4811-bc1f-bd331ead236a","resolution":{"observed_at":"2026-08-02T01:14:15.566364Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.02078","last_updated":"2024-03-11T13:44:49Z","snapshot_observed_at":"2026-08-16T16:44:55.888598Z","submitted_at":"2023-05-03T12:32:18Z","title":"EMPRESS. XIII. Chemical Enrichments of Young Galaxies Near and Far at z ~ 0 and 4-10: Fe/O, Ar/O, S/O, and N/O Measurements with Chemical Evolution Model Comparisons","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.02078","snapshot_observed_at":"2026-08-01T14:10:50.594286Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.18868","last_updated":"2026-07-21T08:59:21Z","snapshot_observed_at":"2026-08-15T22:55:44.404302Z","submitted_at":"2026-07-21T08:59:21Z","title":"Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-01T14:10:50.594286Z"},"links":{"cited_paper":"/paper/2305.02078","citing_paper":"/paper/2607.18868"},"observation_digest":"sha256:3ffb4ad4ba5d7b71ceb2b135917bcfefd46f8b5e808038e7a820271491243fd0","observation_id":"f024661f-a69c-4d08-8fdf-0a582c0535dd","resolution":{"observed_at":"2026-08-01T14:10:50.594286Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.02078","last_updated":"2024-03-11T13:44:49Z","snapshot_observed_at":"2026-08-16T16:44:55.888598Z","submitted_at":"2023-05-03T12:32:18Z","title":"EMPRESS. XIII. Chemical Enrichments of Young Galaxies Near and Far at z ~ 0 and 4-10: Fe/O, Ar/O, S/O, and N/O Measurements with Chemical Evolution Model Comparisons","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.02078","snapshot_observed_at":"2026-08-14T04:17:46.838763Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10063","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-16T05:16:54.846569Z","submitted_at":"2026-08-10T18:00:00Z","title":"Unveiling and Characterising Ubiquitous Nitrogen Enhancement in $6 \\leq z \\leq 10$ Galaxies with JWST Spectroscopy","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-14T04:17:46.838763Z"},"links":{"cited_paper":"/paper/2305.02078","citing_paper":"/paper/2608.10063"},"observation_digest":"sha256:7c035948b4390b45aae73781a365fb43ab3de6ffff21c5cc62260d8e8bcf68d1","observation_id":"ccc4fa17-9148-4507-9452-333ea3b70c6d","resolution":{"observed_at":"2026-08-14T04:17:46.838763Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.02078","last_updated":"2024-03-11T13:44:49Z","snapshot_observed_at":"2026-08-16T16:44:55.888598Z","submitted_at":"2023-05-03T12:32:18Z","title":"EMPRESS. XIII. Chemical Enrichments of Young Galaxies Near and Far at z ~ 0 and 4-10: Fe/O, Ar/O, S/O, and N/O Measurements with Chemical Evolution Model Comparisons","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.02078","snapshot_observed_at":"2026-08-16T00:12:18.420238Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12466","last_updated":"2026-08-16T17:08:46Z","snapshot_observed_at":"2026-08-18T23:17:44.794459Z","submitted_at":"2026-08-12T18:00:02Z","title":"Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics","version":1},"reference_index":188,"source":"arxiv_source","source_observed_at":"2026-08-16T00:12:18.420238Z"},"links":{"cited_paper":"/paper/2305.02078","citing_paper":"/paper/2608.12466"},"observation_digest":"sha256:7583ec164dd05a4d75180810fbb336303a496f0e295901fae0f5fd08ba0e3a94","observation_id":"66ef5d93-0900-418a-848b-a5d8792da319","resolution":{"observed_at":"2026-08-16T00:12:18.420238Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2305.02078/citation-record","integrity":"/paper/2305.02078/integrity","json":"/paper/2305.02078/citation-record.json","paper":"/paper/2305.02078"},"outbound":[],"paper":{"arxiv_id":"2305.02078","last_updated":"2024-03-11T13:44:49Z","latest_version":4,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-16T16:44:55.888598Z","submitted_at":"2023-05-03T12:32:18Z","title":"EMPRESS. XIII. Chemical Enrichments of Young Galaxies Near and Far at z ~ 0 and 4-10: Fe/O, Ar/O, S/O, and N/O Measurements with Chemical Evolution Model Comparisons"},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2305.02078."}