{"as_of":"2026-08-09T23:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d855b6d0b83809f75ae90389e9bb3f0e89923062f1d541a0964fb962f5b63898","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-09T14:45:24.510549Z","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":"2026-07-02T00:46:23.888902Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2212.11638","last_updated":"2024-02-14T12:40:53Z","snapshot_observed_at":"2026-07-06T14:33:55.811891Z","submitted_at":"2022-12-22T12:08:33Z","title":"A population of faint, old, and massive quiescent galaxies at 3 < z < 4 revealed by JWST NIRSpec Spectroscopy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.11638","snapshot_observed_at":"2026-08-09T14:45:24.510549Z","title":"2212.11638","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.01724","last_updated":"2025-02-03T19:00:00Z","snapshot_observed_at":"2026-08-09T14:38:59.360524Z","submitted_at":"2025-02-03T19:00:00Z","title":"Cosmic quenching","version":1},"reference_index":3724,"source":"pdf_text","source_observed_at":"2026-08-09T14:45:24.510549Z"},"links":{"cited_paper":"/paper/2212.11638","citing_paper":"/paper/2502.01724"},"observation_digest":"sha256:47aba88cdacb01a5eb2041a59e5e20add74b8167ea4922a69b90a78ed4bc2a61","observation_id":"cb3a8164-d10d-4a85-be45-5acfbb471f56","resolution":{"observed_at":"2026-08-09T14:45:24.510549Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.11638","last_updated":"2024-02-14T12:40:53Z","snapshot_observed_at":"2026-07-06T14:33:55.811891Z","submitted_at":"2022-12-22T12:08:33Z","title":"A population of faint, old, and massive quiescent galaxies at 3 < z < 4 revealed by JWST NIRSpec Spectroscopy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.11638","snapshot_observed_at":"2026-08-08T20:32:19.119723Z","title":"Scientific Reports 14, 3724 (2024) https://doi","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.05048","last_updated":"2025-02-07T16:10:58Z","snapshot_observed_at":"2026-08-09T03:09:57.254511Z","submitted_at":"2025-02-07T16:10:58Z","title":"A prevalent population of normal-mass central black holes in high-redshift massive galaxies","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-08T20:32:19.119723Z"},"links":{"cited_paper":"/paper/2212.11638","citing_paper":"/paper/2502.05048"},"observation_digest":"sha256:ef3005ac8503a20d8c67507c0ce82f86a11c3354851c99e6685657fdaba96ead","observation_id":"426c1d67-3c39-45bc-a8eb-321e78be5de2","resolution":{"observed_at":"2026-08-08T20:32:19.119723Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.11638","last_updated":"2024-02-14T12:40:53Z","snapshot_observed_at":"2026-07-06T14:33:55.811891Z","submitted_at":"2022-12-22T12:08:33Z","title":"A population of faint, old, and massive quiescent galaxies at 3 < z < 4 revealed by JWST NIRSpec Spectroscopy","version":3},"cited_work":{"arxiv_id":"2212.11638","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2212.11638","snapshot_observed_at":"2026-07-02T00:46:23.888902Z","title":"Scientific Reports , volume =","venue":null,"work_id":"fa18c4b8-b914-4e1e-a141-f73dde8511ae","year":2024},"citing_paper":{"arxiv_id":"2606.02097","last_updated":"2026-06-01T11:28:21Z","snapshot_observed_at":"2026-08-06T05:31:00.560567Z","submitted_at":"2026-06-01T11:28:21Z","title":"Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-06-28T13:17:56.799399Z"},"links":{"cited_paper":"/paper/2212.11638","citing_paper":"/paper/2606.02097"},"observation_digest":"sha256:0b5b9fa39d80b31e470c09ee4a0c4973396451fc14af6f22a44987a3f11f8ef3","observation_id":"e0975886-4de6-4cbf-946a-9a45857d278c","resolution":{"observed_at":"2026-07-02T00:46:23.891071Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2212.11638/citation-record","integrity":"/paper/2212.11638/integrity","json":"/paper/2212.11638/citation-record.json","paper":"/paper/2212.11638"},"outbound":[],"paper":{"arxiv_id":"2212.11638","last_updated":"2024-02-14T12:40:53Z","latest_version":3,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T14:33:55.811891Z","submitted_at":"2022-12-22T12:08:33Z","title":"A population of faint, old, and massive quiescent galaxies at 3 < z < 4 revealed by JWST NIRSpec Spectroscopy"},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2212.11638."}