{"as_of":"2026-08-22T09:52:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:1ae17fe2bd580cf3498eb0a90f87a53e7dd4eff6a99254013fb98e33319e0d47","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-22T06:32:14.747728+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T23:27:53.912260Z","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":"2026-08-04T12:16:13.904932Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2410.20530","last_updated":"2025-07-07T13:21:52Z","snapshot_observed_at":"2026-08-16T13:05:36.663753Z","submitted_at":"2024-10-27T17:47:33Z","title":"On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.20530","snapshot_observed_at":"2026-08-07T23:27:53.912260Z","title":"L., Teyssier , R., & Dekel , A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.08885","last_updated":"2025-08-22T05:59:58Z","snapshot_observed_at":"2026-08-18T23:08:45.320182Z","submitted_at":"2025-02-13T01:55:24Z","title":"Morphological Demographics of Galaxies at $z\\sim 10-16$: Log-Normal Size Distribution and Exponential Profiles Consistent with the Disk Formation Scenario","version":2},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-07T23:27:53.912260Z"},"links":{"cited_paper":"/paper/2410.20530","citing_paper":"/paper/2502.08885"},"observation_digest":"sha256:e6c74e9ee6f0fcdc86f73d17bf4f61cb85101cbcf23a06d56c0e5e8eabb96fc0","observation_id":"10cb97f1-0e43-432a-bde0-ca02be97ef54","resolution":{"observed_at":"2026-08-07T23:27:53.912260Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.20530","last_updated":"2025-07-07T13:21:52Z","snapshot_observed_at":"2026-08-16T13:05:36.663753Z","submitted_at":"2024-10-27T17:47:33Z","title":"On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.20530","snapshot_observed_at":"2026-08-07T14:14:20.196619Z","title":"L., Teyssier R., Dekel A., 2024, arXiv, arXiv:2410.20530","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.19832","last_updated":"2025-05-26T11:11:12Z","snapshot_observed_at":"2026-08-17T20:32:27.840015Z","submitted_at":"2025-05-26T11:11:12Z","title":"Reconciling extragalactic star formation efficiencies with theory: insights from PHANGS","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-07T14:14:20.196619Z"},"links":{"cited_paper":"/paper/2410.20530","citing_paper":"/paper/2505.19832"},"observation_digest":"sha256:ed06e0d30cfa392eb45c87e522aff7756613c887c8db30fc4ad48326899f2bde","observation_id":"10dac9d4-7a5d-4eeb-add0-35f058738330","resolution":{"observed_at":"2026-08-07T14:14:20.196619Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.20530","last_updated":"2025-07-07T13:21:52Z","snapshot_observed_at":"2026-08-16T13:05:36.663753Z","submitted_at":"2024-10-27T17:47:33Z","title":"On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn","version":3},"cited_work":{"arxiv_id":"2410.20530","doi":"10.48550/arxiv.2410.20530","metadata_source":"pith","pith_arxiv_id":"2410.20530","snapshot_observed_at":"2026-08-04T12:16:13.904932Z","title":"On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn","venue":"astro-ph.GA","work_id":"70bd7d17-a82f-4213-a5a6-1f427641dfb9","year":2024},"citing_paper":{"arxiv_id":"2510.19822","last_updated":"2026-06-11T15:03:57Z","snapshot_observed_at":"2026-08-18T18:05:43.029929Z","submitted_at":"2025-10-22T17:59:30Z","title":"Supermassive Black Hole Growth in Massive Galaxies at Cosmic Dawn","version":2},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-04T08:39:34.425496Z"},"links":{"cited_paper":"/paper/2410.20530","citing_paper":"/paper/2510.19822"},"observation_digest":"sha256:4960b4e46cefc4ebaa86c7f8091745f7a0ef7cb0c2a3d51c0569a66ab01ae9be","observation_id":"1c65570f-4405-433e-9d1a-4671f747a6bc","resolution":{"observed_at":"2026-08-04T08:44:11.012112Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.20530","last_updated":"2025-07-07T13:21:52Z","snapshot_observed_at":"2026-08-16T13:05:36.663753Z","submitted_at":"2024-10-27T17:47:33Z","title":"On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.20530","snapshot_observed_at":"2026-08-04T00:10:17.361423Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.02906","last_updated":"2026-07-13T21:59:28Z","snapshot_observed_at":"2026-08-16T10:51:02.401539Z","submitted_at":"2025-11-04T19:00:01Z","title":"Dark Secrets of Baryons: Illuminating Dark Matter-Baryon Interactions with JWST","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-04T00:10:17.361423Z"},"links":{"cited_paper":"/paper/2410.20530","citing_paper":"/paper/2511.02906"},"observation_digest":"sha256:09afefbd401ddecaeb19a5af4ab0517025b5335d5a835a3e9026c8c2f360cbfb","observation_id":"8821bad7-5db6-4313-9980-4ab15ba54172","resolution":{"observed_at":"2026-08-04T00:10:17.361423Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.20530","last_updated":"2025-07-07T13:21:52Z","snapshot_observed_at":"2026-08-16T13:05:36.663753Z","submitted_at":"2024-10-27T17:47:33Z","title":"On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.20530","snapshot_observed_at":"2026-08-01T14:10:56.250345Z","title":", keywords =","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":96,"source":"arxiv_source","source_observed_at":"2026-08-01T14:10:56.250345Z"},"links":{"cited_paper":"/paper/2410.20530","citing_paper":"/paper/2607.18868"},"observation_digest":"sha256:7002e233a443b8de2a8c3c1ed108a27211abb8f84b2862307ba9c3890bed75ab","observation_id":"a4abef17-3449-4624-94fe-b0de23c956b1","resolution":{"observed_at":"2026-08-01T14:10:56.250345Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2410.20530/citation-record","integrity":"/paper/2410.20530/integrity","json":"/paper/2410.20530/citation-record.json","paper":"/paper/2410.20530"},"outbound":[],"paper":{"arxiv_id":"2410.20530","last_updated":"2025-07-07T13:21:52Z","latest_version":3,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-16T13:05:36.663753Z","submitted_at":"2024-10-27T17:47:33Z","title":"On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn"},"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":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"thesis":"As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2410.20530."}