{"as_of":"2026-08-19T14:00:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a203507cff304057a750feafcc32b5f836597908f3421e2b3c15fd07312eabe6","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":8,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":8,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T14:54:41.579732Z","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":"2026-07-11T06:47:55.492064Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2406.02672","last_updated":"2024-11-25T22:40:18Z","snapshot_observed_at":"2026-08-16T13:46:09.345438Z","submitted_at":"2024-06-04T18:00:01Z","title":"A comparison of pre-existing $\\Lambda$CDM predictions with the abundance of {\\it JWST} galaxies at high redshift","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.02672","snapshot_observed_at":"2026-08-12T12:42:56.194782Z","title":"S., Bose, S., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.17007","last_updated":"2025-02-04T07:59:13Z","snapshot_observed_at":"2026-08-14T12:10:12.850186Z","submitted_at":"2024-11-26T00:31:45Z","title":"Simulating High-redshift Galaxies: Enhancing UV Luminosity with Star Formation Efficiency and a Top-heavy IMF","version":3},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-12T12:42:56.194782Z"},"links":{"cited_paper":"/paper/2406.02672","citing_paper":"/paper/2411.17007"},"observation_digest":"sha256:8b90bf5bdfe9c24cd1fba9225da4e7df550f89ae60f8bd0dfe63250eee6274ae","observation_id":"5cc0f3c4-a8df-492a-aa57-8a6bb7b4f22b","resolution":{"observed_at":"2026-08-12T12:42:56.194782Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.02672","last_updated":"2024-11-25T22:40:18Z","snapshot_observed_at":"2026-08-16T13:46:09.345438Z","submitted_at":"2024-06-04T18:00:01Z","title":"A comparison of pre-existing $\\Lambda$CDM predictions with the abundance of {\\it JWST} galaxies at high redshift","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.02672","snapshot_observed_at":"2026-08-08T21:53:52.902195Z","title":"S., Bose, S., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04702","last_updated":"2025-02-07T07:14:02Z","snapshot_observed_at":"2026-08-16T07:41:18.900996Z","submitted_at":"2025-02-07T07:14:02Z","title":"Explaining JWST counts with galaxy formation models","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-08T21:53:52.902195Z"},"links":{"cited_paper":"/paper/2406.02672","citing_paper":"/paper/2502.04702"},"observation_digest":"sha256:2dd64e31c5d08a5245ac8f4811513dffdcae41129e4c4245f7147e6b0b4af761","observation_id":"a996cf8a-860e-4a11-8eca-c6ee9c1b93c6","resolution":{"observed_at":"2026-08-08T21:53:52.902195Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.02672","last_updated":"2024-11-25T22:40:18Z","snapshot_observed_at":"2026-08-16T13:46:09.345438Z","submitted_at":"2024-06-04T18:00:01Z","title":"A comparison of pre-existing $\\Lambda$CDM predictions with the abundance of {\\it JWST} galaxies at high redshift","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.02672","snapshot_observed_at":"2026-08-06T12:54:06.459380Z","title":"S., Bose S., Lacey C","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.21409","last_updated":"2025-07-29T00:33:44Z","snapshot_observed_at":"2026-08-16T16:36:07.997157Z","submitted_at":"2025-07-29T00:33:44Z","title":"Explaining the \"too massive\" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-06T12:54:06.459380Z"},"links":{"cited_paper":"/paper/2406.02672","citing_paper":"/paper/2507.21409"},"observation_digest":"sha256:9f723fbb1a8da78b5f515d64d47f19ea37317a7820117e29cae4d11f170a96df","observation_id":"6cd62eb8-6a1c-40fa-9e31-a0b99ae06a6f","resolution":{"observed_at":"2026-08-06T12:54:06.459380Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.02672","last_updated":"2024-11-25T22:40:18Z","snapshot_observed_at":"2026-08-16T13:46:09.345438Z","submitted_at":"2024-06-04T18:00:01Z","title":"A comparison of pre-existing $\\Lambda$CDM predictions with the abundance of {\\it JWST} galaxies at high redshift","version":2},"cited_work":{"arxiv_id":"2406.02672","doi":null,"metadata_source":"pith","pith_arxiv_id":"2406.02672","snapshot_observed_at":"2026-07-11T06:47:55.492064Z","title":"A comparison of pre-existing $\\Lambda$CDM predictions with the abundance of {\\it JWST} galaxies at high redshift","venue":"astro-ph.GA","work_id":"0d76d1b3-45cd-4cf2-acd4-edf423a9ae01","year":2024},"citing_paper":{"arxiv_id":"2607.05505","last_updated":"2026-07-06T18:00:03Z","snapshot_observed_at":"2026-08-12T13:18:05.644944Z","submitted_at":"2026-07-06T18:00:03Z","title":"The dark matter halo mass function in the $\\Lambda\\mathrm{CDM}$ cosmology at all times and over all scales -- from planetary to galaxy cluster masses","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-07-11T06:41:50.562143Z"},"links":{"cited_paper":"/paper/2406.02672","citing_paper":"/paper/2607.05505"},"observation_digest":"sha256:64ae5293e0555f71c9f1461e76b12fc9c320369d20ced308bf526c96e5a9d3ef","observation_id":"1d3e448a-b8db-4d17-b30d-9d4d13e7cbdc","resolution":{"observed_at":"2026-07-11T06:47:55.494958Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.02672","last_updated":"2024-11-25T22:40:18Z","snapshot_observed_at":"2026-08-16T13:46:09.345438Z","submitted_at":"2024-06-04T18:00:01Z","title":"A comparison of pre-existing $\\Lambda$CDM predictions with the abundance of {\\it JWST} galaxies at high redshift","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.02672","snapshot_observed_at":"2026-08-02T00:50:16.068926Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14901","last_updated":"2026-07-16T12:17:52Z","snapshot_observed_at":"2026-08-15T18:41:04.932439Z","submitted_at":"2026-07-16T12:17:52Z","title":"The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations","version":1},"reference_index":300,"source":"arxiv_source","source_observed_at":"2026-08-02T00:50:16.068926Z"},"links":{"cited_paper":"/paper/2406.02672","citing_paper":"/paper/2607.14901"},"observation_digest":"sha256:7503cddb840e0bff13cc5b97049f758ad29d9e818202adff4f18c5259559f506","observation_id":"a4d57437-3319-4ab9-b286-d49b9e1e353c","resolution":{"observed_at":"2026-08-02T00:50:16.068926Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.02672","last_updated":"2024-11-25T22:40:18Z","snapshot_observed_at":"2026-08-16T13:46:09.345438Z","submitted_at":"2024-06-04T18:00:01Z","title":"A comparison of pre-existing $\\Lambda$CDM predictions with the abundance of {\\it JWST} galaxies at high redshift","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.02672","snapshot_observed_at":"2026-08-01T14:10:56.666464Z","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":150,"source":"arxiv_source","source_observed_at":"2026-08-01T14:10:56.666464Z"},"links":{"cited_paper":"/paper/2406.02672","citing_paper":"/paper/2607.18868"},"observation_digest":"sha256:a4a623e92d6a1c11c0b0161d5c28dbc94fa09e5ca859fbc4f781d9556b0dfa8a","observation_id":"58a74ac5-f1d8-47de-a1e1-eb3fef21c220","resolution":{"observed_at":"2026-08-01T14:10:56.666464Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.02672","last_updated":"2024-11-25T22:40:18Z","snapshot_observed_at":"2026-08-16T13:46:09.345438Z","submitted_at":"2024-06-04T18:00:01Z","title":"A comparison of pre-existing $\\Lambda$CDM predictions with the abundance of {\\it JWST} galaxies at high redshift","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.02672","snapshot_observed_at":"2026-08-15T14:54:41.579732Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.03441","last_updated":"2026-08-04T10:36:35Z","snapshot_observed_at":"2026-08-18T09:22:32.553111Z","submitted_at":"2026-08-04T10:36:35Z","title":"SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-15T14:54:41.579732Z"},"links":{"cited_paper":"/paper/2406.02672","citing_paper":"/paper/2608.03441"},"observation_digest":"sha256:29b179efa7fbb516fb00627e4dff077892d3ece35bc42c8f8eef354bf267fe51","observation_id":"3e88b09c-33bb-47f7-96a2-b57ccbafd1ad","resolution":{"observed_at":"2026-08-15T14:54:41.579732Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.02672","last_updated":"2024-11-25T22:40:18Z","snapshot_observed_at":"2026-08-16T13:46:09.345438Z","submitted_at":"2024-06-04T18:00:01Z","title":"A comparison of pre-existing $\\Lambda$CDM predictions with the abundance of {\\it JWST} galaxies at high redshift","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.02672","snapshot_observed_at":"2026-08-11T00:30:25.903483Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07668","last_updated":"2026-08-07T18:00:13Z","snapshot_observed_at":"2026-08-18T10:40:57.814763Z","submitted_at":"2026-08-07T18:00:13Z","title":"First Light and Assembly of GalaxieS (FLAGS) I: The JWST/NIRCam Number Counts and IGL as Constraints on Galaxy Formation Models","version":1},"reference_index":127,"source":"arxiv_source","source_observed_at":"2026-08-11T00:30:25.903483Z"},"links":{"cited_paper":"/paper/2406.02672","citing_paper":"/paper/2608.07668"},"observation_digest":"sha256:5cff782704fc6b75871fe54c0f7befc40ce195ce05ba8be95b68afdef391639e","observation_id":"1aee1e8c-d331-491a-8964-5c511cc91de1","resolution":{"observed_at":"2026-08-11T00:30:25.903483Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2406.02672/citation-record","integrity":"/paper/2406.02672/integrity","json":"/paper/2406.02672/citation-record.json","paper":"/paper/2406.02672"},"outbound":[],"paper":{"arxiv_id":"2406.02672","last_updated":"2024-11-25T22:40:18Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-16T13:46:09.345438Z","submitted_at":"2024-06-04T18:00:01Z","title":"A comparison of pre-existing $\\Lambda$CDM predictions with the abundance of {\\it JWST} galaxies at high redshift"},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2406.02672."}