{"as_of":"2026-08-11T05:33:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:bfca12f0de0211ee445f2c9012433be27f9644c72c0d9ff6c16e693d10f3c962","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":"2026-08-10T06:31:04.303077+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":"2026-08-10T20:15:33.601437Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":1,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2403.07986","last_updated":"2024-09-04T11:50:23Z","snapshot_observed_at":"2026-08-10T22:09:47.368843Z","submitted_at":"2024-03-12T18:00:24Z","title":"EIGER VI. The Correlation Function, Host Halo Mass and Duty Cycle of Luminous Quasars at $z\\gtrsim6$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.07986","snapshot_observed_at":"2026-08-10T20:15:33.601437Z","title":"2024, arXiv e-prints, arXiv:2403.07986, doi: 10.48550/arXiv.2403.07986","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.09077","last_updated":"2025-01-18T17:07:43Z","snapshot_observed_at":"2026-08-10T22:08:40.298825Z","submitted_at":"2025-01-15T19:00:08Z","title":"Assessing the dark matter content of two quasar host galaxies at z~6 through gas kinematics","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-10T20:15:33.601437Z"},"links":{"cited_paper":"/paper/2403.07986","citing_paper":"/paper/2501.09077"},"observation_digest":"sha256:2ea4ddd895e94a3d7e83b4591a676c9392dedc498699b0059a92f77b3cbbddd6","observation_id":"e8c0aa56-764b-48cb-b271-dce4319392f8","resolution":{"observed_at":"2026-08-10T20:15:33.601437Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.07986","last_updated":"2024-09-04T11:50:23Z","snapshot_observed_at":"2026-08-10T22:09:47.368843Z","submitted_at":"2024-03-12T18:00:24Z","title":"EIGER VI. The Correlation Function, Host Halo Mass and Duty Cycle of Luminous Quasars at $z\\gtrsim6$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.07986","snapshot_observed_at":"2026-08-05T06:04:37.088035Z","title":"arXiv:2403.07986","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.04553","last_updated":"2025-09-04T18:00:00Z","snapshot_observed_at":"2026-08-08T10:49:44.672709Z","submitted_at":"2025-09-04T18:00:00Z","title":"Characterizing the roles of transitory obscured phases and inner torus in shaping the fractions of obscured AGN at cosmic noon","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-05T06:04:37.088035Z"},"links":{"cited_paper":"/paper/2403.07986","citing_paper":"/paper/2509.04553"},"observation_digest":"sha256:9f92509b4e8e4c93e14020fee54c27cc9a6037213788888112e1d379e79ef9d0","observation_id":"140356e1-3cbc-4301-9a75-3deb1c522220","resolution":{"observed_at":"2026-08-05T06:04:37.088035Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.07986","last_updated":"2024-09-04T11:50:23Z","snapshot_observed_at":"2026-08-10T22:09:47.368843Z","submitted_at":"2024-03-12T18:00:24Z","title":"EIGER VI. The Correlation Function, Host Halo Mass and Duty Cycle of Luminous Quasars at $z\\gtrsim6$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.07986","snapshot_observed_at":"2026-08-03T04:27:56.500192Z","title":"2024, arXiv e-prints, arXiv:2403.07986, 10.48550/arXiv.2403.07986","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2602.04979","last_updated":"2026-06-30T14:43:31Z","snapshot_observed_at":"2026-08-10T19:13:05.572991Z","submitted_at":"2026-02-04T19:09:27Z","title":"ASPIRE: The Environments and Dark Matter Halos of Luminous Quasars in the Epoch of Reionization","version":2},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-03T04:27:56.500192Z"},"links":{"cited_paper":"/paper/2403.07986","citing_paper":"/paper/2602.04979"},"observation_digest":"sha256:d70402736af4d395a15748197781265bab2dd3fd486d54a5d31fbbfe3d803938","observation_id":"153d68bf-f25b-4ca2-a57f-720f3d7f13cf","resolution":{"observed_at":"2026-08-03T04:27:56.500192Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.07986","last_updated":"2024-09-04T11:50:23Z","snapshot_observed_at":"2026-08-10T22:09:47.368843Z","submitted_at":"2024-03-12T18:00:24Z","title":"EIGER VI. The Correlation Function, Host Halo Mass and Duty Cycle of Luminous Quasars at $z\\gtrsim6$","version":2},"cited_work":{"arxiv_id":"2403.07986","doi":"10.48550/arxiv.2403.07986","metadata_source":"arxiv_reference","pith_arxiv_id":"2403.07986","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"The Correlation Function, Host Halo Mass and Duty Cycle of Luminous Quasars at zrsim6","venue":"arXiv (Cornell University)","work_id":"ca2cfb10-d9aa-4885-928e-219b26358883","year":null},"citing_paper":{"arxiv_id":"2605.11077","last_updated":"2026-05-11T18:00:03Z","snapshot_observed_at":"2026-07-06T23:22:57.012338Z","submitted_at":"2026-05-11T18:00:03Z","title":"The Impact of Cosmic Variance and Satellites on JWST Clustering Measurements at Redshift around 6","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-05-13T00:49:39.736837Z"},"links":{"cited_paper":"/paper/2403.07986","citing_paper":"/paper/2605.11077"},"observation_digest":"sha256:85b1922ce9bdfc2965fc670d86aac54782e39c003537fed1af766cfa1f303edf","observation_id":"3b846d59-88a5-44ae-85f7-d0d143e17d2b","resolution":{"observed_at":"2026-05-13T00:51:58.950632Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2403.07986","last_updated":"2024-09-04T11:50:23Z","snapshot_observed_at":"2026-08-10T22:09:47.368843Z","submitted_at":"2024-03-12T18:00:24Z","title":"EIGER VI. The Correlation Function, Host Halo Mass and Duty Cycle of Luminous Quasars at $z\\gtrsim6$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.07986","snapshot_observed_at":"2026-08-02T12:34:29.988431Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2606.02773","last_updated":"2026-07-21T13:31:25Z","snapshot_observed_at":"2026-08-09T00:17:02.457287Z","submitted_at":"2026-06-01T18:35:41Z","title":"Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-02T12:34:29.988431Z"},"links":{"cited_paper":"/paper/2403.07986","citing_paper":"/paper/2606.02773"},"observation_digest":"sha256:1efe396e309faaec29627b55a09d0ff3c56ea49438e3f86971314d3932b160ce","observation_id":"9209fe3e-9186-4506-bc05-a53b512eed9b","resolution":{"observed_at":"2026-08-02T12:34:29.988431Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2403.07986/citation-record","integrity":"/paper/2403.07986/integrity","json":"/paper/2403.07986/citation-record.json","paper":"/paper/2403.07986"},"outbound":[],"paper":{"arxiv_id":"2403.07986","last_updated":"2024-09-04T11:50:23Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-10T22:09:47.368843Z","submitted_at":"2024-03-12T18:00:24Z","title":"EIGER VI. The Correlation Function, Host Halo Mass and Duty Cycle of Luminous Quasars at $z\\gtrsim6$"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2403.07986."}