{"as_of":"2026-08-09T20:05:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a5b3cd8c25659044601aeaae67c71a11b89fec981c79a880a672d5d91e10acf4","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":"2026-08-09T06:31:02.800959+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":"2026-08-06T15:06:54.251098Z","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":"2026-07-09T00:45:49.010771Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2007.14720","last_updated":"2021-07-13T10:41:57Z","snapshot_observed_at":"2026-07-06T09:42:43.821599Z","submitted_at":"2020-07-29T10:12:42Z","title":"The Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.14720","snapshot_observed_at":"2026-08-06T15:06:54.251098Z","title":"Ishiyama, F","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.16745","last_updated":"2025-07-22T16:34:49Z","snapshot_observed_at":"2026-08-08T23:33:37.668229Z","submitted_at":"2025-07-22T16:34:49Z","title":"Artifacts in Halo Shapes: Imprints of the Initial Condition","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T15:06:54.251098Z"},"links":{"cited_paper":"/paper/2007.14720","citing_paper":"/paper/2507.16745"},"observation_digest":"sha256:e6ebfd69a5578c76225922cbd23acc0dd4aea00833176d3e43d673eae02be765","observation_id":"461e8cff-42b0-4b1e-8866-eb96f1716fcb","resolution":{"observed_at":"2026-08-06T15:06:54.251098Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.14720","last_updated":"2021-07-13T10:41:57Z","snapshot_observed_at":"2026-07-06T09:42:43.821599Z","submitted_at":"2020-07-29T10:12:42Z","title":"The Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations","version":3},"cited_work":{"arxiv_id":"2007.14720","doi":null,"metadata_source":"pith","pith_arxiv_id":"2007.14720","snapshot_observed_at":"2026-07-09T00:45:49.010771Z","title":"Ishiyama, F","venue":"astro-ph.CO","work_id":"2b79c471-668a-4ec0-b20c-765081fb78bc","year":2020},"citing_paper":{"arxiv_id":"2510.00753","last_updated":"2026-02-10T13:06:38Z","snapshot_observed_at":"2026-07-06T22:31:20.110402Z","submitted_at":"2025-10-01T10:40:48Z","title":"Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-05-18T10:55:19.521613Z"},"links":{"cited_paper":"/paper/2007.14720","citing_paper":"/paper/2510.00753"},"observation_digest":"sha256:6c30543510f1edfe26df36622850e92010b38f508544e2f00ed5b142a1da1a34","observation_id":"70625051-5769-499e-98ab-5d1d78936ef3","resolution":{"observed_at":"2026-05-18T10:56:17.166420Z","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"}},{"citation":{"cited_paper":{"arxiv_id":"2007.14720","last_updated":"2021-07-13T10:41:57Z","snapshot_observed_at":"2026-07-06T09:42:43.821599Z","submitted_at":"2020-07-29T10:12:42Z","title":"The Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations","version":3},"cited_work":{"arxiv_id":"2007.14720","doi":null,"metadata_source":"pith","pith_arxiv_id":"2007.14720","snapshot_observed_at":"2026-07-09T00:45:49.010771Z","title":"Ishiyama, F","venue":"astro-ph.CO","work_id":"2b79c471-668a-4ec0-b20c-765081fb78bc","year":2020},"citing_paper":{"arxiv_id":"2604.26072","last_updated":"2026-04-28T19:21:36Z","snapshot_observed_at":"2026-07-06T23:11:48.524898Z","submitted_at":"2026-04-28T19:21:36Z","title":"Caught in the Cosmic Web: Environmental Impacts on the Halo Substructure Boosts to Dark Matter Annihilation Signals","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-05-07T14:42:49.502885Z"},"links":{"cited_paper":"/paper/2007.14720","citing_paper":"/paper/2604.26072"},"observation_digest":"sha256:aaa1509a3695ea7d8b2f121019b1b4e9a90366207b8978579b1520fff47f4410","observation_id":"04caea70-d116-4573-b9fe-a7018aeda013","resolution":{"observed_at":"2026-05-12T00:41:24.749199Z","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"}},{"citation":{"cited_paper":{"arxiv_id":"2007.14720","last_updated":"2021-07-13T10:41:57Z","snapshot_observed_at":"2026-07-06T09:42:43.821599Z","submitted_at":"2020-07-29T10:12:42Z","title":"The Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations","version":3},"cited_work":{"arxiv_id":"2007.14720","doi":null,"metadata_source":"pith","pith_arxiv_id":"2007.14720","snapshot_observed_at":"2026-07-09T00:45:49.010771Z","title":"Ishiyama, F","venue":"astro-ph.CO","work_id":"2b79c471-668a-4ec0-b20c-765081fb78bc","year":2020},"citing_paper":{"arxiv_id":"2606.28559","last_updated":"2026-06-26T19:22:26Z","snapshot_observed_at":"2026-08-02T20:32:06.095390Z","submitted_at":"2026-06-26T19:22:26Z","title":"DESI DR2 Reference Mocks: Clustering results from UCHUU ELGs and QSOs","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-06-30T00:37:57.208511Z"},"links":{"cited_paper":"/paper/2007.14720","citing_paper":"/paper/2606.28559"},"observation_digest":"sha256:015d1ff6582731f24add0cdee2377229f6cf0e1853b23aaf26b4a04b456c95c7","observation_id":"18cc3afd-633a-4af8-b423-bb081665edb1","resolution":{"observed_at":"2026-07-01T16:25:50.222376Z","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"}},{"citation":{"cited_paper":{"arxiv_id":"2007.14720","last_updated":"2021-07-13T10:41:57Z","snapshot_observed_at":"2026-07-06T09:42:43.821599Z","submitted_at":"2020-07-29T10:12:42Z","title":"The Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations","version":3},"cited_work":{"arxiv_id":"2007.14720","doi":null,"metadata_source":"pith","pith_arxiv_id":"2007.14720","snapshot_observed_at":"2026-07-09T00:45:49.010771Z","title":"Ishiyama, F","venue":"astro-ph.CO","work_id":"2b79c471-668a-4ec0-b20c-765081fb78bc","year":2020},"citing_paper":{"arxiv_id":"2606.30459","last_updated":"2026-06-29T15:25:40Z","snapshot_observed_at":"2026-07-07T00:04:20.023800Z","submitted_at":"2026-06-29T15:25:40Z","title":"Cosmology-dependent covariance in galaxy cluster number counts: consequences for parameter inference","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-06-30T04:52:09.974573Z"},"links":{"cited_paper":"/paper/2007.14720","citing_paper":"/paper/2606.30459"},"observation_digest":"sha256:ac6dfd71f64c8f1671c3091b9e7ce5f1b045bcb6bbc1be5dedbb15c5b4860274","observation_id":"7b096eda-091e-4c79-96ac-14ae67451502","resolution":{"observed_at":"2026-06-30T04:54:16.808576Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"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"}},{"citation":{"cited_paper":{"arxiv_id":"2007.14720","last_updated":"2021-07-13T10:41:57Z","snapshot_observed_at":"2026-07-06T09:42:43.821599Z","submitted_at":"2020-07-29T10:12:42Z","title":"The Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations","version":3},"cited_work":{"arxiv_id":"2007.14720","doi":null,"metadata_source":"pith","pith_arxiv_id":"2007.14720","snapshot_observed_at":"2026-07-09T00:45:49.010771Z","title":"Ishiyama, F","venue":"astro-ph.CO","work_id":"2b79c471-668a-4ec0-b20c-765081fb78bc","year":2020},"citing_paper":{"arxiv_id":"2607.06977","last_updated":"2026-07-08T03:59:33Z","snapshot_observed_at":"2026-08-02T12:50:00.237921Z","submitted_at":"2026-07-08T03:59:33Z","title":"XRISM Reveals a Kinematically Coherent Core System of the Nearby Cool-Core Cluster Abell 2199","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2007.14720","citing_paper":"/paper/2607.06977"},"observation_digest":"sha256:ad0288871facd28622789431b657f221be9c34a3d8e3bd12e549089bebbae069","observation_id":"055d8cba-fefa-4b6d-9569-21e192849e8b","resolution":{"observed_at":"2026-07-09T00:45:49.012078Z","resolver_source":"local_arxiv","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"}},{"citation":{"cited_paper":{"arxiv_id":"2007.14720","last_updated":"2021-07-13T10:41:57Z","snapshot_observed_at":"2026-07-06T09:42:43.821599Z","submitted_at":"2020-07-29T10:12:42Z","title":"The Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.14720","snapshot_observed_at":"2026-08-01T06:39:31.008174Z","title":"Ishiyamaet al., Mon","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.21834","last_updated":"2026-07-23T21:52:06Z","snapshot_observed_at":"2026-08-09T15:55:40.823637Z","submitted_at":"2026-07-23T21:52:06Z","title":"The diffraction-lensing interpretation of GW231123 with astrophysical priors","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-01T06:39:31.008174Z"},"links":{"cited_paper":"/paper/2007.14720","citing_paper":"/paper/2607.21834"},"observation_digest":"sha256:035a604b7cad8f7b05062e70e661a384149bb9886cbfcd79762c1c821a3a52d0","observation_id":"7ac05579-2ba7-466e-99b9-c73201cae21b","resolution":{"observed_at":"2026-08-01T06:39:31.008174Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.14720","last_updated":"2021-07-13T10:41:57Z","snapshot_observed_at":"2026-07-06T09:42:43.821599Z","submitted_at":"2020-07-29T10:12:42Z","title":"The Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.14720","snapshot_observed_at":"2026-07-31T04:54:06.928585Z","title":"Ishiyama et al.,The Uchuu simulations: Data Release 1 and dark matter halo concentrations,Mon","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.28517","last_updated":"2026-07-30T16:55:29Z","snapshot_observed_at":"2026-08-09T14:20:10.461308Z","submitted_at":"2026-07-30T16:55:29Z","title":"Dynamical flattening of halo density cusps by Q-ball dark matter","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-07-31T04:54:06.928585Z"},"links":{"cited_paper":"/paper/2007.14720","citing_paper":"/paper/2607.28517"},"observation_digest":"sha256:210852e17b115568e9be469021e70e376f3f0fec68115d7c00f3b330912e01d2","observation_id":"f1c3b66e-4394-4a05-b177-6b5a7543d8d4","resolution":{"observed_at":"2026-07-31T04:54:06.928585Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2007.14720/citation-record","integrity":"/paper/2007.14720/integrity","json":"/paper/2007.14720/citation-record.json","paper":"/paper/2007.14720"},"outbound":[],"paper":{"arxiv_id":"2007.14720","last_updated":"2021-07-13T10:41:57Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T09:42:43.821599Z","submitted_at":"2020-07-29T10:12:42Z","title":"The Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations"},"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 8 inbound Pith citation observations for arXiv:2007.14720."}