{"as_of":"2026-08-17T00:09:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:127f83f6ba96a70fc6d8287a86aa13863dbc8f009ebc8a65040a9d6e274eb13f","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":9,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":9,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T10:37:59.460964Z","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":"2026-07-04T05:29:35.359947Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2108.00581","last_updated":"2022-04-15T01:36:51Z","snapshot_observed_at":"2026-08-16T18:05:58.740382Z","submitted_at":"2021-08-02T01:26:47Z","title":"An 8\\% Determination of the Hubble Constant from localized Fast Radio Bursts","version":2},"cited_work":{"arxiv_id":"2108.00581","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2108.00581","snapshot_observed_at":"2026-07-04T05:29:35.359947Z","title":"Wu, G.-Q","venue":null,"work_id":"44b6e402-4464-4b00-8932-793424c62063","year":2022},"citing_paper":{"arxiv_id":"2402.07716","last_updated":"2026-04-28T16:55:09Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-02-12T15:29:10Z","title":"$\\Lambda_{\\rm s}$CDM cosmology from a type-II minimally modified gravity","version":3},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-24T03:50:50.435997Z"},"links":{"cited_paper":"/paper/2108.00581","citing_paper":"/paper/2402.07716"},"observation_digest":"sha256:81bdabda7f0216da7f75bacd45324121b9757d8b0f707ee0b54fc4c5b915050e","observation_id":"2293cc1f-9a72-404d-bb9a-ec95e0ae969d","resolution":{"observed_at":"2026-05-24T03:53:54.909229Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.00581","last_updated":"2022-04-15T01:36:51Z","snapshot_observed_at":"2026-08-16T18:05:58.740382Z","submitted_at":"2021-08-02T01:26:47Z","title":"An 8\\% Determination of the Hubble Constant from localized Fast Radio Bursts","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.00581","snapshot_observed_at":"2026-08-16T10:37:59.460964Z","title":"Wu, G.-Q","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.17859","last_updated":"2026-05-30T14:20:03Z","snapshot_observed_at":"2026-08-16T19:36:53.850063Z","submitted_at":"2025-04-24T18:04:55Z","title":"Updated Constraints on Omnipotent Dark Energy: A Comprehensive Analysis with CMB and BAO Data","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-16T10:37:59.460964Z"},"links":{"cited_paper":"/paper/2108.00581","citing_paper":"/paper/2504.17859"},"observation_digest":"sha256:827fa56f25707bc715c904d498f8ac1ea9013105a6d8e1cdd312d2955ea93fd6","observation_id":"6c3581b8-81fd-4f6c-85f0-78f230e69aab","resolution":{"observed_at":"2026-08-16T10:37:59.460964Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.00581","last_updated":"2022-04-15T01:36:51Z","snapshot_observed_at":"2026-08-16T18:05:58.740382Z","submitted_at":"2021-08-02T01:26:47Z","title":"An 8\\% Determination of the Hubble Constant from localized Fast Radio Bursts","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.00581","snapshot_observed_at":"2026-08-16T05:24:45.627921Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.21129","last_updated":"2025-04-29T19:24:29Z","snapshot_observed_at":"2026-08-16T23:50:19.764702Z","submitted_at":"2025-04-29T19:24:29Z","title":"Cosmological-model independent limits on photon mass from FRB and SNe data","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-16T05:24:45.627921Z"},"links":{"cited_paper":"/paper/2108.00581","citing_paper":"/paper/2504.21129"},"observation_digest":"sha256:fb76b53c0f6787239c3304be9b97de132e5a9f4e4b62f89588984d5c12559c50","observation_id":"49e2b22c-24b7-4176-81c0-c20b6fb8c837","resolution":{"observed_at":"2026-08-16T05:24:45.627921Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.00581","last_updated":"2022-04-15T01:36:51Z","snapshot_observed_at":"2026-08-16T18:05:58.740382Z","submitted_at":"2021-08-02T01:26:47Z","title":"An 8\\% Determination of the Hubble Constant from localized Fast Radio Bursts","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.00581","snapshot_observed_at":"2026-08-07T11:09:32.344896Z","title":"Wu, G.-Q","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.03536","last_updated":"2026-07-30T03:27:01Z","snapshot_observed_at":"2026-08-12T16:30:43.815468Z","submitted_at":"2025-06-04T03:34:29Z","title":"Constraining the Baryon Fraction in Extragalactic Diffuse Ionized Gas with 124 Localized Fast Radio Bursts","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-07T11:09:32.344896Z"},"links":{"cited_paper":"/paper/2108.00581","citing_paper":"/paper/2506.03536"},"observation_digest":"sha256:c2aaea17b33ea5060a6827556f4b84f1250df0cf7fc85f52c507bdfe6c9fdc62","observation_id":"c6d1e7d3-ca17-4191-9062-d7ab8fac8601","resolution":{"observed_at":"2026-08-07T11:09:32.344896Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.00581","last_updated":"2022-04-15T01:36:51Z","snapshot_observed_at":"2026-08-16T18:05:58.740382Z","submitted_at":"2021-08-02T01:26:47Z","title":"An 8\\% Determination of the Hubble Constant from localized Fast Radio Bursts","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.00581","snapshot_observed_at":"2026-08-15T18:25:01.695684Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.17693","last_updated":"2025-07-23T16:59:32Z","snapshot_observed_at":"2026-08-15T18:16:22.283008Z","submitted_at":"2025-07-23T16:59:32Z","title":"Estimating the baryon fraction in the IGM from well-localized FRBs and DESI data","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-15T18:25:01.695684Z"},"links":{"cited_paper":"/paper/2108.00581","citing_paper":"/paper/2507.17693"},"observation_digest":"sha256:be0e5a978c2c666b2b22c994444b752a45bd35a6411af17316d8d5c3c4b18df1","observation_id":"168d8da5-e2f7-4353-8105-bbbe4f4d405a","resolution":{"observed_at":"2026-08-15T18:25:01.695684Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.00581","last_updated":"2022-04-15T01:36:51Z","snapshot_observed_at":"2026-08-16T18:05:58.740382Z","submitted_at":"2021-08-02T01:26:47Z","title":"An 8\\% Determination of the Hubble Constant from localized Fast Radio Bursts","version":2},"cited_work":{"arxiv_id":"2108.00581","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2108.00581","snapshot_observed_at":"2026-07-04T05:29:35.359947Z","title":"Wu, G.-Q","venue":null,"work_id":"44b6e402-4464-4b00-8932-793424c62063","year":2022},"citing_paper":{"arxiv_id":"2508.19770","last_updated":"2026-04-26T17:29:46Z","snapshot_observed_at":"2026-08-08T18:41:46.199980Z","submitted_at":"2025-08-27T10:53:41Z","title":"Gravitational particle production, the cosmological tensions and fast radio bursts","version":3},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-05-18T20:50:39.710186Z"},"links":{"cited_paper":"/paper/2108.00581","citing_paper":"/paper/2508.19770"},"observation_digest":"sha256:94fd5b97eff4216ff1427907daea31bde513b35c2fa713c8b8b81bc3dfea9cc3","observation_id":"ba721c6c-7ee1-45b1-a45f-aa467d9fb449","resolution":{"observed_at":"2026-05-18T20:51:50.458071Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.00581","last_updated":"2022-04-15T01:36:51Z","snapshot_observed_at":"2026-08-16T18:05:58.740382Z","submitted_at":"2021-08-02T01:26:47Z","title":"An 8\\% Determination of the Hubble Constant from localized Fast Radio Bursts","version":2},"cited_work":{"arxiv_id":"2108.00581","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2108.00581","snapshot_observed_at":"2026-07-04T05:29:35.359947Z","title":"Wu, G.-Q","venue":null,"work_id":"44b6e402-4464-4b00-8932-793424c62063","year":2022},"citing_paper":{"arxiv_id":"2510.09463","last_updated":"2026-05-01T12:31:00Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-10-10T15:15:00Z","title":"Generalized Distributions of Host Dispersion Measures in the Fast Radio Burst Cosmology","version":3},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-05-18T07:54:36.758648Z"},"links":{"cited_paper":"/paper/2108.00581","citing_paper":"/paper/2510.09463"},"observation_digest":"sha256:b9f49263f3ababdc7d13edb5a5c0dacec70815563c65ae12a84ff6c371ad0fb3","observation_id":"63e32eea-0353-41cd-8552-7c5c11a68604","resolution":{"observed_at":"2026-05-18T07:56:04.541286Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.00581","last_updated":"2022-04-15T01:36:51Z","snapshot_observed_at":"2026-08-16T18:05:58.740382Z","submitted_at":"2021-08-02T01:26:47Z","title":"An 8\\% Determination of the Hubble Constant from localized Fast Radio Bursts","version":2},"cited_work":{"arxiv_id":"2108.00581","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2108.00581","snapshot_observed_at":"2026-07-04T05:29:35.359947Z","title":"Wu, G.-Q","venue":null,"work_id":"44b6e402-4464-4b00-8932-793424c62063","year":2022},"citing_paper":{"arxiv_id":"2604.03769","last_updated":"2026-04-04T15:41:30Z","snapshot_observed_at":"2026-08-11T09:14:11.855136Z","submitted_at":"2026-04-04T15:41:30Z","title":"Dispersion Measure Distribution of Unlocalized Fast Radio Bursts as a Probe of the Hubble Constant","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-13T17:12:38.566382Z"},"links":{"cited_paper":"/paper/2108.00581","citing_paper":"/paper/2604.03769"},"observation_digest":"sha256:cb7b1ba6bb04bdfb5f329cd42c3f3fa91f18877e2e3cafad442557e7e1a75673","observation_id":"ec315dba-70c4-4e6c-b3e4-31ac6fba0972","resolution":{"observed_at":"2026-05-13T17:13:01.021058Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.00581","last_updated":"2022-04-15T01:36:51Z","snapshot_observed_at":"2026-08-16T18:05:58.740382Z","submitted_at":"2021-08-02T01:26:47Z","title":"An 8\\% Determination of the Hubble Constant from localized Fast Radio Bursts","version":2},"cited_work":{"arxiv_id":"2108.00581","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2108.00581","snapshot_observed_at":"2026-07-04T05:29:35.359947Z","title":"Wu, G.-Q","venue":null,"work_id":"44b6e402-4464-4b00-8932-793424c62063","year":2022},"citing_paper":{"arxiv_id":"2606.20471","last_updated":"2026-06-18T16:52:06Z","snapshot_observed_at":"2026-07-06T23:55:38.979306Z","submitted_at":"2026-06-18T16:52:06Z","title":"The impact of FRB dispersion measure probability distribution functions on cosmographic estimates","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-06-26T16:01:06.661486Z"},"links":{"cited_paper":"/paper/2108.00581","citing_paper":"/paper/2606.20471"},"observation_digest":"sha256:24044c000c581633bc588bb5cb55a896a7dac14aecb90cceb34512d462807c7a","observation_id":"2bbf2354-0e4f-42b8-a1a9-7b8e55a2eebe","resolution":{"observed_at":"2026-07-04T05:29:35.361216Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2108.00581/citation-record","integrity":"/paper/2108.00581/integrity","json":"/paper/2108.00581/citation-record.json","paper":"/paper/2108.00581"},"outbound":[],"paper":{"arxiv_id":"2108.00581","last_updated":"2022-04-15T01:36:51Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-16T18:05:58.740382Z","submitted_at":"2021-08-02T01:26:47Z","title":"An 8\\% Determination of the Hubble Constant from localized Fast Radio Bursts"},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2108.00581."}