{"as_of":"2026-08-08T21:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a65e5880797fce7075055e52ad683ce7960331583883da6d6d9dbece22446605","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":13,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":13,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":13,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":13,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T20:33:58.039755Z","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":"2026-07-04T05:19:35.884692Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2009.10733","last_updated":"2021-03-03T11:10:28Z","snapshot_observed_at":"2026-07-06T09:57:54.236173Z","submitted_at":"2020-09-22T18:00:02Z","title":"Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies","version":2},"cited_work":{"arxiv_id":"2009.10733","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2009.10733","snapshot_observed_at":"2026-07-04T05:19:35.884692Z","title":"Murgia, G","venue":null,"work_id":"1042f66b-0873-47bf-844d-1ab06c969c83","year":2021},"citing_paper":{"arxiv_id":"2103.01183","last_updated":"2021-06-05T10:18:21Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2021-03-01T18:27:48Z","title":"In the Realm of the Hubble tension $-$ a Review of Solutions","version":3},"reference_index":105,"source":"pdf_text","source_observed_at":"2026-05-15T11:50:20.600831Z"},"links":{"cited_paper":"/paper/2009.10733","citing_paper":"/paper/2103.01183"},"observation_digest":"sha256:f52d2ff45fbcef15b1c549fc0b18da813c8acb0f111039de8a6554dee60bad60","observation_id":"4325eded-457d-43d2-8bac-c0a897b26333","resolution":{"observed_at":"2026-05-15T11:50:21.119823Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10733","last_updated":"2021-03-03T11:10:28Z","snapshot_observed_at":"2026-07-06T09:57:54.236173Z","submitted_at":"2020-09-22T18:00:02Z","title":"Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.10733","snapshot_observed_at":"2026-08-07T20:33:58.039755Z","title":"Murgia, G","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.09810","last_updated":"2025-03-28T12:50:30Z","snapshot_observed_at":"2026-08-07T20:22:54.211210Z","submitted_at":"2025-02-13T23:02:39Z","title":"$\\Lambda$CDM and early dark energy in latent space: a data-driven parametrization of the CMB temperature power spectrum","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-07T20:33:58.039755Z"},"links":{"cited_paper":"/paper/2009.10733","citing_paper":"/paper/2502.09810"},"observation_digest":"sha256:3b7618e9236d15f6e263e80b4fb2dcfa33804d8a27c24451b51d7b668bc67535","observation_id":"612f3b88-acb4-41e9-b4fd-08ca4b2d9d96","resolution":{"observed_at":"2026-08-07T20:33:58.039755Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10733","last_updated":"2021-03-03T11:10:28Z","snapshot_observed_at":"2026-07-06T09:57:54.236173Z","submitted_at":"2020-09-22T18:00:02Z","title":"Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies","version":2},"cited_work":{"arxiv_id":"2009.10733","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2009.10733","snapshot_observed_at":"2026-07-04T05:19:35.884692Z","title":"Murgia, G","venue":null,"work_id":"1042f66b-0873-47bf-844d-1ab06c969c83","year":2021},"citing_paper":{"arxiv_id":"2604.13535","last_updated":"2026-04-15T06:29:12Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-15T06:29:12Z","title":"Double the axions, half the tension: multi-field early dark energy eases the Hubble tension","version":1},"reference_index":159,"source":"pdf_text","source_observed_at":"2026-05-10T12:56:21.466420Z"},"links":{"cited_paper":"/paper/2009.10733","citing_paper":"/paper/2604.13535"},"observation_digest":"sha256:34d929a04d73f52aac1a83049135035c4e045ffc46993412c50a35bf14bff479","observation_id":"06cfe82b-01ac-437c-a3e5-81710359ef03","resolution":{"observed_at":"2026-05-11T11:41:01.672057Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10733","last_updated":"2021-03-03T11:10:28Z","snapshot_observed_at":"2026-07-06T09:57:54.236173Z","submitted_at":"2020-09-22T18:00:02Z","title":"Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies","version":2},"cited_work":{"arxiv_id":"2009.10733","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2009.10733","snapshot_observed_at":"2026-07-04T05:19:35.884692Z","title":"Murgia, G","venue":null,"work_id":"1042f66b-0873-47bf-844d-1ab06c969c83","year":2021},"citing_paper":{"arxiv_id":"2605.14977","last_updated":"2026-08-06T13:45:13Z","snapshot_observed_at":"2026-08-08T20:15:48.967189Z","submitted_at":"2026-05-14T15:41:53Z","title":"Unified dark sector and Hubble-tension alleviation in scalar-vector-tensor gravity","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-06-30T20:07:39.265059Z"},"links":{"cited_paper":"/paper/2009.10733","citing_paper":"/paper/2605.14977"},"observation_digest":"sha256:b23d0f223ba717ce795599d571a1ccd0f071da0bf80e3513d84a114e4033f357","observation_id":"ec5a0ae3-d94f-4097-882d-7f1637fa6a57","resolution":{"observed_at":"2026-06-30T20:15:05.502025Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10733","last_updated":"2021-03-03T11:10:28Z","snapshot_observed_at":"2026-07-06T09:57:54.236173Z","submitted_at":"2020-09-22T18:00:02Z","title":"Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies","version":2},"cited_work":{"arxiv_id":"2009.10733","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2009.10733","snapshot_observed_at":"2026-07-04T05:19:35.884692Z","title":"Murgia, G","venue":null,"work_id":"1042f66b-0873-47bf-844d-1ab06c969c83","year":2021},"citing_paper":{"arxiv_id":"2605.26116","last_updated":"2026-05-25T17:59:53Z","snapshot_observed_at":"2026-07-06T23:36:01.564747Z","submitted_at":"2026-05-25T17:59:53Z","title":"Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-06-29T20:17:08.107860Z"},"links":{"cited_paper":"/paper/2009.10733","citing_paper":"/paper/2605.26116"},"observation_digest":"sha256:d43447eef9308bbaf5d863ad4d0a4f39cc51f0b34d5d5a94a5abb8120d5987d9","observation_id":"54b89638-5d5d-461b-924b-c1b62c637005","resolution":{"observed_at":"2026-07-01T16:45:50.944457Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10733","last_updated":"2021-03-03T11:10:28Z","snapshot_observed_at":"2026-07-06T09:57:54.236173Z","submitted_at":"2020-09-22T18:00:02Z","title":"Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies","version":2},"cited_work":{"arxiv_id":"2009.10733","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2009.10733","snapshot_observed_at":"2026-07-04T05:19:35.884692Z","title":"Murgia, G","venue":null,"work_id":"1042f66b-0873-47bf-844d-1ab06c969c83","year":2021},"citing_paper":{"arxiv_id":"2606.17176","last_updated":"2026-06-15T18:15:02Z","snapshot_observed_at":"2026-07-06T23:52:47.494791Z","submitted_at":"2026-06-15T18:15:02Z","title":"Tracing Ultra Light Axions in Post-reionization, Lyman-$\\alpha$ and CMB Missions","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-06-27T02:35:03.699513Z"},"links":{"cited_paper":"/paper/2009.10733","citing_paper":"/paper/2606.17176"},"observation_digest":"sha256:bf105f9657ccec5c8268a3f66f5ce70b85682952acc2897280810cc5a735d909","observation_id":"a9ca0f16-40bc-4e67-a44d-59657aeb198e","resolution":{"observed_at":"2026-07-03T18:38:49.717425Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10733","last_updated":"2021-03-03T11:10:28Z","snapshot_observed_at":"2026-07-06T09:57:54.236173Z","submitted_at":"2020-09-22T18:00:02Z","title":"Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies","version":2},"cited_work":{"arxiv_id":"2009.10733","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2009.10733","snapshot_observed_at":"2026-07-04T05:19:35.884692Z","title":"Murgia, G","venue":null,"work_id":"1042f66b-0873-47bf-844d-1ab06c969c83","year":2021},"citing_paper":{"arxiv_id":"2606.20434","last_updated":"2026-07-14T16:58:56Z","snapshot_observed_at":"2026-07-17T23:19:04.117001Z","submitted_at":"2026-06-18T16:12:11Z","title":"The Hubble tension: A decade review","version":1},"reference_index":291,"source":"pdf_text","source_observed_at":"2026-06-26T16:04:43.230344Z"},"links":{"cited_paper":"/paper/2009.10733","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:990d1965cefbca47fabf6ca5603181d3443e7fe6617a712e85ab1e4bc14e126f","observation_id":"f68afe39-c87d-405f-b398-6b4b690452ee","resolution":{"observed_at":"2026-07-04T05:19:35.886347Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10733","last_updated":"2021-03-03T11:10:28Z","snapshot_observed_at":"2026-07-06T09:57:54.236173Z","submitted_at":"2020-09-22T18:00:02Z","title":"Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.10733","snapshot_observed_at":"2026-07-15T10:41:50.733215Z","title":"Murgia, G","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2606.20434","last_updated":"2026-07-14T16:58:56Z","snapshot_observed_at":"2026-07-17T23:19:04.117001Z","submitted_at":"2026-06-18T16:12:11Z","title":"The Hubble tension: A decade review","version":2},"reference_index":291,"source":"pdf_text","source_observed_at":"2026-07-15T10:41:50.733215Z"},"links":{"cited_paper":"/paper/2009.10733","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:cb59915c9e00d33c64e9c7cab7657911f120bb27a056a7f22a7e7e21699ac7d4","observation_id":"56b56d42-8eb9-4e3d-9252-4de19d6bb1e2","resolution":{"observed_at":"2026-07-15T10:41:50.733215Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10733","last_updated":"2021-03-03T11:10:28Z","snapshot_observed_at":"2026-07-06T09:57:54.236173Z","submitted_at":"2020-09-22T18:00:02Z","title":"Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies","version":2},"cited_work":{"arxiv_id":"2009.10733","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2009.10733","snapshot_observed_at":"2026-07-04T05:19:35.884692Z","title":"Murgia, G","venue":null,"work_id":"1042f66b-0873-47bf-844d-1ab06c969c83","year":2021},"citing_paper":{"arxiv_id":"2606.31362","last_updated":"2026-06-30T08:57:18Z","snapshot_observed_at":"2026-08-08T20:19:14.509926Z","submitted_at":"2026-06-30T08:57:18Z","title":"Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension","version":1},"reference_index":300,"source":"pdf_text","source_observed_at":"2026-07-01T04:31:47.886338Z"},"links":{"cited_paper":"/paper/2009.10733","citing_paper":"/paper/2606.31362"},"observation_digest":"sha256:2fea9b5db27bc45a42817271def7acc974b9aa59386c47d55ff5b312e1cf6dcf","observation_id":"c673ce19-b01e-499e-9bd2-fa2075523518","resolution":{"observed_at":"2026-07-01T11:25:45.248421Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10733","last_updated":"2021-03-03T11:10:28Z","snapshot_observed_at":"2026-07-06T09:57:54.236173Z","submitted_at":"2020-09-22T18:00:02Z","title":"Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.10733","snapshot_observed_at":"2026-08-02T05:41:37.579815Z","title":"Murgia, G","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.13282","last_updated":"2026-07-14T21:35:59Z","snapshot_observed_at":"2026-08-07T12:43:59.128919Z","submitted_at":"2026-07-14T21:35:59Z","title":"The $H_0$ World Cup. I. Summary of the baseline group stage results","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-02T05:41:37.579815Z"},"links":{"cited_paper":"/paper/2009.10733","citing_paper":"/paper/2607.13282"},"observation_digest":"sha256:1729c0f0eccbb921137d288f89ebb3e0cd3ec8be9fe20fbedfa48381453f6872","observation_id":"41073d42-19e8-4d6e-803e-e241855ee6dc","resolution":{"observed_at":"2026-08-02T05:41:37.579815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10733","last_updated":"2021-03-03T11:10:28Z","snapshot_observed_at":"2026-07-06T09:57:54.236173Z","submitted_at":"2020-09-22T18:00:02Z","title":"Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.10733","snapshot_observed_at":"2026-08-02T05:48:11.176943Z","title":"Murgia, G","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.13283","last_updated":"2026-07-14T21:36:00Z","snapshot_observed_at":"2026-08-07T20:25:34.943645Z","submitted_at":"2026-07-14T21:36:00Z","title":"The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-02T05:48:11.176943Z"},"links":{"cited_paper":"/paper/2009.10733","citing_paper":"/paper/2607.13283"},"observation_digest":"sha256:084f05b14093e8f50d30d7df61db32f8486acf916b6e884fcdef3886e43fd61d","observation_id":"893aa03c-83b2-46b5-82d6-c85ae7625829","resolution":{"observed_at":"2026-08-02T05:48:11.176943Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10733","last_updated":"2021-03-03T11:10:28Z","snapshot_observed_at":"2026-07-06T09:57:54.236173Z","submitted_at":"2020-09-22T18:00:02Z","title":"Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.10733","snapshot_observed_at":"2026-08-01T08:08:39.536179Z","title":"Murgia, G","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.21244","last_updated":"2026-07-23T12:08:39Z","snapshot_observed_at":"2026-08-03T05:59:43.108747Z","submitted_at":"2026-07-23T12:08:39Z","title":"Hubble tension: the shape wall","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-01T08:08:39.536179Z"},"links":{"cited_paper":"/paper/2009.10733","citing_paper":"/paper/2607.21244"},"observation_digest":"sha256:da443b3e5c88c621ff3ec0cfb3af4f386cb600b67d16b99e6c7e84f9662fe386","observation_id":"847455ec-ab14-4568-b07b-b74ceea8c6a7","resolution":{"observed_at":"2026-08-01T08:08:39.536179Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10733","last_updated":"2021-03-03T11:10:28Z","snapshot_observed_at":"2026-07-06T09:57:54.236173Z","submitted_at":"2020-09-22T18:00:02Z","title":"Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.10733","snapshot_observed_at":"2026-08-01T02:46:22.667346Z","title":"Murgia, G","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.26101","last_updated":"2026-07-28T06:59:44Z","snapshot_observed_at":"2026-08-06T07:30:17.682688Z","submitted_at":"2026-07-28T06:59:44Z","title":"Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-01T02:46:22.667346Z"},"links":{"cited_paper":"/paper/2009.10733","citing_paper":"/paper/2607.26101"},"observation_digest":"sha256:5f016cd9261fb0bab92494ac8ce3b1a2b97ef73d32faefe0021250a4c591489c","observation_id":"b907c30f-c660-4505-8cf8-ba9400fb2290","resolution":{"observed_at":"2026-08-01T02:46:22.667346Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2009.10733/citation-record","integrity":"/paper/2009.10733/integrity","json":"/paper/2009.10733/citation-record.json","paper":"/paper/2009.10733"},"outbound":[],"paper":{"arxiv_id":"2009.10733","last_updated":"2021-03-03T11:10:28Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T09:57:54.236173Z","submitted_at":"2020-09-22T18:00:02Z","title":"Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies"},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 13 inbound Pith citation observations for arXiv:2009.10733."}