{"as_of":"2026-08-10T02:55:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b3253effba5355686fe0db4f93098bc7eb7f2e1bd092b19c89b18c41c05a33ae","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":"2026-08-09T06:31:02.800959+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":"2026-08-06T14:43:34.963765Z","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":"2026-07-04T02:29:22.971499Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2012.15200","last_updated":"2021-05-27T13:08:11Z","snapshot_observed_at":"2026-08-07T17:10:13.446479Z","submitted_at":"2020-12-30T15:40:40Z","title":"Minimal models for $g-2$ and dark matter confront asymptotic safety","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.15200","snapshot_observed_at":"2026-08-06T14:43:34.963765Z","title":"Kowalska and E","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.17862","last_updated":"2025-07-23T18:34:53Z","snapshot_observed_at":"2026-08-08T10:10:52.915452Z","submitted_at":"2025-07-23T18:34:53Z","title":"Matter Spectral Functions from Quantum Gravity","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-06T14:43:34.963765Z"},"links":{"cited_paper":"/paper/2012.15200","citing_paper":"/paper/2507.17862"},"observation_digest":"sha256:70631fdee9467d824b03e57f85ae5fd8292be9258847498d4c021de6d53face1","observation_id":"aa70c135-ffb6-4e74-bad8-1cc0a48a5bca","resolution":{"observed_at":"2026-08-06T14:43:34.963765Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.15200","last_updated":"2021-05-27T13:08:11Z","snapshot_observed_at":"2026-08-07T17:10:13.446479Z","submitted_at":"2020-12-30T15:40:40Z","title":"Minimal models for $g-2$ and dark matter confront asymptotic safety","version":2},"cited_work":{"arxiv_id":"2012.15200","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2012.15200","snapshot_observed_at":"2026-07-04T02:29:22.971499Z","title":"Kowalska and E.M","venue":null,"work_id":"02761bb4-feaf-4f26-89ac-4bbe6bb71f18","year":2021},"citing_paper":{"arxiv_id":"2510.23808","last_updated":"2026-04-30T10:07:37Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-10-27T19:45:23Z","title":"Towards theory constraints on ultralight dark matter from quantum gravity","version":3},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-05-18T03:54:40.890399Z"},"links":{"cited_paper":"/paper/2012.15200","citing_paper":"/paper/2510.23808"},"observation_digest":"sha256:80030f8437a41ecd4992d37e6e892d9044ca4050443f15403109898100a2157d","observation_id":"c4fb7654-7928-4704-948a-11e410953397","resolution":{"observed_at":"2026-05-18T03:55:50.648391Z","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":"2012.15200","last_updated":"2021-05-27T13:08:11Z","snapshot_observed_at":"2026-08-07T17:10:13.446479Z","submitted_at":"2020-12-30T15:40:40Z","title":"Minimal models for $g-2$ and dark matter confront asymptotic safety","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.15200","snapshot_observed_at":"2026-08-03T16:21:43.975231Z","title":"Kowalska and E","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2512.14009","last_updated":"2026-05-26T07:28:50Z","snapshot_observed_at":"2026-08-08T07:53:47.664730Z","submitted_at":"2025-12-16T02:06:07Z","title":"Scaling solutions for gauge invariant flow equations in dilaton quantum gravity","version":2},"reference_index":143,"source":"pdf_text","source_observed_at":"2026-08-03T16:21:43.975231Z"},"links":{"cited_paper":"/paper/2012.15200","citing_paper":"/paper/2512.14009"},"observation_digest":"sha256:4440294a776f44b9da9226fcf0c014d8d8721b6bf89b8ad46a5215ab7b927d71","observation_id":"952ae62e-d941-4e9b-b5fd-dafd6c5750c3","resolution":{"observed_at":"2026-08-03T16:21:43.975231Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.15200","last_updated":"2021-05-27T13:08:11Z","snapshot_observed_at":"2026-08-07T17:10:13.446479Z","submitted_at":"2020-12-30T15:40:40Z","title":"Minimal models for $g-2$ and dark matter confront asymptotic safety","version":2},"cited_work":{"arxiv_id":"2012.15200","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2012.15200","snapshot_observed_at":"2026-07-04T02:29:22.971499Z","title":"Kowalska and E.M","venue":null,"work_id":"02761bb4-feaf-4f26-89ac-4bbe6bb71f18","year":2021},"citing_paper":{"arxiv_id":"2604.03033","last_updated":"2026-06-26T14:51:30Z","snapshot_observed_at":"2026-07-13T13:37:12.242264Z","submitted_at":"2026-04-03T13:38:11Z","title":"Quantum gravity contributions to the gauge and Yukawa couplings in proper time flow","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-05-13T18:05:47.533100Z"},"links":{"cited_paper":"/paper/2012.15200","citing_paper":"/paper/2604.03033"},"observation_digest":"sha256:f54c764582013454f54095f18de6a19ca8a4ecefe58a9e921d575540a2bc94d3","observation_id":"fb9aa562-455b-4883-bfa6-4011dc0ece07","resolution":{"observed_at":"2026-05-13T18:08:15.674562Z","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":"2012.15200","last_updated":"2021-05-27T13:08:11Z","snapshot_observed_at":"2026-08-07T17:10:13.446479Z","submitted_at":"2020-12-30T15:40:40Z","title":"Minimal models for $g-2$ and dark matter confront asymptotic safety","version":2},"cited_work":{"arxiv_id":"2012.15200","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2012.15200","snapshot_observed_at":"2026-07-04T02:29:22.971499Z","title":"Kowalska and E.M","venue":null,"work_id":"02761bb4-feaf-4f26-89ac-4bbe6bb71f18","year":2021},"citing_paper":{"arxiv_id":"2606.19321","last_updated":"2026-06-17T17:47:50Z","snapshot_observed_at":"2026-08-07T00:37:05.110998Z","submitted_at":"2026-06-17T17:47:50Z","title":"Spectral Functions of Lorentzian Quantum Gravity","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-06-26T19:43:53.736595Z"},"links":{"cited_paper":"/paper/2012.15200","citing_paper":"/paper/2606.19321"},"observation_digest":"sha256:b080eafa18d9c60458a22b9d029e32640e3c07097f02df480579f278d328a875","observation_id":"d03044d9-1475-4cb4-ad69-c167a51c3ef5","resolution":{"observed_at":"2026-07-04T02:29:22.972794Z","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"}}],"links":{"evidence":"/evidence","html":"/paper/2012.15200/citation-record","integrity":"/paper/2012.15200/integrity","json":"/paper/2012.15200/citation-record.json","paper":"/paper/2012.15200"},"outbound":[],"paper":{"arxiv_id":"2012.15200","last_updated":"2021-05-27T13:08:11Z","latest_version":2,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-07T17:10:13.446479Z","submitted_at":"2020-12-30T15:40:40Z","title":"Minimal models for $g-2$ and dark matter confront asymptotic safety"},"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 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2012.15200."}