{"as_of":"2026-08-21T07:43:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d8d776aba3e64a5a0770383725545d734b6f16651f8276ff6100d0f09ca5d2cf","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":1,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":1,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-21T06:32:19.484+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T21:07:26.742024Z","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":"2026-08-15T21:07:27.211695Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2205.03283","last_updated":"2022-05-25T21:31:36Z","snapshot_observed_at":"2026-08-20T22:43:32.693447Z","submitted_at":"2022-05-06T15:11:42Z","title":"Universal relations for quasinormal modes of neutron stars in $R^2$ gravity","version":2},"cited_work":{"arxiv_id":"2205.03283","doi":null,"metadata_source":"pith","pith_arxiv_id":"2205.03283","snapshot_observed_at":"2026-08-15T21:07:27.211695Z","title":"Universal relations for quasinormal modes of neutron stars in $R^2$ gravity","venue":"gr-qc","work_id":"70ac4c25-3f46-4c41-b646-dfc6e1b00ba1","year":2022},"citing_paper":{"arxiv_id":"2505.11073","last_updated":"2025-05-16T10:06:57Z","snapshot_observed_at":"2026-08-16T21:02:01.842510Z","submitted_at":"2025-05-16T10:06:57Z","title":"Can we distinguish whether black holes have singularities or not through echoes and light rings?","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-15T21:07:26.742024Z"},"links":{"cited_paper":"/paper/2205.03283","citing_paper":"/paper/2505.11073"},"observation_digest":"sha256:b5fb228df3b71587b5620218889588a265662bd8ded355de4e08c22813329083","observation_id":"5ffeadf2-de3c-40eb-9b90-fdfe8a22a163","resolution":{"observed_at":"2026-08-15T21:07:27.215653Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2205.03283/citation-record","integrity":"/paper/2205.03283/integrity","json":"/paper/2205.03283/citation-record.json","paper":"/paper/2205.03283"},"outbound":[],"paper":{"arxiv_id":"2205.03283","last_updated":"2022-05-25T21:31:36Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-20T22:43:32.693447Z","submitted_at":"2022-05-06T15:11:42Z","title":"Universal relations for quasinormal modes of neutron stars in $R^2$ gravity"},"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":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2205.03283."}