{"as_of":"2026-08-16T22:01:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7ebae6f149c4a3c053c274e98c2164fee28027984895a7eaf62dba91d44e7081","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T20:35:36.138419Z","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":"2026-07-02T05:06:39.632869Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2212.00163","last_updated":"2023-07-25T12:42:43Z","snapshot_observed_at":"2026-08-16T16:11:55.275233Z","submitted_at":"2022-11-30T23:24:59Z","title":"Using Gray Sirens to Resolve the Hubble-Lema\\^{i}tre Tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.00163","snapshot_observed_at":"2026-08-15T20:35:36.138419Z","title":"Using grey sirens to resolve the Hubble–Lemaˆ ıtre tension,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.12678","last_updated":"2025-07-08T04:39:52Z","snapshot_observed_at":"2026-08-15T20:26:32.596525Z","submitted_at":"2025-05-19T03:53:26Z","title":"Measuring the cosmic dipole with golden dark sirens in the era of next-generation ground-based gravitational wave detectors","version":3},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-15T20:35:36.138419Z"},"links":{"cited_paper":"/paper/2212.00163","citing_paper":"/paper/2505.12678"},"observation_digest":"sha256:4b8ecd40f8d9eb86e6078165d8873259e3b2522c5db0955e2f3cfc0959355cb5","observation_id":"ba397fc3-6394-45d8-b8be-10a329fe14da","resolution":{"observed_at":"2026-08-15T20:35:36.138419Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.00163","last_updated":"2023-07-25T12:42:43Z","snapshot_observed_at":"2026-08-16T16:11:55.275233Z","submitted_at":"2022-11-30T23:24:59Z","title":"Using Gray Sirens to Resolve the Hubble-Lema\\^{i}tre Tension","version":2},"cited_work":{"arxiv_id":"2212.00163","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2212.00163","snapshot_observed_at":"2026-07-02T05:06:39.632869Z","title":"Gupta, Mon","venue":null,"work_id":"fe75e3e4-f5c3-489d-9c7e-a371e678fa36","year":2023},"citing_paper":{"arxiv_id":"2604.11871","last_updated":"2026-04-13T18:00:00Z","snapshot_observed_at":"2026-08-14T13:30:23.001709Z","submitted_at":"2026-04-13T18:00:00Z","title":"Not too close! Evaluating the impact of the baseline on the localization of binary black holes by next-generation gravitational-wave detectors","version":1},"reference_index":117,"source":"pdf_text","source_observed_at":"2026-05-10T15:27:10.838625Z"},"links":{"cited_paper":"/paper/2212.00163","citing_paper":"/paper/2604.11871"},"observation_digest":"sha256:f8096f932a799b80e2904185aa3df337dc9f06de6d7dbd30e01f397dd96aac03","observation_id":"a0ebb15d-44e8-464e-8b7e-e320fffb1bfd","resolution":{"observed_at":"2026-05-11T10:31:02.631973Z","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":"2212.00163","last_updated":"2023-07-25T12:42:43Z","snapshot_observed_at":"2026-08-16T16:11:55.275233Z","submitted_at":"2022-11-30T23:24:59Z","title":"Using Gray Sirens to Resolve the Hubble-Lema\\^{i}tre Tension","version":2},"cited_work":{"arxiv_id":"2212.00163","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2212.00163","snapshot_observed_at":"2026-07-02T05:06:39.632869Z","title":"Gupta, Mon","venue":null,"work_id":"fe75e3e4-f5c3-489d-9c7e-a371e678fa36","year":2023},"citing_paper":{"arxiv_id":"2606.04216","last_updated":"2026-06-02T21:05:20Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-06-02T21:05:20Z","title":"Shape of U: Measuring the Curvature of the Universe with Gravitational Waves","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-06-28T08:35:28.520653Z"},"links":{"cited_paper":"/paper/2212.00163","citing_paper":"/paper/2606.04216"},"observation_digest":"sha256:549b7f42ca82280e25c5cc3c86a9e5bb231971a2911b7b0c0dd83cfbddde6380","observation_id":"38473014-683a-4d0d-bce7-3563cc8f99eb","resolution":{"observed_at":"2026-07-02T05:06:39.634130Z","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/2212.00163/citation-record","integrity":"/paper/2212.00163/integrity","json":"/paper/2212.00163/citation-record.json","paper":"/paper/2212.00163"},"outbound":[],"paper":{"arxiv_id":"2212.00163","last_updated":"2023-07-25T12:42:43Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-16T16:11:55.275233Z","submitted_at":"2022-11-30T23:24:59Z","title":"Using Gray Sirens to Resolve the Hubble-Lema\\^{i}tre Tension"},"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 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2212.00163."}