{"as_of":"2026-08-11T12:02:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:03c3470dd82fd1857ff0bc9a2fbe325f66690a6975cf7e38d0cd24c08b93c90b","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-02T01:02:10.597583Z","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":"2026-07-02T11:16:53.277015Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2307.15194","last_updated":"2023-07-27T20:59:02Z","snapshot_observed_at":"2026-07-06T15:59:30.956483Z","submitted_at":"2023-07-27T20:59:02Z","title":"Inhomogeneous Cosmology using General Relativistic Smoothed Particle Hydrodynamics coupled to Numerical Relativity","version":1},"cited_work":{"arxiv_id":"2307.15194","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2307.15194","snapshot_observed_at":"2026-07-02T11:16:53.277015Z","title":null,"venue":null,"work_id":"b61796ca-a2ac-46d0-a786-218acb224ee9","year":2023},"citing_paper":{"arxiv_id":"2606.05479","last_updated":"2026-06-03T21:57:07Z","snapshot_observed_at":"2026-08-03T03:09:40.685832Z","submitted_at":"2026-06-03T21:57:07Z","title":"On the potential for inhomogeneities to mimic an evolving dark energy","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-06-28T04:24:31.631297Z"},"links":{"cited_paper":"/paper/2307.15194","citing_paper":"/paper/2606.05479"},"observation_digest":"sha256:e1ba623e8cc149863e295673d8322d5daacfbf927e4197d79d2747e715a3a955","observation_id":"091884a5-b83a-4a2a-a357-1f3546da951f","resolution":{"observed_at":"2026-07-02T11:16:53.279279Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.15194","last_updated":"2023-07-27T20:59:02Z","snapshot_observed_at":"2026-07-06T15:59:30.956483Z","submitted_at":"2023-07-27T20:59:02Z","title":"Inhomogeneous Cosmology using General Relativistic Smoothed Particle Hydrodynamics coupled to Numerical Relativity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.15194","snapshot_observed_at":"2026-08-02T01:02:10.597583Z","title":"arXiv , journal =:2307.15194 , number =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14828","last_updated":"2026-07-16T10:46:59Z","snapshot_observed_at":"2026-08-08T04:14:25.891566Z","submitted_at":"2026-07-16T10:46:59Z","title":"SPH methods in the modelling of compact objects","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-02T01:02:10.597583Z"},"links":{"cited_paper":"/paper/2307.15194","citing_paper":"/paper/2607.14828"},"observation_digest":"sha256:83ea2191621184f255f21b2604be5b82394b58f7feef7057d2740633407f6e95","observation_id":"4f404d50-a03a-44fa-9b3d-e708cd9d2963","resolution":{"observed_at":"2026-08-02T01:02:10.597583Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2307.15194/citation-record","integrity":"/paper/2307.15194/integrity","json":"/paper/2307.15194/citation-record.json","paper":"/paper/2307.15194"},"outbound":[],"paper":{"arxiv_id":"2307.15194","last_updated":"2023-07-27T20:59:02Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T15:59:30.956483Z","submitted_at":"2023-07-27T20:59:02Z","title":"Inhomogeneous Cosmology using General Relativistic Smoothed Particle Hydrodynamics coupled to Numerical Relativity"},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2307.15194."}