{"as_of":"2026-08-16T21:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:27d1e48c3a4baf6481c832288de877745bdadc9979d3f6d58d6399465f454332","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":"2026-08-16T06:30:59.297886+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":"2026-06-28T13:20:12.804063Z","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":"2026-07-02T00:36:24.185293Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2503.03189","last_updated":"2025-07-11T11:31:27Z","snapshot_observed_at":"2026-08-16T12:52:59.598397Z","submitted_at":"2025-03-05T05:12:44Z","title":"Equations of motion for compact binary systems in general relativity: Do they depend on the bodies' internal structure at the third post-Newtonian order?","version":2},"cited_work":{"arxiv_id":"2503.03189","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.03189","snapshot_observed_at":"2026-07-02T00:36:24.185293Z","title":null,"venue":null,"work_id":"ccb227cb-7700-4eb9-84f8-6d5c76d16d13","year":2025},"citing_paper":{"arxiv_id":"2605.15160","last_updated":"2026-05-14T17:53:26Z","snapshot_observed_at":"2026-08-11T15:15:38.373630Z","submitted_at":"2026-05-14T17:53:26Z","title":"N-body next-to-leading order gravitational spin-orbit interaction via effective field theory","version":1},"reference_index":116,"source":"pdf_text","source_observed_at":"2026-05-15T03:03:16.273348Z"},"links":{"cited_paper":"/paper/2503.03189","citing_paper":"/paper/2605.15160"},"observation_digest":"sha256:0c8bc0ad07617a4708dd432dda8e7ec48ed3fdea335ac407dc58df4982d793eb","observation_id":"e6207f99-1365-4787-8eed-653fc250bed3","resolution":{"observed_at":"2026-05-15T03:03:56.837364Z","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":"2503.03189","last_updated":"2025-07-11T11:31:27Z","snapshot_observed_at":"2026-08-16T12:52:59.598397Z","submitted_at":"2025-03-05T05:12:44Z","title":"Equations of motion for compact binary systems in general relativity: Do they depend on the bodies' internal structure at the third post-Newtonian order?","version":2},"cited_work":{"arxiv_id":"2503.03189","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.03189","snapshot_observed_at":"2026-07-02T00:36:24.185293Z","title":null,"venue":null,"work_id":"ccb227cb-7700-4eb9-84f8-6d5c76d16d13","year":2025},"citing_paper":{"arxiv_id":"2606.02329","last_updated":"2026-06-01T14:41:03Z","snapshot_observed_at":"2026-08-06T19:41:30.782936Z","submitted_at":"2026-06-01T14:41:03Z","title":"Equivalence Principle violation in metric-affine gravity and finite-temperature effects","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-06-28T13:20:12.804063Z"},"links":{"cited_paper":"/paper/2503.03189","citing_paper":"/paper/2606.02329"},"observation_digest":"sha256:9dd9449e56b1eefac52da67c6817e73450f01bfe15b0e273b7a2a0480479759f","observation_id":"2fe2fee7-61fa-4e3c-905f-120071a22188","resolution":{"observed_at":"2026-07-02T00:36:24.186752Z","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/2503.03189/citation-record","integrity":"/paper/2503.03189/integrity","json":"/paper/2503.03189/citation-record.json","paper":"/paper/2503.03189"},"outbound":[],"paper":{"arxiv_id":"2503.03189","last_updated":"2025-07-11T11:31:27Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-16T12:52:59.598397Z","submitted_at":"2025-03-05T05:12:44Z","title":"Equations of motion for compact binary systems in general relativity: Do they depend on the bodies' internal structure at the third post-Newtonian order?"},"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 2 inbound Pith citation observations for arXiv:2503.03189."}