{"as_of":"2026-08-13T06:30:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:90994b9516a62954243c7429f3a3526a120fef1805c16f9aa857203886257ebe","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T11:29:07.698617Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":100,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1312.6328","last_updated":"2014-04-20T13:52:02Z","snapshot_observed_at":"2026-07-06T03:31:37.428348Z","submitted_at":"2013-12-22T01:58:54Z","title":"Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.6328","snapshot_observed_at":"2026-08-12T11:29:07.698617Z","title":"Li and X","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.18300","last_updated":"2025-07-10T15:45:02Z","snapshot_observed_at":"2026-08-13T02:04:26.045413Z","submitted_at":"2024-11-27T12:47:00Z","title":"Interacting phantom dark energy: new accelerating scaling attractors","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-12T11:29:07.698617Z"},"links":{"cited_paper":"/paper/1312.6328","citing_paper":"/paper/2411.18300"},"observation_digest":"sha256:3dba14f708a7f1418f058e55302fe0146cc8f44684d1ff25575c18229f35d77f","observation_id":"7fbeb86a-e949-4e41-aa6c-00528e01185b","resolution":{"observed_at":"2026-08-12T11:29:07.698617Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.6328","last_updated":"2014-04-20T13:52:02Z","snapshot_observed_at":"2026-07-06T03:31:37.428348Z","submitted_at":"2013-12-22T01:58:54Z","title":"Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.6328","snapshot_observed_at":"2026-08-06T18:14:13.005429Z","title":"Li and X","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.09258","last_updated":"2025-07-12T11:35:53Z","snapshot_observed_at":"2026-08-07T05:45:09.556857Z","submitted_at":"2025-07-12T11:35:53Z","title":"Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T18:14:13.005429Z"},"links":{"cited_paper":"/paper/1312.6328","citing_paper":"/paper/2507.09258"},"observation_digest":"sha256:12e1557bd9a4aa4b49f918320d0455e6701e81b9ee70ca300bd8a4a15a98a445","observation_id":"379c1baa-39b3-4b7b-8ff0-ca6efc6cc28d","resolution":{"observed_at":"2026-08-06T18:14:13.005429Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.6328","last_updated":"2014-04-20T13:52:02Z","snapshot_observed_at":"2026-07-06T03:31:37.428348Z","submitted_at":"2013-12-22T01:58:54Z","title":"Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.6328","snapshot_observed_at":"2026-08-05T16:03:01.162859Z","title":"Li and X","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2508.19109","last_updated":"2025-08-26T15:13:27Z","snapshot_observed_at":"2026-08-05T23:53:28.863082Z","submitted_at":"2025-08-26T15:13:27Z","title":"Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-05T16:03:01.162859Z"},"links":{"cited_paper":"/paper/1312.6328","citing_paper":"/paper/2508.19109"},"observation_digest":"sha256:e1dc17d2f83db8ae5974d296c38169b8f2820483ed3e96cf22094437977e5730","observation_id":"a01a08d4-5908-4350-a489-57191bec7b5f","resolution":{"observed_at":"2026-08-05T16:03:01.162859Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.6328","last_updated":"2014-04-20T13:52:02Z","snapshot_observed_at":"2026-07-06T03:31:37.428348Z","submitted_at":"2013-12-22T01:58:54Z","title":"Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints","version":3},"cited_work":{"arxiv_id":"1312.6328","doi":"10.1103/physrevd.89.083009","metadata_source":"pith","pith_arxiv_id":"1312.6328","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints","venue":"astro-ph.CO","work_id":"bc4ea8f5-bfe2-41a1-ad60-084da79db293","year":2013},"citing_paper":{"arxiv_id":"2606.21826","last_updated":"2026-07-16T15:49:18Z","snapshot_observed_at":"2026-08-02T10:41:21.508983Z","submitted_at":"2026-06-20T01:29:51Z","title":"Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\\Lambda$CDM Interpretations, and Tensions","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1312.6328","citing_paper":"/paper/2606.21826"},"observation_digest":"sha256:ae04f6ea9afbd4c021739e92940e8b3d0aaaea6492ebb269278352e762d9d84c","observation_id":"878428dc-2abf-416b-88ba-fb15365b24b9","resolution":{"observed_at":"2026-06-26T12:39:28.292718Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1312.6328/citation-record","integrity":"/paper/1312.6328/integrity","json":"/paper/1312.6328/citation-record.json","paper":"/paper/1312.6328"},"outbound":[],"paper":{"arxiv_id":"1312.6328","last_updated":"2014-04-20T13:52:02Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T03:31:37.428348Z","submitted_at":"2013-12-22T01:58:54Z","title":"Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1312.6328."}