{"as_of":"2026-08-15T21:13:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:91db600050998ee0ff6c1bb90814f4895d0b1c926f154b35af5e0045035cdaee","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":"2026-08-15T06:32:42.880941+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":"2026-08-14T14:30:02.103664Z","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":"2026-07-12T18:39:00.130667Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1609.09855","last_updated":"2016-09-30T18:42:58Z","snapshot_observed_at":"2026-08-15T06:00:39.463663Z","submitted_at":"2016-09-30T18:42:58Z","title":"Testing coupled dark energy models with their cosmological background evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.09855","snapshot_observed_at":"2026-08-14T14:30:02.103664Z","title":"van de Bruck, J","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03098","last_updated":"2020-05-28T13:31:30Z","snapshot_observed_at":"2026-08-15T17:08:55.607498Z","submitted_at":"2019-08-08T14:39:57Z","title":"Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy","version":3},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-14T14:30:02.103664Z"},"links":{"cited_paper":"/paper/1609.09855","citing_paper":"/paper/1908.03098"},"observation_digest":"sha256:c503f636a476b1b8beedee8818256b9658a8814c551fb950936b783d4f516772","observation_id":"aa35272e-40c2-4bae-abbe-1c984d9f9953","resolution":{"observed_at":"2026-08-14T14:30:02.103664Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.09855","last_updated":"2016-09-30T18:42:58Z","snapshot_observed_at":"2026-08-15T06:00:39.463663Z","submitted_at":"2016-09-30T18:42:58Z","title":"Testing coupled dark energy models with their cosmological background evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.09855","snapshot_observed_at":"2026-08-06T18:14:19.693664Z","title":"van de Bruck, J","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.09258","last_updated":"2025-07-12T11:35:53Z","snapshot_observed_at":"2026-08-13T11:10:19.237636Z","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":118,"source":"pdf_text","source_observed_at":"2026-08-06T18:14:19.693664Z"},"links":{"cited_paper":"/paper/1609.09855","citing_paper":"/paper/2507.09258"},"observation_digest":"sha256:2ed7ee37ec8058fa29b5ba2e6e3e5268899c4f223ab1e7cda37cd31f54d1bac0","observation_id":"f89dbd83-83b4-4c92-8675-b454378a32fc","resolution":{"observed_at":"2026-08-06T18:14:19.693664Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.09855","last_updated":"2016-09-30T18:42:58Z","snapshot_observed_at":"2026-08-15T06:00:39.463663Z","submitted_at":"2016-09-30T18:42:58Z","title":"Testing coupled dark energy models with their cosmological background evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.09855","snapshot_observed_at":"2026-08-05T16:03:01.203992Z","title":"van de Bruck, J","venue":null,"work_id":null,"year":2017},"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":41,"source":"pdf_text","source_observed_at":"2026-08-05T16:03:01.203992Z"},"links":{"cited_paper":"/paper/1609.09855","citing_paper":"/paper/2508.19109"},"observation_digest":"sha256:b4dafd94c8bab5b158b35487ec3ff368c8df765c5414787cb4a44ded668adfcc","observation_id":"d6ea4314-7b19-44c0-8a95-023002d9eda3","resolution":{"observed_at":"2026-08-05T16:03:01.203992Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.09855","last_updated":"2016-09-30T18:42:58Z","snapshot_observed_at":"2026-08-15T06:00:39.463663Z","submitted_at":"2016-09-30T18:42:58Z","title":"Testing coupled dark energy models with their cosmological background evolution","version":1},"cited_work":{"arxiv_id":"1609.09855","doi":null,"metadata_source":"pith","pith_arxiv_id":"1609.09855","snapshot_observed_at":"2026-07-12T18:39:00.130667Z","title":"Testing coupled dark energy models with their cosmological background evolution","venue":"astro-ph.CO","work_id":"709f753b-ca10-4693-a63c-cee34a0cbb60","year":2016},"citing_paper":{"arxiv_id":"2604.21770","last_updated":"2026-06-05T08:25:09Z","snapshot_observed_at":"2026-08-11T12:44:09.340715Z","submitted_at":"2026-04-23T15:28:34Z","title":"Accelerating scaling solutions from dark matter particle creation","version":2},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-07-12T18:37:05.978670Z"},"links":{"cited_paper":"/paper/1609.09855","citing_paper":"/paper/2604.21770"},"observation_digest":"sha256:69b0fd767986e570925eb0c87576980c3a0c0d2528114583920b457641749cd0","observation_id":"43682f3b-b539-45ee-85be-e7b1cfdf790e","resolution":{"observed_at":"2026-07-12T18:39:00.135398Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1609.09855/citation-record","integrity":"/paper/1609.09855/integrity","json":"/paper/1609.09855/citation-record.json","paper":"/paper/1609.09855"},"outbound":[],"paper":{"arxiv_id":"1609.09855","last_updated":"2016-09-30T18:42:58Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-15T06:00:39.463663Z","submitted_at":"2016-09-30T18:42:58Z","title":"Testing coupled dark energy models with their cosmological background evolution"},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1609.09855."}