{"as_of":"2026-08-13T15:53:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:336c02c5cb1ca7ee6ff472ba0d33c12e10eb34574147c46ea843477c4a6d5ea0","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":9,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":9,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T11:29:07.596584Z","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":"2026-07-03T07:47:45.327395Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2310.07260","last_updated":"2024-10-25T19:17:58Z","snapshot_observed_at":"2026-08-13T05:52:24.919533Z","submitted_at":"2023-10-11T07:37:16Z","title":"On the interacting dark energy scenarios $-$ the case for Hubble constant tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.07260","snapshot_observed_at":"2026-08-12T11:29:07.596584Z","title":"Pan and W","venue":null,"work_id":null,"year":2023},"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":35,"source":"pdf_text","source_observed_at":"2026-08-12T11:29:07.596584Z"},"links":{"cited_paper":"/paper/2310.07260","citing_paper":"/paper/2411.18300"},"observation_digest":"sha256:e43845e1b0f9af67d67bf421e47c2ccc7d1b1257c2682d2ba80066fbd27fb49a","observation_id":"cb8282ee-4233-421c-911e-b074b8bc2322","resolution":{"observed_at":"2026-08-12T11:29:07.596584Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.07260","last_updated":"2024-10-25T19:17:58Z","snapshot_observed_at":"2026-08-13T05:52:24.919533Z","submitted_at":"2023-10-11T07:37:16Z","title":"On the interacting dark energy scenarios $-$ the case for Hubble constant tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.07260","snapshot_observed_at":"2026-08-10T19:20:16.867186Z","title":"Pan and W","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.10323","last_updated":"2025-02-24T12:41:54Z","snapshot_observed_at":"2026-08-11T14:26:14.335628Z","submitted_at":"2025-01-17T17:52:49Z","title":"Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-10T19:20:16.867186Z"},"links":{"cited_paper":"/paper/2310.07260","citing_paper":"/paper/2501.10323"},"observation_digest":"sha256:f712ee60b39762aa320dff0f581919c2f878bd825813b2a33ace3ef62f377052","observation_id":"0e7293b8-85b3-4baf-b29c-3101f20618aa","resolution":{"observed_at":"2026-08-10T19:20:16.867186Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.07260","last_updated":"2024-10-25T19:17:58Z","snapshot_observed_at":"2026-08-13T05:52:24.919533Z","submitted_at":"2023-10-11T07:37:16Z","title":"On the interacting dark energy scenarios $-$ the case for Hubble constant tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.07260","snapshot_observed_at":"2026-08-06T18:14:17.692001Z","title":"Pan and W","venue":null,"work_id":null,"year":2023},"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":96,"source":"pdf_text","source_observed_at":"2026-08-06T18:14:17.692001Z"},"links":{"cited_paper":"/paper/2310.07260","citing_paper":"/paper/2507.09258"},"observation_digest":"sha256:b0efea562ea825bbfe5ac8f7165aaf4c84dd34c5c8ef594acbe2a853810e0d78","observation_id":"f6dc93f5-9ba1-41c0-bed3-79a89554703f","resolution":{"observed_at":"2026-08-06T18:14:17.692001Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.07260","last_updated":"2024-10-25T19:17:58Z","snapshot_observed_at":"2026-08-13T05:52:24.919533Z","submitted_at":"2023-10-11T07:37:16Z","title":"On the interacting dark energy scenarios $-$ the case for Hubble constant tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.07260","snapshot_observed_at":"2026-08-03T11:11:48.807359Z","title":"Pan and W","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2601.07361","last_updated":"2026-07-15T07:08:06Z","snapshot_observed_at":"2026-08-13T05:33:14.828344Z","submitted_at":"2026-01-12T09:36:30Z","title":"Robust Preference for Dark Sector Interactions","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-03T11:11:48.807359Z"},"links":{"cited_paper":"/paper/2310.07260","citing_paper":"/paper/2601.07361"},"observation_digest":"sha256:98bfd56c95212827e107afcba16487b8594df0c16b54e3c70b9eb31071a33c48","observation_id":"d3e731ab-8677-49b8-9209-3fe8b5f39565","resolution":{"observed_at":"2026-08-03T11:11:48.807359Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.07260","last_updated":"2024-10-25T19:17:58Z","snapshot_observed_at":"2026-08-13T05:52:24.919533Z","submitted_at":"2023-10-11T07:37:16Z","title":"On the interacting dark energy scenarios $-$ the case for Hubble constant tension","version":2},"cited_work":{"arxiv_id":"2310.07260","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2310.07260","snapshot_observed_at":"2026-07-03T07:47:45.327395Z","title":"Pan and W","venue":null,"work_id":"31f6635d-076b-4c71-a9ac-8cc3dccb804b","year":2023},"citing_paper":{"arxiv_id":"2601.14222","last_updated":"2026-04-27T15:45:53Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-01-20T18:32:34Z","title":"Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-05-16T12:15:01.997389Z"},"links":{"cited_paper":"/paper/2310.07260","citing_paper":"/paper/2601.14222"},"observation_digest":"sha256:b93b1a948e33faaa2109c39e2c6ecc123d142c529c8f9e342c7653bb103e9484","observation_id":"7afc5884-f35e-45c5-8482-d486460bf67e","resolution":{"observed_at":"2026-05-16T12:17:52.577601Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.07260","last_updated":"2024-10-25T19:17:58Z","snapshot_observed_at":"2026-08-13T05:52:24.919533Z","submitted_at":"2023-10-11T07:37:16Z","title":"On the interacting dark energy scenarios $-$ the case for Hubble constant tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.07260","snapshot_observed_at":"2026-08-02T19:12:04.349265Z","title":"Pan and W","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2603.03468","last_updated":"2026-07-01T12:01:45Z","snapshot_observed_at":"2026-08-08T06:33:55.364180Z","submitted_at":"2026-03-03T19:25:24Z","title":"Background dynamics and observational constraints of flat and non-flat $\\Lambda(t)$CDM models from $H(z)$ and DESI DR2 BAO measurements","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-02T19:12:04.349265Z"},"links":{"cited_paper":"/paper/2310.07260","citing_paper":"/paper/2603.03468"},"observation_digest":"sha256:dce6da074096e5875758f545de598c29dfb66545400200a57c01806946620994","observation_id":"de34a67a-e7a4-4484-b3b6-13538cc11563","resolution":{"observed_at":"2026-08-02T19:12:04.349265Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.07260","last_updated":"2024-10-25T19:17:58Z","snapshot_observed_at":"2026-08-13T05:52:24.919533Z","submitted_at":"2023-10-11T07:37:16Z","title":"On the interacting dark energy scenarios $-$ the case for Hubble constant tension","version":2},"cited_work":{"arxiv_id":"2310.07260","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2310.07260","snapshot_observed_at":"2026-07-03T07:47:45.327395Z","title":"Pan and W","venue":null,"work_id":"31f6635d-076b-4c71-a9ac-8cc3dccb804b","year":2023},"citing_paper":{"arxiv_id":"2605.26116","last_updated":"2026-05-25T17:59:53Z","snapshot_observed_at":"2026-07-06T23:36:01.564747Z","submitted_at":"2026-05-25T17:59:53Z","title":"Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions","version":1},"reference_index":192,"source":"pdf_text","source_observed_at":"2026-06-29T20:17:08.107860Z"},"links":{"cited_paper":"/paper/2310.07260","citing_paper":"/paper/2605.26116"},"observation_digest":"sha256:d6f83cd72616193c94e60e0d9dd5dfea24454c59ac7a39cb32c5197cf35c5a5a","observation_id":"8f2f7a8a-5073-44ab-b05e-df54261c0a65","resolution":{"observed_at":"2026-07-01T16:45:51.350687Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.07260","last_updated":"2024-10-25T19:17:58Z","snapshot_observed_at":"2026-08-13T05:52:24.919533Z","submitted_at":"2023-10-11T07:37:16Z","title":"On the interacting dark energy scenarios $-$ the case for Hubble constant tension","version":2},"cited_work":{"arxiv_id":"2310.07260","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2310.07260","snapshot_observed_at":"2026-07-03T07:47:45.327395Z","title":"Pan and W","venue":null,"work_id":"31f6635d-076b-4c71-a9ac-8cc3dccb804b","year":2023},"citing_paper":{"arxiv_id":"2606.11368","last_updated":"2026-06-09T18:49:28Z","snapshot_observed_at":"2026-08-05T23:51:47.113522Z","submitted_at":"2026-06-09T18:49:28Z","title":"Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-06-27T11:43:20.857862Z"},"links":{"cited_paper":"/paper/2310.07260","citing_paper":"/paper/2606.11368"},"observation_digest":"sha256:5c6b6671624eb566ea99ddd93740f961cbcac41706b5fe2a0163314fe91de28e","observation_id":"498e418b-aa9a-4c44-8705-b6daca62ea8e","resolution":{"observed_at":"2026-07-03T07:47:45.328815Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.07260","last_updated":"2024-10-25T19:17:58Z","snapshot_observed_at":"2026-08-13T05:52:24.919533Z","submitted_at":"2023-10-11T07:37:16Z","title":"On the interacting dark energy scenarios $-$ the case for Hubble constant tension","version":2},"cited_work":{"arxiv_id":"2310.07260","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2310.07260","snapshot_observed_at":"2026-07-03T07:47:45.327395Z","title":"Pan and W","venue":null,"work_id":"31f6635d-076b-4c71-a9ac-8cc3dccb804b","year":2023},"citing_paper":{"arxiv_id":"2606.28288","last_updated":"2026-06-26T17:33:53Z","snapshot_observed_at":"2026-07-31T17:00:11.536162Z","submitted_at":"2026-06-26T17:33:53Z","title":"Generalizing the interacting dilatonic ghost condensate as a dark energy model","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-06-29T02:45:31.549336Z"},"links":{"cited_paper":"/paper/2310.07260","citing_paper":"/paper/2606.28288"},"observation_digest":"sha256:36a634cd93e71c7ba83a30055feaa319d57275e75d3e83b8e4c0181636f9b046","observation_id":"e3c8a52c-789d-49e0-8187-2dc883bd5254","resolution":{"observed_at":"2026-07-01T17:55:52.605436Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2310.07260/citation-record","integrity":"/paper/2310.07260/integrity","json":"/paper/2310.07260/citation-record.json","paper":"/paper/2310.07260"},"outbound":[],"paper":{"arxiv_id":"2310.07260","last_updated":"2024-10-25T19:17:58Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-13T05:52:24.919533Z","submitted_at":"2023-10-11T07:37:16Z","title":"On the interacting dark energy scenarios $-$ the case for Hubble constant 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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2310.07260."}