{"as_of":"2026-08-14T09:17:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7b73c34200be00ee0d16eb9f29ac010da416d400effa4a4163515acfeb5e35d5","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T17:28:33.776348Z","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":"2026-07-02T10:36:52.604810Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2310.16911","last_updated":"2024-04-12T13:44:53Z","snapshot_observed_at":"2026-08-13T05:40:26.006507Z","submitted_at":"2023-10-25T18:22:34Z","title":"Observational Constraints on Dynamical Dark Energy Models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.16911","snapshot_observed_at":"2026-08-11T17:28:33.776348Z","title":"Avsajanishvili, G.Y","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.09064","last_updated":"2025-06-24T01:24:27Z","snapshot_observed_at":"2026-08-12T15:08:50.818044Z","submitted_at":"2024-12-12T08:51:54Z","title":"A comprehensive numerical study on four categories of holographic dark energy models","version":3},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-11T17:28:33.776348Z"},"links":{"cited_paper":"/paper/2310.16911","citing_paper":"/paper/2412.09064"},"observation_digest":"sha256:b7ddd704b35b86355113a0ccb1daee4fdeed8bffedb2bfdb26b0bd2c3dfa18a8","observation_id":"76ff4db7-c6fe-4162-a2d9-f3faf30bb290","resolution":{"observed_at":"2026-08-11T17:28:33.776348Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.16911","last_updated":"2024-04-12T13:44:53Z","snapshot_observed_at":"2026-08-13T05:40:26.006507Z","submitted_at":"2023-10-25T18:22:34Z","title":"Observational Constraints on Dynamical Dark Energy Models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.16911","snapshot_observed_at":"2026-08-10T14:54:50.562529Z","title":"Avsajanishvili, G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.14909","last_updated":"2025-01-24T20:22:55Z","snapshot_observed_at":"2026-08-11T03:26:23.244488Z","submitted_at":"2025-01-24T20:22:55Z","title":"Cuscuton-like contribution to dark energy evolution","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-10T14:54:50.562529Z"},"links":{"cited_paper":"/paper/2310.16911","citing_paper":"/paper/2501.14909"},"observation_digest":"sha256:22bc6651ed4264d68984f5f1cb60d52959161dbf8a81c53d1c919c13f447f0d2","observation_id":"22faf81b-bdd3-4d1e-8de2-cb9e4c026c64","resolution":{"observed_at":"2026-08-10T14:54:50.562529Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.16911","last_updated":"2024-04-12T13:44:53Z","snapshot_observed_at":"2026-08-13T05:40:26.006507Z","submitted_at":"2023-10-25T18:22:34Z","title":"Observational Constraints on Dynamical Dark Energy Models","version":2},"cited_work":{"arxiv_id":"2310.16911","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2310.16911","snapshot_observed_at":"2026-07-02T10:36:52.604810Z","title":"Avsajanishvili, G","venue":null,"work_id":"5ecdb19b-24f8-48c3-8b1f-786e7b252931","year":2024},"citing_paper":{"arxiv_id":"2606.05352","last_updated":"2026-06-14T13:15:33Z","snapshot_observed_at":"2026-08-10T23:30:42.015278Z","submitted_at":"2026-06-03T18:55:18Z","title":"Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-06-28T04:59:43.971930Z"},"links":{"cited_paper":"/paper/2310.16911","citing_paper":"/paper/2606.05352"},"observation_digest":"sha256:0053ab3ac22ffb37067debe94de8f447da8a259b0dded6d14d770b006c0449df","observation_id":"ac96b8d7-82e4-4ed0-8943-6c1adb734f8c","resolution":{"observed_at":"2026-07-02T10:36:52.606136Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.16911","last_updated":"2024-04-12T13:44:53Z","snapshot_observed_at":"2026-08-13T05:40:26.006507Z","submitted_at":"2023-10-25T18:22:34Z","title":"Observational Constraints on Dynamical Dark Energy Models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.16911","snapshot_observed_at":"2026-07-12T15:09:17.581029Z","title":"Avsajanishvili, G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2606.05352","last_updated":"2026-06-14T13:15:33Z","snapshot_observed_at":"2026-08-10T23:30:42.015278Z","submitted_at":"2026-06-03T18:55:18Z","title":"Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-07-12T15:09:17.581029Z"},"links":{"cited_paper":"/paper/2310.16911","citing_paper":"/paper/2606.05352"},"observation_digest":"sha256:2e17b8d44bed29fe979f2a2715d951b0db086a6a251ccc489eecfd271ca8781d","observation_id":"2b9c0cbf-491a-490f-91f0-f65bfcd677c5","resolution":{"observed_at":"2026-07-12T15:09:17.581029Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.16911","last_updated":"2024-04-12T13:44:53Z","snapshot_observed_at":"2026-08-13T05:40:26.006507Z","submitted_at":"2023-10-25T18:22:34Z","title":"Observational Constraints on Dynamical Dark Energy Models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.16911","snapshot_observed_at":"2026-07-12T11:44:30.277942Z","title":"Avsajanishvili, G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2606.27441","last_updated":"2026-07-08T21:37:21Z","snapshot_observed_at":"2026-08-10T03:21:22.346591Z","submitted_at":"2026-06-25T18:03:16Z","title":"Collider Probes of Dark Energy Microphysics","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-07-12T11:44:30.277942Z"},"links":{"cited_paper":"/paper/2310.16911","citing_paper":"/paper/2606.27441"},"observation_digest":"sha256:cd54e42514fc1b60fc8b3ef1eb392bd521dff9deb1b63adcbad45f988f8cff85","observation_id":"a20356ac-0928-48f2-8291-a3518b76e12d","resolution":{"observed_at":"2026-07-12T11:44:30.277942Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2310.16911/citation-record","integrity":"/paper/2310.16911/integrity","json":"/paper/2310.16911/citation-record.json","paper":"/paper/2310.16911"},"outbound":[],"paper":{"arxiv_id":"2310.16911","last_updated":"2024-04-12T13:44:53Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-13T05:40:26.006507Z","submitted_at":"2023-10-25T18:22:34Z","title":"Observational Constraints on Dynamical Dark Energy Models"},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2310.16911."}