{"as_of":"2026-08-15T08:04:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ccfe3d44a69f449c44460cd5e55684e69784d49c6ce5c73d85672ba4f336361c","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":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-05T16:03:01.338975Z","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":"2026-07-04T22:30:10.373469Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2105.09249","last_updated":"2021-10-27T14:20:56Z","snapshot_observed_at":"2026-08-14T20:58:04.228985Z","submitted_at":"2021-05-19T16:51:19Z","title":"Dark energy-dark matter interactions as a solution to the $S_8$ tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.09249","snapshot_observed_at":"2026-08-05T16:03:01.338975Z","title":"Lucca, Dark energy–dark matter interactions as a solution to the S8 tension, Phys","venue":null,"work_id":null,"year":2021},"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":84,"source":"pdf_text","source_observed_at":"2026-08-05T16:03:01.338975Z"},"links":{"cited_paper":"/paper/2105.09249","citing_paper":"/paper/2508.19109"},"observation_digest":"sha256:096aa57356da68952ef8a4dc7e0844733d4344f23d61e168fa2f7aa009b3639d","observation_id":"8e31857c-15d2-4972-a2f7-fb51439dbd58","resolution":{"observed_at":"2026-08-05T16:03:01.338975Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.09249","last_updated":"2021-10-27T14:20:56Z","snapshot_observed_at":"2026-08-14T20:58:04.228985Z","submitted_at":"2021-05-19T16:51:19Z","title":"Dark energy-dark matter interactions as a solution to the $S_8$ tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.09249","snapshot_observed_at":"2026-08-03T11:11:48.899277Z","title":"Lucca, Phys","venue":null,"work_id":null,"year":2021},"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":110,"source":"pdf_text","source_observed_at":"2026-08-03T11:11:48.899277Z"},"links":{"cited_paper":"/paper/2105.09249","citing_paper":"/paper/2601.07361"},"observation_digest":"sha256:693be3f4e78bd54faf31a1b3cbc1c78ae67cbb456b9e252872bd9395503bba92","observation_id":"414679e8-aaea-4e03-a585-a5d33c299798","resolution":{"observed_at":"2026-08-03T11:11:48.899277Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.09249","last_updated":"2021-10-27T14:20:56Z","snapshot_observed_at":"2026-08-14T20:58:04.228985Z","submitted_at":"2021-05-19T16:51:19Z","title":"Dark energy-dark matter interactions as a solution to the $S_8$ tension","version":2},"cited_work":{"arxiv_id":"2105.09249","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2105.09249","snapshot_observed_at":"2026-07-04T22:30:10.373469Z","title":"Lucca, Phys","venue":null,"work_id":"df711805-d137-4a3f-9f5c-52d20aeff930","year":2021},"citing_paper":{"arxiv_id":"2604.21670","last_updated":"2026-06-10T15:20:34Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-23T13:36:10Z","title":"Effective field theory interpretation of ATLAS measurements involving the Higgs boson, electroweak bosons and the top quark","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-07-04T22:27:16.736476Z"},"links":{"cited_paper":"/paper/2105.09249","citing_paper":"/paper/2604.21670"},"observation_digest":"sha256:3c7a00521cb6d6f177098995c3b13d992d0d1da65b29007892ec2cb034ccc22a","observation_id":"7a731dee-5725-47cf-9f90-b9de1d8424e2","resolution":{"observed_at":"2026-07-04T22:30:10.375073Z","resolver_source":"arxiv_id","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"}},{"citation":{"cited_paper":{"arxiv_id":"2105.09249","last_updated":"2021-10-27T14:20:56Z","snapshot_observed_at":"2026-08-14T20:58:04.228985Z","submitted_at":"2021-05-19T16:51:19Z","title":"Dark energy-dark matter interactions as a solution to the $S_8$ tension","version":2},"cited_work":{"arxiv_id":"2105.09249","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2105.09249","snapshot_observed_at":"2026-07-04T22:30:10.373469Z","title":"Lucca, Phys","venue":null,"work_id":"df711805-d137-4a3f-9f5c-52d20aeff930","year":2021},"citing_paper":{"arxiv_id":"2604.21671","last_updated":"2026-04-23T13:36:31Z","snapshot_observed_at":"2026-08-15T05:11:44.105082Z","submitted_at":"2026-04-23T13:36:31Z","title":"Saturation Mechanisms in the Interacting Dark Sector","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-08T14:11:14.739262Z"},"links":{"cited_paper":"/paper/2105.09249","citing_paper":"/paper/2604.21671"},"observation_digest":"sha256:9dbb23d98b69c583d54937d570c0d1f99dd451e57a013a92641ffa1f70d3ab45","observation_id":"cf4f1074-2f26-495a-8599-8391016be8ae","resolution":{"observed_at":"2026-05-11T18:46:06.893143Z","resolver_source":"arxiv_id","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"}},{"citation":{"cited_paper":{"arxiv_id":"2105.09249","last_updated":"2021-10-27T14:20:56Z","snapshot_observed_at":"2026-08-14T20:58:04.228985Z","submitted_at":"2021-05-19T16:51:19Z","title":"Dark energy-dark matter interactions as a solution to the $S_8$ tension","version":2},"cited_work":{"arxiv_id":"2105.09249","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2105.09249","snapshot_observed_at":"2026-07-04T22:30:10.373469Z","title":"Lucca, Phys","venue":null,"work_id":"df711805-d137-4a3f-9f5c-52d20aeff930","year":2021},"citing_paper":{"arxiv_id":"2606.05005","last_updated":"2026-06-03T15:26:36Z","snapshot_observed_at":"2026-07-06T23:45:02.342193Z","submitted_at":"2026-06-03T15:26:36Z","title":"Neutrino mass constraints in interacting dark energy models after DESI DR2","version":1},"reference_index":148,"source":"pdf_text","source_observed_at":"2026-06-28T04:52:33.342231Z"},"links":{"cited_paper":"/paper/2105.09249","citing_paper":"/paper/2606.05005"},"observation_digest":"sha256:4c9378f2e0d6b0a62b08800a906046739386ae5a1b5abc2184b47bb427c201d6","observation_id":"491c025e-d26f-43e7-abaa-d19575c1a869","resolution":{"observed_at":"2026-07-02T10:56:52.453711Z","resolver_source":"arxiv_id","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"}},{"citation":{"cited_paper":{"arxiv_id":"2105.09249","last_updated":"2021-10-27T14:20:56Z","snapshot_observed_at":"2026-08-14T20:58:04.228985Z","submitted_at":"2021-05-19T16:51:19Z","title":"Dark energy-dark matter interactions as a solution to the $S_8$ tension","version":2},"cited_work":{"arxiv_id":"2105.09249","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2105.09249","snapshot_observed_at":"2026-07-04T22:30:10.373469Z","title":"Lucca, Phys","venue":null,"work_id":"df711805-d137-4a3f-9f5c-52d20aeff930","year":2021},"citing_paper":{"arxiv_id":"2606.28288","last_updated":"2026-06-26T17:33:53Z","snapshot_observed_at":"2026-08-15T04:44:43.118826Z","submitted_at":"2026-06-26T17:33:53Z","title":"Generalizing the interacting dilatonic ghost condensate as a dark energy model","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-06-29T02:45:31.549336Z"},"links":{"cited_paper":"/paper/2105.09249","citing_paper":"/paper/2606.28288"},"observation_digest":"sha256:a0517e61b1dc997bc65aad70f05cecf1199f9e67f3997c518b96b26286081369","observation_id":"df92fb9a-9c91-47b5-8c4f-017c4f5cea2b","resolution":{"observed_at":"2026-07-01T18:05:58.099821Z","resolver_source":"arxiv_id","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/2105.09249/citation-record","integrity":"/paper/2105.09249/integrity","json":"/paper/2105.09249/citation-record.json","paper":"/paper/2105.09249"},"outbound":[],"paper":{"arxiv_id":"2105.09249","last_updated":"2021-10-27T14:20:56Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T20:58:04.228985Z","submitted_at":"2021-05-19T16:51:19Z","title":"Dark energy-dark matter interactions as a solution to the $S_8$ 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":"2026-08-15T06:32:42.880941+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 6 inbound Pith citation observations for arXiv:2105.09249."}