{"as_of":"2026-08-13T16:59:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:cd688262713c92c76f73d2f70172d1cba0cd885140efe2a07cb19b53cdc39cbd","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":11,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":11,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":11,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":11,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-05T16:03:01.382246Z","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":"2026-07-03T07:57:44.208058Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2207.05955","last_updated":"2024-05-30T07:58:59Z","snapshot_observed_at":"2026-08-13T15:05:14.357879Z","submitted_at":"2022-07-13T04:15:51Z","title":"Can interacting dark energy with dynamical coupling resolve the Hubble tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.05955","snapshot_observed_at":"2026-08-05T16:03:01.382246Z","title":"Yao and X.-H","venue":null,"work_id":null,"year":2023},"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":98,"source":"pdf_text","source_observed_at":"2026-08-05T16:03:01.382246Z"},"links":{"cited_paper":"/paper/2207.05955","citing_paper":"/paper/2508.19109"},"observation_digest":"sha256:399d32c6713d164e92664d24e8b8b14967d976bc73c7c0497a0781631e59541d","observation_id":"f70551d1-aeed-49c4-acb6-1f4a3a93791c","resolution":{"observed_at":"2026-08-05T16:03:01.382246Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.05955","last_updated":"2024-05-30T07:58:59Z","snapshot_observed_at":"2026-08-13T15:05:14.357879Z","submitted_at":"2022-07-13T04:15:51Z","title":"Can interacting dark energy with dynamical coupling resolve the Hubble tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.05955","snapshot_observed_at":"2026-08-04T12:53:52.778676Z","title":"Yao and X.-H","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2510.01974","last_updated":"2026-01-19T10:15:04Z","snapshot_observed_at":"2026-08-04T12:53:22.243014Z","submitted_at":"2025-10-02T12:47:51Z","title":"BAO miscalibration cannot rescue late-time solutions to the Hubble tension","version":2},"reference_index":233,"source":"pdf_text","source_observed_at":"2026-08-04T12:53:52.778676Z"},"links":{"cited_paper":"/paper/2207.05955","citing_paper":"/paper/2510.01974"},"observation_digest":"sha256:b8c52f21c8745b957d2855de2dd236ecf461b67fc02f866acc91b104fc42931f","observation_id":"01bfb308-6251-4b7c-b101-1579b80f9ebc","resolution":{"observed_at":"2026-08-04T12:53:52.778676Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.05955","last_updated":"2024-05-30T07:58:59Z","snapshot_observed_at":"2026-08-13T15:05:14.357879Z","submitted_at":"2022-07-13T04:15:51Z","title":"Can interacting dark energy with dynamical coupling resolve the Hubble tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.05955","snapshot_observed_at":"2026-08-04T09:59:19.551619Z","title":"Yao and X.-H","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2510.12627","last_updated":"2026-06-20T07:00:45Z","snapshot_observed_at":"2026-08-12T13:22:12.009948Z","submitted_at":"2025-10-14T15:24:50Z","title":"Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-04T09:59:19.551619Z"},"links":{"cited_paper":"/paper/2207.05955","citing_paper":"/paper/2510.12627"},"observation_digest":"sha256:0acbf20dbe854d22a4fddd5f569750401aeb9614db5a7f6afabcf38126a394fc","observation_id":"8374d64a-05ec-47a9-b294-d2cbaf1f79cb","resolution":{"observed_at":"2026-08-04T09:59:19.551619Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.05955","last_updated":"2024-05-30T07:58:59Z","snapshot_observed_at":"2026-08-13T15:05:14.357879Z","submitted_at":"2022-07-13T04:15:51Z","title":"Can interacting dark energy with dynamical coupling resolve the Hubble tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.05955","snapshot_observed_at":"2026-08-04T07:19:39.893145Z","title":"Yao and X.-H","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2510.26355","last_updated":"2026-07-07T01:20:38Z","snapshot_observed_at":"2026-08-12T22:27:53.420894Z","submitted_at":"2025-10-30T11:06:11Z","title":"Model-independent late-universe measurements of $H_0$ and $\\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-04T07:19:39.893145Z"},"links":{"cited_paper":"/paper/2207.05955","citing_paper":"/paper/2510.26355"},"observation_digest":"sha256:786ceeb6f79d3bcd5708b2db8f9d55728bc01cb39803e74040b58c084bce99c9","observation_id":"855c2265-d53d-4930-a2ea-ea80ae1550f8","resolution":{"observed_at":"2026-08-04T07:19:39.893145Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.05955","last_updated":"2024-05-30T07:58:59Z","snapshot_observed_at":"2026-08-13T15:05:14.357879Z","submitted_at":"2022-07-13T04:15:51Z","title":"Can interacting dark energy with dynamical coupling resolve the Hubble tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.05955","snapshot_observed_at":"2026-08-03T11:11:48.843808Z","title":"Yao and X.-H","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":87,"source":"pdf_text","source_observed_at":"2026-08-03T11:11:48.843808Z"},"links":{"cited_paper":"/paper/2207.05955","citing_paper":"/paper/2601.07361"},"observation_digest":"sha256:4a6962025f5fcb9d9e9188c13faeb85dadd9a2104282c8feeb1046d95bb85a23","observation_id":"84eee012-9f90-405b-9866-a6bf251efc18","resolution":{"observed_at":"2026-08-03T11:11:48.843808Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.05955","last_updated":"2024-05-30T07:58:59Z","snapshot_observed_at":"2026-08-13T15:05:14.357879Z","submitted_at":"2022-07-13T04:15:51Z","title":"Can interacting dark energy with dynamical coupling resolve the Hubble tension","version":3},"cited_work":{"arxiv_id":"2207.05955","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.05955","snapshot_observed_at":"2026-07-03T07:57:44.208058Z","title":"Yao and X.-H","venue":null,"work_id":"0b254e5a-355a-4a8b-9d96-e5802b466f35","year":2023},"citing_paper":{"arxiv_id":"2605.14977","last_updated":"2026-08-06T13:45:13Z","snapshot_observed_at":"2026-08-09T23:12:14.655552Z","submitted_at":"2026-05-14T15:41:53Z","title":"Unified dark sector and Hubble-tension alleviation in scalar-vector-tensor gravity","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-06-30T20:07:39.265059Z"},"links":{"cited_paper":"/paper/2207.05955","citing_paper":"/paper/2605.14977"},"observation_digest":"sha256:b29e85728c0d11bfd61b8e1f39bb3ca9761141fb0928ab219b050beeb40a2f3a","observation_id":"e59ecc6b-1570-4fd6-9e00-cb7c22e0aef7","resolution":{"observed_at":"2026-06-30T20:15:05.543143Z","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":"2207.05955","last_updated":"2024-05-30T07:58:59Z","snapshot_observed_at":"2026-08-13T15:05:14.357879Z","submitted_at":"2022-07-13T04:15:51Z","title":"Can interacting dark energy with dynamical coupling resolve the Hubble tension","version":3},"cited_work":{"arxiv_id":"2207.05955","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.05955","snapshot_observed_at":"2026-07-03T07:57:44.208058Z","title":"Yao and X.-H","venue":null,"work_id":"0b254e5a-355a-4a8b-9d96-e5802b466f35","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":181,"source":"pdf_text","source_observed_at":"2026-06-29T20:17:08.107860Z"},"links":{"cited_paper":"/paper/2207.05955","citing_paper":"/paper/2605.26116"},"observation_digest":"sha256:471894ca2d3a22a13ff19403add4b6a0ce3014d19253821a0a50d4e313b33c64","observation_id":"9f5b41a3-bb6a-41ce-bf3f-aa34feaedf53","resolution":{"observed_at":"2026-07-01T16:35:50.598593Z","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":"2207.05955","last_updated":"2024-05-30T07:58:59Z","snapshot_observed_at":"2026-08-13T15:05:14.357879Z","submitted_at":"2022-07-13T04:15:51Z","title":"Can interacting dark energy with dynamical coupling resolve the Hubble tension","version":3},"cited_work":{"arxiv_id":"2207.05955","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.05955","snapshot_observed_at":"2026-07-03T07:57:44.208058Z","title":"Yao and X.-H","venue":null,"work_id":"0b254e5a-355a-4a8b-9d96-e5802b466f35","year":2023},"citing_paper":{"arxiv_id":"2606.06495","last_updated":"2026-06-04T17:59:59Z","snapshot_observed_at":"2026-08-08T14:37:47.002746Z","submitted_at":"2026-06-04T17:59:59Z","title":"What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-06-27T23:47:15.644279Z"},"links":{"cited_paper":"/paper/2207.05955","citing_paper":"/paper/2606.06495"},"observation_digest":"sha256:beeda1d7890601d906081603490dd2ab46bafaa9d77b76c6ce8feeee29b66374","observation_id":"c39e76a5-d669-4de9-bc0b-5015885f480e","resolution":{"observed_at":"2026-07-02T15:37:06.545947Z","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":"2207.05955","last_updated":"2024-05-30T07:58:59Z","snapshot_observed_at":"2026-08-13T15:05:14.357879Z","submitted_at":"2022-07-13T04:15:51Z","title":"Can interacting dark energy with dynamical coupling resolve the Hubble tension","version":3},"cited_work":{"arxiv_id":"2207.05955","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.05955","snapshot_observed_at":"2026-07-03T07:57:44.208058Z","title":"Yao and X.-H","venue":null,"work_id":"0b254e5a-355a-4a8b-9d96-e5802b466f35","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":71,"source":"pdf_text","source_observed_at":"2026-06-27T11:43:20.857862Z"},"links":{"cited_paper":"/paper/2207.05955","citing_paper":"/paper/2606.11368"},"observation_digest":"sha256:32113457e5fcdd35b707a77b74aa1f3ab1ab2c838c0869cb06dd57775de40352","observation_id":"0aa84d7a-e104-4a0c-b0ae-b9f7f2b9d4a9","resolution":{"observed_at":"2026-07-03T07:57:44.209713Z","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":"2207.05955","last_updated":"2024-05-30T07:58:59Z","snapshot_observed_at":"2026-08-13T15:05:14.357879Z","submitted_at":"2022-07-13T04:15:51Z","title":"Can interacting dark energy with dynamical coupling resolve the Hubble tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.05955","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Yao and X.-H","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2207.05955","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:30c4b635968a735b11cf34a183c888e758ab31a96a79e49e0349fecf73fc6b0b","observation_id":"2a229e3b-70c3-4664-b78a-6bd38701fc10","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.05955","last_updated":"2024-05-30T07:58:59Z","snapshot_observed_at":"2026-08-13T15:05:14.357879Z","submitted_at":"2022-07-13T04:15:51Z","title":"Can interacting dark energy with dynamical coupling resolve the Hubble tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.05955","snapshot_observed_at":"2026-08-01T02:46:22.867328Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.26101","last_updated":"2026-07-28T06:59:44Z","snapshot_observed_at":"2026-08-12T16:58:48.467477Z","submitted_at":"2026-07-28T06:59:44Z","title":"Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-01T02:46:22.867328Z"},"links":{"cited_paper":"/paper/2207.05955","citing_paper":"/paper/2607.26101"},"observation_digest":"sha256:316787080afc03b5fb1dcb62a15467a0a1f58623b51828235c764497fa434976","observation_id":"239321f4-39b2-47f6-973a-b4b4decc5b0f","resolution":{"observed_at":"2026-08-01T02:46:22.867328Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2207.05955/citation-record","integrity":"/paper/2207.05955/integrity","json":"/paper/2207.05955/citation-record.json","paper":"/paper/2207.05955"},"outbound":[],"paper":{"arxiv_id":"2207.05955","last_updated":"2024-05-30T07:58:59Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-13T15:05:14.357879Z","submitted_at":"2022-07-13T04:15:51Z","title":"Can interacting dark energy with dynamical coupling resolve the Hubble 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 11 inbound Pith citation observations for arXiv:2207.05955."}