{"as_of":"2026-08-15T05:02:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:72b3b84cf28de9c124b8d34d9b53814fe2fd466d0bb1fd9946811f12a639468c","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":"2026-08-14T06:32:32.682623+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":"2026-08-13T21:07:15.374582Z","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":"sha256:0d401878f53a48957986d1c9c36ee327eb40c630b12f2d06b18ecf3275627b1f","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":"2026-08-13T21:07:15.374582Z","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":"2026-08-14T00:44:55.106734Z","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":"sha256:1d9488565446ed1df1a5368206d49a364a785d0efd39dd1ac41a3acc7aa9ec84","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":"2026-08-13T21:07:15.374582Z","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":"sha256:0c12fd2e1ae971f2d5dfc90c2ec804ab572a93326a77a4409f6cf72d51235a1f","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":"2026-08-13T21:07:15.374582Z","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":"sha256:23788b436c5cd71422dc62e743cb54b5340d64a363c32e146ee20e66de462d13","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":"2026-08-13T21:07:15.374582Z","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:bc0ec185337d9caedb177cc64a195cb4f236162a3bb15a692a209d3bc3f31739","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":"2026-08-13T21:07:15.374582Z","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:a742b70775f459dea95cebe1d93bb003aa9571ea1f94a6d1f568b1cc0191c938","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 2026-08-14T06:32:32.682623+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":"2207.05955","last_updated":"2024-05-30T07:58:59Z","snapshot_observed_at":"2026-08-13T21:07:15.374582Z","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:eecd77293e8040802f60c59775f539050456e91243d3ff65d60a3dec538880ab","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 2026-08-14T06:32:32.682623+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":"2207.05955","last_updated":"2024-05-30T07:58:59Z","snapshot_observed_at":"2026-08-13T21:07:15.374582Z","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":"2026-08-13T23:27:08.774753Z","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":"sha256:8382ec105c2f51084cad0650bba142d90f9062ac06710e44f3c3dd1ef23752c3","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 2026-08-14T06:32:32.682623+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":"2207.05955","last_updated":"2024-05-30T07:58:59Z","snapshot_observed_at":"2026-08-13T21:07:15.374582Z","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":"sha256:6420affd3be144984093669cf7d425529afb0c52967852c7f1b9fc52002533ac","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 2026-08-14T06:32:32.682623+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":"2207.05955","last_updated":"2024-05-30T07:58:59Z","snapshot_observed_at":"2026-08-13T21:07:15.374582Z","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":"sha256:4909947d90385b632e6ac127bbf89a9ddf0af8758bdee8e3d7e24551938e6e9e","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":"2026-08-13T21:07:15.374582Z","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":"2026-08-14T18:52:26.745814Z","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:b94a53a4a7b282bbeadf7798986ac562a5e307ecb48efb9086328b640e6bd5a6","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":"2026-08-13T21:07:15.374582Z","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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2207.05955."}