{"as_of":"2026-08-15T03:14:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:43347303d7dbe4a3d8d95d637c85b0643e69c6de096ed002ec9d022251c20670","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":"2026-08-14T06:32:32.682623+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":"2026-08-14T15:21:27.728044Z","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":"2026-06-30T20:15:05.424906Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1710.09366","last_updated":"2019-08-20T18:49:02Z","snapshot_observed_at":"2026-08-14T20:20:19.142456Z","submitted_at":"2017-10-25T17:53:28Z","title":"$H_0$ tension as a hint for a transition in gravitational theory","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.09366","snapshot_observed_at":"2026-08-14T15:21:27.728044Z","title":"Khosravi, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.01391","last_updated":"2019-12-01T12:03:17Z","snapshot_observed_at":"2026-08-14T17:42:34.108580Z","submitted_at":"2019-08-04T19:35:10Z","title":"Cosmological constraints in extended parameter space from the Planck 2018 Legacy release","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T15:21:27.728044Z"},"links":{"cited_paper":"/paper/1710.09366","citing_paper":"/paper/1908.01391"},"observation_digest":"sha256:b31629d0ce4aa576bb6057bd177f1e7674a18e372907965dccc4d4d02d2aadd7","observation_id":"2b15aa2e-c801-4d38-a65a-19a34612875e","resolution":{"observed_at":"2026-08-14T15:21:27.728044Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.09366","last_updated":"2019-08-20T18:49:02Z","snapshot_observed_at":"2026-08-14T20:20:19.142456Z","submitted_at":"2017-10-25T17:53:28Z","title":"$H_0$ tension as a hint for a transition in gravitational theory","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.09366","snapshot_observed_at":"2026-08-14T14:24:14.528369Z","title":"Khosravi, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03324","last_updated":"2020-09-24T15:12:03Z","snapshot_observed_at":"2026-08-14T15:35:16.927409Z","submitted_at":"2019-08-09T06:00:26Z","title":"Resolving Hubble Tension with Quintom Dark Energy Model","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T14:24:14.528369Z"},"links":{"cited_paper":"/paper/1710.09366","citing_paper":"/paper/1908.03324"},"observation_digest":"sha256:cdad09599d77c8166a6a54ea121c9be81bdd6e7b8659eed326a7844787014a13","observation_id":"99dd6aa8-4ce5-4286-a904-f3a4067e495e","resolution":{"observed_at":"2026-08-14T14:24:14.528369Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.09366","last_updated":"2019-08-20T18:49:02Z","snapshot_observed_at":"2026-08-14T20:20:19.142456Z","submitted_at":"2017-10-25T17:53:28Z","title":"$H_0$ tension as a hint for a transition in gravitational theory","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.09366","snapshot_observed_at":"2026-08-14T13:51:08.370305Z","title":"Khosravi, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.04281","last_updated":"2020-07-01T09:13:30Z","snapshot_observed_at":"2026-08-14T21:44:35.303861Z","submitted_at":"2019-08-12T17:48:35Z","title":"Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T13:51:08.370305Z"},"links":{"cited_paper":"/paper/1710.09366","citing_paper":"/paper/1908.04281"},"observation_digest":"sha256:de701131601e205729ae33d8eadc0846c7ebe05755af8d62d2cbe4b7eca49b61","observation_id":"01f31f19-cd87-4b54-855a-33989a96162b","resolution":{"observed_at":"2026-08-14T13:51:08.370305Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.09366","last_updated":"2019-08-20T18:49:02Z","snapshot_observed_at":"2026-08-14T20:20:19.142456Z","submitted_at":"2017-10-25T17:53:28Z","title":"$H_0$ tension as a hint for a transition in gravitational theory","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.09366","snapshot_observed_at":"2026-08-14T11:06:35.339568Z","title":"H0 tension as a hint for a tran- sition in gravitational theory,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.09843","last_updated":"2021-01-10T05:49:45Z","snapshot_observed_at":"2026-08-14T17:27:35.816206Z","submitted_at":"2019-08-26T18:00:03Z","title":"Dark Neutrino interactions phase out the Hubble tension","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T11:06:35.339568Z"},"links":{"cited_paper":"/paper/1710.09366","citing_paper":"/paper/1908.09843"},"observation_digest":"sha256:472b736c7e6a9dcc6f51eb19dc9822c53503ae82811ccbccfd0d900acbb8f92b","observation_id":"ad60c311-a851-472d-be09-b1f4bd989fe1","resolution":{"observed_at":"2026-08-14T11:06:35.339568Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.09366","last_updated":"2019-08-20T18:49:02Z","snapshot_observed_at":"2026-08-14T20:20:19.142456Z","submitted_at":"2017-10-25T17:53:28Z","title":"$H_0$ tension as a hint for a transition in gravitational theory","version":4},"cited_work":{"arxiv_id":"1710.09366","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1710.09366","snapshot_observed_at":"2026-06-30T20:15:05.424906Z","title":"Khosravi, S","venue":null,"work_id":"0c0609ff-7357-4eed-8e0c-666e23f44d99","year":2019},"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":47,"source":"pdf_text","source_observed_at":"2026-06-30T20:07:39.265059Z"},"links":{"cited_paper":"/paper/1710.09366","citing_paper":"/paper/2605.14977"},"observation_digest":"sha256:519a6e1c2b70bd17124f78ff7307c7899ee1cb1b598a89eca41f3d27f46029fb","observation_id":"88a4116e-386a-4d93-a2ff-753847673cb4","resolution":{"observed_at":"2026-06-30T20:15:05.426874Z","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":"1710.09366","last_updated":"2019-08-20T18:49:02Z","snapshot_observed_at":"2026-08-14T20:20:19.142456Z","submitted_at":"2017-10-25T17:53:28Z","title":"$H_0$ tension as a hint for a transition in gravitational theory","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.09366","snapshot_observed_at":"2026-08-01T02:46:22.909741Z","title":"Khosravi, S","venue":null,"work_id":null,"year":2019},"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":51,"source":"pdf_text","source_observed_at":"2026-08-01T02:46:22.909741Z"},"links":{"cited_paper":"/paper/1710.09366","citing_paper":"/paper/2607.26101"},"observation_digest":"sha256:e103709fbe8aaed9ad7906f403758b3959685e13c601d7e97a10f25f385a5a1d","observation_id":"25688ad0-d199-4b2f-ad25-4b34442de44e","resolution":{"observed_at":"2026-08-01T02:46:22.909741Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1710.09366/citation-record","integrity":"/paper/1710.09366/integrity","json":"/paper/1710.09366/citation-record.json","paper":"/paper/1710.09366"},"outbound":[],"paper":{"arxiv_id":"1710.09366","last_updated":"2019-08-20T18:49:02Z","latest_version":4,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T20:20:19.142456Z","submitted_at":"2017-10-25T17:53:28Z","title":"$H_0$ tension as a hint for a transition in gravitational theory"},"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 6 inbound Pith citation observations for arXiv:1710.09366."}