{"as_of":"2026-08-12T09:32:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ae005d086a367c770a55547c3930f1424e99f330fd28940497f9362df372b52a","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":19,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":19,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":19,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":19,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T04:57:06.739292Z","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":"2026-07-04T14:19:54.788341Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":"2309.07795","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-07-04T14:19:54.788341Z","title":"G´ omez-Valent, A","venue":null,"work_id":"bd4bea36-c205-4797-b95c-683945496b3d","year":2024},"citing_paper":{"arxiv_id":"2402.07716","last_updated":"2026-04-28T16:55:09Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-02-12T15:29:10Z","title":"$\\Lambda_{\\rm s}$CDM cosmology from a type-II minimally modified gravity","version":3},"reference_index":114,"source":"pdf_text","source_observed_at":"2026-05-24T03:50:50.435997Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2402.07716"},"observation_digest":"sha256:9bfb110d80ccff86d4be3f1d759c642baa68aebf36e811b1dc7c198b9bbe4c01","observation_id":"d1c8452f-cbf9-4c78-b77d-3e33e870709a","resolution":{"observed_at":"2026-05-24T03:53:54.590232Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-08-12T04:57:06.739292Z","title":"Gómez-Valent, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.00931","last_updated":"2025-02-15T06:07:09Z","snapshot_observed_at":"2026-08-12T04:49:14.768938Z","submitted_at":"2024-12-01T18:41:32Z","title":"Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-12T04:57:06.739292Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2412.00931"},"observation_digest":"sha256:eb157642d9df5b7900c46a878299d16da3098adba61ef395d41095d1e2a42730","observation_id":"743a822a-2239-43e9-b0b3-28ad954831d2","resolution":{"observed_at":"2026-08-12T04:57:06.739292Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-08-11T11:44:52.605101Z","title":"Late-time phenomenology re- quired to solve the H0 tension in view of the cosmic ladders and the anisotropic and angular BAO datasets,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.15124","last_updated":"2025-03-10T16:54:24Z","snapshot_observed_at":"2026-08-11T17:17:42.978165Z","submitted_at":"2024-12-19T18:03:19Z","title":"Composite Dark Energy and the Cosmological Tensions","version":3},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-11T11:44:52.605101Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2412.15124"},"observation_digest":"sha256:55ef735a8a1207b489d8e07c7262122412a4b36dcce79ae9c5bca7eae7af7885","observation_id":"09c881c6-73c2-4a86-bc68-202eaa9dc3a1","resolution":{"observed_at":"2026-08-11T11:44:52.605101Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-08-10T18:12:34.913494Z","title":"Gómez-Valent, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.11571","last_updated":"2025-06-17T07:05:51Z","snapshot_observed_at":"2026-08-10T20:17:39.475166Z","submitted_at":"2025-01-20T16:20:59Z","title":"Illustrating the consequences of a misuse of $\\sigma_8$ in cosmology","version":2},"reference_index":254,"source":"pdf_text","source_observed_at":"2026-08-10T18:12:34.913494Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2501.11571"},"observation_digest":"sha256:08205704c8724b1d42d71b042ed46a0f57f5e564e95c2c07a7aa3e614398905c","observation_id":"66c64e51-0fde-4633-8501-9626610bb0b2","resolution":{"observed_at":"2026-08-10T18:12:34.913494Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-08-10T05:59:55.408094Z","title":"G´ omez-Valent, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.16883","last_updated":"2025-05-01T04:08:13Z","snapshot_observed_at":"2026-08-10T12:08:50.413654Z","submitted_at":"2025-01-28T12:12:12Z","title":"Can the sound horizon-free measurement of $H_0$ constrain early new physics?","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-10T05:59:55.408094Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2501.16883"},"observation_digest":"sha256:429436d360deaa4a7ffd7e5d46f169426c81e9298ef356a01badfe9e2145d395","observation_id":"8bd40c86-5441-4455-b1b2-a283b393b4d9","resolution":{"observed_at":"2026-08-10T05:59:55.408094Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":"2309.07795","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-07-04T14:19:54.788341Z","title":"G´ omez-Valent, A","venue":null,"work_id":"bd4bea36-c205-4797-b95c-683945496b3d","year":2024},"citing_paper":{"arxiv_id":"2510.18741","last_updated":"2026-04-10T13:03:33Z","snapshot_observed_at":"2026-08-11T01:15:58.758365Z","submitted_at":"2025-10-21T15:46:25Z","title":"Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\\Lambda_{\\rm s}$CDM versus $\\Lambda$CDM","version":2},"reference_index":185,"source":"pdf_text","source_observed_at":"2026-05-18T04:46:14.832965Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2510.18741"},"observation_digest":"sha256:8f28e73d35e3f50135c4e6baae25e4365353e6429e1d81a0a902fc0045284853","observation_id":"2b053aea-3f3b-47dd-b3a0-71d0f0d67c08","resolution":{"observed_at":"2026-05-18T04:50:54.960960Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-08-03T11:53:06.032393Z","title":"G´ omez-Valent, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2601.05218","last_updated":"2026-06-14T12:30:47Z","snapshot_observed_at":"2026-08-07T11:51:09.807257Z","submitted_at":"2026-01-08T18:43:36Z","title":"Towards a unified quantum field theory of dark energy and inflation: unstable de Sitter vacuum and running vacuum","version":3},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-03T11:53:06.032393Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2601.05218"},"observation_digest":"sha256:f4503c5c44e6d2424824b87c71d3d8153b7ab4015325d998b2516720b86cc2c9","observation_id":"727f8e1f-f2b5-4084-9506-0e577c1a704b","resolution":{"observed_at":"2026-08-03T11:53:06.032393Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":"2309.07795","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-07-04T14:19:54.788341Z","title":"G´ omez-Valent, A","venue":null,"work_id":"bd4bea36-c205-4797-b95c-683945496b3d","year":2024},"citing_paper":{"arxiv_id":"2602.11936","last_updated":"2026-08-10T08:18:00Z","snapshot_observed_at":"2026-08-12T09:16:28.425738Z","submitted_at":"2026-02-12T13:35:54Z","title":"Probing dynamical dark energy with late-time data: Evidence, tensions, and the limits of the $w_0w_a$CDM framework","version":3},"reference_index":135,"source":"pdf_text","source_observed_at":"2026-05-21T13:29:05.147292Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2602.11936"},"observation_digest":"sha256:e71fa2cef57ee786ab0dcdb2affc049305c8a52ae048c90e0fa8143345fb55e2","observation_id":"7b4ce396-035f-4d58-bf2b-34c5210f64e7","resolution":{"observed_at":"2026-05-21T13:30:12.579820Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-07-15T12:01:04.317365Z","title":"G´ omez-Valent, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.14693","last_updated":"2026-07-14T04:50:03Z","snapshot_observed_at":"2026-08-10T07:05:44.565362Z","submitted_at":"2026-03-16T01:02:08Z","title":"Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families","version":2},"reference_index":147,"source":"pdf_text","source_observed_at":"2026-07-15T12:01:04.317365Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2603.14693"},"observation_digest":"sha256:7e68fffeb27ca4e2eb328b7e567ba6ffa24b95d33d7dfdc0ac60ea6eddd4d34d","observation_id":"07ad128a-dd7f-4e4e-8d3a-5a82833c1f9f","resolution":{"observed_at":"2026-07-15T12:01:04.317365Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":"2309.07795","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-07-04T14:19:54.788341Z","title":"G´ omez-Valent, A","venue":null,"work_id":"bd4bea36-c205-4797-b95c-683945496b3d","year":2024},"citing_paper":{"arxiv_id":"2603.26560","last_updated":"2026-05-26T09:42:59Z","snapshot_observed_at":"2026-07-13T17:26:51.495350Z","submitted_at":"2026-03-27T16:25:41Z","title":"Exploring the interplay of late-time dynamical dark energy and new physics before recombination","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-05-14T23:13:02.830649Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2603.26560"},"observation_digest":"sha256:a91353288641c7e6ecd3a3345a70af139defd0fc09700eeb5a74d89e7fdf3823","observation_id":"66da1f4a-59cd-4e99-9e4a-dce1e8b8396e","resolution":{"observed_at":"2026-05-14T23:13:14.722633Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":"2309.07795","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-07-04T14:19:54.788341Z","title":"G´ omez-Valent, A","venue":null,"work_id":"bd4bea36-c205-4797-b95c-683945496b3d","year":2024},"citing_paper":{"arxiv_id":"2604.13535","last_updated":"2026-04-15T06:29:12Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-15T06:29:12Z","title":"Double the axions, half the tension: multi-field early dark energy eases the Hubble tension","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-05-10T12:56:21.466420Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2604.13535"},"observation_digest":"sha256:069f2051448ee376db8c10d62cb8a5ff44dc08909583eddc6a5cf566531059da","observation_id":"2e03751c-9cf4-4f85-95b3-77e2af90cf52","resolution":{"observed_at":"2026-05-11T11:36:03.555603Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":"2309.07795","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-07-04T14:19:54.788341Z","title":"G´ omez-Valent, A","venue":null,"work_id":"bd4bea36-c205-4797-b95c-683945496b3d","year":2024},"citing_paper":{"arxiv_id":"2604.25813","last_updated":"2026-04-28T16:22:13Z","snapshot_observed_at":"2026-08-11T17:31:33.518155Z","submitted_at":"2026-04-28T16:22:13Z","title":"Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-05-07T14:55:55.250283Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2604.25813"},"observation_digest":"sha256:b69ea6f9b908d148501d989052aa1c5a67754c6f86f2f7664f1f3db4146e66c7","observation_id":"15930d2c-f605-47b1-99c3-e8e525d6b2fd","resolution":{"observed_at":"2026-05-12T00:36:16.390548Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":"2309.07795","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-07-04T14:19:54.788341Z","title":"G´ omez-Valent, A","venue":null,"work_id":"bd4bea36-c205-4797-b95c-683945496b3d","year":2024},"citing_paper":{"arxiv_id":"2605.26050","last_updated":"2026-05-25T17:12:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-25T17:12:16Z","title":"Early- and Late-Time Modifications to $\\Lambda$CDM: Implications for the Hubble Tension","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-06-29T20:29:06.417337Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2605.26050"},"observation_digest":"sha256:82854702e0219ac040b91dd4c1dcae0693584591745baf8fc002059a942e9c74","observation_id":"8aa42d47-9bba-48f3-a41e-5a41306a934b","resolution":{"observed_at":"2026-06-30T00:14:05.197507Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":"2309.07795","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-07-04T14:19:54.788341Z","title":"G´ omez-Valent, A","venue":null,"work_id":"bd4bea36-c205-4797-b95c-683945496b3d","year":2024},"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":78,"source":"pdf_text","source_observed_at":"2026-06-27T23:47:15.644279Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2606.06495"},"observation_digest":"sha256:696b796af804cd386820beb27a69ecef7e71911ca8d0f4a2179f6de390682f30","observation_id":"6af31aba-e4d2-4620-8acd-7b4777710848","resolution":{"observed_at":"2026-07-02T15:37:06.341480Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":"2309.07795","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-07-04T14:19:54.788341Z","title":"G´ omez-Valent, A","venue":null,"work_id":"bd4bea36-c205-4797-b95c-683945496b3d","year":2024},"citing_paper":{"arxiv_id":"2606.12822","last_updated":"2026-06-11T02:35:35Z","snapshot_observed_at":"2026-07-06T23:51:40.528967Z","submitted_at":"2026-06-11T02:35:35Z","title":"Geometric obstruction to resolving the Hubble tension: orthogonality of scale and shape in distance measurements","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-06-27T06:23:50.957273Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2606.12822"},"observation_digest":"sha256:57539f0da0880560aa714e39f551535f58d8cad9133f68ba891bd34af3e60cf6","observation_id":"0ea1f0e3-31de-4f1c-98cc-6dc634fab875","resolution":{"observed_at":"2026-07-03T15:38:33.958155Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":"2309.07795","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-07-04T14:19:54.788341Z","title":"G´ omez-Valent, A","venue":null,"work_id":"bd4bea36-c205-4797-b95c-683945496b3d","year":2024},"citing_paper":{"arxiv_id":"2606.27173","last_updated":"2026-06-25T15:41:19Z","snapshot_observed_at":"2026-07-07T00:01:24.919835Z","submitted_at":"2026-06-25T15:41:19Z","title":"Redshift-Dependent Intrinsic Dispersion in the Quasar UV/X-ray Luminosity Relation","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-06-26T03:57:10.956237Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2606.27173"},"observation_digest":"sha256:309dfa75ac80910d285a6ab4517e735de3ab48692d848fb5805176d62e07fa01","observation_id":"c5c0b839-82bd-445c-a101-3c71658f287a","resolution":{"observed_at":"2026-07-04T14:19:54.789622Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":"2309.07795","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-07-04T14:19:54.788341Z","title":"G´ omez-Valent, A","venue":null,"work_id":"bd4bea36-c205-4797-b95c-683945496b3d","year":2024},"citing_paper":{"arxiv_id":"2606.31362","last_updated":"2026-06-30T08:57:18Z","snapshot_observed_at":"2026-08-09T03:11:42.668077Z","submitted_at":"2026-06-30T08:57:18Z","title":"Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension","version":1},"reference_index":211,"source":"pdf_text","source_observed_at":"2026-07-01T04:31:47.886338Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2606.31362"},"observation_digest":"sha256:028401ac6ae334b76ef0ce8a0c02e066755b5e6303cc1e0507674e37e76c1fa4","observation_id":"eb2d408e-8d1f-4ef1-b0da-a7ff3212bafc","resolution":{"observed_at":"2026-07-01T11:25:45.626815Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-07-11T09:40:49.196932Z","title":"Gómez-Valent, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.05044","last_updated":"2026-07-06T13:21:04Z","snapshot_observed_at":"2026-08-06T06:21:38.078437Z","submitted_at":"2026-07-06T13:21:04Z","title":"Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus","version":1},"reference_index":125,"source":"pdf_text","source_observed_at":"2026-07-11T09:40:49.196932Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2607.05044"},"observation_digest":"sha256:e5bb290843acb5377d3af73132fe02543fdb59c531bb479c4cc1c7444c1a335a","observation_id":"e1b9b377-642f-4937-b876-6f987f76080a","resolution":{"observed_at":"2026-07-11T09:40:49.196932Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.07795","snapshot_observed_at":"2026-08-01T08:08:46.209758Z","title":"G´ omez-Valent, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.21244","last_updated":"2026-07-23T12:08:39Z","snapshot_observed_at":"2026-08-08T21:46:06.090866Z","submitted_at":"2026-07-23T12:08:39Z","title":"Hubble tension: the shape wall","version":1},"reference_index":133,"source":"pdf_text","source_observed_at":"2026-08-01T08:08:46.209758Z"},"links":{"cited_paper":"/paper/2309.07795","citing_paper":"/paper/2607.21244"},"observation_digest":"sha256:6944223c6b7d0a6d962f4430e897932d4fa7df53a25c05453f37246aa7df854e","observation_id":"cde66b08-3737-4b49-a155-3dd59ed28b68","resolution":{"observed_at":"2026-08-01T08:08:46.209758Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2309.07795/citation-record","integrity":"/paper/2309.07795/integrity","json":"/paper/2309.07795/citation-record.json","paper":"/paper/2309.07795"},"outbound":[],"paper":{"arxiv_id":"2309.07795","last_updated":"2023-12-21T10:17:11Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T16:18:33.331149Z","submitted_at":"2023-09-14T15:32:51Z","title":"Late-time phenomenology required to solve the $H_0$ tension in view of the cosmic ladders and the anisotropic and angular BAO data sets"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 19 inbound Pith citation observations for arXiv:2309.07795."}