{"as_of":"2026-08-09T03:16:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:cd3b0d86115cc2cd20f7f5e963145650c01d3d2ddcd3b637d3fa5f203660b88c","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":20,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":20,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":20,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":20,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T21:15:08.514767Z","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":"2026-07-04T02:19:23.624008Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":"2301.06097","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-07-04T02:19:23.624008Z","title":"Bernui, E","venue":null,"work_id":"a9bc7810-f0cd-491b-8900-f01489621b93","year":2023},"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":136,"source":"pdf_text","source_observed_at":"2026-05-24T03:50:50.435997Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2402.07716"},"observation_digest":"sha256:63998de93bb2c0070e67a5f2538be225a5a90e8534e0126a074e910f214c4c9c","observation_id":"cab0717f-1592-4390-ac90-50970bb78282","resolution":{"observed_at":"2026-05-24T03:53:54.471388Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-08-06T21:15:08.514767Z","title":", author Di Valentino , E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.00779","last_updated":"2025-07-01T14:19:03Z","snapshot_observed_at":"2026-08-07T19:08:25.815510Z","submitted_at":"2025-07-01T14:19:03Z","title":"Is $\\omega_0 \\omega_a$CDM a good model for the clumpy Universe?","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-06T21:15:08.514767Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2507.00779"},"observation_digest":"sha256:9ab12f66b2733100a56c55366c0dec7aeb4650b8b360f1317ef5f3d32e2b77b8","observation_id":"1dfcf052-823e-417c-a7f7-fe47019ea744","resolution":{"observed_at":"2026-08-06T21:15:08.514767Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-08-06T05:29:01.353564Z","title":"Bernui, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:01.353564Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:f12743d9b116fa589ad159e4e9ae967a6198b00902a43bb546ad475131351ca8","observation_id":"c3d0989d-07b8-4c2b-bab8-8c1158ab1214","resolution":{"observed_at":"2026-08-06T05:29:01.353564Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-08-04T12:53:45.932175Z","title":"Bernui, E","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":159,"source":"pdf_text","source_observed_at":"2026-08-04T12:53:45.932175Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2510.01974"},"observation_digest":"sha256:0d1e8d2a72b1d1be5628afc85f0c597bb934b4333fbec2e24f9ff710617ccfd1","observation_id":"9d01db31-1bbc-49ba-80e5-e99f078d8896","resolution":{"observed_at":"2026-08-04T12:53:45.932175Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-08-04T09:25:48.495161Z","title":"Bernui, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2510.15650","last_updated":"2026-07-31T16:49:28Z","snapshot_observed_at":"2026-08-08T10:21:06.620126Z","submitted_at":"2025-10-17T13:41:45Z","title":"High-redshift transverse BAO measurements with the SDSS quasar catalog","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-04T09:25:48.495161Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2510.15650"},"observation_digest":"sha256:58eb0de0085daa18d0411459bd0d1bd6cb1049f2189985bbbba0222b804f3e04","observation_id":"cc6d701d-ff8d-4992-8f52-1f347d61f6bc","resolution":{"observed_at":"2026-08-04T09:25:48.495161Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":"2301.06097","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-07-04T02:19:23.624008Z","title":"Bernui, E","venue":null,"work_id":"a9bc7810-f0cd-491b-8900-f01489621b93","year":2023},"citing_paper":{"arxiv_id":"2510.18741","last_updated":"2026-04-10T13:03:33Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","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":93,"source":"pdf_text","source_observed_at":"2026-05-18T04:46:14.832965Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2510.18741"},"observation_digest":"sha256:5eaedd8c0e8140df752c393d4f92dfd90f87281230ca72b14484daee8ca332f4","observation_id":"13bd6c89-71d0-4694-b154-845429370cce","resolution":{"observed_at":"2026-05-18T04:50:55.061924Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":"2301.06097","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-07-04T02:19:23.624008Z","title":"Bernui, E","venue":null,"work_id":"a9bc7810-f0cd-491b-8900-f01489621b93","year":2023},"citing_paper":{"arxiv_id":"2511.16244","last_updated":"2026-04-27T06:56:08Z","snapshot_observed_at":"2026-08-03T21:51:02.344479Z","submitted_at":"2025-11-20T11:24:10Z","title":"Constraining interacting dark energy models with black hole superradiance","version":3},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-17T21:08:20.630611Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2511.16244"},"observation_digest":"sha256:b248172b41409fc839bd5d929c65578592d5b115438886c94de09fb6dadf37ae","observation_id":"df62826f-4494-4784-ac25-2c0a21d32a09","resolution":{"observed_at":"2026-05-17T21:10:16.866491Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-08-03T11:41:15.314976Z","title":"Bernui, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2601.05646","last_updated":"2026-06-25T07:04:53Z","snapshot_observed_at":"2026-08-03T11:41:11.085957Z","submitted_at":"2026-01-09T09:06:09Z","title":"A microphysically inspired approach to dark matter-dark energy interactions: first bounds on dark-sector scattering cross sections","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-03T11:41:15.314976Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2601.05646"},"observation_digest":"sha256:f5c36652c7e26911f9dca066e46afa69fa3a138f1d103331b44962ce5b8f7a55","observation_id":"a2f1ccf7-bb0c-414f-9dbb-0296e4f7dc1b","resolution":{"observed_at":"2026-08-03T11:41:15.314976Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":"2301.06097","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-07-04T02:19:23.624008Z","title":"Bernui, E","venue":null,"work_id":"a9bc7810-f0cd-491b-8900-f01489621b93","year":2023},"citing_paper":{"arxiv_id":"2601.14222","last_updated":"2026-04-27T15:45:53Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-01-20T18:32:34Z","title":"Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-05-16T12:15:01.997389Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2601.14222"},"observation_digest":"sha256:9730f5aa9e2ea89bdeeb4628160ffdb193c757ed456fcf11a84da36a0c6ea86d","observation_id":"f7ccce8a-6fa4-448e-b847-cf2c47192772","resolution":{"observed_at":"2026-05-16T12:17:52.220710Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":"2301.06097","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-07-04T02:19:23.624008Z","title":"Bernui, E","venue":null,"work_id":"a9bc7810-f0cd-491b-8900-f01489621b93","year":2023},"citing_paper":{"arxiv_id":"2602.11936","last_updated":"2026-05-18T12:54:32Z","snapshot_observed_at":"2026-08-02T13:51:44.487752Z","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":64,"source":"pdf_text","source_observed_at":"2026-05-21T13:29:05.147292Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2602.11936"},"observation_digest":"sha256:eb905f22d45a087fe377bd616a7b89d1da782fce98258d7d5db18597a4b5f296","observation_id":"8b9c187d-bcb0-4dc2-aef5-8d90904d1d2e","resolution":{"observed_at":"2026-05-21T13:30:11.962169Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-07-15T12:01:04.317365Z","title":"Bernui, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2603.14693","last_updated":"2026-07-14T04:50:03Z","snapshot_observed_at":"2026-08-06T08:35:01.524662Z","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":73,"source":"pdf_text","source_observed_at":"2026-07-15T12:01:04.317365Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2603.14693"},"observation_digest":"sha256:e907ee26a6f3f550bc64bb8fd54a89b831453238625d248d1179e167a92ba637","observation_id":"76c46cba-1554-49f7-93b8-4d47f0c97a5b","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":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":"2301.06097","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-07-04T02:19:23.624008Z","title":"Bernui, E","venue":null,"work_id":"a9bc7810-f0cd-491b-8900-f01489621b93","year":2023},"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":154,"source":"pdf_text","source_observed_at":"2026-05-14T23:13:02.830649Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2603.26560"},"observation_digest":"sha256:55d36d0a6fcb6ba9583af6579459895f83d0bfade530bb0fe957e7446ca370c7","observation_id":"d0d5eb76-f999-40f2-b8d9-79a2ccc4ce29","resolution":{"observed_at":"2026-05-14T23:13:14.796343Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":"2301.06097","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-07-04T02:19:23.624008Z","title":"Bernui, E","venue":null,"work_id":"a9bc7810-f0cd-491b-8900-f01489621b93","year":2023},"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":58,"source":"pdf_text","source_observed_at":"2026-05-10T12:56:21.466420Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2604.13535"},"observation_digest":"sha256:78f30c3434562d8fe61ad014dc85f49345601efbc64a4bb358523d055a76dc2f","observation_id":"aa1e5141-74db-48bf-a004-7807ebd7d288","resolution":{"observed_at":"2026-05-11T11:36:03.734613Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":"2301.06097","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-07-04T02:19:23.624008Z","title":"Bernui, E","venue":null,"work_id":"a9bc7810-f0cd-491b-8900-f01489621b93","year":2023},"citing_paper":{"arxiv_id":"2604.25813","last_updated":"2026-04-28T16:22:13Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-28T16:22:13Z","title":"Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-05-07T14:55:55.250283Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2604.25813"},"observation_digest":"sha256:70f7d412352811cdff7ab6d4dc2b40a7654f10891fa2bb53e8155e4f7df8e59a","observation_id":"66d13f9b-037d-4f77-8c79-0b8e7ca76166","resolution":{"observed_at":"2026-05-12T00:36:16.285973Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":"2301.06097","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-07-04T02:19:23.624008Z","title":"Bernui, E","venue":null,"work_id":"a9bc7810-f0cd-491b-8900-f01489621b93","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":187,"source":"pdf_text","source_observed_at":"2026-06-29T20:17:08.107860Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2605.26116"},"observation_digest":"sha256:8813f9eea381d2b70af5948cfb3b2e3972cee384dc24ed24f7e2c79a2da5c69e","observation_id":"955f2436-1c04-47b3-9eb7-0b6c786ea288","resolution":{"observed_at":"2026-07-01T16:35:50.565459Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":"2301.06097","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-07-04T02:19:23.624008Z","title":"Bernui, E","venue":null,"work_id":"a9bc7810-f0cd-491b-8900-f01489621b93","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":61,"source":"pdf_text","source_observed_at":"2026-06-27T23:47:15.644279Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2606.06495"},"observation_digest":"sha256:a55595e7adf9fa4b40a9d95c87ce6ee2c9d45056f2328e7a0e631b489bc3ff15","observation_id":"5ef85a24-746e-416b-a5da-0411f4431452","resolution":{"observed_at":"2026-07-02T15:37:06.426119Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":"2301.06097","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-07-04T02:19:23.624008Z","title":"Bernui, E","venue":null,"work_id":"a9bc7810-f0cd-491b-8900-f01489621b93","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":57,"source":"pdf_text","source_observed_at":"2026-06-27T11:43:20.857862Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2606.11368"},"observation_digest":"sha256:0eb903a65664384bc24ebf9febae2a5e39d8248bbf011d428a84f3f8b192930f","observation_id":"fc3a5a10-cb4d-4375-b744-a14e2d03849c","resolution":{"observed_at":"2026-07-03T07:47:45.242759Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":"2301.06097","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-07-04T02:19:23.624008Z","title":"Bernui, E","venue":null,"work_id":"a9bc7810-f0cd-491b-8900-f01489621b93","year":2023},"citing_paper":{"arxiv_id":"2606.19090","last_updated":"2026-06-17T13:58:39Z","snapshot_observed_at":"2026-07-06T23:54:27.624372Z","submitted_at":"2026-06-17T13:58:39Z","title":"Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-06-26T19:48:32.340111Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2606.19090"},"observation_digest":"sha256:53d722bdbf4f30064aafa073bbee0d39010ea99928281c0d85f7d1eccfe91fb7","observation_id":"ba831a68-6e4d-4ccd-9b39-12251196764f","resolution":{"observed_at":"2026-07-04T02:19:23.625350Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":"2301.06097","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-07-04T02:19:23.624008Z","title":"Bernui, E","venue":null,"work_id":"a9bc7810-f0cd-491b-8900-f01489621b93","year":2023},"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":205,"source":"pdf_text","source_observed_at":"2026-07-01T04:31:47.886338Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2606.31362"},"observation_digest":"sha256:554c7c61080c5e999405ba89466e8f24b5f1399d25fd9c926d17eecb96550d8c","observation_id":"2325b31e-c49a-4f96-8591-8c7526ede824","resolution":{"observed_at":"2026-07-01T11:25:45.522749Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-08-01T08:08:44.992645Z","title":"Bernui, E","venue":null,"work_id":null,"year":2023},"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":122,"source":"pdf_text","source_observed_at":"2026-08-01T08:08:44.992645Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2607.21244"},"observation_digest":"sha256:b2b14d90bd34850c1934289a0bf51991dcb5ea2ce7cb2dce5c0fa6413fe4bbda","observation_id":"a5b76b4f-deea-44e3-9112-44eb62a9fcaa","resolution":{"observed_at":"2026-08-01T08:08:44.992645Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2301.06097/citation-record","integrity":"/paper/2301.06097/integrity","json":"/paper/2301.06097/citation-record.json","paper":"/paper/2301.06097"},"outbound":[],"paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements"},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 20 inbound Pith citation observations for arXiv:2301.06097."}