{"as_of":"2026-08-10T20:32:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:574f2a96a8ad216a0520012a5862879ba8ffb210e5ba986832d06620651b9884","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":28,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":28,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":28,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":28,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T19:20:17.123773Z","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":"2026-07-03T07:07:44.927665Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":"2307.10899","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-07-03T07:07:44.927665Z","title":"Akarsu, E","venue":null,"work_id":"28b76d4b-635e-4c3b-a97e-c87981bfe72f","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":83,"source":"pdf_text","source_observed_at":"2026-05-24T03:50:50.435997Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2402.07716"},"observation_digest":"sha256:654f5860fa0c61d26f8c187cc9219f2b1bcb0f81dbc8c39f3bd8ff113fc51504","observation_id":"be48be62-ee75-4b1e-9fac-bec38cb63ac0","resolution":{"observed_at":"2026-05-24T03:53:54.948871Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-08-10T19:20:17.123773Z","title":"Akarsu, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.10323","last_updated":"2025-02-24T12:41:54Z","snapshot_observed_at":"2026-08-10T19:09:54.981683Z","submitted_at":"2025-01-17T17:52:49Z","title":"Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions","version":2},"reference_index":128,"source":"pdf_text","source_observed_at":"2026-08-10T19:20:17.123773Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2501.10323"},"observation_digest":"sha256:565741e8e7cd99ad49e0f156087254edf57a31a2bc0b8de0c47ce519495e5ea4","observation_id":"2baf2676-8275-495d-875b-c03c139846a6","resolution":{"observed_at":"2026-08-10T19:20:17.123773Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-08-10T18:12:34.923695Z","title":"Akarsu, E","venue":null,"work_id":null,"year":2023},"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":256,"source":"pdf_text","source_observed_at":"2026-08-10T18:12:34.923695Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2501.11571"},"observation_digest":"sha256:2ab9457aaeeb2685a1bc7089fadc62f407b185a48fe55e12767381402c05ca9e","observation_id":"faa95196-7e34-42f4-b3ea-7b91b1e5b665","resolution":{"observed_at":"2026-08-10T18:12:34.923695Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-08-10T01:13:35.460355Z","title":"Akarsu, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.18031","last_updated":"2025-01-29T22:37:59Z","snapshot_observed_at":"2026-08-10T16:58:29.949696Z","submitted_at":"2025-01-29T22:37:59Z","title":"Mapping the $\\Lambda_{\\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-10T01:13:35.460355Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2501.18031"},"observation_digest":"sha256:fbbb852ddb9dec2d324d86b9a449e2a859937786d509058f5cb22bf39aca964b","observation_id":"0f5aff15-cab2-4641-a0f5-d4c3d68a6531","resolution":{"observed_at":"2026-08-10T01:13:35.460355Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-08-07T10:52:56.762567Z","title":"Akarsu, E","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.04306","last_updated":"2025-06-04T17:51:05Z","snapshot_observed_at":"2026-08-07T14:10:01.304994Z","submitted_at":"2025-06-04T17:51:05Z","title":"Can the universe experience an AdS landscape since matter-radiation equality?","version":1},"reference_index":141,"source":"pdf_text","source_observed_at":"2026-08-07T10:52:56.762567Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2506.04306"},"observation_digest":"sha256:d347b928388a171a07deae0fdb7f1406ebac4147e725934133374646643cbce6","observation_id":"54749ce4-53e7-417a-baae-ccb916a69d9c","resolution":{"observed_at":"2026-08-07T10:52:56.762567Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-08-07T01:08:39.487108Z","title":"Akarsu, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.12139","last_updated":"2025-09-08T10:10:32Z","snapshot_observed_at":"2026-08-09T12:56:29.371423Z","submitted_at":"2025-06-13T18:01:48Z","title":"Cosmographic analysis of sign-switching dark energy","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-07T01:08:39.487108Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2506.12139"},"observation_digest":"sha256:4d91719c3ea0269f62437511acffa109807c1ad6b7f38c3b3d3267a3e953a378","observation_id":"a3eee2e0-e2d1-4cf3-86f9-006376bbd3a4","resolution":{"observed_at":"2026-08-07T01:08:39.487108Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":"2307.10899","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-07-03T07:07:44.927665Z","title":"Akarsu, E","venue":null,"work_id":"28b76d4b-635e-4c3b-a97e-c87981bfe72f","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":134,"source":"pdf_text","source_observed_at":"2026-05-18T04:46:14.832965Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2510.18741"},"observation_digest":"sha256:6b9239bb3d476719ce9bacecd1ccb144bb45eb60ebb97b5fdfb781d373b666ee","observation_id":"97dff122-5765-4c90-b5fe-f52d0f6fb839","resolution":{"observed_at":"2026-05-18T04:50:55.604631Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-08-03T17:24:30.791074Z","title":"Akarsu, E","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2512.09991","last_updated":"2026-06-01T10:52:35Z","snapshot_observed_at":"2026-08-03T17:24:26.448316Z","submitted_at":"2025-12-10T19:00:02Z","title":"Observational constraints on 3-forms dark energy","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-03T17:24:30.791074Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2512.09991"},"observation_digest":"sha256:8425c7cd299ee3e77837deb919a3e3fbc34c3e1d2f376e24a0ca0ec28a03967f","observation_id":"96392066-9ff2-44c9-9d06-91a07d07bf71","resolution":{"observed_at":"2026-08-03T17:24:30.791074Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-08-03T11:53:06.030154Z","title":"Akarsuet al., Λ sCDM model: A promising scenario for alleviation of cosmological tensions, arXiv:2307.10899","venue":null,"work_id":null,"year":null},"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":60,"source":"pdf_text","source_observed_at":"2026-08-03T11:53:06.030154Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2601.05218"},"observation_digest":"sha256:4212419d426bb1804c7da60bfa647b056bc5b1e0af54b3f5418cf2e6ed09c734","observation_id":"308cd773-23ac-46d8-b6eb-8f42a0fe0a5c","resolution":{"observed_at":"2026-08-03T11:53:06.030154Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":"2307.10899","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-07-03T07:07:44.927665Z","title":"Akarsu, E","venue":null,"work_id":"28b76d4b-635e-4c3b-a97e-c87981bfe72f","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":77,"source":"pdf_text","source_observed_at":"2026-05-21T13:29:05.147292Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2602.11936"},"observation_digest":"sha256:43e3721ce8cc9948e198f01c7f5d0955ec79e330fc51b0649fc0cae55c544cc0","observation_id":"e5c1240f-1bcd-40be-910a-204a8af5314b","resolution":{"observed_at":"2026-05-21T13:30:12.033468Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":"2307.10899","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-07-03T07:07:44.927665Z","title":"Akarsu, E","venue":null,"work_id":"28b76d4b-635e-4c3b-a97e-c87981bfe72f","year":2023},"citing_paper":{"arxiv_id":"2602.12347","last_updated":"2026-05-14T14:22:35Z","snapshot_observed_at":"2026-08-02T15:18:59.160316Z","submitted_at":"2026-02-12T19:08:27Z","title":"Sign-Switching Dark Energy: Smooth Transitions with Recent DESI DR2 Observations","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-05-16T05:18:35.958352Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2602.12347"},"observation_digest":"sha256:452ad6c072639a11d42e2d19be8f3c5d7cab0c09343d196ff9617950fd061865","observation_id":"574f6b71-be03-4699-9118-6e8a480d9f76","resolution":{"observed_at":"2026-05-16T05:20:39.657598Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-08-02T18:35:49.054528Z","title":"Akarsu, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2603.09270","last_updated":"2026-07-22T07:14:15Z","snapshot_observed_at":"2026-08-09T11:44:48.266368Z","submitted_at":"2026-03-10T06:56:54Z","title":"Statistical consistency of sign-switching vacuum energy with cosmological observations","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-02T18:35:49.054528Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2603.09270"},"observation_digest":"sha256:a0036ffaf4fe8651203f1cb39b9d4b5cb82591f8601eaccfd56fe899ad121f0c","observation_id":"10b6286b-cdb4-4f77-822c-5f5e02263ed1","resolution":{"observed_at":"2026-08-02T18:35:49.054528Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-07-15T12:01:04.317365Z","title":"Akarsu, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2603.14693","last_updated":"2026-07-14T04:50:03Z","snapshot_observed_at":"2026-08-10T07:05:44.565362Z","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":86,"source":"pdf_text","source_observed_at":"2026-07-15T12:01:04.317365Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2603.14693"},"observation_digest":"sha256:6b4db6d3904aa93cdb6a6a7927d4283f361f1a9bea9913c12a046306dbd56a8a","observation_id":"a4c408a7-2901-4537-bc91-d5855112e87e","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":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":"2307.10899","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-07-03T07:07:44.927665Z","title":"Akarsu, E","venue":null,"work_id":"28b76d4b-635e-4c3b-a97e-c87981bfe72f","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":155,"source":"pdf_text","source_observed_at":"2026-05-14T23:13:02.830649Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2603.26560"},"observation_digest":"sha256:f088d165fa3924080f2962715b612e6f555c01717be70784971a4011381178ca","observation_id":"ab46ceac-75bd-4861-a90d-4e6ab9e96999","resolution":{"observed_at":"2026-05-14T23:13:15.325694Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":"2307.10899","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-07-03T07:07:44.927665Z","title":"Akarsu, E","venue":null,"work_id":"28b76d4b-635e-4c3b-a97e-c87981bfe72f","year":2023},"citing_paper":{"arxiv_id":"2604.12987","last_updated":"2026-04-14T17:22:34Z","snapshot_observed_at":"2026-08-08T20:13:05.608575Z","submitted_at":"2026-04-14T17:22:34Z","title":"Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe?","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-10T14:10:57.749079Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2604.12987"},"observation_digest":"sha256:ea6b6f788665b7e7669883ee7320bdaebf9191e3f41ecdee9f9882e8eb5f3eaa","observation_id":"ae479f4c-4d24-40f3-a450-ae22bcd27524","resolution":{"observed_at":"2026-05-10T14:15:30.121242Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":"2307.10899","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-07-03T07:07:44.927665Z","title":"Akarsu, E","venue":null,"work_id":"28b76d4b-635e-4c3b-a97e-c87981bfe72f","year":2023},"citing_paper":{"arxiv_id":"2605.21456","last_updated":"2026-05-20T17:46:56Z","snapshot_observed_at":"2026-07-06T23:31:56.199912Z","submitted_at":"2026-05-20T17:46:56Z","title":"Negative neutrino mass or negative dark energy?","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-21T03:03:07.191130Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2605.21456"},"observation_digest":"sha256:7b6dec3a8f7486309b7d176a3f2540a26bbf29190a045b0e6090d5703a6462e5","observation_id":"eff79b87-c4ac-4887-9bc2-cdaf02799b3c","resolution":{"observed_at":"2026-05-21T03:03:55.414249Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":"2307.10899","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-07-03T07:07:44.927665Z","title":"Akarsu, E","venue":null,"work_id":"28b76d4b-635e-4c3b-a97e-c87981bfe72f","year":2023},"citing_paper":{"arxiv_id":"2606.05352","last_updated":"2026-06-14T13:15:33Z","snapshot_observed_at":"2026-08-03T06:21:51.465232Z","submitted_at":"2026-06-03T18:55:18Z","title":"Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy","version":1},"reference_index":119,"source":"pdf_text","source_observed_at":"2026-06-28T04:59:43.971930Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2606.05352"},"observation_digest":"sha256:f8a2cfdcc967c597b1f47d1f01fd2bfe08af3d32ef54d57a992de5123982e927","observation_id":"7f4dfb8c-81dd-4363-9da8-e893ad72f992","resolution":{"observed_at":"2026-07-02T10:36:52.539867Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-07-12T15:09:17.581029Z","title":"Akarsu, E","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.05352","last_updated":"2026-06-14T13:15:33Z","snapshot_observed_at":"2026-08-03T06:21:51.465232Z","submitted_at":"2026-06-03T18:55:18Z","title":"Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy","version":2},"reference_index":119,"source":"pdf_text","source_observed_at":"2026-07-12T15:09:17.581029Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2606.05352"},"observation_digest":"sha256:03e2ae4c4c368c462c3de1afcd9c692122f4e33c8b7494197aac81e3e89da40a","observation_id":"c36b9fc7-fb22-42ed-9678-cab962ffa428","resolution":{"observed_at":"2026-07-12T15:09:17.581029Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":"2307.10899","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-07-03T07:07:44.927665Z","title":"Akarsu, E","venue":null,"work_id":"28b76d4b-635e-4c3b-a97e-c87981bfe72f","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":75,"source":"pdf_text","source_observed_at":"2026-06-27T23:47:15.644279Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2606.06495"},"observation_digest":"sha256:c27c554c7bf81e2d71a339869bd378c24e692463a5f4f48eb253355fd6541b93","observation_id":"59060634-8b35-4c5a-96a1-7a05ed900a0a","resolution":{"observed_at":"2026-07-02T15:37:06.191381Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-07-12T14:25:03.782538Z","title":"Akarsu E","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.11061","last_updated":"2026-07-06T04:28:26Z","snapshot_observed_at":"2026-07-12T14:25:03.436159Z","submitted_at":"2026-06-09T16:22:18Z","title":"Endpoint Logarithms in the NLO Mueller-Navelet Jet Vertex: Threshold Matching and BLM/MOM Prescription Sensitivity","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-07-12T14:25:03.782538Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2606.11061"},"observation_digest":"sha256:4d2706d3f84874c8f27052b0ab9dc46eae6df220cb20f2711777e4793a06e64f","observation_id":"ef5257cb-c270-45b1-b833-981481974a31","resolution":{"observed_at":"2026-07-12T14:25:03.782538Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":"2307.10899","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-07-03T07:07:44.927665Z","title":"Akarsu, E","venue":null,"work_id":"28b76d4b-635e-4c3b-a97e-c87981bfe72f","year":2023},"citing_paper":{"arxiv_id":"2606.11062","last_updated":"2026-06-09T16:23:08Z","snapshot_observed_at":"2026-08-01T22:02:37.358175Z","submitted_at":"2026-06-09T16:23:08Z","title":"A Friendly Phantom: Late-time AdS-to-dS transition and cosmological tensions","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-06-27T12:16:15.909335Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2606.11062"},"observation_digest":"sha256:cdb617b8f0a67801e280fc28162adc70846d48d07552a3895786dddc99b79405","observation_id":"b74d3024-31b8-4202-9a52-edcd9d8074a2","resolution":{"observed_at":"2026-07-03T07:07:44.929042Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":"2307.10899","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-07-03T07:07:44.927665Z","title":"Akarsu, E","venue":null,"work_id":"28b76d4b-635e-4c3b-a97e-c87981bfe72f","year":2023},"citing_paper":{"arxiv_id":"2606.27436","last_updated":"2026-07-10T09:33:28Z","snapshot_observed_at":"2026-08-08T13:50:38.175219Z","submitted_at":"2026-06-25T18:00:19Z","title":"Three-form dark energy: constraints and multi-probe comparison with $\\Lambda$CDM","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-06-29T01:30:43.118529Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2606.27436"},"observation_digest":"sha256:c7d3024b2e36b2b63b7871255f840c63a918e598c5f88f53d1085052e8f297cc","observation_id":"27355eb2-5642-4f86-88cc-f69b836cff5b","resolution":{"observed_at":"2026-07-01T18:45:59.607866Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-07-13T07:19:36.090369Z","title":"Akarsu, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2606.27436","last_updated":"2026-07-10T09:33:28Z","snapshot_observed_at":"2026-08-08T13:50:38.175219Z","submitted_at":"2026-06-25T18:00:19Z","title":"Three-form dark energy: constraints and multi-probe comparison with $\\Lambda$CDM","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-07-13T07:19:36.090369Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2606.27436"},"observation_digest":"sha256:1ad0654613c972c99486517f1bd03901a34040802ddcd8f1aff0cc358a90e39d","observation_id":"951e4e5b-2aa3-4180-b522-ce5259a655fe","resolution":{"observed_at":"2026-07-13T07:19:36.090369Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-08-02T05:48:21.309580Z","title":"Akarsu, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.13283","last_updated":"2026-07-14T21:36:00Z","snapshot_observed_at":"2026-08-07T20:25:34.943645Z","submitted_at":"2026-07-14T21:36:00Z","title":"The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions","version":1},"reference_index":167,"source":"pdf_text","source_observed_at":"2026-08-02T05:48:21.309580Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2607.13283"},"observation_digest":"sha256:8cae2ba573a56e1fc20be71150a34ec79bc734356e00c937051efdbe34d8b573","observation_id":"26998a0f-81a7-4172-98b0-f81c8f4973ee","resolution":{"observed_at":"2026-08-02T05:48:21.309580Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-08-01T16:30:00.991506Z","title":"Akarsu, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:00.991506Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:5f620b7eb54769936910ae0bcf090b8507aeac4f91fad29e5c8da3771939f613","observation_id":"db9aa56b-7912-467b-b3f8-94849ed69dc0","resolution":{"observed_at":"2026-08-01T16:30:00.991506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-08-01T08:08:45.977735Z","title":"Akarsu, 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":131,"source":"pdf_text","source_observed_at":"2026-08-01T08:08:45.977735Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2607.21244"},"observation_digest":"sha256:fc3ca6aaf0f6b9281b1d6d65665ae30a8ac9f53de0b14186f6728d2cc1de4205","observation_id":"33cef7eb-8b04-4001-a844-cc6d7ff850a9","resolution":{"observed_at":"2026-08-01T08:08:45.977735Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-08-01T00:51:49.815182Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.26050","last_updated":"2026-08-01T11:27:56Z","snapshot_observed_at":"2026-08-10T18:11:19.299370Z","submitted_at":"2026-07-28T17:58:23Z","title":"$\\Lambda$XCDM: a running vacuum strategy for crossing the phantom divide","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-01T00:51:49.815182Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2607.26050"},"observation_digest":"sha256:c34939c8fd2a9a3d0068be8b64dc8cc747eac64f40ed77f441ce5af528341962","observation_id":"5a449b1f-192c-48b8-98c1-8d8d80746539","resolution":{"observed_at":"2026-08-01T00:51:49.815182Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-08-04T01:33:29.309989Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.26050","last_updated":"2026-08-01T11:27:56Z","snapshot_observed_at":"2026-08-10T18:11:19.299370Z","submitted_at":"2026-07-28T17:58:23Z","title":"$\\Lambda$XCDM: a running vacuum strategy for crossing the phantom divide","version":2},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-04T01:33:29.309989Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2607.26050"},"observation_digest":"sha256:8392a620aa3c5856676f224b4703511dd4a6815e485040819c98e0624a1c86ad","observation_id":"3908ca2b-40fb-475e-8194-022a472c51ea","resolution":{"observed_at":"2026-08-04T01:33:29.309989Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2307.10899/citation-record","integrity":"/paper/2307.10899/integrity","json":"/paper/2307.10899/citation-record.json","paper":"/paper/2307.10899"},"outbound":[],"paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 28 inbound Pith citation observations for arXiv:2307.10899."}