{"as_of":"2026-08-12T16:57:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:8250772b6bbcd68dcc838e6bf4c9947f57415d14f80b9bbde57a9edb65c70f11","coverage":[{"denominator":40,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":40,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T15:07:16.440283Z","state":"measured"},{"denominator":44,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":44,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T18:36:59.514284Z","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":"2026-05-15T13:15:50.209661Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.16438","snapshot_observed_at":"2026-08-06T18:36:59.514284Z","title":"Goswami and S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.07798","last_updated":"2025-07-10T14:26:06Z","snapshot_observed_at":"2026-08-10T05:27:39.960371Z","submitted_at":"2025-07-10T14:26:06Z","title":"Exploring non-cold dark matter in a scenario of dynamical dark energy with DESI DR2 data","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T18:36:59.514284Z"},"links":{"cited_paper":"/paper/2505.16438","citing_paper":"/paper/2507.07798"},"observation_digest":"sha256:e7dde8d30b2b2303f229a9642071d63bc14e2544b864523199efa736080db254","observation_id":"67bc321b-a70d-4b2e-9b42-6fa0f763c410","resolution":{"observed_at":"2026-08-06T18:36:59.514284Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.16438","snapshot_observed_at":"2026-08-06T15:12:34.115810Z","title":"Goswami and S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.16589","last_updated":"2026-06-23T13:43:52Z","snapshot_observed_at":"2026-08-08T06:56:16.966820Z","submitted_at":"2025-07-22T13:45:38Z","title":"Cosmological preference for a positive neutrino mass at 2.7$\\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data","version":3},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T15:12:34.115810Z"},"links":{"cited_paper":"/paper/2505.16438","citing_paper":"/paper/2507.16589"},"observation_digest":"sha256:94230b3c0a56ff6314cdb4f94b9db413e0bbac82fde6edc3921ce91be28ba4fe","observation_id":"f3d54fa6-1357-4941-b604-a1b71c2fd1c0","resolution":{"observed_at":"2026-08-06T15:12:34.115810Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.16438","snapshot_observed_at":"2026-08-04T09:59:23.412413Z","title":"Goswami and S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.12627","last_updated":"2026-06-20T07:00:45Z","snapshot_observed_at":"2026-08-12T13:22:12.009948Z","submitted_at":"2025-10-14T15:24:50Z","title":"Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2","version":2},"reference_index":129,"source":"pdf_text","source_observed_at":"2026-08-04T09:59:23.412413Z"},"links":{"cited_paper":"/paper/2505.16438","citing_paper":"/paper/2510.12627"},"observation_digest":"sha256:66d5e675afd0952e5c1c9c0fc9190ca7a2daa58b024634599fa873687f298ca8","observation_id":"b20fea1d-86d1-4b3e-8250-e638c2b13dbd","resolution":{"observed_at":"2026-08-04T09:59:23.412413Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"cited_work":{"arxiv_id":"2505.16438","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2505.16438","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Goswami and S","venue":null,"work_id":"f544806f-f725-4bb9-be1d-dffc4891f555","year":2025},"citing_paper":{"arxiv_id":"2603.10787","last_updated":"2026-03-11T14:00:06Z","snapshot_observed_at":"2026-08-11T15:40:03.224454Z","submitted_at":"2026-03-11T14:00:06Z","title":"Measuring neutrino mass in light of ACT DR6 and DESI DR2","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-05-15T13:14:03.491513Z"},"links":{"cited_paper":"/paper/2505.16438","citing_paper":"/paper/2603.10787"},"observation_digest":"sha256:85cf9111b30c2087159665810222a4234d163fb4d1eb1b4bb55025bd0e7e7ca5","observation_id":"eb2ed846-6baa-4efe-b9e3-51c1a2ed183d","resolution":{"observed_at":"2026-05-15T13:15:50.211325Z","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"}}],"links":{"evidence":"/evidence","html":"/paper/2505.16438/citation-record","integrity":"/paper/2505.16438/integrity","json":"/paper/2505.16438/citation-record.json","paper":"/paper/2505.16438"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:20.064627Z","title":null,"venue":null,"work_id":"0cf88428-b78e-4f11-8a80-1b7d1c7772a7","year":1998},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:13.898130Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:93b0ae0e52dfdc0d128a1eb6691e272a954fff33a98e889dd3206639bb17d3c0","observation_id":"21806e0f-e213-4f5a-8c25-0253b36c8f22","resolution":{"observed_at":"2026-08-07T15:07:20.130808Z","resolver_source":"raw_fallback","status":"unresolved"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:19.885254Z","title":"Perlmutter, G","venue":null,"work_id":"7d0ae1e2-93dd-4d0c-8413-aa2bbd0baa9a","year":1999},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:13.972156Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:d667b6045a6915df0d357eef9526d8940e4b8ed5df8895321434267c0188a748","observation_id":"7447b1be-7bb3-43aa-b660-db7b798c44c7","resolution":{"observed_at":"2026-08-07T15:07:19.958947Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:19.746993Z","title":"Arnaud, M","venue":null,"work_id":"3eb73079-73c6-48c9-bf62-1ebe078e6796","year":2016},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:14.063137Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:3f2cfe4f342c22752659a1d8b48877ad4c5c0bb7fbfb3cc1508a1295cdcc48ac","observation_id":"373de35b-e6a5-46e3-85f2-00856b988c8e","resolution":{"observed_at":"2026-08-07T15:07:19.811577Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:19.581242Z","title":null,"venue":null,"work_id":"d5079ea3-fa86-4c7b-999e-172058489bc5","year":2012},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:14.145539Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:6e0fdbfecd1e7f65c25a5310b7e478b45e8dfe9cad644f44375d15dd4f6fa1fd","observation_id":"87d68020-678f-4bd1-946e-adec1b7beda2","resolution":{"observed_at":"2026-08-07T15:07:19.614068Z","resolver_source":"raw_fallback","status":"unresolved"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:19.509560Z","title":"Jarosik, C","venue":null,"work_id":"6fcc9493-b877-4146-9fe1-f3f49c5d0cd5","year":2011},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:14.237447Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:c6ceb4d9b9894ffaf804cc0f59fc73916f5959b2f88cf0d65471cf82b936e4f7","observation_id":"e67f1ea1-6123-45b6-9a66-450d939a8e78","resolution":{"observed_at":"2026-08-07T15:07:19.533254Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:14.305563Z","title":"Ratra, P","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:14.305563Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:e0e373564733506de43d6d2ef1e6b39d96d5739d7061da3e907402465a9483d2","observation_id":"a5ec755e-3ac2-48f9-a698-53f91e4caff1","resolution":{"observed_at":"2026-08-07T15:07:14.305563Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:14.375710Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:14.375710Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:ec8c48783dbcb876ffd4691bae1ac7525c860dfe7c47e64419dc8aaaccd2bc78","observation_id":"fed2dcb8-4dbf-4d56-8ad2-4721bba9df62","resolution":{"observed_at":"2026-08-07T15:07:14.375710Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:14.473816Z","title":"Caldwell, A phantom menace? cosmological consequences of a dark energy component with super-negative equation of state, Physics Letters B 545 (1–2) (2002) 23–29","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:14.473816Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:cca0c5636485626b4e058288bb7c0ea9eb33285822b1c66fc3a2963c8f880aa9","observation_id":"47fc3d6d-2de5-4b35-82db-0e977406c2f9","resolution":{"observed_at":"2026-08-07T15:07:14.473816Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:14.530992Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:14.530992Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:c61bb572193b45a335d15ffbfb6a9d5058f879b9edc7db145c9b1cef0978f825","observation_id":"0d1dee69-f378-4e29-97b0-0235dc61fdac","resolution":{"observed_at":"2026-08-07T15:07:14.530992Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:14.592639Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:14.592639Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:f3663494bcce24afcb4737f2a95c0136bbc34c8732435821f0eba51eba17a02c","observation_id":"6c7f6a2b-cc34-4342-9cb2-befee0974761","resolution":{"observed_at":"2026-08-07T15:07:14.592639Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:14.635878Z","title":"Bousso, The holographic principle, Reviews of Modern Physics 74 (3) (2002) 825–874","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:14.635878Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:c677fbb31e82c54bf956479b6388140177beb4cdfd3a4388d678712076d7e993","observation_id":"df8fddc7-3972-49ec-8ef3-571606d1926d","resolution":{"observed_at":"2026-08-07T15:07:14.635878Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9806039","last_updated":"1998-06-11T22:31:30Z","snapshot_observed_at":"2026-07-07T05:16:56.294112Z","submitted_at":"1998-06-04T18:48:23Z","title":"Holography and Cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/9806039","snapshot_observed_at":"2026-08-07T15:07:14.717890Z","title":"Fischler, L","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:14.717890Z"},"links":{"cited_paper":"/paper/hep-th/9806039","citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:4873a80c8ef9207416bc7e4de70ca5e5f4b2540f8070ef9a2cd0075f59e832bd","observation_id":"f41886af-04d6-46f1-b7b7-d7d02dd2d132","resolution":{"observed_at":"2026-08-07T15:07:14.717890Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.01183","last_updated":"2021-06-05T10:18:21Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2021-03-01T18:27:48Z","title":"In the Realm of the Hubble tension $-$ a Review of Solutions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.01183","snapshot_observed_at":"2026-08-07T15:07:14.792619Z","title":"Di Valentino, O","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:14.792619Z"},"links":{"cited_paper":"/paper/2103.01183","citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:fb3f3dc4379f1eeed24eaefc32c0c54215dfeea61aedd4630aea3b8675f0409a","observation_id":"62146bbb-b466-4633-af7c-6989c743125b","resolution":{"observed_at":"2026-08-07T15:07:14.792619Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:19.437310Z","title":"Zimdahl, D","venue":null,"work_id":"140e44ac-1bd5-4c7c-9aa5-c3467883d95b","year":2004},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:14.854198Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:973e02b9152a193f0510c2f62e2318481ea7c24ead9eb24c89a3dea5f389d7df","observation_id":"b3e6514b-a0b1-4ce0-a6d5-53aa8e874fa8","resolution":{"observed_at":"2026-08-07T15:07:19.473394Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"1204.5892","last_updated":"2012-04-26T11:52:07Z","snapshot_observed_at":"2026-07-06T02:47:06.314943Z","submitted_at":"2012-04-26T11:52:07Z","title":"Models of Interacting Dark Energy","version":1},"cited_work":{"arxiv_id":"1204.5892","doi":null,"metadata_source":"pith","pith_arxiv_id":"1204.5892","snapshot_observed_at":"2026-08-07T15:07:17.366555Z","title":"Models of Interacting Dark Energy","venue":"astro-ph.CO","work_id":"d9224f9d-14d3-40bc-9215-765abf6bce50","year":2012},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:14.942303Z"},"links":{"cited_paper":"/paper/1204.5892","citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:849f286dd690c5698334420ed56f1ce3b5068a71e2db8f2c2d4a5ec3e01222ef","observation_id":"f04f40c8-ff9c-44cb-b410-060944f7d6cb","resolution":{"observed_at":"2026-08-07T15:07:17.475545Z","resolver_source":"local_arxiv","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:19.281135Z","title":"Del Campo, R","venue":null,"work_id":"ae6993c2-3315-4150-a9fc-1e80be9b8c8e","year":2009},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:15.004932Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:b421f120d5bba39704ecd4fb676b194723e8dd85f5de3ace334a19ffbe99dbe0","observation_id":"490f0658-6c05-4c28-b05e-ab172e1a5369","resolution":{"observed_at":"2026-08-07T15:07:19.337900Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:19.144145Z","title":"Olivares, F","venue":null,"work_id":"459f76d7-d774-419f-a631-c25ede7a40d8","year":2005},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:15.066349Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:1301224d6bc7056528a14ccbc14659e0dd9a782fd0e10a27d8e0c2244deda407","observation_id":"0c575312-0560-4dbd-86a0-04d9bc5d8d18","resolution":{"observed_at":"2026-08-07T15:07:19.192772Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:19.023366Z","title":"Sinha, M","venue":null,"work_id":"54d8ced5-1727-452d-a6f2-62e2f9581175","year":2023},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:15.144806Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:7cdce586583c9bcf07fea1553f12d1976020e169797261d4de6a42a514838b2a","observation_id":"45171475-7554-47ad-b92b-01f451336dc8","resolution":{"observed_at":"2026-08-07T15:07:19.086293Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:18.873050Z","title":null,"venue":null,"work_id":"b37be0d9-75e2-4975-9f52-552e1ff5ea93","year":2015},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:15.228173Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:e044a71239f7fb7c7cbd964bf1dc1964fa265cfdebf382830c8bd9bd97b5e86d","observation_id":"7dc29041-b6a8-4763-91f2-523ae95a3506","resolution":{"observed_at":"2026-08-07T15:07:18.935164Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2407.16644","last_updated":"2024-10-23T15:06:00Z","snapshot_observed_at":"2026-07-06T18:50:48.181248Z","submitted_at":"2024-07-23T16:58:14Z","title":"Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae","version":3},"cited_work":{"arxiv_id":"2407.16644","doi":null,"metadata_source":"pith","pith_arxiv_id":"2407.16644","snapshot_observed_at":"2026-08-07T15:07:17.252702Z","title":"Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae","venue":"astro-ph.CO","work_id":"40003e5e-fdf2-41fb-96df-e5f3e33097eb","year":2024},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:15.323964Z"},"links":{"cited_paper":"/paper/2407.16644","citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:153981befec4ef4de6cb3f73541b76e7cf23e24829012eb6da1c92a79c599f6c","observation_id":"d5d7def0-6d7c-46c1-8ff0-6f9bb11d7ebc","resolution":{"observed_at":"2026-08-07T15:07:17.285023Z","resolver_source":"local_arxiv","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:18.709269Z","title":"Brout, D","venue":null,"work_id":"732a83dc-63d6-407b-93fc-3f46f6a5341b","year":2022},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:15.411766Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:89e73959419fda4855066a709219eec85b4ae021e59900b30495a4864b29fc6a","observation_id":"19e3de20-e3e9-4630-9f2d-87fec0cbb063","resolution":{"observed_at":"2026-08-07T15:07:18.794754Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:15.497484Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:15.497484Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:b7adf06026c52bbb35beaebfa5d24b34f28a6f3c9b67110b1c487cdfb598f99a","observation_id":"2b030d0a-255a-4eb6-8046-5086e29ee45a","resolution":{"observed_at":"2026-08-07T15:07:15.497484Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.00876","last_updated":"2021-04-30T05:24:01Z","snapshot_observed_at":"2026-08-12T08:47:40.512670Z","submitted_at":"2021-04-30T05:24:01Z","title":"Cosmic acceleration with bulk viscosity in modified $f(Q)$ gravity","version":1},"cited_work":{"arxiv_id":"2105.00876","doi":null,"metadata_source":"pith","pith_arxiv_id":"2105.00876","snapshot_observed_at":"2026-08-07T15:07:17.096654Z","title":"Cosmic acceleration with bulk viscosity in modified $f(Q)$ gravity","venue":"gr-qc","work_id":"4ec2a5ee-122c-49c5-9132-0a0a4f85328e","year":2021},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:15.562028Z"},"links":{"cited_paper":"/paper/2105.00876","citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:5dfcbaa77b233ba6f162eefa1d5c1925f31e8c5839e82ed5ef270edce1392743","observation_id":"55c34b6f-f2ca-41d2-aec1-700b005c41ed","resolution":{"observed_at":"2026-08-07T15:07:17.165576Z","resolver_source":"local_arxiv","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":"2304.03783","last_updated":"2024-06-01T14:38:07Z","snapshot_observed_at":"2026-07-06T15:13:28.897516Z","submitted_at":"2023-04-07T12:06:41Z","title":"New parametrization of the dark-energy equation of state with a single parameter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.03783","snapshot_observed_at":"2026-08-07T15:07:15.633690Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:15.633690Z"},"links":{"cited_paper":"/paper/2304.03783","citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:3f05cb3979cd234890559bc8fbfa05137e6561c06fd407deb6d36992d9943685","observation_id":"bd27f4e3-3803-4a54-b1b3-c35e1448c200","resolution":{"observed_at":"2026-08-07T15:07:15.633690Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:18.517257Z","title":null,"venue":null,"work_id":"00c5afb3-a187-4fe6-81d8-b02035a839fb","year":2018},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:15.701338Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:966f00b09ed909fef359a7b2affb299038c5ff6ddef1cb8a3be2b56948b93cb1","observation_id":"6decf81e-a9e2-46ce-aa36-26eb147bc5d7","resolution":{"observed_at":"2026-08-07T15:07:18.592911Z","resolver_source":"raw_fallback","status":"unresolved"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:18.324773Z","title":null,"venue":null,"work_id":"f99e194d-ec85-41a8-b2cb-7dbf27f1dedd","year":2021},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:15.770845Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:ac3af1e9ada54c0a4f6339400475e3572aed2e8793aac82381b73b32b1287c9d","observation_id":"5e01231f-ebf9-48ff-bf6f-4dc010743f4e","resolution":{"observed_at":"2026-08-07T15:07:18.430939Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"1911.07688","last_updated":"2019-11-18T15:10:42Z","snapshot_observed_at":"2026-07-06T08:37:51.370343Z","submitted_at":"2019-11-18T15:10:42Z","title":"emcee v3: A Python ensemble sampling toolkit for affine-invariant MCMC","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.07688","snapshot_observed_at":"2026-08-07T15:07:15.843895Z","title":"Foreman-Mackey, W","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:15.843895Z"},"links":{"cited_paper":"/paper/1911.07688","citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:83f9e2edf2587687eb749481a4e367f8f4aeb6f5e6a311b50b7583f79aa775f5","observation_id":"6f7cbe68-dded-4066-9767-0bcf99dcd1fc","resolution":{"observed_at":"2026-08-07T15:07:15.843895Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.13970","last_updated":"2025-07-09T12:22:45Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2019-10-30T16:38:10Z","title":"GetDist: a Python package for analysing Monte Carlo samples","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.13970","snapshot_observed_at":"2026-08-07T15:07:15.892242Z","title":"Lewis, Getdist: a python package for analysing monte carlo samples, arXiv preprint arXiv:1910.13970 (2019)","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:15.892242Z"},"links":{"cited_paper":"/paper/1910.13970","citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:9fa6e1f9153a67d07415b0a2785e536d16072a63f2afb970014e8b5f68ad9cc2","observation_id":"725c5a5f-a035-4202-b106-fcd9dcfe9d52","resolution":{"observed_at":"2026-08-07T15:07:15.892242Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.10095","last_updated":"2025-03-16T06:29:27Z","snapshot_observed_at":"2026-07-06T15:05:00.197020Z","submitted_at":"2023-03-17T16:16:03Z","title":"The Pantheon Sample Analysis of Cosmological Constraints under New Models","version":2},"cited_work":{"arxiv_id":"2303.10095","doi":null,"metadata_source":"pith","pith_arxiv_id":"2303.10095","snapshot_observed_at":"2026-08-07T15:07:16.939751Z","title":"The Pantheon Sample Analysis of Cosmological Constraints under New Models","venue":"astro-ph.CO","work_id":"2b614192-b177-49cc-9d47-901aa79d9ec6","year":2023},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:15.939838Z"},"links":{"cited_paper":"/paper/2303.10095","citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:9be562afc2638ef6859ef518e70302c74ca614ef80815d7f61b3d19bd53094ba","observation_id":"65d6d060-bb6a-4ec1-b559-c298a90d9c4a","resolution":{"observed_at":"2026-08-07T15:07:16.982048Z","resolver_source":"local_arxiv","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:15.971701Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:15.971701Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:bd4e7eabfee4e0dce4172c53c7e9191640130fce5a66a24ae56d9f9c095afa0d","observation_id":"5e269171-50a9-4949-b219-3ad23ed55df1","resolution":{"observed_at":"2026-08-07T15:07:15.971701Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:16.016172Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:16.016172Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:49e3e42c2ff40cb5b1319287ec540eaa52d93ce29a447d4c1ac0bf0a2950a077","observation_id":"c035ecc0-19e3-427b-854c-52f48d4de9a3","resolution":{"observed_at":"2026-08-07T15:07:16.016172Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1142/s0218271824500317","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Goswami, S","venue":"International Journal of Modern Physics D","work_id":"fa0a2493-cdc4-4338-9345-9e003bbe6657","year":2024},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:16.049406Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:e548641a181d4fed656689cce1b8030a7f750284d586c3f10faa7cc6a67c5daf","observation_id":"936170bc-f696-4b57-9165-3cf379291708","resolution":{"observed_at":"2026-08-07T15:07:16.649499Z","resolver_source":"doi","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:18.099065Z","title":null,"venue":null,"work_id":"240bad7c-9333-4fe4-8405-8cfdd872b5d9","year":1995},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:16.098178Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:2b7c966d4d75f2b59a937a3ad6aea0b0b80c339d6713a77771a11a13013e8a43","observation_id":"f5a5c831-f9b5-447f-a144-a70337cbcd48","resolution":{"observed_at":"2026-08-07T15:07:18.258168Z","resolver_source":"raw_fallback","status":"unresolved"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:16.142908Z","title":"Mandal, S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:16.142908Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:85c6845a8ecfe72214bff2bb4fb7fbfc75a5b8d6b81578c961987b1f3f5fb78c","observation_id":"7f423890-7a20-4882-b4fe-8395fb535dd8","resolution":{"observed_at":"2026-08-07T15:07:16.142908Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.09900","last_updated":"2018-07-16T21:19:43Z","snapshot_observed_at":"2026-07-06T06:41:07.943229Z","submitted_at":"2018-05-24T21:09:46Z","title":"The impact of the cosmic variance on $H_0$ on cosmological analyses","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.09900","snapshot_observed_at":"2026-08-07T15:07:16.178724Z","title":"Camarena, V","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:16.178724Z"},"links":{"cited_paper":"/paper/1805.09900","citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:77d05bad4704b9adf4d0a7c39f2ef9b506f673e63667f637e176a3fb787f4d21","observation_id":"511dd456-d871-42b3-9927-b14393e3f06b","resolution":{"observed_at":"2026-08-07T15:07:16.178724Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.10509","last_updated":"2023-07-22T05:49:59Z","snapshot_observed_at":"2026-07-06T14:54:00.594534Z","submitted_at":"2023-02-21T08:17:30Z","title":"Exploring the Possibility of Interacting Quintessence Model as an Alternative to the $\\Lambda$CDM Model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.10509","snapshot_observed_at":"2026-08-07T15:07:16.215708Z","title":"Roy, Exploring the possibility of interacting quintessence model as an alternative to the ΛCDM model, Gen","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:16.215708Z"},"links":{"cited_paper":"/paper/2302.10509","citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:5adf47aaed049c3be7011fd050bacb08b4afa86adb4c10415f02741b17be544d","observation_id":"95948f39-3e13-4084-b797-df3fc706c44f","resolution":{"observed_at":"2026-08-07T15:07:16.215708Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-07T15:07:16.267640Z","title":"Aghanim, et al., Planck 2018 results","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:16.267640Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:7d589371615902c02db2d9f1e1700bfb0a7fda7e0eecd5d82566576ae8af4647","observation_id":"be19b283-3e27-40b2-bacd-2c14a347fbb0","resolution":{"observed_at":"2026-08-07T15:07:16.267640Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:16.322376Z","title":"Sahni, A","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:16.322376Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:ff10684d9146d9ef1e7ab166386131271099c0434a140f278435f49dd75ab9a1","observation_id":"dbfd008c-9628-4d26-96c6-aa015a92c477","resolution":{"observed_at":"2026-08-07T15:07:16.322376Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:07:17.818502Z","title":"Pav ´on, B","venue":null,"work_id":"20ba528c-a491-4470-87ab-ec966697a79d","year":2009},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:16.383087Z"},"links":{"citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:2e4e1d187c1d91d3f5f33f904fd23dde1cf3dac9308e58db6fdecc77a0e1f548","observation_id":"11201cff-d179-480a-b2ab-d1856761ea5e","resolution":{"observed_at":"2026-08-07T15:07:17.963581Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2407.14934","last_updated":"2024-11-12T01:42:43Z","snapshot_observed_at":"2026-08-06T12:07:52.318618Z","submitted_at":"2024-07-20T16:52:17Z","title":"Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.14934","snapshot_observed_at":"2026-08-07T15:07:16.440283Z","title":"Li, P.-J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:16.440283Z"},"links":{"cited_paper":"/paper/2407.14934","citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:516803c12d56c5e6b5ed78d7e0172bf69b6f34cb1f48bbea1292921c8f790d47","observation_id":"fcabd56b-c216-4e42-8c88-c59cfd6beed8","resolution":{"observed_at":"2026-08-07T15:07:16.440283Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-12T08:47:13.329083Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario"},"reference_resolution":{"displayed":40,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":26,"verified_exact":5,"verified_fuzzy":9},"total_outbound_references":40},"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 40 of 40 outbound references and 4 inbound Pith citation observations for arXiv:2505.16438."}