{"as_of":"2026-08-09T23:50:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b61e0128e178f2dc6aa13a87e0e27ed430f0c47bf7550314fef0c65c0fcf9322","coverage":[{"denominator":46,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":46,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T20:51:11.711685Z","state":"measured"},{"denominator":47,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":47,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T16:47:56.193625Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":1,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"cited_work":{"arxiv_id":"2502.09709","doi":"10.48550/arxiv.2502.09709","metadata_source":"pith","pith_arxiv_id":"2502.09709","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","venue":"astro-ph.CO","work_id":"8fae738a-d89d-4662-bfc2-0dbb421446e5","year":2025},"citing_paper":{"arxiv_id":"2512.12304","last_updated":"2026-06-29T09:05:20Z","snapshot_observed_at":"2026-08-09T00:03:49.980545Z","submitted_at":"2025-12-13T12:08:36Z","title":"Local Nonlinear Transforms Effectively Extract Cosmological Information From Large-Scale Structure","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-03T16:47:56.193625Z"},"links":{"cited_paper":"/paper/2502.09709","citing_paper":"/paper/2512.12304"},"observation_digest":"sha256:cad0e559e5f9beec012f0e302fc86ccd74a99b975c864b320f34a653817c18ad","observation_id":"972cfb68-43df-4913-b23b-7cb71e805fca","resolution":{"observed_at":"2026-08-03T16:49:35.344930Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2502.09709/citation-record","integrity":"/paper/2502.09709/integrity","json":"/paper/2502.09709/citation-record.json","paper":"/paper/2502.09709"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T20:51:11.381476Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.381476Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:d515800b41b5518dd4a75da3ff0551c485cab1771e2478ff6d81a3cad3e32d20","observation_id":"8c5a3e09-aee0-4c6a-a892-dbeba41f13a7","resolution":{"observed_at":"2026-08-07T20:51:11.381476Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.14289","last_updated":"2023-03-13T13:14:26Z","snapshot_observed_at":"2026-08-04T10:53:26.160185Z","submitted_at":"2022-03-27T12:35:41Z","title":"An Introduction to Multiparameter Persistence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.14289","snapshot_observed_at":"2026-08-07T20:51:11.387313Z","title":"G., Aguilar, J., Ahlen, S., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.387313Z"},"links":{"cited_paper":"/paper/2203.14289","citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:9fc351cee2c31ee7227505445b10c687f0f7f414fe8ebe6b27c681a75bbd2278","observation_id":"116fcce4-a2c3-43cf-a67b-68b0f0dc1567","resolution":{"observed_at":"2026-08-07T20:51:11.387313Z","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":"2026-08-07T20:51:11.408740Z","title":"2021a, MNRAS, 500, 5479, doi: 10.1093/mnras/staa3604 —","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.408740Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:fbc70d24c50c3e2ab70c7f17d9226664ea36c3e49cf068a3ee27baf2fc0b8eea","observation_id":"6fa89a8c-127a-4f78-bc7b-c3315b49ecad","resolution":{"observed_at":"2026-08-07T20:51:11.408740Z","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":"2026-08-07T20:51:11.457159Z","title":"2024, MNRAS, 529, 4325, doi:10.1093/mnras/stae543","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.457159Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:a4cd33e8a98f41541aa3963a67a03fbaf8cf9bde24cd6a167dfd7706e47f27f2","observation_id":"1784b87b-050b-475b-8266-721a538d3266","resolution":{"observed_at":"2026-08-07T20:51:11.457159Z","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":"2026-08-07T20:51:11.461752Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.461752Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:bea5dfa3cfa6723434eb770735fedf3da6587718a6564dacf71a9e2583f246dc","observation_id":"54efcdc0-6a1c-43c0-990c-8dae026a7ec2","resolution":{"observed_at":"2026-08-07T20:51:11.461752Z","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":"2026-08-07T20:51:11.467382Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.467382Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:cbfc7ab609cb91be7b825559f2f4b625145399af34a2c49288ecb3f1e3fd137b","observation_id":"bbaeb298-a535-46af-aef9-fbca801549ab","resolution":{"observed_at":"2026-08-07T20:51:11.467382Z","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":"2026-08-07T20:51:11.472449Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.472449Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:135fea7cd314667ee0234ab838ffd2d1356bb76a767e57e94c91b12ea19693e3","observation_id":"f12682ae-e1d9-4661-bc26-3e1416691474","resolution":{"observed_at":"2026-08-07T20:51:11.472449Z","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":"2026-08-07T20:51:11.476862Z","title":"2009, Bulletin of the American Mathematical Society, 46, 255, doi: 10.1090/s0273-0979-09-01249-x","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.476862Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:1adac6a4a0bb7f43afd569c2190833f55d777985ba1eb8a019488a553b6fe57f","observation_id":"d24ffb2c-1aa7-4127-adec-1da334a7472a","resolution":{"observed_at":"2026-08-07T20:51:11.476862Z","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/s0218654305000761","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T20:51:12.170638Z","title":null,"venue":null,"work_id":"58fe2beb-f1f3-499d-8026-c4567354078e","year":2005},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.481037Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:ace77c67d136d47477e3c50a8dce5705ad6c686a2fbbec92cd34d5fbc5ec9258","observation_id":"15b543b9-b9dc-48ac-84a7-fe1244d6022f","resolution":{"observed_at":"2026-08-07T20:51:12.174888Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-07T20:51:11.485544Z","title":"2013, A&A, 551, A88, doi:10.1051/0004-6361/201220538","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.485544Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:579a33ab7a59e371bda015e1d5336f0cb146135c78823c04e0c4fc7d48335520","observation_id":"6afcb2e2-93a0-4a90-b8a5-adcd29fb4b80","resolution":{"observed_at":"2026-08-07T20:51:11.485544Z","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":"10.1103/physrevd.106.023521","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T20:51:12.146949Z","title":"T., Hellwing, W., et al","venue":null,"work_id":"d83a9c69-758a-425e-8964-4fe3dd74449b","year":2022},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.490458Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:6a1c4a96b48abe13323de1f0773fb5f51d950094e2702730be90aa46636b1854","observation_id":"96d081d7-c594-44e4-a331-d3700c8e71c6","resolution":{"observed_at":"2026-08-07T20:51:12.151295Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-07T20:51:11.495464Z","title":"R., Abel, T., & Banerjee, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.495464Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:f1610b6393879a0d73ecba48a08b27a21d095a254077a98037eab8d7b665127b","observation_id":"76384650-7169-43c0-99c7-de56315a4e53","resolution":{"observed_at":"2026-08-07T20:51:11.495464Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.08994","last_updated":"2023-06-03T14:15:39Z","snapshot_observed_at":"2026-08-09T21:12:40.972779Z","submitted_at":"2023-05-15T20:20:55Z","title":"How to estimate Fisher information matrices from simulations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.08994","snapshot_observed_at":"2026-08-07T20:51:11.500405Z","title":"R., & Wandelt, B","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.500405Z"},"links":{"cited_paper":"/paper/2305.08994","citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:f8b89867588ca5de1ce618d9e426ab4edb95dc54e991e042a02d7c54bac2ab3e","observation_id":"a4222057-2646-4fdd-bdc3-5d5617aab1cc","resolution":{"observed_at":"2026-08-07T20:51:11.500405Z","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":"10.5281/zenodo.5229640","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T20:51:12.105978Z","title":null,"venue":null,"work_id":"e3022527-fe6e-4d38-be62-50ff7ac4fe98","year":2021},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.505875Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:216b441dc64d098f7001be8a3e11e7e8672826a061bbc0a2ed2dba9610cc0fb0","observation_id":"918d781b-27a8-40fb-b5ed-233fdc5905d0","resolution":{"observed_at":"2026-08-07T20:51:12.110771Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-07T20:51:11.510957Z","title":"2002, Discrete & Computational Geometry, 28, 511, doi:10.1007/s00454-002-2885-2","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.510957Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:752a8b201f6b36fbe85ac5750e565e83659081a810d9bfed7cd4c21ed215f1d2","observation_id":"f02fa8fb-b290-4cf2-a464-9c8d8e791f81","resolution":{"observed_at":"2026-08-07T20:51:11.510957Z","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":"2026-08-07T20:51:11.515589Z","title":"1983, IEEE Transactions on Information Theory, 29, 551, doi:10.1109/tit.1983.1056714","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.515589Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:7d1ec1cac62f0c0b28901ef2cba3feefca99c5155c17e6a3785902a90df39dce","observation_id":"40cdd9e5-e8fc-4c59-ba52-f44793ac0913","resolution":{"observed_at":"2026-08-07T20:51:11.515589Z","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":"4462.15663","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T20:51:12.492543Z","title":null,"venue":null,"work_id":"cde12d5e-e64d-433a-abde-237b1b3f9b7c","year":1994},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.520400Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:f93f78ac03d226b124dcbae8a018f6fc3347bbc3e444e34bfe380b774e54beb5","observation_id":"3ecf0788-a120-4715-adf0-a927cc91a9df","resolution":{"observed_at":"2026-08-07T20:51:12.500708Z","resolver_source":"raw_fallback","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-07T20:51:11.525786Z","title":"2019, MNRAS, 486, 1523, doi: 10.1093/mnras/stz908 —","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.525786Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:ae2aae632e413452a16641bd547a805e6d59e238d5f4075ffdd9795b6fad0a56","observation_id":"fe510432-17c6-4d4e-98c0-09ad74a95613","resolution":{"observed_at":"2026-08-07T20:51:11.525786Z","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":"2026-08-07T20:51:11.530250Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.530250Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:b857b0a7f8e6518f44b6a2f2fcd2cedfdcbf572787364c19b9533595ab2e863c","observation_id":"a5b94375-6e04-41aa-9d0f-130d16c15cae","resolution":{"observed_at":"2026-08-07T20:51:11.530250Z","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":"2026-08-07T20:51:11.535221Z","title":"2025, arXiv e-prints, arXiv:2502.07713","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.535221Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:09705b54894ea492fca60329eec519ddf8c9751f3cbd8ed2c986f4ad28c09460","observation_id":"b123418a-0786-4372-a307-15032b9692ef","resolution":{"observed_at":"2026-08-07T20:51:11.535221Z","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":"2026-08-07T20:51:11.539694Z","title":"K., & Mellema, G","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.539694Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:f777217b34a04edcf9131492c53eb649d38d47d0612c5efb621eaef534282bfb","observation_id":"fef95770-0389-4be4-887f-534e1977e5e1","resolution":{"observed_at":"2026-08-07T20:51:11.539694Z","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":"2026-08-07T20:51:11.544294Z","title":"R., & Banerjee, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.544294Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:71773130ccf2dfaf8a5d11c132ed251a0f41d10ef275fb70c2a37ae0e4d49662","observation_id":"6aeb5a90-82fc-4884-8f88-670220614b29","resolution":{"observed_at":"2026-08-07T20:51:11.544294Z","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":"2026-08-07T20:51:11.549308Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.549308Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:55e74c046e08555922e44bdf0b21c0266dc425c9aae69ad2bbf2c80375e0ca2a","observation_id":"ddfd7a2e-6a0f-44b9-a337-952f571e9e98","resolution":{"observed_at":"2026-08-07T20:51:11.549308Z","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":"2026-08-07T20:51:11.554005Z","title":"R., Millman, K","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.554005Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:469e6b996ec54d1b627a4587a833cff97cf28983b60d6e66f3eaaec3fd7dca6b","observation_id":"b0207a80-f518-44bb-a636-e1c388085e02","resolution":{"observed_at":"2026-08-07T20:51:11.554005Z","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":"2026-08-07T20:51:11.558572Z","title":"2007, A&A, 464, 399, doi: 10.1051/0004-6361:20066170","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.558572Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:1cf41c43514150b1f84e3415ae327c7ab36633fe5c3b25d00b2e580f6d8441f9","observation_id":"5a24b0ae-affa-49c1-8d5f-0f2e835b6de1","resolution":{"observed_at":"2026-08-07T20:51:11.558572Z","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":"2026-08-07T20:51:11.563560Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.563560Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:38600e0c5a7638c115bc9c5b25a65b92540b9eadc087777ec2e7c56df6212d1e","observation_id":"9934ef5e-8629-47d3-aec3-1f10448e8c9f","resolution":{"observed_at":"2026-08-07T20:51:11.563560Z","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":"2026-08-07T20:51:11.568557Z","title":"2019, arXiv e-prints, arXiv:1910.13970, doi: 10.48550/arXiv.1910.13970","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.568557Z"},"links":{"cited_paper":"/paper/1910.13970","citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:87588084617b5533545f025d8c5ba85796f13bb4d2e4f416bc2a98494957f197","observation_id":"c7f53c85-b1f0-452e-a148-db760d622b16","resolution":{"observed_at":"2026-08-07T20:51:11.568557Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1506.08903","last_updated":"2017-09-12T14:10:44Z","snapshot_observed_at":"2026-07-06T04:22:23.546609Z","submitted_at":"2015-06-30T00:00:31Z","title":"A roadmap for the computation of persistent homology","version":7},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.08903","snapshot_observed_at":"2026-08-07T20:51:11.590442Z","title":"A., Tillmann, U., Grindrod, P., & Harrington, H","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.590442Z"},"links":{"cited_paper":"/paper/1506.08903","citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:cd20f13e72c85d0f89d468bb5b44b95b539806b10aa7a786d958c53330e30237","observation_id":"24d7ff9f-e4b9-4818-ba8d-5055629d15c8","resolution":{"observed_at":"2026-08-07T20:51:11.590442Z","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":"10.1093/mnras/stad1765","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T20:51:11.969723Z","title":"2023, MNRAS, 523, 5738, doi: 10.1093/mnras/stad1765","venue":null,"work_id":"cba27621-00cf-48ba-9e5a-ea4fca605b34","year":2023},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.611435Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:78b343cdfb26ad8ea4d8da349848a2919a9891d511a4842ef18b445b7ca7e7d6","observation_id":"bb9d69e3-08c2-4cac-a164-2bcbbc526fe0","resolution":{"observed_at":"2026-08-07T20:51:11.974197Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-07T20:51:11.620518Z","title":"2023, MNRAS, 522, 606, doi: 10.1093/mnras/stad1017","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.620518Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:1a596aff37e20c6b85f22d6d12f8e700f856898f6037b487408e547e9ee3eb70","observation_id":"cf9d1788-3879-42a4-b209-ee00fc4dbcca","resolution":{"observed_at":"2026-08-07T20:51:11.620518Z","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":"2026-08-07T20:51:11.629659Z","title":"2017, MNRAS, 465, 4281, doi:10.1093/mnras/stw2862","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.629659Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:6c85f011dbf7a19ecde4c4103f4ddaa29b829a0934578177be23a394d2ee4261","observation_id":"30d02232-670e-44ba-97d7-7b210c112dda","resolution":{"observed_at":"2026-08-07T20:51:11.629659Z","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":"10.1086/184398","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T20:51:11.935098Z","title":"S., & Turner, E","venue":null,"work_id":"4463d0e5-66db-492e-b6c3-42867d6a63f0","year":1984},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.637921Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:ad0836ade6525800675313168d90c20952da1a2cd310a6c6638e134ef9d78f3f","observation_id":"61292331-e5be-41ec-a3f2-f91eb0cbab2d","resolution":{"observed_at":"2026-08-07T20:51:11.939821Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-07T20:51:11.646661Z","title":"2006, Phys","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.646661Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:ba30fe1f7e20cd3151f62d0ca5200fb16d0a24448057b3ad6b130757d472530e","observation_id":"a9c5d847-fd04-4d3b-879d-0b25ab81900d","resolution":{"observed_at":"2026-08-07T20:51:11.646661Z","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":"2026-08-07T20:51:11.655619Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.655619Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:9a3be370f9616036557117ff502c4fd0a3bf696b7218abc2a8f2714c11bdeed3","observation_id":"98f63de4-0ff0-4c78-9f8c-ed27cdb117ab","resolution":{"observed_at":"2026-08-07T20:51:11.655619Z","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":"2026-08-07T20:51:11.660391Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.660391Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:6f8e3cbaa6193fcaebd03e6ccf3a0166e65cf6f5a42b922539335008aa125250","observation_id":"9928db11-c8fa-4cea-93e4-e5d8d0923202","resolution":{"observed_at":"2026-08-07T20:51:11.660391Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.10029","last_updated":"2024-12-19T18:31:41Z","snapshot_observed_at":"2026-07-06T16:48:41.065654Z","submitted_at":"2023-11-16T17:26:27Z","title":"On the evolution of Betti curves in the Cosmic web","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.10029","snapshot_observed_at":"2026-08-07T20:51:11.665583Z","title":"2023, arXiv e-prints, arXiv:2311.10029, doi:10.48550/arXiv.2311.10029 Uhlemann,C.,Friedrich,O.,Villaescusa-Navarro,F.,Banerjee,A.,&Codis, S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.665583Z"},"links":{"cited_paper":"/paper/2311.10029","citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:976295430c7e3d1b9e8567901c66049f38bf476f75686afb0a108dce4d0eb287","observation_id":"b80969c9-f776-413d-bb42-027f1c9cf8db","resolution":{"observed_at":"2026-08-07T20:51:11.665583Z","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":"2026-08-07T20:51:11.670395Z","title":"2022, Phys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.670395Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:cbc117f471c682bc0a505ea6ebbe9ead4c53f55cca0157452e4f84bc125f8838","observation_id":"2e345947-6109-49be-8db7-cc405aca3e42","resolution":{"observed_at":"2026-08-07T20:51:11.670395Z","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":"10.1007/978-3-642-25249-5_3","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T00:03:45.533247Z","title":"6970, 60–101, doi:10.1007/978-3-642-25249-5_3","venue":"Lecture notes in computer science","work_id":"5e746f4d-b689-4da9-869b-5c26ec36df86","year":null},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.675177Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:d4c99b38e203d3accb899c327d24ef30aa27d72db5a17a7fc8220b23eaf06c5f","observation_id":"d3cdd62a-1626-46ac-bc76-4677de645dd1","resolution":{"observed_at":"2026-08-07T20:51:11.870130Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-07T20:51:11.679828Z","title":"2020, ApJS, 250, 2, doi: 10.3847/1538-4365/ab9d82","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.679828Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:77b8cbc118a12592fe0c2a83658a7126f5c5f508e6137151e38de95a2de8d8e2","observation_id":"d1496a74-c4b4-44bd-a74e-06ddfc3017df","resolution":{"observed_at":"2026-08-07T20:51:11.679828Z","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":"10.1093/mnras/stac1551","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T20:51:11.840561Z","title":"2022, MNRAS, 514, 3828, doi: 10.1093/mnras/stac1551","venue":null,"work_id":"f7b2ff2c-0bdd-4486-8d08-174f418b5d4f","year":2022},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.684209Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:2b40c42f44bda7edf8608f06e4ef538c4709066f07cc0efb338f0c4c398cfb4d","observation_id":"f75377d0-cd1d-4f58-a009-5d46d9a4f748","resolution":{"observed_at":"2026-08-07T20:51:11.845812Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevd.111.l041302","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T20:51:11.824224Z","title":"2025, Phys","venue":null,"work_id":"316d0af3-3c6e-4e36-80b5-6dcf2f067235","year":2025},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.688943Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:a30e0e04253910474eb607be73ff45814bf04094e80d343b9fe8a90878b8d88f","observation_id":"5d2b377a-9929-426a-9bb9-638b44f511ee","resolution":{"observed_at":"2026-08-07T20:51:11.829490Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-07T20:51:11.693458Z","title":"2021, MNRAS, 507, 2968, doi:10.1093/mnras/stab2326","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.693458Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:6ac918346d803bc2c1645dfba111656e20488f33dc9ee3d545914778b4beb390","observation_id":"83b24e3e-d3ba-4655-87da-8a9720f1a88e","resolution":{"observed_at":"2026-08-07T20:51:11.693458Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.06067","last_updated":"2024-06-10T07:22:59Z","snapshot_observed_at":"2026-07-06T18:27:58.433967Z","submitted_at":"2024-06-10T07:22:59Z","title":"Fisher's Mirage: Noise Tightening of Cosmological Constraints in Simulation-Based Inference","version":1},"cited_work":{"arxiv_id":"2406.06067","doi":"10.48550/arxiv.2406.06067","metadata_source":"pith","pith_arxiv_id":"2406.06067","snapshot_observed_at":"2026-08-08T00:16:16.039225Z","title":"Fisher's Mirage: Noise Tightening of Cosmological Constraints in Simulation-Based Inference","venue":"astro-ph.CO","work_id":"bd3b6900-1464-47fa-b765-35127bdb92c3","year":2024},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.697992Z"},"links":{"cited_paper":"/paper/2406.06067","citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:495a3a0aca6b4d45c198f412c57aa52a5b5092ea37a4facc36ee74cda276bc15","observation_id":"20edb78c-23d6-4020-983b-4b95a3bc55ad","resolution":{"observed_at":"2026-08-07T20:51:11.802856Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/1475-7516/2024/09/034","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T20:51:11.774032Z","title":null,"venue":null,"work_id":"4e52a3bf-613c-4cba-a4b7-6ed272519eff","year":2024},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.702952Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:dc908559eb19a5f12aec0b1763b4f28ecd10243a0ca9f080da50bf0c30b3c67f","observation_id":"71c7f254-700a-4ae5-98fd-76357277d993","resolution":{"observed_at":"2026-08-07T20:51:11.779518Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-07T20:51:11.707224Z","title":"2023, MNRAS, 522, 3935, doi: 10.1093/mnras/stad1275","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.707224Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:18e029852ba02ac1abea304fd6db02b06edd7b18eb59124cee324f1ef713ea4c","observation_id":"ec5156c4-cd04-494e-9944-02e8922c0c2a","resolution":{"observed_at":"2026-08-07T20:51:11.707224Z","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":"10.3847/1538-4357/ad924c","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T20:51:11.744462Z","title":"2025, ApJ, 979, 194, doi: 10.3847/1538-4357/ad924c APPENDIX A","venue":null,"work_id":"1d25b162-877b-4e30-8082-abc834e27341","year":2023},"citing_paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-07T20:51:11.711685Z"},"links":{"citing_paper":"/paper/2502.09709"},"observation_digest":"sha256:8fbd6443cd1be560be8b914ec3f9de54f0a44f42602bf18a34d4f37fc57e7c34","observation_id":"4a4eb0b8-5640-4ea8-afda-94d8ef50ff39","resolution":{"observed_at":"2026-08-07T20:51:11.751090Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2502.09709","last_updated":"2025-02-25T20:51:05Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-09T04:29:49.012476Z","submitted_at":"2025-02-13T19:00:30Z","title":"Cosmological information content of Betti curves and $k$-nearest neighbor distributions"},"reference_resolution":{"displayed":46,"state_counts":{"malformed_identifier":0,"metadata_mismatch":2,"parse_uncertain":0,"unresolved":34,"verified_exact":10,"verified_fuzzy":0},"total_outbound_references":46},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 46 of 46 outbound references and 1 inbound Pith citation observation for arXiv:2502.09709."}