{"as_of":"2026-08-09T07:24:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:928c15008517e304e235c56dbac8b683e2b4523a967a78ba732730a7e8f8149d","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":18,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":18,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":18,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":18,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-09T04:39:47.184947Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":5,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03220","snapshot_observed_at":"2026-08-09T04:39:47.184947Z","title":"2024, How much information can be extracted from galaxy clustering at the field level?, arXiv, 10.48550/ARXIV.2403.03220","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.03522","last_updated":"2025-05-06T22:06:44Z","snapshot_observed_at":"2026-08-09T04:34:16.246096Z","submitted_at":"2025-02-05T19:00:01Z","title":"Towards characterizing dark matter subhalo perturbations in stellar streams with graph neural networks","version":2},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-09T04:39:47.184947Z"},"links":{"cited_paper":"/paper/2403.03220","citing_paper":"/paper/2502.03522"},"observation_digest":"sha256:e81e7ae3bb0526fdf5b0cc702fdbf6638e481c75a1d31cad811e1f320a2837e3","observation_id":"dace2466-9200-4180-9b92-17b4ea7677ea","resolution":{"observed_at":"2026-08-09T04:39:47.184947Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03220","snapshot_observed_at":"2026-08-07T05:50:31.640171Z","title":"Nguyen, F","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.07105","last_updated":"2025-06-08T12:28:15Z","snapshot_observed_at":"2026-08-07T11:22:48.926743Z","submitted_at":"2025-06-08T12:28:15Z","title":"Renormalized Perturbation Theory at Field-level: the LSS bootstrap in GridSPT","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-07T05:50:31.640171Z"},"links":{"cited_paper":"/paper/2403.03220","citing_paper":"/paper/2506.07105"},"observation_digest":"sha256:741243b5e7ec04af262ca55c17c0b0149bb683d5f4d71d7a95df47776e212592","observation_id":"3150e3df-53c9-4c47-8e76-56f8dce1a98d","resolution":{"observed_at":"2026-08-07T05:50:31.640171Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03220","snapshot_observed_at":"2026-08-06T21:30:54.695470Z","title":"Nguyen, F","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.00118","last_updated":"2025-06-30T18:00:01Z","snapshot_observed_at":"2026-08-08T17:58:16.664935Z","submitted_at":"2025-06-30T18:00:01Z","title":"Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.695470Z"},"links":{"cited_paper":"/paper/2403.03220","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:23aa7cf70e48d3db36c28eada38a02e63cd7b51631cbb09a6d4508b99c4a5959","observation_id":"c7e36254-7807-48ed-b316-6b70830a3760","resolution":{"observed_at":"2026-08-06T21:30:54.695470Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03220","snapshot_observed_at":"2026-08-06T21:27:24.786013Z","title":"Nguyen, F","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.00284","last_updated":"2025-06-30T21:53:00Z","snapshot_observed_at":"2026-08-08T11:20:44.619645Z","submitted_at":"2025-06-30T21:53:00Z","title":"Modeling the Cosmological Lyman-$\\alpha$ Forest at the Field Level","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-06T21:27:24.786013Z"},"links":{"cited_paper":"/paper/2403.03220","citing_paper":"/paper/2507.00284"},"observation_digest":"sha256:7edc88aea1229b10c33926460045f5bb2158814a10c9c86bb7c302743c5c3b0d","observation_id":"06008e1c-5177-4962-99da-7291c759b23a","resolution":{"observed_at":"2026-08-06T21:27:24.786013Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03220","snapshot_observed_at":"2026-08-06T19:34:06.286855Z","title":"Nguyen, F","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.05378","last_updated":"2025-07-07T18:04:52Z","snapshot_observed_at":"2026-08-09T03:49:44.593476Z","submitted_at":"2025-07-07T18:04:52Z","title":"Equivalence of the field-level inference and conventional analyses on large scales","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T19:34:06.286855Z"},"links":{"cited_paper":"/paper/2403.03220","citing_paper":"/paper/2507.05378"},"observation_digest":"sha256:c4fa737118419647422609521a0c436b226fea362ba3041e0064fcfaef0cc9f3","observation_id":"c6502973-84ab-49ce-8fdd-42e11359b7f0","resolution":{"observed_at":"2026-08-06T19:34:06.286855Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03220","snapshot_observed_at":"2026-08-06T16:23:47.257707Z","title":"Nguyen, F","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.13905","last_updated":"2026-07-09T05:53:14Z","snapshot_observed_at":"2026-08-06T18:12:48.063812Z","submitted_at":"2025-07-18T13:35:35Z","title":"Two-loop renormalization and running of galaxy bias","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T16:23:47.257707Z"},"links":{"cited_paper":"/paper/2403.03220","citing_paper":"/paper/2507.13905"},"observation_digest":"sha256:f210e465f7f66e7116bf7e9f6227beefecaf486d0a95028deedbd4dc5b5bfed4","observation_id":"f34d5994-1dcb-41f1-9594-415c438d8c65","resolution":{"observed_at":"2026-08-06T16:23:47.257707Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03220","snapshot_observed_at":"2026-08-06T13:22:38.718671Z","title":"Nguyen, F","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.20991","last_updated":"2025-07-28T16:50:33Z","snapshot_observed_at":"2026-08-07T01:20:31.920144Z","submitted_at":"2025-07-28T16:50:33Z","title":"Debiasing inference in large-scale structure with non-flat volume measures","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-06T13:22:38.718671Z"},"links":{"cited_paper":"/paper/2403.03220","citing_paper":"/paper/2507.20991"},"observation_digest":"sha256:0f170b727369d8c4d4954739dbe82dd991d1bd3dff8b82f4f40506539871b555","observation_id":"d90bad49-25c2-4bec-8921-e998727c9d9f","resolution":{"observed_at":"2026-08-06T13:22:38.718671Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03220","snapshot_observed_at":"2026-08-04T11:25:25.514689Z","title":"Nguyen, F","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2510.05206","last_updated":"2025-10-06T18:00:05Z","snapshot_observed_at":"2026-08-04T12:26:03.726898Z","submitted_at":"2025-10-06T18:00:05Z","title":"DISCO-DJ II: a differentiable particle-mesh code for cosmology","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-04T11:25:25.514689Z"},"links":{"cited_paper":"/paper/2403.03220","citing_paper":"/paper/2510.05206"},"observation_digest":"sha256:79e175f949ab76a48fa1b35834ee78f16ac28ca1ec6ec1cba82fe6483cf18864","observation_id":"8f6a79a9-ab29-4af4-ac5d-b8c7f2e70a3a","resolution":{"observed_at":"2026-08-04T11:25:25.514689Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03220","snapshot_observed_at":"2026-08-04T09:46:17.103168Z","title":"Nguyen, F","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2510.14089","last_updated":"2026-06-11T13:09:31Z","snapshot_observed_at":"2026-08-06T08:03:16.019106Z","submitted_at":"2025-10-15T20:49:30Z","title":"Field-level likelihood for projected fields: Evolved projected fields from initial projected fields","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-04T09:46:17.103168Z"},"links":{"cited_paper":"/paper/2403.03220","citing_paper":"/paper/2510.14089"},"observation_digest":"sha256:29831b94b8bb6d69545d54f7464aabe5954307c83d5270280e5f9c67bf44efff","observation_id":"d5aa0274-2149-4fc1-ada5-4c647561f743","resolution":{"observed_at":"2026-08-04T09:46:17.103168Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03220","snapshot_observed_at":"2026-08-03T23:38:16.829576Z","title":"Nguyen, F","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.05484","last_updated":"2026-07-08T12:26:06Z","snapshot_observed_at":"2026-08-08T02:35:05.707984Z","submitted_at":"2025-11-07T18:53:39Z","title":"Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-03T23:38:16.829576Z"},"links":{"cited_paper":"/paper/2403.03220","citing_paper":"/paper/2511.05484"},"observation_digest":"sha256:aebdecbb8bcfae0abcf23d725c11be8051deaf95828f9db973ea9f3aacccd1ff","observation_id":"d4e7a9a8-51f4-481e-80af-b2abf52747a2","resolution":{"observed_at":"2026-08-03T23:38:16.829576Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?","version":3},"cited_work":{"arxiv_id":"2403.03220","doi":"10.48550/arxiv.2403.03220","metadata_source":"arxiv_reference","pith_arxiv_id":"2403.03220","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Nguyen, F","venue":"arXiv (Cornell University)","work_id":"0a108a92-0c75-4bb1-b9c4-a29625ae3fbf","year":2024},"citing_paper":{"arxiv_id":"2604.25385","last_updated":"2026-04-28T08:51:44Z","snapshot_observed_at":"2026-07-31T06:02:57.362095Z","submitted_at":"2026-04-28T08:51:44Z","title":"On the Relation Between Field-Level Posteriors, Correlators, and their Likelihoods","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-07T15:04:42.546535Z"},"links":{"cited_paper":"/paper/2403.03220","citing_paper":"/paper/2604.25385"},"observation_digest":"sha256:9e2bca39142e94b276d5da3d48b6973cfcbe7e957e56ff12f8cad8123a2e7abc","observation_id":"033123f8-800a-4fd3-b280-7881265a5feb","resolution":{"observed_at":"2026-05-12T00:31:19.780960Z","resolver_source":"arxiv_id","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":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?","version":3},"cited_work":{"arxiv_id":"2403.03220","doi":"10.48550/arxiv.2403.03220","metadata_source":"arxiv_reference","pith_arxiv_id":"2403.03220","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Nguyen, F","venue":"arXiv (Cornell University)","work_id":"0a108a92-0c75-4bb1-b9c4-a29625ae3fbf","year":2024},"citing_paper":{"arxiv_id":"2605.13298","last_updated":"2026-05-13T10:12:06Z","snapshot_observed_at":"2026-08-03T01:12:04.794816Z","submitted_at":"2026-05-13T10:12:06Z","title":"Probing nonlinear structure formation beyond $\\Lambda$CDM with the LSS bootstrap: a joint power spectrum and bispectrum analysis","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-05-14T17:39:05.401310Z"},"links":{"cited_paper":"/paper/2403.03220","citing_paper":"/paper/2605.13298"},"observation_digest":"sha256:b9ab477bea22f10b4bfa5a2664e8169410bc8a47f3968d46ad576cace5f93b35","observation_id":"0b5e89fb-0412-4506-94f0-aa725eaf3b2b","resolution":{"observed_at":"2026-05-14T17:42:32.802578Z","resolver_source":"arxiv_id","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":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?","version":3},"cited_work":{"arxiv_id":"2403.03220","doi":"10.48550/arxiv.2403.03220","metadata_source":"arxiv_reference","pith_arxiv_id":"2403.03220","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Nguyen, F","venue":"arXiv (Cornell University)","work_id":"0a108a92-0c75-4bb1-b9c4-a29625ae3fbf","year":2024},"citing_paper":{"arxiv_id":"2606.18227","last_updated":"2026-06-16T17:53:06Z","snapshot_observed_at":"2026-08-06T20:33:40.369579Z","submitted_at":"2026-06-16T17:53:06Z","title":"Field-level vs summaries: convergence of information in non-Gaussian density fields","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-06-26T23:17:48.555984Z"},"links":{"cited_paper":"/paper/2403.03220","citing_paper":"/paper/2606.18227"},"observation_digest":"sha256:7ac1afba862333f72eb033f8d0bd6019815393c67cbd432826b266add6332e45","observation_id":"abf1f01f-267e-45f6-9bbe-546cb53b0aac","resolution":{"observed_at":"2026-07-03T22:49:01.233759Z","resolver_source":"arxiv_id","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":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?","version":3},"cited_work":{"arxiv_id":"2403.03220","doi":"10.48550/arxiv.2403.03220","metadata_source":"arxiv_reference","pith_arxiv_id":"2403.03220","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Nguyen, F","venue":"arXiv (Cornell University)","work_id":"0a108a92-0c75-4bb1-b9c4-a29625ae3fbf","year":2024},"citing_paper":{"arxiv_id":"2606.26234","last_updated":"2026-06-24T18:00:02Z","snapshot_observed_at":"2026-08-06T10:28:45.654237Z","submitted_at":"2026-06-24T18:00:02Z","title":"Lyman-Alpha Forest and its Cross-Correlation with High-Redshift Galaxies in Effective Field Theory at the Field Level","version":1},"reference_index":204,"source":"pdf_text","source_observed_at":"2026-06-26T01:38:09.398349Z"},"links":{"cited_paper":"/paper/2403.03220","citing_paper":"/paper/2606.26234"},"observation_digest":"sha256:cf91992f9d528fbc6b782a668c4e8565ee5f4dec4ad1160e83f8661c8c7d14a9","observation_id":"574ebee4-39cc-4e5b-b247-63a71700b921","resolution":{"observed_at":"2026-07-04T15:19:57.117120Z","resolver_source":"arxiv_id","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":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?","version":3},"cited_work":{"arxiv_id":"2403.03220","doi":"10.48550/arxiv.2403.03220","metadata_source":"arxiv_reference","pith_arxiv_id":"2403.03220","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Nguyen, F","venue":"arXiv (Cornell University)","work_id":"0a108a92-0c75-4bb1-b9c4-a29625ae3fbf","year":2024},"citing_paper":{"arxiv_id":"2606.26237","last_updated":"2026-06-24T18:00:03Z","snapshot_observed_at":"2026-07-07T00:00:36.766142Z","submitted_at":"2026-06-24T18:00:03Z","title":"First full-shape joint analysis of the two- and three-point correlation functions on real data: $\\Lambda$CDM cosmological constraints from BOSS DR12","version":1},"reference_index":227,"source":"arxiv_source","source_observed_at":"2026-06-26T01:35:05.451125Z"},"links":{"cited_paper":"/paper/2403.03220","citing_paper":"/paper/2606.26237"},"observation_digest":"sha256:fde22fcffbded22fe8f990f77e7de836705d15980e2fce9e16105db543fdd13d","observation_id":"526a854f-bb53-41b5-9f27-23181445859c","resolution":{"observed_at":"2026-06-26T01:38:51.631934Z","resolver_source":"arxiv_id","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":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03220","snapshot_observed_at":"2026-08-01T09:37:45.309457Z","title":"Nguyen, F","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.27320","last_updated":"2026-07-29T18:00:01Z","snapshot_observed_at":"2026-08-07T22:37:37.856422Z","submitted_at":"2026-07-29T18:00:01Z","title":"Emulating Cosmic Structure Formation with a Lagrangian Neural Cellular Automaton","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-01T09:37:45.309457Z"},"links":{"cited_paper":"/paper/2403.03220","citing_paper":"/paper/2607.27320"},"observation_digest":"sha256:6c4a3b75a19277183979ffc3ba18cd9c34733a1994ccf585aa7b8cf2748433d2","observation_id":"6660cf96-bacf-4e86-8ca2-7a3afb7b6a92","resolution":{"observed_at":"2026-08-01T09:37:45.309457Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03220","snapshot_observed_at":"2026-07-31T11:32:44.916759Z","title":"Nguyen, F","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.28314","last_updated":"2026-07-30T14:48:56Z","snapshot_observed_at":"2026-08-06T13:16:24.972090Z","submitted_at":"2026-07-30T14:48:56Z","title":"GGI Lectures on Large-Scale Structure Perturbation Theory (Effective Field Theory)","version":1},"reference_index":152,"source":"pdf_text","source_observed_at":"2026-07-31T11:32:44.916759Z"},"links":{"cited_paper":"/paper/2403.03220","citing_paper":"/paper/2607.28314"},"observation_digest":"sha256:f487d0dcd012ec5162aa8fa828edfd781244c5660b05ac4d7f9d3fe8eb762258","observation_id":"5a31f242-3922-43d3-bb19-0c17c92a6677","resolution":{"observed_at":"2026-07-31T11:32:44.916759Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03220","snapshot_observed_at":"2026-08-03T00:28:17.443304Z","title":"Nguyen, F","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.28800","last_updated":"2026-07-30T19:48:33Z","snapshot_observed_at":"2026-08-09T04:37:43.207204Z","submitted_at":"2026-07-30T19:48:33Z","title":"Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-03T00:28:17.443304Z"},"links":{"cited_paper":"/paper/2403.03220","citing_paper":"/paper/2607.28800"},"observation_digest":"sha256:f2380db41a230c52296ed868b764e234049afc7ab9cce20ab294e990c0d131e7","observation_id":"04236630-a759-48ba-9515-ff0ad903070a","resolution":{"observed_at":"2026-08-03T00:28:17.443304Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2403.03220/citation-record","integrity":"/paper/2403.03220/integrity","json":"/paper/2403.03220/citation-record.json","paper":"/paper/2403.03220"},"outbound":[],"paper":{"arxiv_id":"2403.03220","last_updated":"2024-10-03T11:15:51Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-08T18:23:44.506476Z","submitted_at":"2024-03-05T18:59:50Z","title":"How much information can be extracted from galaxy clustering at the field level?"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-09T06:31:02.800959+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 0 of 0 outbound references and 18 inbound Pith citation observations for arXiv:2403.03220."}