{"as_of":"2026-08-09T11:21:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4b6bcfe541440d546c3e471935173c26ab6d568123f135dd10cfcf75b2f95d04","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":12,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":12,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":12,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":12,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T22:50:01.427176Z","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":3,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2404.07249","last_updated":"2025-07-14T08:22:56Z","snapshot_observed_at":"2026-07-06T17:58:25.894552Z","submitted_at":"2024-04-10T18:00:00Z","title":"PolyBin3D: A Suite of Optimal and Efficient Power Spectrum and Bispectrum Estimators for Large-Scale Structure","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07249","snapshot_observed_at":"2026-08-08T22:50:01.427176Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04434","last_updated":"2025-05-28T18:15:24Z","snapshot_observed_at":"2026-08-09T06:41:30.647303Z","submitted_at":"2025-02-06T19:00:00Z","title":"Searching for Inflationary Physics with the CMB Trispectrum: 1. Primordial Theory & Optimal Estimators","version":3},"reference_index":218,"source":"pdf_text","source_observed_at":"2026-08-08T22:50:01.427176Z"},"links":{"cited_paper":"/paper/2404.07249","citing_paper":"/paper/2502.04434"},"observation_digest":"sha256:4047bade8d3194ea12a7233ba4ce58749365a753bf72694c26f853531cc91a65","observation_id":"7403a225-2191-43fa-b6c3-aa3942ff6505","resolution":{"observed_at":"2026-08-08T22:50:01.427176Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07249","last_updated":"2025-07-14T08:22:56Z","snapshot_observed_at":"2026-07-06T17:58:25.894552Z","submitted_at":"2024-04-10T18:00:00Z","title":"PolyBin3D: A Suite of Optimal and Efficient Power Spectrum and Bispectrum Estimators for Large-Scale Structure","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07249","snapshot_observed_at":"2026-08-08T20:05:19.673602Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.05258","last_updated":"2025-05-28T20:04:21Z","snapshot_observed_at":"2026-08-09T04:36:11.649820Z","submitted_at":"2025-02-07T19:00:00Z","title":"Searching for Inflationary Physics with the CMB Trispectrum: 2. Code & Validation","version":3},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-08T20:05:19.673602Z"},"links":{"cited_paper":"/paper/2404.07249","citing_paper":"/paper/2502.05258"},"observation_digest":"sha256:14989b49b5f36a3e9528dec3d9ff39c059af52b4cb18f3030825cd4269249148","observation_id":"e3e7ce49-16f2-423a-8e8c-cffca238c379","resolution":{"observed_at":"2026-08-08T20:05:19.673602Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07249","last_updated":"2025-07-14T08:22:56Z","snapshot_observed_at":"2026-07-06T17:58:25.894552Z","submitted_at":"2024-04-10T18:00:00Z","title":"PolyBin3D: A Suite of Optimal and Efficient Power Spectrum and Bispectrum Estimators for Large-Scale Structure","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07249","snapshot_observed_at":"2026-08-08T14:22:19.803486Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.06931","last_updated":"2025-05-28T18:18:25Z","snapshot_observed_at":"2026-08-08T18:55:41.963312Z","submitted_at":"2025-02-10T19:00:00Z","title":"Searching for Inflationary Physics with the CMB Trispectrum: 3. Constraints from Planck","version":3},"reference_index":116,"source":"pdf_text","source_observed_at":"2026-08-08T14:22:19.803486Z"},"links":{"cited_paper":"/paper/2404.07249","citing_paper":"/paper/2502.06931"},"observation_digest":"sha256:93de22b4b0d150ff85c6fc4e53b0022fa1af68fd75c4a521540f0453714c41cd","observation_id":"ce53d17a-dae4-41d9-ad08-9a0796d6e070","resolution":{"observed_at":"2026-08-08T14:22:19.803486Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07249","last_updated":"2025-07-14T08:22:56Z","snapshot_observed_at":"2026-07-06T17:58:25.894552Z","submitted_at":"2024-04-10T18:00:00Z","title":"PolyBin3D: A Suite of Optimal and Efficient Power Spectrum and Bispectrum Estimators for Large-Scale Structure","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07249","snapshot_observed_at":"2026-08-06T12:12:39.961305Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.22110","last_updated":"2026-07-22T14:21:38Z","snapshot_observed_at":"2026-08-08T09:47:30.240488Z","submitted_at":"2025-07-29T18:00:00Z","title":"One-Loop Galaxy Bispectrum: Consistent Theory, Efficient Analysis with COBRA, and Implications for Cosmological Parameters","version":4},"reference_index":125,"source":"pdf_text","source_observed_at":"2026-08-06T12:12:39.961305Z"},"links":{"cited_paper":"/paper/2404.07249","citing_paper":"/paper/2507.22110"},"observation_digest":"sha256:04387a29f538f1aeb0869864517894d9a4cff14ac5c101470f877637cb92b1b1","observation_id":"686f947b-c528-4ab6-b57d-b07c446fa5c2","resolution":{"observed_at":"2026-08-06T12:12:39.961305Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07249","last_updated":"2025-07-14T08:22:56Z","snapshot_observed_at":"2026-07-06T17:58:25.894552Z","submitted_at":"2024-04-10T18:00:00Z","title":"PolyBin3D: A Suite of Optimal and Efficient Power Spectrum and Bispectrum Estimators for Large-Scale Structure","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07249","snapshot_observed_at":"2026-08-04T11:02:33.090418Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2510.07375","last_updated":"2026-05-22T19:00:07Z","snapshot_observed_at":"2026-08-04T11:02:23.348972Z","submitted_at":"2025-10-08T18:00:00Z","title":"Control variates from Eulerian and Lagrangian perturbation theory: Application to the bispectrum","version":2},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-04T11:02:33.090418Z"},"links":{"cited_paper":"/paper/2404.07249","citing_paper":"/paper/2510.07375"},"observation_digest":"sha256:8babded70a6c02634fa4a98add2e69e996ffbd5b52a0c2eae740e45d68305150","observation_id":"4662282f-a8b6-48ad-9d62-8feb0d0f8c48","resolution":{"observed_at":"2026-08-04T11:02:33.090418Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07249","last_updated":"2025-07-14T08:22:56Z","snapshot_observed_at":"2026-07-06T17:58:25.894552Z","submitted_at":"2024-04-10T18:00:00Z","title":"PolyBin3D: A Suite of Optimal and Efficient Power Spectrum and Bispectrum Estimators for Large-Scale Structure","version":3},"cited_work":{"arxiv_id":"2404.07249","doi":"10.48550/arxiv.2404.07249","metadata_source":"arxiv_reference","pith_arxiv_id":"2404.07249","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"650d9085-bd0a-42f0-9112-01542a9d2684","year":2024},"citing_paper":{"arxiv_id":"2511.20757","last_updated":"2026-04-14T17:58:15Z","snapshot_observed_at":"2026-07-06T22:36:59.311174Z","submitted_at":"2025-11-25T19:00:04Z","title":"Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses","version":2},"reference_index":122,"source":"pdf_text","source_observed_at":"2026-05-17T04:15:18.730245Z"},"links":{"cited_paper":"/paper/2404.07249","citing_paper":"/paper/2511.20757"},"observation_digest":"sha256:41b740cdd585b984f9a070c0e3cc00e99090571cafc75a02f11bb04e7e4b7a8e","observation_id":"ed0e77a5-7076-4b1d-821d-122a4b407aa6","resolution":{"observed_at":"2026-05-17T04:19:01.043412Z","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":"2404.07249","last_updated":"2025-07-14T08:22:56Z","snapshot_observed_at":"2026-07-06T17:58:25.894552Z","submitted_at":"2024-04-10T18:00:00Z","title":"PolyBin3D: A Suite of Optimal and Efficient Power Spectrum and Bispectrum Estimators for Large-Scale Structure","version":3},"cited_work":{"arxiv_id":"2404.07249","doi":"10.48550/arxiv.2404.07249","metadata_source":"arxiv_reference","pith_arxiv_id":"2404.07249","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"650d9085-bd0a-42f0-9112-01542a9d2684","year":2024},"citing_paper":{"arxiv_id":"2604.18581","last_updated":"2026-04-20T17:59:34Z","snapshot_observed_at":"2026-08-02T18:55:32.863776Z","submitted_at":"2026-04-20T17:59:34Z","title":"If at First You Don't Succeed, Trispectrum: I. Estimating the Matter Power Spectrum Covariance with Higher-Order Statistics","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-05-10T03:22:25.185479Z"},"links":{"cited_paper":"/paper/2404.07249","citing_paper":"/paper/2604.18581"},"observation_digest":"sha256:df3aa9ea06eba1d2c683698541b3a59d0daf33be11c60b1628a6c99b9be39ff1","observation_id":"cd3803a7-7e4a-4690-bb61-183bc2ad5696","resolution":{"observed_at":"2026-05-11T12:31:06.952625Z","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":"2404.07249","last_updated":"2025-07-14T08:22:56Z","snapshot_observed_at":"2026-07-06T17:58:25.894552Z","submitted_at":"2024-04-10T18:00:00Z","title":"PolyBin3D: A Suite of Optimal and Efficient Power Spectrum and Bispectrum Estimators for Large-Scale Structure","version":3},"cited_work":{"arxiv_id":"2404.07249","doi":"10.48550/arxiv.2404.07249","metadata_source":"arxiv_reference","pith_arxiv_id":"2404.07249","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"650d9085-bd0a-42f0-9112-01542a9d2684","year":2024},"citing_paper":{"arxiv_id":"2606.19452","last_updated":"2026-06-17T18:00:08Z","snapshot_observed_at":"2026-07-06T23:54:46.974663Z","submitted_at":"2026-06-17T18:00:08Z","title":"Validation of the Hybrid Bias Expansion model for the galaxy bispectrum","version":1},"reference_index":116,"source":"arxiv_source","source_observed_at":"2026-06-26T19:39:44.745239Z"},"links":{"cited_paper":"/paper/2404.07249","citing_paper":"/paper/2606.19452"},"observation_digest":"sha256:a8021c718a428decb8ddd4fe7899b606dc3e6a47b37d5c835e2ad5d027ad2498","observation_id":"2ffe5c9e-a7c4-4fe0-aacb-54751037a759","resolution":{"observed_at":"2026-06-26T19:39:50.110159Z","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":"2404.07249","last_updated":"2025-07-14T08:22:56Z","snapshot_observed_at":"2026-07-06T17:58:25.894552Z","submitted_at":"2024-04-10T18:00:00Z","title":"PolyBin3D: A Suite of Optimal and Efficient Power Spectrum and Bispectrum Estimators for Large-Scale Structure","version":3},"cited_work":{"arxiv_id":"2404.07249","doi":"10.48550/arxiv.2404.07249","metadata_source":"arxiv_reference","pith_arxiv_id":"2404.07249","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"650d9085-bd0a-42f0-9112-01542a9d2684","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":198,"source":"arxiv_source","source_observed_at":"2026-06-26T01:35:05.451125Z"},"links":{"cited_paper":"/paper/2404.07249","citing_paper":"/paper/2606.26237"},"observation_digest":"sha256:7117bc7264a0ac4494320e6845acaae323d6a85f8793ca980567be60fec847e3","observation_id":"1e324aeb-7697-4dce-935f-3719acbd1474","resolution":{"observed_at":"2026-06-26T01:38:51.686865Z","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":"2404.07249","last_updated":"2025-07-14T08:22:56Z","snapshot_observed_at":"2026-07-06T17:58:25.894552Z","submitted_at":"2024-04-10T18:00:00Z","title":"PolyBin3D: A Suite of Optimal and Efficient Power Spectrum and Bispectrum Estimators for Large-Scale Structure","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07249","snapshot_observed_at":"2026-07-30T20:54:14.302261Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.23494","last_updated":"2026-07-26T06:49:56Z","snapshot_observed_at":"2026-08-07T16:30:07.735647Z","submitted_at":"2026-07-26T06:49:56Z","title":"Hermes - Towards an Optimal High-Performance Algorithm for Cosmic Statistics of Large Data Sets","version":1},"reference_index":246,"source":"arxiv_source","source_observed_at":"2026-07-30T20:54:14.302261Z"},"links":{"cited_paper":"/paper/2404.07249","citing_paper":"/paper/2607.23494"},"observation_digest":"sha256:c3a6bed788456825a47313ca2a6fb7010d41c155e018ca575e158c9c32467ed2","observation_id":"9fcc1ec2-9763-431b-882d-d22a77e9e780","resolution":{"observed_at":"2026-07-30T20:54:14.302261Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07249","last_updated":"2025-07-14T08:22:56Z","snapshot_observed_at":"2026-07-06T17:58:25.894552Z","submitted_at":"2024-04-10T18:00:00Z","title":"PolyBin3D: A Suite of Optimal and Efficient Power Spectrum and Bispectrum Estimators for Large-Scale Structure","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07249","snapshot_observed_at":"2026-07-31T07:10:45.714902Z","title":"Philcox and T","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.28445","last_updated":"2026-07-30T16:16:22Z","snapshot_observed_at":"2026-08-08T23:25:52.591944Z","submitted_at":"2026-07-30T16:16:22Z","title":"Inflation, Open Universes, and Dark Energy","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-07-31T07:10:45.714902Z"},"links":{"cited_paper":"/paper/2404.07249","citing_paper":"/paper/2607.28445"},"observation_digest":"sha256:a583591f8c0ae6a32ed4b9b1ffc1186d07ac7083ef6a27a9c46d8bff5aa5d797","observation_id":"5761fa71-ec68-4aa6-8301-4068d0257563","resolution":{"observed_at":"2026-07-31T07:10:45.714902Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07249","last_updated":"2025-07-14T08:22:56Z","snapshot_observed_at":"2026-07-06T17:58:25.894552Z","submitted_at":"2024-04-10T18:00:00Z","title":"PolyBin3D: A Suite of Optimal and Efficient Power Spectrum and Bispectrum Estimators for Large-Scale Structure","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07249","snapshot_observed_at":"2026-08-03T02:37:22.824624Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.29652","last_updated":"2026-07-31T17:29:15Z","snapshot_observed_at":"2026-08-09T05:00:22.379059Z","submitted_at":"2026-07-31T17:29:15Z","title":"An optimal quadratic estimator for window-free cosmic shear power spectra","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-03T02:37:22.824624Z"},"links":{"cited_paper":"/paper/2404.07249","citing_paper":"/paper/2607.29652"},"observation_digest":"sha256:e8e355c8446c47eb51fa5e6cfb0e95a5df0dbbbfe41d65da8e31cd351e951fb5","observation_id":"a4a619b8-c15c-4adc-b232-d75f4f56582e","resolution":{"observed_at":"2026-08-03T02:37:22.824624Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2404.07249/citation-record","integrity":"/paper/2404.07249/integrity","json":"/paper/2404.07249/citation-record.json","paper":"/paper/2404.07249"},"outbound":[],"paper":{"arxiv_id":"2404.07249","last_updated":"2025-07-14T08:22:56Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T17:58:25.894552Z","submitted_at":"2024-04-10T18:00:00Z","title":"PolyBin3D: A Suite of Optimal and Efficient Power Spectrum and Bispectrum Estimators for Large-Scale Structure"},"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 12 inbound Pith citation observations for arXiv:2404.07249."}