{"as_of":"2026-08-17T22:56:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4bdd1fcf27c2372eacf005e2633b02d04e0d362c08bdb0b24c7321062a12ccbe","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":21,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":21,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":21,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":21,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T05:21:13.817073Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-03T22:39:02.372255Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-08-12T15:18:36.691618Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.14377","last_updated":"2024-11-21T18:11:16Z","snapshot_observed_at":"2026-08-17T15:48:30.376900Z","submitted_at":"2024-11-21T18:11:16Z","title":"The constraining power of the Marked Power Spectrum: an analytical study","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:36.691618Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2411.14377"},"observation_digest":"sha256:506fb33ca18c65627f2387ff26bce8c42f58ffc9ecc89aafd65e489a08400a15","observation_id":"db314e6b-464e-4763-bcf9-b8796215d913","resolution":{"observed_at":"2026-08-12T15:18:36.691618Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-08-12T00:58:57.455339Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.01888","last_updated":"2024-12-02T19:00:00Z","snapshot_observed_at":"2026-08-14T21:45:40.519052Z","submitted_at":"2024-12-02T19:00:00Z","title":"The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field level","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-12T00:58:57.455339Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2412.01888"},"observation_digest":"sha256:506aa6b9489f02f756f532fc7c53d8947b1f58c155ff6d356de0e679c41becd0","observation_id":"5454feb0-fe86-4ebc-8fba-f53f6be674d9","resolution":{"observed_at":"2026-08-12T00:58:57.455339Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-08-09T22:58:53.424913Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.18597","last_updated":"2025-01-30T18:59:56Z","snapshot_observed_at":"2026-08-13T09:35:09.299544Z","submitted_at":"2025-01-30T18:59:56Z","title":"Boosting galaxy clustering analyses with non-perturbative modelling of redshift-space distortions","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-09T22:58:53.424913Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2501.18597"},"observation_digest":"sha256:ab24233be08269ad901236ed48255ddae9a1a4a5182a30a5bd77adf053e3af7e","observation_id":"303d960a-5157-49d7-b871-2e92fcacc1a4","resolution":{"observed_at":"2026-08-09T22:58:53.424913Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-08-09T11:45:58.353097Z","title":"Ivanov, O.H.E","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.02636","last_updated":"2025-05-31T03:47:43Z","snapshot_observed_at":"2026-08-13T09:35:13.775028Z","submitted_at":"2025-02-04T19:00:01Z","title":"Bounds on Velocity-Dependent Dark Matter-Baryon Scattering from Large-Scale Structure","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-09T11:45:58.353097Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2502.02636"},"observation_digest":"sha256:9451646883bd3505271920a5bc9a06b315df72bda14b524672db269e1364a174","observation_id":"c0b90d1a-e976-4520-82c3-1f05795eed82","resolution":{"observed_at":"2026-08-09T11:45:58.353097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-08-16T05:21:13.817073Z","title":"Ivanov, O.H.E","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.21133","last_updated":"2025-07-01T17:51:09Z","snapshot_observed_at":"2026-08-17T08:45:05.607427Z","submitted_at":"2025-04-29T19:28:30Z","title":"Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation","version":2},"reference_index":110,"source":"pdf_text","source_observed_at":"2026-08-16T05:21:13.817073Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2504.21133"},"observation_digest":"sha256:3f66dc5b525c4a68bbaa5b59184bbf85271bbb999d51db062a19c41e4317cebe","observation_id":"5c64460a-2850-4a9b-b5b7-8887b5eb30f1","resolution":{"observed_at":"2026-08-16T05:21:13.817073Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-08-06T21:30:54.755827Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.00118","last_updated":"2025-06-30T18:00:01Z","snapshot_observed_at":"2026-08-16T16:57:09.921790Z","submitted_at":"2025-06-30T18:00:01Z","title":"Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.755827Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:50d103507fcd95eb04be4da6179a173a1c5fd04b9b902595121ade0afae611fd","observation_id":"8a9bd3e4-f1f0-4674-81d4-7586b88a5637","resolution":{"observed_at":"2026-08-06T21:30:54.755827Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-08-06T19:34:09.991274Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.05378","last_updated":"2025-07-07T18:04:52Z","snapshot_observed_at":"2026-08-17T01:15:04.732221Z","submitted_at":"2025-07-07T18:04:52Z","title":"Equivalence of the field-level inference and conventional analyses on large scales","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-06T19:34:09.991274Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2507.05378"},"observation_digest":"sha256:9ee81209b781398752fb15feaa8b26af630acce7f8858c10eec815f7c98f0bc8","observation_id":"0cfe87ee-1d29-4d55-bc3d-e7349223b667","resolution":{"observed_at":"2026-08-06T19:34:09.991274Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-08-06T12:12:39.596318Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.22110","last_updated":"2026-07-22T14:21:38Z","snapshot_observed_at":"2026-08-14T05:12:23.733244Z","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":33,"source":"pdf_text","source_observed_at":"2026-08-06T12:12:39.596318Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2507.22110"},"observation_digest":"sha256:fc1748f589601787164ef6e78abe9d403369a61f8d4a8891e192d92c7e45ba19","observation_id":"510f0332-4ca9-4bfe-93fc-2e7ec57ff12b","resolution":{"observed_at":"2026-08-06T12:12:39.596318Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":"2110.10161","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-07-03T22:39:02.372255Z","title":"Ivanov, O.H.E","venue":null,"work_id":"d4632a43-ebf5-4f5d-9257-8925b0fdb7be","year":2022},"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":100,"source":"pdf_text","source_observed_at":"2026-05-17T04:15:18.730245Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2511.20757"},"observation_digest":"sha256:144f8fb6407f545b93131a8d88026208df3bc7f2fe8c4338a09203149c5a9c32","observation_id":"0bc5aeea-e095-4b3a-96b0-a664bd3a16b9","resolution":{"observed_at":"2026-05-17T04:19:01.056989Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-08-03T08:41:59.488301Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2601.16165","last_updated":"2026-07-22T13:53:51Z","snapshot_observed_at":"2026-08-12T12:58:30.592699Z","submitted_at":"2026-01-22T18:10:50Z","title":"Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy","version":2},"reference_index":108,"source":"pdf_text","source_observed_at":"2026-08-03T08:41:59.488301Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2601.16165"},"observation_digest":"sha256:8b912c51e247b71ffc7b13e85cd7ffc9294650f414a6eb06ed9e5b17b69e48fe","observation_id":"603f2147-d935-4810-b3fe-e5ce19dbe8e1","resolution":{"observed_at":"2026-08-03T08:41:59.488301Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-08-02T22:01:23.919562Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2602.18554","last_updated":"2026-07-18T17:18:40Z","snapshot_observed_at":"2026-08-10T05:21:31.758327Z","submitted_at":"2026-02-20T19:00:00Z","title":"Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-02T22:01:23.919562Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2602.18554"},"observation_digest":"sha256:ef3ab3115166b2d3f8a4d990c08192118d5b07456d7cc2043c45faad5eab3a51","observation_id":"6bccb82f-2ff4-4977-8054-1602e1c0b0c8","resolution":{"observed_at":"2026-08-02T22:01:23.919562Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":"2110.10161","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-07-03T22:39:02.372255Z","title":"Ivanov, O.H.E","venue":null,"work_id":"d4632a43-ebf5-4f5d-9257-8925b0fdb7be","year":2022},"citing_paper":{"arxiv_id":"2604.08895","last_updated":"2026-04-10T02:59:01Z","snapshot_observed_at":"2026-08-10T21:50:32.664752Z","submitted_at":"2026-04-10T02:59:01Z","title":"FolpsD: combining EFT and phenomenological approaches for joint power spectrum and bispectrum analyses","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-10T17:38:15.169909Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2604.08895"},"observation_digest":"sha256:b8a12936ff2b61ad1efeb9a32ac44c156b364ddf6fe3d934a267c01411a97e85","observation_id":"d5ab0973-1188-4451-8818-8804366b06a2","resolution":{"observed_at":"2026-05-11T06:26:00.102291Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":"2110.10161","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-07-03T22:39:02.372255Z","title":"Ivanov, O.H.E","venue":null,"work_id":"d4632a43-ebf5-4f5d-9257-8925b0fdb7be","year":2022},"citing_paper":{"arxiv_id":"2605.13298","last_updated":"2026-05-13T10:12:06Z","snapshot_observed_at":"2026-08-15T03:23:28.290442Z","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":25,"source":"pdf_text","source_observed_at":"2026-05-14T17:39:05.401310Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2605.13298"},"observation_digest":"sha256:45f05dcda3efea46ee24b12c3c39650a20f6e54a207d9a7e48a4e8efbe1cc5a6","observation_id":"b9afafc1-434d-4f2f-bf70-b6a886b3fc01","resolution":{"observed_at":"2026-05-14T17:42:32.867651Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":"2110.10161","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-07-03T22:39:02.372255Z","title":"Ivanov, O.H.E","venue":null,"work_id":"d4632a43-ebf5-4f5d-9257-8925b0fdb7be","year":2022},"citing_paper":{"arxiv_id":"2606.18227","last_updated":"2026-06-16T17:53:06Z","snapshot_observed_at":"2026-08-17T12:09:02.605268Z","submitted_at":"2026-06-16T17:53:06Z","title":"Field-level vs summaries: convergence of information in non-Gaussian density fields","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-06-26T23:17:48.555984Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2606.18227"},"observation_digest":"sha256:79e7b742da71a12cc3e1c6d78c297b411f6b2e6d6683eeb69b53f81a473da746","observation_id":"536edf6f-a16d-4858-bc6d-cbeff00a973f","resolution":{"observed_at":"2026-07-03T22:39:02.373626Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":"2110.10161","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-07-03T22:39:02.372255Z","title":"Ivanov, O.H.E","venue":null,"work_id":"d4632a43-ebf5-4f5d-9257-8925b0fdb7be","year":2022},"citing_paper":{"arxiv_id":"2606.28172","last_updated":"2026-06-26T15:04:26Z","snapshot_observed_at":"2026-07-07T00:02:18.989389Z","submitted_at":"2026-06-26T15:04:26Z","title":"Searching for primordial features with radio surveys: synergy between the power spectrum and bispectrum","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-06-29T02:50:45.187677Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2606.28172"},"observation_digest":"sha256:45a34ac43fc2ba6965accd18841fc9526572116cfead48ab74c70274096c9fd3","observation_id":"7f2d7b6e-6f13-42eb-b3eb-6ba150c78841","resolution":{"observed_at":"2026-07-01T17:55:52.079779Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":"2110.10161","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-07-03T22:39:02.372255Z","title":"Ivanov, O.H.E","venue":null,"work_id":"d4632a43-ebf5-4f5d-9257-8925b0fdb7be","year":2022},"citing_paper":{"arxiv_id":"2606.30713","last_updated":"2026-06-29T18:00:00Z","snapshot_observed_at":"2026-08-16T03:32:37.297820Z","submitted_at":"2026-06-29T18:00:00Z","title":"Galaxy Power Spectrum at Two-Loop Order: Implications for Weak Lensing Surveys and New Physics","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-07-01T02:01:27.807230Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2606.30713"},"observation_digest":"sha256:87aad63b6ec7abba345ab192f7c826891891234b2ee350203409984824e9b9f7","observation_id":"a99cd51b-fd48-458f-a9f3-4a2326594d7e","resolution":{"observed_at":"2026-07-01T12:35:43.533954Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-07-12T03:43:52.393274Z","title":"and Philcox, Oliver H","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.03259","last_updated":"2026-07-03T12:21:14Z","snapshot_observed_at":"2026-08-08T08:24:39.969103Z","submitted_at":"2026-07-03T12:21:14Z","title":"Cosmology with HI Intensity Mapping","version":1},"reference_index":196,"source":"arxiv_source","source_observed_at":"2026-07-12T03:43:52.393274Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2607.03259"},"observation_digest":"sha256:38537316fcb781c36a93ad11eb274a68351463154ded41990e7c0f097e62a678","observation_id":"627bb312-0444-40e8-9a2f-0715b80d031a","resolution":{"observed_at":"2026-07-12T03:43:52.393274Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-07-14T14:25:37.540627Z","title":"and Nishimichi, Takahiro and Simonovic, Marko and Takada, Masahiro and Zaldarriaga, Matias , doi =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.09943","last_updated":"2026-07-15T12:28:21Z","snapshot_observed_at":"2026-08-15T03:18:58.160434Z","submitted_at":"2026-07-10T19:49:34Z","title":"Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations","version":1},"reference_index":120,"source":"arxiv_source","source_observed_at":"2026-07-14T14:25:37.540627Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2607.09943"},"observation_digest":"sha256:ad4f40841b6f181c72d5d5df352a6f67df7d150ef8f008f7d66f97d86f13d233","observation_id":"0742187e-4456-4179-a019-6959fe5dbf78","resolution":{"observed_at":"2026-07-14T14:25:37.540627Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-08-02T07:32:53.807697Z","title":"and Nishimichi, Takahiro and Simonovic, Marko and Takada, Masahiro and Zaldarriaga, Matias , doi =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.09943","last_updated":"2026-07-15T12:28:21Z","snapshot_observed_at":"2026-08-15T03:18:58.160434Z","submitted_at":"2026-07-10T19:49:34Z","title":"Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations","version":2},"reference_index":126,"source":"arxiv_source","source_observed_at":"2026-08-02T07:32:53.807697Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2607.09943"},"observation_digest":"sha256:88df75bc616b7d82d4201d835d4845f9bda4d4b085798637ed0fffc305a0204e","observation_id":"a4cc534b-0e13-4851-b4ef-ff6d7c2de32a","resolution":{"observed_at":"2026-08-02T07:32:53.807697Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-08-01T23:46:15.487953Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.15337","last_updated":"2026-07-16T18:00:25Z","snapshot_observed_at":"2026-08-16T02:56:24.477375Z","submitted_at":"2026-07-16T18:00:25Z","title":"Searching for Folded Primordial Non-Gaussianity with Galaxy Surveys","version":1},"reference_index":104,"source":"pdf_text","source_observed_at":"2026-08-01T23:46:15.487953Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2607.15337"},"observation_digest":"sha256:e9d7753da3b77513fccd7cf6eb0e6825711fbeee6682accdaa4f64a8e2cc4d14","observation_id":"d3a03bbf-23b8-47e5-af35-bdda3e60358d","resolution":{"observed_at":"2026-08-01T23:46:15.487953Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.10161","snapshot_observed_at":"2026-07-31T07:10:45.668532Z","title":"Ivanov, O.H.E","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.28445","last_updated":"2026-07-30T16:16:22Z","snapshot_observed_at":"2026-08-16T01:36:52.922280Z","submitted_at":"2026-07-30T16:16:22Z","title":"Inflation, Open Universes, and Dark Energy","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-07-31T07:10:45.668532Z"},"links":{"cited_paper":"/paper/2110.10161","citing_paper":"/paper/2607.28445"},"observation_digest":"sha256:80e0909364db51d6fdfd56efd4792169c6289f6f019d44e1d38eb0ed55e3ca4b","observation_id":"a52039c8-980a-47cf-bf95-b752ca412b03","resolution":{"observed_at":"2026-07-31T07:10:45.668532Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2110.10161/citation-record","integrity":"/paper/2110.10161/integrity","json":"/paper/2110.10161/citation-record.json","paper":"/paper/2110.10161"},"outbound":[],"paper":{"arxiv_id":"2110.10161","last_updated":"2021-10-19T18:00:00Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-17T21:55:55.915555Z","submitted_at":"2021-10-19T18:00:00Z","title":"Precision analysis of the redshift-space galaxy bispectrum"},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 21 inbound Pith citation observations for arXiv:2110.10161."}