{"as_of":"2026-08-08T03:04:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2082903d7b47053a22569b6759caaa2eb7ce48169ffad51efb31d5caea0db38b","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":8,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":8,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T05:50:31.557827Z","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":"2026-06-29T16:33:39.588072Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2108.07821","last_updated":"2022-05-18T19:27:13Z","snapshot_observed_at":"2026-07-06T11:39:06.926826Z","submitted_at":"2021-08-17T18:00:04Z","title":"Towards an Optimal Estimation of Cosmological Parameters with the Wavelet Scattering Transform","version":2},"cited_work":{"arxiv_id":"2108.07821","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2108.07821","snapshot_observed_at":"2026-06-29T16:33:39.588072Z","title":"Valogiannis and C","venue":null,"work_id":"4ea8b98d-6ba1-4d67-9271-ded98c63070c","year":2022},"citing_paper":{"arxiv_id":"2411.14748","last_updated":"2026-04-22T18:02:29Z","snapshot_observed_at":"2026-08-04T02:59:48.283737Z","submitted_at":"2024-11-22T05:53:46Z","title":"Cosmological Analysis with Calibrated Neural Quantile Estimation and Approximate Simulators","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-23T16:42:50.485680Z"},"links":{"cited_paper":"/paper/2108.07821","citing_paper":"/paper/2411.14748"},"observation_digest":"sha256:cedaceb285be3848614383c5246c2b1ef2163e092142bf87b7d00e1c1ace2d62","observation_id":"8254db5e-490d-41c9-81c9-6a1139b20655","resolution":{"observed_at":"2026-05-23T16:43:11.342960Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.07821","last_updated":"2022-05-18T19:27:13Z","snapshot_observed_at":"2026-07-06T11:39:06.926826Z","submitted_at":"2021-08-17T18:00:04Z","title":"Towards an Optimal Estimation of Cosmological Parameters with the Wavelet Scattering Transform","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.07821","snapshot_observed_at":"2026-08-07T05:50:31.557827Z","title":"Valogiannis and C","venue":null,"work_id":null,"year":2022},"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":15,"source":"pdf_text","source_observed_at":"2026-08-07T05:50:31.557827Z"},"links":{"cited_paper":"/paper/2108.07821","citing_paper":"/paper/2506.07105"},"observation_digest":"sha256:c2d3b2e86693529b1d58f55f9750e45dc748449805eb8b500e64f014d5220fdf","observation_id":"e69fe954-6c87-4b7d-ba68-f8e43fed892a","resolution":{"observed_at":"2026-08-07T05:50:31.557827Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.07821","last_updated":"2022-05-18T19:27:13Z","snapshot_observed_at":"2026-07-06T11:39:06.926826Z","submitted_at":"2021-08-17T18:00:04Z","title":"Towards an Optimal Estimation of Cosmological Parameters with the Wavelet Scattering Transform","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.07821","snapshot_observed_at":"2026-08-06T20:24:55.911486Z","title":"Valogiannis and C","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.03086","last_updated":"2025-07-03T18:01:03Z","snapshot_observed_at":"2026-08-06T20:16:05.538741Z","submitted_at":"2025-07-03T18:01:03Z","title":"Mitigating Model Misspecification in Simulation-Based Inference for Galaxy Clustering","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T20:24:55.911486Z"},"links":{"cited_paper":"/paper/2108.07821","citing_paper":"/paper/2507.03086"},"observation_digest":"sha256:66ac343b90950c648f62da23ddc993bb61dc99dbf63ee1b7a71ee5b53e9f6898","observation_id":"4fe16794-15e5-4e68-afa9-c01657a3f0d1","resolution":{"observed_at":"2026-08-06T20:24:55.911486Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.07821","last_updated":"2022-05-18T19:27:13Z","snapshot_observed_at":"2026-07-06T11:39:06.926826Z","submitted_at":"2021-08-17T18:00:04Z","title":"Towards an Optimal Estimation of Cosmological Parameters with the Wavelet Scattering Transform","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.07821","snapshot_observed_at":"2026-08-04T07:57:25.630485Z","title":"Valogiannis and C","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2510.23597","last_updated":"2025-10-27T17:58:09Z","snapshot_observed_at":"2026-08-05T15:57:56.325376Z","submitted_at":"2025-10-27T17:58:09Z","title":"The Compressed 3D Lyman-Alpha Forest Bispectrum","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-04T07:57:25.630485Z"},"links":{"cited_paper":"/paper/2108.07821","citing_paper":"/paper/2510.23597"},"observation_digest":"sha256:1750c2c980d27f82f3d68c54aaa6822680d49c13ea8f3cc6343700da35954847","observation_id":"ef086c2f-20fc-4f6a-b09b-fafc4f482885","resolution":{"observed_at":"2026-08-04T07:57:25.630485Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.07821","last_updated":"2022-05-18T19:27:13Z","snapshot_observed_at":"2026-07-06T11:39:06.926826Z","submitted_at":"2021-08-17T18:00:04Z","title":"Towards an Optimal Estimation of Cosmological Parameters with the Wavelet Scattering Transform","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.07821","snapshot_observed_at":"2026-08-03T21:51:29.138732Z","title":"& Dvorkin, C","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.13393","last_updated":"2026-06-27T08:18:53Z","snapshot_observed_at":"2026-08-07T14:58:57.874025Z","submitted_at":"2025-11-17T14:06:53Z","title":"Learning Cosmology from Nearest Neighbour Statistics","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-03T21:51:29.138732Z"},"links":{"cited_paper":"/paper/2108.07821","citing_paper":"/paper/2511.13393"},"observation_digest":"sha256:042eea7fdbc18b70bf2441d26f3629bb0e6f2213f8c773cac8e6d4981846224c","observation_id":"b568041a-8731-4fd1-a837-a0d28c92c13c","resolution":{"observed_at":"2026-08-03T21:51:29.138732Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.07821","last_updated":"2022-05-18T19:27:13Z","snapshot_observed_at":"2026-07-06T11:39:06.926826Z","submitted_at":"2021-08-17T18:00:04Z","title":"Towards an Optimal Estimation of Cosmological Parameters with the Wavelet Scattering Transform","version":2},"cited_work":{"arxiv_id":"2108.07821","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2108.07821","snapshot_observed_at":"2026-06-29T16:33:39.588072Z","title":"Valogiannis and C","venue":null,"work_id":"4ea8b98d-6ba1-4d67-9271-ded98c63070c","year":2022},"citing_paper":{"arxiv_id":"2605.27087","last_updated":"2026-06-02T03:39:14Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-26T14:35:10Z","title":"Cosmological Constraints from Bias-Robust Wavelet Scattering Statistics for Stage-IV Galaxy Surveys","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-06-29T15:49:18.200446Z"},"links":{"cited_paper":"/paper/2108.07821","citing_paper":"/paper/2605.27087"},"observation_digest":"sha256:dec9aec48ee5afd3d1a22029affe3cfd1ee858f0398e896cb6e388bdf18e2332","observation_id":"75ba78c2-9ae3-413e-bf99-1a68a8d1ea6a","resolution":{"observed_at":"2026-06-29T16:33:39.589387Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.07821","last_updated":"2022-05-18T19:27:13Z","snapshot_observed_at":"2026-07-06T11:39:06.926826Z","submitted_at":"2021-08-17T18:00:04Z","title":"Towards an Optimal Estimation of Cosmological Parameters with the Wavelet Scattering Transform","version":2},"cited_work":{"arxiv_id":"2108.07821","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2108.07821","snapshot_observed_at":"2026-06-29T16:33:39.588072Z","title":"Valogiannis and C","venue":null,"work_id":"4ea8b98d-6ba1-4d67-9271-ded98c63070c","year":2022},"citing_paper":{"arxiv_id":"2605.30305","last_updated":"2026-05-28T17:50:30Z","snapshot_observed_at":"2026-08-07T00:41:46.942064Z","submitted_at":"2026-05-28T17:50:30Z","title":"Augmented Correlation Functions for Spectroscopic Galaxy Surveys","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-06-29T05:37:00.270273Z"},"links":{"cited_paper":"/paper/2108.07821","citing_paper":"/paper/2605.30305"},"observation_digest":"sha256:2e28f8720486e98647175e86ceda58c85ab613d3c81cf05540ed31bb363653e8","observation_id":"b41aa99e-164e-4442-809d-98e7fb76a767","resolution":{"observed_at":"2026-06-29T05:43:08.629235Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.07821","last_updated":"2022-05-18T19:27:13Z","snapshot_observed_at":"2026-07-06T11:39:06.926826Z","submitted_at":"2021-08-17T18:00:04Z","title":"Towards an Optimal Estimation of Cosmological Parameters with the Wavelet Scattering Transform","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.07821","snapshot_observed_at":"2026-08-01T00:53:53.466653Z","title":"Valogiannis and C","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.26021","last_updated":"2026-07-28T17:32:56Z","snapshot_observed_at":"2026-08-06T00:45:04.443657Z","submitted_at":"2026-07-28T17:32:56Z","title":"Weighted Webs: Morphology-Informed Marked Fields","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-01T00:53:53.466653Z"},"links":{"cited_paper":"/paper/2108.07821","citing_paper":"/paper/2607.26021"},"observation_digest":"sha256:da803c8f1a35317af8dbe9aba327db3a80d2ee341b7e9923e422d5b84d938537","observation_id":"6c12d8b0-bc97-496d-95e5-57b565cb409c","resolution":{"observed_at":"2026-08-01T00:53:53.466653Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2108.07821/citation-record","integrity":"/paper/2108.07821/integrity","json":"/paper/2108.07821/citation-record.json","paper":"/paper/2108.07821"},"outbound":[],"paper":{"arxiv_id":"2108.07821","last_updated":"2022-05-18T19:27:13Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T11:39:06.926826Z","submitted_at":"2021-08-17T18:00:04Z","title":"Towards an Optimal Estimation of Cosmological Parameters with the Wavelet Scattering Transform"},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2108.07821."}