{"as_of":"2026-08-13T17:35:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9d530e4d2341256007570cec0be0787decf3eb51cc0e6219204921dee612d5a6","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":"2026-08-13T06:32:02.005865+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":"2026-08-10T06:07:09.898974Z","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":"2026-07-04T18:10:01.263948Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2505.03626","last_updated":"2025-05-06T15:23:09Z","snapshot_observed_at":"2026-08-07T23:30:15.406999Z","submitted_at":"2025-05-06T15:23:09Z","title":"High-redshift Millennium and Astrid galaxies in effective field theory at the field level","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.03626","snapshot_observed_at":"2026-08-06T21:30:54.542883Z","title":null,"venue":null,"work_id":null,"year":2025},"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":43,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.542883Z"},"links":{"cited_paper":"/paper/2505.03626","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:a163c197f942e749cf8e996a6dedc416fdde59d20f4704f83013b0b755a8234d","observation_id":"94be9440-a4bb-4d81-9d0b-9de6642ff03d","resolution":{"observed_at":"2026-08-06T21:30:54.542883Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.03626","last_updated":"2025-05-06T15:23:09Z","snapshot_observed_at":"2026-08-07T23:30:15.406999Z","submitted_at":"2025-05-06T15:23:09Z","title":"High-redshift Millennium and Astrid galaxies in effective field theory at the field level","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.03626","snapshot_observed_at":"2026-08-06T21:27:28.272370Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.00284","last_updated":"2025-06-30T21:53:00Z","snapshot_observed_at":"2026-08-12T23:22:09.901763Z","submitted_at":"2025-06-30T21:53:00Z","title":"Modeling the Cosmological Lyman-$\\alpha$ Forest at the Field Level","version":1},"reference_index":120,"source":"pdf_text","source_observed_at":"2026-08-06T21:27:28.272370Z"},"links":{"cited_paper":"/paper/2505.03626","citing_paper":"/paper/2507.00284"},"observation_digest":"sha256:f163e03c1b9d05d50308e03431cb8e9d88f0048e18d55af8b1a8e7a3265216de","observation_id":"167d731e-0922-48f3-873e-ef739105a7d2","resolution":{"observed_at":"2026-08-06T21:27:28.272370Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.03626","last_updated":"2025-05-06T15:23:09Z","snapshot_observed_at":"2026-08-07T23:30:15.406999Z","submitted_at":"2025-05-06T15:23:09Z","title":"High-redshift Millennium and Astrid galaxies in effective field theory at the field level","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.03626","snapshot_observed_at":"2026-08-06T12:12:39.918233Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.22110","last_updated":"2026-07-22T14:21:38Z","snapshot_observed_at":"2026-08-13T09:05:49.962559Z","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":114,"source":"pdf_text","source_observed_at":"2026-08-06T12:12:39.918233Z"},"links":{"cited_paper":"/paper/2505.03626","citing_paper":"/paper/2507.22110"},"observation_digest":"sha256:cdc2b975ffd79a4432c869da5edd658f8eb0d4ffb9d24b94777f1323c980e906","observation_id":"e7acb00b-5ee0-4bbb-8fdf-a3cc24efee50","resolution":{"observed_at":"2026-08-06T12:12:39.918233Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.03626","last_updated":"2025-05-06T15:23:09Z","snapshot_observed_at":"2026-08-07T23:30:15.406999Z","submitted_at":"2025-05-06T15:23:09Z","title":"High-redshift Millennium and Astrid galaxies in effective field theory at the field level","version":1},"cited_work":{"arxiv_id":"2505.03626","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2505.03626","snapshot_observed_at":"2026-07-04T18:10:01.263948Z","title":null,"venue":null,"work_id":"b5e8c050-36c7-4b68-b1d7-ad599cca1aa3","year":2025},"citing_paper":{"arxiv_id":"2606.24852","last_updated":"2026-06-23T17:31:23Z","snapshot_observed_at":"2026-07-06T23:59:23.407216Z","submitted_at":"2026-06-23T17:31:23Z","title":"The 3D clustering of Lyman Alpha Emitters measured with DESI","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-06-25T23:02:45.609207Z"},"links":{"cited_paper":"/paper/2505.03626","citing_paper":"/paper/2606.24852"},"observation_digest":"sha256:6163fa9f62872d1bf3eba606b826c77248f191c04a4cb1b74214e08e140f187a","observation_id":"a9beceb6-ae72-4ef1-bbc2-ea6c5b648d4c","resolution":{"observed_at":"2026-07-04T18:10:01.266219Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.03626","last_updated":"2025-05-06T15:23:09Z","snapshot_observed_at":"2026-08-07T23:30:15.406999Z","submitted_at":"2025-05-06T15:23:09Z","title":"High-redshift Millennium and Astrid galaxies in effective field theory at the field level","version":1},"cited_work":{"arxiv_id":"2505.03626","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2505.03626","snapshot_observed_at":"2026-07-04T18:10:01.263948Z","title":null,"venue":null,"work_id":"b5e8c050-36c7-4b68-b1d7-ad599cca1aa3","year":2025},"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":155,"source":"pdf_text","source_observed_at":"2026-06-26T01:38:09.398349Z"},"links":{"cited_paper":"/paper/2505.03626","citing_paper":"/paper/2606.26234"},"observation_digest":"sha256:b431883795defc993e04942a84092f1cce535f6ccf4d5582548b2ffcf7d2ca9d","observation_id":"580c9957-2b86-4620-bd00-65dc2db9db34","resolution":{"observed_at":"2026-07-04T15:29:55.275115Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.03626","last_updated":"2025-05-06T15:23:09Z","snapshot_observed_at":"2026-08-07T23:30:15.406999Z","submitted_at":"2025-05-06T15:23:09Z","title":"High-redshift Millennium and Astrid galaxies in effective field theory at the field level","version":1},"cited_work":{"arxiv_id":"2505.03626","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2505.03626","snapshot_observed_at":"2026-07-04T18:10:01.263948Z","title":null,"venue":null,"work_id":"b5e8c050-36c7-4b68-b1d7-ad599cca1aa3","year":2025},"citing_paper":{"arxiv_id":"2606.30713","last_updated":"2026-06-29T18:00:00Z","snapshot_observed_at":"2026-07-07T00:04:29.879877Z","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":97,"source":"pdf_text","source_observed_at":"2026-07-01T02:01:27.807230Z"},"links":{"cited_paper":"/paper/2505.03626","citing_paper":"/paper/2606.30713"},"observation_digest":"sha256:8abe883c0cf3ef6b4b28c2749d0b91a1ab6b32bdb870519f9d797a9f333a2443","observation_id":"a6b95d4a-d8e5-486f-9b44-f92c8e1ac034","resolution":{"observed_at":"2026-07-01T12:35:43.572418Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.03626","last_updated":"2025-05-06T15:23:09Z","snapshot_observed_at":"2026-08-07T23:30:15.406999Z","submitted_at":"2025-05-06T15:23:09Z","title":"High-redshift Millennium and Astrid galaxies in effective field theory at the field level","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.03626","snapshot_observed_at":"2026-07-31T11:32:44.236063Z","title":"Sullivan, C","venue":null,"work_id":null,"year":2025},"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":114,"source":"pdf_text","source_observed_at":"2026-07-31T11:32:44.236063Z"},"links":{"cited_paper":"/paper/2505.03626","citing_paper":"/paper/2607.28314"},"observation_digest":"sha256:0547f731961d4aa666bcbb15a0a2e2861dc87a7f0fa7aefb90e19a304daebdf6","observation_id":"1ed7ceb8-e14d-4496-a81a-9969536ac21b","resolution":{"observed_at":"2026-07-31T11:32:44.236063Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.03626","last_updated":"2025-05-06T15:23:09Z","snapshot_observed_at":"2026-08-07T23:30:15.406999Z","submitted_at":"2025-05-06T15:23:09Z","title":"High-redshift Millennium and Astrid galaxies in effective field theory at the field level","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.03626","snapshot_observed_at":"2026-08-10T06:07:09.898974Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.07339","last_updated":"2026-08-07T15:36:28Z","snapshot_observed_at":"2026-08-13T10:33:03.948411Z","submitted_at":"2026-08-07T15:36:28Z","title":"Sample Variance Cancellation for Future Spectroscopic Surveys","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-10T06:07:09.898974Z"},"links":{"cited_paper":"/paper/2505.03626","citing_paper":"/paper/2608.07339"},"observation_digest":"sha256:a8213f9946e5c4ea9fe1f6f97c452bc19e65d471fe9d314f110b3fb724d5a128","observation_id":"69d6a7a3-f0f5-4808-9012-492205ce85ed","resolution":{"observed_at":"2026-08-10T06:07:09.898974Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2505.03626/citation-record","integrity":"/paper/2505.03626/integrity","json":"/paper/2505.03626/citation-record.json","paper":"/paper/2505.03626"},"outbound":[],"paper":{"arxiv_id":"2505.03626","last_updated":"2025-05-06T15:23:09Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-07T23:30:15.406999Z","submitted_at":"2025-05-06T15:23:09Z","title":"High-redshift Millennium and Astrid galaxies in effective field theory 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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2505.03626."}