{"as_of":"2026-08-10T21:36:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:698f06ee3b63b3e0431dadb0fab8dc9f10d68645448711f1dbe07e989d5ae17d","coverage":[{"denominator":104,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T21:30:54.992988Z","state":"measured"},{"denominator":107,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":107,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":7,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":7,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T21:30:54.279301Z","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":"2026-05-17T04:19:00.846851Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.00118","snapshot_observed_at":"2026-08-06T21:30:54.279301Z","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":1,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.279301Z"},"links":{"cited_paper":"/paper/2507.00118","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:fbd4023917766ddd738a36a281727010363b128838796f16adbe06ff95a1a6e8","observation_id":"7627e816-bdc8-473c-86ef-70ff4f90f75a","resolution":{"observed_at":"2026-08-06T21:30:54.279301Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.00118","snapshot_observed_at":"2026-08-04T10:38:03.277184Z","title":"Chen and M.M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.09563","last_updated":"2026-07-06T19:12:15Z","snapshot_observed_at":"2026-08-07T22:16:31.334726Z","submitted_at":"2025-10-10T17:14:29Z","title":"Low-redshift constraints on structure growth from CMB lensing tomography","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-04T10:38:03.277184Z"},"links":{"cited_paper":"/paper/2507.00118","citing_paper":"/paper/2510.09563"},"observation_digest":"sha256:2ba3d716102c0fcc7af3f4960a2f199c5a4a6741f978d96fdad254922b790204","observation_id":"92a54218-4e62-4b03-abfc-0497aee76a41","resolution":{"observed_at":"2026-08-04T10:38:03.277184Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":"2507.00118","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2507.00118","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Chen and M","venue":null,"work_id":"9e5a0900-4927-43e1-aed8-2fb50e634e8b","year":2025},"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":19,"source":"pdf_text","source_observed_at":"2026-05-17T04:15:18.730245Z"},"links":{"cited_paper":"/paper/2507.00118","citing_paper":"/paper/2511.20757"},"observation_digest":"sha256:4621a35d42181ba4c3e0348ffdff22a87a938533fe9cf5e493d51a8bc3e7706e","observation_id":"6fe91a3a-8e3a-4a4c-9803-22430536034f","resolution":{"observed_at":"2026-05-17T04:19:00.848615Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.00118","snapshot_observed_at":"2026-08-03T08:42:10.727237Z","title":"Chen and M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2601.16165","last_updated":"2026-07-22T13:53:51Z","snapshot_observed_at":"2026-08-08T14:24:16.036685Z","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":208,"source":"pdf_text","source_observed_at":"2026-08-03T08:42:10.727237Z"},"links":{"cited_paper":"/paper/2507.00118","citing_paper":"/paper/2601.16165"},"observation_digest":"sha256:5c7e3092ee9eec89a08a1e8a9df6da3376c7f444c7a3f5ad77057e153ad8a9e5","observation_id":"c73080c8-c333-41d7-94bd-bea54d664cfa","resolution":{"observed_at":"2026-08-03T08:42:10.727237Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.00118","snapshot_observed_at":"2026-08-02T22:01:22.296024Z","title":"Chen and M","venue":null,"work_id":null,"year":2025},"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":50,"source":"pdf_text","source_observed_at":"2026-08-02T22:01:22.296024Z"},"links":{"cited_paper":"/paper/2507.00118","citing_paper":"/paper/2602.18554"},"observation_digest":"sha256:0b70ee4f1c1276a87cc45c2717e0b8e35150ea47f05d690c03cbe1d76fcacdd2","observation_id":"33633291-b3c8-4815-8f7b-1db39fa99e55","resolution":{"observed_at":"2026-08-02T22:01:22.296024Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.00118","snapshot_observed_at":"2026-08-02T02:52:34.323473Z","title":"Chen and M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.14206","last_updated":"2026-07-15T18:00:00Z","snapshot_observed_at":"2026-08-08T17:37:53.554810Z","submitted_at":"2026-07-15T18:00:00Z","title":"Simulation-Based Priors for HI Bias from Halo Occupation Physics","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-02T02:52:34.323473Z"},"links":{"cited_paper":"/paper/2507.00118","citing_paper":"/paper/2607.14206"},"observation_digest":"sha256:115d98802dceeb544c2cf5f75a6e418210f740265709687de5eaeb8c0937dce8","observation_id":"3915240b-d39b-4c0c-97f4-5097f27d6bd2","resolution":{"observed_at":"2026-08-02T02:52:34.323473Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.00118","snapshot_observed_at":"2026-07-31T11:32:43.680106Z","title":"Chen and M.M","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":109,"source":"pdf_text","source_observed_at":"2026-07-31T11:32:43.680106Z"},"links":{"cited_paper":"/paper/2507.00118","citing_paper":"/paper/2607.28314"},"observation_digest":"sha256:dc22431454e4daa602af6d484b806d44c75fb74fd5bcccb028909a1ed50fcce2","observation_id":"6c098446-e334-4594-8221-dd37cccb6e3e","resolution":{"observed_at":"2026-07-31T11:32:43.680106Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2507.00118/citation-record","integrity":"/paper/2507.00118/integrity","json":"/paper/2507.00118/citation-record.json","paper":"/paper/2507.00118"},"outbound":[{"citation":{"cited_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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.00118","snapshot_observed_at":"2026-08-06T21:30:54.279301Z","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":1,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.279301Z"},"links":{"cited_paper":"/paper/2507.00118","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:fbd4023917766ddd738a36a281727010363b128838796f16adbe06ff95a1a6e8","observation_id":"7627e816-bdc8-473c-86ef-70ff4f90f75a","resolution":{"observed_at":"2026-08-06T21:30:54.279301Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:30:54.285266Z","title":"For instance, even at the level of the power spec- trum alone, there are eleven EFT nuisance parameters that must be marginalized over to constrain cosmological parameters","venue":null,"work_id":null,"year":null},"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":2,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.285266Z"},"links":{"citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:8b8796558c0f3ecd02c575434b2ac554c958d25fc8d70e596ea2b665b579c64f","observation_id":"b948eff6-c865-42fa-97a6-36cac3a48b2b","resolution":{"observed_at":"2026-08-06T21:30:54.285266Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:30:54.290088Z","title":"We will present the detail of each experiment here and explain the pa- rameters varied in this section","venue":null,"work_id":null,"year":2018},"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":3,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.290088Z"},"links":{"citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:0fb8bbe183185539e534c6132d1043d6e5375a4c4b7f1b087a9a154c623d8329","observation_id":"65f33602-5cde-4140-b847-19fa394a003a","resolution":{"observed_at":"2026-08-06T21:30:54.290088Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:30:54.295851Z","title":"Gaussian","venue":null,"work_id":null,"year":2018},"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":4,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.295851Z"},"links":{"citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:5441b3ce89aa9beccdc09cffb7afc9d3070264ac664166a8d7f2b02a5a8f7aa5","observation_id":"a7b177c1-a02c-4be8-a916-bd2e1570c49b","resolution":{"observed_at":"2026-08-06T21:30:54.295851Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:30:54.301672Z","title":null,"venue":null,"work_id":null,"year":null},"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":5,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.301672Z"},"links":{"citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:e7f8d21d98552796015194994740710a689789c90364efc95d688efdf64015ec","observation_id":"1c695ac2-f751-4021-9798-8fcde43f4e3b","resolution":{"observed_at":"2026-08-06T21:30:54.301672Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.03002","last_updated":"2024-11-04T16:43:36Z","snapshot_observed_at":"2026-07-06T17:55:21.083912Z","submitted_at":"2024-04-03T18:41:51Z","title":"DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.03002","snapshot_observed_at":"2026-08-06T21:30:54.306260Z","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":6,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.306260Z"},"links":{"cited_paper":"/paper/2404.03002","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:907400a591feec3b69e1081d89d146a87b8a0049758aad1ceeb842fbcd524361","observation_id":"859a32ee-f9e7-4e8d-8a01-585c5b411b1e","resolution":{"observed_at":"2026-08-06T21:30:54.306260Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.03000","last_updated":"2024-04-03T18:41:49Z","snapshot_observed_at":"2026-08-09T18:42:58.809582Z","submitted_at":"2024-04-03T18:41:49Z","title":"DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.03000","snapshot_observed_at":"2026-08-06T21:30:54.311700Z","title":null,"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":7,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.311700Z"},"links":{"cited_paper":"/paper/2404.03000","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:837711538c29ea04d975c99f539df0c11a94639d6e131d0f1b9a5c190eb8c13b","observation_id":"059a5092-64a5-47b4-b966-81424a55fa32","resolution":{"observed_at":"2026-08-06T21:30:54.311700Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14738","last_updated":"2025-10-09T16:45:28Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-03-18T21:14:12Z","title":"DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14738","snapshot_observed_at":"2026-08-06T21:30:54.316372Z","title":"Abdul Karim et al","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":8,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.316372Z"},"links":{"cited_paper":"/paper/2503.14738","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:05e470c264a89316b6219393a9b396827417dab8cf02e91ac106f888988f57d5","observation_id":"c6f8f6ad-b20f-4c34-9f71-bcbaa61ec642","resolution":{"observed_at":"2026-08-06T21:30:54.316372Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14743","last_updated":"2025-04-03T13:50:59Z","snapshot_observed_at":"2026-07-06T20:55:04.493800Z","submitted_at":"2025-03-18T21:14:17Z","title":"Extended Dark Energy analysis using DESI DR2 BAO measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14743","snapshot_observed_at":"2026-08-06T21:30:54.324449Z","title":"Lodha et al","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":9,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.324449Z"},"links":{"cited_paper":"/paper/2503.14743","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:7374ecffddfd7868f6309ad7e3acb1975ad2f247c05ff8c1379fec49316b65c2","observation_id":"77796c6b-a2a1-4ae0-a30b-0afd3987f2e0","resolution":{"observed_at":"2026-08-06T21:30:54.324449Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1110.3193","last_updated":"2011-10-14T12:57:07Z","snapshot_observed_at":"2026-07-06T02:35:48.625634Z","submitted_at":"2011-10-14T12:57:07Z","title":"Euclid Definition Study Report","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.3193","snapshot_observed_at":"2026-08-06T21:30:54.331878Z","title":"Laureijs et al","venue":null,"work_id":null,"year":2011},"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":10,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.331878Z"},"links":{"cited_paper":"/paper/1110.3193","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:75bac882dd3bc74707b30f9f897716de2ef40693555c7fcb90fe3e4b5ed07c3a","observation_id":"7ce3cee7-64de-410a-a3f1-ab12539422f0","resolution":{"observed_at":"2026-08-06T21:30:54.331878Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0805.2366","last_updated":"2018-05-23T19:18:23Z","snapshot_observed_at":"2026-08-08T10:58:38.132550Z","submitted_at":"2008-05-15T18:10:13Z","title":"LSST: from Science Drivers to Reference Design and Anticipated Data Products","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0805.2366","snapshot_observed_at":"2026-08-06T21:30:54.337528Z","title":"Ivezi´ cet al","venue":null,"work_id":null,"year":2019},"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":11,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.337528Z"},"links":{"cited_paper":"/paper/0805.2366","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:b61ab3698c4e2493e1b92ce7544caf4a0cbc0f3670cd7738a42046b60a6abdee","observation_id":"65d0bdf3-da30-4182-8e37-a162fa87b3e5","resolution":{"observed_at":"2026-08-06T21:30:54.337528Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.05569","last_updated":"2019-02-14T19:15:58Z","snapshot_observed_at":"2026-07-06T07:33:12.016548Z","submitted_at":"2019-02-14T19:15:58Z","title":"The Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.05569","snapshot_observed_at":"2026-08-06T21:30:54.344966Z","title":"Akeson et al., (2019), arXiv:1902.05569 [astro-ph.IM]","venue":null,"work_id":null,"year":2019},"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":12,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.344966Z"},"links":{"cited_paper":"/paper/1902.05569","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:78aa796e3dbbee387589033511105377b536a4f09bb9a732ad29fd2cff7018cc","observation_id":"3be237c7-4291-478c-8f68-e8c26dc3b16c","resolution":{"observed_at":"2026-08-06T21:30:54.344966Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.01320","last_updated":"2016-08-25T11:29:08Z","snapshot_observed_at":"2026-07-06T04:32:06.122689Z","submitted_at":"2015-10-05T20:04:27Z","title":"The EAGLE simulations of galaxy formation: public release of halo and galaxy catalogues","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.01320","snapshot_observed_at":"2026-08-06T21:30:54.350992Z","title":"McAlpine et al","venue":null,"work_id":null,"year":2016},"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":13,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.350992Z"},"links":{"cited_paper":"/paper/1510.01320","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:0cf90a618838e5700869a971974f8ed534ea53960cbca176a835cb26d6d210cf","observation_id":"841d6954-b332-4b65-bcf8-bf40391528ed","resolution":{"observed_at":"2026-08-06T21:30:54.350992Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.03397","last_updated":"2017-12-21T12:49:59Z","snapshot_observed_at":"2026-08-10T10:37:00.201799Z","submitted_at":"2017-07-11T18:00:01Z","title":"First results from the IllustrisTNG simulations: matter and galaxy clustering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.03397","snapshot_observed_at":"2026-08-06T21:30:54.355930Z","title":"Springel et al., Mon","venue":null,"work_id":null,"year":2018},"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":14,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.355930Z"},"links":{"cited_paper":"/paper/1707.03397","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:ea5388e4870d2a4030305e45e1d45462a47bda8c03b68d4901a8b24369ca24ca","observation_id":"ccd98637-fad4-41ee-b570-15966766157d","resolution":{"observed_at":"2026-08-06T21:30:54.355930Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.10059","last_updated":"2023-05-01T08:54:53Z","snapshot_observed_at":"2026-08-09T18:12:13.947857Z","submitted_at":"2022-10-18T18:00:01Z","title":"The MillenniumTNG Project: High-precision predictions for matter clustering and halo statistics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.10059","snapshot_observed_at":"2026-08-06T21:30:54.363314Z","title":"Hern´ andez-Aguayoet al., Mon","venue":null,"work_id":null,"year":2023},"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":15,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.363314Z"},"links":{"cited_paper":"/paper/2210.10059","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:d26da5ae5e289f38d3ca4191d521b3b671284de911f17d459ff273043a5cad47","observation_id":"2e029b6c-689e-416c-9996-ac310b37ccf8","resolution":{"observed_at":"2026-08-06T21:30:54.363314Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0109001","last_updated":"2002-04-22T23:21:58Z","snapshot_observed_at":"2026-07-07T00:21:09.886224Z","submitted_at":"2001-09-01T00:39:10Z","title":"The Halo Occupation Distribution: Towards an Empirical Determination of the Relation Between Galaxies and Mass","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0109001","snapshot_observed_at":"2026-08-06T21:30:54.370356Z","title":null,"venue":null,"work_id":null,"year":2002},"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":16,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.370356Z"},"links":{"cited_paper":"/paper/astro-ph/0109001","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:2badee09538655318c288315a7a118fa9913347708e11c6571a244318e156f7c","observation_id":"7244e37d-b665-4e7c-ab34-3e1ecb783b6b","resolution":{"observed_at":"2026-08-06T21:30:54.370356Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0308519","last_updated":"2004-05-15T00:28:33Z","snapshot_observed_at":"2026-07-07T00:35:54.344067Z","submitted_at":"2003-08-29T16:03:32Z","title":"The Dark Side of the Halo Occupation Distribution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0308519","snapshot_observed_at":"2026-08-06T21:30:54.375843Z","title":null,"venue":null,"work_id":null,"year":2004},"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":17,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.375843Z"},"links":{"cited_paper":"/paper/astro-ph/0308519","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:9fce30fc0d0374c0394f37b35194fcb27324d8c5fd8e6c2b3b756c58e26ab689","observation_id":"d028dafd-7fcc-4f30-98ad-9682fb9ca8f4","resolution":{"observed_at":"2026-08-06T21:30:54.375843Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:30:54.381658Z","title":"Zheng, A","venue":null,"work_id":null,"year":2005},"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":18,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.381658Z"},"links":{"citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:a844eee0f7f2cf21610832f52e45df8d20ad22e5a0586bd8281b56fde049e225","observation_id":"08972ae1-87a5-44a3-848f-9b1434612cda","resolution":{"observed_at":"2026-08-06T21:30:54.381658Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.03050","last_updated":"2015-12-09T21:00:00Z","snapshot_observed_at":"2026-08-02T09:37:08.322182Z","submitted_at":"2015-12-09T21:00:00Z","title":"Introducing Decorated HODs: modeling assembly bias in the galaxy-halo connection","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.03050","snapshot_observed_at":"2026-08-06T21:30:54.387381Z","title":null,"venue":null,"work_id":null,"year":2016},"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":19,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.387381Z"},"links":{"cited_paper":"/paper/1512.03050","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:de9acc08351144afdfb70d75518e955e971ee832030876a96450f550d2395ad9","observation_id":"96ebd98d-b822-4865-b1bf-3f040d0dec8b","resolution":{"observed_at":"2026-08-06T21:30:54.387381Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03097","last_updated":"2018-04-09T16:51:59Z","snapshot_observed_at":"2026-07-06T06:32:29.028840Z","submitted_at":"2018-04-09T16:51:59Z","title":"The Connection between Galaxies and their Dark Matter Halos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.03097","snapshot_observed_at":"2026-08-06T21:30:54.393471Z","title":null,"venue":null,"work_id":null,"year":2018},"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":20,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.393471Z"},"links":{"cited_paper":"/paper/1804.03097","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:a9ac68797c41e2ea6cde1ebfdbb6c3fa58ff1a4c09e848a3d447c7a5299855e9","observation_id":"b26f42e3-b5d7-420a-8ac5-05be2197b9d5","resolution":{"observed_at":"2026-08-06T21:30:54.393471Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.02252","last_updated":"2026-07-15T16:04:50Z","snapshot_observed_at":"2026-07-18T23:18:57.209844Z","submitted_at":"2024-05-03T17:09:52Z","title":"A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.02252","snapshot_observed_at":"2026-08-06T21:30:54.402080Z","title":"Krause et al","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":21,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.402080Z"},"links":{"cited_paper":"/paper/2405.02252","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:03e6ae0cee70f312115e3f180b84e9dd1ae88064ba2da7e89debcc1b9c4860c1","observation_id":"60fdbb4f-6d48-4c48-b7c4-bf093963d716","resolution":{"observed_at":"2026-08-06T21:30:54.402080Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.03155","last_updated":"2016-07-11T20:29:52Z","snapshot_observed_at":"2026-07-06T05:03:11.934242Z","submitted_at":"2016-07-11T20:29:52Z","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.03155","snapshot_observed_at":"2026-08-06T21:30:54.408199Z","title":"Alam et al","venue":null,"work_id":null,"year":2017},"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":22,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.408199Z"},"links":{"cited_paper":"/paper/1607.03155","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:2e77806a1b5862f9b4055d8241a5a7736f136d4c6a770929d8ca699dfb9e7ba5","observation_id":"9726fccf-5757-44c4-993b-30b6979dbeb4","resolution":{"observed_at":"2026-08-06T21:30:54.408199Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.06969","last_updated":"2022-03-11T01:14:43Z","snapshot_observed_at":"2026-07-06T11:57:39.282469Z","submitted_at":"2021-10-13T18:16:31Z","title":"Full-shape cosmology analysis of SDSS-III BOSS galaxy power spectrum using emulator-based halo model: a $5\\%$ determination of $\\sigma_8$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.06969","snapshot_observed_at":"2026-08-06T21:30:54.413066Z","title":"Kobayashi, T","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.00118","last_updated":"2025-06-30T18:00:01Z","snapshot_observed_at":"2026-08-08T17:58:16.664935Z","submitted_at":"2025-06-30T18:00:01Z","title":"Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.413066Z"},"links":{"cited_paper":"/paper/2110.06969","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:db19d5f27626962c2a5efde1610bf7d905039d6141c9ac1c0b31943e12a80f1e","observation_id":"512607ed-c6e5-461f-9070-761d05fe4856","resolution":{"observed_at":"2026-08-06T21:30:54.413066Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.16539","last_updated":"2023-10-02T17:38:22Z","snapshot_observed_at":"2026-07-06T16:25:01.609308Z","submitted_at":"2023-09-28T15:53:30Z","title":"SUNBIRD: A simulation-based model for full-shape density-split clustering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.16539","snapshot_observed_at":"2026-08-06T21:30:54.418513Z","title":"Cuesta-Lazaro et al., (2023), arXiv:2309.16539 [astro- ph.CO]","venue":null,"work_id":null,"year":2023},"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":24,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.418513Z"},"links":{"cited_paper":"/paper/2309.16539","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:ab41007fe1d48b618836bba324ec76a8eaea3c7bcf2a3270969f72579d25556e","observation_id":"28513114-1913-4f40-9ecc-7beaf7fef39e","resolution":{"observed_at":"2026-08-06T21:30:54.418513Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.16116","last_updated":"2025-05-14T21:43:01Z","snapshot_observed_at":"2026-07-06T16:38:02.155336Z","submitted_at":"2023-10-24T18:33:11Z","title":"Precise Cosmological Constraints from BOSS Galaxy Clustering with a Simulation-Based Emulator of the Wavelet Scattering Transform","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.16116","snapshot_observed_at":"2026-08-06T21:30:54.423644Z","title":"Valogiannis, S","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":25,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.423644Z"},"links":{"cited_paper":"/paper/2310.16116","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:1ab3bc08bb2e029d5f4c416d5d6a2977e806cea2be4ee1559bacf1181e46a5b6","observation_id":"993400d3-19b4-4c30-b03d-518b7541fd2b","resolution":{"observed_at":"2026-08-06T21:30:54.423644Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.15243","last_updated":"2023-10-23T18:01:04Z","snapshot_observed_at":"2026-08-03T09:02:09.723963Z","submitted_at":"2023-10-23T18:01:04Z","title":"${\\rm S{\\scriptsize IM}BIG}$: The First Cosmological Constraints from the Non-Linear Galaxy Bispectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.15243","snapshot_observed_at":"2026-08-06T21:30:54.432891Z","title":null,"venue":null,"work_id":null,"year":2023},"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":26,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.432891Z"},"links":{"cited_paper":"/paper/2310.15243","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:49cdce5a2534feb576beabe831628e7b4f0c5afb622cdad5d0cae5cf6c703e60","observation_id":"82692922-1dc1-4e42-a7a1-cbe7eab81a28","resolution":{"observed_at":"2026-08-06T21:30:54.432891Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.15074","last_updated":"2024-01-26T18:54:57Z","snapshot_observed_at":"2026-07-06T17:21:01.918787Z","submitted_at":"2024-01-26T18:54:57Z","title":"${\\rm S{\\scriptsize IM}BIG}$: Cosmological Constraints from the Redshift-Space Galaxy Skew Spectra","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.15074","snapshot_observed_at":"2026-08-06T21:30:54.437956Z","title":null,"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":27,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.437956Z"},"links":{"cited_paper":"/paper/2401.15074","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:ecf4220e912a26e6a0e901a3f07a848bdd34c7b54ca6f757527db2a4fe166668","observation_id":"2e7d8c29-a067-43a8-aa82-21c253cdd66c","resolution":{"observed_at":"2026-08-06T21:30:54.437956Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1004.2488","last_updated":"2010-04-14T20:00:03Z","snapshot_observed_at":"2026-07-06T02:06:43.432085Z","submitted_at":"2010-04-14T20:00:03Z","title":"Cosmological Non-Linearities as an Effective Fluid","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1004.2488","snapshot_observed_at":"2026-08-06T21:30:54.445267Z","title":"Baumann, A","venue":null,"work_id":null,"year":2012},"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":28,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.445267Z"},"links":{"cited_paper":"/paper/1004.2488","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:130078e844b4f04715068a85ef5e06fa80192fd355f7a00a13ef486376ed14a7","observation_id":"cda9db17-3dc0-4abb-8086-7f5205640115","resolution":{"observed_at":"2026-08-06T21:30:54.445267Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1206.2926","last_updated":"2012-10-16T15:42:07Z","snapshot_observed_at":"2026-08-10T09:42:36.081244Z","submitted_at":"2012-06-13T20:00:04Z","title":"The Effective Field Theory of Cosmological Large Scale Structures","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.2926","snapshot_observed_at":"2026-08-06T21:30:54.449829Z","title":null,"venue":null,"work_id":null,"year":2012},"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":29,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.449829Z"},"links":{"cited_paper":"/paper/1206.2926","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:6d600eb0fab433eb759755e96343900956dfc3eadb8a2875ce208e6e201f6cfe","observation_id":"e173aefe-af18-4c3a-adb4-6a806d5f32cf","resolution":{"observed_at":"2026-08-06T21:30:54.449829Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.08488","last_updated":"2022-12-16T14:01:42Z","snapshot_observed_at":"2026-08-02T01:23:20.624289Z","submitted_at":"2022-12-16T14:01:42Z","title":"Effective Field Theory for Large Scale Structure","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.08488","snapshot_observed_at":"2026-08-06T21:30:54.455647Z","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":"2026-08-08T17:58:16.664935Z","submitted_at":"2025-06-30T18:00:01Z","title":"Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.455647Z"},"links":{"cited_paper":"/paper/2212.08488","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:cd99eabff32d3187c89ba8a1b8f0e1942907fea8583cd6fc3f8ac326cc17661d","observation_id":"c6fdbfd8-23ba-41ab-92b1-a10cf69491a4","resolution":{"observed_at":"2026-08-06T21:30:54.455647Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.09787","last_updated":"2019-01-14T18:30:24Z","snapshot_observed_at":"2026-08-09T01:53:49.525776Z","submitted_at":"2016-11-29T18:57:56Z","title":"Large-Scale Galaxy Bias","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.09787","snapshot_observed_at":"2026-08-06T21:30:54.463076Z","title":"Desjacques, D","venue":null,"work_id":null,"year":2018},"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":31,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.463076Z"},"links":{"cited_paper":"/paper/1611.09787","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:d3e3908ee7f121b8636e9d2eb38b66229605c63cb21d61a52d119501491a07af","observation_id":"ad56386c-41b2-48ed-b734-ed23b5cf9830","resolution":{"observed_at":"2026-08-06T21:30:54.463076Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.05277","last_updated":"2020-05-27T14:49:48Z","snapshot_observed_at":"2026-08-09T05:58:40.990824Z","submitted_at":"2019-09-11T18:06:18Z","title":"Cosmological Parameters from the BOSS Galaxy Power Spectrum","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.05277","snapshot_observed_at":"2026-08-06T21:30:54.468523Z","title":null,"venue":null,"work_id":null,"year":2020},"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":32,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.468523Z"},"links":{"cited_paper":"/paper/1909.05277","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:9a34f0adc0de081922f735e93c39d1803d24b457a6b63a170938164ba29d8a0c","observation_id":"adf1a551-a00b-4ddf-8c7d-85562050b64a","resolution":{"observed_at":"2026-08-06T21:30:54.468523Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.05271","last_updated":"2019-09-11T18:00:28Z","snapshot_observed_at":"2026-08-08T00:28:21.002318Z","submitted_at":"2019-09-11T18:00:28Z","title":"The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.05271","snapshot_observed_at":"2026-08-06T21:30:54.477397Z","title":"D’Amico, J","venue":null,"work_id":null,"year":2019},"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":33,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.477397Z"},"links":{"cited_paper":"/paper/1909.05271","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:d096388fe91d244504008a02e67b5897f027758f45f2f198dceed3391a117444","observation_id":"0fe581c5-b8e8-4418-92f3-b1695c0451e1","resolution":{"observed_at":"2026-08-06T21:30:54.477397Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.05530","last_updated":"2022-01-18T16:49:31Z","snapshot_observed_at":"2026-08-05T04:36:08.958138Z","submitted_at":"2021-10-11T18:11:38Z","title":"A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.05530","snapshot_observed_at":"2026-08-06T21:30:54.485586Z","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":"2026-08-08T17:58:16.664935Z","submitted_at":"2025-06-30T18:00:01Z","title":"Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.485586Z"},"links":{"cited_paper":"/paper/2110.05530","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:fb97b2a9dc4538720b70f33cfd31c5167f5dd0d4efe441d5408f934a552a70df","observation_id":"362c9707-1c22-4e7a-815d-3e5ce77abc14","resolution":{"observed_at":"2026-08-06T21:30:54.485586Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.04515","last_updated":"2022-01-31T02:48:30Z","snapshot_observed_at":"2026-08-09T08:02:11.377549Z","submitted_at":"2021-12-08T19:00:04Z","title":"The BOSS DR12 Full-Shape Cosmology: $\\Lambda$CDM Constraints from the Large-Scale Galaxy Power Spectrum and Bispectrum Monopole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.04515","snapshot_observed_at":"2026-08-06T21:30:54.494259Z","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":"2026-08-08T17:58:16.664935Z","submitted_at":"2025-06-30T18:00:01Z","title":"Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.494259Z"},"links":{"cited_paper":"/paper/2112.04515","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:6326b7428b46c0b30f0d75e273ef65014f68d008a21b2a2c9a004647970c9b93","observation_id":"6e46ea83-d6e9-44cd-898e-0c2dffffa2fb","resolution":{"observed_at":"2026-08-06T21:30:54.494259Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.04414","last_updated":"2023-02-09T03:01:25Z","snapshot_observed_at":"2026-08-10T03:19:43.143539Z","submitted_at":"2023-02-09T03:01:25Z","title":"Cosmology with the Galaxy Bispectrum Multipoles: Optimal Estimation and Application to BOSS Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.04414","snapshot_observed_at":"2026-08-06T21:30:54.499689Z","title":null,"venue":null,"work_id":null,"year":2023},"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":36,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.499689Z"},"links":{"cited_paper":"/paper/2302.04414","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:463b6cbdd3f3af79778c4d8be983012bcb43e491b6db8e227e529c6d42045b4b","observation_id":"b68a82a7-386e-446a-a1e3-9bdd59b3d449","resolution":{"observed_at":"2026-08-06T21:30:54.499689Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.13388","last_updated":"2024-11-18T18:51:19Z","snapshot_observed_at":"2026-07-06T18:33:32.806635Z","submitted_at":"2024-06-19T09:30:04Z","title":"Suppression without Thawing: Constraining Structure Formation and Dark Energy with Galaxy Clustering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.13388","snapshot_observed_at":"2026-08-06T21:30:54.506129Z","title":null,"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":37,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.506129Z"},"links":{"cited_paper":"/paper/2406.13388","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:1ee8273c81df4a7de7bfbc6b1ccf5c68818434a3c84f39210d68cb15e4253f90","observation_id":"182c724b-6cb6-4312-9164-103bae84968d","resolution":{"observed_at":"2026-08-06T21:30:54.506129Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.13310","last_updated":"2024-09-09T18:00:20Z","snapshot_observed_at":"2026-08-09T22:00:53.352888Z","submitted_at":"2024-02-20T19:00:00Z","title":"Full-shape analysis with simulation-based priors: constraints on single field inflation from BOSS","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.13310","snapshot_observed_at":"2026-08-06T21:30:54.513122Z","title":null,"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":38,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.513122Z"},"links":{"cited_paper":"/paper/2402.13310","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:e9734f2c5fae582602087b98e1f38620adcc559e7fc15dfbdd5b84501818d66b","observation_id":"b4923a69-91ba-418f-a76f-4265391df4ba","resolution":{"observed_at":"2026-08-06T21:30:54.513122Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.10609","last_updated":"2025-03-06T20:32:36Z","snapshot_observed_at":"2026-08-06T19:09:19.733947Z","submitted_at":"2024-09-16T18:00:03Z","title":"Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.10609","snapshot_observed_at":"2026-08-06T21:30:54.521158Z","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":39,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.521158Z"},"links":{"cited_paper":"/paper/2409.10609","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:f87066d0dfc9415134ee668d0ea0b77568446fc91cad40bb3e41f1c5a587f3e6","observation_id":"7e63e80b-c6b4-4250-8c8b-6d7561b66e1d","resolution":{"observed_at":"2026-08-06T21:30:54.521158Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.01894","last_updated":"2025-02-13T11:35:57Z","snapshot_observed_at":"2026-08-06T18:33:12.648395Z","submitted_at":"2024-04-02T12:35:29Z","title":"BOSS Constraints on Massive Particles during Inflation: The Cosmological Collider in Action","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.01894","snapshot_observed_at":"2026-08-06T21:30:54.527370Z","title":"Cabass, O","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":40,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.527370Z"},"links":{"cited_paper":"/paper/2404.01894","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:f9f93e6ee620093222c1120bb587425b214f3fd1b7c8b92e5e352e78d2463886","observation_id":"43e5637a-9167-4d1f-970d-37c0e4b33df5","resolution":{"observed_at":"2026-08-06T21:30:54.527370Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.01888","last_updated":"2024-12-02T19:00:00Z","snapshot_observed_at":"2026-07-06T20:00:28.112838Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.01888","snapshot_observed_at":"2026-08-06T21:30:54.532095Z","title":null,"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":41,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.532095Z"},"links":{"cited_paper":"/paper/2412.01888","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:02eb31f072fcbe3dce32413c95c69b50716b0d37293731fa9c3873d83d4952e5","observation_id":"2c5c067b-d1c0-4b97-bc48-49935e6864ca","resolution":{"observed_at":"2026-08-06T21:30:54.532095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.07270","last_updated":"2025-03-10T12:50:44Z","snapshot_observed_at":"2026-08-07T17:16:58.784747Z","submitted_at":"2025-03-10T12:50:44Z","title":"Simulation-Based Priors without Simulations: an Analytic Perspective on EFT Parameters of Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.07270","snapshot_observed_at":"2026-08-06T21:30:54.537353Z","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":42,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.537353Z"},"links":{"cited_paper":"/paper/2503.07270","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:0302a7053dcd62d8afc80f7c4753d6e6b0cdc71cb285448186df31735f33ddbc","observation_id":"74198b84-c3a5-435c-be5e-fa10d082c97a","resolution":{"observed_at":"2026-08-06T21:30:54.537353Z","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":"2026-08-06T21:30:54.542883Z","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":"2104.10676","last_updated":"2024-06-10T16:17:53Z","snapshot_observed_at":"2026-08-10T17:15:38.911371Z","submitted_at":"2021-04-21T17:56:55Z","title":"An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.10676","snapshot_observed_at":"2026-08-06T21:30:54.548679Z","title":null,"venue":null,"work_id":null,"year":2021},"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":44,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.548679Z"},"links":{"cited_paper":"/paper/2104.10676","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:49bf7dd297bbe92e7cfd454bbae5473442397fac1bb4b7cf9be49e41d6ed8174","observation_id":"896f3ed7-7609-45dc-a18e-d285c75a3e6f","resolution":{"observed_at":"2026-08-06T21:30:54.548679Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.12398","last_updated":"2023-11-30T11:46:23Z","snapshot_observed_at":"2026-07-06T13:35:06.611122Z","submitted_at":"2022-07-25T17:59:50Z","title":"Modeling HI at the field level","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.12398","snapshot_observed_at":"2026-08-06T21:30:54.555606Z","title":"Obuljen, M","venue":null,"work_id":null,"year":2023},"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":45,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.555606Z"},"links":{"cited_paper":"/paper/2207.12398","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:e93d8560e8d049f5f135700174422612950dc2510d307259650b6d0a26f6272a","observation_id":"39d009c2-ccc9-4728-8e81-cf9683eea983","resolution":{"observed_at":"2026-08-06T21:30:54.555606Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.10270","last_updated":"2023-09-19T02:51:26Z","snapshot_observed_at":"2026-08-02T19:58:25.675391Z","submitted_at":"2023-09-19T02:51:26Z","title":"Hybrid SBI or How I Learned to Stop Worrying and Learn the Likelihood","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.10270","snapshot_observed_at":"2026-08-06T21:30:54.561851Z","title":"Modi and O","venue":null,"work_id":null,"year":2023},"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":46,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.561851Z"},"links":{"cited_paper":"/paper/2309.10270","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:209dda2da403befc0e56941088049007f3b60219364f5bae27a114737ddfcc6a","observation_id":"c551da39-4a9f-4bf7-9ce2-f9ebe6e32f90","resolution":{"observed_at":"2026-08-06T21:30:54.561851Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.08998","last_updated":"2024-10-11T17:09:29Z","snapshot_observed_at":"2026-08-08T04:05:06.475055Z","submitted_at":"2024-10-11T17:09:29Z","title":"Mapping the galaxy-halo connection to the galaxy bias: implication to the HOD-informed prior","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.08998","snapshot_observed_at":"2026-08-06T21:30:54.567911Z","title":"Akitsu, (2024), arXiv:2410.08998 [astro-ph.CO]","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":47,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.567911Z"},"links":{"cited_paper":"/paper/2410.08998","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:76972b148a783999af6cd7a72a67de981afcd4b1651a310df78b092dbc3a19c9","observation_id":"7f33f24b-94f7-46f1-bc80-b5f37e5c6751","resolution":{"observed_at":"2026-08-06T21:30:54.567911Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.12937","last_updated":"2025-03-17T20:04:24Z","snapshot_observed_at":"2026-08-10T15:42:56.793436Z","submitted_at":"2024-09-19T17:48:35Z","title":"HOD-informed prior for EFT-based full-shape analyses of LSS","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.12937","snapshot_observed_at":"2026-08-06T21:30:54.574685Z","title":"Zhang, M","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":48,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.574685Z"},"links":{"cited_paper":"/paper/2409.12937","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:ee964c0d83ed83e99c2715ea9ff3c25205ef8b5712f6bb4220dfc5d0cf88e76a","observation_id":"e75f5742-3386-42f7-b8e1-8b40c8f6d9b7","resolution":{"observed_at":"2026-08-06T21:30:54.574685Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.10407","last_updated":"2025-04-14T16:54:49Z","snapshot_observed_at":"2026-08-07T16:05:48.794754Z","submitted_at":"2025-04-14T16:54:49Z","title":"Enhancing DESI DR1 Full-Shape analyses using HOD-informed priors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.10407","snapshot_observed_at":"2026-08-06T21:30:54.580118Z","title":"Zhang et al","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":49,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.580118Z"},"links":{"cited_paper":"/paper/2504.10407","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:c422879e54bddb7a74af357dbbe98c524d15de9c42969d9e0337eb359e4091f1","observation_id":"7f0724c3-f259-4c4c-9b22-79120d8e7404","resolution":{"observed_at":"2026-08-06T21:30:54.580118Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.13591","last_updated":"2025-05-19T18:00:00Z","snapshot_observed_at":"2026-08-07T15:42:57.961958Z","submitted_at":"2025-05-19T18:00:00Z","title":"Modeling Galaxy Surveys with Hybrid SBI","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.13591","snapshot_observed_at":"2026-08-06T21:30:54.585910Z","title":"Zhang, C","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":50,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.585910Z"},"links":{"cited_paper":"/paper/2505.13591","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:7f1dabd4d9ba4eac8978d3a0b18f5c5f9c8d7bc5b39c72d48b6e4471e1df967c","observation_id":"3875fad6-16e4-4553-928a-bfe10ddb3f19","resolution":{"observed_at":"2026-08-06T21:30:54.585910Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.10640","last_updated":"2019-07-04T13:21:16Z","snapshot_observed_at":"2026-08-09T10:34:43.538421Z","submitted_at":"2018-11-26T19:00:19Z","title":"Modeling Biased Tracers at the Field Level","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.10640","snapshot_observed_at":"2026-08-06T21:30:54.591396Z","title":"Schmittfull, M","venue":null,"work_id":null,"year":2019},"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":51,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.591396Z"},"links":{"cited_paper":"/paper/1811.10640","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:a1e2a4264b4f6739d26efbff247bfe12cad32c2380a52cbabed40850931b6a11","observation_id":"24c3fe6e-9c34-4c03-8e33-53a5387d221b","resolution":{"observed_at":"2026-08-06T21:30:54.591396Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.03334","last_updated":"2020-12-06T17:43:29Z","snapshot_observed_at":"2026-08-10T12:13:09.215902Z","submitted_at":"2020-12-06T17:43:29Z","title":"Modeling Galaxies in Redshift Space at the Field Level","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.03334","snapshot_observed_at":"2026-08-06T21:30:54.597407Z","title":"Schmittfull, M","venue":null,"work_id":null,"year":2021},"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":52,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.597407Z"},"links":{"cited_paper":"/paper/2012.03334","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:bdbbde8850f4150529155c2d2f3d563f1e410deec56c86a76d71beb82f889c67","observation_id":"33b44dfa-d6e4-4610-a6af-c6e8c12f7398","resolution":{"observed_at":"2026-08-06T21:30:54.597407Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.18559","last_updated":"2024-10-25T04:32:08Z","snapshot_observed_at":"2026-08-10T13:50:48.537405Z","submitted_at":"2024-05-28T20:06:01Z","title":"Improving cosmological analyses of HI clustering by reducing stochastic noise","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.18559","snapshot_observed_at":"2026-08-06T21:30:54.602992Z","title":"Foreman, A","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":53,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.602992Z"},"links":{"cited_paper":"/paper/2405.18559","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:6fbe66fe3489f35475c3c9190771f689c9d15521d3ee8b0e907ab96cfa2df94a","observation_id":"c9bb7fb0-d01e-44c3-aff0-38401457e8be","resolution":{"observed_at":"2026-08-06T21:30:54.602992Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.6595","last_updated":"2015-03-06T16:40:43Z","snapshot_observed_at":"2026-08-04T17:21:22.459942Z","submitted_at":"2014-11-24T20:09:24Z","title":"Near optimal bispectrum estimators for large-scale structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.6595","snapshot_observed_at":"2026-08-06T21:30:54.609055Z","title":"Schmittfull, T","venue":null,"work_id":null,"year":2015},"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":54,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.609055Z"},"links":{"cited_paper":"/paper/1411.6595","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:a69879b08951201c9bee9fe753ff7dd58f65ca0d6123890c28c7a9f67e041223","observation_id":"268b9c65-657d-4f74-85d9-e5056529770f","resolution":{"observed_at":"2026-08-06T21:30:54.609055Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.07531","last_updated":"2018-09-10T01:32:00Z","snapshot_observed_at":"2026-08-01T03:41:44.417715Z","submitted_at":"2017-12-20T15:42:04Z","title":"Beyond LIMD bias: a measurement of the complete set of third-order halo bias parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.07531","snapshot_observed_at":"2026-08-06T21:30:54.615708Z","title":"Lazeyras and F","venue":null,"work_id":null,"year":2018},"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":55,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.615708Z"},"links":{"cited_paper":"/paper/1712.07531","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:63507b3a469912081d521a644f20624f5f901eb9e07402b9c45175ba566f4ea9","observation_id":"24fbea34-bc86-405f-a819-f387abd02e52","resolution":{"observed_at":"2026-08-06T21:30:54.615708Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.07622","last_updated":"2018-07-20T17:16:40Z","snapshot_observed_at":"2026-07-06T06:24:34.702383Z","submitted_at":"2018-02-21T15:51:25Z","title":"Cubic Halo Bias in Eulerian and Lagrangian Space","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.07622","snapshot_observed_at":"2026-08-06T21:30:54.621796Z","title":null,"venue":null,"work_id":null,"year":2018},"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":56,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.621796Z"},"links":{"cited_paper":"/paper/1802.07622","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:8e26e3ba6ff1ab18be73145686ca0498577221349e8191e18e133f4f1ba2209c","observation_id":"60d97db2-4312-4cb7-bd71-9cee67f2db23","resolution":{"observed_at":"2026-08-06T21:30:54.621796Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.02002","last_updated":"2019-01-10T17:25:15Z","snapshot_observed_at":"2026-08-06T13:11:43.948659Z","submitted_at":"2018-08-06T17:39:35Z","title":"A rigorous EFT-based forward model for large-scale structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.02002","snapshot_observed_at":"2026-08-06T21:30:54.629657Z","title":"Schmidt, F","venue":null,"work_id":null,"year":2019},"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":57,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.629657Z"},"links":{"cited_paper":"/paper/1808.02002","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:540e7e648df7d7d3f314705c1939e4d2bde63370972f924801795aafe8f88852","observation_id":"4dd19cb1-89c5-4a66-a8ec-bc15004b4f04","resolution":{"observed_at":"2026-08-06T21:30:54.629657Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.07143","last_updated":"2020-01-31T18:20:46Z","snapshot_observed_at":"2026-08-03T17:38:06.385014Z","submitted_at":"2019-06-17T17:31:57Z","title":"Cosmology Inference from Biased Tracers using the EFT-based Likelihood","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.07143","snapshot_observed_at":"2026-08-06T21:30:54.637193Z","title":"Elsner, F","venue":null,"work_id":null,"year":2020},"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":58,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.637193Z"},"links":{"cited_paper":"/paper/1906.07143","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:a8cde05ceb9a91ecc5c94d47d140de1ce8e62871c77e92ab24c2bd5031d65b20","observation_id":"9bbe2620-422f-4e3e-b8c4-3c14ecbb01a3","resolution":{"observed_at":"2026-08-06T21:30:54.637193Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.04022","last_updated":"2020-04-17T13:19:44Z","snapshot_observed_at":"2026-08-08T22:55:16.887227Z","submitted_at":"2019-09-09T17:59:28Z","title":"The EFT Likelihood for Large-Scale Structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.04022","snapshot_observed_at":"2026-08-06T21:30:54.648337Z","title":"Cabass and F","venue":null,"work_id":null,"year":2020},"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":59,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.648337Z"},"links":{"cited_paper":"/paper/1909.04022","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:ef2e8ff776d18de74451abfbc095b104b26248866abb6e3f052ac537b51a6d75","observation_id":"f8508abd-69d8-4873-814f-a3efc9a84c0a","resolution":{"observed_at":"2026-08-06T21:30:54.648337Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.07097","last_updated":"2020-01-23T16:42:55Z","snapshot_observed_at":"2026-08-10T16:47:45.916987Z","submitted_at":"2019-10-15T23:11:34Z","title":"Simulations and symmetries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.07097","snapshot_observed_at":"2026-08-06T21:30:54.660937Z","title":"Modi, S.-F","venue":null,"work_id":null,"year":2020},"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":60,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.660937Z"},"links":{"cited_paper":"/paper/1910.07097","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:71b19a13a04780bd000f14ac9fe95981a41d95a681f8c4f6a0297040cd167a66","observation_id":"3fc4b614-45fa-4ed0-b210-5b2a58ed17a4","resolution":{"observed_at":"2026-08-06T21:30:54.660937Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.14176","last_updated":"2021-04-22T07:59:37Z","snapshot_observed_at":"2026-08-10T06:52:56.071783Z","submitted_at":"2020-09-29T17:41:51Z","title":"Sigma-Eight at the Percent Level: The EFT Likelihood in Real Space","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.14176","snapshot_observed_at":"2026-08-06T21:30:54.667686Z","title":"Schmidt, (2020), arXiv:2009.14176 [astro-ph.CO]","venue":null,"work_id":null,"year":2020},"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":61,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.667686Z"},"links":{"cited_paper":"/paper/2009.14176","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:9c1685a621da630806e01b4947dabd341461aaf6db7b8cefd09554a74210a324","observation_id":"ee59ae21-c76f-4542-a9f4-8b72315fccce","resolution":{"observed_at":"2026-08-06T21:30:54.667686Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.06707","last_updated":"2020-11-05T16:59:32Z","snapshot_observed_at":"2026-08-07T12:18:47.666450Z","submitted_at":"2020-04-14T17:56:45Z","title":"Unbiased Cosmology Inference from Biased Tracers using the EFT Likelihood","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.06707","snapshot_observed_at":"2026-08-06T21:30:54.674478Z","title":"Schmidt, G","venue":null,"work_id":null,"year":2020},"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":62,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.674478Z"},"links":{"cited_paper":"/paper/2004.06707","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:cdab467a5cc8a4e693ca1259529ac3b9a017d7ae147ce172959fda33511dc521","observation_id":"97896322-91fb-4021-aabe-08260ee25bb3","resolution":{"observed_at":"2026-08-06T21:30:54.674478Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.14713","last_updated":"2021-11-08T09:26:38Z","snapshot_observed_at":"2026-07-06T11:23:47.260847Z","submitted_at":"2021-06-28T13:44:34Z","title":"Assembly bias in quadratic bias parameters of dark matter halos from forward modeling","version":2},"cited_work":{"arxiv_id":"2106.14713","doi":null,"metadata_source":"pith","pith_arxiv_id":"2106.14713","snapshot_observed_at":"2026-08-06T21:30:56.891367Z","title":"Assembly bias in quadratic bias parameters of dark matter halos from forward modeling","venue":"astro-ph.CO","work_id":"fb985e21-645b-419f-88bb-817c99bce695","year":2021},"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":63,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.683333Z"},"links":{"cited_paper":"/paper/2106.14713","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:01034b7d02e7d5ee599c6f28f9beee4c8aea83147e20517443ca925a3a2d6f54","observation_id":"1b0303b6-899e-4907-b62e-e77ce9613cd5","resolution":{"observed_at":"2026-08-06T21:30:56.904024Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2303.09876","last_updated":"2023-10-30T13:10:47Z","snapshot_observed_at":"2026-08-10T16:47:30.625655Z","submitted_at":"2023-03-17T10:43:36Z","title":"Cosmology inference at the field level from biased tracers in redshift-space","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.09876","snapshot_observed_at":"2026-08-06T21:30:54.690215Z","title":"Stadler, F","venue":null,"work_id":null,"year":2023},"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":64,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.690215Z"},"links":{"cited_paper":"/paper/2303.09876","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:0b12d66c5bf229a5a5daa5f8697189e8d3608b8fb8cd09ff3da117797ba377fb","observation_id":"ebb1a074-51bf-4296-99a9-0fe0f4c4d64c","resolution":{"observed_at":"2026-08-06T21:30:54.690215Z","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":"2009.10106","last_updated":"2021-02-13T22:56:26Z","snapshot_observed_at":"2026-08-09T07:58:36.443765Z","submitted_at":"2020-09-21T18:05:16Z","title":"Constraints on the curvature of the Universe and dynamical dark energy from the Full-shape and BAO data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.10106","snapshot_observed_at":"2026-08-06T21:30:54.702515Z","title":"Chudaykin, K","venue":null,"work_id":null,"year":2021},"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":66,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.702515Z"},"links":{"cited_paper":"/paper/2009.10106","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:a64cf295ee1515c0da3a6756f916929dc1764f54fc35e60df778fb9137234f2e","observation_id":"dc0cc32c-601e-4caa-ac83-26a2141b1c88","resolution":{"observed_at":"2026-08-06T21:30:54.702515Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.03311","last_updated":"2021-01-18T16:33:19Z","snapshot_observed_at":"2026-07-06T09:53:36.874865Z","submitted_at":"2020-09-07T18:00:00Z","title":"Fewer Mocks and Less Noise: Reducing the Dimensionality of Cosmological Observables with Subspace Projections","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.03311","snapshot_observed_at":"2026-08-06T21:30:54.709787Z","title":null,"venue":null,"work_id":null,"year":2021},"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":67,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.709787Z"},"links":{"cited_paper":"/paper/2009.03311","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:002adc3686db35efafdd03069a2908948443c57c663e2e04d9dff355a298b503","observation_id":"fa74b654-37d8-4dce-9900-b53cf2b137fb","resolution":{"observed_at":"2026-08-06T21:30:54.709787Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-06T21:30:54.714968Z","title":"Aghanim et al","venue":null,"work_id":null,"year":2020},"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":68,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.714968Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:925e61b97818330ba8e46eb99f406db7a602d6049444196287dc72e71ab48e27","observation_id":"5c13206e-b906-4b19-8100-7f81b66174d7","resolution":{"observed_at":"2026-08-06T21:30:54.714968Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03863","last_updated":"2022-02-07T19:00:01Z","snapshot_observed_at":"2026-07-06T12:16:15.735863Z","submitted_at":"2021-12-07T17:57:21Z","title":"The Pantheon+ Analysis: The Full Dataset and Light-Curve Release","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.03863","snapshot_observed_at":"2026-08-06T21:30:54.721619Z","title":"Scolnic et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.00118","last_updated":"2025-06-30T18:00:01Z","snapshot_observed_at":"2026-08-08T17:58:16.664935Z","submitted_at":"2025-06-30T18:00:01Z","title":"Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.721619Z"},"links":{"cited_paper":"/paper/2112.03863","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:b74f7a749971155c32d3872119358a25033f3929d17693c05034cfe918c8a16e","observation_id":"10738bcc-2e83-4a36-8f49-a8a94afecda7","resolution":{"observed_at":"2026-08-06T21:30:54.721619Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.04077","last_updated":"2022-11-14T21:28:25Z","snapshot_observed_at":"2026-08-01T22:04:41.273741Z","submitted_at":"2022-02-08T19:00:00Z","title":"The Pantheon+ Analysis: Cosmological Constraints","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.04077","snapshot_observed_at":"2026-08-06T21:30:54.731173Z","title":"Brout et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.00118","last_updated":"2025-06-30T18:00:01Z","snapshot_observed_at":"2026-08-08T17:58:16.664935Z","submitted_at":"2025-06-30T18:00:01Z","title":"Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.731173Z"},"links":{"cited_paper":"/paper/2202.04077","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:a9889e2d2bd679fd2e2fd0e2ddcff1deb5b779df9c445858d74c2c47fb5af1b4","observation_id":"e97eae9b-02e2-47cc-969a-9532b57029a0","resolution":{"observed_at":"2026-08-06T21:30:54.731173Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.08208","last_updated":"2019-12-17T19:00:01Z","snapshot_observed_at":"2026-08-10T01:25:50.914023Z","submitted_at":"2019-12-17T19:00:01Z","title":"Cosmological Parameters and Neutrino Masses from the Final Planck and Full-Shape BOSS Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.08208","snapshot_observed_at":"2026-08-06T21:30:54.738095Z","title":null,"venue":null,"work_id":null,"year":2020},"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":71,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.738095Z"},"links":{"cited_paper":"/paper/1912.08208","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:0b55c54582d5ebe225eb3e1a48952645d9f7d451f3d6a52c31207c706179941a","observation_id":"d7274eac-984c-423f-9ba1-db78ab7cd6c9","resolution":{"observed_at":"2026-08-06T21:30:54.738095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10724","last_updated":"2021-02-13T22:42:18Z","snapshot_observed_at":"2026-08-05T04:39:36.105770Z","submitted_at":"2020-09-22T18:00:00Z","title":"Optimizing large-scale structure data analysis with the theoretical error likelihood","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.10724","snapshot_observed_at":"2026-08-06T21:30:54.750452Z","title":"Chudaykin, M","venue":null,"work_id":null,"year":2021},"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":72,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.750452Z"},"links":{"cited_paper":"/paper/2009.10724","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:5191c910d6cc67e34ec9b97ebe27c8ad3ef3461f749bfe50670054347954b482","observation_id":"471ea66b-8d38-4fdf-a939-27ea97bfef10","resolution":{"observed_at":"2026-08-06T21:30:54.750452Z","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":"2026-07-06T11:59:39.730712Z","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":"2026-08-08T17:58:16.664935Z","submitted_at":"2025-06-30T18:00:01Z","title":"Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors","version":1},"reference_index":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":"sha256:56b9219c2f6c7207148d0e816aecb80e99b037783a82889876289fc1da0b121e","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:30:54.762212Z","title":"Bernardeau, S","venue":null,"work_id":null,"year":2002},"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":74,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.762212Z"},"links":{"citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:40c1d85c4e0c2b606038ba7c16a1f887af032ce262713e19bee359d2c66d8ad5","observation_id":"4335c02e-2b44-4be0-b32f-2a9e0b4c9093","resolution":{"observed_at":"2026-08-06T21:30:54.762212Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.10607","last_updated":"2020-08-29T14:33:20Z","snapshot_observed_at":"2026-08-09T03:17:43.880995Z","submitted_at":"2020-04-22T14:46:20Z","title":"Non-linear perturbation theory extension of the Boltzmann code CLASS","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.10607","snapshot_observed_at":"2026-08-06T21:30:54.771030Z","title":"Chudaykin, M","venue":null,"work_id":null,"year":2020},"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":75,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.771030Z"},"links":{"cited_paper":"/paper/2004.10607","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:11dd3eb212c8a9dfd0176cab368bcbfc47bba30b484a1e932ecda6db1524ca1f","observation_id":"4a6035af-076d-4dd6-8c24-1d27a0bf4f8d","resolution":{"observed_at":"2026-08-06T21:30:54.771030Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.07379","last_updated":"2024-07-24T08:58:52Z","snapshot_observed_at":"2026-08-10T03:28:28.062331Z","submitted_at":"2023-08-14T18:02:37Z","title":"The two-loop power spectrum in redshift space","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.07379","snapshot_observed_at":"2026-08-06T21:30:54.776062Z","title":"Taule and M","venue":null,"work_id":null,"year":2023},"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":76,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.776062Z"},"links":{"cited_paper":"/paper/2308.07379","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:326bd720280a1173ae595425dd02a58f3e445a981efa89aa370b4e9ebd535d73","observation_id":"60615dd3-48a2-4e3c-9fd8-73ed8c313026","resolution":{"observed_at":"2026-08-06T21:30:54.776062Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0810.3908","last_updated":"2008-10-21T19:47:59Z","snapshot_observed_at":"2026-07-06T01:46:49.973926Z","submitted_at":"2008-10-21T19:47:59Z","title":"Fingers of God","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0810.3908","snapshot_observed_at":"2026-08-06T21:30:54.782634Z","title":null,"venue":null,"work_id":null,"year":1972},"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":77,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.782634Z"},"links":{"cited_paper":"/paper/0810.3908","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:fabaabb7fd98234447ac0827f043d1caa0e70874f852f403fd53d21baeee691f","observation_id":"24ea5e24-4408-4f56-b870-b761f369dc1e","resolution":{"observed_at":"2026-08-06T21:30:54.782634Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09321","last_updated":"2016-10-28T17:22:23Z","snapshot_observed_at":"2026-08-01T20:41:49.868020Z","submitted_at":"2016-10-28T17:22:23Z","title":"Biased Tracers in Redshift Space in the EFT of Large-Scale Structure","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09321","snapshot_observed_at":"2026-08-06T21:30:54.792128Z","title":"Perko, L","venue":null,"work_id":null,"year":2016},"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":78,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.792128Z"},"links":{"cited_paper":"/paper/1610.09321","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:8ccdacdfd7b6be34314480796b5234c9d51d4d29336aa432c4e25c15425abd94","observation_id":"d4e5bc7f-97e2-45f3-a19e-503163d0b5d6","resolution":{"observed_at":"2026-08-06T21:30:54.792128Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1208.0022","last_updated":"2012-11-07T22:32:13Z","snapshot_observed_at":"2026-07-06T02:52:54.937210Z","submitted_at":"2012-07-31T20:05:09Z","title":"The Baryon Oscillation Spectroscopic Survey of SDSS-III","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.0022","snapshot_observed_at":"2026-08-06T21:30:54.798320Z","title":null,"venue":null,"work_id":null,"year":2013},"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":79,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.798320Z"},"links":{"cited_paper":"/paper/1208.0022","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:66f3bcaa3490f511d14949f75bde156c8c1e3c71832b48ec6af9b228423bffcd","observation_id":"07eab98a-09c6-4136-9572-3ba60e69d0b3","resolution":{"observed_at":"2026-08-06T21:30:54.798320Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.00006","last_updated":"2022-02-23T16:12:49Z","snapshot_observed_at":"2026-08-09T03:38:49.191527Z","submitted_at":"2021-09-30T18:00:00Z","title":"Cosmological constraints without fingers of God","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.00006","snapshot_observed_at":"2026-08-06T21:30:54.805234Z","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":"2026-08-08T17:58:16.664935Z","submitted_at":"2025-06-30T18:00:01Z","title":"Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.805234Z"},"links":{"cited_paper":"/paper/2110.00006","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:ad606b4a3650f47be4ddf6a40ba9f5d191e40421248e7b63a31deb24b34d2091","observation_id":"16c4482b-0daa-4204-b43e-394505bff32a","resolution":{"observed_at":"2026-08-06T21:30:54.805234Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.04035","last_updated":"2020-05-13T19:13:00Z","snapshot_observed_at":"2026-08-04T17:00:41.192234Z","submitted_at":"2020-02-10T19:00:00Z","title":"Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.04035","snapshot_observed_at":"2026-08-06T21:30:54.812184Z","title":null,"venue":null,"work_id":null,"year":2020},"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":81,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.812184Z"},"links":{"cited_paper":"/paper/2002.04035","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:ad3e38db6a98d1f1f6cad543c7ec54b8d04268426a093c49739b72453d70f34e","observation_id":"aea6ea0a-5e8f-44c1-9603-e1d8b2fb390c","resolution":{"observed_at":"2026-08-06T21:30:54.812184Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:30:54.821297Z","title":"Chudaykin, M","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":82,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.821297Z"},"links":{"citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:f167a973ff2129663ea67b5043a372d65cbd41d0f005774031f0e1c2bd626cdb","observation_id":"7d2b3e01-f1f3-426e-9a74-1aacf2d8e193","resolution":{"observed_at":"2026-08-06T21:30:54.821297Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.09389","last_updated":"2021-04-05T23:07:08Z","snapshot_observed_at":"2026-07-06T10:25:17.556512Z","submitted_at":"2020-12-17T04:43:09Z","title":"Cosmology Without Windows: Quadratic Estimators for the Galaxy Power Spectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.09389","snapshot_observed_at":"2026-08-06T21:30:54.828529Z","title":null,"venue":null,"work_id":null,"year":2021},"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":83,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.828529Z"},"links":{"cited_paper":"/paper/2012.09389","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:ab6b6bfdf092eb3d390a0d1b78e82a1df8de65f53db1618f9100b0fdddb7135b","observation_id":"feb42ea7-1112-41c4-9b90-4b6c4baf9870","resolution":{"observed_at":"2026-08-06T21:30:54.828529Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.06287","last_updated":"2021-10-03T15:15:49Z","snapshot_observed_at":"2026-08-10T17:46:35.361762Z","submitted_at":"2021-07-13T18:00:00Z","title":"Cosmology Without Window Functions: Cubic Estimators for the Galaxy Bispectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.06287","snapshot_observed_at":"2026-08-06T21:30:54.838718Z","title":null,"venue":null,"work_id":null,"year":2021},"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":84,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.838718Z"},"links":{"cited_paper":"/paper/2107.06287","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:990dc90672c5fb1a0acfa128cefbcb2ba73407c38912cc34b1728e8541997f7e","observation_id":"e9cbe3ab-4b42-4b37-bea1-3bc084944636","resolution":{"observed_at":"2026-08-06T21:30:54.838718Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.12021","last_updated":"2025-11-24T12:55:36Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-11-18T20:03:34Z","title":"DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.12021","snapshot_observed_at":"2026-08-06T21:30:54.846038Z","title":null,"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":85,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.846038Z"},"links":{"cited_paper":"/paper/2411.12021","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:9ea7675f4be7a1f82e18489aa62b6012e3816cef35612de23dfbb8cbee6d59ef","observation_id":"1955ea4f-5e9b-41b3-bac6-e9d22992b121","resolution":{"observed_at":"2026-08-06T21:30:54.846038Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.12875","last_updated":"2020-09-15T15:02:27Z","snapshot_observed_at":"2026-07-06T08:11:09.285762Z","submitted_at":"2019-07-30T13:11:32Z","title":"Planck 2018 results. V. CMB power spectra and likelihoods","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.12875","snapshot_observed_at":"2026-08-06T21:30:54.852722Z","title":"Aghanim et al","venue":null,"work_id":null,"year":2020},"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":86,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.852722Z"},"links":{"cited_paper":"/paper/1907.12875","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:40037bbf5333e172559e13bc7df605dafde5d866402a07841a11e6e16c127583","observation_id":"0f0ef580-eb69-4d93-a027-d070f2668a19","resolution":{"observed_at":"2026-08-06T21:30:54.852722Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06205","last_updated":"2019-12-03T18:36:28Z","snapshot_observed_at":"2026-08-06T20:42:17.427266Z","submitted_at":"2018-07-17T04:05:03Z","title":"Planck 2018 results. I. Overview and the cosmological legacy of Planck","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06205","snapshot_observed_at":"2026-08-06T21:30:54.862860Z","title":"Aghanim et al","venue":null,"work_id":null,"year":2020},"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":87,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.862860Z"},"links":{"cited_paper":"/paper/1807.06205","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:79d7eecb080368b100e5ca9cc81bdaaec549f7830986bdb646de9f118b3e5022","observation_id":"a361211a-4f7e-4633-b3cd-beb865f8577f","resolution":{"observed_at":"2026-08-06T21:30:54.862860Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0609591","last_updated":"2006-09-20T21:20:16Z","snapshot_observed_at":"2026-07-07T01:03:10.885429Z","submitted_at":"2006-09-20T21:20:16Z","title":"Report of the Dark Energy Task Force","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0609591","snapshot_observed_at":"2026-08-06T21:30:54.876685Z","title":"Albrecht et al","venue":null,"work_id":null,"year":2006},"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":88,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.876685Z"},"links":{"cited_paper":"/paper/astro-ph/0609591","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:52d5890c4f845d48214087bce463955e43f8cb0a279232f0435b42f4f9c33cc8","observation_id":"06a98ab0-a570-4f88-b815-401737bf7649","resolution":{"observed_at":"2026-08-06T21:30:54.876685Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.04430","last_updated":"2025-03-22T21:18:35Z","snapshot_observed_at":"2026-08-04T09:40:08.517363Z","submitted_at":"2024-12-05T18:52:01Z","title":"Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\\Omega_m$ and $H_0$ Across Cosmological Probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.04430","snapshot_observed_at":"2026-08-06T21:30:54.881986Z","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":89,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.881986Z"},"links":{"cited_paper":"/paper/2412.04430","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:f1f73639a69e17380ce2f5e513c65d150c665bb986c47eb7fd332f617fddbcbd","observation_id":"dceb52c2-cde5-4240-afc1-e657ca23729c","resolution":{"observed_at":"2026-08-06T21:30:54.881986Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:30:54.889632Z","title":"Sailer, G","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":90,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.889632Z"},"links":{"citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:aae8cdb866a5e7e69cc59c9d96f4b21bccfb5ee96f0afdfab0016b8fcf6a3306","observation_id":"af26d374-4a05-41cc-b922-e983d4d7cd4e","resolution":{"observed_at":"2026-08-06T21:30:54.889632Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.09664","last_updated":"2022-04-16T18:07:09Z","snapshot_observed_at":"2026-08-07T04:48:01.703217Z","submitted_at":"2021-07-20T17:59:59Z","title":"Cosmological Constraints on Light (but Massive) Relics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.09664","snapshot_observed_at":"2026-08-06T21:30:54.897815Z","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":"2026-08-08T17:58:16.664935Z","submitted_at":"2025-06-30T18:00:01Z","title":"Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.897815Z"},"links":{"cited_paper":"/paper/2107.09664","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:3f201f9746ad18e494c4b115ef8164e70d9f84a5f8f14cf67b8a3049743eb2f4","observation_id":"25d43ac1-3d9a-4c54-b1e1-9f92b853261e","resolution":{"observed_at":"2026-08-06T21:30:54.897815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.08361","last_updated":"2023-05-18T21:48:48Z","snapshot_observed_at":"2026-07-06T14:43:00.671754Z","submitted_at":"2023-01-19T23:48:56Z","title":"Ultra-light axions and the $S_8$ tension: joint constraints from the cosmic microwave background and galaxy clustering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.08361","snapshot_observed_at":"2026-08-06T21:30:54.928895Z","title":null,"venue":null,"work_id":null,"year":2023},"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":92,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.928895Z"},"links":{"cited_paper":"/paper/2301.08361","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:29548665d007dac32e2489ebcdcad372fb135a43892eec1077139de0ce63a32b","observation_id":"6776c901-a329-4d7f-ab84-35a47692929f","resolution":{"observed_at":"2026-08-06T21:30:54.928895Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.08260","last_updated":"2023-05-30T17:03:02Z","snapshot_observed_at":"2026-07-06T14:42:57.101630Z","submitted_at":"2023-01-19T19:00:01Z","title":"$S_8$ Tension in the Context of Dark Matter-Baryon Scattering","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.08260","snapshot_observed_at":"2026-08-06T21:30:54.937966Z","title":null,"venue":null,"work_id":null,"year":2023},"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":93,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.937966Z"},"links":{"cited_paper":"/paper/2301.08260","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:11df5fc770dc7b8019011c5f6f3ca881a1befb040262dd6cb5901f4f6c5b6202","observation_id":"2936a765-fc6b-48a2-a874-9b2b431f128c","resolution":{"observed_at":"2026-08-06T21:30:54.937966Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.03956","last_updated":"2024-05-30T20:50:50Z","snapshot_observed_at":"2026-08-09T19:18:18.491643Z","submitted_at":"2023-09-07T18:03:53Z","title":"Self-Interacting Neutrinos in Light of Large-Scale Structure Data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.03956","snapshot_observed_at":"2026-08-06T21:30:54.943883Z","title":null,"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":94,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.943883Z"},"links":{"cited_paper":"/paper/2309.03956","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:dcbecbaad53de5bcdd3493e540550ea5267992954d9a8b835b7090efdf634678","observation_id":"ae889dbe-7ed5-4ee6-9d98-eb51b08a0ad5","resolution":{"observed_at":"2026-08-06T21:30:54.943883Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.02636","last_updated":"2025-05-31T03:47:43Z","snapshot_observed_at":"2026-08-09T18:09:46.064864Z","submitted_at":"2025-02-04T19:00:01Z","title":"Bounds on Velocity-Dependent Dark Matter-Baryon Scattering from Large-Scale Structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.02636","snapshot_observed_at":"2026-08-06T21:30:54.952619Z","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":95,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.952619Z"},"links":{"cited_paper":"/paper/2502.02636","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:565586295b557dbd11924d9b244ecfc55ac9635aa854b0c40db897c7dca3b87e","observation_id":"aa32c113-7843-4f99-a6af-2dca5d223134","resolution":{"observed_at":"2026-08-06T21:30:54.952619Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.11235","last_updated":"2020-10-07T17:52:42Z","snapshot_observed_at":"2026-08-10T12:09:38.817443Z","submitted_at":"2020-06-19T17:15:28Z","title":"Constraining Early Dark Energy with Large-Scale Structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.11235","snapshot_observed_at":"2026-08-06T21:30:54.963624Z","title":null,"venue":null,"work_id":null,"year":2020},"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":96,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.963624Z"},"links":{"cited_paper":"/paper/2006.11235","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:a35b5b59fd0276e6cea840b3d21f09db2f43bbb5997b9b308aac9a715e2e2333","observation_id":"6ee0b670-4b72-4528-9c04-e3036eef26df","resolution":{"observed_at":"2026-08-06T21:30:54.963624Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.19899","last_updated":"2023-10-30T18:09:28Z","snapshot_observed_at":"2026-08-10T12:09:26.434747Z","submitted_at":"2023-10-30T18:09:28Z","title":"Observational constraints on early dark energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.19899","snapshot_observed_at":"2026-08-06T21:30:54.972872Z","title":"McDonough, J","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":97,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.972872Z"},"links":{"cited_paper":"/paper/2310.19899","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:1a84f0709f3f36433bd9e3727bfccf07c7deae04f1d77d1b946d1b7cb48e01c1","observation_id":"c5a782d2-dd8c-4258-ab35-7e6311778b24","resolution":{"observed_at":"2026-08-06T21:30:54.972872Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.09029","last_updated":"2024-09-13T17:55:48Z","snapshot_observed_at":"2026-08-10T16:26:04.112939Z","submitted_at":"2024-09-13T17:55:48Z","title":"Learning Theory Informed Priors for Bayesian Inference: A Case Study with Early Dark Energy","version":1},"cited_work":{"arxiv_id":"2409.09029","doi":null,"metadata_source":"pith","pith_arxiv_id":"2409.09029","snapshot_observed_at":"2026-08-06T21:30:55.426207Z","title":"Learning Theory Informed Priors for Bayesian Inference: A Case Study with Early Dark Energy","venue":"astro-ph.CO","work_id":"da023d0c-8bff-4fcb-911e-4840712d4ad8","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":98,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.978829Z"},"links":{"cited_paper":"/paper/2409.09029","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:0f42b4db17f42cf62d19a6b3a795434de490232923b794efb5c23c93a020a4f8","observation_id":"324792a2-152c-4057-895a-97f1ad8f17a5","resolution":{"observed_at":"2026-08-06T21:30:55.435171Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.10133","last_updated":"2024-01-03T14:12:04Z","snapshot_observed_at":"2026-08-09T09:37:49.337500Z","submitted_at":"2023-09-18T20:13:33Z","title":"Don't miss the forest for the trees: the Lyman alpha forest power spectrum in effective field theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.10133","snapshot_observed_at":"2026-08-06T21:30:54.985193Z","title":null,"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":99,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.985193Z"},"links":{"cited_paper":"/paper/2309.10133","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:90ac71e34987d31512a1d2eddf0d3251a74cf0cacd6f2f2971525162fc599562","observation_id":"d1435927-83d1-465f-84b0-039d03b1b317","resolution":{"observed_at":"2026-08-06T21:30:54.985193Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13208","last_updated":"2025-02-20T16:25:30Z","snapshot_observed_at":"2026-07-06T18:17:38.280988Z","submitted_at":"2024-05-21T21:23:29Z","title":"Fundamental physics with the Lyman-alpha forest: constraints on the growth of structure and neutrino masses from SDSS with effective field theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.13208","snapshot_observed_at":"2026-08-06T21:30:54.992988Z","title":null,"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":100,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.992988Z"},"links":{"cited_paper":"/paper/2405.13208","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:7b729f1f3e155ed71c6129551bc3f9f86f099e28f5896a0fa9cc3e94a977b58b","observation_id":"34a3ceae-d536-4fed-a7b0-6d2733582732","resolution":{"observed_at":"2026-08-06T21:30:54.992988Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2507.00118","last_updated":"2025-06-30T18:00:01Z","latest_version":1,"primary_category":"astro-ph.CO","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"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":98,"verified_exact":2,"verified_fuzzy":0},"total_outbound_references":104},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 100 of 104 outbound references and 7 inbound Pith citation observations for arXiv:2507.00118."}