{"as_of":"2026-08-07T19:46:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ac4145acbe3437a8d4c247917736d7309b814fe5f551a9b4c5f4ab109480c1fd","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":14,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":14,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":14,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":14,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T21:30:54.567911Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":3,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2410.08998","last_updated":"2024-10-11T17:09:29Z","snapshot_observed_at":"2026-07-06T19:31:57.906994Z","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":"2026-08-07T11:10:22.278337Z","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":"sha256:1a4c2fa3979dafd8ab1ad6b05499799f55af6a856cd932855b890c6806346e1e","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":"2410.08998","last_updated":"2024-10-11T17:09:29Z","snapshot_observed_at":"2026-07-06T19:31:57.906994Z","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":"2026-08-06T21:27:28.262325Z","title":"Akitsu, Mapping the galaxy-halo connection to the galaxy bias: implication to the HOD-informed prior , 2410.08998","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.00284","last_updated":"2025-06-30T21:53:00Z","snapshot_observed_at":"2026-08-06T21:42:00.012527Z","submitted_at":"2025-06-30T21:53:00Z","title":"Modeling the Cosmological Lyman-$\\alpha$ Forest at the Field Level","version":1},"reference_index":118,"source":"pdf_text","source_observed_at":"2026-08-06T21:27:28.262325Z"},"links":{"cited_paper":"/paper/2410.08998","citing_paper":"/paper/2507.00284"},"observation_digest":"sha256:42f39f5bd7b7e858458888b44b6ba25ce0718ce7892696066edcd4652c10d758","observation_id":"3e57e8fb-2306-4a62-b71c-511b949e8003","resolution":{"observed_at":"2026-08-06T21:27:28.262325Z","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":"2026-07-06T19:31:57.906994Z","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":"2026-08-06T19:34:11.494695Z","title":"Akitsu, Mapping the galaxy-halo connection to the galaxy bias: implication to the HOD-informed prior, (2024), arXiv:2410.08998 [astro-ph.CO]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.05378","last_updated":"2025-07-07T18:04:52Z","snapshot_observed_at":"2026-08-07T11:23:16.450335Z","submitted_at":"2025-07-07T18:04:52Z","title":"Equivalence of the field-level inference and conventional analyses on large scales","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-06T19:34:11.494695Z"},"links":{"cited_paper":"/paper/2410.08998","citing_paper":"/paper/2507.05378"},"observation_digest":"sha256:c785e8d1a68f9bc4d477984163c3bf43442c00f6699757a672a49d4effbe1648","observation_id":"a33fa0b9-46e3-4425-8aa2-e79042eb2c73","resolution":{"observed_at":"2026-08-06T19:34:11.494695Z","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":"2026-07-06T19:31:57.906994Z","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":"2026-08-06T12:12:39.899404Z","title":"Akitsu, (2024), arXiv:2410.08998 [astro-ph.CO]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.22110","last_updated":"2026-07-22T14:21:38Z","snapshot_observed_at":"2026-08-06T22:13:22.612779Z","submitted_at":"2025-07-29T18:00:00Z","title":"One-Loop Galaxy Bispectrum: Consistent Theory, Efficient Analysis with COBRA, and Implications for Cosmological Parameters","version":4},"reference_index":109,"source":"pdf_text","source_observed_at":"2026-08-06T12:12:39.899404Z"},"links":{"cited_paper":"/paper/2410.08998","citing_paper":"/paper/2507.22110"},"observation_digest":"sha256:4a0a941972e8c08f7e764d201f571cfd2777abcde2d3ef60c670f245fd4feb65","observation_id":"79ab415c-a1d7-4326-afec-3a46c0929973","resolution":{"observed_at":"2026-08-06T12:12:39.899404Z","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":"2026-07-06T19:31:57.906994Z","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":"2026-08-03T08:42:10.856535Z","title":"Akitsu, (2024), arXiv:2410.08998 [astro-ph.CO]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2601.16165","last_updated":"2026-07-22T13:53:51Z","snapshot_observed_at":"2026-08-05T15:31:32.728995Z","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":209,"source":"pdf_text","source_observed_at":"2026-08-03T08:42:10.856535Z"},"links":{"cited_paper":"/paper/2410.08998","citing_paper":"/paper/2601.16165"},"observation_digest":"sha256:97277138ff471878a759a32c038172fdb76b0bf5f94af4dfb36cca2b31afd1ec","observation_id":"e90c15cf-f915-461c-8572-77cb4b0dfb61","resolution":{"observed_at":"2026-08-03T08:42:10.856535Z","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":"2026-07-06T19:31:57.906994Z","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":"2026-08-02T22:01:22.114264Z","title":"Akitsu, (2024), arXiv:2410.08998 [astro-ph.CO]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2602.18554","last_updated":"2026-07-18T17:18:40Z","snapshot_observed_at":"2026-08-07T15:21:25.685152Z","submitted_at":"2026-02-20T19:00:00Z","title":"Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-02T22:01:22.114264Z"},"links":{"cited_paper":"/paper/2410.08998","citing_paper":"/paper/2602.18554"},"observation_digest":"sha256:5da414dbc3c444075cdad1dec67e9a24096a9a596917266d93564b78ccc1d71b","observation_id":"2e1e9bfb-f322-4d95-bd7e-c02c8082a32f","resolution":{"observed_at":"2026-08-02T22:01:22.114264Z","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":"2026-07-06T19:31:57.906994Z","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":"2026-07-14T21:55:54.028883Z","title":"Akitsu, Mapping the galaxy-halo connection to the galaxy bias: implication to the hod-informed prior (2024), arXiv:2410.08998 [astro-ph.CO]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.13030","last_updated":"2026-07-01T15:32:03Z","snapshot_observed_at":"2026-07-14T21:55:53.060873Z","submitted_at":"2026-03-13T14:42:17Z","title":"Floquet Dissipative Phase Transitions","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-07-14T21:55:54.028883Z"},"links":{"cited_paper":"/paper/2410.08998","citing_paper":"/paper/2603.13030"},"observation_digest":"sha256:18a5cfe7aae445d231700d983c8262a1d69b095a4226019d3398f99ebf1ef745","observation_id":"4ca6d0ad-dd6a-4a9e-b453-7541e74b007b","resolution":{"observed_at":"2026-07-14T21:55:54.028883Z","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":"2026-07-06T19:31:57.906994Z","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":"2410.08998","doi":"10.48550/arxiv.2410.08998","metadata_source":"arxiv_reference","pith_arxiv_id":"2410.08998","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Akitsu, Mapping the galaxy-halo connection to the galaxy bias: implication to the HOD-informed prior (2024), arXiv:2410.08998 [astro-ph.CO]","venue":"arXiv (Cornell University)","work_id":"f6ba542c-2a3e-4e86-9f30-79de69d0c8d8","year":2024},"citing_paper":{"arxiv_id":"2604.25171","last_updated":"2026-05-05T18:16:20Z","snapshot_observed_at":"2026-07-06T23:11:07.254460Z","submitted_at":"2026-04-28T03:20:00Z","title":"Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-05-07T15:27:13.991071Z"},"links":{"cited_paper":"/paper/2410.08998","citing_paper":"/paper/2604.25171"},"observation_digest":"sha256:129df3e00a1ba0eee11785b6e66bde001bd746f2235caf9c5993a130a795e8e4","observation_id":"cd317e35-1f41-4d6c-8e75-a3ce4a058058","resolution":{"observed_at":"2026-05-12T00:21:26.449421Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.08998","last_updated":"2024-10-11T17:09:29Z","snapshot_observed_at":"2026-07-06T19:31:57.906994Z","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":"2410.08998","doi":"10.48550/arxiv.2410.08998","metadata_source":"arxiv_reference","pith_arxiv_id":"2410.08998","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Akitsu, Mapping the galaxy-halo connection to the galaxy bias: implication to the HOD-informed prior (2024), arXiv:2410.08998 [astro-ph.CO]","venue":"arXiv (Cornell University)","work_id":"f6ba542c-2a3e-4e86-9f30-79de69d0c8d8","year":2024},"citing_paper":{"arxiv_id":"2604.25171","last_updated":"2026-05-05T18:16:20Z","snapshot_observed_at":"2026-07-06T23:11:07.254460Z","submitted_at":"2026-04-28T03:20:00Z","title":"Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-05-08T03:31:29.946089Z"},"links":{"cited_paper":"/paper/2410.08998","citing_paper":"/paper/2604.25171"},"observation_digest":"sha256:02aeb310bbe89ffd4372b48fe953bd63883d8c252958f4c7c2206e710d7cfdf5","observation_id":"2d1f3721-19cd-4f89-aac8-814bc89f6bf9","resolution":{"observed_at":"2026-05-11T22:01:13.758138Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.08998","last_updated":"2024-10-11T17:09:29Z","snapshot_observed_at":"2026-07-06T19:31:57.906994Z","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":"2410.08998","doi":"10.48550/arxiv.2410.08998","metadata_source":"arxiv_reference","pith_arxiv_id":"2410.08998","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Akitsu, Mapping the galaxy-halo connection to the galaxy bias: implication to the HOD-informed prior (2024), arXiv:2410.08998 [astro-ph.CO]","venue":"arXiv (Cornell University)","work_id":"f6ba542c-2a3e-4e86-9f30-79de69d0c8d8","year":2024},"citing_paper":{"arxiv_id":"2605.13298","last_updated":"2026-05-13T10:12:06Z","snapshot_observed_at":"2026-08-03T01:12:04.794816Z","submitted_at":"2026-05-13T10:12:06Z","title":"Probing nonlinear structure formation beyond $\\Lambda$CDM with the LSS bootstrap: a joint power spectrum and bispectrum analysis","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-05-14T17:39:05.401310Z"},"links":{"cited_paper":"/paper/2410.08998","citing_paper":"/paper/2605.13298"},"observation_digest":"sha256:6ffa2b11073aa60380d3328a946072fd9c1963bbfc07a2ebbf881d4bb64a8116","observation_id":"0e094c73-9877-4569-8864-a45b2a0ceb33","resolution":{"observed_at":"2026-05-14T17:42:32.780016Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.08998","last_updated":"2024-10-11T17:09:29Z","snapshot_observed_at":"2026-07-06T19:31:57.906994Z","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":"2410.08998","doi":"10.48550/arxiv.2410.08998","metadata_source":"arxiv_reference","pith_arxiv_id":"2410.08998","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Akitsu, Mapping the galaxy-halo connection to the galaxy bias: implication to the HOD-informed prior (2024), arXiv:2410.08998 [astro-ph.CO]","venue":"arXiv (Cornell University)","work_id":"f6ba542c-2a3e-4e86-9f30-79de69d0c8d8","year":2024},"citing_paper":{"arxiv_id":"2606.12405","last_updated":"2026-06-10T17:59:34Z","snapshot_observed_at":"2026-08-02T04:38:40.169291Z","submitted_at":"2026-06-10T17:59:34Z","title":"Bounding the Effect of HOD Assumptions on Small-Scale Clustering Constraints","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-06-27T08:42:05.889407Z"},"links":{"cited_paper":"/paper/2410.08998","citing_paper":"/paper/2606.12405"},"observation_digest":"sha256:d8864f1237efa96f7c1f6d30b5e6789ba14a38f933ef0760e5e05d73b59e9c12","observation_id":"04cf9fff-0593-4b2a-975d-8a7e48136d0f","resolution":{"observed_at":"2026-06-27T11:10:52.150735Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.08998","last_updated":"2024-10-11T17:09:29Z","snapshot_observed_at":"2026-07-06T19:31:57.906994Z","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":"2410.08998","doi":"10.48550/arxiv.2410.08998","metadata_source":"arxiv_reference","pith_arxiv_id":"2410.08998","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Akitsu, Mapping the galaxy-halo connection to the galaxy bias: implication to the HOD-informed prior (2024), arXiv:2410.08998 [astro-ph.CO]","venue":"arXiv (Cornell University)","work_id":"f6ba542c-2a3e-4e86-9f30-79de69d0c8d8","year":2024},"citing_paper":{"arxiv_id":"2606.26234","last_updated":"2026-06-24T18:00:02Z","snapshot_observed_at":"2026-08-06T10:28:45.654237Z","submitted_at":"2026-06-24T18:00:02Z","title":"Lyman-Alpha Forest and its Cross-Correlation with High-Redshift Galaxies in Effective Field Theory at the Field Level","version":1},"reference_index":185,"source":"pdf_text","source_observed_at":"2026-06-26T01:38:09.398349Z"},"links":{"cited_paper":"/paper/2410.08998","citing_paper":"/paper/2606.26234"},"observation_digest":"sha256:0a6edf89cf2de8a806cbd80d05285f485607c17a515eddbe516ef210c3df4889","observation_id":"f5e8cf4b-a0cd-4831-af3a-2f6d62167fe8","resolution":{"observed_at":"2026-07-04T15:29:55.236346Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.08998","last_updated":"2024-10-11T17:09:29Z","snapshot_observed_at":"2026-07-06T19:31:57.906994Z","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":"2026-08-02T02:52:34.650546Z","title":"Akitsu, arXiv e-prints (2024), arXiv:2410.08998 [astro-ph.CO]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.14206","last_updated":"2026-07-15T18:00:00Z","snapshot_observed_at":"2026-08-07T03:47:05.986777Z","submitted_at":"2026-07-15T18:00:00Z","title":"Simulation-Based Priors for HI Bias from Halo Occupation Physics","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-02T02:52:34.650546Z"},"links":{"cited_paper":"/paper/2410.08998","citing_paper":"/paper/2607.14206"},"observation_digest":"sha256:ae9d4442c0b8c7829a571892acc0d050d8042aa6d031ffc1e98f2dd0a446024f","observation_id":"2244d01f-0c8b-4d98-9b40-2ee9eb5a9a60","resolution":{"observed_at":"2026-08-02T02:52:34.650546Z","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":"2026-07-06T19:31:57.906994Z","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":"2026-08-01T07:53:23.366140Z","title":"Akitsu,Mapping the galaxy-halo connection to the galaxy bias: implication to the HOD-informed prior,arXiv e-prints(2024) , [2410.08998]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.21334","last_updated":"2026-07-23T14:01:15Z","snapshot_observed_at":"2026-08-01T07:53:00.788731Z","submitted_at":"2026-07-23T14:01:15Z","title":"Web-Halo Model Peak-Background Split (WHM-PBS): halo bias as a distribution, not a number","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-01T07:53:23.366140Z"},"links":{"cited_paper":"/paper/2410.08998","citing_paper":"/paper/2607.21334"},"observation_digest":"sha256:33879458f12f8bb1b52f768e91b4e74c2e29c55934f9dfe60ebb40a9001cc20b","observation_id":"920d3606-a840-4c2f-bd30-38ef9c2f3c14","resolution":{"observed_at":"2026-08-01T07:53:23.366140Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2410.08998/citation-record","integrity":"/paper/2410.08998/integrity","json":"/paper/2410.08998/citation-record.json","paper":"/paper/2410.08998"},"outbound":[],"paper":{"arxiv_id":"2410.08998","last_updated":"2024-10-11T17:09:29Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T19:31:57.906994Z","submitted_at":"2024-10-11T17:09:29Z","title":"Mapping the galaxy-halo connection to the galaxy bias: implication to the HOD-informed prior"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:2410.08998."}