{"as_of":"2026-08-15T21:52:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:bdea6aa17e97aae09e5ef67a94caf2677775a991ddb5b014ceee6fbdae6e1d9c","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T18:08:58.282287Z","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":"2026-05-12T00:41:15.144189Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2210.10075","last_updated":"2022-12-13T21:14:32Z","snapshot_observed_at":"2026-08-13T21:44:48.534769Z","submitted_at":"2022-10-18T18:11:21Z","title":"The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.10075","snapshot_observed_at":"2026-08-12T18:08:58.282287Z","title":"E., Springel , V., et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.11830","last_updated":"2024-11-18T18:48:45Z","snapshot_observed_at":"2026-08-12T20:04:22.550921Z","submitted_at":"2024-11-18T18:48:45Z","title":"Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-12T18:08:58.282287Z"},"links":{"cited_paper":"/paper/2210.10075","citing_paper":"/paper/2411.11830"},"observation_digest":"sha256:fb279467eb8235f1d570bde68ceaf33d3d71be5b8bf216aaa332bd5dac9e8376","observation_id":"9c7ff3a6-5b1d-460d-b45e-65a91e24cca5","resolution":{"observed_at":"2026-08-12T18:08:58.282287Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.10075","last_updated":"2022-12-13T21:14:32Z","snapshot_observed_at":"2026-08-13T21:44:48.534769Z","submitted_at":"2022-10-18T18:11:21Z","title":"The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching","version":2},"cited_work":{"arxiv_id":"2210.10075","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2210.10075","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Contreras, R.E","venue":null,"work_id":"346ba9dd-4768-40af-bb83-721be7d55e98","year":2023},"citing_paper":{"arxiv_id":"2604.26022","last_updated":"2026-04-30T00:23:11Z","snapshot_observed_at":"2026-07-06T23:11:48.524898Z","submitted_at":"2026-04-28T18:05:05Z","title":"Secondary Dependence of Baryonic Effects on the Density Profile of Dark Matter Halos","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-05-07T14:53:02.246257Z"},"links":{"cited_paper":"/paper/2210.10075","citing_paper":"/paper/2604.26022"},"observation_digest":"sha256:aa80f10f8a74057f64fc8a7b211e104e0cd62979ae9b0b62addac21c36a4c7f9","observation_id":"83594467-a5b3-4ca5-a329-d603cbdc6913","resolution":{"observed_at":"2026-05-12T00:41:15.153132Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2210.10075","last_updated":"2022-12-13T21:14:32Z","snapshot_observed_at":"2026-08-13T21:44:48.534769Z","submitted_at":"2022-10-18T18:11:21Z","title":"The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.10075","snapshot_observed_at":"2026-08-02T06:10:16.005125Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.13151","last_updated":"2026-07-14T18:01:38Z","snapshot_observed_at":"2026-08-15T18:54:07.654644Z","submitted_at":"2026-07-14T18:01:38Z","title":"Evaluating the flexibility of the MillenniumTNG galaxy formation model with multi-zoom re-simulations","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-02T06:10:16.005125Z"},"links":{"cited_paper":"/paper/2210.10075","citing_paper":"/paper/2607.13151"},"observation_digest":"sha256:92966403e6deab82fa1cbd81e4b4a29f290274839eeb4e5b678c5266cb967c63","observation_id":"456c78f6-507d-4215-b93e-aebd17e52e04","resolution":{"observed_at":"2026-08-02T06:10:16.005125Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2210.10075/citation-record","integrity":"/paper/2210.10075/integrity","json":"/paper/2210.10075/citation-record.json","paper":"/paper/2210.10075"},"outbound":[],"paper":{"arxiv_id":"2210.10075","last_updated":"2022-12-13T21:14:32Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-13T21:44:48.534769Z","submitted_at":"2022-10-18T18:11:21Z","title":"The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching"},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2210.10075."}