{"as_of":"2026-08-15T22:46:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:bf8b505a384d6e78ec32f67a6eee0f2eec3d5e507bf3e0425e43205e0514ce8b","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-02T07:31:58.643897Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2205.10413","last_updated":"2022-08-02T21:34:57Z","snapshot_observed_at":"2026-08-15T04:12:24.620370Z","submitted_at":"2022-05-20T19:06:32Z","title":"Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.10413","snapshot_observed_at":"2026-07-13T06:20:04.707661Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.08846","last_updated":"2026-07-09T18:11:36Z","snapshot_observed_at":"2026-08-12T13:37:15.348773Z","submitted_at":"2026-07-09T18:11:36Z","title":"mitigating the overcooling problem with sink-based bursty star formation in a high-z dwarf galaxy","version":1},"reference_index":105,"source":"arxiv_source","source_observed_at":"2026-07-13T06:20:04.707661Z"},"links":{"cited_paper":"/paper/2205.10413","citing_paper":"/paper/2607.08846"},"observation_digest":"sha256:77b343863afb4e33efde0f6c5616f30733bf43fe688759b948a24274c46d9b1d","observation_id":"fc79f854-d272-4fb1-a5f2-6df8636da951","resolution":{"observed_at":"2026-07-13T06:20:04.707661Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.10413","last_updated":"2022-08-02T21:34:57Z","snapshot_observed_at":"2026-08-15T04:12:24.620370Z","submitted_at":"2022-05-20T19:06:32Z","title":"Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.10413","snapshot_observed_at":"2026-07-14T15:02:03.459139Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.09858","last_updated":"2026-07-15T11:28:58Z","snapshot_observed_at":"2026-08-13T11:40:02.972783Z","submitted_at":"2026-07-10T18:00:03Z","title":"How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-07-14T15:02:03.459139Z"},"links":{"cited_paper":"/paper/2205.10413","citing_paper":"/paper/2607.09858"},"observation_digest":"sha256:bc8befa09b03439665c81d03e1866adbe881aec4062da293362b0b783686d545","observation_id":"245c0aa5-85dc-493d-896a-3da3999a29b4","resolution":{"observed_at":"2026-07-14T15:02:03.459139Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.10413","last_updated":"2022-08-02T21:34:57Z","snapshot_observed_at":"2026-08-15T04:12:24.620370Z","submitted_at":"2022-05-20T19:06:32Z","title":"Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.10413","snapshot_observed_at":"2026-08-02T07:31:58.643897Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.09858","last_updated":"2026-07-15T11:28:58Z","snapshot_observed_at":"2026-08-13T11:40:02.972783Z","submitted_at":"2026-07-10T18:00:03Z","title":"How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching","version":2},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-02T07:31:58.643897Z"},"links":{"cited_paper":"/paper/2205.10413","citing_paper":"/paper/2607.09858"},"observation_digest":"sha256:d26b6439a4c2ba55dfe3d28797fd13de85c39121064ef5a7e7a574ec1b1f6e28","observation_id":"ca21fc16-ec41-43dd-bca4-8e3c31e73327","resolution":{"observed_at":"2026-08-02T07:31:58.643897Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.10413","last_updated":"2022-08-02T21:34:57Z","snapshot_observed_at":"2026-08-15T04:12:24.620370Z","submitted_at":"2022-05-20T19:06:32Z","title":"Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.10413","snapshot_observed_at":"2026-08-02T02:36:23.388113Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14294","last_updated":"2026-07-17T20:52:38Z","snapshot_observed_at":"2026-08-14T02:12:36.218054Z","submitted_at":"2026-07-15T18:58:56Z","title":"Preferential alignment of Class 0, Class I protostellar disks in multiple systems across nine nearby molecular clouds","version":2},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-02T02:36:23.388113Z"},"links":{"cited_paper":"/paper/2205.10413","citing_paper":"/paper/2607.14294"},"observation_digest":"sha256:b20006eb858537b24b3ca16bb60c5e52236db612606d0f31468aca085798c840","observation_id":"ea0a34aa-450b-4c4d-a212-d06537c4f41b","resolution":{"observed_at":"2026-08-02T02:36:23.388113Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2205.10413/citation-record","integrity":"/paper/2205.10413/integrity","json":"/paper/2205.10413/citation-record.json","paper":"/paper/2205.10413"},"outbound":[],"paper":{"arxiv_id":"2205.10413","last_updated":"2022-08-02T21:34:57Z","latest_version":3,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-15T04:12:24.620370Z","submitted_at":"2022-05-20T19:06:32Z","title":"Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations"},"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 4 inbound Pith citation observations for arXiv:2205.10413."}