{"as_of":"2026-08-13T09:04:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d9f8fd0f2ec066609f4977775e72165ed279e0a3423769933b8d95257efb64a4","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":"2026-08-13T06:32:02.005865+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":"2026-08-12T05:43:30.349762Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-10T17:42:32.786111Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2410.08387","last_updated":"2024-10-10T21:46:54Z","snapshot_observed_at":"2026-08-12T22:25:53.922142Z","submitted_at":"2024-10-10T21:46:54Z","title":"RUBIES: JWST/NIRSpec resolves evolutionary phases of dusty star-forming galaxies at $z\\sim2$","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.08387","snapshot_observed_at":"2026-08-12T05:43:30.349762Z","title":"R., Brammer , G., Heintz , K","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.00188","last_updated":"2024-12-09T11:23:08Z","snapshot_observed_at":"2026-08-12T05:36:04.802938Z","submitted_at":"2024-11-29T19:00:01Z","title":"Evolution of the star formation rate surface density main sequence. Insights from a semi-analytic simulation since $z = 12$","version":2},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-12T05:43:30.349762Z"},"links":{"cited_paper":"/paper/2410.08387","citing_paper":"/paper/2412.00188"},"observation_digest":"sha256:7b222df4379a86cc9c83395d451e235bfa0ffc680bf97080999d322b3ecfadb5","observation_id":"cec997b5-50c5-4324-aedb-55dfb49b7fb1","resolution":{"observed_at":"2026-08-12T05:43:30.349762Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.08387","last_updated":"2024-10-10T21:46:54Z","snapshot_observed_at":"2026-08-12T22:25:53.922142Z","submitted_at":"2024-10-10T21:46:54Z","title":"RUBIES: JWST/NIRSpec resolves evolutionary phases of dusty star-forming galaxies at $z\\sim2$","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.08387","snapshot_observed_at":"2026-08-11T19:25:25.536385Z","title":"R., Brammer, G., Heintz, K","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.536385Z"},"links":{"cited_paper":"/paper/2410.08387","citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:3b59faeb7db6788ad4ca0cc6e66bb68d6546849731135ac1b84f243ebe69c9b8","observation_id":"666b6d97-4871-420a-bca6-c29ea8237cd5","resolution":{"observed_at":"2026-08-11T19:25:25.536385Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.08387","last_updated":"2024-10-10T21:46:54Z","snapshot_observed_at":"2026-08-12T22:25:53.922142Z","submitted_at":"2024-10-10T21:46:54Z","title":"RUBIES: JWST/NIRSpec resolves evolutionary phases of dusty star-forming galaxies at $z\\sim2$","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.08387","snapshot_observed_at":"2026-08-10T19:16:28.447763Z","title":"R., et al., 2024, preprint (arXiv:2410.08387)","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.10541","last_updated":"2025-01-17T20:27:48Z","snapshot_observed_at":"2026-08-13T06:21:24.813320Z","submitted_at":"2025-01-17T20:27:48Z","title":"REBELS-IFU: Dust attenuation curves of 12 massive galaxies at $z\\simeq7$","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-10T19:16:28.447763Z"},"links":{"cited_paper":"/paper/2410.08387","citing_paper":"/paper/2501.10541"},"observation_digest":"sha256:abcba7a9c40aceee48a33e894fe852a68a0f615c8ac665ccdc9217b524062b0e","observation_id":"39f04c37-ae28-416c-bb99-8df1e48d4e1e","resolution":{"observed_at":"2026-08-10T19:16:28.447763Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.08387","last_updated":"2024-10-10T21:46:54Z","snapshot_observed_at":"2026-08-12T22:25:53.922142Z","submitted_at":"2024-10-10T21:46:54Z","title":"RUBIES: JWST/NIRSpec resolves evolutionary phases of dusty star-forming galaxies at $z\\sim2$","version":1},"cited_work":{"arxiv_id":"2410.08387","doi":null,"metadata_source":"pith","pith_arxiv_id":"2410.08387","snapshot_observed_at":"2026-08-10T17:42:32.786111Z","title":"RUBIES: JWST/NIRSpec resolves evolutionary phases of dusty star-forming galaxies at $z\\sim2$","venue":"astro-ph.GA","work_id":"c8839a87-874e-451c-a344-92f5dc1202bd","year":2024},"citing_paper":{"arxiv_id":"2501.12008","last_updated":"2025-02-18T15:22:48Z","snapshot_observed_at":"2026-08-11T05:50:25.190606Z","submitted_at":"2025-01-21T10:00:46Z","title":"The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer","version":2},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-10T17:42:32.136748Z"},"links":{"cited_paper":"/paper/2410.08387","citing_paper":"/paper/2501.12008"},"observation_digest":"sha256:b2d17de23912360795880355be236d50c3eda9535a6f845ea4cf47a97b0236e5","observation_id":"8b84e519-f6d4-4ae2-aef8-83923dc6da8f","resolution":{"observed_at":"2026-08-10T17:42:32.793433Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2410.08387/citation-record","integrity":"/paper/2410.08387/integrity","json":"/paper/2410.08387/citation-record.json","paper":"/paper/2410.08387"},"outbound":[],"paper":{"arxiv_id":"2410.08387","last_updated":"2024-10-10T21:46:54Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-12T22:25:53.922142Z","submitted_at":"2024-10-10T21:46:54Z","title":"RUBIES: JWST/NIRSpec resolves evolutionary phases of dusty star-forming galaxies at $z\\sim2$"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2410.08387."}