{"as_of":"2026-08-18T19:04:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b286afdfa1f7d706c763570f4cedd073293c5f1b65415cb36df123734fc21f17","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":"2026-08-18T06:34:40.430872+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":"2026-08-12T00:39:28.954225Z","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":"2026-05-19T08:22:11.013291Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2004.00934","last_updated":"2021-01-15T12:10:30Z","snapshot_observed_at":"2026-08-17T15:45:45.818740Z","submitted_at":"2020-04-02T11:07:19Z","title":"High-redshift star formation in the ALMA era","version":2},"cited_work":{"arxiv_id":"2004.00934","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2004.00934","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"b06a66ee-1b7e-45e6-b823-57ee34fcf207","year":2020},"citing_paper":{"arxiv_id":"2506.22046","last_updated":"2026-01-28T17:35:33Z","snapshot_observed_at":"2026-08-17T11:42:00.240965Z","submitted_at":"2025-06-27T09:43:10Z","title":"The NIKA2 cosmological legacy survey at 2 mm: catalogs, colors, redshift distributions, and implications for deep surveys","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-19T08:19:39.371302Z"},"links":{"cited_paper":"/paper/2004.00934","citing_paper":"/paper/2506.22046"},"observation_digest":"sha256:0a5a409dcff141059847c23ba91c8c3ed1deb6741b78b9d9e55d57e61255dc37","observation_id":"d9185cd4-be6a-4c83-b1e0-68dd54a3f85f","resolution":{"observed_at":"2026-05-19T08:22:11.016586Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2004.00934","last_updated":"2021-01-15T12:10:30Z","snapshot_observed_at":"2026-08-17T15:45:45.818740Z","submitted_at":"2020-04-02T11:07:19Z","title":"High-redshift star formation in the ALMA era","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.00934","snapshot_observed_at":"2026-08-01T15:29:42.251772Z","title":"Royal Society Open Science , keywords =","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.18440","last_updated":"2026-07-20T18:49:40Z","snapshot_observed_at":"2026-08-07T05:38:29.953994Z","submitted_at":"2026-07-20T18:49:40Z","title":"Vz-GAL Dusty Star-Forming Galaxies: Revisiting the CO-H2 Conversion Factor Tension","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-01T15:29:42.251772Z"},"links":{"cited_paper":"/paper/2004.00934","citing_paper":"/paper/2607.18440"},"observation_digest":"sha256:2622a44c89d985c26dce62da91e844765eb3caa1e2eb6156d2f0ecfc7bf6925e","observation_id":"fb545d34-e943-44f2-a301-b9f90d1fe5fe","resolution":{"observed_at":"2026-08-01T15:29:42.251772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.00934","last_updated":"2021-01-15T12:10:30Z","snapshot_observed_at":"2026-08-17T15:45:45.818740Z","submitted_at":"2020-04-02T11:07:19Z","title":"High-redshift star formation in the ALMA era","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.00934","snapshot_observed_at":"2026-08-01T10:02:14.740779Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.20404","last_updated":"2026-07-22T17:39:32Z","snapshot_observed_at":"2026-08-14T22:26:15.829134Z","submitted_at":"2026-07-22T17:39:32Z","title":"Spectral Data-cube Cleaning for CCAT Deep Spectroscopic Survey. I. Effect of correlated noise and filtering on the power spectrum","version":1},"reference_index":133,"source":"arxiv_source","source_observed_at":"2026-08-01T10:02:14.740779Z"},"links":{"cited_paper":"/paper/2004.00934","citing_paper":"/paper/2607.20404"},"observation_digest":"sha256:23bcf0c2b6d1294d861dca87d6b4c22809fdca3981c8936a39a97223b3225d81","observation_id":"3cd3a2e0-36bb-4c47-8b16-1e60a5732fcf","resolution":{"observed_at":"2026-08-01T10:02:14.740779Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.00934","last_updated":"2021-01-15T12:10:30Z","snapshot_observed_at":"2026-08-17T15:45:45.818740Z","submitted_at":"2020-04-02T11:07:19Z","title":"High-redshift star formation in the ALMA era","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.00934","snapshot_observed_at":"2026-08-12T00:39:28.954225Z","title":"Royal Society Open Science , keywords =","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2608.08015","last_updated":"2026-08-08T08:53:26Z","snapshot_observed_at":"2026-08-18T10:22:51.530891Z","submitted_at":"2026-08-08T08:53:26Z","title":"Breathing Fire: Hot Dust in the Big Three Dragons at z = 7.15","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-12T00:39:28.954225Z"},"links":{"cited_paper":"/paper/2004.00934","citing_paper":"/paper/2608.08015"},"observation_digest":"sha256:178990032ae894d3eed36c19e6a3ce6e529b668e0d34c576e98169e0c72b0438","observation_id":"079997d5-6c3c-440e-8fb7-92dcd03326dd","resolution":{"observed_at":"2026-08-12T00:39:28.954225Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2004.00934/citation-record","integrity":"/paper/2004.00934/integrity","json":"/paper/2004.00934/citation-record.json","paper":"/paper/2004.00934"},"outbound":[],"paper":{"arxiv_id":"2004.00934","last_updated":"2021-01-15T12:10:30Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-17T15:45:45.818740Z","submitted_at":"2020-04-02T11:07:19Z","title":"High-redshift star formation in the ALMA era"},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2004.00934."}