{"as_of":"2026-08-19T15:58:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e473f5a43ea78adf882c5c8d026b945b33df21cb5683fc886f2e6bd56024eb49","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":"2026-08-19T06:32:44.657259+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":"2026-08-03T00:21:45.716018Z","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":"2001.10792","last_updated":"2020-04-07T00:20:36Z","snapshot_observed_at":"2026-08-10T23:17:10.811777Z","submitted_at":"2020-01-29T13:02:12Z","title":"Cosmological constraints from line intensity mapping with interlopers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.10792","snapshot_observed_at":"2026-08-01T12:40:13.170280Z","title":", keywords =","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2607.19504","last_updated":"2026-07-21T18:33:34Z","snapshot_observed_at":"2026-08-16T19:46:13.213045Z","submitted_at":"2026-07-21T18:33:34Z","title":"Reading Between the Lines: Forward Modeling Dust, Continuum, and Spectral Cleaning for Multi-Line Intensity Mapping","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-01T12:40:13.170280Z"},"links":{"cited_paper":"/paper/2001.10792","citing_paper":"/paper/2607.19504"},"observation_digest":"sha256:acc1bd0da075484bf38c8dff884cc66b611cbab3925984a83e34a7cc302d9738","observation_id":"fb31424d-8aa1-462f-a785-a5da36a5f8e8","resolution":{"observed_at":"2026-08-01T12:40:13.170280Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.10792","last_updated":"2020-04-07T00:20:36Z","snapshot_observed_at":"2026-08-10T23:17:10.811777Z","submitted_at":"2020-01-29T13:02:12Z","title":"Cosmological constraints from line intensity mapping with interlopers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.10792","snapshot_observed_at":"2026-07-31T06:02:16.307768Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.24917","last_updated":"2026-07-27T18:00:01Z","snapshot_observed_at":"2026-08-14T17:35:47.451428Z","submitted_at":"2026-07-27T18:00:01Z","title":"Interlopers as Signal in Line Intensity Mapping","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-07-31T06:02:16.307768Z"},"links":{"cited_paper":"/paper/2001.10792","citing_paper":"/paper/2607.24917"},"observation_digest":"sha256:723392f3dafc9d3c9e81b5d6ab8e1d0b795026025a2cf528169a96c065d1b4df","observation_id":"fa162347-878a-4db5-b67c-c343dcf7e097","resolution":{"observed_at":"2026-07-31T06:02:16.307768Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.10792","last_updated":"2020-04-07T00:20:36Z","snapshot_observed_at":"2026-08-10T23:17:10.811777Z","submitted_at":"2020-01-29T13:02:12Z","title":"Cosmological constraints from line intensity mapping with interlopers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.10792","snapshot_observed_at":"2026-08-03T00:21:45.716018Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.28713","last_updated":"2026-07-30T18:00:00Z","snapshot_observed_at":"2026-08-19T11:18:19.622551Z","submitted_at":"2026-07-30T18:00:00Z","title":"Searching for Population III stars with line intensity mapping cross-correlations","version":1},"reference_index":165,"source":"pdf_text","source_observed_at":"2026-08-03T00:21:45.716018Z"},"links":{"cited_paper":"/paper/2001.10792","citing_paper":"/paper/2607.28713"},"observation_digest":"sha256:dca43d79cdf62d5a529b3e6fa82d55a47a79128f965f52cffdcb1c50d973b01c","observation_id":"c41efa02-e5ff-429b-9057-6c274b4bbf27","resolution":{"observed_at":"2026-08-03T00:21:45.716018Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2001.10792/citation-record","integrity":"/paper/2001.10792/integrity","json":"/paper/2001.10792/citation-record.json","paper":"/paper/2001.10792"},"outbound":[],"paper":{"arxiv_id":"2001.10792","last_updated":"2020-04-07T00:20:36Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-10T23:17:10.811777Z","submitted_at":"2020-01-29T13:02:12Z","title":"Cosmological constraints from line intensity mapping with interlopers"},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2001.10792."}