{"as_of":"2026-08-15T20:44:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4c3ec514a697a369efb7fcceaf1ad2dc5be82bc0968b5b0e633ec7d35523c302","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T05:55:49.258250Z","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":"1412.3854","last_updated":"2014-12-11T22:59:01Z","snapshot_observed_at":"2026-08-14T23:07:55.158831Z","submitted_at":"2014-12-11T22:59:01Z","title":"Designing an Inflation Galaxy Survey: how to measure $\\sigma(f_{\\rm NL}) \\sim 1$ using scale-dependent galaxy bias","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.3854","snapshot_observed_at":"2026-08-07T05:55:49.258250Z","title":"de Putter and O","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.06902","last_updated":"2025-09-12T17:34:08Z","snapshot_observed_at":"2026-08-14T05:14:36.846399Z","submitted_at":"2025-06-07T19:26:26Z","title":"Separating Angular and Radial Modes with Spherical-Fourier Bessel Power Spectrum on All Scales and Implications for Systematics Mitigation","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-07T05:55:49.258250Z"},"links":{"cited_paper":"/paper/1412.3854","citing_paper":"/paper/2506.06902"},"observation_digest":"sha256:6fb39c7efcaad2790898550bf8e0f76712e526633d920d5d7e9917bf4a215502","observation_id":"4d5a955f-1c39-4f21-9678-7d0ba0306603","resolution":{"observed_at":"2026-08-07T05:55:49.258250Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.3854","last_updated":"2014-12-11T22:59:01Z","snapshot_observed_at":"2026-08-14T23:07:55.158831Z","submitted_at":"2014-12-11T22:59:01Z","title":"Designing an Inflation Galaxy Survey: how to measure $\\sigma(f_{\\rm NL}) \\sim 1$ using scale-dependent galaxy bias","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.3854","snapshot_observed_at":"2026-07-30T11:03:11.533685Z","title":"de Putter and O","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.27175","last_updated":"2026-07-29T17:47:24Z","snapshot_observed_at":"2026-08-05T21:53:11.321037Z","submitted_at":"2026-07-29T17:47:24Z","title":"Searching for signatures of inflationary massive fields in DESI Imaging data and Stage-V galaxy surveys","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-07-30T11:03:11.533685Z"},"links":{"cited_paper":"/paper/1412.3854","citing_paper":"/paper/2607.27175"},"observation_digest":"sha256:6df179ec225fac9c1e53c6dc9db59269bd5418ca24e769595081730f641b19c8","observation_id":"98e64d0b-c17c-43d4-a991-e4e853418cd0","resolution":{"observed_at":"2026-07-30T11:03:11.533685Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1412.3854/citation-record","integrity":"/paper/1412.3854/integrity","json":"/paper/1412.3854/citation-record.json","paper":"/paper/1412.3854"},"outbound":[],"paper":{"arxiv_id":"1412.3854","last_updated":"2014-12-11T22:59:01Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T23:07:55.158831Z","submitted_at":"2014-12-11T22:59:01Z","title":"Designing an Inflation Galaxy Survey: how to measure $\\sigma(f_{\\rm NL}) \\sim 1$ using scale-dependent galaxy bias"},"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 2 inbound Pith citation observations for arXiv:1412.3854."}