{"as_of":"2026-08-19T03:49:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:485f2c175a008ed7337db50fa02dc9adccff0b1e118ba801b4e0c53d19d4d080","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":7,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":7,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-18T06:34:40.430872+00:00","state":"measured"},{"denominator":7,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":7,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T17:30:09.556070Z","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":"2026-07-10T23:17:42.438675Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2302.09066","last_updated":"2023-09-19T10:09:38Z","snapshot_observed_at":"2026-08-16T15:54:32.859368Z","submitted_at":"2023-02-17T18:59:47Z","title":"Towards optimal and robust $f_{\\rm NL}$ constraints with multi-tracer analyses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.09066","snapshot_observed_at":"2026-08-11T19:40:38.997450Z","title":"Barreira and E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06553","last_updated":"2025-06-23T09:25:35Z","snapshot_observed_at":"2026-08-18T13:43:16.464580Z","submitted_at":"2024-12-09T15:02:38Z","title":"Primordial non-Gaussianity -- the effects of relativistic and wide-angle corrections to the power spectrum","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-11T19:40:38.997450Z"},"links":{"cited_paper":"/paper/2302.09066","citing_paper":"/paper/2412.06553"},"observation_digest":"sha256:c7268322efe0c194f15c6c89a38e136b0c7459835ff717c3c08b200cdee2cff8","observation_id":"72ea1b87-2570-4066-869c-d0141529cdf7","resolution":{"observed_at":"2026-08-11T19:40:38.997450Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.09066","last_updated":"2023-09-19T10:09:38Z","snapshot_observed_at":"2026-08-16T15:54:32.859368Z","submitted_at":"2023-02-17T18:59:47Z","title":"Towards optimal and robust $f_{\\rm NL}$ constraints with multi-tracer analyses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.09066","snapshot_observed_at":"2026-08-15T17:30:09.556070Z","title":"Barreira \\ and\\ author E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.11798","last_updated":"2025-08-15T20:47:51Z","snapshot_observed_at":"2026-08-17T10:14:08.425457Z","submitted_at":"2025-08-15T20:47:51Z","title":"Where does non-Universality in Assembly Bias come from?","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-15T17:30:09.556070Z"},"links":{"cited_paper":"/paper/2302.09066","citing_paper":"/paper/2508.11798"},"observation_digest":"sha256:6ff8e5e773271d3697425be674362ea9af95477f2f8a515a4770a15525f9e674","observation_id":"8977897f-dc05-4da9-b66b-4fb9cda559f4","resolution":{"observed_at":"2026-08-15T17:30:09.556070Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.09066","last_updated":"2023-09-19T10:09:38Z","snapshot_observed_at":"2026-08-16T15:54:32.859368Z","submitted_at":"2023-02-17T18:59:47Z","title":"Towards optimal and robust $f_{\\rm NL}$ constraints with multi-tracer analyses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.09066","snapshot_observed_at":"2026-08-03T22:43:43.096186Z","title":"Barreira and E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.09466","last_updated":"2026-06-18T18:40:30Z","snapshot_observed_at":"2026-08-09T18:20:52.996463Z","submitted_at":"2025-11-12T16:33:34Z","title":"Unbiased analysis of primordial non-Gaussianity: the multipoles of the full relativistic power spectrum","version":3},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-03T22:43:43.096186Z"},"links":{"cited_paper":"/paper/2302.09066","citing_paper":"/paper/2511.09466"},"observation_digest":"sha256:ab580ba20944321f61c2a0f2932c5dd203311f6bda87dc233b6d1aceb849a69a","observation_id":"b9989b30-4581-4509-b6b8-20a47c0a7a3b","resolution":{"observed_at":"2026-08-03T22:43:43.096186Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.09066","last_updated":"2023-09-19T10:09:38Z","snapshot_observed_at":"2026-08-16T15:54:32.859368Z","submitted_at":"2023-02-17T18:59:47Z","title":"Towards optimal and robust $f_{\\rm NL}$ constraints with multi-tracer analyses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.09066","snapshot_observed_at":"2026-08-04T06:23:28.778139Z","title":"Barreira and E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2601.19438","last_updated":"2026-08-03T17:50:09Z","snapshot_observed_at":"2026-08-16T01:53:35.143934Z","submitted_at":"2026-01-27T10:18:40Z","title":"Large-scale Modeling of the Observed Power Spectrum Multipoles","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-04T06:23:28.778139Z"},"links":{"cited_paper":"/paper/2302.09066","citing_paper":"/paper/2601.19438"},"observation_digest":"sha256:3cde4a5b41bb4d2374d5777b9c4f962b90e178ded5d5dcd47a0044d74264b7ed","observation_id":"a186a6b9-1f2c-4e31-be9e-6a958933362d","resolution":{"observed_at":"2026-08-04T06:23:28.778139Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.09066","last_updated":"2023-09-19T10:09:38Z","snapshot_observed_at":"2026-08-16T15:54:32.859368Z","submitted_at":"2023-02-17T18:59:47Z","title":"Towards optimal and robust $f_{\\rm NL}$ constraints with multi-tracer analyses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.09066","snapshot_observed_at":"2026-07-12T03:43:52.393274Z","title":"Towards optimal and robust f \\_ nl constraints with multi-tracer analyses","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.03259","last_updated":"2026-07-03T12:21:14Z","snapshot_observed_at":"2026-08-08T08:24:39.969103Z","submitted_at":"2026-07-03T12:21:14Z","title":"Cosmology with HI Intensity Mapping","version":1},"reference_index":158,"source":"arxiv_source","source_observed_at":"2026-07-12T03:43:52.393274Z"},"links":{"cited_paper":"/paper/2302.09066","citing_paper":"/paper/2607.03259"},"observation_digest":"sha256:8ec7e8f24705f87ab11f5a1eaffcbcf8b28a7b9364ffb46d0738c4d24b0315a6","observation_id":"1be9f416-7e97-4c3a-a384-4858d6530d68","resolution":{"observed_at":"2026-07-12T03:43:52.393274Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.09066","last_updated":"2023-09-19T10:09:38Z","snapshot_observed_at":"2026-08-16T15:54:32.859368Z","submitted_at":"2023-02-17T18:59:47Z","title":"Towards optimal and robust $f_{\\rm NL}$ constraints with multi-tracer analyses","version":2},"cited_work":{"arxiv_id":"2302.09066","doi":null,"metadata_source":"pith","pith_arxiv_id":"2302.09066","snapshot_observed_at":"2026-07-10T23:17:42.438675Z","title":"Towards optimal and robust $f_{\\rm NL}$ constraints with multi-tracer analyses","venue":"astro-ph.CO","work_id":"7dd66481-d844-455a-93ba-4bae3dcc679a","year":2023},"citing_paper":{"arxiv_id":"2607.06697","last_updated":"2026-07-07T18:15:25Z","snapshot_observed_at":"2026-08-18T01:32:18.472666Z","submitted_at":"2026-07-07T18:15:25Z","title":"Impact and measurability of linear relativistic effects in galaxy surveys","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-07-10T23:12:29.350615Z"},"links":{"cited_paper":"/paper/2302.09066","citing_paper":"/paper/2607.06697"},"observation_digest":"sha256:6e5776e2f842ab2286c1d23e7cc74ba45d4773f1d6ffc320bb5a417c45b93a5a","observation_id":"8b4a68ca-e443-4bd1-b4ee-b8f5f2c67b42","resolution":{"observed_at":"2026-07-10T23:17:42.458652Z","resolver_source":"local_arxiv","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":"2302.09066","last_updated":"2023-09-19T10:09:38Z","snapshot_observed_at":"2026-08-16T15:54:32.859368Z","submitted_at":"2023-02-17T18:59:47Z","title":"Towards optimal and robust $f_{\\rm NL}$ constraints with multi-tracer analyses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.09066","snapshot_observed_at":"2026-08-10T06:07:09.875939Z","title":"Barreira and E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.07339","last_updated":"2026-08-07T15:36:28Z","snapshot_observed_at":"2026-08-15T08:56:56.807876Z","submitted_at":"2026-08-07T15:36:28Z","title":"Sample Variance Cancellation for Future Spectroscopic Surveys","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-10T06:07:09.875939Z"},"links":{"cited_paper":"/paper/2302.09066","citing_paper":"/paper/2608.07339"},"observation_digest":"sha256:06a1648bafe0ef27f4befd0e86e45931c4aae77b708408d958524827a983226e","observation_id":"b3983851-f17e-40d8-becc-9ddd0c3291f2","resolution":{"observed_at":"2026-08-10T06:07:09.875939Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2302.09066/citation-record","integrity":"/paper/2302.09066/integrity","json":"/paper/2302.09066/citation-record.json","paper":"/paper/2302.09066"},"outbound":[],"paper":{"arxiv_id":"2302.09066","last_updated":"2023-09-19T10:09:38Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-16T15:54:32.859368Z","submitted_at":"2023-02-17T18:59:47Z","title":"Towards optimal and robust $f_{\\rm NL}$ constraints with multi-tracer analyses"},"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 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2302.09066."}