{"as_of":"2026-08-07T10:07:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:38200c7057fa1d6f406f8769bd1f02786930c500b50a970ef6643cbbd913abc7","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T20:59:59.860311Z","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":"2026-07-02T05:16:39.043450Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1609.05978","last_updated":"2017-02-16T17:33:49Z","snapshot_observed_at":"2026-07-06T05:11:25.849188Z","submitted_at":"2016-09-20T00:51:07Z","title":"FAST-PT II: an algorithm to calculate convolution integrals of general tensor quantities in cosmological perturbation theory","version":2},"cited_work":{"arxiv_id":"1609.05978","doi":null,"metadata_source":"pith","pith_arxiv_id":"1609.05978","snapshot_observed_at":"2026-07-02T05:16:39.043450Z","title":"FAST-PT II: an algorithm to calculate convolution integrals of general tensor quantities in cosmological perturbation theory","venue":"astro-ph.CO","work_id":"5da9ec0d-146b-4b6a-841c-8a200711f7ca","year":2016},"citing_paper":{"arxiv_id":"2105.13549","last_updated":"2022-03-21T13:57:33Z","snapshot_observed_at":"2026-08-02T14:00:01.779912Z","submitted_at":"2021-05-28T01:58:58Z","title":"Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing","version":3},"reference_index":188,"source":"pdf_text","source_observed_at":"2026-05-19T09:35:12.156800Z"},"links":{"cited_paper":"/paper/1609.05978","citing_paper":"/paper/2105.13549"},"observation_digest":"sha256:27ae74343e5acf0dbc1871cec58ae53d35faa4e0f91084d41de2a2993124f6b0","observation_id":"cf415484-ae22-4e12-9e56-e0500749a67c","resolution":{"observed_at":"2026-05-19T09:35:12.931975Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1609.05978","last_updated":"2017-02-16T17:33:49Z","snapshot_observed_at":"2026-07-06T05:11:25.849188Z","submitted_at":"2016-09-20T00:51:07Z","title":"FAST-PT II: an algorithm to calculate convolution integrals of general tensor quantities in cosmological perturbation theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.05978","snapshot_observed_at":"2026-08-06T20:59:59.860311Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.01386","last_updated":"2025-07-24T20:35:38Z","snapshot_observed_at":"2026-08-06T20:50:23.570617Z","submitted_at":"2025-07-02T06:03:29Z","title":"Cosmology and Source Redshift Constraints from Galaxy Clustering and Tomographic Weak Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-06T20:59:59.860311Z"},"links":{"cited_paper":"/paper/1609.05978","citing_paper":"/paper/2507.01386"},"observation_digest":"sha256:6945b5722da6deed59cf0cecc1fe82d307962d927f83284152b46d5ccce529f7","observation_id":"7d9448d5-775e-4fbf-9904-c8e1d8b60376","resolution":{"observed_at":"2026-08-06T20:59:59.860311Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.05978","last_updated":"2017-02-16T17:33:49Z","snapshot_observed_at":"2026-07-06T05:11:25.849188Z","submitted_at":"2016-09-20T00:51:07Z","title":"FAST-PT II: an algorithm to calculate convolution integrals of general tensor quantities in cosmological perturbation theory","version":2},"cited_work":{"arxiv_id":"1609.05978","doi":null,"metadata_source":"pith","pith_arxiv_id":"1609.05978","snapshot_observed_at":"2026-07-02T05:16:39.043450Z","title":"FAST-PT II: an algorithm to calculate convolution integrals of general tensor quantities in cosmological perturbation theory","venue":"astro-ph.CO","work_id":"5da9ec0d-146b-4b6a-841c-8a200711f7ca","year":2016},"citing_paper":{"arxiv_id":"2511.20757","last_updated":"2026-04-14T17:58:15Z","snapshot_observed_at":"2026-07-06T22:36:59.311174Z","submitted_at":"2025-11-25T19:00:04Z","title":"Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses","version":2},"reference_index":115,"source":"pdf_text","source_observed_at":"2026-05-17T04:15:18.730245Z"},"links":{"cited_paper":"/paper/1609.05978","citing_paper":"/paper/2511.20757"},"observation_digest":"sha256:0cef7f62846fe66ec7061a3a84acbc6861db835af8d79b9e13e39474b1b9836a","observation_id":"6d6850b9-5a23-4a66-8ae3-b52a3c996f8e","resolution":{"observed_at":"2026-05-17T04:19:01.112446Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1609.05978","last_updated":"2017-02-16T17:33:49Z","snapshot_observed_at":"2026-07-06T05:11:25.849188Z","submitted_at":"2016-09-20T00:51:07Z","title":"FAST-PT II: an algorithm to calculate convolution integrals of general tensor quantities in cosmological perturbation theory","version":2},"cited_work":{"arxiv_id":"1609.05978","doi":null,"metadata_source":"pith","pith_arxiv_id":"1609.05978","snapshot_observed_at":"2026-07-02T05:16:39.043450Z","title":"FAST-PT II: an algorithm to calculate convolution integrals of general tensor quantities in cosmological perturbation theory","venue":"astro-ph.CO","work_id":"5da9ec0d-146b-4b6a-841c-8a200711f7ca","year":2016},"citing_paper":{"arxiv_id":"2606.03860","last_updated":"2026-06-02T16:34:38Z","snapshot_observed_at":"2026-07-06T23:44:05.167767Z","submitted_at":"2026-06-02T16:34:38Z","title":"Biased tracers, Hybrid Effective Field Theory and Modified Gravity","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-06-28T08:25:11.252554Z"},"links":{"cited_paper":"/paper/1609.05978","citing_paper":"/paper/2606.03860"},"observation_digest":"sha256:2df46e3647c70d6c9edf3bf98044c7786c294b66ca5e5287499f6916eb3b3b62","observation_id":"770b8460-d89f-4f70-9db0-297ab223ddef","resolution":{"observed_at":"2026-07-02T05:16:39.044748Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1609.05978","last_updated":"2017-02-16T17:33:49Z","snapshot_observed_at":"2026-07-06T05:11:25.849188Z","submitted_at":"2016-09-20T00:51:07Z","title":"FAST-PT II: an algorithm to calculate convolution integrals of general tensor quantities in cosmological perturbation theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.05978","snapshot_observed_at":"2026-07-31T11:14:47.124410Z","title":"and McEwen, Joseph E","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.28326","last_updated":"2026-07-30T14:57:39Z","snapshot_observed_at":"2026-08-03T03:24:50.671196Z","submitted_at":"2026-07-30T14:57:39Z","title":"Growth, geometry, and early-universe split of the matter density parameter $\\Omega_{\\rm m}$","version":1},"reference_index":142,"source":"arxiv_source","source_observed_at":"2026-07-31T11:14:47.124410Z"},"links":{"cited_paper":"/paper/1609.05978","citing_paper":"/paper/2607.28326"},"observation_digest":"sha256:6a3a102c163b91e8fa930614c09ef771963d2a6d3b9d8b018ed1934a4614bcfa","observation_id":"8cc829b6-32de-4134-903d-099242f8f0a1","resolution":{"observed_at":"2026-07-31T11:14:47.124410Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1609.05978/citation-record","integrity":"/paper/1609.05978/integrity","json":"/paper/1609.05978/citation-record.json","paper":"/paper/1609.05978"},"outbound":[],"paper":{"arxiv_id":"1609.05978","last_updated":"2017-02-16T17:33:49Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T05:11:25.849188Z","submitted_at":"2016-09-20T00:51:07Z","title":"FAST-PT II: an algorithm to calculate convolution integrals of general tensor quantities in cosmological perturbation theory"},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1609.05978."}