{"as_of":"2026-08-12T17:08:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7840d19fe1b4314de4f1da61d159077bffba8532fba96adf2855a8154dc28a33","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":11,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":11,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":11,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":11,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T10:38:55.174456Z","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":"2026-07-04T17:20:01.416340Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2408.09964","last_updated":"2025-06-04T07:21:19Z","snapshot_observed_at":"2026-08-10T01:47:13.313294Z","submitted_at":"2024-08-19T13:10:53Z","title":"Extended $\\delta N$ formalism: Nonspatially Flat Separate Universe Approach","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.09964","snapshot_observed_at":"2026-08-11T10:38:55.174456Z","title":"Artigas, S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.16463","last_updated":"2024-12-21T03:30:13Z","snapshot_observed_at":"2026-08-11T15:59:53.857718Z","submitted_at":"2024-12-21T03:30:13Z","title":"A complete analysis of inflation with piecewise quadratic potential","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-11T10:38:55.174456Z"},"links":{"cited_paper":"/paper/2408.09964","citing_paper":"/paper/2412.16463"},"observation_digest":"sha256:0da7fab88c7b6a443c233570a2e84f5544db2cdfe0b3504fd49dab4e369f7619","observation_id":"881ef80d-d00c-4479-b407-401ae004c6f2","resolution":{"observed_at":"2026-08-11T10:38:55.174456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.09964","last_updated":"2025-06-04T07:21:19Z","snapshot_observed_at":"2026-08-10T01:47:13.313294Z","submitted_at":"2024-08-19T13:10:53Z","title":"Extended $\\delta N$ formalism: Nonspatially Flat Separate Universe Approach","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.09964","snapshot_observed_at":"2026-08-10T15:00:43.958677Z","title":"Artigas, S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.14681","last_updated":"2025-08-25T07:56:14Z","snapshot_observed_at":"2026-08-12T08:11:04.680281Z","submitted_at":"2025-01-24T17:58:44Z","title":"How deep is the dip and how tall are the wiggles in inflationary power spectra?","version":3},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-10T15:00:43.958677Z"},"links":{"cited_paper":"/paper/2408.09964","citing_paper":"/paper/2501.14681"},"observation_digest":"sha256:314a1b30ccdf4d5d81be7d037b077d9d6558319fb6839303946e1357407889e1","observation_id":"737119af-f008-41b6-8583-a934e2928284","resolution":{"observed_at":"2026-08-10T15:00:43.958677Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.09964","last_updated":"2025-06-04T07:21:19Z","snapshot_observed_at":"2026-08-10T01:47:13.313294Z","submitted_at":"2024-08-19T13:10:53Z","title":"Extended $\\delta N$ formalism: Nonspatially Flat Separate Universe Approach","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.09964","snapshot_observed_at":"2026-08-07T12:38:10.844655Z","title":"Artigas, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.24590","last_updated":"2026-07-26T14:35:58Z","snapshot_observed_at":"2026-08-07T12:14:58.020993Z","submitted_at":"2025-05-30T13:39:09Z","title":"$\\delta n$ formalism: A new formulation for the probability density of the curvature perturbation","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-07T12:38:10.844655Z"},"links":{"cited_paper":"/paper/2408.09964","citing_paper":"/paper/2505.24590"},"observation_digest":"sha256:abb2c64ff1e5a7658630b860a933c26b869dab35f831859cb98c4c06d70a5610","observation_id":"efb81405-7f41-42c3-8c56-70019b0f211f","resolution":{"observed_at":"2026-08-07T12:38:10.844655Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.09964","last_updated":"2025-06-04T07:21:19Z","snapshot_observed_at":"2026-08-10T01:47:13.313294Z","submitted_at":"2024-08-19T13:10:53Z","title":"Extended $\\delta N$ formalism: Nonspatially Flat Separate Universe Approach","version":2},"cited_work":{"arxiv_id":"2408.09964","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2408.09964","snapshot_observed_at":"2026-07-04T17:20:01.416340Z","title":"Artigas, S","venue":null,"work_id":"7a93accc-afd5-4eab-be46-2de1d0eb7af7","year":2025},"citing_paper":{"arxiv_id":"2512.14649","last_updated":"2026-05-01T11:59:33Z","snapshot_observed_at":"2026-07-06T22:39:14.117332Z","submitted_at":"2025-12-16T18:11:34Z","title":"Stochastic Inflation in Numerical Relativity","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-05-16T21:59:29.414284Z"},"links":{"cited_paper":"/paper/2408.09964","citing_paper":"/paper/2512.14649"},"observation_digest":"sha256:a075152cedd0eb46f0d6aef13e3df105c85bee3c5599cdfa13437feca8ea9b1a","observation_id":"69735c59-2a58-4561-877b-011630f3df23","resolution":{"observed_at":"2026-05-16T22:01:17.885705Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2408.09964","last_updated":"2025-06-04T07:21:19Z","snapshot_observed_at":"2026-08-10T01:47:13.313294Z","submitted_at":"2024-08-19T13:10:53Z","title":"Extended $\\delta N$ formalism: Nonspatially Flat Separate Universe Approach","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.09964","snapshot_observed_at":"2026-08-03T06:50:38.962974Z","title":"Artigas, S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2601.22219","last_updated":"2026-07-27T18:16:29Z","snapshot_observed_at":"2026-08-06T07:51:06.124054Z","submitted_at":"2026-01-29T19:00:01Z","title":"When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity","version":3},"reference_index":120,"source":"pdf_text","source_observed_at":"2026-08-03T06:50:38.962974Z"},"links":{"cited_paper":"/paper/2408.09964","citing_paper":"/paper/2601.22219"},"observation_digest":"sha256:847d8bb7b0dc9ebc3d6f6c7413cc75ed538eaf812e2bbab862f806e205bceedf","observation_id":"6e125a52-4ba3-431b-963f-4380e336eae0","resolution":{"observed_at":"2026-08-03T06:50:38.962974Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.09964","last_updated":"2025-06-04T07:21:19Z","snapshot_observed_at":"2026-08-10T01:47:13.313294Z","submitted_at":"2024-08-19T13:10:53Z","title":"Extended $\\delta N$ formalism: Nonspatially Flat Separate Universe Approach","version":2},"cited_work":{"arxiv_id":"2408.09964","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2408.09964","snapshot_observed_at":"2026-07-04T17:20:01.416340Z","title":"Artigas, S","venue":null,"work_id":"7a93accc-afd5-4eab-be46-2de1d0eb7af7","year":2025},"citing_paper":{"arxiv_id":"2604.15219","last_updated":"2026-04-28T15:13:43Z","snapshot_observed_at":"2026-08-11T12:19:28.748330Z","submitted_at":"2026-04-16T16:50:33Z","title":"Nonperturbative stochastic inflation in perturbative dynamical background","version":2},"reference_index":120,"source":"pdf_text","source_observed_at":"2026-05-10T09:51:09.373721Z"},"links":{"cited_paper":"/paper/2408.09964","citing_paper":"/paper/2604.15219"},"observation_digest":"sha256:138e2ba502a8adf658072f2fc45ca5ef349b53887f4832b634e3ad269fbb4834","observation_id":"00dff4c7-5e8d-4179-bb87-ccc0570fbea9","resolution":{"observed_at":"2026-05-10T10:04:07.436000Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2408.09964","last_updated":"2025-06-04T07:21:19Z","snapshot_observed_at":"2026-08-10T01:47:13.313294Z","submitted_at":"2024-08-19T13:10:53Z","title":"Extended $\\delta N$ formalism: Nonspatially Flat Separate Universe Approach","version":2},"cited_work":{"arxiv_id":"2408.09964","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2408.09964","snapshot_observed_at":"2026-07-04T17:20:01.416340Z","title":"Artigas, S","venue":null,"work_id":"7a93accc-afd5-4eab-be46-2de1d0eb7af7","year":2025},"citing_paper":{"arxiv_id":"2606.24111","last_updated":"2026-06-23T03:56:37Z","snapshot_observed_at":"2026-08-05T23:39:59.933680Z","submitted_at":"2026-06-23T03:56:37Z","title":"Constant-Roll Inflation: Analytical Formulae for Power Spectrum and Implications for Induced Gravitational Waves","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-06-25T23:44:36.834692Z"},"links":{"cited_paper":"/paper/2408.09964","citing_paper":"/paper/2606.24111"},"observation_digest":"sha256:63d2dc6404069289a94027a8cb45e1ec96c632b4e24bd39f5fc082c520c65884","observation_id":"c598b254-3045-4e88-831a-9422961a375e","resolution":{"observed_at":"2026-07-04T17:20:01.417912Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2408.09964","last_updated":"2025-06-04T07:21:19Z","snapshot_observed_at":"2026-08-10T01:47:13.313294Z","submitted_at":"2024-08-19T13:10:53Z","title":"Extended $\\delta N$ formalism: Nonspatially Flat Separate Universe Approach","version":2},"cited_work":{"arxiv_id":"2408.09964","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2408.09964","snapshot_observed_at":"2026-07-04T17:20:01.416340Z","title":"Artigas, S","venue":null,"work_id":"7a93accc-afd5-4eab-be46-2de1d0eb7af7","year":2025},"citing_paper":{"arxiv_id":"2606.29796","last_updated":"2026-07-13T06:20:09Z","snapshot_observed_at":"2026-07-16T23:18:46.329568Z","submitted_at":"2026-06-29T05:15:54Z","title":"Superhorizon curvature perturbations in hybrid inflation revisited","version":1},"reference_index":114,"source":"pdf_text","source_observed_at":"2026-06-30T05:34:57.532391Z"},"links":{"cited_paper":"/paper/2408.09964","citing_paper":"/paper/2606.29796"},"observation_digest":"sha256:7fc882af57789d50c85ff71d9326b5ff4c91a0152b88626ddd3852b567dcbf49","observation_id":"d46ef02b-2b23-4d4e-8f4a-ff6c7678a687","resolution":{"observed_at":"2026-06-30T14:14:46.390227Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2408.09964","last_updated":"2025-06-04T07:21:19Z","snapshot_observed_at":"2026-08-10T01:47:13.313294Z","submitted_at":"2024-08-19T13:10:53Z","title":"Extended $\\delta N$ formalism: Nonspatially Flat Separate Universe Approach","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.09964","snapshot_observed_at":"2026-07-14T17:01:04.250468Z","title":"Artigas, S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2606.29796","last_updated":"2026-07-13T06:20:09Z","snapshot_observed_at":"2026-07-16T23:18:46.329568Z","submitted_at":"2026-06-29T05:15:54Z","title":"Superhorizon curvature perturbations in hybrid inflation revisited","version":2},"reference_index":114,"source":"pdf_text","source_observed_at":"2026-07-14T17:01:04.250468Z"},"links":{"cited_paper":"/paper/2408.09964","citing_paper":"/paper/2606.29796"},"observation_digest":"sha256:264aa2132d51060ffa0eb5dda048fe3d90fc61d450aed19b37126f96db025c12","observation_id":"42a01f83-752b-4e89-8a99-c0dbba45e3b9","resolution":{"observed_at":"2026-07-14T17:01:04.250468Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.09964","last_updated":"2025-06-04T07:21:19Z","snapshot_observed_at":"2026-08-10T01:47:13.313294Z","submitted_at":"2024-08-19T13:10:53Z","title":"Extended $\\delta N$ formalism: Nonspatially Flat Separate Universe Approach","version":2},"cited_work":{"arxiv_id":"2408.09964","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2408.09964","snapshot_observed_at":"2026-07-04T17:20:01.416340Z","title":"Artigas, S","venue":null,"work_id":"7a93accc-afd5-4eab-be46-2de1d0eb7af7","year":2025},"citing_paper":{"arxiv_id":"2606.30087","last_updated":"2026-06-29T10:27:35Z","snapshot_observed_at":"2026-08-04T09:16:17.016040Z","submitted_at":"2026-06-29T10:27:35Z","title":"Compaction function in stochastic inflation: a \\texttt{FOREST} of type I and II primordial black holes","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-06-30T05:26:28.825729Z"},"links":{"cited_paper":"/paper/2408.09964","citing_paper":"/paper/2606.30087"},"observation_digest":"sha256:670af0769daba6fea89cac12f3fe2fd7f9f11849c157a73f433400283ab2ee06","observation_id":"10ad1fc2-6656-4c22-a67f-cdb1c51a1823","resolution":{"observed_at":"2026-06-30T14:24:45.657092Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2408.09964","last_updated":"2025-06-04T07:21:19Z","snapshot_observed_at":"2026-08-10T01:47:13.313294Z","submitted_at":"2024-08-19T13:10:53Z","title":"Extended $\\delta N$ formalism: Nonspatially Flat Separate Universe Approach","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.09964","snapshot_observed_at":"2026-08-05T14:10:01.271464Z","title":"ExtendedδN Formalism: Nonspatially Flat Separate-Universe Approach","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.03725","last_updated":"2026-08-04T14:22:53Z","snapshot_observed_at":"2026-08-12T16:09:44.142920Z","submitted_at":"2026-08-04T14:22:53Z","title":"How Dilatation Invariance Suppresses Loop Corrections to Curvature Perturbations on CMB Scales","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-05T14:10:01.271464Z"},"links":{"cited_paper":"/paper/2408.09964","citing_paper":"/paper/2608.03725"},"observation_digest":"sha256:ac2a3406574a183a9074f92c5b9e30ae36b5930fd5e38ace82529ac7e9a468b7","observation_id":"e22b6d41-333b-4ff3-8c1f-ead853c74318","resolution":{"observed_at":"2026-08-05T14:10:01.271464Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2408.09964/citation-record","integrity":"/paper/2408.09964/integrity","json":"/paper/2408.09964/citation-record.json","paper":"/paper/2408.09964"},"outbound":[],"paper":{"arxiv_id":"2408.09964","last_updated":"2025-06-04T07:21:19Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-10T01:47:13.313294Z","submitted_at":"2024-08-19T13:10:53Z","title":"Extended $\\delta N$ formalism: Nonspatially Flat Separate Universe Approach"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2408.09964."}