{"as_of":"2026-08-12T23:12:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:cb62e128cb2b36ff53f4ec53bab6be0304107e935ec26abc4aa5a83039d51e2c","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":10,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":10,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":10,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":10,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T18:30:00.636051Z","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":"2026-07-02T15:07:04.675857Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2409.12950","last_updated":"2025-09-03T16:54:05Z","snapshot_observed_at":"2026-08-12T22:41:32.284843Z","submitted_at":"2024-09-19T17:57:02Z","title":"Stochastic Axion-like Curvaton: Non-Gaussianity and Primordial Black Holes Without Large Power Spectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.12950","snapshot_observed_at":"2026-08-10T18:30:00.636051Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.11320","last_updated":"2025-05-21T08:43:23Z","snapshot_observed_at":"2026-08-10T18:22:13.706121Z","submitted_at":"2025-01-20T07:47:31Z","title":"Reconstructing Primordial Curvature Perturbations via Scalar-Induced Gravitational Waves with LISA","version":2},"reference_index":202,"source":"pdf_text","source_observed_at":"2026-08-10T18:30:00.636051Z"},"links":{"cited_paper":"/paper/2409.12950","citing_paper":"/paper/2501.11320"},"observation_digest":"sha256:394f9891b5375e4a6dbeafbe74b664ecf4b0cdb6bcf7ad64065c963b8ea5ecc0","observation_id":"4ffb433a-8a85-4f1e-86c8-12eddb2dd76b","resolution":{"observed_at":"2026-08-10T18:30:00.636051Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.12950","last_updated":"2025-09-03T16:54:05Z","snapshot_observed_at":"2026-08-12T22:41:32.284843Z","submitted_at":"2024-09-19T17:57:02Z","title":"Stochastic Axion-like Curvaton: Non-Gaussianity and Primordial Black Holes Without Large Power Spectrum","version":2},"cited_work":{"arxiv_id":"2409.12950","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2409.12950","snapshot_observed_at":"2026-07-02T15:07:04.675857Z","title":null,"venue":null,"work_id":"424e366d-f983-4c67-a1cb-6398416bb2a8","year":2025},"citing_paper":{"arxiv_id":"2505.16820","last_updated":"2026-04-13T03:10:33Z","snapshot_observed_at":"2026-07-06T21:28:38.694043Z","submitted_at":"2025-05-22T15:55:50Z","title":"Isotropy, anisotropies and non-Gaussianity in the scalar-induced gravitational-wave background: diagrammatic approach for primordial non-Gaussianity up to arbitrary order","version":3},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-05-22T01:55:13.345095Z"},"links":{"cited_paper":"/paper/2409.12950","citing_paper":"/paper/2505.16820"},"observation_digest":"sha256:10aa74dfc528e4e0725a8d19d6c41c60f49ace113ce86c61256f66fe1f7f6a52","observation_id":"a57e9535-ac6c-4d99-92a8-270bc12b561c","resolution":{"observed_at":"2026-05-22T01:55:55.051505Z","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":"2409.12950","last_updated":"2025-09-03T16:54:05Z","snapshot_observed_at":"2026-08-12T22:41:32.284843Z","submitted_at":"2024-09-19T17:57:02Z","title":"Stochastic Axion-like Curvaton: Non-Gaussianity and Primordial Black Holes Without Large Power Spectrum","version":2},"cited_work":{"arxiv_id":"2409.12950","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2409.12950","snapshot_observed_at":"2026-07-02T15:07:04.675857Z","title":null,"venue":null,"work_id":"424e366d-f983-4c67-a1cb-6398416bb2a8","year":2025},"citing_paper":{"arxiv_id":"2510.05967","last_updated":"2026-04-29T13:37:17Z","snapshot_observed_at":"2026-08-06T11:11:47.105759Z","submitted_at":"2025-10-07T14:23:00Z","title":"Stochastic Gravitational Waves from Modulated Reheating","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-05-18T08:59:33.023939Z"},"links":{"cited_paper":"/paper/2409.12950","citing_paper":"/paper/2510.05967"},"observation_digest":"sha256:808a45a00a23d57afbbafd9fcf2c7bd445c068422fd174c6c678cfa8c97019f4","observation_id":"94792911-1a52-4c32-9805-bd5dc1420451","resolution":{"observed_at":"2026-05-18T09:01:09.100584Z","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":"2409.12950","last_updated":"2025-09-03T16:54:05Z","snapshot_observed_at":"2026-08-12T22:41:32.284843Z","submitted_at":"2024-09-19T17:57:02Z","title":"Stochastic Axion-like Curvaton: Non-Gaussianity and Primordial Black Holes Without Large Power Spectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.12950","snapshot_observed_at":"2026-08-02T22:42:35.693688Z","title":"Stochastic axionlike curvaton: Non-Gaussianity and primordial black holes without a large power spectrum,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2602.16292","last_updated":"2026-07-02T07:44:17Z","snapshot_observed_at":"2026-08-09T23:46:50.343503Z","submitted_at":"2026-02-18T09:20:24Z","title":"Gravitational Waves from Primordial Black Holes formed by Null Energy Condition Violation during Inflation","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-02T22:42:35.693688Z"},"links":{"cited_paper":"/paper/2409.12950","citing_paper":"/paper/2602.16292"},"observation_digest":"sha256:2ee3d00661e73a985c011a460712046b2cac8a2111744edeca1dab0a5b6900ac","observation_id":"748ab011-12ed-4bae-8cfc-369cdbed61db","resolution":{"observed_at":"2026-08-02T22:42:35.693688Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.12950","last_updated":"2025-09-03T16:54:05Z","snapshot_observed_at":"2026-08-12T22:41:32.284843Z","submitted_at":"2024-09-19T17:57:02Z","title":"Stochastic Axion-like Curvaton: Non-Gaussianity and Primordial Black Holes Without Large Power Spectrum","version":2},"cited_work":{"arxiv_id":"2409.12950","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2409.12950","snapshot_observed_at":"2026-07-02T15:07:04.675857Z","title":null,"venue":null,"work_id":"424e366d-f983-4c67-a1cb-6398416bb2a8","year":2025},"citing_paper":{"arxiv_id":"2605.15197","last_updated":"2026-07-29T13:49:49Z","snapshot_observed_at":"2026-08-11T08:04:45.518387Z","submitted_at":"2026-05-14T17:59:55Z","title":"Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-05-15T02:53:41.149271Z"},"links":{"cited_paper":"/paper/2409.12950","citing_paper":"/paper/2605.15197"},"observation_digest":"sha256:250aae9c9cd2ea07d8b1ba76a6e278ef5bbfe760faaba01ad4c19f723bed58eb","observation_id":"b1bd57d5-1831-47a7-b0fa-6e0fb817d216","resolution":{"observed_at":"2026-05-15T02:59:41.818878Z","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":"2409.12950","last_updated":"2025-09-03T16:54:05Z","snapshot_observed_at":"2026-08-12T22:41:32.284843Z","submitted_at":"2024-09-19T17:57:02Z","title":"Stochastic Axion-like Curvaton: Non-Gaussianity and Primordial Black Holes Without Large Power Spectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.12950","snapshot_observed_at":"2026-08-02T14:03:38.861268Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.15197","last_updated":"2026-07-29T13:49:49Z","snapshot_observed_at":"2026-08-11T08:04:45.518387Z","submitted_at":"2026-05-14T17:59:55Z","title":"Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-02T14:03:38.861268Z"},"links":{"cited_paper":"/paper/2409.12950","citing_paper":"/paper/2605.15197"},"observation_digest":"sha256:7505b1a51d749c982aa5d21bc8a96885e1734be91e291aed0cd4c772565c76af","observation_id":"293c53ff-834f-4a81-b040-53f2f555adbb","resolution":{"observed_at":"2026-08-02T14:03:38.861268Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.12950","last_updated":"2025-09-03T16:54:05Z","snapshot_observed_at":"2026-08-12T22:41:32.284843Z","submitted_at":"2024-09-19T17:57:02Z","title":"Stochastic Axion-like Curvaton: Non-Gaussianity and Primordial Black Holes Without Large Power Spectrum","version":2},"cited_work":{"arxiv_id":"2409.12950","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2409.12950","snapshot_observed_at":"2026-07-02T15:07:04.675857Z","title":null,"venue":null,"work_id":"424e366d-f983-4c67-a1cb-6398416bb2a8","year":2025},"citing_paper":{"arxiv_id":"2606.06355","last_updated":"2026-06-22T12:59:38Z","snapshot_observed_at":"2026-07-06T23:46:10.612537Z","submitted_at":"2026-06-04T16:23:24Z","title":"$\\tt BlackHawk$ $\\tt v3.0$: Hawking Radiation from Regular Black Holes","version":2},"reference_index":181,"source":"pdf_text","source_observed_at":"2026-06-28T00:05:44.496054Z"},"links":{"cited_paper":"/paper/2409.12950","citing_paper":"/paper/2606.06355"},"observation_digest":"sha256:fa4ecc334aabd05d147af713e8541453a0b752ca9861ff1c055b31e1e55163f6","observation_id":"8de71a0c-73d6-45fe-aef1-09ac743ad6b1","resolution":{"observed_at":"2026-07-02T15:07:04.677112Z","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":"2409.12950","last_updated":"2025-09-03T16:54:05Z","snapshot_observed_at":"2026-08-12T22:41:32.284843Z","submitted_at":"2024-09-19T17:57:02Z","title":"Stochastic Axion-like Curvaton: Non-Gaussianity and Primordial Black Holes Without Large Power Spectrum","version":2},"cited_work":{"arxiv_id":"2409.12950","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2409.12950","snapshot_observed_at":"2026-07-02T15:07:04.675857Z","title":null,"venue":null,"work_id":"424e366d-f983-4c67-a1cb-6398416bb2a8","year":2025},"citing_paper":{"arxiv_id":"2606.28296","last_updated":"2026-06-26T17:40:06Z","snapshot_observed_at":"2026-08-06T06:31:36.117462Z","submitted_at":"2026-06-26T17:40:06Z","title":"Memoirs of the curvaton: non-perturbative non-Gaussianity and supermassive primordial black holes","version":1},"reference_index":111,"source":"pdf_text","source_observed_at":"2026-06-29T02:29:32.722846Z"},"links":{"cited_paper":"/paper/2409.12950","citing_paper":"/paper/2606.28296"},"observation_digest":"sha256:4fd9aebcf93efbe98f2e7e31556d3be17141793e037e9ca75a769a6ff8fad22f","observation_id":"4c8a3b65-ad7e-4cb9-8a67-703346b57c3d","resolution":{"observed_at":"2026-07-01T18:15:57.656869Z","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":"2409.12950","last_updated":"2025-09-03T16:54:05Z","snapshot_observed_at":"2026-08-12T22:41:32.284843Z","submitted_at":"2024-09-19T17:57:02Z","title":"Stochastic Axion-like Curvaton: Non-Gaussianity and Primordial Black Holes Without Large Power Spectrum","version":2},"cited_work":{"arxiv_id":"2409.12950","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2409.12950","snapshot_observed_at":"2026-07-02T15:07:04.675857Z","title":null,"venue":null,"work_id":"424e366d-f983-4c67-a1cb-6398416bb2a8","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":107,"source":"pdf_text","source_observed_at":"2026-06-30T05:34:57.532391Z"},"links":{"cited_paper":"/paper/2409.12950","citing_paper":"/paper/2606.29796"},"observation_digest":"sha256:ecf021ac9ff0054f0525376f84eb0278daa9756ead4326d74e98a98571d9be95","observation_id":"4d8ba979-0483-43d4-a548-12d6baeda205","resolution":{"observed_at":"2026-06-30T14:14:46.322194Z","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":"2409.12950","last_updated":"2025-09-03T16:54:05Z","snapshot_observed_at":"2026-08-12T22:41:32.284843Z","submitted_at":"2024-09-19T17:57:02Z","title":"Stochastic Axion-like Curvaton: Non-Gaussianity and Primordial Black Holes Without Large Power Spectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.12950","snapshot_observed_at":"2026-07-14T17:01:04.250468Z","title":null,"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":107,"source":"pdf_text","source_observed_at":"2026-07-14T17:01:04.250468Z"},"links":{"cited_paper":"/paper/2409.12950","citing_paper":"/paper/2606.29796"},"observation_digest":"sha256:a39f03c25e2dd84d197934a42cd0144e7cda963576cb8dece2b9798cd7c674ea","observation_id":"0f80f262-1f8b-4e03-82a8-0c1ee962ca2c","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"}}],"links":{"evidence":"/evidence","html":"/paper/2409.12950/citation-record","integrity":"/paper/2409.12950/integrity","json":"/paper/2409.12950/citation-record.json","paper":"/paper/2409.12950"},"outbound":[],"paper":{"arxiv_id":"2409.12950","last_updated":"2025-09-03T16:54:05Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-12T22:41:32.284843Z","submitted_at":"2024-09-19T17:57:02Z","title":"Stochastic Axion-like Curvaton: Non-Gaussianity and Primordial Black Holes Without Large Power Spectrum"},"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 10 inbound Pith citation observations for arXiv:2409.12950."}