{"as_of":"2026-08-10T13:44:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:675acf424c449ea93337ef86769e97a9035784c72b2d285b1a77ebe9414cfcf8","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":"2026-08-10T06:31:04.303077+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":"2026-08-07T11:09:43.504352Z","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":"2026-06-30T17:04:56.959061Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2211.07598","last_updated":"2023-04-25T20:31:48Z","snapshot_observed_at":"2026-08-08T15:00:26.501973Z","submitted_at":"2022-11-14T18:24:52Z","title":"Cosmic decoherence: primordial power spectra and non-Gaussianities","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.07598","snapshot_observed_at":"2026-08-07T11:09:43.504352Z","title":"Cosmic decoherence: primordial power spectra and non-Gaussianities,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.03860","last_updated":"2025-06-04T11:46:58Z","snapshot_observed_at":"2026-08-09T05:29:30.126271Z","submitted_at":"2025-06-04T11:46:58Z","title":"Stochastic inflation as a superfluid","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-07T11:09:43.504352Z"},"links":{"cited_paper":"/paper/2211.07598","citing_paper":"/paper/2506.03860"},"observation_digest":"sha256:33d98ee205013b0371ee8a63e3c5430ebec1e2e2e82c8a1b1354ddc7df2cd257","observation_id":"dff8290c-08a6-4f81-a7e8-b008ca55dab1","resolution":{"observed_at":"2026-08-07T11:09:43.504352Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.07598","last_updated":"2023-04-25T20:31:48Z","snapshot_observed_at":"2026-08-08T15:00:26.501973Z","submitted_at":"2022-11-14T18:24:52Z","title":"Cosmic decoherence: primordial power spectra and non-Gaussianities","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.07598","snapshot_observed_at":"2026-08-06T20:51:53.224275Z","title":"Daddi Hammou and N","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.02070","last_updated":"2025-09-13T16:20:39Z","snapshot_observed_at":"2026-08-08T07:41:34.159807Z","submitted_at":"2025-07-02T18:12:34Z","title":"Stochastic inflation as an open quantum system","version":3},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-06T20:51:53.224275Z"},"links":{"cited_paper":"/paper/2211.07598","citing_paper":"/paper/2507.02070"},"observation_digest":"sha256:c43610a84debee4c15f35eb0a6a47908c5331f865ac5ffed3e0f7d6e7c842b35","observation_id":"a365d88b-2a30-4607-9e38-3d56f7e1d4d2","resolution":{"observed_at":"2026-08-06T20:51:53.224275Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.07598","last_updated":"2023-04-25T20:31:48Z","snapshot_observed_at":"2026-08-08T15:00:26.501973Z","submitted_at":"2022-11-14T18:24:52Z","title":"Cosmic decoherence: primordial power spectra and non-Gaussianities","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.07598","snapshot_observed_at":"2026-08-04T21:50:11.613755Z","title":"Daddi Hammou and N","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.07769","last_updated":"2026-07-14T22:18:52Z","snapshot_observed_at":"2026-08-06T05:54:19.059257Z","submitted_at":"2025-09-09T14:04:54Z","title":"Inflationary Decoherence from the Gravitational Floor","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-04T21:50:11.613755Z"},"links":{"cited_paper":"/paper/2211.07598","citing_paper":"/paper/2509.07769"},"observation_digest":"sha256:639c8458b6d67b7412e568f59cc692df8df1720b693f6d6d74005a54e5c31d46","observation_id":"cf489f90-913e-4d98-bf28-362ed9581321","resolution":{"observed_at":"2026-08-04T21:50:11.613755Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.07598","last_updated":"2023-04-25T20:31:48Z","snapshot_observed_at":"2026-08-08T15:00:26.501973Z","submitted_at":"2022-11-14T18:24:52Z","title":"Cosmic decoherence: primordial power spectra and non-Gaussianities","version":2},"cited_work":{"arxiv_id":"2211.07598","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2211.07598","snapshot_observed_at":"2026-06-30T17:04:56.959061Z","title":"Daddi Hammou and N","venue":null,"work_id":"88ed5f36-ef97-4650-8303-350dbf8afcc1","year":2023},"citing_paper":{"arxiv_id":"2512.17089","last_updated":"2026-05-22T14:38:51Z","snapshot_observed_at":"2026-07-06T22:39:28.855621Z","submitted_at":"2025-12-18T21:35:55Z","title":"Gauging Open EFTs from the top down","version":3},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-05-25T06:58:36.613669Z"},"links":{"cited_paper":"/paper/2211.07598","citing_paper":"/paper/2512.17089"},"observation_digest":"sha256:7ad71dc0f20ed17dea2c218b26c59a9add3363447253069e7e645ee98700c311","observation_id":"5555eab6-c186-47ce-845f-6ff54f1095cf","resolution":{"observed_at":"2026-05-25T07:00:26.625914Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.07598","last_updated":"2023-04-25T20:31:48Z","snapshot_observed_at":"2026-08-08T15:00:26.501973Z","submitted_at":"2022-11-14T18:24:52Z","title":"Cosmic decoherence: primordial power spectra and non-Gaussianities","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.07598","snapshot_observed_at":"2026-08-03T06:50:28.877895Z","title":"Daddi Hammou and N","venue":null,"work_id":null,"year":2023},"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":37,"source":"pdf_text","source_observed_at":"2026-08-03T06:50:28.877895Z"},"links":{"cited_paper":"/paper/2211.07598","citing_paper":"/paper/2601.22219"},"observation_digest":"sha256:c9ecd0f75f11bc3cc6fb59dffd51a7e0c0e2e173479bd3ede971799e44414931","observation_id":"5c1ebd34-1a13-42b2-9863-eb861e8b6aa5","resolution":{"observed_at":"2026-08-03T06:50:28.877895Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.07598","last_updated":"2023-04-25T20:31:48Z","snapshot_observed_at":"2026-08-08T15:00:26.501973Z","submitted_at":"2022-11-14T18:24:52Z","title":"Cosmic decoherence: primordial power spectra and non-Gaussianities","version":2},"cited_work":{"arxiv_id":"2211.07598","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2211.07598","snapshot_observed_at":"2026-06-30T17:04:56.959061Z","title":"Daddi Hammou and N","venue":null,"work_id":"88ed5f36-ef97-4650-8303-350dbf8afcc1","year":2023},"citing_paper":{"arxiv_id":"2604.15219","last_updated":"2026-04-28T15:13:43Z","snapshot_observed_at":"2026-07-06T23:02:49.302337Z","submitted_at":"2026-04-16T16:50:33Z","title":"Nonperturbative stochastic inflation in perturbative dynamical background","version":2},"reference_index":112,"source":"pdf_text","source_observed_at":"2026-05-10T09:51:09.373721Z"},"links":{"cited_paper":"/paper/2211.07598","citing_paper":"/paper/2604.15219"},"observation_digest":"sha256:99d8936898adcd03cf7776d77c94558aa4c1254c8c36abb50bff6fd040313e69","observation_id":"22a08fc0-4aa3-4cff-a5c8-76cf83db69c9","resolution":{"observed_at":"2026-05-10T10:04:07.491308Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.07598","last_updated":"2023-04-25T20:31:48Z","snapshot_observed_at":"2026-08-08T15:00:26.501973Z","submitted_at":"2022-11-14T18:24:52Z","title":"Cosmic decoherence: primordial power spectra and non-Gaussianities","version":2},"cited_work":{"arxiv_id":"2211.07598","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2211.07598","snapshot_observed_at":"2026-06-30T17:04:56.959061Z","title":"Daddi Hammou and N","venue":null,"work_id":"88ed5f36-ef97-4650-8303-350dbf8afcc1","year":2023},"citing_paper":{"arxiv_id":"2604.26941","last_updated":"2026-05-22T14:30:35Z","snapshot_observed_at":"2026-07-06T23:12:29.385105Z","submitted_at":"2026-04-29T17:52:04Z","title":"Schwinger-Keldysh Path Integral for Gauge theories","version":1},"reference_index":140,"source":"pdf_text","source_observed_at":"2026-05-07T08:34:39.997424Z"},"links":{"cited_paper":"/paper/2211.07598","citing_paper":"/paper/2604.26941"},"observation_digest":"sha256:48a3228afb032c36699b8abe25620aed0fa4180eafcfac2e9e1a6dbc23ee2e3a","observation_id":"9a8caaad-7ec3-4f16-a931-948ebf102367","resolution":{"observed_at":"2026-05-12T09:56:28.672865Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.07598","last_updated":"2023-04-25T20:31:48Z","snapshot_observed_at":"2026-08-08T15:00:26.501973Z","submitted_at":"2022-11-14T18:24:52Z","title":"Cosmic decoherence: primordial power spectra and non-Gaussianities","version":2},"cited_work":{"arxiv_id":"2211.07598","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2211.07598","snapshot_observed_at":"2026-06-30T17:04:56.959061Z","title":"Daddi Hammou and N","venue":null,"work_id":"88ed5f36-ef97-4650-8303-350dbf8afcc1","year":2023},"citing_paper":{"arxiv_id":"2604.26941","last_updated":"2026-05-22T14:30:35Z","snapshot_observed_at":"2026-07-06T23:12:29.385105Z","submitted_at":"2026-04-29T17:52:04Z","title":"Schwinger-Keldysh Path Integral for Gauge theories","version":2},"reference_index":140,"source":"pdf_text","source_observed_at":"2026-05-25T06:27:51.835823Z"},"links":{"cited_paper":"/paper/2211.07598","citing_paper":"/paper/2604.26941"},"observation_digest":"sha256:34da4b3ae899c5378970e8c386658c360fb2ea209dd6fe4925a7c60a23bba565","observation_id":"38b68d21-12e9-4dcb-8eac-4f9c9276f146","resolution":{"observed_at":"2026-05-25T06:30:24.720235Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.07598","last_updated":"2023-04-25T20:31:48Z","snapshot_observed_at":"2026-08-08T15:00:26.501973Z","submitted_at":"2022-11-14T18:24:52Z","title":"Cosmic decoherence: primordial power spectra and non-Gaussianities","version":2},"cited_work":{"arxiv_id":"2211.07598","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2211.07598","snapshot_observed_at":"2026-06-30T17:04:56.959061Z","title":"Daddi Hammou and N","venue":null,"work_id":"88ed5f36-ef97-4650-8303-350dbf8afcc1","year":2023},"citing_paper":{"arxiv_id":"2605.21929","last_updated":"2026-06-20T21:27:46Z","snapshot_observed_at":"2026-08-01T15:50:02.368617Z","submitted_at":"2026-05-21T02:57:40Z","title":"Stochastic inflation as an open quantum system II: open effective field theory and stochastic matching","version":1},"reference_index":142,"source":"pdf_text","source_observed_at":"2026-05-22T05:40:46.666696Z"},"links":{"cited_paper":"/paper/2211.07598","citing_paper":"/paper/2605.21929"},"observation_digest":"sha256:86d61b9fbc873163bf10fb67b4d462ed9e0237d2b0119544998d8652a6e6141b","observation_id":"e9091dbf-a0b4-4201-b694-1a6d5df4058d","resolution":{"observed_at":"2026-05-22T05:41:08.125951Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.07598","last_updated":"2023-04-25T20:31:48Z","snapshot_observed_at":"2026-08-08T15:00:26.501973Z","submitted_at":"2022-11-14T18:24:52Z","title":"Cosmic decoherence: primordial power spectra and non-Gaussianities","version":2},"cited_work":{"arxiv_id":"2211.07598","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2211.07598","snapshot_observed_at":"2026-06-30T17:04:56.959061Z","title":"Daddi Hammou and N","venue":null,"work_id":"88ed5f36-ef97-4650-8303-350dbf8afcc1","year":2023},"citing_paper":{"arxiv_id":"2605.21929","last_updated":"2026-06-20T21:27:46Z","snapshot_observed_at":"2026-08-01T15:50:02.368617Z","submitted_at":"2026-05-21T02:57:40Z","title":"Stochastic inflation as an open quantum system II: open effective field theory and stochastic matching","version":2},"reference_index":142,"source":"pdf_text","source_observed_at":"2026-06-30T16:59:26.792559Z"},"links":{"cited_paper":"/paper/2211.07598","citing_paper":"/paper/2605.21929"},"observation_digest":"sha256:f46ec4f66f85d2693acb6cf6b27e26b070a5d3e6c5fdb2df6a429c87006e80db","observation_id":"18a07946-96fb-4295-9c97-23f100dd92c1","resolution":{"observed_at":"2026-06-30T17:04:56.960588Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2211.07598/citation-record","integrity":"/paper/2211.07598/integrity","json":"/paper/2211.07598/citation-record.json","paper":"/paper/2211.07598"},"outbound":[],"paper":{"arxiv_id":"2211.07598","last_updated":"2023-04-25T20:31:48Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-08T15:00:26.501973Z","submitted_at":"2022-11-14T18:24:52Z","title":"Cosmic decoherence: primordial power spectra and non-Gaussianities"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2211.07598."}