{"as_of":"2026-08-21T02:00:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:fdb239b17d1819127c27c05c2780b805f3ec146e3cbf1d3e70753ced3e075822","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":8,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":8,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-20T06:33:59.587034+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T12:03:21.993772Z","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":"2026-07-01T11:15:41.838922Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2204.02190","last_updated":"2022-09-28T17:20:46Z","snapshot_observed_at":"2026-08-19T16:16:24.018517Z","submitted_at":"2022-04-05T13:13:43Z","title":"Healing the cosmological constant problem during inflation through a unified quasi-quintessence matter field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.02190","snapshot_observed_at":"2026-08-10T04:37:02.458003Z","title":"D’Agostino, O","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.18007","last_updated":"2025-04-14T10:08:54Z","snapshot_observed_at":"2026-08-18T15:23:12.555374Z","submitted_at":"2025-01-29T21:47:30Z","title":"Nonlocal gravity in a proper tetrad frame: traversable wormholes","version":3},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-10T04:37:02.458003Z"},"links":{"cited_paper":"/paper/2204.02190","citing_paper":"/paper/2501.18007"},"observation_digest":"sha256:355395ff97cf1bda1a6757aaa5559b8957b28a3398ac46ba10a52a551520b942","observation_id":"9018fa5f-bfb0-40ad-bfdf-261d12442fe6","resolution":{"observed_at":"2026-08-10T04:37:02.458003Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.02190","last_updated":"2022-09-28T17:20:46Z","snapshot_observed_at":"2026-08-19T16:16:24.018517Z","submitted_at":"2022-04-05T13:13:43Z","title":"Healing the cosmological constant problem during inflation through a unified quasi-quintessence matter field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.02190","snapshot_observed_at":"2026-08-16T12:03:21.993772Z","title":"D’Agostino, O","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.14229","last_updated":"2025-04-19T08:38:48Z","snapshot_observed_at":"2026-08-19T16:08:48.223942Z","submitted_at":"2025-04-19T08:38:48Z","title":"K-essence sources of Kerr-Schild spacetimes","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-16T12:03:21.993772Z"},"links":{"cited_paper":"/paper/2204.02190","citing_paper":"/paper/2504.14229"},"observation_digest":"sha256:9d761f2036d71ed601f5e783084397e398643900654965d5fbb823bd56307331","observation_id":"206afdae-ec25-45e7-8549-6b96cf77afb9","resolution":{"observed_at":"2026-08-16T12:03:21.993772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.02190","last_updated":"2022-09-28T17:20:46Z","snapshot_observed_at":"2026-08-19T16:16:24.018517Z","submitted_at":"2022-04-05T13:13:43Z","title":"Healing the cosmological constant problem during inflation through a unified quasi-quintessence matter field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.02190","snapshot_observed_at":"2026-08-15T23:56:22.960069Z","title":"D’Agostino, O","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.03644","last_updated":"2025-05-06T15:51:13Z","snapshot_observed_at":"2026-08-20T23:44:03.676254Z","submitted_at":"2025-05-06T15:51:13Z","title":"Consequences of non-minimal coupling for mass mixing in spontaneous baryogenesis","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-15T23:56:22.960069Z"},"links":{"cited_paper":"/paper/2204.02190","citing_paper":"/paper/2505.03644"},"observation_digest":"sha256:327ebbb47b029ef3e775bc420fa8fb1f30766919f404fc9bf2969e7823c444e9","observation_id":"6e6b495b-3d3f-444f-b536-82b78b5dfbfe","resolution":{"observed_at":"2026-08-15T23:56:22.960069Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.02190","last_updated":"2022-09-28T17:20:46Z","snapshot_observed_at":"2026-08-19T16:16:24.018517Z","submitted_at":"2022-04-05T13:13:43Z","title":"Healing the cosmological constant problem during inflation through a unified quasi-quintessence matter field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.02190","snapshot_observed_at":"2026-08-07T13:42:39.659689Z","title":"D’Agostino, O","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.21359","last_updated":"2025-05-27T15:52:14Z","snapshot_observed_at":"2026-08-16T06:46:25.246040Z","submitted_at":"2025-05-27T15:52:14Z","title":"Teleparallel dark energy in a nonflat universe","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-07T13:42:39.659689Z"},"links":{"cited_paper":"/paper/2204.02190","citing_paper":"/paper/2505.21359"},"observation_digest":"sha256:88935177009c4ad9d25fc2e74a355462fb1012e8e38af00cf76129999ea2d6e7","observation_id":"0d9521b3-0508-4ba9-96cc-b3def8bc2a27","resolution":{"observed_at":"2026-08-07T13:42:39.659689Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.02190","last_updated":"2022-09-28T17:20:46Z","snapshot_observed_at":"2026-08-19T16:16:24.018517Z","submitted_at":"2022-04-05T13:13:43Z","title":"Healing the cosmological constant problem during inflation through a unified quasi-quintessence matter field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.02190","snapshot_observed_at":"2026-08-06T20:53:53.044894Z","title":"D’Agostino, O","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.01698","last_updated":"2025-08-27T14:11:04Z","snapshot_observed_at":"2026-08-10T08:12:26.183595Z","submitted_at":"2025-07-02T13:28:11Z","title":"Quasinormal modes of nonlocal gravity black holes","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T20:53:53.044894Z"},"links":{"cited_paper":"/paper/2204.02190","citing_paper":"/paper/2507.01698"},"observation_digest":"sha256:586c62c7156ec6d02150a672ca0dfc76f76819249a12c65cb5d3a12b27a5fa38","observation_id":"2531a49b-460d-4320-b735-ef2ff29a7cdf","resolution":{"observed_at":"2026-08-06T20:53:53.044894Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.02190","last_updated":"2022-09-28T17:20:46Z","snapshot_observed_at":"2026-08-19T16:16:24.018517Z","submitted_at":"2022-04-05T13:13:43Z","title":"Healing the cosmological constant problem during inflation through a unified quasi-quintessence matter field","version":2},"cited_work":{"arxiv_id":"2204.02190","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2204.02190","snapshot_observed_at":"2026-07-01T11:15:41.838922Z","title":"D’Agostino, O","venue":null,"work_id":"24462f4c-2a77-4c2c-8e41-238f14c50d62","year":2022},"citing_paper":{"arxiv_id":"2604.13223","last_updated":"2026-04-14T18:48:44Z","snapshot_observed_at":"2026-08-20T10:32:30.697576Z","submitted_at":"2026-04-14T18:48:44Z","title":"Observational constraints on nonlocal black holes via gravitational lensing","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-05-10T14:12:31.058346Z"},"links":{"cited_paper":"/paper/2204.02190","citing_paper":"/paper/2604.13223"},"observation_digest":"sha256:4a85778b7f288c8aee516d815d94b62f78acd15e0f863c61512582c41cccde33","observation_id":"607f6bc3-930a-4dc0-8def-b19661a3e7dc","resolution":{"observed_at":"2026-05-10T14:15:29.496576Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2204.02190","last_updated":"2022-09-28T17:20:46Z","snapshot_observed_at":"2026-08-19T16:16:24.018517Z","submitted_at":"2022-04-05T13:13:43Z","title":"Healing the cosmological constant problem during inflation through a unified quasi-quintessence matter field","version":2},"cited_work":{"arxiv_id":"2204.02190","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2204.02190","snapshot_observed_at":"2026-07-01T11:15:41.838922Z","title":"D’Agostino, O","venue":null,"work_id":"24462f4c-2a77-4c2c-8e41-238f14c50d62","year":2022},"citing_paper":{"arxiv_id":"2605.06147","last_updated":"2026-05-07T12:41:16Z","snapshot_observed_at":"2026-08-11T02:20:00.276502Z","submitted_at":"2026-05-07T12:41:16Z","title":"Cosmological Dynamics of a Non-Canonical Generalised Brans-Dicke Theory","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-05-08T07:21:03.498420Z"},"links":{"cited_paper":"/paper/2204.02190","citing_paper":"/paper/2605.06147"},"observation_digest":"sha256:ce8fe318e8b6809721c43addada91507ec24bdffdab9e13473c46cb4e02d20bb","observation_id":"bb9d446a-5bfb-48ce-a211-a966aea0dc99","resolution":{"observed_at":"2026-05-11T21:01:12.849349Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2204.02190","last_updated":"2022-09-28T17:20:46Z","snapshot_observed_at":"2026-08-19T16:16:24.018517Z","submitted_at":"2022-04-05T13:13:43Z","title":"Healing the cosmological constant problem during inflation through a unified quasi-quintessence matter field","version":2},"cited_work":{"arxiv_id":"2204.02190","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2204.02190","snapshot_observed_at":"2026-07-01T11:15:41.838922Z","title":"D’Agostino, O","venue":null,"work_id":"24462f4c-2a77-4c2c-8e41-238f14c50d62","year":2022},"citing_paper":{"arxiv_id":"2606.31299","last_updated":"2026-06-30T08:11:29Z","snapshot_observed_at":"2026-08-19T05:11:02.307405Z","submitted_at":"2026-06-30T08:11:29Z","title":"Distance duality relation in symmetric teleparallel gravity","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-07-01T04:41:07.434638Z"},"links":{"cited_paper":"/paper/2204.02190","citing_paper":"/paper/2606.31299"},"observation_digest":"sha256:c131ec4170ed157f05089bfc3f28b77878e0311aeb6a4e47d7660abd986160c3","observation_id":"8cfcdabd-5aeb-47d8-8fbc-208ba90e0ffd","resolution":{"observed_at":"2026-07-01T11:15:41.840226Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2204.02190/citation-record","integrity":"/paper/2204.02190/integrity","json":"/paper/2204.02190/citation-record.json","paper":"/paper/2204.02190"},"outbound":[],"paper":{"arxiv_id":"2204.02190","last_updated":"2022-09-28T17:20:46Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-19T16:16:24.018517Z","submitted_at":"2022-04-05T13:13:43Z","title":"Healing the cosmological constant problem during inflation through a unified quasi-quintessence matter field"},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2204.02190."}