{"as_of":"2026-08-11T20:35:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:93c661968c290a744ad5d3fb2058237cbe9dd7ab363d8153144d579c2b89a098","coverage":[{"denominator":116,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T04:18:40.330925Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2608.07774/citation-record","integrity":"/paper/2608.07774/integrity","json":"/paper/2608.07774/citation-record.json","paper":"/paper/2608.07774"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.145198Z","title":"Twistor theory: An approach to the quantisation of fields and space-time,","venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.145198Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:079ce251071925b28cd9d0b3921b06ce12946431dec6f2072cf2822d94a9aa3c","observation_id":"d9aefa5a-9bd6-46c6-9d99-fd7c63eea26e","resolution":{"observed_at":"2026-08-11T04:18:39.145198Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.07464","last_updated":"2017-09-08T12:50:08Z","snapshot_observed_at":"2026-07-06T05:39:09.619914Z","submitted_at":"2017-04-24T20:59:58Z","title":"Twistor theory at fifty: from contour integrals to twistor strings","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.07464","snapshot_observed_at":"2026-08-11T04:18:39.176844Z","title":"Twistor theory at fifty: from contour integrals to twistor strings,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.176844Z"},"links":{"cited_paper":"/paper/1704.07464","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:933fdd307aadaec64a73a234c4c518d08d1be34689e824f35e91a1a55aacd4c2","observation_id":"8dfd32f7-2555-4f46-bf32-c44a97875fe6","resolution":{"observed_at":"2026-08-11T04:18:39.176844Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.238135Z","title":"Nonlinear gravitons and curved twistor theory,","venue":null,"work_id":null,"year":1976},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.238135Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:a017e011caf9af891469c1de74464df261fcc2378957ffecf3b22779347c9768","observation_id":"2ea7d48b-00c9-4311-8c04-8ce71c400eda","resolution":{"observed_at":"2026-08-11T04:18:39.238135Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0808.3907","last_updated":"2009-10-26T17:07:25Z","snapshot_observed_at":"2026-08-10T07:13:02.104657Z","submitted_at":"2008-08-28T16:32:06Z","title":"Gravity, Twistors and the MHV Formalism","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0808.3907","snapshot_observed_at":"2026-08-11T04:18:39.272002Z","title":"Gravity, twistors and the MHV formalism,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.272002Z"},"links":{"cited_paper":"/paper/0808.3907","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:02ce9f982931c56c45f61c3ce19a2002677518a208b1220ebc064383959fd74c","observation_id":"6440e32a-85b7-4bcd-9b6a-cd98471170bf","resolution":{"observed_at":"2026-08-11T04:18:39.272002Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.276637Z","title":"A connection between the Einstein and Yang-Mills equations,","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.276637Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:886d0661922ec899df025235e6801802f1b8a17ae04ba49c9f379496cec67e5a","observation_id":"8a1829df-828c-427b-941d-28299bd63d2e","resolution":{"observed_at":"2026-08-11T04:18:39.276637Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.280703Z","title":"Some solutions of complex Einstein equations,","venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.280703Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:d443131badc0685033649a938aa313f5a1d5801ece71591cce21e5aa8919b140","observation_id":"16e48cc7-9bf7-42c0-b9e7-13cc6a730223","resolution":{"observed_at":"2026-08-11T04:18:39.280703Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.285039Z","title":"On the separation of Einsteinian substructures,","venue":null,"work_id":null,"year":1977},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.285039Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:977a0987724e5c0a80330715bc57952060b52a62b68c822cbb3cde498d9b9477","observation_id":"c5fb3e6c-2c99-4b16-bdf0-da7ea0baccb3","resolution":{"observed_at":"2026-08-11T04:18:39.285039Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.289219Z","title":"Self-dual two-forms and gravity,","venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.289219Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:11735ca5b9e731e078739c05c1cf61507e0f0d3f6d52cfa5b601a5a0ff4d7bfb","observation_id":"7f8f6548-062c-4963-a201-c04b0ba170f7","resolution":{"observed_at":"2026-08-11T04:18:39.289219Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.292650Z","title":"Sur le probl` eme de Pfaff,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.292650Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:1e96710b0ecd18b067cc4c3bb06f73f137936d2a616caa94fe45dad2e59b7b50","observation_id":"2050c2e2-8425-4e7d-afcc-5f1e1196d690","resolution":{"observed_at":"2026-08-11T04:18:39.292650Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.16984","last_updated":"2022-01-17T15:18:42Z","snapshot_observed_at":"2026-08-11T19:55:32.201319Z","submitted_at":"2021-03-31T11:00:48Z","title":"Twistor sigma models for quaternionic geometry and graviton scattering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.16984","snapshot_observed_at":"2026-08-11T04:18:39.296665Z","title":"Twistor sigma models for quaternionic geometry and graviton scattering,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.296665Z"},"links":{"cited_paper":"/paper/2103.16984","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:3b1e71cb70bf2c4116d9810c23b3176781b0b00c5066aaad250730adc70a5ddc","observation_id":"833cb4bc-05ce-4da0-9a63-a9d7b531f677","resolution":{"observed_at":"2026-08-11T04:18:39.296665Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"math/0001008","last_updated":"2000-01-03T19:19:51Z","snapshot_observed_at":"2026-08-06T01:44:37.912589Z","submitted_at":"2000-01-03T19:19:51Z","title":"Hyper-K{\\\"a}hler Hierarchies and their twistor theory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"math/0001008","snapshot_observed_at":"2026-08-11T04:18:39.301889Z","title":"Hyper-K¨ ahler hierarchies and their twistor theory,","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.301889Z"},"links":{"cited_paper":"/paper/math/0001008","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:738b52a8067ccc3231520b6864b75daabdb004da17891927d2ad6e6b66ce2dfc","observation_id":"68345a18-2ab3-4cff-ab73-1ba7eddf30b8","resolution":{"observed_at":"2026-08-11T04:18:39.301889Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.306737Z","title":"Heavenly hierarchies and curved twistor spaces,","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.306737Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:30a8c3912915abfc7e272399620d466fb420f79cb0c9b407ba60c78d8a05af3e","observation_id":"d099e136-fb23-40c5-842b-7a4ebb9651ce","resolution":{"observed_at":"2026-08-11T04:18:39.306737Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.310303Z","title":"A recursion operator for ASD vacuums and z.r.m fields,","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.310303Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:f8544b5b7e6abde6dcc979481472bf4e883ac346a39016d264c0e8c4a2376e47","observation_id":"209e392a-c823-4c48-9fc4-89a8a236a61f","resolution":{"observed_at":"2026-08-11T04:18:39.310303Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.03834","last_updated":"2024-11-11T15:22:54Z","snapshot_observed_at":"2026-08-07T04:57:49.778215Z","submitted_at":"2023-09-07T16:49:01Z","title":"Scattering on self-dual Taub-NUT","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.03834","snapshot_observed_at":"2026-08-11T04:18:39.314120Z","title":"Scattering on self-dual Taub-NUT,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.314120Z"},"links":{"cited_paper":"/paper/2309.03834","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:5c91bf2848dd81378809d9d6001c6b8ca70ca07879f501984bcafb8daf733102","observation_id":"1d8dce0b-118c-4a34-8d4b-4203c7a1e502","resolution":{"observed_at":"2026-08-11T04:18:39.314120Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2507.18605","last_updated":"2026-04-29T09:35:15Z","snapshot_observed_at":"2026-08-03T07:43:33.216943Z","submitted_at":"2025-07-24T17:38:25Z","title":"Graviton scattering on self-dual black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.18605","snapshot_observed_at":"2026-08-11T04:18:39.318243Z","title":"Graviton scattering on self-dual black holes,","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.318243Z"},"links":{"cited_paper":"/paper/2507.18605","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:47bbe49455b380b3478450d249020236b7082b549cbf0838c55057f1ea2540c2","observation_id":"5d20d1d1-8620-4fe0-9195-96a3dc37455c","resolution":{"observed_at":"2026-08-11T04:18:39.318243Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03954","last_updated":"2021-12-07T19:24:22Z","snapshot_observed_at":"2026-08-10T13:51:52.795781Z","submitted_at":"2021-12-07T19:24:22Z","title":"Black Holes in Klein Space","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.03954","snapshot_observed_at":"2026-08-11T04:18:39.355586Z","title":"Black holes in Klein space,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.355586Z"},"links":{"cited_paper":"/paper/2112.03954","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:2041a91a1bbdd9a34e1a28334643732db5e56afb0253514b4f5aff1722eebccd","observation_id":"f6fb4bad-eb98-43d5-b62b-f5b4ed365d0d","resolution":{"observed_at":"2026-08-11T04:18:39.355586Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.06661","last_updated":"2023-02-13T19:47:06Z","snapshot_observed_at":"2026-07-30T16:22:15.016715Z","submitted_at":"2023-02-13T19:47:06Z","title":"Self-Dual Black Holes in Celestial Holography","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.06661","snapshot_observed_at":"2026-08-11T04:18:39.404167Z","title":"Self-dual black holes in celestial holography,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.404167Z"},"links":{"cited_paper":"/paper/2302.06661","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:0709955bfab9ed9db6c2b8a6ce72d88fc98ad926567ef93994d878f855630ce1","observation_id":"d84bfe82-bf7b-4b79-8756-e6ff3bff790e","resolution":{"observed_at":"2026-08-11T04:18:39.404167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.07933","last_updated":"2024-01-23T14:34:31Z","snapshot_observed_at":"2026-08-10T06:54:20.807894Z","submitted_at":"2023-11-14T06:23:05Z","title":"Self Dual Black Holes as the Hydrogen Atom","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.07933","snapshot_observed_at":"2026-08-11T04:18:39.448557Z","title":"Self dual black holes as the hydrogen atom,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.448557Z"},"links":{"cited_paper":"/paper/2311.07933","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:4ac2ae64fb536991810dba0da11fb5e17c31f1fb22cd2833f92997f9df84f9db","observation_id":"6d8d32d3-1d32-49a8-bd73-187253576afe","resolution":{"observed_at":"2026-08-11T04:18:39.448557Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.19627","last_updated":"2024-12-27T13:13:27Z","snapshot_observed_at":"2026-08-11T19:26:08.626368Z","submitted_at":"2024-12-27T13:13:27Z","title":"An Exact Black Hole Scattering Amplitude","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.19627","snapshot_observed_at":"2026-08-11T04:18:39.461920Z","title":"An exact black hole scattering amplitude,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.461920Z"},"links":{"cited_paper":"/paper/2412.19627","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:3db216aea3b7ece60d601083397f384c8b3792614af1a43ae5d1e570dbfb80b7","observation_id":"9e6fa5cb-d4b1-4c0a-965f-e7a51f9226fd","resolution":{"observed_at":"2026-08-11T04:18:39.461920Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2511.18637","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:41.370765Z","title":"New near extremal black holes and love symmetry,","venue":null,"work_id":"e02cca9c-aede-4e88-8da3-323bcf75ecf6","year":null},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.467295Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:3abe1aaf5a56b9cf27dddf1a69e1dfb285b119209de26a39c72f4a07cb72201d","observation_id":"11ff85fb-2612-4c9b-a2db-35fccd24b70b","resolution":{"observed_at":"2026-08-11T04:18:41.385246Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.471347Z","title":"Note on the Kerr spinning-particle equations of motion,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.471347Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:ddbe02c35252677aa89f97cb6c06e000de767d4adb134dd3c2cf8f3466264959","observation_id":"fd9c6e57-13a0-4597-811a-5e5aa8cab7b3","resolution":{"observed_at":"2026-08-11T04:18:39.471347Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.09518","last_updated":"2024-12-21T20:18:52Z","snapshot_observed_at":"2026-08-08T00:34:26.392713Z","submitted_at":"2024-05-15T17:19:28Z","title":"Single Kerr-Schild Metric for Taub-NUT Instanton","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.09518","snapshot_observed_at":"2026-08-11T04:18:39.475360Z","title":"Single Kerr-Schild metric for Taub-NUT instanton,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.475360Z"},"links":{"cited_paper":"/paper/2405.09518","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:f8d3c68336cdd3c93d1bafd43591665283a17c810b04ec81848eb556f9ddb62a","observation_id":"f79abfe4-8369-41d3-861d-db99a98389c4","resolution":{"observed_at":"2026-08-11T04:18:39.475360Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.19611","last_updated":"2026-01-19T14:24:46Z","snapshot_observed_at":"2026-08-11T05:05:05.215468Z","submitted_at":"2024-12-27T12:16:20Z","title":"Newman-Janis Algorithm from Taub-NUT Instantons","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.19611","snapshot_observed_at":"2026-08-11T04:18:39.479668Z","title":"Newman-Janis algorithm from Taub-NUT instantons,","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.479668Z"},"links":{"cited_paper":"/paper/2412.19611","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:d927548012d369cae119b0029f1af12c17f40e2a0ff0ce80e47f61e26076eec2","observation_id":"7df61088-d731-4291-bbad-46158ef10e09","resolution":{"observed_at":"2026-08-11T04:18:39.479668Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.483769Z","title":"The dual twistor theory of self-dual black holes,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.483769Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:0600e67f0e69f8b8a7a47f33c887e0baf5decff45a6a58c4e7a38ad6b6b192e0","observation_id":"7ec84e01-18d7-4153-adcc-8812df6e8321","resolution":{"observed_at":"2026-08-11T04:18:39.483769Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2508.18804","last_updated":"2025-08-26T08:38:37Z","snapshot_observed_at":"2026-08-06T02:58:50.224063Z","submitted_at":"2025-08-26T08:38:37Z","title":"Higher-spins on Taub-NUT and higher-spin Taub-NUT","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2508.18804","snapshot_observed_at":"2026-08-11T04:18:39.487934Z","title":"Higher-spins on Taub-NUT and higher-spin Taub-NUT,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.487934Z"},"links":{"cited_paper":"/paper/2508.18804","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:1cfdfb60581bd743bfd29393402a9d2206736364239c03ab75e09b4ff7aec606","observation_id":"c69769c4-803e-4522-9153-10a0d39d1c04","resolution":{"observed_at":"2026-08-11T04:18:39.487934Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2603.24365","last_updated":"2026-06-01T12:30:08Z","snapshot_observed_at":"2026-08-09T18:11:12.868178Z","submitted_at":"2026-03-25T14:45:40Z","title":"Memory effect from the scattering of Taub-NUT black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2603.24365","snapshot_observed_at":"2026-08-11T04:18:39.493558Z","title":"Memory effect from the scattering of Taub-NUT black holes,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.493558Z"},"links":{"cited_paper":"/paper/2603.24365","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:db3b1a61e527db3467be4f495f7c50d251cfb0895e62894b649db03148d4e979","observation_id":"15fcf257-bd1b-409d-9e06-673cd9afeb60","resolution":{"observed_at":"2026-08-11T04:18:39.493558Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.503433Z","title":"Rotating, charged, and uniformly accelerating mass in general relativity,","venue":null,"work_id":null,"year":1976},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.503433Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:abe46cd781e37a306f6d53b2a19cbffb2c47b745306a952369fe6a716e372741","observation_id":"332984d5-506a-43ef-a21f-f7203e35fb87","resolution":{"observed_at":"2026-08-11T04:18:39.503433Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.531560Z","title":"Asymptotically flat selfdual solutions to Euclidean gravity,","venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.531560Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:1fb38f5415ec0c77112cab9df13859ba116978bee775f2c63301833eb1561579","observation_id":"79bb84b7-1a38-4340-a4d8-ab0115b9a26f","resolution":{"observed_at":"2026-08-11T04:18:39.531560Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.558633Z","title":"Selfdual solutions to Euclidean gravity,","venue":null,"work_id":null,"year":1979},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.558633Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:739600cfd74d61f1db3bc157c08f5712a26b7fb8c83be1ec32319e3c27aceb5a","observation_id":"c275b2fc-bcda-4984-8485-2f9d54a3f96d","resolution":{"observed_at":"2026-08-11T04:18:39.558633Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.583132Z","title":"Gravitational instantons,","venue":null,"work_id":null,"year":1979},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.583132Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:4b0633df4085450f7366478e6a349c112eb43eeefb9c6666cd1282d5c5f13e61","observation_id":"e6001083-67eb-4a4f-bd42-998bc8a93004","resolution":{"observed_at":"2026-08-11T04:18:39.583132Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.605916Z","title":"Gravitational instantons,","venue":null,"work_id":null,"year":1977},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.605916Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:5edd09ed42dbb0f9051bfa8a9f2773dcfa5ec35885f4a15549d7cdb45a934f77","observation_id":"1e2e8398-11cd-48e1-93f3-7db923a2e0b0","resolution":{"observed_at":"2026-08-11T04:18:39.605916Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.627868Z","title":"Gravitational multi-instantons,","venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.627868Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:c7ad22e0fa7f2678ff5d3e0ba92174c10aa3a27f8d67acfa3e1fdc0452e0a2e5","observation_id":"fe3546b3-fa13-4953-ab20-a42b33c127bc","resolution":{"observed_at":"2026-08-11T04:18:39.627868Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0110280","last_updated":"2002-03-25T17:03:40Z","snapshot_observed_at":"2026-07-07T04:41:32.540814Z","submitted_at":"2001-10-30T16:52:47Z","title":"U(1) x U(1) Quaternionic Metrics from Harmonic Superspace","version":2},"cited_work":{"arxiv_id":"hep-th/0110280","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-th/0110280","snapshot_observed_at":"2026-08-11T04:18:41.047276Z","title":"U(1) x U(1) Quaternionic Metrics from Harmonic Superspace","venue":"hep-th","work_id":"556a7533-67f7-4405-a520-2e089c6f84ba","year":2001},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.631792Z"},"links":{"cited_paper":"/paper/hep-th/0110280","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:27fc50dd9d36fface1fe27140e78bb9f463b5a30819e4e5c91107260bd97a0ab","observation_id":"5c143709-03a3-4c77-89da-446f328df868","resolution":{"observed_at":"2026-08-11T04:18:41.081317Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1510.07470","last_updated":"2016-05-16T02:33:24Z","snapshot_observed_at":"2026-07-06T04:34:14.912841Z","submitted_at":"2015-10-26T13:21:52Z","title":"Killing-Yano tensor and supersymmetry of the self-dual Plebanski-Demianski solution","version":3},"cited_work":{"arxiv_id":"1510.07470","doi":null,"metadata_source":"pith","pith_arxiv_id":"1510.07470","snapshot_observed_at":"2026-08-11T04:18:41.030946Z","title":"Killing-Yano tensor and supersymmetry of the self-dual Plebanski-Demianski solution","venue":"hep-th","work_id":"9b5705af-726b-4485-a256-83f9a4497a94","year":2015},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.636705Z"},"links":{"cited_paper":"/paper/1510.07470","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:a3e0f4898a379d71344147cc62cf9b306b42a13a16a93481f634cf3689fa97b1","observation_id":"5a3ea283-8fcf-4a49-a3ea-237dc0558f10","resolution":{"observed_at":"2026-08-11T04:18:41.035530Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.05617","last_updated":"2024-11-11T08:55:19Z","snapshot_observed_at":"2026-07-06T16:17:04.004519Z","submitted_at":"2023-09-11T17:05:43Z","title":"Hidden symmetries of generalised gravitational instantons","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.05617","snapshot_observed_at":"2026-08-11T04:18:39.640294Z","title":"Hidden symmetries of generalised gravitational instantons,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.640294Z"},"links":{"cited_paper":"/paper/2309.05617","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:8b9ba4832d479e0515cc9797e58cef649af607c1a39427ed4c3e07c705b3e73e","observation_id":"2ca17cc2-7abd-4ac8-9e92-d994eb3b240a","resolution":{"observed_at":"2026-08-11T04:18:39.640294Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.644349Z","title":"Self-dual Kerr-Schild metrics and null Maxwell fields,","venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.644349Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:26688b91a88338a77d008349d7e442d9d55032018a4534b19c8929d74cbe2ba0","observation_id":"1059afd3-17e0-46f6-a071-4029d17e986f","resolution":{"observed_at":"2026-08-11T04:18:39.644349Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.648098Z","title":"Sparling-Tod metric = Eguchi-Hanson,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.648098Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:8d30f8382e6b07f99235e0b418eacd3b886a0cbb69c962d5a3a7fe8e3a9e34c3","observation_id":"2b016420-c53d-4a70-9a53-d4cf8c381eb2","resolution":{"observed_at":"2026-08-11T04:18:39.648098Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.04063","last_updated":"2018-09-27T15:43:42Z","snapshot_observed_at":"2026-08-08T17:13:17.639836Z","submitted_at":"2018-09-11T17:51:53Z","title":"The self-dual classical double copy, and the Eguchi-Hanson instanton","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.04063","snapshot_observed_at":"2026-08-11T04:18:39.656815Z","title":"The self-dual classical double copy, and the Eguchi-Hanson instanton,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.656815Z"},"links":{"cited_paper":"/paper/1809.04063","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:245e49f7a26f10e4eec1b01b05a6069c96c52992c1ccdb679e4a32b0004ba399","observation_id":"a0d56419-c671-4e56-bb80-3797bd85bb8f","resolution":{"observed_at":"2026-08-11T04:18:39.656815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.661075Z","title":"The non-linear graviton representing the analogue of schwarzschild or kerr black holes,","venue":null,"work_id":null,"year":1976},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.661075Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:2066cfabffcbf35aa60add1a2b4ae74f36add9860c51934a3746f4483a1fa244","observation_id":"3c39d750-564e-4a2c-8151-1cc62c0f4efa","resolution":{"observed_at":"2026-08-11T04:18:39.661075Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.664846Z","title":"Polygons and gravitons,","venue":null,"work_id":null,"year":1979},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.664846Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:e59ea728181f769aa1c3c6ee7f3d2453e1224de77a09b481659ae311169a71e9","observation_id":"415d5ac5-0917-4e20-963f-f9adbd699ea0","resolution":{"observed_at":"2026-08-11T04:18:39.664846Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.668914Z","title":"Complete ricci-flat k¨ ahler metrics onC n need not be flat,","venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.668914Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:969352f27478184c4c0436d3d4f0788a013146acac304384ea06c3cff96ef53b","observation_id":"8fe94069-deb7-4c6a-82a0-1c434ae852b4","resolution":{"observed_at":"2026-08-11T04:18:39.668914Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2607.06236","last_updated":"2026-07-07T13:05:53Z","snapshot_observed_at":"2026-08-08T07:12:11.066661Z","submitted_at":"2026-07-07T13:05:53Z","title":"Schwarzschild black holes from twistor space","version":1},"cited_work":{"arxiv_id":"2607.06236","doi":null,"metadata_source":"pith","pith_arxiv_id":"2607.06236","snapshot_observed_at":"2026-08-11T04:18:40.956165Z","title":"Schwarzschild black holes from twistor space","venue":"hep-th","work_id":"cc809f61-c073-4d99-8ec8-c119bcee81c1","year":2026},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.682592Z"},"links":{"cited_paper":"/paper/2607.06236","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:09556ccb580bd2052c274953dae6ac12f72ca8eac95978432dd5b35b90b6a019","observation_id":"ca998d2f-74a9-403c-a0d9-8adc6387c261","resolution":{"observed_at":"2026-08-11T04:18:40.997173Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.09451","last_updated":"2023-09-02T13:12:51Z","snapshot_observed_at":"2026-08-09T16:44:37.105742Z","submitted_at":"2023-05-16T14:13:46Z","title":"The Celestial Chiral Algebra of Self-Dual Gravity on Eguchi-Hanson Space","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.09451","snapshot_observed_at":"2026-08-11T04:18:39.702968Z","title":"The celestial chiral algebra of self-dual gravity on Eguchi-Hanson space,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.702968Z"},"links":{"cited_paper":"/paper/2305.09451","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:c83bbac1b5f1d284c2ac42f5834f81ffae80646629454c47141eefa54f5d073f","observation_id":"18b7ed8d-90dc-4c44-bb27-29d051d2ad6a","resolution":{"observed_at":"2026-08-11T04:18:39.702968Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.719600Z","title":"The geometry of complex self-dual Einstein spaces,","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.719600Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:b0dc5596ec19dbcf6c5c2c595287508a961ef17a2fda9f884598deb9e58803bc","observation_id":"2c2a254b-0975-4f07-a6e8-54c4a02f0928","resolution":{"observed_at":"2026-08-11T04:18:39.719600Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.730093Z","title":"The geometry of W-gravity,","venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.730093Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:22f1d4d0eda374a0f4d921e5b5be4114b3d0fddf42312c7656e3fac934a779b3","observation_id":"5d564958-717a-4751-b013-e8803acdd6f1","resolution":{"observed_at":"2026-08-11T04:18:39.730093Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.739182Z","title":"Canonical structures on anti-self-dual four-manifolds and the diffeomorphism group,","venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.739182Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:b3a082859b13f722af73c4a350910ae951b84370be74fa5533c7c72302b8f665","observation_id":"80e96101-26f6-4856-ba8c-c038be03ef5a","resolution":{"observed_at":"2026-08-11T04:18:39.739182Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.747946Z","title":"Self-dual gravity via Hitchin’s equations,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.747946Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:49919b50f2ae966fde5aab8128a2048627d2ba7a25bc7005f8e76210771dcf38","observation_id":"0c383c5b-ada5-473b-b353-05a731b3b8eb","resolution":{"observed_at":"2026-08-11T04:18:39.747946Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.758205Z","title":"A construction of hyper-K¨ ahler metrics,","venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.758205Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:51fa4ee220aec81e4540b4c9b576c8f17e3bb4845171732928c1ea0c57b8fb92","observation_id":"d64008f7-b222-4207-9df5-0ae2af204279","resolution":{"observed_at":"2026-08-11T04:18:39.758205Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1105.2565","last_updated":"2011-07-26T16:06:15Z","snapshot_observed_at":"2026-07-06T02:27:40.449397Z","submitted_at":"2011-05-12T20:00:42Z","title":"The Kinematic Algebra From the Self-Dual Sector","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1105.2565","snapshot_observed_at":"2026-08-11T04:18:39.766788Z","title":"The kinematic algebra from the self-dual sector,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.766788Z"},"links":{"cited_paper":"/paper/1105.2565","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:3b819c04e33901c2141fbe56cf696a55990a8d2dfe5fac91489297141cc9a9a4","observation_id":"dea47a5d-5038-44d8-b08b-b278ae2c0cfb","resolution":{"observed_at":"2026-08-11T04:18:39.766788Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.774602Z","title":"The Moyal deformation of the 2 nd heavenly equation,","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.774602Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:3bf4175d9ba364fed66c30b0ee36ee775e4269fbcca47acc15ca9a6e164e405e","observation_id":"21cd9c08-5370-4018-bc0e-9904731dacab","resolution":{"observed_at":"2026-08-11T04:18:39.774602Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.778341Z","title":"From principal chiral model to self-dual gravity,","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.778341Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:a65d3ecac84783462cef60d916b795b8c4c6645dffc06b3a8271ac5d01ca1389","observation_id":"cf7bec76-bd48-4764-8e8f-38415ad578c2","resolution":{"observed_at":"2026-08-11T04:18:39.778341Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.782887Z","title":"The Lagrangian of a self-dual gravitational field as a limit of the SDYM Lagrangian,","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.782887Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:fcd44f72b1d3f3e504bdee6e9a44374391b4b808a713185c1530c261461d5a27","observation_id":"21424021-475c-4763-8a8d-5b08321c817e","resolution":{"observed_at":"2026-08-11T04:18:39.782887Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9905078","last_updated":"1999-05-20T15:29:31Z","snapshot_observed_at":"2026-07-07T03:30:28.049014Z","submitted_at":"1999-05-20T15:29:31Z","title":"Nonlinear Graviton as a Limit of sl(N;C) Chiral Fields as N--> infty","version":1},"cited_work":{"arxiv_id":"gr-qc/9905078","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/9905078","snapshot_observed_at":"2026-08-11T04:18:40.805008Z","title":"Nonlinear Graviton as a Limit of sl(N;C) Chiral Fields as N--> infty","venue":"gr-qc","work_id":"43c0a886-f5e0-48f6-8171-e719e6bddf04","year":1999},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.787803Z"},"links":{"cited_paper":"/paper/gr-qc/9905078","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:7e69c22214ae0c8410b5b257ae33d5993fa5ddef729d05ffd5d764791c0774eb","observation_id":"c2e0a8b0-7d5d-40ae-b615-6d408974e56a","resolution":{"observed_at":"2026-08-11T04:18:40.850380Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.791279Z","title":"Self-dual gravity as a large-nlimit of the 2d non-linear sigma model,","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.791279Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:4daf774e3d3f0f2e4c1f4e9d9117ba720d379a7697d421db67634e0d0f97e69d","observation_id":"08543a6a-f13a-4c85-90dc-b4f2044ef322","resolution":{"observed_at":"2026-08-11T04:18:39.791279Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.794189Z","title":"SU(inf ty) (super) gauge theories and self-dual (super) gravity,","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.794189Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:f938e77c96fa5d65a00d1f3bc4cf40b21e6b12d82d11b275bf0598ece36bed7f","observation_id":"d747ba13-917b-4079-8fcd-653ec5260c81","resolution":{"observed_at":"2026-08-11T04:18:39.794189Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.797514Z","title":"Hidden symmetry of the galileon,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.797514Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:feb3b0c4a766f084018ce92394f6aaeb491d3da8fe741c43989d75f5d2c598f9","observation_id":"d6bec57a-1996-4127-acce-4d37e8c309a5","resolution":{"observed_at":"2026-08-11T04:18:39.797514Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.801137Z","title":"On integrability properties of SU(2) Yang–Mills fields. I. Infinitesimal part,","venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.801137Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:1bf93232d7990c02f7b7a93d72e153199e546427cd47a22716193af5c1caef79","observation_id":"e44945a5-fdaf-435e-a4ee-cbeeb9ddf146","resolution":{"observed_at":"2026-08-11T04:18:39.801137Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.804674Z","title":"A new characterization of half-flat solutions to einstein’s equation,","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.804674Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:afaca480531267df855b716edebed64086c53459494d3a2d2b76e650fa1bf061","observation_id":"c65cdb97-9c50-4c52-990e-4ea12d69509f","resolution":{"observed_at":"2026-08-11T04:18:39.804674Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.808022Z","title":"Selfduality in four-dimensional Riemannian geometry,","venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.808022Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:e630be5af667007b20b839a574ec13e4c41ebe7b3472b333e48e6e7463aeab94","observation_id":"f8bf5659-55f1-4f99-b817-811bdefa84ee","resolution":{"observed_at":"2026-08-11T04:18:39.808022Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.811638Z","title":"An example of anH-space,","venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.811638Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:e1d7ac4db2903be7261e2c8c029caf507074a0e727679b44d0d717f55958cd22","observation_id":"affe776a-ae67-43cf-9316-9216faafadf4","resolution":{"observed_at":"2026-08-11T04:18:39.811638Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.784334Z","title":"The non-linear graviton representing the analogue of Schwarzschild or Kerr black holes,","venue":null,"work_id":"ec8fda79-c541-4ff8-9634-f90bad5dd71b","year":1976},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.815180Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:ffcf080cbb8d851f95803fde30e051e09cfa0e3dd1c85ace2b531a1de1d05dff","observation_id":"71bc609f-30b6-4355-a235-e8fe1e5d3aec","resolution":{"observed_at":"2026-08-11T04:18:42.788779Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.771803Z","title":"An asymptotically flatH-space,","venue":null,"work_id":"1c23f3b4-eb4b-4a3b-bc28-f3c05462f445","year":1981},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.818673Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:9d5ca0b7f6094582cb205ed06b691ae17719b5b0b0419a89cc9128f43ce3c20e","observation_id":"975a2ae5-3bb1-4e98-a878-d72bf7726e52","resolution":{"observed_at":"2026-08-11T04:18:42.775576Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.758517Z","title":"Equivalence of Eguchi-Hanson metric to two-center Gibbons-Hawking metric,","venue":null,"work_id":"370802ed-8092-45a5-866e-6b29a3540095","year":1979},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.821995Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:4c9964088a8af25bd396abbbf6b313284fc707431a59797750777aac225c75ef","observation_id":"8c5b5549-4b75-4fdc-9030-806a6678d4c8","resolution":{"observed_at":"2026-08-11T04:18:42.762640Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0703030","last_updated":"2007-03-04T18:32:42Z","snapshot_observed_at":"2026-08-08T19:59:06.745131Z","submitted_at":"2007-03-04T18:32:42Z","title":"The Disjointed Thermodynamics of Rotating Black Holes With a NUT Twist","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0703030","snapshot_observed_at":"2026-08-11T04:18:39.825900Z","title":"The disjointed thermodynamics of rotating black holes with a NUT twist,","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.825900Z"},"links":{"cited_paper":"/paper/hep-th/0703030","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:bb54ce56492e795b46fe93c802028722673141a3c40c9214d0936c3266d7c65e","observation_id":"900afddd-bbb1-4fb2-83d5-359eb3e67968","resolution":{"observed_at":"2026-08-11T04:18:39.825900Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.745242Z","title":"The flatter regions of Newman, Unti, and tamburino’s generalized Schwarzschild space,","venue":null,"work_id":"e64967f8-0367-473f-8c71-ce2a6c83dd10","year":1963},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.830113Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:d14075f52cee835b0bc34ebe6028f438a4805d8dc94f7c44a5550c0c46c74ac0","observation_id":"f0a95f23-9201-443b-912e-6ebb19c2beb8","resolution":{"observed_at":"2026-08-11T04:18:42.750278Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.833673Z","title":"A new interpretation of the NUT metric in general relativity,","venue":null,"work_id":null,"year":1969},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.833673Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:53455704968cda4ee04d9688a8b855524ebfa9b2f0b41046d964dea7bec4a289","observation_id":"d8838364-b1e8-420e-bc68-4ab7559a6fb8","resolution":{"observed_at":"2026-08-11T04:18:39.833673Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.724313Z","title":"Physical interpretation of NUT metric,","venue":null,"work_id":"b0ef0dd4-08a4-4279-a421-ee3df1cd2925","year":1971},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.837062Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:ec99417e1a08dc8b8dd30aed9af4a53d7c8abff00e68fb9af3ed87d241f9bbee","observation_id":"9bdd501b-1ce3-4539-aebf-b718fa714dac","resolution":{"observed_at":"2026-08-11T04:18:42.728730Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.644767Z","title":"Spinning cosmic strings and quantization of energy,","venue":null,"work_id":"94c4474e-4e5d-407c-bfba-e2675fab0e92","year":1986},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.840608Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:df9fcf3fcd4f55e233922fa3f81699fb131ec080abcecec12b4dffa6bac74643","observation_id":"fe309877-2d9b-43f5-a7d6-c2a2f30a6862","resolution":{"observed_at":"2026-08-11T04:18:42.692765Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.602311Z","title":null,"venue":null,"work_id":"a2da9217-7add-4a77-8289-686c86bc02ab","year":2009},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.843590Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:873e23548993f6ef01283a9a1b491269a7e5b942b32b947f00bc9a5e8e4da200","observation_id":"bf8d0765-323e-4cf6-88b1-2cbcc24b43bd","resolution":{"observed_at":"2026-08-11T04:18:42.605931Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.846771Z","title":"A combined Kerr-NUT solution of the Einstein field equations,","venue":null,"work_id":null,"year":1966},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.846771Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:a64ad3ad97c0caead2e4efacc785d7155f6bc1a2eca8b28adca1dbbaadb07eaa","observation_id":"78e70d70-b6c9-4cb2-9aee-f568e47d259b","resolution":{"observed_at":"2026-08-11T04:18:39.846771Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:39.850407Z","title":"The NUT solution as a gravitational dyon,","venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.850407Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:f23fcc5e019d0ae72bc657730f434ad222a5b2842bbf0d07587570e11d6ebce0","observation_id":"ac775699-5564-4a55-b52b-988adc1c2d71","resolution":{"observed_at":"2026-08-11T04:18:39.850407Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.573284Z","title":"The gravitational analogues of magnetic monopoles,","venue":null,"work_id":"4b01ebed-a298-424e-acfa-8352e7a141da","year":1967},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.853453Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:4ac03b2fd306f58f414ee8e17a13b4137bc462b88388f5e6debad732493a9258","observation_id":"6e9683eb-89d0-430b-beac-79f08091ec0c","resolution":{"observed_at":"2026-08-11T04:18:42.577489Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.559955Z","title":"Dual-mass in general relativity,","venue":null,"work_id":"139bc2e6-2a55-4a51-8d5d-a0aceeb56261","year":1981},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.870855Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:b59898376da85d2763f54d55ea44e594889bb57bde74d9274c3c5fbd2cfd6a33","observation_id":"85fa0f70-9eae-491a-98a9-b5336ec83147","resolution":{"observed_at":"2026-08-11T04:18:42.564279Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.547274Z","title":"A gravitational analog of the Dirac monopole,","venue":null,"work_id":"dea66083-ca25-45c3-8fcd-ab3c973d7b3e","year":1986},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.896866Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:1b4536bdc5969e2041181c83d5855a18b5ad53b913b095cca39f4541c8a91d24","observation_id":"ca79b446-e1cf-494d-86c5-680c22702a24","resolution":{"observed_at":"2026-08-11T04:18:42.551195Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.430221Z","title":null,"venue":null,"work_id":"8f6d17a9-2c1d-40e6-9b3d-c0d28073f343","year":2009},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.930303Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:b518c1f648e06b3bcbef1b62c7e14760d09edce0a469b8dd608a8b5c1c896e1d","observation_id":"e62624cc-fa20-4df6-887c-a4c58a35ad97","resolution":{"observed_at":"2026-08-11T04:18:42.493908Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.412844Z","title":"L’ether lumineux demontre par l’effet du vent relatif d’ether dans un interferometre en rotation uniforme,","venue":null,"work_id":"2ecaeeee-5a54-4b80-b1f5-5069c94f5497","year":1913},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.949900Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:f5bcb1bb549ee840ecab832249219b169401b8a69a7655e34d0d9d3ac086f34e","observation_id":"673927df-b783-4f71-98fa-1a37f4279d6e","resolution":{"observed_at":"2026-08-11T04:18:42.417107Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.399881Z","title":"Sur la preuve de la realite de l’ether lumineux par l’experience de l’interferographe tournant,","venue":null,"work_id":"09b8f243-1952-4b34-ad22-cba5b34d7219","year":1913},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.976766Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:fbf7daff7a87447bbc0ef2eb51a97fde6a7f5837bfcc21208ef0299be4885e8a","observation_id":"430187b1-291a-45b3-a9f1-4e437774518e","resolution":{"observed_at":"2026-08-11T04:18:42.404169Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.387306Z","title":"The Sagnac effect in general relativity,","venue":null,"work_id":"db0ad7fb-e268-4b3c-8165-21e41d1fb1fe","year":1975},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.980867Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:ba5a9e5e75c1e894b9a39ea2f93cd9c336dbd6b4639af5b6bd1e422d0e8b0946","observation_id":"dba93d0d-53a8-4d98-bdc1-cc1831f59e45","resolution":{"observed_at":"2026-08-11T04:18:42.391654Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.373409Z","title":"Comments on quantum-mechanical interference due to the earth’s rotation,","venue":null,"work_id":"b6373738-ca5b-46ae-affa-20d6b582b3b4","year":1980},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.984557Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:568f2df197e7b9bec81a2d5918552806caee63d243e10e3c6fa44e360de885a5","observation_id":"786c5dd4-eb8b-4ecb-8ccb-a0921a2286e0","resolution":{"observed_at":"2026-08-11T04:18:42.377952Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.340327Z","title":"Sagnac effect in relativistic and nonrelativistic physics,","venue":null,"work_id":"4bf08a37-d6b3-4e06-87e3-26a0d533f037","year":1981},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.988730Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:2f0fc0468643ae123fa072eb510189ba4edf69c70ce62c8e6fc01dda4d788406","observation_id":"4b5ac1cb-e361-42e1-b90d-e0dacb75233f","resolution":{"observed_at":"2026-08-11T04:18:42.364284Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.08756","last_updated":"2023-05-15T16:10:35Z","snapshot_observed_at":"2026-08-02T20:42:08.004020Z","submitted_at":"2023-05-15T16:10:35Z","title":"Complex conformal transformations and zero-rest-mass fields","version":1},"cited_work":{"arxiv_id":"2305.08756","doi":null,"metadata_source":"pith","pith_arxiv_id":"2305.08756","snapshot_observed_at":"2026-08-11T04:18:40.777613Z","title":"Complex conformal transformations and zero-rest-mass fields","venue":"gr-qc","work_id":"7747af7a-ad2e-4e2e-b2e2-cd538fd8d080","year":2023},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.992479Z"},"links":{"cited_paper":"/paper/2305.08756","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:b5aa55cf3702ffaa3e659a614b000da5bcd1e412650172713bd4f40fe0803b7a","observation_id":"b6f4ec57-14c9-4302-a020-781d0517abaa","resolution":{"observed_at":"2026-08-11T04:18:40.781391Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.241355Z","title":"Taylor’s theorem in the tensor calculus,","venue":null,"work_id":"442aec64-755c-4d76-bc05-8de19532a2b0","year":1931},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:39.996493Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:b029984a3b563a2a0f19130c70a1fd7fdb562f28bc8fad9b25245b795abd4d9a","observation_id":"bf35b4d7-8f36-4d87-a0aa-ccb7d6670ede","resolution":{"observed_at":"2026-08-11T04:18:42.287182Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.150624Z","title":"A characteristic function in Riemannian space and its application to the solution of geodesic triangles,","venue":null,"work_id":"ef76db58-a49a-456b-b646-453dedac057f","year":1931},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:40.002076Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:fc1ee086cdcf25a9f527109a8468714ef68f8af3abe4e5cbddad68c891b17708","observation_id":"01e6b4d8-9ba3-41e3-9b9a-7552d756dfe9","resolution":{"observed_at":"2026-08-11T04:18:42.193792Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1102.0529","last_updated":"2011-09-26T00:05:55Z","snapshot_observed_at":"2026-08-03T19:46:14.740088Z","submitted_at":"2011-02-02T18:40:22Z","title":"The motion of point particles in curved spacetime","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1102.0529","snapshot_observed_at":"2026-08-11T04:18:40.005845Z","title":"The motion of point particles in curved spacetime,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:40.005845Z"},"links":{"cited_paper":"/paper/1102.0529","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:52896479a153d164b36ad3bce5a679b7776a4cb87f7eaff6c0d0f0efd955e9d1","observation_id":"7aa3eab6-1421-4127-afd0-16e8f7636759","resolution":{"observed_at":"2026-08-11T04:18:40.005845Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.137914Z","title":"Green’s Functions for Gravitational Multi-Instantons,","venue":null,"work_id":"48560b2f-40b1-4d5c-9e09-4aa4495b50e1","year":1979},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:40.009384Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:e3cf29890519611c3b72ddbea9eb7dd35f4d64a0f3d9cd66cf5c042864bf32cd","observation_id":"ca396c87-3432-4a38-9094-52282d76c470","resolution":{"observed_at":"2026-08-11T04:18:42.142747Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.09165","last_updated":"2024-06-13T14:27:40Z","snapshot_observed_at":"2026-08-11T13:52:35.216603Z","submitted_at":"2024-06-13T14:27:40Z","title":"Gluon scattering on the self-dual dyon","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.09165","snapshot_observed_at":"2026-08-11T04:18:40.012572Z","title":"Gluon scattering on the self-dual dyon,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:40.012572Z"},"links":{"cited_paper":"/paper/2406.09165","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:a48f53faa7418933746c6ac62585a37e0e8d7ea6e1d81a5847cc5ea3a1681d8e","observation_id":"8a05698e-123a-49fc-8e93-6a12925425b7","resolution":{"observed_at":"2026-08-11T04:18:40.012572Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.01888","last_updated":"2025-06-02T17:15:31Z","snapshot_observed_at":"2026-08-07T21:53:40.440539Z","submitted_at":"2025-06-02T17:15:31Z","title":"S-algebra in Gauge Theory: Twistor, Spacetime and Holographic Perspectives","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.01888","snapshot_observed_at":"2026-08-11T04:18:40.015915Z","title":"S-algebra in gauge theory: twistor, spacetime and holographic perspectives,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:40.015915Z"},"links":{"cited_paper":"/paper/2506.01888","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:b9bf4b9f63ed0e5324d17a25606acc85bed2f395f71b975552425326d057691e","observation_id":"35c76994-95f6-47f5-bd92-cda32fa83771","resolution":{"observed_at":"2026-08-11T04:18:40.015915Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.125422Z","title":"Solutions of the zero-rest-mass equations,","venue":null,"work_id":"fbf0955e-6160-4aef-882c-a884cd64d16d","year":1969},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:40.019380Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:d3505efabfcbab0253e8b8120ee6635935fa52057fa1c65f24e68a8e50276387","observation_id":"cdbd530c-21f8-42c5-bc15-e52a0608de83","resolution":{"observed_at":"2026-08-11T04:18:42.129559Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:40.022902Z","title":"Note on the Kerr spinning particle metric,","venue":null,"work_id":null,"year":1965},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:40.022902Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:147296c406b88793e125e4705503ed9893537c39f02cbaa348262536d8f28dbf","observation_id":"4bab5766-4005-45b1-865f-78719badf262","resolution":{"observed_at":"2026-08-11T04:18:40.022902Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.16441","last_updated":"2021-03-30T15:38:51Z","snapshot_observed_at":"2026-08-11T18:56:52.849819Z","submitted_at":"2021-03-30T15:38:51Z","title":"The Weyl double copy from twistor space","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.16441","snapshot_observed_at":"2026-08-11T04:18:40.026585Z","title":"The Weyl double copy from twistor space,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:40.026585Z"},"links":{"cited_paper":"/paper/2103.16441","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:ff051bf4c5f3a01cabe54d6e50660f299624cff98717cb2cf88a0d56f9a7e915","observation_id":"f59b6b7e-8003-4936-9107-a49ddbf56485","resolution":{"observed_at":"2026-08-11T04:18:40.026585Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.02479","last_updated":"2020-12-04T09:15:48Z","snapshot_observed_at":"2026-08-10T03:40:30.845186Z","submitted_at":"2020-12-04T09:15:48Z","title":"A Twistorial Foundation for the Classical Double Copy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.02479","snapshot_observed_at":"2026-08-11T04:18:40.030339Z","title":"Twistorial Foundation for the Classical Double Copy,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:40.030339Z"},"links":{"cited_paper":"/paper/2012.02479","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:7329251d1bac30c4c4d7e60e4a73f673c9ee61f1152f1d9fad8ef734e4d264a8","observation_id":"2f4dc154-c55d-40e9-a3c1-0d487c6a8279","resolution":{"observed_at":"2026-08-11T04:18:40.030339Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.05111","last_updated":"2021-12-09T18:47:54Z","snapshot_observed_at":"2026-07-06T12:17:07.084920Z","submitted_at":"2021-12-09T18:47:54Z","title":"Reconstructing Classical Spacetimes from the S-Matrix in Twistor Space","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.05111","snapshot_observed_at":"2026-08-11T04:18:40.033714Z","title":"Reconstructing classical spacetimes from the S-Matrix in twistor space,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:40.033714Z"},"links":{"cited_paper":"/paper/2112.05111","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:b3e6b70408e911d510ec2fb19e443ed09cc4f4d4b0977c0f56f4c1b815a8299d","observation_id":"e012b939-df89-487d-a7be-1302a97580b2","resolution":{"observed_at":"2026-08-11T04:18:40.033714Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.10491","last_updated":"2022-12-20T18:06:31Z","snapshot_observed_at":"2026-08-07T21:07:55.604073Z","submitted_at":"2022-12-20T18:06:31Z","title":"Twistor quadrics and black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.10491","snapshot_observed_at":"2026-08-11T04:18:40.037531Z","title":"Twistor quadrics and black holes,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:40.037531Z"},"links":{"cited_paper":"/paper/2212.10491","citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:525e4f429f22c56015f55352bd9ac9797df86a05992fbcf7f7ad9140e4d38deb","observation_id":"56ac6001-e2f8-469e-9625-84458a1c35f2","resolution":{"observed_at":"2026-08-11T04:18:40.037531Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.104999Z","title":"The theory of gravitation,","venue":null,"work_id":"dfe8bf8d-5a83-4b21-9dde-617d5da79d13","year":1917},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:40.104169Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:c098335037df650a256b482dc35ff5b723e03b293521197c43f44eeb42b78678","observation_id":"ee2cd4d6-c453-41f7-b370-a349395ebd2b","resolution":{"observed_at":"2026-08-11T04:18:42.109349Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:42.068339Z","title":"Uniformly accelerating charged mass in general relativity,","venue":null,"work_id":"11696b70-1c80-4270-ad18-55780309e932","year":1970},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:40.176029Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:bc7f159f953a239d1bae1c04dbb7af4fb56f14a710f4f3696572a6ccfaa235a6","observation_id":"060075d2-4c7a-4a9b-af11-465b5e55c89b","resolution":{"observed_at":"2026-08-11T04:18:42.096078Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:41.909449Z","title":"Linear superposition of two type-N nonlinear gravitons,","venue":null,"work_id":"0cfff1b2-dcca-4c12-8c60-ffb531a9f648","year":1998},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:40.235660Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:a58f4074d86fcd371ba6048de5014cc8bc68640591a26e9deabe8dc429c12732","observation_id":"cffc3042-cfab-4689-8c6a-ae953b020bab","resolution":{"observed_at":"2026-08-11T04:18:41.984614Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:41.897634Z","title":"Extending half-flat metrics,","venue":null,"work_id":"0c11ddfb-5444-49d1-bbbb-5f314698aaea","year":1998},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:40.318656Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:7128d8bb2ad5aa27852db4fb141af7df58ddeda7d1784560ea47b4e879f7ce9b","observation_id":"5ef69da7-c99b-4704-a1e6-94f35494f220","resolution":{"observed_at":"2026-08-11T04:18:41.901513Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:41.885274Z","title":"Some real and complex solutions of Einstein’s equations,","venue":null,"work_id":"ae59a3d3-1b19-469a-8093-def42b496777","year":1987},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:40.322692Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:459cbc427cd192aaf7a0b97c1ef3a84df8a02037903219e767c5428f4a09efe1","observation_id":"f1f69d22-05d7-4cd2-b080-8ca82d8ab86c","resolution":{"observed_at":"2026-08-11T04:18:41.889633Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:41.872671Z","title":"Magnetic monopoles in Kaluza-Klein theories,","venue":null,"work_id":"597986db-8306-4995-b322-7002356d3e22","year":1983},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:40.326764Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:a397889af1f48b6e6d7813cfcf45a43e1921e1fc56eea489985a35f69f37fb55","observation_id":"ec80188c-0dc4-43f1-80fc-929398ad6a9d","resolution":{"observed_at":"2026-08-11T04:18:41.877060Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:18:41.859114Z","title":"Penrose and W","venue":null,"work_id":"13a35064-05a0-46cd-8473-405929093043","year":1988},"citing_paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-11T04:18:40.330925Z"},"links":{"citing_paper":"/paper/2608.07774"},"observation_digest":"sha256:d1659a2f13e0448534f6b3658da48f9fc3c01f531713f50caa291c7a476cf096","observation_id":"d0e44337-d880-42b4-b4b9-312b9ccc064f","resolution":{"observed_at":"2026-08-11T04:18:41.863718Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2608.07774","last_updated":"2026-08-07T21:45:16Z","latest_version":1,"primary_category":"hep-th","snapshot_observed_at":"2026-08-11T20:13:16.480510Z","submitted_at":"2026-08-07T21:45:16Z","title":"Incidence Relations for Self-Dual Black Holes"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":69,"verified_exact":6,"verified_fuzzy":25},"total_outbound_references":116},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 100 of 116 outbound references and 0 inbound Pith citation observations for arXiv:2608.07774."}