{"as_of":"2026-08-21T06:17:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d1228358c181df1f0c8c4ac4cf113cba3e3b902c8b0b658b0fbff3d88ad99e78","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-20T06:33:59.587034+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T11:29:11.212879Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-10T20:37:34.273339Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1412.1464","last_updated":"2014-12-03T20:46:33Z","snapshot_observed_at":"2026-08-14T23:09:04.252193Z","submitted_at":"2014-12-03T20:46:33Z","title":"Higher spin extension of cosmological spacetimes in 3D: asymptotically flat behaviour with chemical potentials and thermodynamics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.1464","snapshot_observed_at":"2026-08-14T11:29:11.212879Z","title":"Matulich, A","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.09150","last_updated":"2019-12-27T14:59:02Z","snapshot_observed_at":"2026-08-15T08:28:46.914991Z","submitted_at":"2019-08-24T15:15:14Z","title":"On the supersymmetric extension of asymptotic symmetries in three spacetime dimensions","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T11:29:11.212879Z"},"links":{"cited_paper":"/paper/1412.1464","citing_paper":"/paper/1908.09150"},"observation_digest":"sha256:fb3b3909da67dd3f06872e2fafb3737e4579be08b651e4b91776dc2fd4c12cf5","observation_id":"c074a16b-6cb6-4213-b8ad-0cd6a9a912f8","resolution":{"observed_at":"2026-08-14T11:29:11.212879Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.1464","last_updated":"2014-12-03T20:46:33Z","snapshot_observed_at":"2026-08-14T23:09:04.252193Z","submitted_at":"2014-12-03T20:46:33Z","title":"Higher spin extension of cosmological spacetimes in 3D: asymptotically flat behaviour with chemical potentials and thermodynamics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.1464","snapshot_observed_at":"2026-08-14T11:18:52.857241Z","title":"Matulich, A","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.09833","last_updated":"2019-08-26T18:00:01Z","snapshot_observed_at":"2026-08-18T01:22:57.120693Z","submitted_at":"2019-08-26T18:00:01Z","title":"Spacetime structure near generic horizons and soft hair","version":1},"reference_index":127,"source":"pdf_text","source_observed_at":"2026-08-14T11:18:52.857241Z"},"links":{"cited_paper":"/paper/1412.1464","citing_paper":"/paper/1908.09833"},"observation_digest":"sha256:de776e13bec579dc6b4e5c17c5fb06ed0c897b24e44fa5922328c8b445d48723","observation_id":"5fbce782-26d9-4b5c-98a6-5ae8a2863d10","resolution":{"observed_at":"2026-08-14T11:18:52.857241Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.1464","last_updated":"2014-12-03T20:46:33Z","snapshot_observed_at":"2026-08-14T23:09:04.252193Z","submitted_at":"2014-12-03T20:46:33Z","title":"Higher spin extension of cosmological spacetimes in 3D: asymptotically flat behaviour with chemical potentials and thermodynamics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.1464","snapshot_observed_at":"2026-08-11T21:12:59.293735Z","title":"Highe r spin extension of cosmological spacetimes in 3D: asymptotically ﬂat behaviour with chemic al potentials and thermodynamics,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.04992","last_updated":"2024-12-06T12:39:43Z","snapshot_observed_at":"2026-08-18T22:35:28.050572Z","submitted_at":"2024-12-06T12:39:43Z","title":"Asymptotic structure of three-dimensional Maxwell Chern-Simons gravity coupled to spin-3 fields","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-11T21:12:59.293735Z"},"links":{"cited_paper":"/paper/1412.1464","citing_paper":"/paper/2412.04992"},"observation_digest":"sha256:0c543c06b390c2de3ad61f43b35be18b809df40150393b438d21b28aabb8a250","observation_id":"ee113d39-ba3b-44eb-b872-d0b1b82940b5","resolution":{"observed_at":"2026-08-11T21:12:59.293735Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.1464","last_updated":"2014-12-03T20:46:33Z","snapshot_observed_at":"2026-08-14T23:09:04.252193Z","submitted_at":"2014-12-03T20:46:33Z","title":"Higher spin extension of cosmological spacetimes in 3D: asymptotically flat behaviour with chemical potentials and thermodynamics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.1464","snapshot_observed_at":"2026-08-10T22:56:45.408152Z","title":"Higher spin extension of cosmological spacetimes in 3D: asymptotically flat behaviour with chemical potentials and thermodynamics,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2501.00439","last_updated":"2025-04-17T08:31:01Z","snapshot_observed_at":"2026-08-17T03:23:16.322698Z","submitted_at":"2024-12-31T13:44:59Z","title":"Enhanced Conformal $BMS_3$ Symmetries","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-10T22:56:45.408152Z"},"links":{"cited_paper":"/paper/1412.1464","citing_paper":"/paper/2501.00439"},"observation_digest":"sha256:d181f6fcc5b58080832d4b789f4773c06450e2824194151b0585311939d219fe","observation_id":"a6de4044-3167-4675-8ff4-63862c88189b","resolution":{"observed_at":"2026-08-10T22:56:45.408152Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.1464","last_updated":"2014-12-03T20:46:33Z","snapshot_observed_at":"2026-08-14T23:09:04.252193Z","submitted_at":"2014-12-03T20:46:33Z","title":"Higher spin extension of cosmological spacetimes in 3D: asymptotically flat behaviour with chemical potentials and thermodynamics","version":1},"cited_work":{"arxiv_id":"1412.1464","doi":null,"metadata_source":"pith","pith_arxiv_id":"1412.1464","snapshot_observed_at":"2026-07-10T20:37:34.273339Z","title":"Higher spin extension of cosmological spacetimes in 3D: asymptotically flat behaviour with chemical potentials and thermodynamics","venue":"hep-th","work_id":"30d114c8-bc2c-4a59-9d3a-c7641bd02e73","year":2014},"citing_paper":{"arxiv_id":"2506.16164","last_updated":"2026-04-29T17:56:22Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-06-19T09:33:44Z","title":"The Carrollian Kaleidoscope","version":3},"reference_index":213,"source":"pdf_text","source_observed_at":"2026-05-19T09:20:26.218747Z"},"links":{"cited_paper":"/paper/1412.1464","citing_paper":"/paper/2506.16164"},"observation_digest":"sha256:704555e53e765391d3695106c580581a00d9121ab83269020cae24657258bd9b","observation_id":"e112750b-8796-4fed-97ec-2ead7cdbc605","resolution":{"observed_at":"2026-05-19T09:22:15.685023Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1412.1464","last_updated":"2014-12-03T20:46:33Z","snapshot_observed_at":"2026-08-14T23:09:04.252193Z","submitted_at":"2014-12-03T20:46:33Z","title":"Higher spin extension of cosmological spacetimes in 3D: asymptotically flat behaviour with chemical potentials and thermodynamics","version":1},"cited_work":{"arxiv_id":"1412.1464","doi":null,"metadata_source":"pith","pith_arxiv_id":"1412.1464","snapshot_observed_at":"2026-07-10T20:37:34.273339Z","title":"Higher spin extension of cosmological spacetimes in 3D: asymptotically flat behaviour with chemical potentials and thermodynamics","venue":"hep-th","work_id":"30d114c8-bc2c-4a59-9d3a-c7641bd02e73","year":2014},"citing_paper":{"arxiv_id":"2607.06826","last_updated":"2026-07-07T21:44:15Z","snapshot_observed_at":"2026-08-14T02:18:01.800834Z","submitted_at":"2026-07-07T21:44:15Z","title":"BMS$_3$ invariant field theories","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-07-10T20:31:35.714699Z"},"links":{"cited_paper":"/paper/1412.1464","citing_paper":"/paper/2607.06826"},"observation_digest":"sha256:b49b2bbf74efd99818ea5d64dc418fc8c5551e99e4704e3343d3d1f58762abd5","observation_id":"570bdda6-7125-49f1-b4b2-a937f46cfaeb","resolution":{"observed_at":"2026-07-10T20:37:34.275007Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1412.1464/citation-record","integrity":"/paper/1412.1464/integrity","json":"/paper/1412.1464/citation-record.json","paper":"/paper/1412.1464"},"outbound":[],"paper":{"arxiv_id":"1412.1464","last_updated":"2014-12-03T20:46:33Z","latest_version":1,"primary_category":"hep-th","snapshot_observed_at":"2026-08-14T23:09:04.252193Z","submitted_at":"2014-12-03T20:46:33Z","title":"Higher spin extension of cosmological spacetimes in 3D: asymptotically flat behaviour with chemical potentials and thermodynamics"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1412.1464."}