{"as_of":"2026-08-13T06:44:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:170488ff18834b355fe98e5e6bcc1f07322f8403626d0fd7526071b05b0dcea3","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T19:44:17.400752Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-13T08:07:31.464258Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2311.12940","last_updated":"2024-07-08T12:35:13Z","snapshot_observed_at":"2026-08-13T05:20:11.220235Z","submitted_at":"2023-11-21T19:03:36Z","title":"Shock waves, black hole interiors and holographic RG flows","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.12940","snapshot_observed_at":"2026-08-11T19:44:17.400752Z","title":"Shock waves, black hole interiors and holographic RG flows,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06536","last_updated":"2024-12-09T14:43:35Z","snapshot_observed_at":"2026-08-12T09:11:38.439877Z","submitted_at":"2024-12-09T14:43:35Z","title":"More on thermal holographic RG flows in a 3D gauged supergravity","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-11T19:44:17.400752Z"},"links":{"cited_paper":"/paper/2311.12940","citing_paper":"/paper/2412.06536"},"observation_digest":"sha256:d2b853bbf3101168e0983883cfbdbf192e4547cc1b7da3659d5f227d01d00ade","observation_id":"bf22822e-a74c-4fd9-a234-eea418f7d4ed","resolution":{"observed_at":"2026-08-11T19:44:17.400752Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.12940","last_updated":"2024-07-08T12:35:13Z","snapshot_observed_at":"2026-08-13T05:20:11.220235Z","submitted_at":"2023-11-21T19:03:36Z","title":"Shock waves, black hole interiors and holographic RG flows","version":3},"cited_work":{"arxiv_id":"2311.12940","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2311.12940","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"C´ aceres, A.K","venue":null,"work_id":"0188a52c-65f1-4585-a19d-efdfecadbf6c","year":2024},"citing_paper":{"arxiv_id":"2604.21447","last_updated":"2026-05-12T10:39:22Z","snapshot_observed_at":"2026-08-08T04:42:03.601289Z","submitted_at":"2026-04-23T09:06:08Z","title":"$O(d,d)$ symmetric gravity and finite coupling holography","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-05-09T21:48:47.867176Z"},"links":{"cited_paper":"/paper/2311.12940","citing_paper":"/paper/2604.21447"},"observation_digest":"sha256:0fa1481d1b7e2d05bf6c3da68bb440d7c5f713c16604a6642eaf19a8c4cc45e9","observation_id":"bafc40d3-37e7-4640-9f97-a8d96dc22649","resolution":{"observed_at":"2026-05-11T14:26:04.232002Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.12940","last_updated":"2024-07-08T12:35:13Z","snapshot_observed_at":"2026-08-13T05:20:11.220235Z","submitted_at":"2023-11-21T19:03:36Z","title":"Shock waves, black hole interiors and holographic RG flows","version":3},"cited_work":{"arxiv_id":"2311.12940","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2311.12940","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"C´ aceres, A.K","venue":null,"work_id":"0188a52c-65f1-4585-a19d-efdfecadbf6c","year":2024},"citing_paper":{"arxiv_id":"2604.21447","last_updated":"2026-05-12T10:39:22Z","snapshot_observed_at":"2026-08-08T04:42:03.601289Z","submitted_at":"2026-04-23T09:06:08Z","title":"$O(d,d)$ symmetric gravity and finite coupling holography","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-05-13T08:03:43.077359Z"},"links":{"cited_paper":"/paper/2311.12940","citing_paper":"/paper/2604.21447"},"observation_digest":"sha256:19a047758cc2fedb2be5563cca08530446bb0fdbe4f2c79e7aaa5f730d661166","observation_id":"e7c7cae9-238a-4b3f-8e3a-c79292dc0578","resolution":{"observed_at":"2026-05-13T08:07:31.467286Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.12940","last_updated":"2024-07-08T12:35:13Z","snapshot_observed_at":"2026-08-13T05:20:11.220235Z","submitted_at":"2023-11-21T19:03:36Z","title":"Shock waves, black hole interiors and holographic RG flows","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.12940","snapshot_observed_at":"2026-08-02T02:48:57.666812Z","title":"C´ aceres, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.14284","last_updated":"2026-07-15T18:46:31Z","snapshot_observed_at":"2026-08-08T10:08:54.959174Z","submitted_at":"2026-07-15T18:46:31Z","title":"Non-Hermitian Holographic Flows to Little Rip Cosmologies","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-02T02:48:57.666812Z"},"links":{"cited_paper":"/paper/2311.12940","citing_paper":"/paper/2607.14284"},"observation_digest":"sha256:7390ed5af1f9f8c116030d3cb71e04341c679993ce7262f920cfc35339ea25ce","observation_id":"a1c2c088-572b-4187-a9f2-dab9019adad0","resolution":{"observed_at":"2026-08-02T02:48:57.666812Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2311.12940/citation-record","integrity":"/paper/2311.12940/integrity","json":"/paper/2311.12940/citation-record.json","paper":"/paper/2311.12940"},"outbound":[],"paper":{"arxiv_id":"2311.12940","last_updated":"2024-07-08T12:35:13Z","latest_version":3,"primary_category":"hep-th","snapshot_observed_at":"2026-08-13T05:20:11.220235Z","submitted_at":"2023-11-21T19:03:36Z","title":"Shock waves, black hole interiors and holographic RG flows"},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2311.12940."}