{"as_of":"2026-08-20T14:04:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:59bcfbd793816410b0a7cd7b206b2fa21ed2855d542d72fca78e02b2beddecc0","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":"2026-08-07T15:00:31.912837Z","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":"2026-05-23T00:45:15.359724Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2304.12750","last_updated":"2023-10-10T08:47:57Z","snapshot_observed_at":"2026-08-16T15:37:53.207318Z","submitted_at":"2023-04-25T11:58:45Z","title":"Black hole hairs in scalar-tensor gravity and the lack thereof","version":3},"cited_work":{"arxiv_id":"2304.12750","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2304.12750","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Black hole hairs in scalar-tensor gravity and the lack thereof","venue":null,"work_id":"dcae2c64-1137-4952-b4db-9e8779b856ae","year":2023},"citing_paper":{"arxiv_id":"2503.05651","last_updated":"2026-04-29T13:21:43Z","snapshot_observed_at":"2026-07-06T20:48:41.069542Z","submitted_at":"2025-03-07T18:15:05Z","title":"Inverting no-hair theorems: How requiring General Relativity solutions restricts scalar-tensor theories","version":3},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-05-23T00:45:03.453709Z"},"links":{"cited_paper":"/paper/2304.12750","citing_paper":"/paper/2503.05651"},"observation_digest":"sha256:52652f8f7412156f56c144e82e7c595ee4868611e45195adbda59398fc6b2cf6","observation_id":"c21d76bb-0fa5-4cb9-a8d0-bf4f93f98732","resolution":{"observed_at":"2026-05-23T00:45:15.362519Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2304.12750","last_updated":"2023-10-10T08:47:57Z","snapshot_observed_at":"2026-08-16T15:37:53.207318Z","submitted_at":"2023-04-25T11:58:45Z","title":"Black hole hairs in scalar-tensor gravity and the lack thereof","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.12750","snapshot_observed_at":"2026-08-07T15:00:31.912837Z","title":"Black hole hairs in scalar-tensor gravity and the lack thereof,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.16883","last_updated":"2025-05-29T16:46:47Z","snapshot_observed_at":"2026-08-09T17:55:07.702089Z","submitted_at":"2025-05-22T16:36:53Z","title":"Test-Field vs Physical Quasi-Normal Modes in Scalar-Tensor Theories","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-07T15:00:31.912837Z"},"links":{"cited_paper":"/paper/2304.12750","citing_paper":"/paper/2505.16883"},"observation_digest":"sha256:cc0abfd53a53bb0ace9b066024261a894c865e0955e0a60551a523063bc077d5","observation_id":"0a42f095-83c4-4627-84c2-1096fc4a3f16","resolution":{"observed_at":"2026-08-07T15:00:31.912837Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.12750","last_updated":"2023-10-10T08:47:57Z","snapshot_observed_at":"2026-08-16T15:37:53.207318Z","submitted_at":"2023-04-25T11:58:45Z","title":"Black hole hairs in scalar-tensor gravity and the lack thereof","version":3},"cited_work":{"arxiv_id":"2304.12750","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2304.12750","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Black hole hairs in scalar-tensor gravity and the lack thereof","venue":null,"work_id":"dcae2c64-1137-4952-b4db-9e8779b856ae","year":2023},"citing_paper":{"arxiv_id":"2603.22398","last_updated":"2026-04-29T08:33:52Z","snapshot_observed_at":"2026-08-15T22:22:56.621518Z","submitted_at":"2026-03-23T18:00:11Z","title":"Stable black hole solutions with cosmological hair","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-15T00:33:06.549204Z"},"links":{"cited_paper":"/paper/2304.12750","citing_paper":"/paper/2603.22398"},"observation_digest":"sha256:6b06eec644d36a9bb99689fed2ae6dcdac80f6b93b121582e6c59f298a47e27b","observation_id":"3eda5d1a-7e85-4db5-bc9d-0dfd87d28711","resolution":{"observed_at":"2026-05-15T00:33:23.169383Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2304.12750","last_updated":"2023-10-10T08:47:57Z","snapshot_observed_at":"2026-08-16T15:37:53.207318Z","submitted_at":"2023-04-25T11:58:45Z","title":"Black hole hairs in scalar-tensor gravity and the lack thereof","version":3},"cited_work":{"arxiv_id":"2304.12750","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2304.12750","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Black hole hairs in scalar-tensor gravity and the lack thereof","venue":null,"work_id":"dcae2c64-1137-4952-b4db-9e8779b856ae","year":2023},"citing_paper":{"arxiv_id":"2605.00580","last_updated":"2026-05-01T11:29:25Z","snapshot_observed_at":"2026-08-16T10:47:51.623808Z","submitted_at":"2026-05-01T11:29:25Z","title":"Scalar emission from binary neutron stars in scalar-tensor theories with kinetic screening","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-05-09T19:11:57.124699Z"},"links":{"cited_paper":"/paper/2304.12750","citing_paper":"/paper/2605.00580"},"observation_digest":"sha256:4dee2cda594935a0f9fa3247e8155ecb26c10865e93ec13cdf8a14b21324b54d","observation_id":"2569e991-2b50-481a-b306-918b00d2178e","resolution":{"observed_at":"2026-05-11T15:47:20.956586Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2304.12750","last_updated":"2023-10-10T08:47:57Z","snapshot_observed_at":"2026-08-16T15:37:53.207318Z","submitted_at":"2023-04-25T11:58:45Z","title":"Black hole hairs in scalar-tensor gravity and the lack thereof","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.12750","snapshot_observed_at":"2026-07-31T21:09:26.152288Z","title":"Capuano, L","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.27991","last_updated":"2026-07-30T10:36:57Z","snapshot_observed_at":"2026-08-14T13:49:21.620291Z","submitted_at":"2026-07-30T10:36:57Z","title":"Towards long and accurate numerical relativity waveforms of binary black holes beyond general relativity","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-07-31T21:09:26.152288Z"},"links":{"cited_paper":"/paper/2304.12750","citing_paper":"/paper/2607.27991"},"observation_digest":"sha256:153c4bcd4e9ba657d582622f8ba9d0db3b793bc99ed15afe13b10bb7da955fe5","observation_id":"a266cc47-0e5f-4810-98d4-b36b119a864a","resolution":{"observed_at":"2026-07-31T21:09:26.152288Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.12750","last_updated":"2023-10-10T08:47:57Z","snapshot_observed_at":"2026-08-16T15:37:53.207318Z","submitted_at":"2023-04-25T11:58:45Z","title":"Black hole hairs in scalar-tensor gravity and the lack thereof","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.12750","snapshot_observed_at":"2026-07-31T20:45:37.813925Z","title":"Capuano, L","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.28003","last_updated":"2026-07-30T10:50:23Z","snapshot_observed_at":"2026-08-18T13:27:07.072276Z","submitted_at":"2026-07-30T10:50:23Z","title":"High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-07-31T20:45:37.813925Z"},"links":{"cited_paper":"/paper/2304.12750","citing_paper":"/paper/2607.28003"},"observation_digest":"sha256:6938af425d520a332adc6ddf230daf774abc06fd5c0cda8849e4c3cecaee6173","observation_id":"31f24bdb-e716-421d-87aa-1bc9aa34728a","resolution":{"observed_at":"2026-07-31T20:45:37.813925Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2304.12750/citation-record","integrity":"/paper/2304.12750/integrity","json":"/paper/2304.12750/citation-record.json","paper":"/paper/2304.12750"},"outbound":[],"paper":{"arxiv_id":"2304.12750","last_updated":"2023-10-10T08:47:57Z","latest_version":3,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-16T15:37:53.207318Z","submitted_at":"2023-04-25T11:58:45Z","title":"Black hole hairs in scalar-tensor gravity and the lack thereof"},"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 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2304.12750."}