{"as_of":"2026-08-08T01:00:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9128f72791e847d7dd0e6b45fb699859571feae6c77238d2f3693bbdb569ae72","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T05:06:55.350988Z","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":"2026-06-30T14:34:46.225574Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2407.02460","last_updated":"2025-02-23T01:08:44Z","snapshot_observed_at":"2026-08-07T17:12:36.215426Z","submitted_at":"2024-07-02T17:37:34Z","title":"A new bump in the night: evidence of a new feature in the binary black hole mass distribution at $70~M_{\\odot}$ from gravitational-wave observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.02460","snapshot_observed_at":"2026-08-07T05:06:55.350988Z","title":"2014, ARA&A, 52, 415, doi: 10.1146/annurev-astro-081811-125615 Maga˜ na Hernandez, I., & Palmese, A","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2506.08801","last_updated":"2025-06-10T13:47:58Z","snapshot_observed_at":"2026-08-07T04:59:19.264135Z","submitted_at":"2025-06-10T13:47:58Z","title":"Using gravitational waves and multi-messenger Astronomy to reverse-engineer the properties of galactic nuclei","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-07T05:06:55.350988Z"},"links":{"cited_paper":"/paper/2407.02460","citing_paper":"/paper/2506.08801"},"observation_digest":"sha256:60bc206f599f2f259749f1852cd4cf7b69d4e6ba9d463a47c6d3cac887daf7b9","observation_id":"d48ee494-df45-4540-a866-5e2f7f9deaf4","resolution":{"observed_at":"2026-08-07T05:06:55.350988Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.02460","last_updated":"2025-02-23T01:08:44Z","snapshot_observed_at":"2026-08-07T17:12:36.215426Z","submitted_at":"2024-07-02T17:37:34Z","title":"A new bump in the night: evidence of a new feature in the binary black hole mass distribution at $70~M_{\\odot}$ from gravitational-wave observations","version":2},"cited_work":{"arxiv_id":"2407.02460","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.02460","snapshot_observed_at":"2026-06-30T14:34:46.225574Z","title":"Maga˜ na Hernandez and A","venue":null,"work_id":"187d371e-9cf8-4f26-a488-2ab9c4a9f7fd","year":2025},"citing_paper":{"arxiv_id":"2602.11282","last_updated":"2026-04-13T22:31:16Z","snapshot_observed_at":"2026-07-06T22:45:34.674215Z","submitted_at":"2026-02-11T19:00:22Z","title":"Measurement prospects for the pair-instability mass cutoff with gravitational waves","version":2},"reference_index":103,"source":"pdf_text","source_observed_at":"2026-05-16T05:35:56.364232Z"},"links":{"cited_paper":"/paper/2407.02460","citing_paper":"/paper/2602.11282"},"observation_digest":"sha256:d9e51eb4d8a6d5a22e7d26c26921a5b1ea9d79eff6e17603592fe2bd1dd383d3","observation_id":"b7068314-d82d-4c91-9f99-c7e5c3a1e91e","resolution":{"observed_at":"2026-05-16T05:37:23.696244Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.02460","last_updated":"2025-02-23T01:08:44Z","snapshot_observed_at":"2026-08-07T17:12:36.215426Z","submitted_at":"2024-07-02T17:37:34Z","title":"A new bump in the night: evidence of a new feature in the binary black hole mass distribution at $70~M_{\\odot}$ from gravitational-wave observations","version":2},"cited_work":{"arxiv_id":"2407.02460","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.02460","snapshot_observed_at":"2026-06-30T14:34:46.225574Z","title":"Maga˜ na Hernandez and A","venue":null,"work_id":"187d371e-9cf8-4f26-a488-2ab9c4a9f7fd","year":2025},"citing_paper":{"arxiv_id":"2604.14290","last_updated":"2026-04-15T18:00:03Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-15T18:00:03Z","title":"Emergent structure in the binary black hole mass distribution and implications for population-based cosmology","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-10T12:31:50.358428Z"},"links":{"cited_paper":"/paper/2407.02460","citing_paper":"/paper/2604.14290"},"observation_digest":"sha256:27549e82ac88bf307b4b7bb79cb8b727da399fb477442be679df1ec45059ae63","observation_id":"5f53601f-478c-4f02-aefa-1638436931d5","resolution":{"observed_at":"2026-05-11T11:51:01.348342Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.02460","last_updated":"2025-02-23T01:08:44Z","snapshot_observed_at":"2026-08-07T17:12:36.215426Z","submitted_at":"2024-07-02T17:37:34Z","title":"A new bump in the night: evidence of a new feature in the binary black hole mass distribution at $70~M_{\\odot}$ from gravitational-wave observations","version":2},"cited_work":{"arxiv_id":"2407.02460","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.02460","snapshot_observed_at":"2026-06-30T14:34:46.225574Z","title":"Maga˜ na Hernandez and A","venue":null,"work_id":"187d371e-9cf8-4f26-a488-2ab9c4a9f7fd","year":2025},"citing_paper":{"arxiv_id":"2606.30144","last_updated":"2026-06-29T11:21:48Z","snapshot_observed_at":"2026-07-07T00:04:00.652252Z","submitted_at":"2026-06-29T11:21:48Z","title":"Joint population and strong-lensing inference for resolved gravitational-wave events probes the black-hole merger rate beyond the peak of star formation","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-06-30T05:24:03.103599Z"},"links":{"cited_paper":"/paper/2407.02460","citing_paper":"/paper/2606.30144"},"observation_digest":"sha256:38e9050a73da641ff4fc20db28159463d5bf7541d5bcc823d2192f631f78319e","observation_id":"6c8a30aa-54da-4643-a322-b3eb5693f658","resolution":{"observed_at":"2026-06-30T14:34:46.226852Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.02460","last_updated":"2025-02-23T01:08:44Z","snapshot_observed_at":"2026-08-07T17:12:36.215426Z","submitted_at":"2024-07-02T17:37:34Z","title":"A new bump in the night: evidence of a new feature in the binary black hole mass distribution at $70~M_{\\odot}$ from gravitational-wave observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.02460","snapshot_observed_at":"2026-07-31T22:07:32.529082Z","title":"A New Bump in the Night: Evidence of a New Feature in the Binary Black Hole Mass Distribution at \\ 70 m\\_ odot \\ from Gravitational-Wave Observations , shorttitle =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.27962","last_updated":"2026-07-30T10:08:21Z","snapshot_observed_at":"2026-08-07T18:12:44.453436Z","submitted_at":"2026-07-30T10:08:21Z","title":"High-mass binary black hole mergers from detailed binary evolution models","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-07-31T22:07:32.529082Z"},"links":{"cited_paper":"/paper/2407.02460","citing_paper":"/paper/2607.27962"},"observation_digest":"sha256:a024a26a1b2827a5298aae5cd7c77ff32899a3354832942a65a643a033b153a4","observation_id":"ba274446-4089-4d1f-9689-9c46facc58e5","resolution":{"observed_at":"2026-07-31T22:07:32.529082Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2407.02460/citation-record","integrity":"/paper/2407.02460/integrity","json":"/paper/2407.02460/citation-record.json","paper":"/paper/2407.02460"},"outbound":[],"paper":{"arxiv_id":"2407.02460","last_updated":"2025-02-23T01:08:44Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-07T17:12:36.215426Z","submitted_at":"2024-07-02T17:37:34Z","title":"A new bump in the night: evidence of a new feature in the binary black hole mass distribution at $70~M_{\\odot}$ from gravitational-wave observations"},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2407.02460."}