{"as_of":"2026-08-11T10:26:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3021e3a3afa8df3e5a8639555f1603f267ea0e0d1a5274a11bdbd4c52d5d04ab","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":9,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":9,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T22:52:12.123246Z","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":"2026-07-03T12:58:07.823030Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2010.16333","last_updated":"2021-02-15T14:39:21Z","snapshot_observed_at":"2026-07-06T10:10:13.204791Z","submitted_at":"2020-10-30T15:48:01Z","title":"The impact of mass-transfer physics on the observable properties of field binary black hole populations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.16333","snapshot_observed_at":"2026-08-06T22:52:12.123246Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.20731","last_updated":"2026-07-15T17:08:17Z","snapshot_observed_at":"2026-08-08T12:25:37.324387Z","submitted_at":"2025-06-25T18:00:52Z","title":"Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T22:52:12.123246Z"},"links":{"cited_paper":"/paper/2010.16333","citing_paper":"/paper/2506.20731"},"observation_digest":"sha256:8bd012a3c914aef4ae22303e48922b6aca294cf67e39852c3e6b0d72198a05ce","observation_id":"ed555f5b-b560-4dbd-a342-8c9f51dd1aa6","resolution":{"observed_at":"2026-08-06T22:52:12.123246Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.16333","last_updated":"2021-02-15T14:39:21Z","snapshot_observed_at":"2026-07-06T10:10:13.204791Z","submitted_at":"2020-10-30T15:48:01Z","title":"The impact of mass-transfer physics on the observable properties of field binary black hole populations","version":2},"cited_work":{"arxiv_id":"2010.16333","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2010.16333","snapshot_observed_at":"2026-07-03T12:58:07.823030Z","title":"2021 A&A 647 A153 (Preprint 2010.16333)","venue":null,"work_id":"07fc0900-6b80-4808-a75b-037a9b1353c9","year":2021},"citing_paper":{"arxiv_id":"2507.23663","last_updated":"2026-04-22T17:03:18Z","snapshot_observed_at":"2026-07-06T22:05:52.712231Z","submitted_at":"2025-07-31T15:40:32Z","title":"Disentangling spinning and nonspinning binary black hole populations with spin sorting","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-19T02:22:28.762392Z"},"links":{"cited_paper":"/paper/2010.16333","citing_paper":"/paper/2507.23663"},"observation_digest":"sha256:780f74cc90fce2db8d5ae528050b1be0965d039e57a0d34a105bd841e2d121e8","observation_id":"c9e3d3a8-aef2-4192-85d2-4db8c9932821","resolution":{"observed_at":"2026-05-19T02:22:56.370195Z","resolver_source":"arxiv_id","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":"2010.16333","last_updated":"2021-02-15T14:39:21Z","snapshot_observed_at":"2026-07-06T10:10:13.204791Z","submitted_at":"2020-10-30T15:48:01Z","title":"The impact of mass-transfer physics on the observable properties of field binary black hole populations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.16333","snapshot_observed_at":"2026-08-05T15:53:32.048440Z","title":"2021 Astron","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.19336","last_updated":"2025-08-26T18:00:09Z","snapshot_observed_at":"2026-08-08T19:51:56.866678Z","submitted_at":"2025-08-26T18:00:09Z","title":"Exploring the astrophysical origins of binary black holes using normalising flows","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-05T15:53:32.048440Z"},"links":{"cited_paper":"/paper/2010.16333","citing_paper":"/paper/2508.19336"},"observation_digest":"sha256:4bb510a4a9fc972f92d1abe38bdaec62b626ea890f84526c9dab5499c5b1e458","observation_id":"2e2c6388-d3de-41f9-abbe-5cfa0681b67f","resolution":{"observed_at":"2026-08-05T15:53:32.048440Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.16333","last_updated":"2021-02-15T14:39:21Z","snapshot_observed_at":"2026-07-06T10:10:13.204791Z","submitted_at":"2020-10-30T15:48:01Z","title":"The impact of mass-transfer physics on the observable properties of field binary black hole populations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.16333","snapshot_observed_at":"2026-08-04T19:47:51.983838Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.09123","last_updated":"2025-09-11T03:28:10Z","snapshot_observed_at":"2026-08-05T05:24:50.033772Z","submitted_at":"2025-09-11T03:28:10Z","title":"Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-04T19:47:51.983838Z"},"links":{"cited_paper":"/paper/2010.16333","citing_paper":"/paper/2509.09123"},"observation_digest":"sha256:ce278a81afa0003429bf2373f622d4a2d6deeff56d165864dc2d5163ad3a9e4a","observation_id":"6ee59522-d896-4b3a-a96d-c3566affb1e2","resolution":{"observed_at":"2026-08-04T19:47:51.983838Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.16333","last_updated":"2021-02-15T14:39:21Z","snapshot_observed_at":"2026-07-06T10:10:13.204791Z","submitted_at":"2020-10-30T15:48:01Z","title":"The impact of mass-transfer physics on the observable properties of field binary black hole populations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.16333","snapshot_observed_at":"2026-08-03T14:34:26.808734Z","title":"S.et al.The impact of mass-transfer physics on the observable properties of field binary black hole populations.Astron","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-04T23:37:26.854248Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:26.808734Z"},"links":{"cited_paper":"/paper/2010.16333","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:c141cf17bb34178cc61c919a80edd46abd3165ecbbcf036f4435d046d69fb06d","observation_id":"b0e80810-f90e-4b39-b14c-74c72c09e0ab","resolution":{"observed_at":"2026-08-03T14:34:26.808734Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.16333","last_updated":"2021-02-15T14:39:21Z","snapshot_observed_at":"2026-07-06T10:10:13.204791Z","submitted_at":"2020-10-30T15:48:01Z","title":"The impact of mass-transfer physics on the observable properties of field binary black hole populations","version":2},"cited_work":{"arxiv_id":"2010.16333","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2010.16333","snapshot_observed_at":"2026-07-03T12:58:07.823030Z","title":"2021 A&A 647 A153 (Preprint 2010.16333)","venue":null,"work_id":"07fc0900-6b80-4808-a75b-037a9b1353c9","year":2021},"citing_paper":{"arxiv_id":"2604.06090","last_updated":"2026-04-08T17:19:33Z","snapshot_observed_at":"2026-08-11T00:41:51.210588Z","submitted_at":"2026-04-07T17:03:44Z","title":"Posterior Predictive Checks for Gravitational-wave Populations: Limitations and Improvements","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-05-10T19:10:35.351205Z"},"links":{"cited_paper":"/paper/2010.16333","citing_paper":"/paper/2604.06090"},"observation_digest":"sha256:29081d4faaa7a870b57615f72ce06ecbd7b98c3a6fcffe5dd7fbecece65735d1","observation_id":"8676d185-009f-4f13-a2e2-57999b620a86","resolution":{"observed_at":"2026-05-10T23:25:50.530707Z","resolver_source":"arxiv_id","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":"2010.16333","last_updated":"2021-02-15T14:39:21Z","snapshot_observed_at":"2026-07-06T10:10:13.204791Z","submitted_at":"2020-10-30T15:48:01Z","title":"The impact of mass-transfer physics on the observable properties of field binary black hole populations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.16333","snapshot_observed_at":"2026-08-02T12:20:51.730201Z","title":"The impact of mass-transfer physics on the observable properties of field binary black hole populations.Astron","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2606.06209","last_updated":"2026-07-29T20:31:40Z","snapshot_observed_at":"2026-08-02T23:18:03.130634Z","submitted_at":"2026-06-04T14:14:46Z","title":"The first decade of gravitational-wave measurements of black hole spins","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-02T12:20:51.730201Z"},"links":{"cited_paper":"/paper/2010.16333","citing_paper":"/paper/2606.06209"},"observation_digest":"sha256:c2a26cfa9a5806edcec64aa6f0f9ccd0e3c919f569c06001185ccfe3e385f4b6","observation_id":"b70dfd88-61bf-4409-8dfd-f8d5ac43627b","resolution":{"observed_at":"2026-08-02T12:20:51.730201Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.16333","last_updated":"2021-02-15T14:39:21Z","snapshot_observed_at":"2026-07-06T10:10:13.204791Z","submitted_at":"2020-10-30T15:48:01Z","title":"The impact of mass-transfer physics on the observable properties of field binary black hole populations","version":2},"cited_work":{"arxiv_id":"2010.16333","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2010.16333","snapshot_observed_at":"2026-07-03T12:58:07.823030Z","title":"2021 A&A 647 A153 (Preprint 2010.16333)","venue":null,"work_id":"07fc0900-6b80-4808-a75b-037a9b1353c9","year":2021},"citing_paper":{"arxiv_id":"2606.12205","last_updated":"2026-06-22T22:41:15Z","snapshot_observed_at":"2026-07-06T23:51:07.629939Z","submitted_at":"2026-06-10T15:21:46Z","title":"Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-06-27T08:41:37.044992Z"},"links":{"cited_paper":"/paper/2010.16333","citing_paper":"/paper/2606.12205"},"observation_digest":"sha256:5806cdb0f2f0b41f605f0986496f19b484e68bacca31c7b094429de9035feca0","observation_id":"68848b62-86a9-4fd2-b882-19f28a2feecb","resolution":{"observed_at":"2026-07-03T12:58:07.824763Z","resolver_source":"arxiv_id","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":"2010.16333","last_updated":"2021-02-15T14:39:21Z","snapshot_observed_at":"2026-07-06T10:10:13.204791Z","submitted_at":"2020-10-30T15:48:01Z","title":"The impact of mass-transfer physics on the observable properties of field binary black hole populations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.16333","snapshot_observed_at":"2026-07-31T01:54:12.413772Z","title":"and others","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.28622","last_updated":"2026-07-30T17:59:19Z","snapshot_observed_at":"2026-08-06T10:14:06.680339Z","submitted_at":"2026-07-30T17:59:19Z","title":"A Four-dimensional Model-agnostic Probe into the Astrophysical Origins of Binary Black Hole Subpopulations","version":1},"reference_index":102,"source":"arxiv_source","source_observed_at":"2026-07-31T01:54:12.413772Z"},"links":{"cited_paper":"/paper/2010.16333","citing_paper":"/paper/2607.28622"},"observation_digest":"sha256:5af46bf14baa9f37d3c65fe2fc4393d531dc1aaa0880534d1eb41de8ab3efabf","observation_id":"bdad1efd-ae67-4d2b-b7d8-c920737359cb","resolution":{"observed_at":"2026-07-31T01:54:12.413772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2010.16333/citation-record","integrity":"/paper/2010.16333/integrity","json":"/paper/2010.16333/citation-record.json","paper":"/paper/2010.16333"},"outbound":[],"paper":{"arxiv_id":"2010.16333","last_updated":"2021-02-15T14:39:21Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T10:10:13.204791Z","submitted_at":"2020-10-30T15:48:01Z","title":"The impact of mass-transfer physics on the observable properties of field binary black hole populations"},"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":"2026-08-11T06:34:44.6726+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 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2010.16333."}