{"as_of":"2026-08-22T20:52:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e07d047f45aeccf7fefc2cfeaa7f23e76ea0fcc59c3d8ebfaf47cdeb6ca8c585","coverage":[{"denominator":169,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T14:34:32.533103Z","state":"measured"},{"denominator":105,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":105,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-22T06:32:14.747728+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":"2026-08-15T14:20:11.341264Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"cited_work":{"arxiv_id":"2512.20054","doi":"10.48550/arxiv.2512.20054","metadata_source":"arxiv_reference","pith_arxiv_id":"2512.20054","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2025a [arXiv:2512.20054]","venue":"arXiv (Cornell University)","work_id":"e24ff444-39f1-4f52-a741-2b401e73e61c","year":2025},"citing_paper":{"arxiv_id":"2604.05492","last_updated":"2026-04-07T06:34:33Z","snapshot_observed_at":"2026-08-02T06:58:45.933537Z","submitted_at":"2026-04-07T06:34:33Z","title":"Remnant recoil and host environments of GWTC-4.0 binary black-hole mergers","version":1},"reference_index":127,"source":"pdf_text","source_observed_at":"2026-05-10T19:50:47.108345Z"},"links":{"cited_paper":"/paper/2512.20054","citing_paper":"/paper/2604.05492"},"observation_digest":"sha256:43015ab51eae0bc968b916380ae8913ef46c94e6806a650f458e3e0a4a610950","observation_id":"f8cc7267-9fde-4e43-9358-fbcd47edfded","resolution":{"observed_at":"2026-07-21T03:21:40.019212Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"cited_work":{"arxiv_id":"2512.20054","doi":"10.48550/arxiv.2512.20054","metadata_source":"arxiv_reference","pith_arxiv_id":"2512.20054","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2025a [arXiv:2512.20054]","venue":"arXiv (Cornell University)","work_id":"e24ff444-39f1-4f52-a741-2b401e73e61c","year":2025},"citing_paper":{"arxiv_id":"2606.03776","last_updated":"2026-06-02T15:28:50Z","snapshot_observed_at":"2026-08-09T15:46:14.461523Z","submitted_at":"2026-06-02T15:28:50Z","title":"Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors","version":1},"reference_index":101,"source":"pdf_text","source_observed_at":"2026-06-28T09:07:09.699995Z"},"links":{"cited_paper":"/paper/2512.20054","citing_paper":"/paper/2606.03776"},"observation_digest":"sha256:811a1830d87bb4e2b50988860e2cdb8cc28aa91c51f18ee0a439ad3a06be9a15","observation_id":"3597fb3b-a19e-4186-babb-8ae7dff30b7d","resolution":{"observed_at":"2026-07-21T03:21:40.019212Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"cited_work":{"arxiv_id":"2512.20054","doi":"10.48550/arxiv.2512.20054","metadata_source":"arxiv_reference","pith_arxiv_id":"2512.20054","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2025a [arXiv:2512.20054]","venue":"arXiv (Cornell University)","work_id":"e24ff444-39f1-4f52-a741-2b401e73e61c","year":2025},"citing_paper":{"arxiv_id":"2606.27852","last_updated":"2026-06-26T08:47:32Z","snapshot_observed_at":"2026-08-18T18:34:48.107654Z","submitted_at":"2026-06-26T08:47:32Z","title":"Mass-Ratio Reversal as an Alternative to Hierarchical Mergers for GW241011","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-06-29T03:13:20.189772Z"},"links":{"cited_paper":"/paper/2512.20054","citing_paper":"/paper/2606.27852"},"observation_digest":"sha256:67788b687278d496614e6cd84d248979aa872098e8359f4de3e0c5592190000b","observation_id":"eaca5c9d-2f9e-4e2a-9373-e7fe0589a95e","resolution":{"observed_at":"2026-07-21T03:21:40.019212Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2512.20054","snapshot_observed_at":"2026-08-05T20:32:25.647332Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.03348","last_updated":"2026-08-04T08:56:37Z","snapshot_observed_at":"2026-08-14T11:48:36.217128Z","submitted_at":"2026-08-04T08:56:37Z","title":"Unravelling Mass Transfer in Algols from Surface Abundances. I. Z Vulpeculae","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-05T20:32:25.647332Z"},"links":{"cited_paper":"/paper/2512.20054","citing_paper":"/paper/2608.03348"},"observation_digest":"sha256:9a0b26bc9fc5649ac0d70c1635e0ee0c2b4d5beaa5b080cec04cf9b43aad6c40","observation_id":"0d453293-cece-4a7a-8f6f-e7f3948caa02","resolution":{"observed_at":"2026-08-05T20:32:25.647332Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2512.20054","snapshot_observed_at":"2026-08-15T14:20:11.341264Z","title":"arXiv:2512.20054","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.11311","last_updated":"2026-08-11T18:01:00Z","snapshot_observed_at":"2026-08-20T23:58:44.728431Z","submitted_at":"2026-08-11T18:01:00Z","title":"A Diverse Distribution of Black Hole Spins from Stable Mass Transfer","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:11.341264Z"},"links":{"cited_paper":"/paper/2512.20054","citing_paper":"/paper/2608.11311"},"observation_digest":"sha256:384cda9eacb4db559cc1e8934c930965a403e4100f7c37242eb333941ebc7f57","observation_id":"dbec9cae-067b-4610-ac68-f9479a85bd8c","resolution":{"observed_at":"2026-08-15T14:20:11.341264Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2512.20054/citation-record","integrity":"/paper/2512.20054/integrity","json":"/paper/2512.20054/citation-record.json","paper":"/paper/2512.20054"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2508.18080","last_updated":"2026-06-26T11:37:39Z","snapshot_observed_at":"2026-08-16T08:27:09.645325Z","submitted_at":"2025-08-25T14:46:07Z","title":"GWTC-4.0: An Introduction to Version 4.0 of the Gravitational-Wave Transient Catalog","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2508.18080","snapshot_observed_at":"2026-08-03T14:34:22.314826Z","title":"2508.18080","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:22.314826Z"},"links":{"cited_paper":"/paper/2508.18080","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:81cf835a861b18e1384bef81c158f150f4fc5eabc2607f94dc28632ec5b8cd35","observation_id":"2eacd42f-e661-46c8-990a-5c400a733658","resolution":{"observed_at":"2026-08-03T14:34:22.314826Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2508.18082","last_updated":"2026-06-26T11:38:00Z","snapshot_observed_at":"2026-08-17T00:03:22.576608Z","submitted_at":"2025-08-25T14:46:09Z","title":"GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2508.18082","snapshot_observed_at":"2026-08-03T14:34:22.358485Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:22.358485Z"},"links":{"cited_paper":"/paper/2508.18082","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:57dccac40b4d4aac551b0daff04d077c6b67906fccc8922089d3255a63f71e65","observation_id":"674c092e-4691-4c68-9ebb-ed9af50d5afe","resolution":{"observed_at":"2026-08-03T14:34:22.358485Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2508.18083","last_updated":"2025-09-17T21:27:18Z","snapshot_observed_at":"2026-08-16T21:22:20.724531Z","submitted_at":"2025-08-25T14:46:10Z","title":"GWTC-4.0: Population Properties of Merging Compact Binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2508.18083","snapshot_observed_at":"2026-08-03T14:34:22.462191Z","title":"GWTC-4.0: Population Properties of Merging Compact Binaries.arXiv e-prints arXiv:2508.18083 (2025).2508.18083","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:22.462191Z"},"links":{"cited_paper":"/paper/2508.18083","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:822391795570fec9f9e3720c4eba060860c0a2d928a930a29309080faceb6842","observation_id":"f79fb8db-6508-4a72-afce-0e8fec387c50","resolution":{"observed_at":"2026-08-03T14:34:22.462191Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06590","last_updated":"2019-04-01T13:03:33Z","snapshot_observed_at":"2026-08-20T23:30:46.555392Z","submitted_at":"2018-07-17T07:34:47Z","title":"Clusters of primordial black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06590","snapshot_observed_at":"2026-08-03T14:34:22.571717Z","title":"M.et al.Clusters of Primordial Black Holes.European Physical Journal C 79, 246 (2019).1807.06590","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:22.571717Z"},"links":{"cited_paper":"/paper/1807.06590","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:7c5700c01298b8afb3807aaa21e74fa27a415b39b655c503a107f6d6da88ab1d","observation_id":"a9791733-6d72-4ed8-ad6b-9783c4e6966a","resolution":{"observed_at":"2026-08-03T14:34:22.571717Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.10260","last_updated":"2019-08-04T13:32:52Z","snapshot_observed_at":"2026-08-17T15:34:08.039010Z","submitted_at":"2019-06-24T22:49:02Z","title":"Black Holes: The Next Generation -- Repeated Mergers in Dense Star Clusters and their Gravitational-Wave Properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.10260","snapshot_observed_at":"2026-08-03T14:34:22.685207Z","title":"L.et al.Black holes: The next generation—repeated mergers in dense star clusters and their gravitational-wave properties.Phys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:22.685207Z"},"links":{"cited_paper":"/paper/1906.10260","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:f80573c1dc0555c3c6b2f95c756b34f86c8119713583b6de8bd18926ddcfac8b","observation_id":"2538c34e-27cb-46fe-a267-0928142f6542","resolution":{"observed_at":"2026-08-03T14:34:22.685207Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.09765","last_updated":"2022-04-21T09:35:41Z","snapshot_observed_at":"2026-08-16T19:12:20.180235Z","submitted_at":"2020-10-19T18:09:12Z","title":"AGN as Potential Factories for Eccentric Black Hole Mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.09765","snapshot_observed_at":"2026-08-03T14:34:22.745375Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:22.745375Z"},"links":{"cited_paper":"/paper/2010.09765","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:d53c3507b9c9a0000011dc7313822cdab6a46c916117511b2dc2e338d6d65393","observation_id":"e61d91eb-00f8-4212-b76e-3c94101395ff","resolution":{"observed_at":"2026-08-03T14:34:22.745375Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.07633","last_updated":"2022-09-07T16:30:36Z","snapshot_observed_at":"2026-08-16T17:21:03.922603Z","submitted_at":"2022-02-15T18:29:42Z","title":"Hydrodynamical Evolution of Black-Hole Binaries Embedded in AGN Discs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.07633","snapshot_observed_at":"2026-08-03T14:34:22.853287Z","title":"& Lai, D","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:22.853287Z"},"links":{"cited_paper":"/paper/2202.07633","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:49ef87be23dfe061478de9473583ea98a7ab2e6ad2bb3e8a09c13dfd43dfba44","observation_id":"879363dd-7a0b-4b5d-a6bb-f982ca97a3ea","resolution":{"observed_at":"2026-08-03T14:34:22.853287Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.13669","last_updated":"2020-12-22T12:05:08Z","snapshot_observed_at":"2026-08-18T19:18:04.169139Z","submitted_at":"2020-10-26T15:45:27Z","title":"Massive Stellar Triples Leading to Sequential Binary Black-Hole Mergers in the Field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.13669","snapshot_observed_at":"2026-08-03T14:34:22.913418Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:22.913418Z"},"links":{"cited_paper":"/paper/2010.13669","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:a52c3326b9e310baf98083ca6df97e14ea406e3015c3fa7568553ecf7f26f1a6","observation_id":"681da8d3-9c40-415e-bb9b-ec215d2bca38","resolution":{"observed_at":"2026-08-03T14:34:22.913418Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.03202","last_updated":"2018-08-12T07:42:20Z","snapshot_observed_at":"2026-08-14T19:17:29.336592Z","submitted_at":"2018-05-08T18:00:00Z","title":"Black Hole and Neutron Star Binary Mergers in Triple Systems: Merger Fraction and Spin-Orbit Misalignment","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.03202","snapshot_observed_at":"2026-08-03T14:34:23.011350Z","title":"& Lai, D","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:23.011350Z"},"links":{"cited_paper":"/paper/1805.03202","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:19bac40d6c29dac7a16ad1d528f018a6678a128138a09d7c0c4599cc4fddec13","observation_id":"8966bc1d-b95b-49c3-834e-67c156454f8a","resolution":{"observed_at":"2026-08-03T14:34:23.011350Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.12455","last_updated":"2021-05-26T10:32:40Z","snapshot_observed_at":"2026-08-16T18:22:07.226143Z","submitted_at":"2021-05-26T10:32:40Z","title":"Binary black hole mergers: formation and populations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.12455","snapshot_observed_at":"2026-08-03T14:34:23.106839Z","title":"Binary black hole mergers: formation and populations.Frontiers in Astron- omy and Space Sciences7, 38 (2020).2105.12455","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:23.106839Z"},"links":{"cited_paper":"/paper/2105.12455","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:78b9930022e2a0954a16c0adaa65726f1bbc48b37a4639c8e23569f96b55b067","observation_id":"77382cf2-4bf0-416e-8937-2f2437c24acd","resolution":{"observed_at":"2026-08-03T14:34:23.106839Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.14239","last_updated":"2022-08-26T05:59:15Z","snapshot_observed_at":"2026-08-19T14:04:36.846784Z","submitted_at":"2021-07-29T18:00:01Z","title":"Rates of Compact Object Coalescences","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.14239","snapshot_observed_at":"2026-08-03T14:34:23.165681Z","title":"& Broekgaarden, F","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:23.165681Z"},"links":{"cited_paper":"/paper/2107.14239","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:8054df80c3920bfcefc2a99e54458560a428dec4bccff2d27c58ec3054cb3cca","observation_id":"060173bf-befa-476a-8135-80796ca61caf","resolution":{"observed_at":"2026-08-03T14:34:23.165681Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.6397","last_updated":"2012-07-26T20:00:01Z","snapshot_observed_at":"2026-08-15T00:51:56.256620Z","submitted_at":"2012-07-26T20:00:01Z","title":"Binary interaction dominates the evolution of massive stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.6397","snapshot_observed_at":"2026-08-03T14:34:23.274311Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:23.274311Z"},"links":{"cited_paper":"/paper/1207.6397","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:8fe58bec35317e162c474117a6ec6b5bcab7dcba22df9141d03fc2d7f4e8c947","observation_id":"752b1bf8-a278-4ada-90af-d9e12c253237","resolution":{"observed_at":"2026-08-03T14:34:23.274311Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.05702","last_updated":"2021-11-05T16:02:11Z","snapshot_observed_at":"2026-08-19T12:35:33.869885Z","submitted_at":"2021-07-12T19:37:30Z","title":"Binary Black Hole Formation with Detailed Modeling: Stable Mass Transfer Leads to Lower Merger Rates","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.05702","snapshot_observed_at":"2026-08-03T14:34:23.387455Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:23.387455Z"},"links":{"cited_paper":"/paper/2107.05702","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:42589c28c1a50e372e45430a0b83f66e95405529edd25240dd3abd48b13d8e91","observation_id":"607b89ef-14cc-405a-b3b1-ea23dc2fb514","resolution":{"observed_at":"2026-08-03T14:34:23.387455Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.05722","last_updated":"2017-08-18T18:00:28Z","snapshot_observed_at":"2026-08-14T20:40:36.242447Z","submitted_at":"2017-08-18T18:00:28Z","title":"The cosmic merger rate of stellar black hole binaries from the Illustris simulation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.05722","snapshot_observed_at":"2026-08-03T14:34:23.442789Z","title":"& Spera, M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:23.442789Z"},"links":{"cited_paper":"/paper/1708.05722","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:d13971663ff3ee716d28c8c3c63fcaf5909f9377424983465cd1b9c101498b59","observation_id":"495e3a53-3020-40ed-9801-e8a565cbb1dd","resolution":{"observed_at":"2026-08-03T14:34:23.442789Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.05433","last_updated":"2018-08-14T12:31:50Z","snapshot_observed_at":"2026-08-14T19:54:35.990174Z","submitted_at":"2018-01-16T19:00:05Z","title":"Progenitors of gravitational wave mergers: Binary evolution with the stellar grid-based code ComBinE","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.05433","snapshot_observed_at":"2026-08-03T14:34:23.551896Z","title":"U., Tauris, T","venue":null,"work_id":null,"year":1908},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:23.551896Z"},"links":{"cited_paper":"/paper/1801.05433","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:e5378b79d01451bad506bb45a45b770b3ea5c6e1e4aabfc1a586bdd61bda771a","observation_id":"4665c906-0f57-4219-a5e1-77a01ff72da6","resolution":{"observed_at":"2026-08-03T14:34:23.551896Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.03565","last_updated":"2021-07-08T02:08:05Z","snapshot_observed_at":"2026-08-16T18:11:33.287505Z","submitted_at":"2021-07-08T02:08:05Z","title":"Population Synthesis of Black Hole Binaries with Compact Star Companions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.03565","snapshot_observed_at":"2026-08-03T14:34:23.611843Z","title":"& Li, X.-D","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:23.611843Z"},"links":{"cited_paper":"/paper/2107.03565","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:6b41c85539dd879ef31160a0581a5032daae8f81122d63c8b1695551e0a1a8bc","observation_id":"f324a1fb-cd6b-4cb6-bd45-2703146c071b","resolution":{"observed_at":"2026-08-03T14:34:23.611843Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.10924","last_updated":"2022-12-21T11:12:16Z","snapshot_observed_at":"2026-08-18T17:11:31.874068Z","submitted_at":"2022-12-21T11:12:16Z","title":"The formation of $30\\,M_\\odot$ merging black holes at solar metallicity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.10924","snapshot_observed_at":"2026-08-03T14:34:23.717747Z","title":"S.et al.The formation of merging black holes with masses beyond 30 M ⊙ at solar metallicity.Nature Astronomy7, 1090–1097 (2023).2212.10924","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:23.717747Z"},"links":{"cited_paper":"/paper/2212.10924","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:ec7ec42dba834e9ae3fc3e38d67f93aa3eb170b9d17bc42f6738145b8c4a8fe0","observation_id":"d5322691-1c88-4938-972e-cde227d80211","resolution":{"observed_at":"2026-08-03T14:34:23.717747Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.04531","last_updated":"2016-06-22T16:33:04Z","snapshot_observed_at":"2026-08-14T22:10:22.620489Z","submitted_at":"2016-02-15T00:21:36Z","title":"The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.04531","snapshot_observed_at":"2026-08-03T14:34:23.865950Z","title":"E., Bulik, T","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:23.865950Z"},"links":{"cited_paper":"/paper/1602.04531","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:2f726002b732cf34e59d03fbb22ff3cb5b979deb59b4657730a8a5aa8e6c56c6","observation_id":"89f2a6f6-f2ec-4fac-9799-b2f0248c5657","resolution":{"observed_at":"2026-08-03T14:34:23.865950Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.01865","last_updated":"2023-11-03T12:16:06Z","snapshot_observed_at":"2026-08-16T14:46:15.129889Z","submitted_at":"2023-11-03T12:16:06Z","title":"The Evolution of Massive Binary Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.01865","snapshot_observed_at":"2026-08-03T14:34:23.902856Z","title":"& Bodensteiner, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:23.902856Z"},"links":{"cited_paper":"/paper/2311.01865","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:37c78dc20b9b8b77bab59493d9950884a8ae07f99abe87b082457597c313a3ba","observation_id":"abb1d418-a8bd-4307-8b9c-87c414470260","resolution":{"observed_at":"2026-08-03T14:34:23.902856Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.4302","last_updated":"2012-12-06T17:35:49Z","snapshot_observed_at":"2026-08-18T02:17:06.122227Z","submitted_at":"2012-09-19T16:34:08Z","title":"Common Envelope Evolution: Where we stand and how we can move forward","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.4302","snapshot_observed_at":"2026-08-03T14:34:23.952843Z","title":"Astrophys","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:23.952843Z"},"links":{"cited_paper":"/paper/1209.4302","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:50119659eb51238893330e3336a62b8952b037c183372784821a05bc81e20f77","observation_id":"ef22961f-226a-41e8-8048-96e6c0745501","resolution":{"observed_at":"2026-08-03T14:34:23.952843Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.00774","last_updated":"2020-06-01T08:08:06Z","snapshot_observed_at":"2026-08-12T14:10:00.200935Z","submitted_at":"2020-06-01T08:08:06Z","title":"The thermal equilibrium mass loss model and its applications in binary evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.00774","snapshot_observed_at":"2026-08-03T14:34:23.975995Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:23.975995Z"},"links":{"cited_paper":"/paper/2006.00774","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:9e4197c5cf1eb800287897767740fdd1cf3d2a4dd71d9d72be4098b8b19bde15","observation_id":"ce9da954-39e3-487a-bd26-708366026d7a","resolution":{"observed_at":"2026-08-03T14:34:23.975995Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:24.028511Z","title":"Astrophys.650, A107 (2021).2103","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:24.028511Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:b389148800d05cc695574528cfe55721e163b64e98eeec7142d7283cb84a14b5","observation_id":"77c03ddb-e7ef-4975-a16f-9aa41cfcdb28","resolution":{"observed_at":"2026-08-03T14:34:24.028511Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.07308","last_updated":"2022-12-14T16:13:31Z","snapshot_observed_at":"2026-08-16T16:08:40.795383Z","submitted_at":"2022-12-14T16:13:31Z","title":"Simulations of common-envelope evolution in binary stellar systems: physical models and numerical techniques","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.07308","snapshot_observed_at":"2026-08-03T14:34:24.119932Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:24.119932Z"},"links":{"cited_paper":"/paper/2212.07308","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:937ed944179ff78372919e34e7a3d5f4b6058b29ece30b98db673887be1973dd","observation_id":"aac0c0bc-090c-4a27-97ae-235d8e0d7f77","resolution":{"observed_at":"2026-08-03T14:34:24.119932Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.20506","last_updated":"2025-07-02T12:54:26Z","snapshot_observed_at":"2026-08-16T12:46:39.386494Z","submitted_at":"2025-03-26T12:46:36Z","title":"Common envelopes in massive stars III. The obstructive role of radiation transport in envelope ejection","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.20506","snapshot_observed_at":"2026-08-03T14:34:24.179176Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:24.179176Z"},"links":{"cited_paper":"/paper/2503.20506","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:6ea7f06ac5ce7cd56b2627bf3a1affb78bd376350830a7023df4bbd54bd8c6f4","observation_id":"7370343b-8c6b-4dfd-a482-75b58e9cedc5","resolution":{"observed_at":"2026-08-03T14:34:24.179176Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:24.262755Z","title":"Radiation pressure and equation of state are important in the envelope unbinding process in common envelope evolution.arXiv e-printsarXiv:2510.14173 (2025).2510","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:24.262755Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:321ed655cf1781c3b30aba85c976fafce91a85ee962268ab5c4148b977ad8834","observation_id":"dd5dd81a-fd7a-489a-8349-61ca33205186","resolution":{"observed_at":"2026-08-03T14:34:24.262755Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0508242","last_updated":"2005-08-10T17:19:01Z","snapshot_observed_at":"2026-08-10T02:00:34.439839Z","submitted_at":"2005-08-10T17:19:01Z","title":"Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0508242","snapshot_observed_at":"2026-08-03T14:34:24.372389Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:24.372389Z"},"links":{"cited_paper":"/paper/astro-ph/0508242","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:c6763207c2387919c661c3ace4b4094f56cd922ee7e11ffe81e4671cf892e807","observation_id":"dc254665-0c4f-4299-b159-d1feb8138a15","resolution":{"observed_at":"2026-08-03T14:34:24.372389Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0508175","last_updated":"2005-08-08T17:59:08Z","snapshot_observed_at":"2026-08-11T23:20:36.536261Z","submitted_at":"2005-08-08T17:59:08Z","title":"The Progenitor Stars of Gamma-Ray Bursts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0508175","snapshot_observed_at":"2026-08-03T14:34:24.519453Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:24.519453Z"},"links":{"cited_paper":"/paper/astro-ph/0508175","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:fc96539046ca0f37be34146a72970e8158ed75b8da916aabbce1ca870325545b","observation_id":"41a9f3b7-a4b5-4fd9-9a32-3ad3e0cdde54","resolution":{"observed_at":"2026-08-03T14:34:24.519453Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.03718","last_updated":"2016-02-09T15:24:01Z","snapshot_observed_at":"2026-08-14T22:14:35.970279Z","submitted_at":"2016-01-14T20:24:13Z","title":"A new route towards merging massive black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.03718","snapshot_observed_at":"2026-08-03T14:34:24.670949Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:24.670949Z"},"links":{"cited_paper":"/paper/1601.03718","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:c098cb33d8d377ee27e499e3130126d05edf6e459699949f9ed61492996fa26a","observation_id":"f0f8464c-4852-41b8-b2d5-17c305f6dff0","resolution":{"observed_at":"2026-08-03T14:34:24.670949Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.03790","last_updated":"2016-07-19T23:36:30Z","snapshot_observed_at":"2026-08-18T05:54:49.082743Z","submitted_at":"2016-02-11T16:51:52Z","title":"BPASS predictions for Binary Black-Hole Mergers","version":6},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.03790","snapshot_observed_at":"2026-08-03T14:34:24.768947Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:24.768947Z"},"links":{"cited_paper":"/paper/1602.03790","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:768726a79052ec42520ddd37153915c990517ef2ba67c0ee61f504902d44d1e6","observation_id":"719fb58f-0585-4c39-89c7-21144952a12c","resolution":{"observed_at":"2026-08-03T14:34:24.768947Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.00007","last_updated":"2016-06-06T11:29:33Z","snapshot_observed_at":"2026-08-14T22:16:18.662663Z","submitted_at":"2015-12-31T21:00:20Z","title":"Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.00007","snapshot_observed_at":"2026-08-03T14:34:24.927264Z","title":"& de Mink, S","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:24.927264Z"},"links":{"cited_paper":"/paper/1601.00007","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:8965484e8b4e72db1ab05e16598db239a9a610c94282e5a58466768f3f025e55","observation_id":"5f9e8a6b-57a4-4fe2-b10f-2a9922e87f2f","resolution":{"observed_at":"2026-08-03T14:34:24.927264Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.11299","last_updated":"2020-07-22T09:33:00Z","snapshot_observed_at":"2026-08-17T18:50:07.823994Z","submitted_at":"2020-07-22T09:33:00Z","title":"Internal circulation in tidally locked massive binary stars -- Consequences for double black hole formation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.11299","snapshot_observed_at":"2026-08-03T14:34:25.054083Z","title":"& Koenigsberger, G","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:25.054083Z"},"links":{"cited_paper":"/paper/2007.11299","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:ae5aee83314700f996a3e4b87411a9b59788e071f891aae416231d99b8e6ea51","observation_id":"cbf72994-8d33-4187-9ebc-5e53903c3e30","resolution":{"observed_at":"2026-08-03T14:34:25.054083Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.10352","last_updated":"2021-12-28T10:56:41Z","snapshot_observed_at":"2026-08-16T17:55:16.395743Z","submitted_at":"2021-09-21T00:35:53Z","title":"Rapid stellar and binary population synthesis with COMPAS","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.10352","snapshot_observed_at":"2026-08-03T14:34:25.099081Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:25.099081Z"},"links":{"cited_paper":"/paper/2109.10352","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:1445dc989bc91013b1b6588536c7d19c98212066b504cb98427a6c7b7134aec7","observation_id":"955e30f7-822d-459f-888e-f02db249117c","resolution":{"observed_at":"2026-08-03T14:34:25.099081Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2509.00154","last_updated":"2025-08-29T18:00:02Z","snapshot_observed_at":"2026-08-13T09:16:31.136312Z","submitted_at":"2025-08-29T18:00:02Z","title":"Very Massive, Rapidly Spinning Binary Black Hole Progenitors through Chemically Homogeneous Evolution -- The Case of GW231123","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.00154","snapshot_observed_at":"2026-08-03T14:34:25.145199Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:25.145199Z"},"links":{"cited_paper":"/paper/2509.00154","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:7631f9fbf405a37ca9ff772061edc7787457c5fb14b88758a24de1e22ba8690e","observation_id":"7fe75f6b-ce5a-4907-bba0-7d9f5d702bdd","resolution":{"observed_at":"2026-08-03T14:34:25.145199Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.13609","last_updated":"2022-11-10T10:27:50Z","snapshot_observed_at":"2026-08-16T16:29:26.481207Z","submitted_at":"2022-09-27T18:05:59Z","title":"No peaks without valleys: The stable mass transfer channel for gravitational-wave sources in light of the neutron star-black hole mass gap","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.13609","snapshot_observed_at":"2026-08-03T14:34:25.192751Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:25.192751Z"},"links":{"cited_paper":"/paper/2209.13609","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:2822f56d78e5f0faf76bf2078afe041c062f592a89a8c0831c54346ee0e7d934","observation_id":"e48ebf5a-c64e-481c-8d36-77149b3aa15b","resolution":{"observed_at":"2026-08-03T14:34:25.192751Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.12426","last_updated":"2024-06-11T11:23:51Z","snapshot_observed_at":"2026-08-16T13:59:39.801690Z","submitted_at":"2024-04-18T18:00:01Z","title":"Unequal-mass, highly-spinning binary black hole mergers in the stable mass transfer formation channel","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.12426","snapshot_observed_at":"2026-08-03T14:34:25.238185Z","title":"Astrophys.689, A305 (2024).2404.12426","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:25.238185Z"},"links":{"cited_paper":"/paper/2404.12426","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:02dbdf4c5f9412e62b372e40d923c354e0870e506d42c3d741beba236b3a38d2","observation_id":"8d4844b4-8a76-45d1-af58-6123b2cee484","resolution":{"observed_at":"2026-08-03T14:34:25.238185Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.05736","last_updated":"2023-09-11T18:03:06Z","snapshot_observed_at":"2026-08-20T09:37:24.380535Z","submitted_at":"2023-09-11T18:03:06Z","title":"Forming merging double compact objects with stable mass transfer","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.05736","snapshot_observed_at":"2026-08-03T14:34:25.285475Z","title":"& Nelemans, G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:25.285475Z"},"links":{"cited_paper":"/paper/2309.05736","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:5748496e124594ca53a64a6ed54bb70aa235be7f60e8c43c90a5976f2efd8784","observation_id":"af99f6b5-e511-4589-be18-3fd9863f777d","resolution":{"observed_at":"2026-08-03T14:34:25.285475Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:25.313562Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:25.313562Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:33045f243e8dc99aa215097e9b8613f4071509c81657ae82c1b28f0bd71a3396","observation_id":"87dd7c81-5c4c-4d44-ae67-0d84dacfb573","resolution":{"observed_at":"2026-08-03T14:34:25.313562Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0201220","last_updated":"2002-01-14T19:30:32Z","snapshot_observed_at":"2026-07-07T00:24:31.117550Z","submitted_at":"2002-01-14T19:30:32Z","title":"Evolution of binary stars and the effect of tides on binary populations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0201220","snapshot_observed_at":"2026-08-03T14:34:25.356951Z","title":"R., Tout, C","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:25.356951Z"},"links":{"cited_paper":"/paper/astro-ph/0201220","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:a73d0716a976aba2fa0665e2d2f35f8395622fec114408db881e6f32459b8a91","observation_id":"6e24c5db-6a3f-4b09-bc91-f5aa15a547f5","resolution":{"observed_at":"2026-08-03T14:34:25.356951Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0511811","last_updated":"2007-06-07T01:40:18Z","snapshot_observed_at":"2026-07-07T00:56:25.882918Z","submitted_at":"2005-11-30T02:07:18Z","title":"Compact Object Modeling with the StarTrack Population Synthesis Code","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0511811","snapshot_observed_at":"2026-08-03T14:34:25.400418Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:25.400418Z"},"links":{"cited_paper":"/paper/astro-ph/0511811","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:c50cd1adc133fa35a5b6747fbede93dcea78b1dffeae30445fce4885e1bffd8e","observation_id":"227479ff-7ec9-4d5a-9702-c269df90e6ef","resolution":{"observed_at":"2026-08-03T14:34:25.400418Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.01693","last_updated":"2022-05-03T18:00:01Z","snapshot_observed_at":"2026-08-16T17:02:50.663253Z","submitted_at":"2022-05-03T18:00:01Z","title":"Signatures of mass ratio reversal in gravitational waves from merging binary black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.01693","snapshot_observed_at":"2026-08-03T14:34:25.455937Z","title":"S., Stevenson, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:25.455937Z"},"links":{"cited_paper":"/paper/2205.01693","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:2f1ad631aed3d91c729f853719bc29f45a868887a7e73612beb68b3b8c44ac08","observation_id":"29a264f1-76ca-40b3-9f52-7af8410ecdc3","resolution":{"observed_at":"2026-08-03T14:34:25.455937Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:25.495705Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:25.495705Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:0a70e08079bf588c3a37c2136bd2e1a4902d223cad4f506be518b078288c5d0a","observation_id":"8147ce66-4542-4063-8bc5-5b999fc0c0e4","resolution":{"observed_at":"2026-08-03T14:34:25.495705Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.00903","last_updated":"2020-09-10T18:51:24Z","snapshot_observed_at":"2026-08-18T22:27:36.053439Z","submitted_at":"2019-11-03T14:42:25Z","title":"COSMIC Variance in Binary Population Synthesis","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.00903","snapshot_observed_at":"2026-08-03T14:34:25.535980Z","title":"J.898, 71 (2020).1911.00903","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:25.535980Z"},"links":{"cited_paper":"/paper/1911.00903","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:4b982b4d460a9c6d3d3d938438b233351482483d1b7ee5c32b855a39e2e31f98","observation_id":"6c8ae79e-fa79-432a-b2d8-079979fdb0ed","resolution":{"observed_at":"2026-08-03T14:34:25.535980Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.14529","last_updated":"2022-03-28T06:49:57Z","snapshot_observed_at":"2026-08-17T17:49:35.659837Z","submitted_at":"2022-03-28T06:49:57Z","title":"Stable mass transfer can explain massive binary black hole mergers with a high spin component","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.14529","snapshot_observed_at":"2026-08-03T14:34:25.575274Z","title":"& Li, X.-D","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:25.575274Z"},"links":{"cited_paper":"/paper/2203.14529","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:7d7d33efc23e81d30ff8076b9cea351933f9f9f00680ac9981dcefeff1c3c56f","observation_id":"00684a30-e7d1-43a7-8e75-ae94643ae5e8","resolution":{"observed_at":"2026-08-03T14:34:25.575274Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.02154","last_updated":"2017-10-05T18:00:08Z","snapshot_observed_at":"2026-08-21T19:03:49.266572Z","submitted_at":"2017-10-05T18:00:08Z","title":"Binary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.02154","snapshot_observed_at":"2026-08-03T14:34:25.618939Z","title":"J.et al.Binary Population and Spectral Synthesis Version 2.1: Construction, Observational Verification, and New Results.Publ","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:25.618939Z"},"links":{"cited_paper":"/paper/1710.02154","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:2660a884cd1669963f65f03e66ce0c6d1c0ae9372222b33dec9aad4135c9121b","observation_id":"a228d653-d35b-435b-8c0b-31e529fcc958","resolution":{"observed_at":"2026-08-03T14:34:25.618939Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.13842","last_updated":"2022-10-03T07:44:12Z","snapshot_observed_at":"2026-08-16T16:49:53.267141Z","submitted_at":"2022-06-28T09:16:27Z","title":"Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.13842","snapshot_observed_at":"2026-08-03T14:34:25.695961Z","title":"M., Stevance, H","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:25.695961Z"},"links":{"cited_paper":"/paper/2206.13842","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:177c10a573c7db86b4cef209397c83a11c4fbc3e85b3486e393138da10f038aa","observation_id":"15b2d893-fcb7-4f33-a26d-a755cfa97bd9","resolution":{"observed_at":"2026-08-03T14:34:25.695961Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.05892","last_updated":"2022-08-07T07:47:37Z","snapshot_observed_at":"2026-08-16T17:21:53.439300Z","submitted_at":"2022-02-11T20:24:04Z","title":"POSYDON: A General-Purpose Population Synthesis Code with Detailed Binary-Evolution Simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.05892","snapshot_observed_at":"2026-08-03T14:34:25.815796Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:25.815796Z"},"links":{"cited_paper":"/paper/2202.05892","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:c9e9585ac6613789af8bf1a8cb11a713b0070da670224c1e60df8f84946f4f88","observation_id":"0e41f720-e043-4e28-a73f-f2bb835727ec","resolution":{"observed_at":"2026-08-03T14:34:25.815796Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1009.1622","last_updated":"2010-09-08T20:00:05Z","snapshot_observed_at":"2026-08-15T05:09:18.642020Z","submitted_at":"2010-09-08T20:00:05Z","title":"Modules for Experiments in Stellar Astrophysics (MESA)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1009.1622","snapshot_observed_at":"2026-08-03T14:34:25.972034Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:25.972034Z"},"links":{"cited_paper":"/paper/1009.1622","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:39d0c7110fb4a81d20a52288d97e08fda7bab8a5155f73e07b785f5cec0c2ddf","observation_id":"031b0a21-72b2-4aef-8490-0b360b4faeb1","resolution":{"observed_at":"2026-08-03T14:34:25.972034Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1301.0319","last_updated":"2013-06-12T19:42:55Z","snapshot_observed_at":"2026-08-12T19:03:26.795307Z","submitted_at":"2013-01-02T21:00:00Z","title":"Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1301.0319","snapshot_observed_at":"2026-08-03T14:34:26.151507Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:26.151507Z"},"links":{"cited_paper":"/paper/1301.0319","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:d2fc0c8982d2eb3a7a055af34616de9b3e84babb98e029eafd522868575b5d78","observation_id":"b740d775-4341-42d8-be8d-9fce70d63b4d","resolution":{"observed_at":"2026-08-03T14:34:26.151507Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1506.03146","last_updated":"2017-01-08T05:04:31Z","snapshot_observed_at":"2026-08-09T12:28:11.007796Z","submitted_at":"2015-06-10T02:23:18Z","title":"Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.03146","snapshot_observed_at":"2026-08-03T14:34:26.312627Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:26.312627Z"},"links":{"cited_paper":"/paper/1506.03146","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:c6a51ce95565c834823ea0291b2700ee4d313c942f5c45eab34c898794e8a443","observation_id":"78b75225-d721-4213-b52d-911891d2815d","resolution":{"observed_at":"2026-08-03T14:34:26.312627Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:26.416036Z","title":"& Langer, N","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:26.416036Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:72d956d361b9659585c4e5e474f9dd2223f197d4dda06ed2dd368d42da611117","observation_id":"f7faf4bc-a0b5-4ad8-8998-65fd11e2e871","resolution":{"observed_at":"2026-08-03T14:34:26.416036Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.10933","last_updated":"2021-09-23T16:02:50Z","snapshot_observed_at":"2026-08-16T18:08:05.951878Z","submitted_at":"2021-07-22T21:29:11Z","title":"Evolution of accretor stars in massive binaries: broader implications from modeling {\\zeta} Ophiuchi","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.10933","snapshot_observed_at":"2026-08-03T14:34:26.478654Z","title":"& G ¨otberg, Y","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:26.478654Z"},"links":{"cited_paper":"/paper/2107.10933","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:84abddb599c962a38ec90db635b1174050e93c8162af0c58b52bc3412cbec488","observation_id":"70ece332-366a-4966-8c5b-f8452a085c71","resolution":{"observed_at":"2026-08-03T14:34:26.478654Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1102.0530","last_updated":"2011-04-19T14:52:44Z","snapshot_observed_at":"2026-08-19T11:44:48.725536Z","submitted_at":"2011-02-02T18:47:17Z","title":"Rotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1102.0530","snapshot_observed_at":"2026-08-03T14:34:26.561071Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:26.561071Z"},"links":{"cited_paper":"/paper/1102.0530","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:0e3c6530ab405e60792facd4d944d8964456d7148cd6241de133a086bab503e5","observation_id":"ebfed133-3424-4890-bca8-30f1f407b46d","resolution":{"observed_at":"2026-08-03T14:34:26.561071Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:26.638003Z","title":"& Weigert, A","venue":null,"work_id":null,"year":1967},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:26.638003Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:294089adb549ddfa2294da40d1bf1b347fad521bfbd759565f093c0cd1697d7f","observation_id":"9ff8d4ed-61e9-464f-bcae-3792220a0176","resolution":{"observed_at":"2026-08-03T14:34:26.638003Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.08612","last_updated":"2024-04-12T17:22:22Z","snapshot_observed_at":"2026-08-19T01:12:04.915239Z","submitted_at":"2024-04-12T17:22:22Z","title":"Analytic approximations for massive close post-mass transfer binary systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.08612","snapshot_observed_at":"2026-08-03T14:34:26.709820Z","title":"Astrophys.690, A282 (2024).2404.08612","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:26.709820Z"},"links":{"cited_paper":"/paper/2404.08612","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:550f477b77e629f47a924151d61adda73eab01e544f437fc6d7b26d79ed3cc61","observation_id":"dc679489-f4db-4ec9-b4f2-593c8bed4bf1","resolution":{"observed_at":"2026-08-03T14:34:26.709820Z","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":"2026-08-19T13:06:12.010812Z","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":"2026-08-14T11:48:00.367296Z","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":"sha256:825e6d659d65898db6a820c6689a73df8231b41e8533b0d4e5de316896fc255e","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":"2109.06872","last_updated":"2021-10-11T15:16:41Z","snapshot_observed_at":"2026-08-17T20:58:00.845856Z","submitted_at":"2021-09-14T17:59:59Z","title":"The implications of high BH spins on the origin of BH-BH mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.06872","snapshot_observed_at":"2026-08-03T14:34:26.888852Z","title":"& Belczynski, K","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:26.888852Z"},"links":{"cited_paper":"/paper/2109.06872","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:875c9f1419ed26f50c855b7625723a9a0fd4db47fcda2e5cf29a0e5b84f01b92","observation_id":"74835b7e-0e6a-4e10-80bc-c304999881bc","resolution":{"observed_at":"2026-08-03T14:34:26.888852Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2511.22093","last_updated":"2026-07-09T15:18:10Z","snapshot_observed_at":"2026-08-20T21:01:45.047995Z","submitted_at":"2025-11-27T04:29:05Z","title":"Characterizing Binary Black Hole Subpopulations in GWTC-4 with Binned Gaussian Processes: On the Origins of the $35M_{\\odot}$ Peak","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2511.22093","snapshot_observed_at":"2026-08-03T14:34:26.960439Z","title":"& Kalogera, V","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:26.960439Z"},"links":{"cited_paper":"/paper/2511.22093","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:85cc3eb9e5e61d46ca682e2fbf79d92943bf28106deb2219756d36d4af4e436d","observation_id":"83ba99da-b143-41ed-8792-cc00b09bcc8b","resolution":{"observed_at":"2026-08-03T14:34:26.960439Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1206.5443","last_updated":"2012-12-12T07:15:34Z","snapshot_observed_at":"2026-08-17T19:24:35.225464Z","submitted_at":"2012-06-23T22:06:33Z","title":"Pre-Supernova Evolution of Massive Single and Binary Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.5443","snapshot_observed_at":"2026-08-03T14:34:27.120494Z","title":"Presupernova Evolution of Massive Single and Binary Stars.Annu","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:27.120494Z"},"links":{"cited_paper":"/paper/1206.5443","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:ab5c0a6b8f3871b9b699606fbee372a41f3410372889ac6cb38f970cee336040","observation_id":"d7a21fbd-77b9-47ba-8442-46847770b31e","resolution":{"observed_at":"2026-08-03T14:34:27.120494Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:27.285745Z","title":"As- trophys.659, A98 (2022).2111.03329","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:27.285745Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:bc26338cde40ca2e19632d0c1b2929c00c207da8b34721c6c24a647ea1fefe4a","observation_id":"42bcd8bc-43db-4b96-9b75-9ba341f9d1e0","resolution":{"observed_at":"2026-08-03T14:34:27.285745Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:27.350077Z","title":"T.et al.Populations of evolved massive binary stars in the Small Magellanic Cloud I: Predictions from detailed evolution models.arXiv e-printsarXiv:2503.23876 (2025)","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:27.350077Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:95d5557f5634338e1aa9412d323c73495bc630d1af99f94616632f5c44ec1c9f","observation_id":"9e20d4be-323d-42f9-9049-be2b2f041422","resolution":{"observed_at":"2026-08-03T14:34:27.350077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:27.403898Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:27.403898Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:f237a2367614e71aa25ab2afd8ecd1e85c5197c87bc6c6b86b8f9466cecaf821","observation_id":"c6d32849-3fda-4cca-90bb-87f6cff3faec","resolution":{"observed_at":"2026-08-03T14:34:27.403898Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1110.1726","last_updated":"2011-10-08T12:04:18Z","snapshot_observed_at":"2026-08-15T11:12:54.839110Z","submitted_at":"2011-10-08T12:04:18Z","title":"Compact Remnant Mass Function: Dependence on the Explosion Mechanism and Metallicity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.1726","snapshot_observed_at":"2026-08-03T14:34:27.473689Z","title":"L.et al.Compact Remnant Mass Function: Dependence on the Explosion Mechanism and Metallicity.Astrophys","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:27.473689Z"},"links":{"cited_paper":"/paper/1110.1726","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:aab6bf2013b3312ffe7d0edd1659d21046e9a6b0da44f0dbeaf502ccc7f334fa","observation_id":"a30ba52e-753d-432c-9c14-de2bbcb37bf6","resolution":{"observed_at":"2026-08-03T14:34:27.473689Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1306.0007","last_updated":"2013-05-31T20:00:02Z","snapshot_observed_at":"2026-08-15T00:15:38.214635Z","submitted_at":"2013-05-31T20:00:02Z","title":"Natal Kicks of Stellar-Mass Black Holes by Asymmetric Mass Ejection in Fallback Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1306.0007","snapshot_observed_at":"2026-08-03T14:34:27.541606Z","title":"Natal kicks of stellar mass black holes by asymmetric mass ejection in fallback supernovae.Mon","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:27.541606Z"},"links":{"cited_paper":"/paper/1306.0007","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:5dd57b7265d588494e2ee6cd4eff5591d09f0430f322ef61eb9b84d1a8e10025","observation_id":"0863dbb8-6247-4c41-b177-da613cd42718","resolution":{"observed_at":"2026-08-03T14:34:27.541606Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1107.5585","last_updated":"2012-01-04T20:16:26Z","snapshot_observed_at":"2026-08-15T04:39:44.892267Z","submitted_at":"2011-07-27T20:09:24Z","title":"Understanding Compact Object Formation and Natal Kicks. III. The case of Cygnus X-1","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1107.5585","snapshot_observed_at":"2026-08-03T14:34:27.629729Z","title":"& Kalogera, V","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:27.629729Z"},"links":{"cited_paper":"/paper/1107.5585","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:f18d41d767fd0d1d79afa3279099eacc50613d414cca71cb031ce097bead2e42","observation_id":"8a20129c-85fc-4c9b-bd74-7ea5df108a72","resolution":{"observed_at":"2026-08-03T14:34:27.629729Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.03871","last_updated":"2015-10-13T20:15:53Z","snapshot_observed_at":"2026-08-14T22:28:00.587096Z","submitted_at":"2015-10-13T20:15:53Z","title":"Estimates of black-hole natal kick velocities from observations of low-mass X-ray binaries","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.03871","snapshot_observed_at":"2026-08-03T14:34:27.743343Z","title":"Estimates of black hole natal kick velocities from observations of low-mass X-ray binaries.Mon","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:27.743343Z"},"links":{"cited_paper":"/paper/1510.03871","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:682b8b782d935edbd6f30de8bf4b38320dad7ad88aebf90ac3ac311ec7a47b63","observation_id":"dac0d3a9-9111-4255-aa9b-b8c30a1bf8fe","resolution":{"observed_at":"2026-08-03T14:34:27.743343Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.01509","last_updated":"2024-04-02T10:51:18Z","snapshot_observed_at":"2026-08-16T14:55:44.765953Z","submitted_at":"2023-10-02T18:04:38Z","title":"Constraints on neutrino natal kicks from black-hole binary VFTS 243","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.01509","snapshot_observed_at":"2026-08-03T14:34:27.813041Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:27.813041Z"},"links":{"cited_paper":"/paper/2310.01509","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:e0425aab538158edfb38d22fe3b3d71196397d53db7f2593abf7586479b4f305","observation_id":"baad1769-4178-4a67-9875-2830e1e58cc0","resolution":{"observed_at":"2026-08-03T14:34:27.813041Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.16669","last_updated":"2025-04-23T12:36:32Z","snapshot_observed_at":"2026-08-20T10:13:09.612484Z","submitted_at":"2025-04-23T12:36:32Z","title":"Binarity at LOw Metallicity (BLOeM): Bayesian inference of natal kicks from inert black hole binaries","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.16669","snapshot_observed_at":"2026-08-03T14:34:27.889066Z","title":"Astrophys.700, A59 (2025).2504.16669","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:27.889066Z"},"links":{"cited_paper":"/paper/2504.16669","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:f2bfc5dfa60975e5f4cdff75df273bdc6e8033e401130884064523a60e15edf5","observation_id":"5582facc-55c5-47b8-a741-7b3bee42ca5f","resolution":{"observed_at":"2026-08-03T14:34:27.889066Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:27.954699Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:27.954699Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:b0377f0e480eab46fdc419887a191cc90a30a45c4c933a0b0007e2e98e5d30c4","observation_id":"b03f5ab6-d7de-4469-bda1-32d84e8cd595","resolution":{"observed_at":"2026-08-03T14:34:27.954699Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.13957","last_updated":"2020-06-24T18:00:17Z","snapshot_observed_at":"2026-08-06T01:24:35.808199Z","submitted_at":"2020-06-24T18:00:17Z","title":"A spectroscopic multiplicity survey of Galactic Wolf-Rayet stars. I. The northern WC sequence","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.13957","snapshot_observed_at":"2026-08-03T14:34:27.993612Z","title":"& Marchant, P","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:27.993612Z"},"links":{"cited_paper":"/paper/2006.13957","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:84256698e3887d93df7bb52845e2e9d580e1ffe08d4565c2250b2fa7ff306d38","observation_id":"31fcac56-3aa7-4b8e-8fd8-c05affde312d","resolution":{"observed_at":"2026-08-03T14:34:27.993612Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.12518","last_updated":"2022-04-26T18:01:11Z","snapshot_observed_at":"2026-08-19T01:38:53.238354Z","submitted_at":"2022-04-26T18:01:11Z","title":"A spectroscopic multiplicity survey of Galactic Wolf-Rayet stars: II. The northern WNE sequence","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.12518","snapshot_observed_at":"2026-08-03T14:34:28.069107Z","title":"& Marchant, P","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:28.069107Z"},"links":{"cited_paper":"/paper/2204.12518","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:69354db5521df3d7ac44bb4b7973966cb061d4f4c750cd3d2cabfe4387e244da","observation_id":"b60a8f39-252b-45ab-a03c-2506da4ab317","resolution":{"observed_at":"2026-08-03T14:34:28.069107Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.06927","last_updated":"2022-12-13T22:48:47Z","snapshot_observed_at":"2026-08-18T18:30:34.894469Z","submitted_at":"2022-12-13T22:48:47Z","title":"A spectroscopic multiplicity survey of Galactic Wolf-Rayet stars. III. The northern late-type nitrogen-rich sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.06927","snapshot_observed_at":"2026-08-03T14:34:28.240315Z","title":"& Marchant, P","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:28.240315Z"},"links":{"cited_paper":"/paper/2212.06927","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:62e6ce5c87fb80954253da1f78e57938de724d8503ec0ba08b7e18fab9b65aef","observation_id":"10591be7-fe8f-4846-8652-104c49876c5c","resolution":{"observed_at":"2026-08-03T14:34:28.240315Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.01022","last_updated":"2016-04-04T20:00:00Z","snapshot_observed_at":"2026-08-14T22:03:07.732765Z","submitted_at":"2016-04-04T20:00:00Z","title":"Wolf-Rayet stars in the Small Magellanic Cloud: II. Analysis of the binaries","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.01022","snapshot_observed_at":"2026-08-03T14:34:28.350426Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:28.350426Z"},"links":{"cited_paper":"/paper/1604.01022","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:55a87f0e161cf90c07279495057fc3aae7e5a031a6c141a0bf2327f4cba94db8","observation_id":"ed400bae-07f4-489a-a6a5-6a92b9996d56","resolution":{"observed_at":"2026-08-03T14:34:28.350426Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.00952","last_updated":"2018-05-02T18:00:48Z","snapshot_observed_at":"2026-08-14T19:19:33.399001Z","submitted_at":"2018-05-02T18:00:48Z","title":"The Shortest-period Wolf-Rayet binary in the Small Magellanic Cloud: Part of a high-order multiple system","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.00952","snapshot_observed_at":"2026-08-03T14:34:28.509750Z","title":"Spectral and orbital analysis of SMC AB 6.As- tron","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:28.509750Z"},"links":{"cited_paper":"/paper/1805.00952","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:e618b7c3d913c994c56da459983d657378c03c6baa42f74221301fe24dced727","observation_id":"265b2b71-440f-47fe-b171-bc02b08cc227","resolution":{"observed_at":"2026-08-03T14:34:28.509750Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.08727","last_updated":"2018-02-07T11:42:12Z","snapshot_observed_at":"2026-08-14T20:29:48.579750Z","submitted_at":"2017-09-25T21:20:31Z","title":"Wolf-Rayet stars in the Small Magellanic Cloud as testbed for massive star evolution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.08727","snapshot_observed_at":"2026-08-03T14:34:28.656467Z","title":"& Langer, N","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:28.656467Z"},"links":{"cited_paper":"/paper/1709.08727","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:dde69a3443abc409b1f4a338edb7e3b5dcf7275750e1fdc8f73156c699558ce1","observation_id":"90e0de8b-03bd-4db6-9bc8-6302f0013d4e","resolution":{"observed_at":"2026-08-03T14:34:28.656467Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.03989","last_updated":"2023-03-07T15:40:22Z","snapshot_observed_at":"2026-08-16T15:50:06.299382Z","submitted_at":"2023-03-07T15:40:22Z","title":"Spectroscopic and evolutionary analyses of the binary system AzV 14 outline paths toward the WR stage at low metallicity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.03989","snapshot_observed_at":"2026-08-03T14:34:28.765491Z","title":"Astrophys.673, A40 (2023)","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:28.765491Z"},"links":{"cited_paper":"/paper/2303.03989","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:1eb0be4b8b4ae0cbf2975df3650e9225eea2d8b167750487c9c6f36be30861f6","observation_id":"bb7a033a-70da-415a-9f81-41c852755197","resolution":{"observed_at":"2026-08-03T14:34:28.765491Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:28.937721Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:28.937721Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:0e2d9edf37d7e9e8125d482398e2ec95b54335b19453838eedcd2a0b964b727d","observation_id":"965eed60-68dd-404a-a5a0-3dfb403f13d3","resolution":{"observed_at":"2026-08-03T14:34:28.937721Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:29.086859Z","title":"A.et al.A new dynamical model for the black hole binary lmc x-1*.The Astro- physical Journal697, 573 (2009)","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:29.086859Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:1aa8ca0e282829eb7227d7035b4daac5b9af633cf55f517d7a1cd55a31b1d63f","observation_id":"729a1c33-edf1-4310-b670-c23493ea8929","resolution":{"observed_at":"2026-08-03T14:34:29.086859Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.07773","last_updated":"2022-08-16T14:36:34Z","snapshot_observed_at":"2026-08-16T16:38:54.050718Z","submitted_at":"2022-08-16T14:36:34Z","title":"Phase-resolved spectroscopic analysis of the eclipsing black hole X-ray binary M33 X-7: System properties, accretion, and evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.07773","snapshot_observed_at":"2026-08-03T14:34:29.235471Z","title":"Astrophys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:29.235471Z"},"links":{"cited_paper":"/paper/2208.07773","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:222c0727170b8954f770dade26bd1e12b9d12a1027807e7d80149c07df698e11","observation_id":"a33f779b-277f-4a6e-b602-ae47c3820bce","resolution":{"observed_at":"2026-08-03T14:34:29.235471Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1208.5455","last_updated":"2012-11-14T14:30:11Z","snapshot_observed_at":"2026-08-15T00:48:44.072224Z","submitted_at":"2012-08-27T17:46:08Z","title":"Cyg X-3: a low-mass black hole or a neutron star","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.5455","snapshot_observed_at":"2026-08-03T14:34:29.348888Z","title":"A., Mikolajewska, J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:29.348888Z"},"links":{"cited_paper":"/paper/1208.5455","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:4e9701d286790bd7fdb938a7df50fededa4534a68f05dedff4f8d00ab0488a2b","observation_id":"5b4b1511-731e-4fb8-96a8-dbbb9889259b","resolution":{"observed_at":"2026-08-03T14:34:29.348888Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/abe6a9","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"A.et al.The wolf–rayet+black hole binary ngc 300 x-1: What is the mass of the black hole?The Astrophysical Journal910, 74 (2021)","venue":"The Astrophysical Journal","work_id":"f4629064-c475-483b-967f-cd301106368d","year":2021},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:29.490112Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:da0eecca8468dabf70d9dd4f0b6d338dc95ae146f507a1de088dd33d106f1d0b","observation_id":"f64172db-5943-45d2-b9c4-0d70a86c92de","resolution":{"observed_at":"2026-08-03T14:38:32.697196Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1410.3417","last_updated":"2014-10-13T18:09:14Z","snapshot_observed_at":"2026-08-14T23:15:55.269100Z","submitted_at":"2014-10-13T18:09:14Z","title":"Chandra and XMM Monitoring of the Black Hole X-ray Binary IC 10 X-1","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1410.3417","snapshot_observed_at":"2026-08-03T14:34:29.626993Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:29.626993Z"},"links":{"cited_paper":"/paper/1410.3417","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:e14d6e2addf01454be3807aef748c217c440e2fbc750d133f5c88d7ec0df04d8","observation_id":"751d8e7b-8479-4e44-a84e-441573187914","resolution":{"observed_at":"2026-08-03T14:34:29.626993Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2509.04637","last_updated":"2026-05-07T12:03:49Z","snapshot_observed_at":"2026-08-15T02:23:59.704429Z","submitted_at":"2025-09-04T19:55:47Z","title":"Gravitational-wave constraints on the pair-instability mass gap and nuclear burning in massive stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.04637","snapshot_observed_at":"2026-08-03T14:34:29.875365Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:29.875365Z"},"links":{"cited_paper":"/paper/2509.04637","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:0aad5674c3575237b762555086a2e5d387340f81134fab738a3fc1f47b7e69e1","observation_id":"41e811c8-313d-481c-8d9c-739865d86002","resolution":{"observed_at":"2026-08-03T14:34:29.875365Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:30.126948Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:30.126948Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:733924c28a2f92f34e951d06edfb17bf72049f45c35663331ad13c3ac9abbd07","observation_id":"da7657ac-b906-42a6-82da-f7fb0f4c62e1","resolution":{"observed_at":"2026-08-03T14:34:30.126948Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2509.15646","last_updated":"2026-05-29T08:49:39Z","snapshot_observed_at":"2026-08-15T15:48:11.554468Z","submitted_at":"2025-09-19T06:14:08Z","title":"Evidence for Three Subpopulations of Merging Binary Black Holes at Different Primary Masses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.15646","snapshot_observed_at":"2026-08-03T14:34:30.342053Z","title":"& Lasky, P","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:30.342053Z"},"links":{"cited_paper":"/paper/2509.15646","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:08d7f20a927fb53c171eba4f803f5e3cc6b535dc99bc66a6c2522fad7800692e","observation_id":"4823815b-fd5c-4e6c-8f00-9a79730044b6","resolution":{"observed_at":"2026-08-03T14:34:30.342053Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.07294","last_updated":"2020-01-06T19:15:19Z","snapshot_observed_at":"2026-08-17T13:08:44.959660Z","submitted_at":"2019-12-16T11:21:03Z","title":"Effects of close binary evolution on the main-sequence morphology of young star clusters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.07294","snapshot_observed_at":"2026-08-03T14:34:30.500956Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:30.500956Z"},"links":{"cited_paper":"/paper/1912.07294","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:df4dd68bc385db885cf825d84ac0ae56f391f7870d0fcef6e0ef38d308579537","observation_id":"b1a502c0-5300-4794-aab3-c7101eb5ee8e","resolution":{"observed_at":"2026-08-03T14:34:30.500956Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0512271","last_updated":"2005-12-11T09:22:59Z","snapshot_observed_at":"2026-08-15T10:18:25.375076Z","submitted_at":"2005-12-11T09:22:59Z","title":"On the Collapsar Model of Long Gamma-Ray Bursts: Constraints from Cosmic Metallicity Evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0512271","snapshot_observed_at":"2026-08-03T14:34:30.604044Z","title":"& Norman, C","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:30.604044Z"},"links":{"cited_paper":"/paper/astro-ph/0512271","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:34ede8a97af7c2e660f157109d031c66a18d12c3085a008e2f46333fa2f13df4","observation_id":"9ef85bc4-97d9-4af7-bdff-3b7d3ce44dbc","resolution":{"observed_at":"2026-08-03T14:34:30.604044Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:30.833639Z","title":"& Kobulnicky, H","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:30.833639Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:f74f7e4e7fd673770f1e1d619e02a956952524ca208c02ec740e41774731c063","observation_id":"d8ca0e82-3915-4ea3-93ae-17e93a8b2ec8","resolution":{"observed_at":"2026-08-03T14:34:30.833639Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:31.034635Z","title":"Evolution of massive stars in the Large Magellanic Cloud : models with semiconvection.Astron","venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:31.034635Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:92e91b509f679bc4088eb167cad75e6eb7851d3ea43d47f7384c8a7dda69355c","observation_id":"d6172a83-b524-468c-a90b-a0e169e1752a","resolution":{"observed_at":"2026-08-03T14:34:31.034635Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0005110","last_updated":"2000-05-05T22:26:05Z","snapshot_observed_at":"2026-07-07T00:11:08.288397Z","submitted_at":"2000-05-05T22:26:05Z","title":"Presupernova Evolution of Rotating Massive Stars II: -- Evolution of the Surface Properties","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0005110","snapshot_observed_at":"2026-08-03T14:34:31.157612Z","title":"& Langer, N","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:31.157612Z"},"links":{"cited_paper":"/paper/astro-ph/0005110","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:94dedb394388464b29cb3147e7275d117a35369e67a1f1f78a089e9208cb9794","observation_id":"736acfac-048e-4e65-83e3-5e4753586576","resolution":{"observed_at":"2026-08-03T14:34:31.157612Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:31.244746Z","title":"S.The Internal Constitution of the Stars( Cambridge University Press, 1926)","venue":null,"work_id":null,"year":1926},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:31.244746Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:cc7dc2e02f401db21ab972920ac68a6009dd2d6b839ef454adb355d7de705ded","observation_id":"88c4b283-0509-41ed-9ad6-6d01e23fea20","resolution":{"observed_at":"2026-08-03T14:34:31.244746Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:31.355226Z","title":"& Schubert, G","venue":null,"work_id":null,"year":1967},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:31.355226Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:cc849319ea3fb0314f3c6e7676d679362152ffe2ea4fcad4e1148a17aac8e150","observation_id":"72fa99e6-c93e-4ec4-bc88-637cd53315e1","resolution":{"observed_at":"2026-08-03T14:34:31.355226Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:31.525913Z","title":"Instabilit ¨at station¨arer Rotation in Sternen.Zeitschrift f¨ ur Astrophysik68, 317 (1968)","venue":null,"work_id":null,"year":1968},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:31.525913Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:ff4720f4cb06cfbf2aad0c257a3dca56602f38622f2ac4fad5a710a743e2cf2f","observation_id":"244238ba-6e3f-40c8-b4c1-93b893ba4788","resolution":{"observed_at":"2026-08-03T14:34:31.525913Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:31.692990Z","title":null,"venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:31.692990Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:2965514e3a68f3f4c4af14fff04b4beaa04e7be37d5d45dbbf212aa8339f1fd8","observation_id":"46817496-2701-48f2-af3b-9ed1c6c989ea","resolution":{"observed_at":"2026-08-03T14:34:31.692990Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:31.782742Z","title":"Stellar evolution with rotation","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:31.782742Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:89f15d9c9b00171c7c21213ad9aba20c817f60e85b0e5cda19d9329b36df78d8","observation_id":"89d8767a-9fac-4d60-a03f-ea5bf68df46c","resolution":{"observed_at":"2026-08-03T14:34:31.782742Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0108207","last_updated":"2001-11-09T12:51:15Z","snapshot_observed_at":"2026-07-07T00:20:35.294349Z","submitted_at":"2001-08-12T21:17:36Z","title":"Dynamo action by differential rotation in a stably stratified stellar interior","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0108207","snapshot_observed_at":"2026-08-03T14:34:31.938197Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:31.938197Z"},"links":{"cited_paper":"/paper/astro-ph/0108207","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:22e58219d4f694b65de1582686d01cbb6b81f597116f2af88b007afebd3b1ac9","observation_id":"71e39f5c-0684-44dc-a122-4c5800f9b47b","resolution":{"observed_at":"2026-08-03T14:34:31.938197Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0008183","last_updated":"2000-08-11T14:01:35Z","snapshot_observed_at":"2026-07-07T00:12:33.114135Z","submitted_at":"2000-08-11T14:01:35Z","title":"New theoretical Mass-loss rates of O and B Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0008183","snapshot_observed_at":"2026-08-03T14:34:32.097539Z","title":"S., de Koter, A","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:32.097539Z"},"links":{"cited_paper":"/paper/astro-ph/0008183","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:533ae2d237996936e1bd2b9d2d24807b6d44859ef32acf7f7a505ae499c97c60","observation_id":"13b27bf4-e957-487c-b803-de4d5fde24b3","resolution":{"observed_at":"2026-08-03T14:34:32.097539Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:32.195439Z","title":"S., de Koter, A","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:32.195439Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:3725ad3ad6ceae09f9d1b67df297ee72d29745c4dbf8530e612d99fda048868c","observation_id":"534e4626-334b-4d93-aa10-8dfee6005d89","resolution":{"observed_at":"2026-08-03T14:34:32.195439Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9908196","last_updated":"1999-08-18T09:30:04Z","snapshot_observed_at":"2026-08-20T02:08:52.381014Z","submitted_at":"1999-08-18T09:30:04Z","title":"On the nature of the bi-stability jump in the winds of early-type supergiants","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9908196","snapshot_observed_at":"2026-08-03T14:34:32.304930Z","title":"S., de Koter, A","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:32.304930Z"},"links":{"cited_paper":"/paper/astro-ph/9908196","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:86daa2c1962d6f07cef1477339661532f1957de144504db5dc1d57a794802c24","observation_id":"ed860e66-8a6c-4866-826e-a665964a9018","resolution":{"observed_at":"2026-08-03T14:34:32.304930Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:32.428022Z","title":"R., Koesterke, L","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:32.428022Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:ba1b2a623e869c2b5492864e74b05737c8a32e4f848522ba4cf77646d8b8640c","observation_id":"02952118-67dc-454f-9280-2ff2eb0630de","resolution":{"observed_at":"2026-08-03T14:34:32.428022Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T14:34:32.533103Z","title":null,"venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":101,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:32.533103Z"},"links":{"citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:e577b44f2d9837eb2c02f8f86c4d868891658cdafb3bab48ba8028be33019003","observation_id":"4b8e643f-094b-4c62-bef9-bafc89c3d09e","resolution":{"observed_at":"2026-08-03T14:34:32.533103Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","latest_version":2,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-14T11:48:00.367296Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":98,"verified_exact":1,"verified_fuzzy":0},"total_outbound_references":169},"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":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"thesis":"As of 22 August 2026, this Paper Citation Record lists 100 of 169 outbound references and 5 inbound Pith citation observations for arXiv:2512.20054."}