{"as_of":"2026-08-16T23:29:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:8dcfc00d1bc98e51022cda9f0179270744f7f1510b77b54314d2815afc3924d9","coverage":[{"denominator":24,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":24,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T17:11:32.171566Z","state":"measured"},{"denominator":24,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":24,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2507.11786/citation-record","integrity":"/paper/2507.11786/integrity","json":"/paper/2507.11786/citation-record.json","paper":"/paper/2507.11786"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2310.01231","last_updated":"2023-10-02T14:22:34Z","snapshot_observed_at":"2026-08-16T14:55:50.926387Z","submitted_at":"2023-10-02T14:22:34Z","title":"Jupiter Mass Binary Objects in the Trapezium Cluster","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.01231","snapshot_observed_at":"2026-08-06T17:11:32.067933Z","title":"arXiv e-prints, 2310–01231 (2023) https://doi.org/10.48550/arXiv","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.067933Z"},"links":{"cited_paper":"/paper/2310.01231","citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:ec748a54abf9062719b91850cc0d78ec76d3fcdfc8e58165c86a68dfc59660a9","observation_id":"05988e54-b1ed-4889-bc9f-948bdadd2f36","resolution":{"observed_at":"2026-08-06T17:11:32.067933Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.06016","last_updated":"2024-05-02T19:09:27Z","snapshot_observed_at":"2026-08-16T14:53:43.352156Z","submitted_at":"2023-10-09T18:00:00Z","title":"Floating binary planets from ejections during close stellar encounters","version":3},"cited_work":{"arxiv_id":"2310.06016","doi":null,"metadata_source":"pith","pith_arxiv_id":"2310.06016","snapshot_observed_at":"2026-08-06T17:11:32.476409Z","title":"Floating binary planets from ejections during close stellar encounters","venue":"astro-ph.EP","work_id":"73f8acc6-7536-4462-8c6a-ef3738643cc3","year":2023},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.073625Z"},"links":{"cited_paper":"/paper/2310.06016","citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:a07b2c8648b3eff2920f17ee3aa131901a8b2fc01be8c4e27c331f740b859646","observation_id":"2760aa20-cffa-46b5-9946-0f7833aafac5","resolution":{"observed_at":"2026-08-06T17:11:32.481680Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.21468/scipostastro.3.1.001","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"SciPost Astronomy3(1), 001 (2024) https: //doi.org/10.21468/SciPostAstro.3.1.001","venue":"SciPost Astronomy","work_id":"87fbdc10-9539-4f9a-9457-19b0a375e21d","year":2024},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.079184Z"},"links":{"citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:3a37958969b8e09c8656c73aaf322cff76133acaa0fd549c829bb3aa1e512eaf","observation_id":"112ce383-43bc-4730-b087-e911c1736a48","resolution":{"observed_at":"2026-08-06T17:11:32.245792Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2403.07224","last_updated":"2024-07-12T00:52:57Z","snapshot_observed_at":"2026-08-16T14:10:46.617122Z","submitted_at":"2024-03-12T00:32:59Z","title":"Free-Floating Planets, Survivor Planets, Captured Planets and Binary Planets from Stellar Flybys","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.07224","snapshot_observed_at":"2026-08-06T17:11:32.083322Z","title":"ApJ 970(1), 97 (2024) https://doi.org/10","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.083322Z"},"links":{"cited_paper":"/paper/2403.07224","citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:69b9f53f63540e7af27fbf52f917925cc50a6c368018e2b3d9ce173c67d77a77","observation_id":"e288e8e0-654f-4928-afcb-183a27cdb1f6","resolution":{"observed_at":"2026-08-06T17:11:32.083322Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:11:32.547754Z","title":"MNRAS 322, 231–246 (2001)","venue":null,"work_id":"624b66f2-78f1-4e10-83e9-d99352e9820e","year":2001},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.087688Z"},"links":{"citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:e0c8cb2ea7863a5666a7f1f1cb2f805c35d439b6b406cd54586d0332a14fe374","observation_id":"4cd5dcb9-9276-49be-af50-cdeb6a568ee0","resolution":{"observed_at":"2026-08-06T17:11:32.552674Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:11:32.537522Z","title":"ApJ 492, 540–553 (1998) https://doi.org/10","venue":null,"work_id":"a490f746-bfad-478e-be5c-b3c4801fd730","year":1998},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.092247Z"},"links":{"citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:fa1b71664c5ca62177b4867e2d5574608b2a62b33a865720ad8808d8f4d11558","observation_id":"485d2239-692f-42c1-b51c-c1098985f51d","resolution":{"observed_at":"2026-08-06T17:11:32.541142Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:11:32.097362Z","title":"I - Numerical experiments for equal masses","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.097362Z"},"links":{"citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:a24a6520581914c208b0f7d2e806143bac378e61f70d0e593d0615004a5e6283","observation_id":"7cd26bcd-4228-46bd-89cf-709ece337d8a","resolution":{"observed_at":"2026-08-06T17:11:32.097362Z","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":"2026-08-06T17:11:32.102319Z","title":"AJ 95, 1755 (1988) https://doi.org/10.1086/114773","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.102319Z"},"links":{"citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:4aaa854bc9cdb01c5447c2589b85db30f51ef7fd8e93cb3341d6647913af8d88","observation_id":"4099930f-55ec-4239-ae0a-be4cafa07a83","resolution":{"observed_at":"2026-08-06T17:11:32.102319Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0506585","last_updated":"2005-06-24T12:42:56Z","snapshot_observed_at":"2026-08-12T16:02:35.845356Z","submitted_at":"2005-06-24T12:42:56Z","title":"Size distribution of circumstellar disks in the Trapezium cluster","version":1},"cited_work":{"arxiv_id":"astro-ph/0506585","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0506585","snapshot_observed_at":"2026-08-06T17:11:32.446226Z","title":"Size distribution of circumstellar disks in the Trapezium cluster","venue":"astro-ph","work_id":"f63f1c60-e3d7-424f-85a2-5459e1a4dfc8","year":2005},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.106801Z"},"links":{"cited_paper":"/paper/astro-ph/0506585","citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:e31d51c42fe9372cda6685ef786afadca5815be0811f31ae55bc90f8488e76d3","observation_id":"7da1c2c4-0ff9-4d00-8fb8-f00b1e46aad9","resolution":{"observed_at":"2026-08-06T17:11:32.451386Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.04045","last_updated":"2017-11-10T23:58:29Z","snapshot_observed_at":"2026-08-14T20:14:45.482704Z","submitted_at":"2017-11-10T23:58:29Z","title":"Measurement of Circumstellar Disk Sizes in the Upper Scorpius OB Association with ALMA","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.04045","snapshot_observed_at":"2026-08-06T17:11:32.111280Z","title":"ApJ 851(2), 85 (2017) https://doi.org/10.3847/1538-4357/aa989d arXiv:1711.04045 [astro-ph.SR]","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.111280Z"},"links":{"cited_paper":"/paper/1711.04045","citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:fb523b21099343ba40153d2b9ed4bc0d74910a9d2afdbcac4ab8d77aeaf04889","observation_id":"ac7d8108-8876-4f88-b6fb-5009d1d0c8e6","resolution":{"observed_at":"2026-08-06T17:11:32.111280Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.04365","last_updated":"2024-02-06T16:20:39Z","snapshot_observed_at":"2026-08-16T14:45:08.100645Z","submitted_at":"2023-11-07T21:59:34Z","title":"Formation of wide-orbit giant planets in protoplanetary disks with a decreasing pebble flux","version":2},"cited_work":{"arxiv_id":"2311.04365","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.04365","snapshot_observed_at":"2026-08-06T17:11:32.417036Z","title":"Formation of wide-orbit giant planets in protoplanetary disks with a decreasing pebble flux","venue":"astro-ph.EP","work_id":"181b975f-acb2-4ee6-8e5d-f7f7a0d24e36","year":2023},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.115794Z"},"links":{"cited_paper":"/paper/2311.04365","citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:631ce6951ffacb59bfe4dc950b52f363c3f1306231ace2dfb66692db54a5115b","observation_id":"8c5a030b-76bf-4a27-a7cd-9fda73e1cebe","resolution":{"observed_at":"2026-08-06T17:11:32.422082Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:11:32.119831Z","title":"Computer Physics Communications 184, 456–468 (2013) https://doi","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.119831Z"},"links":{"citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:9ddc9dfcaf125944e925c17c14dca15930bb89e8944640a0f5cb10b7b10f59c2","observation_id":"a09ff9bf-ae84-4091-b9f1-8add91f016dd","resolution":{"observed_at":"2026-08-06T17:11:32.119831Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:11:32.526711Z","title":"MNRAS 71, 460–470 (1911) 7","venue":null,"work_id":"d0130162-842a-4e66-8789-f4a815a952c8","year":1911},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.124227Z"},"links":{"citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:7192ebd0c4cd71aec5831bbfb22dc0305bc833101beed8f9d4338091950e5a74","observation_id":"5f985052-013a-46a0-89ca-ed66d17cb675","resolution":{"observed_at":"2026-08-06T17:11:32.530430Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0610039","last_updated":"2006-10-02T14:06:53Z","snapshot_observed_at":"2026-08-15T11:01:42.560574Z","submitted_at":"2006-10-02T14:06:53Z","title":"The minimum mass for star formation, and the origin of binary brown dwarfs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0610039","snapshot_observed_at":"2026-08-06T17:11:32.128826Z","title":"A&A 458(3), 817–829 (2006) https://doi","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.128826Z"},"links":{"cited_paper":"/paper/astro-ph/0610039","citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:9a6c97e48d1f7e2df5bdef9ea0d20dbc420d9f679814d1b922f0d4a4bc8a71e6","observation_id":"e71656b5-4e96-4fbd-ac77-2cee26e2147a","resolution":{"observed_at":"2026-08-06T17:11:32.128826Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.05772","last_updated":"2016-08-24T23:03:26Z","snapshot_observed_at":"2026-08-14T21:56:46.294600Z","submitted_at":"2016-05-18T22:07:12Z","title":"ALMA Observations of Circumstellar Disks in the Upper Scorpius OB Association","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.05772","snapshot_observed_at":"2026-08-06T17:11:32.133154Z","title":"ApJ 827(2), 142 (2016) https://doi.org/10.3847/0004-637X/827/2/142 arXiv:1605.05772 [astro-ph.EP]","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.133154Z"},"links":{"cited_paper":"/paper/1605.05772","citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:ce43443853f6d9b7bf18c8d33540acaee463d6eb53fe666e916bc298aacff070","observation_id":"b6f58008-6d30-4a36-9181-eed426f7cbc0","resolution":{"observed_at":"2026-08-06T17:11:32.133154Z","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":"10.5281/z","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:11:32.209078Z","title":"Zenodo (2018)","venue":null,"work_id":"9ca84b1a-bbb1-400a-9e83-6b44a0572e38","year":2018},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.137690Z"},"links":{"citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:168b62af157263255a72d3e9b7d2ab094c68688535d5c9997fbd13a380e58939","observation_id":"4f5685be-92c0-4360-8c36-c3b9e46ad5dd","resolution":{"observed_at":"2026-08-06T17:11:32.214384Z","resolver_source":"doi_truncated","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0310333","last_updated":"2003-10-13T17:03:27Z","snapshot_observed_at":"2026-07-07T00:37:16.792675Z","submitted_at":"2003-10-13T17:03:27Z","title":"The dynamical evolution of fractal star clusters: the survival of substructure","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0310333","snapshot_observed_at":"2026-08-06T17:11:32.142200Z","title":"A&A 413, 929–937 (2004) https://doi.org/10","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.142200Z"},"links":{"cited_paper":"/paper/astro-ph/0310333","citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:cfadbb5987c4719f4e35bb5deb4ee4d5ea5ac32ef842bb2c52001fafeada3519","observation_id":"ffdbcde9-60ae-4986-a764-73a10fef8443","resolution":{"observed_at":"2026-08-06T17:11:32.142200Z","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":"2026-08-06T17:11:32.146759Z","title":"Computing in Science Engineering 13(2), 22–30 (2011) https://doi.org/10.1109/MCSE.2011.37","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.146759Z"},"links":{"citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:b46bfe666826a410286e4d93eb37ee81454ba0b4024de09c3a48a88485f51241","observation_id":"272823e2-6536-4bdf-a3b4-db20decfd365","resolution":{"observed_at":"2026-08-06T17:11:32.146759Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.11012","last_updated":"2021-11-17T08:57:42Z","snapshot_observed_at":"2026-08-16T17:54:44.466060Z","submitted_at":"2021-09-22T20:00:17Z","title":"Chaos in self-gravitating many-body systems: Lyapunov time dependence of $N$ and the influence of general relativity","version":2},"cited_work":{"arxiv_id":"2109.11012","doi":null,"metadata_source":"pith","pith_arxiv_id":"2109.11012","snapshot_observed_at":"2026-08-06T17:11:32.366863Z","title":"Chaos in self-gravitating many-body systems: Lyapunov time dependence of $N$ and the influence of general relativity","venue":"nlin.CD","work_id":"f7b4f483-ff3b-4131-8b51-90983d392973","year":2021},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.150932Z"},"links":{"cited_paper":"/paper/2109.11012","citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:c9d4344d705a5b57c31cfa1c9aa7f2ee8cd0fb8a1dcf17d7278331aacdccc7c4","observation_id":"c20176e4-b053-4473-a334-c70496122277","resolution":{"observed_at":"2026-08-06T17:11:32.372011Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:11:32.155721Z","title":"Computing in Science and Engineering 9, 90–95 (2007) https://doi.org/10.1109/MCSE.2007.55","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.155721Z"},"links":{"citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:c7a17166e2896f85c210c2adf5637ed507f128a91c1d56891d15b70982959af6","observation_id":"f05fc701-2d9e-4833-9ef0-1cafb97a9896","resolution":{"observed_at":"2026-08-06T17:11:32.155721Z","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":"2026-08-06T17:11:32.159834Z","title":"CreateSpace, Scotts Valley, CA (2009)","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.159834Z"},"links":{"citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:74e5699016dbf8444550d106a79170f1ec3a9637b15f86e617926c16b504694a","observation_id":"4dd07dea-2900-46ae-ad05-e2034012902c","resolution":{"observed_at":"2026-08-06T17:11:32.159834Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:11:32.504740Z","title":"A&A 309, 179–196 (1996)","venue":null,"work_id":"db83ec53-0f23-4439-83ee-27ebeb113f27","year":1996},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.163850Z"},"links":{"citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:1466ad8a9f76d26eea8cfc17ec17fbef74bad62322268467e39c0357aa81d61c","observation_id":"eb464f44-4ca2-4362-be19-78eaf8db9b80","resolution":{"observed_at":"2026-08-06T17:11:32.509730Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:11:32.491249Z","title":"http://www.scipy.org/","venue":null,"work_id":"8f99f095-a0f6-4d18-93e5-fdb8e7ae5fdd","year":2001},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.168194Z"},"links":{"citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:58c6490abaab8d8f285a75bf51b38654c848375fde6c8a61b93b02c83c3393ef","observation_id":"dbacf13f-2633-4536-9030-66dff9b110dd","resolution":{"observed_at":"2026-08-06T17:11:32.495949Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T17:11:32.171566Z","title":"Dissection of an open star cluster: spectroscopy","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T17:11:32.171566Z"},"links":{"citing_paper":"/paper/2507.11786"},"observation_digest":"sha256:9560b12a767c252bb28ab8259220007b97333c5c6f6a28a1143367521bd4c4bb","observation_id":"e0f30d9c-6d2f-4e76-ae1a-7d04b4758ba3","resolution":{"observed_at":"2026-08-06T17:11:32.171566Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2507.11786","last_updated":"2025-07-15T23:03:36Z","latest_version":1,"primary_category":"astro-ph.EP","snapshot_observed_at":"2026-08-10T08:12:26.241201Z","submitted_at":"2025-07-15T23:03:36Z","title":"Why Wide Jupiter-Mass Binary-Objects Cannot Form"},"reference_resolution":{"displayed":24,"state_counts":{"malformed_identifier":1,"metadata_mismatch":3,"parse_uncertain":0,"unresolved":13,"verified_exact":2,"verified_fuzzy":5},"total_outbound_references":24},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 24 of 24 outbound references and 0 inbound Pith citation observations for arXiv:2507.11786."}