{"as_of":"2026-08-12T20:07:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c0873f45767bf7eb635d6e9da11e3e57fe51612e53e43b4aa795914ff0fffa7f","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":10,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":10,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":10,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":10,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T19:45:09.527204Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-06-30T16:24:58.956638Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2108.01284","last_updated":"2021-10-19T20:47:09Z","snapshot_observed_at":"2026-08-05T12:37:14.416607Z","submitted_at":"2021-08-03T04:11:04Z","title":"Signs of eccentricity in two gravitational-wave signals may indicate a sub-population of dynamically assembled binary black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.01284","snapshot_observed_at":"2026-08-11T19:45:09.527204Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.06433","last_updated":"2025-02-04T11:05:33Z","snapshot_observed_at":"2026-08-11T19:37:33.313791Z","submitted_at":"2024-12-09T12:21:00Z","title":"A geometric template bank for the detection of spinning low-mass compact binaries with moderate orbital eccentricity","version":3},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-11T19:45:09.527204Z"},"links":{"cited_paper":"/paper/2108.01284","citing_paper":"/paper/2412.06433"},"observation_digest":"sha256:fd2f55a49f81c52445ce1cd82a51dfe7c6a029b368fc082958b1113b1f451a35","observation_id":"4ee93477-ccc8-4bd6-9a88-00d34a2e362d","resolution":{"observed_at":"2026-08-11T19:45:09.527204Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.01284","last_updated":"2021-10-19T20:47:09Z","snapshot_observed_at":"2026-08-05T12:37:14.416607Z","submitted_at":"2021-08-03T04:11:04Z","title":"Signs of eccentricity in two gravitational-wave signals may indicate a sub-population of dynamically assembled binary black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.01284","snapshot_observed_at":"2026-08-11T14:41:19.170933Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.11749","last_updated":"2025-08-08T11:13:24Z","snapshot_observed_at":"2026-08-11T20:49:53.995756Z","submitted_at":"2024-12-16T13:06:44Z","title":"Inferring additional physics through unmodelled signal reconstructions","version":3},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-11T14:41:19.170933Z"},"links":{"cited_paper":"/paper/2108.01284","citing_paper":"/paper/2412.11749"},"observation_digest":"sha256:d15bec679f5581b07ff01989c8a56ab32d2d2d4ef2b9ce7b41b55203866d3534","observation_id":"93abf1b2-607b-4f04-a3db-14a70713f145","resolution":{"observed_at":"2026-08-11T14:41:19.170933Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.01284","last_updated":"2021-10-19T20:47:09Z","snapshot_observed_at":"2026-08-05T12:37:14.416607Z","submitted_at":"2021-08-03T04:11:04Z","title":"Signs of eccentricity in two gravitational-wave signals may indicate a sub-population of dynamically assembled binary black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.01284","snapshot_observed_at":"2026-08-11T13:49:12.958911Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.12823","last_updated":"2025-08-21T18:54:24Z","snapshot_observed_at":"2026-08-11T13:39:17.730415Z","submitted_at":"2024-12-17T11:42:40Z","title":"Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM","version":2},"reference_index":107,"source":"pdf_text","source_observed_at":"2026-08-11T13:49:12.958911Z"},"links":{"cited_paper":"/paper/2108.01284","citing_paper":"/paper/2412.12823"},"observation_digest":"sha256:c15803697232dbef1a1fd9765c810eb9617feae71e02e914cbc9c4675b5ab986","observation_id":"9cca575c-3ef6-4fc7-a565-7ba6d0dbbdb8","resolution":{"observed_at":"2026-08-11T13:49:12.958911Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.01284","last_updated":"2021-10-19T20:47:09Z","snapshot_observed_at":"2026-08-05T12:37:14.416607Z","submitted_at":"2021-08-03T04:11:04Z","title":"Signs of eccentricity in two gravitational-wave signals may indicate a sub-population of dynamically assembled binary black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.01284","snapshot_observed_at":"2026-08-07T05:02:46.255500Z","title":"Romero-Shaw, P","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.09140","last_updated":"2025-08-08T07:52:21Z","snapshot_observed_at":"2026-08-10T03:14:43.767781Z","submitted_at":"2025-06-10T18:00:46Z","title":"Dissecting environmental effects with eccentric gravitational wave sources","version":3},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-07T05:02:46.255500Z"},"links":{"cited_paper":"/paper/2108.01284","citing_paper":"/paper/2506.09140"},"observation_digest":"sha256:79696ad15b3df6bb1e73db15bf32294763dc0c5bc836ef2b09c5c9848b906775","observation_id":"ee8dd180-843d-4415-90c6-2b59251f7f1c","resolution":{"observed_at":"2026-08-07T05:02:46.255500Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.01284","last_updated":"2021-10-19T20:47:09Z","snapshot_observed_at":"2026-08-05T12:37:14.416607Z","submitted_at":"2021-08-03T04:11:04Z","title":"Signs of eccentricity in two gravitational-wave signals may indicate a sub-population of dynamically assembled binary black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.01284","snapshot_observed_at":"2026-08-04T13:34:53.933979Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2510.00116","last_updated":"2026-07-21T22:58:27Z","snapshot_observed_at":"2026-08-09T19:02:57.611707Z","submitted_at":"2025-09-30T18:00:25Z","title":"Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates","version":3},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-04T13:34:53.933979Z"},"links":{"cited_paper":"/paper/2108.01284","citing_paper":"/paper/2510.00116"},"observation_digest":"sha256:036a4cc8e15f930c4a580f4fcdc0921db1f24ae001a54f45bfd14ffb789c4bd9","observation_id":"49b666a8-8d1a-481e-b449-7b892bc2d8d8","resolution":{"observed_at":"2026-08-04T13:34:53.933979Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.01284","last_updated":"2021-10-19T20:47:09Z","snapshot_observed_at":"2026-08-05T12:37:14.416607Z","submitted_at":"2021-08-03T04:11:04Z","title":"Signs of eccentricity in two gravitational-wave signals may indicate a sub-population of dynamically assembled binary black holes","version":2},"cited_work":{"arxiv_id":"2108.01284","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2108.01284","snapshot_observed_at":"2026-06-30T16:24:58.956638Z","title":"Romero-Shaw, P","venue":null,"work_id":"a1ad3edc-3ba4-4a5e-85f1-f967f5cb2ac0","year":2021},"citing_paper":{"arxiv_id":"2602.11030","last_updated":"2026-05-14T13:56:54Z","snapshot_observed_at":"2026-08-11T02:43:12.290359Z","submitted_at":"2026-02-11T16:55:29Z","title":"Population Properties of Binary Black Holes with Eccentricity","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-05-16T02:28:53.190725Z"},"links":{"cited_paper":"/paper/2108.01284","citing_paper":"/paper/2602.11030"},"observation_digest":"sha256:4cbda4a09444d64dd97ebe27b2f1c4cee22f654ee0644619fc5646f99c8fe4c6","observation_id":"08ecc5ed-d1a3-48b4-8c15-0f91591bcb7d","resolution":{"observed_at":"2026-05-16T02:30:31.599455Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.01284","last_updated":"2021-10-19T20:47:09Z","snapshot_observed_at":"2026-08-05T12:37:14.416607Z","submitted_at":"2021-08-03T04:11:04Z","title":"Signs of eccentricity in two gravitational-wave signals may indicate a sub-population of dynamically assembled binary black holes","version":2},"cited_work":{"arxiv_id":"2108.01284","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2108.01284","snapshot_observed_at":"2026-06-30T16:24:58.956638Z","title":"Romero-Shaw, P","venue":null,"work_id":"a1ad3edc-3ba4-4a5e-85f1-f967f5cb2ac0","year":2021},"citing_paper":{"arxiv_id":"2604.15431","last_updated":"2026-04-16T18:00:02Z","snapshot_observed_at":"2026-08-02T05:54:54.327009Z","submitted_at":"2026-04-16T18:00:02Z","title":"Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-05-10T10:16:15.923894Z"},"links":{"cited_paper":"/paper/2108.01284","citing_paper":"/paper/2604.15431"},"observation_digest":"sha256:1aa3bd2390f3a0486ea56fad50d5f93c9c3e88a3382994522057880067475f06","observation_id":"e3bceeea-b4c2-4ca9-b18c-adac12e25e0d","resolution":{"observed_at":"2026-05-10T10:19:20.985065Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.01284","last_updated":"2021-10-19T20:47:09Z","snapshot_observed_at":"2026-08-05T12:37:14.416607Z","submitted_at":"2021-08-03T04:11:04Z","title":"Signs of eccentricity in two gravitational-wave signals may indicate a sub-population of dynamically assembled binary black holes","version":2},"cited_work":{"arxiv_id":"2108.01284","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2108.01284","snapshot_observed_at":"2026-06-30T16:24:58.956638Z","title":"Romero-Shaw, P","venue":null,"work_id":"a1ad3edc-3ba4-4a5e-85f1-f967f5cb2ac0","year":2021},"citing_paper":{"arxiv_id":"2605.12818","last_updated":"2026-05-12T23:23:08Z","snapshot_observed_at":"2026-08-11T07:09:14.444345Z","submitted_at":"2026-05-12T23:23:08Z","title":"Assessing the imprint of eccentricity in GW signatures using two independent waveform models","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-14T19:19:56.792712Z"},"links":{"cited_paper":"/paper/2108.01284","citing_paper":"/paper/2605.12818"},"observation_digest":"sha256:1252339e6f80e292982a26a527cb7111f9850431984cd02a5bd57ce7953bdca7","observation_id":"decde233-759c-4f2a-bbb1-ddfeac923809","resolution":{"observed_at":"2026-05-14T19:22:51.027196Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.01284","last_updated":"2021-10-19T20:47:09Z","snapshot_observed_at":"2026-08-05T12:37:14.416607Z","submitted_at":"2021-08-03T04:11:04Z","title":"Signs of eccentricity in two gravitational-wave signals may indicate a sub-population of dynamically assembled binary black holes","version":2},"cited_work":{"arxiv_id":"2108.01284","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2108.01284","snapshot_observed_at":"2026-06-30T16:24:58.956638Z","title":"Romero-Shaw, P","venue":null,"work_id":"a1ad3edc-3ba4-4a5e-85f1-f967f5cb2ac0","year":2021},"citing_paper":{"arxiv_id":"2605.18742","last_updated":"2026-05-18T17:58:22Z","snapshot_observed_at":"2026-07-06T23:29:33.702647Z","submitted_at":"2026-05-18T17:58:22Z","title":"A universal framework to identify eccentric binary mergers: GW200105 case study","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-20T08:51:43.355150Z"},"links":{"cited_paper":"/paper/2108.01284","citing_paper":"/paper/2605.18742"},"observation_digest":"sha256:df6e9ed19536a8ffb371bf18b3ca01f33e018964d608c11fd5b46d1cc8902ee6","observation_id":"585dd4da-1465-4483-b3c2-5db7d035e4a8","resolution":{"observed_at":"2026-05-20T08:53:10.043185Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.01284","last_updated":"2021-10-19T20:47:09Z","snapshot_observed_at":"2026-08-05T12:37:14.416607Z","submitted_at":"2021-08-03T04:11:04Z","title":"Signs of eccentricity in two gravitational-wave signals may indicate a sub-population of dynamically assembled binary black holes","version":2},"cited_work":{"arxiv_id":"2108.01284","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2108.01284","snapshot_observed_at":"2026-06-30T16:24:58.956638Z","title":"Romero-Shaw, P","venue":null,"work_id":"a1ad3edc-3ba4-4a5e-85f1-f967f5cb2ac0","year":2021},"citing_paper":{"arxiv_id":"2606.30594","last_updated":"2026-06-29T17:35:10Z","snapshot_observed_at":"2026-08-09T11:41:29.556340Z","submitted_at":"2026-06-29T17:35:10Z","title":"Efficient Eccentric Effective-One-Body Dynamics via Near-Identity Averaging Transformations","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-06-30T04:42:30.728872Z"},"links":{"cited_paper":"/paper/2108.01284","citing_paper":"/paper/2606.30594"},"observation_digest":"sha256:4a28cdf03af590ac001cbcb3ab2d77239d38e96dd1ede4420d1ded419ee07497","observation_id":"59653803-0d21-4241-8483-194afa9fdd93","resolution":{"observed_at":"2026-06-30T16:24:58.962137Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2108.01284/citation-record","integrity":"/paper/2108.01284/integrity","json":"/paper/2108.01284/citation-record.json","paper":"/paper/2108.01284"},"outbound":[],"paper":{"arxiv_id":"2108.01284","last_updated":"2021-10-19T20:47:09Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-05T12:37:14.416607Z","submitted_at":"2021-08-03T04:11:04Z","title":"Signs of eccentricity in two gravitational-wave signals may indicate a sub-population of dynamically assembled binary black holes"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2108.01284."}