{"as_of":"2026-08-23T08:01:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e7151511869931ecb4fb87b2e096f719cd02ece43af1611d1a5cf6f631aad8a9","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":9,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":9,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-23T06:30:58.430688+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T15:58:53.903748Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-02T09:26:51.290599Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1509.00512","last_updated":"2015-09-01T21:42:29Z","snapshot_observed_at":"2026-08-18T23:41:41.468607Z","submitted_at":"2015-09-01T21:42:29Z","title":"Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.00512","snapshot_observed_at":"2026-08-14T11:35:56.195075Z","title":"Pannarale, E","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.08822","last_updated":"2019-12-09T07:53:33Z","snapshot_observed_at":"2026-08-16T18:52:47.869436Z","submitted_at":"2019-08-23T13:39:38Z","title":"Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T11:35:56.195075Z"},"links":{"cited_paper":"/paper/1509.00512","citing_paper":"/paper/1908.08822"},"observation_digest":"sha256:9e6166fd1f5d9bb85a4834afa02556122c167504a2d610c4b87b7b350ecf4b96","observation_id":"75569314-2469-4081-bc09-417ec1ebaea1","resolution":{"observed_at":"2026-08-14T11:35:56.195075Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.00512","last_updated":"2015-09-01T21:42:29Z","snapshot_observed_at":"2026-08-18T23:41:41.468607Z","submitted_at":"2015-09-01T21:42:29Z","title":"Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.00512","snapshot_observed_at":"2026-08-06T22:29:59.440960Z","title":"Pannarale, E","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2506.21530","last_updated":"2026-06-24T11:29:49Z","snapshot_observed_at":"2026-08-13T11:49:17.024024Z","submitted_at":"2025-06-26T17:50:19Z","title":"Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T22:29:59.440960Z"},"links":{"cited_paper":"/paper/1509.00512","citing_paper":"/paper/2506.21530"},"observation_digest":"sha256:2c2a4e30ef00a6433c4d098c7a6b7d54faa81ca98dad1dfffd3141a6591ab670","observation_id":"6e37acb4-5159-488d-8f3d-845b31d600aa","resolution":{"observed_at":"2026-08-06T22:29:59.440960Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.00512","last_updated":"2015-09-01T21:42:29Z","snapshot_observed_at":"2026-08-18T23:41:41.468607Z","submitted_at":"2015-09-01T21:42:29Z","title":"Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.00512","snapshot_observed_at":"2026-08-06T21:32:50.544798Z","title":"Pannarale, E","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.00113","last_updated":"2026-06-11T14:27:27Z","snapshot_observed_at":"2026-08-17T20:33:39.409665Z","submitted_at":"2025-06-30T18:00:00Z","title":"Black-hole - neutron-star mergers: new numerical-relativity simulations and multipolar effective-one-body model with spin precession and eccentricity","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-06T21:32:50.544798Z"},"links":{"cited_paper":"/paper/1509.00512","citing_paper":"/paper/2507.00113"},"observation_digest":"sha256:bc1c4fe5c94b6677efb9385b516c184f19c1b5d5ed48d0448552f0c8eb1b304b","observation_id":"55d74e2b-5a25-44f8-a164-b43b9f0e9e94","resolution":{"observed_at":"2026-08-06T21:32:50.544798Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.00512","last_updated":"2015-09-01T21:42:29Z","snapshot_observed_at":"2026-08-18T23:41:41.468607Z","submitted_at":"2015-09-01T21:42:29Z","title":"Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model","version":1},"cited_work":{"arxiv_id":"1509.00512","doi":null,"metadata_source":"pith","pith_arxiv_id":"1509.00512","snapshot_observed_at":"2026-07-02T09:26:51.290599Z","title":"Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model","venue":"gr-qc","work_id":"243b37e0-3a23-4c99-bb91-2d2b8745ad5c","year":2015},"citing_paper":{"arxiv_id":"2509.04028","last_updated":"2026-05-19T16:22:50Z","snapshot_observed_at":"2026-08-16T05:15:05.633771Z","submitted_at":"2025-09-04T09:04:42Z","title":"Primordial black holes versus their impersonators at gravitational wave observatories","version":3},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-05-21T22:15:03.407886Z"},"links":{"cited_paper":"/paper/1509.00512","citing_paper":"/paper/2509.04028"},"observation_digest":"sha256:6dd6bb33de213688aa404990129843f45d274fef9d19bc5d0039e152d17b7090","observation_id":"84cb1307-99a2-4444-a93e-1627c5032299","resolution":{"observed_at":"2026-05-21T22:15:42.066281Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1509.00512","last_updated":"2015-09-01T21:42:29Z","snapshot_observed_at":"2026-08-18T23:41:41.468607Z","submitted_at":"2015-09-01T21:42:29Z","title":"Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.00512","snapshot_observed_at":"2026-08-15T15:58:53.903748Z","title":"Pannarale, E","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.10420","last_updated":"2025-09-12T17:18:32Z","snapshot_observed_at":"2026-08-17T10:16:18.455362Z","submitted_at":"2025-09-12T17:18:32Z","title":"Testing the nature of compact objects in the lower mass gap using gravitational wave observations","version":1},"reference_index":104,"source":"pdf_text","source_observed_at":"2026-08-15T15:58:53.903748Z"},"links":{"cited_paper":"/paper/1509.00512","citing_paper":"/paper/2509.10420"},"observation_digest":"sha256:e640cbc8f8223fce8c383cadc1578c71a1d5b7988e63306ec8c24e5caf3a8f0f","observation_id":"9fe9fb22-edf1-4f7a-8f88-22a39821f455","resolution":{"observed_at":"2026-08-15T15:58:53.903748Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.00512","last_updated":"2015-09-01T21:42:29Z","snapshot_observed_at":"2026-08-18T23:41:41.468607Z","submitted_at":"2015-09-01T21:42:29Z","title":"Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model","version":1},"cited_work":{"arxiv_id":"1509.00512","doi":null,"metadata_source":"pith","pith_arxiv_id":"1509.00512","snapshot_observed_at":"2026-07-02T09:26:51.290599Z","title":"Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model","venue":"gr-qc","work_id":"243b37e0-3a23-4c99-bb91-2d2b8745ad5c","year":2015},"citing_paper":{"arxiv_id":"2606.04810","last_updated":"2026-07-31T09:53:50Z","snapshot_observed_at":"2026-08-05T23:10:45.274273Z","submitted_at":"2026-06-03T12:35:35Z","title":"Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-06-28T05:31:01.574505Z"},"links":{"cited_paper":"/paper/1509.00512","citing_paper":"/paper/2606.04810"},"observation_digest":"sha256:691786e24a9119c1f5726206b0553dd294f5fb6d9fb08176913d4d0923bd62f0","observation_id":"95c8bda4-8812-449d-820a-b3dd7f47afa7","resolution":{"observed_at":"2026-07-02T09:26:51.291808Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1509.00512","last_updated":"2015-09-01T21:42:29Z","snapshot_observed_at":"2026-08-18T23:41:41.468607Z","submitted_at":"2015-09-01T21:42:29Z","title":"Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.00512","snapshot_observed_at":"2026-08-03T02:15:35.934622Z","title":"Pannarale, E","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2606.04810","last_updated":"2026-07-31T09:53:50Z","snapshot_observed_at":"2026-08-05T23:10:45.274273Z","submitted_at":"2026-06-03T12:35:35Z","title":"Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-03T02:15:35.934622Z"},"links":{"cited_paper":"/paper/1509.00512","citing_paper":"/paper/2606.04810"},"observation_digest":"sha256:419bb379135b4b4f7c9d2741a310e578de664898a4e1e343ab6ec3c836adcc01","observation_id":"8f5b0010-8af4-403a-9bb4-9f5805c2b313","resolution":{"observed_at":"2026-08-03T02:15:35.934622Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.00512","last_updated":"2015-09-01T21:42:29Z","snapshot_observed_at":"2026-08-18T23:41:41.468607Z","submitted_at":"2015-09-01T21:42:29Z","title":"Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.00512","snapshot_observed_at":"2026-08-01T09:55:45.286465Z","title":"Pannarale, E","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.20609","last_updated":"2026-07-22T18:00:00Z","snapshot_observed_at":"2026-08-17T01:31:05.841219Z","submitted_at":"2026-07-22T18:00:00Z","title":"Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-01T09:55:45.286465Z"},"links":{"cited_paper":"/paper/1509.00512","citing_paper":"/paper/2607.20609"},"observation_digest":"sha256:bafa540e9640b2d4ab7c31776230247cc3297690e51eb34e27c920565fbf97e8","observation_id":"3ebbccd8-4a77-4529-bffc-99449d1be16e","resolution":{"observed_at":"2026-08-01T09:55:45.286465Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.00512","last_updated":"2015-09-01T21:42:29Z","snapshot_observed_at":"2026-08-18T23:41:41.468607Z","submitted_at":"2015-09-01T21:42:29Z","title":"Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.00512","snapshot_observed_at":"2026-08-01T07:26:22.596653Z","title":"Pannarale, E","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.21484","last_updated":"2026-07-23T16:25:42Z","snapshot_observed_at":"2026-08-20T06:31:35.982793Z","submitted_at":"2026-07-23T16:25:42Z","title":"A story about a tipsy kangaroo: Reversible jump MCMC for model selection in the analysis of gravitational-wave signals from the coalescence of compact objects","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-01T07:26:22.596653Z"},"links":{"cited_paper":"/paper/1509.00512","citing_paper":"/paper/2607.21484"},"observation_digest":"sha256:d35485f1a5dc3624817e58a83f10780b3aa19134aab373e79c204e1b3f7bf0e9","observation_id":"161bf264-dfb4-424e-abe4-b0819a8e4ef0","resolution":{"observed_at":"2026-08-01T07:26:22.596653Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1509.00512/citation-record","integrity":"/paper/1509.00512/integrity","json":"/paper/1509.00512/citation-record.json","paper":"/paper/1509.00512"},"outbound":[],"paper":{"arxiv_id":"1509.00512","last_updated":"2015-09-01T21:42:29Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-18T23:41:41.468607Z","submitted_at":"2015-09-01T21:42:29Z","title":"Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model"},"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":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"thesis":"As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:1509.00512."}