{"as_of":"2026-08-14T12:14:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:396e6ea5fe876a91f10a0927ec7cf45ebf25dc4d68a1080532f75f2de3b220fa","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":"2026-08-14T06:32:32.682623+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":"2026-08-12T14:17:14.898116Z","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":"2026-05-20T03:03:21.494791Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2101.12660","last_updated":"2021-07-16T13:15:57Z","snapshot_observed_at":"2026-08-10T22:25:54.709947Z","submitted_at":"2021-01-29T16:05:28Z","title":"Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation","version":3},"cited_work":{"arxiv_id":"2101.12660","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2101.12660","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Finke, S","venue":null,"work_id":"d10cade8-14cc-4270-b3ee-96efe4a5d035","year":2021},"citing_paper":{"arxiv_id":"2103.01183","last_updated":"2021-06-05T10:18:21Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2021-03-01T18:27:48Z","title":"In the Realm of the Hubble tension $-$ a Review of Solutions","version":3},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-15T11:50:20.600831Z"},"links":{"cited_paper":"/paper/2101.12660","citing_paper":"/paper/2103.01183"},"observation_digest":"sha256:56b58f18f3e66fa13275b2ab26df7d02d9ebc8b9dfabdd96c6377e123f0cd0b0","observation_id":"e7f22e48-1d4b-4abc-87bf-198c6d0fddd9","resolution":{"observed_at":"2026-05-15T11:50:20.877168Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.12660","last_updated":"2021-07-16T13:15:57Z","snapshot_observed_at":"2026-08-10T22:25:54.709947Z","submitted_at":"2021-01-29T16:05:28Z","title":"Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.12660","snapshot_observed_at":"2026-08-12T14:17:14.898116Z","title":"Finke, S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.15506","last_updated":"2025-06-27T15:42:35Z","snapshot_observed_at":"2026-08-13T14:35:36.336430Z","submitted_at":"2024-11-23T09:55:03Z","title":"Null Stream Based Third-generation-ready Glitch Mitigation for Gravitational Wave Measurements","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-12T14:17:14.898116Z"},"links":{"cited_paper":"/paper/2101.12660","citing_paper":"/paper/2411.15506"},"observation_digest":"sha256:4ccf8cba968f2adafd4ab7948b47e34bb893a1b35c8e25bf6d80da377d5b84d0","observation_id":"8a1d2fe4-b0be-48ac-a9ab-a32f16fde7de","resolution":{"observed_at":"2026-08-12T14:17:14.898116Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.12660","last_updated":"2021-07-16T13:15:57Z","snapshot_observed_at":"2026-08-10T22:25:54.709947Z","submitted_at":"2021-01-29T16:05:28Z","title":"Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.12660","snapshot_observed_at":"2026-08-12T05:45:52.891660Z","title":"Finke, S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.00202","last_updated":"2025-03-06T04:01:35Z","snapshot_observed_at":"2026-08-13T13:27:52.391598Z","submitted_at":"2024-11-29T19:01:11Z","title":"A robust cosmic standard ruler from the cross-correlations of galaxies and dark sirens","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-12T05:45:52.891660Z"},"links":{"cited_paper":"/paper/2101.12660","citing_paper":"/paper/2412.00202"},"observation_digest":"sha256:4a033c061ed0e7ae981205010d7c9c1d597178919d221c2bd6b36f2921c4ec18","observation_id":"6a6523bc-862d-4aca-8f75-8ca9c2031ea7","resolution":{"observed_at":"2026-08-12T05:45:52.891660Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.12660","last_updated":"2021-07-16T13:15:57Z","snapshot_observed_at":"2026-08-10T22:25:54.709947Z","submitted_at":"2021-01-29T16:05:28Z","title":"Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.12660","snapshot_observed_at":"2026-08-10T21:21:31.899710Z","title":"Finke, S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.05560","last_updated":"2025-05-28T10:49:38Z","snapshot_observed_at":"2026-08-13T04:54:52.394484Z","submitted_at":"2025-01-09T20:11:51Z","title":"A Bright Future? Prospects for Cosmological Tests of GR with Multimessenger Gravitational Wave Events","version":2},"reference_index":108,"source":"pdf_text","source_observed_at":"2026-08-10T21:21:31.899710Z"},"links":{"cited_paper":"/paper/2101.12660","citing_paper":"/paper/2501.05560"},"observation_digest":"sha256:5101240950199062d8d5b6881ef9cb3b945e07e7100b9686a769e346e910099b","observation_id":"c42a09e5-e1e4-44f4-9bdb-01de47b20d33","resolution":{"observed_at":"2026-08-10T21:21:31.899710Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.12660","last_updated":"2021-07-16T13:15:57Z","snapshot_observed_at":"2026-08-10T22:25:54.709947Z","submitted_at":"2021-01-29T16:05:28Z","title":"Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.12660","snapshot_observed_at":"2026-08-06T22:30:00.286771Z","title":"Finke, S","venue":null,"work_id":null,"year":2021},"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":82,"source":"pdf_text","source_observed_at":"2026-08-06T22:30:00.286771Z"},"links":{"cited_paper":"/paper/2101.12660","citing_paper":"/paper/2506.21530"},"observation_digest":"sha256:923bcef7a3a0dcf1fc32ab24043f147419e86bda1fe393a28bc6ad2e1c1351ac","observation_id":"f15b3cd8-72e4-45b3-acf6-6f7de63fb5d8","resolution":{"observed_at":"2026-08-06T22:30:00.286771Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.12660","last_updated":"2021-07-16T13:15:57Z","snapshot_observed_at":"2026-08-10T22:25:54.709947Z","submitted_at":"2021-01-29T16:05:28Z","title":"Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.12660","snapshot_observed_at":"2026-08-03T06:51:32.936607Z","title":"Finke, S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2601.21820","last_updated":"2026-05-28T08:19:01Z","snapshot_observed_at":"2026-08-13T13:08:09.900415Z","submitted_at":"2026-01-29T15:04:37Z","title":"Forecasting Constraints on Cosmology and Modified Gravitational-wave Propagation by Combining Strongly Lensed Gravitational Waves and Galaxy Surveys","version":3},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-03T06:51:32.936607Z"},"links":{"cited_paper":"/paper/2101.12660","citing_paper":"/paper/2601.21820"},"observation_digest":"sha256:665f28b9f93c12f8025c9457fde5475058e59c9526855b718ecdefffd9b02a26","observation_id":"b9285efb-fb04-4408-8ffd-d4b10f55c086","resolution":{"observed_at":"2026-08-03T06:51:32.936607Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.12660","last_updated":"2021-07-16T13:15:57Z","snapshot_observed_at":"2026-08-10T22:25:54.709947Z","submitted_at":"2021-01-29T16:05:28Z","title":"Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation","version":3},"cited_work":{"arxiv_id":"2101.12660","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2101.12660","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Finke, S","venue":null,"work_id":"d10cade8-14cc-4270-b3ee-96efe4a5d035","year":2021},"citing_paper":{"arxiv_id":"2604.10942","last_updated":"2026-04-13T03:20:49Z","snapshot_observed_at":"2026-08-11T13:31:43.286648Z","submitted_at":"2026-04-13T03:20:49Z","title":"Probing Active Galactic Nuclei and Measuring the Hubble constant with Extreme-Mass-Ratio Inspirals","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-05-10T15:58:14.292439Z"},"links":{"cited_paper":"/paper/2101.12660","citing_paper":"/paper/2604.10942"},"observation_digest":"sha256:f25379c3d6f018f98f14af8eed5f816e0feba10848b0f8f341311bac63965adf","observation_id":"bbb40ca6-64a4-4455-a92f-08b64acfe2f0","resolution":{"observed_at":"2026-05-11T09:31:05.258302Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.12660","last_updated":"2021-07-16T13:15:57Z","snapshot_observed_at":"2026-08-10T22:25:54.709947Z","submitted_at":"2021-01-29T16:05:28Z","title":"Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation","version":3},"cited_work":{"arxiv_id":"2101.12660","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2101.12660","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Finke, S","venue":null,"work_id":"d10cade8-14cc-4270-b3ee-96efe4a5d035","year":2021},"citing_paper":{"arxiv_id":"2604.11871","last_updated":"2026-04-13T18:00:00Z","snapshot_observed_at":"2026-08-11T08:45:39.528049Z","submitted_at":"2026-04-13T18:00:00Z","title":"Not too close! Evaluating the impact of the baseline on the localization of binary black holes by next-generation gravitational-wave detectors","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-05-10T15:27:10.838625Z"},"links":{"cited_paper":"/paper/2101.12660","citing_paper":"/paper/2604.11871"},"observation_digest":"sha256:e26d69b35752fce5588e97828fa792cba5fb961649c83ab5aed51d81475cfbbd","observation_id":"fd3ddc7d-2569-4fab-b978-05928600780d","resolution":{"observed_at":"2026-05-11T10:31:03.005910Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.12660","last_updated":"2021-07-16T13:15:57Z","snapshot_observed_at":"2026-08-10T22:25:54.709947Z","submitted_at":"2021-01-29T16:05:28Z","title":"Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation","version":3},"cited_work":{"arxiv_id":"2101.12660","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2101.12660","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Finke, S","venue":null,"work_id":"d10cade8-14cc-4270-b3ee-96efe4a5d035","year":2021},"citing_paper":{"arxiv_id":"2605.19476","last_updated":"2026-07-14T05:19:43Z","snapshot_observed_at":"2026-08-01T14:11:35.513868Z","submitted_at":"2026-05-19T07:28:18Z","title":"Prospect of Measuring the Cosmic Dipole by Associating Strongly Lensed Gravitational Waves with Galaxy Surveys","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-05-20T03:03:06.326603Z"},"links":{"cited_paper":"/paper/2101.12660","citing_paper":"/paper/2605.19476"},"observation_digest":"sha256:66b15a6eebdcec4362ac23be9abaec975759fe8870db8c8c3c1228f25d1cfaa5","observation_id":"e1ad919a-c4ae-4693-8a8d-476004772961","resolution":{"observed_at":"2026-05-20T03:03:21.498519Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2101.12660/citation-record","integrity":"/paper/2101.12660/integrity","json":"/paper/2101.12660/citation-record.json","paper":"/paper/2101.12660"},"outbound":[],"paper":{"arxiv_id":"2101.12660","last_updated":"2021-07-16T13:15:57Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-10T22:25:54.709947Z","submitted_at":"2021-01-29T16:05:28Z","title":"Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation"},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2101.12660."}