{"as_of":"2026-08-17T03:12:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:0a6a2314fcae2f5c0b27f90ca06e2558d62ed7385e1d147e311e4f09a226e401","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":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T04:42:52.206074Z","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":"2026-05-22T01:55:55.513422Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1810.13435","last_updated":"2019-03-22T17:33:36Z","snapshot_observed_at":"2026-08-14T18:06:12.482892Z","submitted_at":"2018-10-31T17:50:44Z","title":"Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions","version":2},"cited_work":{"arxiv_id":"1810.13435","doi":null,"metadata_source":"pith","pith_arxiv_id":"1810.13435","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions","venue":"astro-ph.CO","work_id":"751118c6-ad93-48d4-a7f9-ba9f72bd8bcc","year":2018},"citing_paper":{"arxiv_id":"1912.02622","last_updated":"2020-03-24T17:57:53Z","snapshot_observed_at":"2026-08-12T18:38:43.637331Z","submitted_at":"2019-12-05T14:57:00Z","title":"Science Case for the Einstein Telescope","version":4},"reference_index":235,"source":"pdf_text","source_observed_at":"2026-05-16T00:13:18.137293Z"},"links":{"cited_paper":"/paper/1810.13435","citing_paper":"/paper/1912.02622"},"observation_digest":"sha256:4714ad40c71cee6057eb8122e81e8b6407c249de6c99a60a18723dc7bd8cdf8d","observation_id":"cfabff48-c3ac-4c46-8ceb-57d12c412069","resolution":{"observed_at":"2026-05-16T00:13:18.819357Z","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":"1810.13435","last_updated":"2019-03-22T17:33:36Z","snapshot_observed_at":"2026-08-14T18:06:12.482892Z","submitted_at":"2018-10-31T17:50:44Z","title":"Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions","version":2},"cited_work":{"arxiv_id":"1810.13435","doi":null,"metadata_source":"pith","pith_arxiv_id":"1810.13435","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions","venue":"astro-ph.CO","work_id":"751118c6-ad93-48d4-a7f9-ba9f72bd8bcc","year":2018},"citing_paper":{"arxiv_id":"2303.15923","last_updated":"2023-06-17T10:49:26Z","snapshot_observed_at":"2026-08-08T01:52:18.464766Z","submitted_at":"2023-03-28T12:29:33Z","title":"Science with the Einstein Telescope: a comparison of different designs","version":2},"reference_index":101,"source":"pdf_text","source_observed_at":"2026-05-17T21:43:29.760310Z"},"links":{"cited_paper":"/paper/1810.13435","citing_paper":"/paper/2303.15923"},"observation_digest":"sha256:27ea75ca7e9cd467e4bb358253b266149282e5f1a503edac52d88be55bce81cb","observation_id":"72d70f97-af57-4d42-8b7e-a6244a2af210","resolution":{"observed_at":"2026-05-17T21:43:30.298282Z","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":{"arxiv_id":"1810.13435","last_updated":"2019-03-22T17:33:36Z","snapshot_observed_at":"2026-08-14T18:06:12.482892Z","submitted_at":"2018-10-31T17:50:44Z","title":"Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.13435","snapshot_observed_at":"2026-08-12T04:42:52.206074Z","title":"Jenkins, R","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.01219","last_updated":"2025-08-16T12:12:35Z","snapshot_observed_at":"2026-08-14T00:58:44.519960Z","submitted_at":"2024-12-02T07:38:18Z","title":"Estimating the gravitational wave background anisotropy: a Bayesian approach boosted by cross-correlation angular power spectrum","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-12T04:42:52.206074Z"},"links":{"cited_paper":"/paper/1810.13435","citing_paper":"/paper/2412.01219"},"observation_digest":"sha256:9ce91d2482a268d69636e26f06bbfae3b38b9b13aeb4241c1e6b797239d482be","observation_id":"8bb13bbd-def8-4183-8ec9-cb8ea6fabc7d","resolution":{"observed_at":"2026-08-12T04:42:52.206074Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.13435","last_updated":"2019-03-22T17:33:36Z","snapshot_observed_at":"2026-08-14T18:06:12.482892Z","submitted_at":"2018-10-31T17:50:44Z","title":"Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions","version":2},"cited_work":{"arxiv_id":"1810.13435","doi":null,"metadata_source":"pith","pith_arxiv_id":"1810.13435","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions","venue":"astro-ph.CO","work_id":"751118c6-ad93-48d4-a7f9-ba9f72bd8bcc","year":2018},"citing_paper":{"arxiv_id":"2505.16820","last_updated":"2026-04-13T03:10:33Z","snapshot_observed_at":"2026-07-06T21:28:38.694043Z","submitted_at":"2025-05-22T15:55:50Z","title":"Isotropy, anisotropies and non-Gaussianity in the scalar-induced gravitational-wave background: diagrammatic approach for primordial non-Gaussianity up to arbitrary order","version":3},"reference_index":185,"source":"pdf_text","source_observed_at":"2026-05-22T01:55:13.345095Z"},"links":{"cited_paper":"/paper/1810.13435","citing_paper":"/paper/2505.16820"},"observation_digest":"sha256:097dde538178aa75883dbcbd5148582e7f13988cb23deb3b5cfd31a398f3e73a","observation_id":"bcc24cbd-45e9-4dac-b128-271e6fef53da","resolution":{"observed_at":"2026-05-22T01:55:55.515241Z","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":{"arxiv_id":"1810.13435","last_updated":"2019-03-22T17:33:36Z","snapshot_observed_at":"2026-08-14T18:06:12.482892Z","submitted_at":"2018-10-31T17:50:44Z","title":"Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.13435","snapshot_observed_at":"2026-08-05T21:42:58.175523Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.08481","last_updated":"2025-08-11T21:34:05Z","snapshot_observed_at":"2026-08-08T22:29:55.585274Z","submitted_at":"2025-08-11T21:34:05Z","title":"Oscillations and parity violation in gravitational wave background from extra tensor modes","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-05T21:42:58.175523Z"},"links":{"cited_paper":"/paper/1810.13435","citing_paper":"/paper/2508.08481"},"observation_digest":"sha256:57cf5c74ba6e3ecd275eebec408232e466c0d4953a49212f5b586d7bde78e250","observation_id":"bc9e0108-5c56-4d27-8d69-a26459a29bd1","resolution":{"observed_at":"2026-08-05T21:42:58.175523Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.13435","last_updated":"2019-03-22T17:33:36Z","snapshot_observed_at":"2026-08-14T18:06:12.482892Z","submitted_at":"2018-10-31T17:50:44Z","title":"Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions","version":2},"cited_work":{"arxiv_id":"1810.13435","doi":null,"metadata_source":"pith","pith_arxiv_id":"1810.13435","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions","venue":"astro-ph.CO","work_id":"751118c6-ad93-48d4-a7f9-ba9f72bd8bcc","year":2018},"citing_paper":{"arxiv_id":"2510.21521","last_updated":"2026-03-24T13:25:09Z","snapshot_observed_at":"2026-08-15T00:32:39.868648Z","submitted_at":"2025-10-24T14:43:09Z","title":"Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies","version":2},"reference_index":113,"source":"pdf_text","source_observed_at":"2026-05-18T04:48:55.126852Z"},"links":{"cited_paper":"/paper/1810.13435","citing_paper":"/paper/2510.21521"},"observation_digest":"sha256:65fad7cd7b6461fe65d3464c37521f313ed1ab0a7642ccb77a0dc6d4bbc7dd9b","observation_id":"aeee62d7-7555-4e78-b031-265cf0e37bfc","resolution":{"observed_at":"2026-05-18T04:50:54.105268Z","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"}}],"links":{"evidence":"/evidence","html":"/paper/1810.13435/citation-record","integrity":"/paper/1810.13435/integrity","json":"/paper/1810.13435/citation-record.json","paper":"/paper/1810.13435"},"outbound":[],"paper":{"arxiv_id":"1810.13435","last_updated":"2019-03-22T17:33:36Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T18:06:12.482892Z","submitted_at":"2018-10-31T17:50:44Z","title":"Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions"},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1810.13435."}