{"as_of":"2026-08-09T09:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:86422c06c28114ba0d87d668e0b80f07d36a55fc44a69ae9a96a87714603e422","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T22:32:29.229125Z","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":"2026-08-05T14:43:18.255707Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1004.3988","last_updated":"2010-06-27T07:04:04Z","snapshot_observed_at":"2026-07-06T02:09:38.416009Z","submitted_at":"2010-04-22T19:14:23Z","title":"Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1004.3988","snapshot_observed_at":"2026-08-06T22:30:00.354644Z","title":"Hirata, D.E","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2506.21530","last_updated":"2026-06-24T11:29:49Z","snapshot_observed_at":"2026-08-08T04:44:08.489839Z","submitted_at":"2025-06-26T17:50:19Z","title":"Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-06T22:30:00.354644Z"},"links":{"cited_paper":"/paper/1004.3988","citing_paper":"/paper/2506.21530"},"observation_digest":"sha256:5a5d37a3d37d650306488173b23bcc57b7573a51f7ffee130b32e2e951c3cc30","observation_id":"3f3e8975-0056-48b4-ad3e-1a13921258c0","resolution":{"observed_at":"2026-08-06T22:30:00.354644Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1004.3988","last_updated":"2010-06-27T07:04:04Z","snapshot_observed_at":"2026-07-06T02:09:38.416009Z","submitted_at":"2010-04-22T19:14:23Z","title":"Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution","version":2},"cited_work":{"arxiv_id":"1004.3988","doi":null,"metadata_source":"pith","pith_arxiv_id":"1004.3988","snapshot_observed_at":"2026-08-05T14:43:18.255707Z","title":"Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution","venue":"astro-ph.CO","work_id":"4fe2eda8-84f6-4663-ac54-93e27ea22695","year":2010},"citing_paper":{"arxiv_id":"2508.20971","last_updated":"2026-06-14T15:39:47Z","snapshot_observed_at":"2026-08-08T08:18:35.611546Z","submitted_at":"2025-08-28T16:25:22Z","title":"Cosmo-Learn: code for learning cosmology using different methods and mock data","version":2},"reference_index":102,"source":"pdf_text","source_observed_at":"2026-08-05T14:43:16.670962Z"},"links":{"cited_paper":"/paper/1004.3988","citing_paper":"/paper/2508.20971"},"observation_digest":"sha256:2896a202e36487bbd5072ae258abe609488c1e552c38130ec6c9b8ced3a548dd","observation_id":"a12baf12-08ff-42d6-9afc-03aee0feb973","resolution":{"observed_at":"2026-08-05T14:43:18.261719Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1004.3988","last_updated":"2010-06-27T07:04:04Z","snapshot_observed_at":"2026-07-06T02:09:38.416009Z","submitted_at":"2010-04-22T19:14:23Z","title":"Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1004.3988","snapshot_observed_at":"2026-08-07T22:32:29.229125Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2608.05846","last_updated":"2026-08-06T10:19:40Z","snapshot_observed_at":"2026-08-09T09:10:53.438806Z","submitted_at":"2026-08-06T10:19:40Z","title":"Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-07T22:32:29.229125Z"},"links":{"cited_paper":"/paper/1004.3988","citing_paper":"/paper/2608.05846"},"observation_digest":"sha256:4c09a4e4d9d63736a49d1430fb7c1a0fa11906dfd0f689d7145307b69cf6ef3f","observation_id":"70b8dd29-3a39-418c-aa37-d482c94a16fe","resolution":{"observed_at":"2026-08-07T22:32:29.229125Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1004.3988/citation-record","integrity":"/paper/1004.3988/integrity","json":"/paper/1004.3988/citation-record.json","paper":"/paper/1004.3988"},"outbound":[],"paper":{"arxiv_id":"1004.3988","last_updated":"2010-06-27T07:04:04Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T02:09:38.416009Z","submitted_at":"2010-04-22T19:14:23Z","title":"Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution"},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1004.3988."}