{"as_of":"2026-08-17T09:55:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:0fe4005d8170f26764a6b6ea4843ab4489e33bc4ac2f9f3a455f7bf752e077c6","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T12:17:22.941744Z","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":"2026-05-16T02:27:10.228754Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1804.03087","last_updated":"2018-06-17T10:15:41Z","snapshot_observed_at":"2026-08-14T19:27:49.783151Z","submitted_at":"2018-04-09T16:28:00Z","title":"Testing the Cosmic Anisotropy with Supernovae Data: Hemisphere Comparison and Dipole Fitting","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.03087","snapshot_observed_at":"2026-08-16T12:17:22.941744Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.13380","last_updated":"2025-08-11T12:24:00Z","snapshot_observed_at":"2026-08-16T12:07:41.561264Z","submitted_at":"2025-04-18T00:00:00Z","title":"Alleviating the Hubble Tension with a Local Void and Transitions of the Absolute Magnitude","version":3},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-16T12:17:22.941744Z"},"links":{"cited_paper":"/paper/1804.03087","citing_paper":"/paper/2504.13380"},"observation_digest":"sha256:06e166ba47f48a956d21f06c2295944c450a78b34d8e16893eced5d3958ae9b3","observation_id":"47fe8850-e163-416d-b2d4-4c2ff3540162","resolution":{"observed_at":"2026-08-16T12:17:22.941744Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03087","last_updated":"2018-06-17T10:15:41Z","snapshot_observed_at":"2026-08-14T19:27:49.783151Z","submitted_at":"2018-04-09T16:28:00Z","title":"Testing the Cosmic Anisotropy with Supernovae Data: Hemisphere Comparison and Dipole Fitting","version":3},"cited_work":{"arxiv_id":"1804.03087","doi":null,"metadata_source":"pith","pith_arxiv_id":"1804.03087","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Testing the Cosmic Anisotropy with Supernovae Data: Hemisphere Comparison and Dipole Fitting","venue":"astro-ph.CO","work_id":"9d2d962b-826d-4ed6-8f6e-933e97965068","year":2018},"citing_paper":{"arxiv_id":"2602.11093","last_updated":"2026-04-18T16:30:32Z","snapshot_observed_at":"2026-08-08T00:16:50.248213Z","submitted_at":"2026-02-11T18:01:44Z","title":"New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method","version":2},"reference_index":185,"source":"pdf_text","source_observed_at":"2026-05-16T02:22:49.920780Z"},"links":{"cited_paper":"/paper/1804.03087","citing_paper":"/paper/2602.11093"},"observation_digest":"sha256:7c5bb54691ec18570190d2ed714c6eb38a6a0c19ad1e7cf6e6cb07249d2e3e84","observation_id":"6a986c20-8d84-40bf-b6a8-89854f347614","resolution":{"observed_at":"2026-05-16T02:27:10.231595Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1804.03087/citation-record","integrity":"/paper/1804.03087/integrity","json":"/paper/1804.03087/citation-record.json","paper":"/paper/1804.03087"},"outbound":[],"paper":{"arxiv_id":"1804.03087","last_updated":"2018-06-17T10:15:41Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T19:27:49.783151Z","submitted_at":"2018-04-09T16:28:00Z","title":"Testing the Cosmic Anisotropy with Supernovae Data: Hemisphere Comparison and Dipole Fitting"},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1804.03087."}