{"as_of":"2026-08-17T18:44:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:dfbd2523beec41ca0d5b57073bd83a9f99b68fe843ad9e5008387c6ffaa37c5b","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":"2026-08-16T04:44:17.906381Z","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":"2026-07-02T08:46:48.319691Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1605.07621","last_updated":"2016-10-28T22:35:03Z","snapshot_observed_at":"2026-08-14T21:55:55.065969Z","submitted_at":"2016-05-24T20:00:02Z","title":"Lens Models Under the Microscope: Comparison of Hubble Frontier Field Cluster Magnification Maps","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.07621","snapshot_observed_at":"2026-08-16T04:44:17.906381Z","title":"Priewe , author L","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.00553","last_updated":"2025-07-07T04:13:10Z","snapshot_observed_at":"2026-08-16T19:54:57.507286Z","submitted_at":"2025-05-01T14:28:50Z","title":"The Jackknife method as a new approach to validate strong lens mass models","version":2},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-16T04:44:17.906381Z"},"links":{"cited_paper":"/paper/1605.07621","citing_paper":"/paper/2505.00553"},"observation_digest":"sha256:4a36afd2b78cbc4adc60488063046f609934dc609b89576ebfd459d1fad27b88","observation_id":"a24b84dc-33a6-45ef-9bcf-da6568514633","resolution":{"observed_at":"2026-08-16T04:44:17.906381Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.07621","last_updated":"2016-10-28T22:35:03Z","snapshot_observed_at":"2026-08-14T21:55:55.065969Z","submitted_at":"2016-05-24T20:00:02Z","title":"Lens Models Under the Microscope: Comparison of Hubble Frontier Field Cluster Magnification Maps","version":2},"cited_work":{"arxiv_id":"1605.07621","doi":null,"metadata_source":"pith","pith_arxiv_id":"1605.07621","snapshot_observed_at":"2026-07-02T08:46:48.319691Z","title":"Lens Models Under the Microscope: Comparison of Hubble Frontier Field Cluster Magnification Maps","venue":"astro-ph.CO","work_id":"51c89903-cee3-410d-8edf-f063bdfa6738","year":2016},"citing_paper":{"arxiv_id":"2607.01129","last_updated":"2026-07-01T16:14:57Z","snapshot_observed_at":"2026-08-02T07:24:12.624750Z","submitted_at":"2026-07-01T16:14:57Z","title":"Tilting at the Turnover: Modeling the Faint-End of the UV Luminosity Function Behind Abell s1063 with JWST","version":1},"reference_index":178,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1605.07621","citing_paper":"/paper/2607.01129"},"observation_digest":"sha256:0f01d0675a52c9827f47f4d372c0b6c5677d349e684bf5c641ba2cc5f61a6d09","observation_id":"ec904187-6b4b-4698-8ac8-2632d7a230ab","resolution":{"observed_at":"2026-07-02T08:46:48.321202Z","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/1605.07621/citation-record","integrity":"/paper/1605.07621/integrity","json":"/paper/1605.07621/citation-record.json","paper":"/paper/1605.07621"},"outbound":[],"paper":{"arxiv_id":"1605.07621","last_updated":"2016-10-28T22:35:03Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T21:55:55.065969Z","submitted_at":"2016-05-24T20:00:02Z","title":"Lens Models Under the Microscope: Comparison of Hubble Frontier Field Cluster Magnification Maps"},"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:1605.07621."}