{"as_of":"2026-08-12T07:33:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:440c050eb62d3dcaac7d86338dbe3fe9306ba1ebe3911e718d928fb702207113","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T04:22:44.352700Z","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":"2026-07-02T15:27:05.144063Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2407.17059","last_updated":"2025-02-19T00:41:24Z","snapshot_observed_at":"2026-08-11T02:15:32.576827Z","submitted_at":"2024-07-24T07:37:05Z","title":"Fuzzy Dark Matter Constraints from the Hubble Frontier Fields","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.17059","snapshot_observed_at":"2026-08-06T21:19:07.745515Z","title":"Sipple, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.00705","last_updated":"2025-07-01T12:04:24Z","snapshot_observed_at":"2026-08-06T22:47:10.673807Z","submitted_at":"2025-07-01T12:04:24Z","title":"Ultralight fuzzy dark matter review","version":1},"reference_index":218,"source":"pdf_text","source_observed_at":"2026-08-06T21:19:07.745515Z"},"links":{"cited_paper":"/paper/2407.17059","citing_paper":"/paper/2507.00705"},"observation_digest":"sha256:51276fb40b09498fb828028e9258f45487341b8b28bfb114ff80338f3ddc86af","observation_id":"6790327b-5fb7-4e4b-a790-3b710e7433fe","resolution":{"observed_at":"2026-08-06T21:19:07.745515Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.17059","last_updated":"2025-02-19T00:41:24Z","snapshot_observed_at":"2026-08-11T02:15:32.576827Z","submitted_at":"2024-07-24T07:37:05Z","title":"Fuzzy Dark Matter Constraints from the Hubble Frontier Fields","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.17059","snapshot_observed_at":"2026-08-03T05:48:41.136214Z","title":"Sipple, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2602.01320","last_updated":"2026-08-09T14:20:31Z","snapshot_observed_at":"2026-08-12T07:14:45.438880Z","submitted_at":"2026-02-01T16:28:06Z","title":"A Variable-Slope Smooth-$k$ Filter for Modeling Halo Abundances with Damped and Oscillatory Power Spectra","version":3},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-03T05:48:41.136214Z"},"links":{"cited_paper":"/paper/2407.17059","citing_paper":"/paper/2602.01320"},"observation_digest":"sha256:22922ce044479ab210516809bbe262fa0cb83c4426a75258a1020c3e6aab976a","observation_id":"f28a22cb-757d-4acb-b6a1-bbcce95a35dd","resolution":{"observed_at":"2026-08-03T05:48:41.136214Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.17059","last_updated":"2025-02-19T00:41:24Z","snapshot_observed_at":"2026-08-11T02:15:32.576827Z","submitted_at":"2024-07-24T07:37:05Z","title":"Fuzzy Dark Matter Constraints from the Hubble Frontier Fields","version":2},"cited_work":{"arxiv_id":"2407.17059","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.17059","snapshot_observed_at":"2026-07-02T15:27:05.144063Z","title":"Sipple, A","venue":null,"work_id":"1b53d0c8-1d2b-407b-b1f8-8be1f4efd09f","year":2025},"citing_paper":{"arxiv_id":"2606.06410","last_updated":"2026-06-04T17:14:22Z","snapshot_observed_at":"2026-08-01T15:17:31.332664Z","submitted_at":"2026-06-04T17:14:22Z","title":"The Atacama Cosmology Telescope: Probing new signatures of ultralight axions with gravitational lensing","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-06-27T23:53:12.581079Z"},"links":{"cited_paper":"/paper/2407.17059","citing_paper":"/paper/2606.06410"},"observation_digest":"sha256:25f694ec0eb49383fcc01a806162ccbe4614423b913e64e9cb85e962848ef4a2","observation_id":"e3f17b39-a2be-40d8-9830-22c7ddb3ac09","resolution":{"observed_at":"2026-07-02T15:27:05.145572Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.17059","last_updated":"2025-02-19T00:41:24Z","snapshot_observed_at":"2026-08-11T02:15:32.576827Z","submitted_at":"2024-07-24T07:37:05Z","title":"Fuzzy Dark Matter Constraints from the Hubble Frontier Fields","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.17059","snapshot_observed_at":"2026-08-11T04:22:44.352700Z","title":"Sipple, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.07803","last_updated":"2026-08-07T22:59:50Z","snapshot_observed_at":"2026-08-12T07:14:00.793282Z","submitted_at":"2026-08-07T22:59:50Z","title":"Inflationary Axion Isocurvature in the CMB across All Ultralight Masses","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-11T04:22:44.352700Z"},"links":{"cited_paper":"/paper/2407.17059","citing_paper":"/paper/2608.07803"},"observation_digest":"sha256:73daa644479ea32dd9b42f4fd5a519369f12c9fd2084a7a4167562e7e47a468a","observation_id":"334dc55a-80ca-4afa-8823-c554bebcbd9f","resolution":{"observed_at":"2026-08-11T04:22:44.352700Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2407.17059/citation-record","integrity":"/paper/2407.17059/integrity","json":"/paper/2407.17059/citation-record.json","paper":"/paper/2407.17059"},"outbound":[],"paper":{"arxiv_id":"2407.17059","last_updated":"2025-02-19T00:41:24Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-11T02:15:32.576827Z","submitted_at":"2024-07-24T07:37:05Z","title":"Fuzzy Dark Matter Constraints from the Hubble Frontier Fields"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2407.17059."}