{"as_of":"2026-08-07T14:05:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b349326823cfe99b9e8da918535fea55b55ac24a56a02b92bb99c821a057f233","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":"2026-08-07T06:34:17.273281+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":"2026-08-04T12:56:21.301128Z","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":"2026-05-14T20:39:27.819523Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2502.18571","last_updated":"2025-08-13T16:06:09Z","snapshot_observed_at":"2026-07-06T20:42:37.899256Z","submitted_at":"2025-02-25T19:01:15Z","title":"Dark Matter Substructure or Source Model Systematics? A Case Study of Cluster Lens Abell S1063","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.18571","snapshot_observed_at":"2026-08-04T12:56:21.301128Z","title":"Ephremidze, C","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.01491","last_updated":"2026-07-15T03:08:10Z","snapshot_observed_at":"2026-08-07T04:55:17.035249Z","submitted_at":"2025-10-01T22:06:50Z","title":"Strong-lensing Perturber Signatures in Self-interacting Dark Matter Simulations","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-04T12:56:21.301128Z"},"links":{"cited_paper":"/paper/2502.18571","citing_paper":"/paper/2510.01491"},"observation_digest":"sha256:8e604f3c2ecaa637f77255801b4e018c11f2e47cc92eb0250b29dd2dbb3a3c68","observation_id":"b09c9720-a1a2-46b5-8727-850acb877f22","resolution":{"observed_at":"2026-08-04T12:56:21.301128Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.18571","last_updated":"2025-08-13T16:06:09Z","snapshot_observed_at":"2026-07-06T20:42:37.899256Z","submitted_at":"2025-02-25T19:01:15Z","title":"Dark Matter Substructure or Source Model Systematics? A Case Study of Cluster Lens Abell S1063","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.18571","snapshot_observed_at":"2026-08-03T23:07:54.325023Z","title":"Ephremidze, C","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.07513","last_updated":"2026-07-01T19:58:59Z","snapshot_observed_at":"2026-08-03T23:07:44.001227Z","submitted_at":"2025-11-10T19:00:00Z","title":"JWST lensed quasar dark matter survey IV: Stringent warm dark matter constraints from the joint reconstruction of extended lensed arcs and quasar flux ratios","version":5},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.325023Z"},"links":{"cited_paper":"/paper/2502.18571","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:83bb26397c3fdcee5b59858396f46faf34d7d13d0665e612b7adb4863be35292","observation_id":"47239ece-4e72-4298-b26b-d07e5359195d","resolution":{"observed_at":"2026-08-03T23:07:54.325023Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.18571","last_updated":"2025-08-13T16:06:09Z","snapshot_observed_at":"2026-07-06T20:42:37.899256Z","submitted_at":"2025-02-25T19:01:15Z","title":"Dark Matter Substructure or Source Model Systematics? A Case Study of Cluster Lens Abell S1063","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.18571","snapshot_observed_at":"2026-08-03T05:51:13.006045Z","title":"Ephremidze, C","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2602.01141","last_updated":"2026-07-07T05:22:21Z","snapshot_observed_at":"2026-08-06T16:09:10.767581Z","submitted_at":"2026-02-01T10:29:54Z","title":"Wigner function shapelets: Symplectic representation of astronomical images","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-03T05:51:13.006045Z"},"links":{"cited_paper":"/paper/2502.18571","citing_paper":"/paper/2602.01141"},"observation_digest":"sha256:13810a885aee680d8b4a42f47e7e0e05378a2d3a235734068afb4789f7cff750","observation_id":"190c10bc-57ad-44bc-a038-d48fd959a485","resolution":{"observed_at":"2026-08-03T05:51:13.006045Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.18571","last_updated":"2025-08-13T16:06:09Z","snapshot_observed_at":"2026-07-06T20:42:37.899256Z","submitted_at":"2025-02-25T19:01:15Z","title":"Dark Matter Substructure or Source Model Systematics? A Case Study of Cluster Lens Abell S1063","version":2},"cited_work":{"arxiv_id":"2502.18571","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.18571","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"arXiv e-prints arXiv:2502.18571 (2025)","venue":null,"work_id":"bd1ee089-641d-4337-9c09-cec336e405ec","year":2025},"citing_paper":{"arxiv_id":"2605.12593","last_updated":"2026-05-12T18:00:01Z","snapshot_observed_at":"2026-07-06T23:24:18.302402Z","submitted_at":"2026-05-12T18:00:01Z","title":"How much dark matter really matters?","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-05-14T20:35:04.325986Z"},"links":{"cited_paper":"/paper/2502.18571","citing_paper":"/paper/2605.12593"},"observation_digest":"sha256:661803bafab0aa05d27b0927d8e6b65a906670a3aa287a2314483070461f21bd","observation_id":"6e595672-8aa3-4e0c-abf8-9545ec9c0f12","resolution":{"observed_at":"2026-05-14T20:39:27.822460Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2502.18571/citation-record","integrity":"/paper/2502.18571/integrity","json":"/paper/2502.18571/citation-record.json","paper":"/paper/2502.18571"},"outbound":[],"paper":{"arxiv_id":"2502.18571","last_updated":"2025-08-13T16:06:09Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T20:42:37.899256Z","submitted_at":"2025-02-25T19:01:15Z","title":"Dark Matter Substructure or Source Model Systematics? A Case Study of Cluster Lens Abell S1063"},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2502.18571."}