{"as_of":"2026-08-07T00:46:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:949a578639eab4b1e07b832870f179d08ec685f45761e8f7627d52a3f55f3426","coverage":[{"denominator":171,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T23:07:54.458270Z","state":"measured"},{"denominator":112,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":112,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-06T06:34:29.942622+00:00","state":"measured"},{"denominator":12,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":12,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T21:29:36.706320Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2511.07513","snapshot_observed_at":"2026-08-03T21:29:36.706320Z","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,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.15430","last_updated":"2025-11-19T13:36:51Z","snapshot_observed_at":"2026-08-04T02:30:03.108556Z","submitted_at":"2025-11-19T13:36:51Z","title":"21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-03T21:29:36.706320Z"},"links":{"cited_paper":"/paper/2511.07513","citing_paper":"/paper/2511.15430"},"observation_digest":"sha256:ad1753b753ac1096037ea8ac55f5541ebd0efda85d9286fbd230b852e8c2713e","observation_id":"45e5f214-f734-49cf-8c0a-99370476ae7b","resolution":{"observed_at":"2026-08-03T21:29:36.706320Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":"2511.07513","doi":"10.48550/arxiv.2511.07513","metadata_source":"pith","pith_arxiv_id":"2511.07513","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"astro-ph.CO","work_id":"cc2d5159-e55c-47fc-845e-77b83e309d88","year":2025},"citing_paper":{"arxiv_id":"2604.05237","last_updated":"2026-04-06T23:00:49Z","snapshot_observed_at":"2026-07-06T22:54:00.211106Z","submitted_at":"2026-04-06T23:00:49Z","title":"JWST Lensed Quasar Dark Matter Survey V: Measuring the minimum halo mass with strong gravitational lensing","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-10T18:42:35.204257Z"},"links":{"cited_paper":"/paper/2511.07513","citing_paper":"/paper/2604.05237"},"observation_digest":"sha256:f72ff06e5509d84f3c2e767ed434c86c15efd413521ccac03198479a7a403a97","observation_id":"ba6dba9e-bc1f-42cb-b02c-e7cafbcb5074","resolution":{"observed_at":"2026-06-05T01:14:30.579137Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":"2511.07513","doi":"10.48550/arxiv.2511.07513","metadata_source":"pith","pith_arxiv_id":"2511.07513","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"astro-ph.CO","work_id":"cc2d5159-e55c-47fc-845e-77b83e309d88","year":2025},"citing_paper":{"arxiv_id":"2605.19217","last_updated":"2026-05-19T00:43:42Z","snapshot_observed_at":"2026-08-02T02:51:01.791696Z","submitted_at":"2026-05-19T00:43:42Z","title":"Taking Inventory of the Most Promising Lensed Radio Sources for Constraining Fundamental Properties of Dark Matter","version":1},"reference_index":206,"source":"arxiv_source","source_observed_at":"2026-05-20T04:55:56.677353Z"},"links":{"cited_paper":"/paper/2511.07513","citing_paper":"/paper/2605.19217"},"observation_digest":"sha256:a97caa7dc99fdba5b025a5931390b9b32789ec1263164d70fc5e0507b6a62c14","observation_id":"be7a6d69-4d50-4ad2-8a64-5030ade374a0","resolution":{"observed_at":"2026-06-05T01:14:30.579137Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":"2511.07513","doi":"10.48550/arxiv.2511.07513","metadata_source":"pith","pith_arxiv_id":"2511.07513","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"astro-ph.CO","work_id":"cc2d5159-e55c-47fc-845e-77b83e309d88","year":2025},"citing_paper":{"arxiv_id":"2605.21212","last_updated":"2026-05-20T14:07:43Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-20T14:07:43Z","title":"Detection of a dark matter subhalo in the strongly lensed system PJ011646","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-05-21T03:18:37.584723Z"},"links":{"cited_paper":"/paper/2511.07513","citing_paper":"/paper/2605.21212"},"observation_digest":"sha256:9744784b4c2990cbefbe2d499853c4fcb1a165464c8e5f76981d485fdd9fda1c","observation_id":"0565155f-b798-4544-80fd-005e6e329f6f","resolution":{"observed_at":"2026-06-05T01:14:30.579137Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":"2511.07513","doi":"10.48550/arxiv.2511.07513","metadata_source":"pith","pith_arxiv_id":"2511.07513","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"astro-ph.CO","work_id":"cc2d5159-e55c-47fc-845e-77b83e309d88","year":2025},"citing_paper":{"arxiv_id":"2605.24174","last_updated":"2026-05-22T19:48:35Z","snapshot_observed_at":"2026-07-06T23:34:18.555542Z","submitted_at":"2026-05-22T19:48:35Z","title":"The Sensitivity of Substructure Lensing to SIDM Core-collapse Model Variation","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-06-30T14:07:25.688498Z"},"links":{"cited_paper":"/paper/2511.07513","citing_paper":"/paper/2605.24174"},"observation_digest":"sha256:a7d4ee48e8ab554cd46c35f297021c63ace3e15db9c2260bb5cfebb0b16ce142","observation_id":"572a4892-1302-4fb4-9ae8-4680216303ea","resolution":{"observed_at":"2026-06-30T14:14:45.689670Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":"2511.07513","doi":"10.48550/arxiv.2511.07513","metadata_source":"pith","pith_arxiv_id":"2511.07513","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"astro-ph.CO","work_id":"cc2d5159-e55c-47fc-845e-77b83e309d88","year":2025},"citing_paper":{"arxiv_id":"2606.05277","last_updated":"2026-06-03T18:00:00Z","snapshot_observed_at":"2026-07-06T23:45:19.055840Z","submitted_at":"2026-06-03T18:00:00Z","title":"The free-streaming length of dark matter from JWST observations of 28 strong gravitational lenses","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-06-28T04:44:44.080590Z"},"links":{"cited_paper":"/paper/2511.07513","citing_paper":"/paper/2606.05277"},"observation_digest":"sha256:692f3b52072aba4f59d6b055fb6d77510483eda44260f9ef2a8f2420eee0ef54","observation_id":"b390161c-ede9-4eaa-8a0c-0b90e003109d","resolution":{"observed_at":"2026-07-02T10:56:53.243401Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":"2511.07513","doi":"10.48550/arxiv.2511.07513","metadata_source":"pith","pith_arxiv_id":"2511.07513","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"astro-ph.CO","work_id":"cc2d5159-e55c-47fc-845e-77b83e309d88","year":2025},"citing_paper":{"arxiv_id":"2606.12137","last_updated":"2026-06-10T14:32:43Z","snapshot_observed_at":"2026-07-06T23:51:07.629939Z","submitted_at":"2026-06-10T14:32:43Z","title":"A Unified Halo Mass Function Across Dark Matter Models from High-Resolution Multi-Scale Simulations","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-06-27T09:21:11.139428Z"},"links":{"cited_paper":"/paper/2511.07513","citing_paper":"/paper/2606.12137"},"observation_digest":"sha256:fa0eead45e7dbfa4c4295f384d0f7b2c0cfbaee9376892a76c2720410b84a4f3","observation_id":"d98bfe85-6a16-4b87-bb60-019874481aef","resolution":{"observed_at":"2026-06-27T09:40:47.899588Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":"2511.07513","doi":"10.48550/arxiv.2511.07513","metadata_source":"pith","pith_arxiv_id":"2511.07513","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"astro-ph.CO","work_id":"cc2d5159-e55c-47fc-845e-77b83e309d88","year":2025},"citing_paper":{"arxiv_id":"2606.12909","last_updated":"2026-06-11T05:08:09Z","snapshot_observed_at":"2026-07-06T23:51:45.306189Z","submitted_at":"2026-06-11T05:08:09Z","title":"SIDM and CDM interpretations of the million-solar-mass lensing perturber JVAS B1938+666-$\\mathcal{V}$","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-06-27T06:50:27.397229Z"},"links":{"cited_paper":"/paper/2511.07513","citing_paper":"/paper/2606.12909"},"observation_digest":"sha256:702a12f00c4d856957d5f64e82f567c8a039cef5b5ef6315e7b9144751073ac8","observation_id":"737696e6-ed3a-4583-a8f3-8117cbc38190","resolution":{"observed_at":"2026-07-03T14:58:32.873188Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":"2511.07513","doi":"10.48550/arxiv.2511.07513","metadata_source":"pith","pith_arxiv_id":"2511.07513","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"astro-ph.CO","work_id":"cc2d5159-e55c-47fc-845e-77b83e309d88","year":2025},"citing_paper":{"arxiv_id":"2606.23808","last_updated":"2026-06-22T18:00:10Z","snapshot_observed_at":"2026-08-01T15:07:14.133505Z","submitted_at":"2026-06-22T18:00:10Z","title":"First measurement of narrow-line flux ratios for a lensed quasar with JWST/NIRSpec IFS","version":1},"reference_index":191,"source":"arxiv_source","source_observed_at":"2026-06-26T07:43:38.930872Z"},"links":{"cited_paper":"/paper/2511.07513","citing_paper":"/paper/2606.23808"},"observation_digest":"sha256:22d327664a296d4197fd3b9fedfae4a83fa9d1bc25bcd7470f12da5a0abd29ea","observation_id":"bbd067cf-d9a5-4322-a09e-7b6f469f106a","resolution":{"observed_at":"2026-06-26T10:39:19.317622Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":"2511.07513","doi":"10.48550/arxiv.2511.07513","metadata_source":"pith","pith_arxiv_id":"2511.07513","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"astro-ph.CO","work_id":"cc2d5159-e55c-47fc-845e-77b83e309d88","year":2025},"citing_paper":{"arxiv_id":"2606.25028","last_updated":"2026-06-23T18:00:04Z","snapshot_observed_at":"2026-07-06T23:59:32.831481Z","submitted_at":"2026-06-23T18:00:04Z","title":"Constraining the Physical Properties of Quadruply Lensed Quasars using Optical-to-X-Ray Data","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-06-25T23:33:41.389182Z"},"links":{"cited_paper":"/paper/2511.07513","citing_paper":"/paper/2606.25028"},"observation_digest":"sha256:4aea0dde0aa068459b91292ab103984a2dae5421e2123f46d6f6745976736fd6","observation_id":"bf294726-8606-4d9d-adeb-caed6417646f","resolution":{"observed_at":"2026-07-04T17:40:00.382340Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":"2511.07513","doi":"10.48550/arxiv.2511.07513","metadata_source":"pith","pith_arxiv_id":"2511.07513","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"astro-ph.CO","work_id":"cc2d5159-e55c-47fc-845e-77b83e309d88","year":2025},"citing_paper":{"arxiv_id":"2606.30620","last_updated":"2026-06-29T17:52:31Z","snapshot_observed_at":"2026-08-02T20:46:18.398982Z","submitted_at":"2026-06-29T17:52:31Z","title":"Gaussian processes on ray-guided transformed uniform grids for fast, flexible, and auto-differentiable adaptive source reconstruction in lens modelling","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-06-30T03:15:35.000616Z"},"links":{"cited_paper":"/paper/2511.07513","citing_paper":"/paper/2606.30620"},"observation_digest":"sha256:e94e7fdf24eb8228272c3672345f08dd08f81c2da8c01b5e72a666b93f79ae66","observation_id":"951aab50-7426-4878-83e4-fd0986231cc1","resolution":{"observed_at":"2026-06-30T03:24:12.343643Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T07:50:42.937048+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2511.07513","snapshot_observed_at":"2026-07-14T04:47:48.052776Z","title":"M., Treu, T., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.11559","last_updated":"2026-07-13T13:40:31Z","snapshot_observed_at":"2026-08-04T18:08:48.537056Z","submitted_at":"2026-07-13T13:40:31Z","title":"Can third- and fourth-order multipoles plus radial variation of iso-density ellipses explain the observed flux ratios in B1422$+$231? YES, and a lesson learned from a TNG100 lensing galaxy sample","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-07-14T04:47:48.052776Z"},"links":{"cited_paper":"/paper/2511.07513","citing_paper":"/paper/2607.11559"},"observation_digest":"sha256:6ee3315cd1058c8bc68dcb216018cc4148a1d7b796d4b1b96af076294755486e","observation_id":"a787a38f-8dd8-464f-be4d-05be5830efdf","resolution":{"observed_at":"2026-07-14T04:47:48.052776Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2511.07513/citation-record","integrity":"/paper/2511.07513/integrity","json":"/paper/2511.07513/citation-record.json","paper":"/paper/2511.07513"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-03T23:07:54.064655Z","title":"Aghanim, Y","venue":null,"work_id":null,"year":2020},"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":1,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.064655Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:2ea120cd4b3e30e35c68baed3a15cf3afb594bdea68d1288152a3b550c25b8cd","observation_id":"62ea240e-e112-456b-8590-05ff46327ee4","resolution":{"observed_at":"2026-08-03T23:07:54.064655Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.08215","last_updated":"2022-12-14T04:14:44Z","snapshot_observed_at":"2026-07-06T13:53:13.702355Z","submitted_at":"2022-09-17T02:09:33Z","title":"Report of the Topical Group on Cosmic Probes of Dark Matter for Snowmass 2021","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.08215","snapshot_observed_at":"2026-08-03T23:07:54.069545Z","title":"Drlica-Wagner, C","venue":null,"work_id":null,"year":2022},"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":2,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.069545Z"},"links":{"cited_paper":"/paper/2209.08215","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:5f0953692b69f61bdde66dbb49aab47919d0c2fc00d41bb4be029315e3c5b940","observation_id":"af27b36a-58fd-4ae4-9ffe-9bccd75a6053","resolution":{"observed_at":"2026-08-03T23:07:54.069545Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9611107","last_updated":"1997-10-21T23:14:37Z","snapshot_observed_at":"2026-07-07T01:15:03.940917Z","submitted_at":"1996-11-13T22:59:55Z","title":"A Universal Density Profile from Hierarchical Clustering","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9611107","snapshot_observed_at":"2026-08-03T23:07:54.073892Z","title":null,"venue":null,"work_id":null,"year":1997},"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":3,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.073892Z"},"links":{"cited_paper":"/paper/astro-ph/9611107","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:80ade2650ab46984346bc789034174a2b4a6d3466afe99a97eb6bbb38398397f","observation_id":"8d30f6bc-2cf4-457d-b894-aad56e7a995d","resolution":{"observed_at":"2026-08-03T23:07:54.073892Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T23:07:54.078118Z","title":null,"venue":null,"work_id":null,"year":2020},"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":4,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.078118Z"},"links":{"citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:fd3ba1f961b73050d3466b8ee9b314ee4509d3f38df8d47a285ac115ac27db34","observation_id":"497ef270-d80c-4f8e-9f93-f7f3a4bdf264","resolution":{"observed_at":"2026-08-03T23:07:54.078118Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T23:07:54.081998Z","title":null,"venue":null,"work_id":null,"year":1983},"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":5,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.081998Z"},"links":{"citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:3b5a9826caf6377c07d40fb131360d68134eb8a43a2ca4ee05d387df239dc6f0","observation_id":"bc552da9-6fba-4f66-83ec-8e5b037a2917","resolution":{"observed_at":"2026-08-03T23:07:54.081998Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0004115","last_updated":"2000-06-06T00:06:27Z","snapshot_observed_at":"2026-07-07T00:10:49.177459Z","submitted_at":"2000-04-07T23:38:28Z","title":"Substructure and halo density profiles in a Warm Dark Matter Cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0004115","snapshot_observed_at":"2026-08-03T23:07:54.086496Z","title":"Col ´ ın, V","venue":null,"work_id":null,"year":2000},"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":6,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.086496Z"},"links":{"cited_paper":"/paper/astro-ph/0004115","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:0cb4a710a48f6fc80215ae54c4bc6d4d5e8d9b809070c88c9d8be6880b839da9","observation_id":"a013e6d2-23d7-460f-991e-d89ba9273779","resolution":{"observed_at":"2026-08-03T23:07:54.086496Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T23:07:54.090384Z","title":"Avila-Reese, P","venue":null,"work_id":null,"year":2001},"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":7,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.090384Z"},"links":{"citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:93a731b902697a2000312a7bf43a12f3ef32b240309d494a676d2f8b81bff23b","observation_id":"69673dc9-0bed-4c4c-af9d-1dca18e5e475","resolution":{"observed_at":"2026-08-03T23:07:54.090384Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.0839","last_updated":"2013-06-11T10:21:04Z","snapshot_observed_at":"2026-07-06T03:07:57.150020Z","submitted_at":"2013-03-04T21:00:02Z","title":"Halo Mass Function and the Free Streaming Scale","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.0839","snapshot_observed_at":"2026-08-03T23:07:54.094007Z","title":"Schneider, R","venue":null,"work_id":null,"year":2013},"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":8,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.094007Z"},"links":{"cited_paper":"/paper/1303.0839","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:e46e39a60578d38ff766730ac187e0e4229b19e189714f10dc4e4be0bffb5463","observation_id":"d9741b8f-a945-4543-9c62-597a986ede71","resolution":{"observed_at":"2026-08-03T23:07:54.094007Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.11781","last_updated":"2023-06-20T18:00:00Z","snapshot_observed_at":"2026-07-06T15:44:46.456226Z","submitted_at":"2023-06-20T18:00:00Z","title":"Strong gravitational lensing as a probe of dark matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.11781","snapshot_observed_at":"2026-08-03T23:07:54.098158Z","title":"Vegetti, S","venue":null,"work_id":null,"year":2024},"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":9,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.098158Z"},"links":{"cited_paper":"/paper/2306.11781","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:b91287d3233fe1029c239711ec235b11888d2306c5fda0c53f9c0916ac099086","observation_id":"874ddf0d-b2a3-497e-9943-1b0b8153171c","resolution":{"observed_at":"2026-08-03T23:07:54.098158Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.00022","last_updated":"2021-03-01T18:00:36Z","snapshot_observed_at":"2026-07-06T09:43:35.929296Z","submitted_at":"2020-07-31T18:13:09Z","title":"Milky Way Satellite Census. III. Constraints on Dark Matter Properties from Observations of Milky Way Satellite Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.00022","snapshot_observed_at":"2026-08-03T23:07:54.102327Z","title":null,"venue":null,"work_id":null,"year":2021},"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":10,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.102327Z"},"links":{"cited_paper":"/paper/2008.00022","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:d06884da3f734d4e57b9299b27fe3dd0af7fbc632e5f8cd92c51883158f0eef5","observation_id":"3da1eb0b-ecb5-49b8-a938-5de5050d098d","resolution":{"observed_at":"2026-08-03T23:07:54.102327Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.02958","last_updated":"2020-07-06T18:00:04Z","snapshot_observed_at":"2026-07-06T09:35:50.977461Z","submitted_at":"2020-07-06T18:00:04Z","title":"Constraining Velocity-dependent Self-Interacting Dark Matter with the Milky Way's dwarf spheroidal galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.02958","snapshot_observed_at":"2026-08-03T23:07:54.106232Z","title":null,"venue":null,"work_id":null,"year":2021},"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":11,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.106232Z"},"links":{"cited_paper":"/paper/2007.02958","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:57ca6355eb5c867c0c299b8cd00242e70501635529b93f9d49bd9d2a68d2173c","observation_id":"dfc40308-a582-4992-9b01-2ea99bb13dae","resolution":{"observed_at":"2026-08-03T23:07:54.106232Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.13137","last_updated":"2023-01-19T21:40:55Z","snapshot_observed_at":"2026-07-06T12:12:10.536267Z","submitted_at":"2021-11-25T15:49:40Z","title":"Warm Dark Matter Constraints Using Milky-Way Satellite Observations and Subhalo Evolution Modeling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.13137","snapshot_observed_at":"2026-08-03T23:07:54.110110Z","title":"Dekker, S","venue":null,"work_id":null,"year":2022},"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":12,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.110110Z"},"links":{"cited_paper":"/paper/2111.13137","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:043b8bd9645cc97f8fc4e6b865dc6cfb8dbf2e7d641cd3b573c87f33579a3afd","observation_id":"950a0f7e-4f1e-4922-bb9f-b6f32d896a4c","resolution":{"observed_at":"2026-08-03T23:07:54.110110Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.03631","last_updated":"2019-06-13T17:48:14Z","snapshot_observed_at":"2026-08-05T08:38:48.431670Z","submitted_at":"2018-11-08T19:00:03Z","title":"The Spur and the Gap in GD-1: Dynamical evidence for a dark substructure in the Milky Way halo","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.03631","snapshot_observed_at":"2026-08-03T23:07:54.114143Z","title":"Bonaca, D","venue":null,"work_id":null,"year":2019},"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":13,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.114143Z"},"links":{"cited_paper":"/paper/1811.03631","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:2e0c028c59f787d496d203c1f7e272788f946dfc14a2b508396f6e966bc11a1d","observation_id":"c6073f13-711f-43e7-8fe8-270a54846782","resolution":{"observed_at":"2026-08-03T23:07:54.114143Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.02663","last_updated":"2021-09-27T18:29:50Z","snapshot_observed_at":"2026-08-06T03:23:26.539762Z","submitted_at":"2019-11-06T22:53:26Z","title":"Novel constraints on the particle nature of dark matter from stellar streams","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.02663","snapshot_observed_at":"2026-08-03T23:07:54.118032Z","title":"Banik, J","venue":null,"work_id":null,"year":2021},"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":14,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.118032Z"},"links":{"cited_paper":"/paper/1911.02663","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:2953369dd2380469018c829288586e4166257c235df235503e8d16979e774203","observation_id":"5ad1eedb-eae6-4235-9aa5-0f373191b1de","resolution":{"observed_at":"2026-08-03T23:07:54.118032Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2510.02247","last_updated":"2026-06-04T17:04:11Z","snapshot_observed_at":"2026-08-04T12:47:20.357820Z","submitted_at":"2025-10-02T17:35:18Z","title":"Measurement of Substructure from the Kinematics of the GD-1 Stellar Stream","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2510.02247","snapshot_observed_at":"2026-08-03T23:07:54.121899Z","title":"Nibauer, A","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":15,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.121899Z"},"links":{"cited_paper":"/paper/2510.02247","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:ed455f958225809a4c48ba7db5d7f8cf6896b7058d982e309f22c25aa2cbd8f1","observation_id":"9f43ae88-f191-449e-a46b-730412bcc907","resolution":{"observed_at":"2026-08-03T23:07:54.121899Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9707187","last_updated":"1997-07-16T15:31:36Z","snapshot_observed_at":"2026-07-07T01:17:47.359349Z","submitted_at":"1997-07-16T15:31:36Z","title":"Evidence for substructure in lens galaxies?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9707187","snapshot_observed_at":"2026-08-03T23:07:54.125691Z","title":"Mao and P","venue":null,"work_id":null,"year":1998},"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":16,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.125691Z"},"links":{"cited_paper":"/paper/astro-ph/9707187","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:b3ffccfad79b9f10b227f8125bca206e412851e37d46d9a91dc214d0d7fb17f0","observation_id":"de6f6b49-908f-461d-99c3-cdc4eeffc752","resolution":{"observed_at":"2026-08-03T23:07:54.125691Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.1496","last_updated":"2014-05-13T19:21:47Z","snapshot_observed_at":"2026-07-06T03:35:20.649520Z","submitted_at":"2014-02-06T21:00:18Z","title":"Detection of substructure with adaptive optics integral field spectroscopy of the gravitational lens B1422+231","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.1496","snapshot_observed_at":"2026-08-03T23:07:54.129615Z","title":null,"venue":null,"work_id":null,"year":2014},"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":17,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.129615Z"},"links":{"cited_paper":"/paper/1402.1496","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:925735e65f99f0e3e73b1cd2432bd28c548e3443b43f34e5d188225df04a59e3","observation_id":"2c888951-ae3d-4409-b8eb-db6336ba2668","resolution":{"observed_at":"2026-08-03T23:07:54.129615Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.05188","last_updated":"2017-06-13T13:22:21Z","snapshot_observed_at":"2026-08-02T05:53:40.052761Z","submitted_at":"2017-01-18T19:00:00Z","title":"Probing dark matter substructure in the gravitational lens HE0435-1223 with the WFC3 grism","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.05188","snapshot_observed_at":"2026-08-03T23:07:54.133726Z","title":null,"venue":null,"work_id":null,"year":2017},"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":18,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.133726Z"},"links":{"cited_paper":"/paper/1701.05188","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:0752ca8b0c557eed15d9b76f2c7857efb9394146ae0f86ee521be6338af1ba3d","observation_id":"d3449ff0-f320-43c7-a49d-e5ecb7d21a2e","resolution":{"observed_at":"2026-08-03T23:07:54.133726Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.00009","last_updated":"2017-05-18T17:20:33Z","snapshot_observed_at":"2026-07-06T05:28:15.588242Z","submitted_at":"2017-01-31T19:00:00Z","title":"Lensing substructure quantification in RXJ1131-1231: A 2 keV lower bound on dark matter thermal relic mass","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.00009","snapshot_observed_at":"2026-08-03T23:07:54.137595Z","title":"Birrer, A","venue":null,"work_id":null,"year":2017},"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":19,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.137595Z"},"links":{"cited_paper":"/paper/1702.00009","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:80bc33f15039c6e486c01b19d7ba4f269d1cb1755901333b528d0b75d0df9578","observation_id":"b987bc19-3c07-4516-937f-dad8a045affb","resolution":{"observed_at":"2026-08-03T23:07:54.137595Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.13221","last_updated":"2022-02-09T13:53:32Z","snapshot_observed_at":"2026-08-06T21:08:17.219331Z","submitted_at":"2020-10-25T21:09:13Z","title":"A forward-modelling method to infer the dark matter particle mass from strong gravitational lenses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.13221","snapshot_observed_at":"2026-08-03T23:07:54.141372Z","title":null,"venue":null,"work_id":null,"year":2022},"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":20,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.141372Z"},"links":{"cited_paper":"/paper/2010.13221","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:2b6916bcc2c8b55ffe0a47d57278ca218834f000885cbde384bd44112f74df7f","observation_id":"faf307a1-c885-468a-aeb4-eb9ec5b5f822","resolution":{"observed_at":"2026-08-03T23:07:54.141372Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.03375","last_updated":"2022-08-18T09:14:19Z","snapshot_observed_at":"2026-08-07T00:17:02.401870Z","submitted_at":"2022-07-07T15:30:28Z","title":"A lensed radio jet at milli-arcsecond resolution I: Bayesian comparison of parametric lens models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.03375","snapshot_observed_at":"2026-08-03T23:07:54.145111Z","title":null,"venue":null,"work_id":null,"year":2022},"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":21,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.145111Z"},"links":{"cited_paper":"/paper/2207.03375","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:067aba8ce66c0fa5f0308bc149a77419c7fb1933c99b6cbeb1c31fd102ae9329","observation_id":"491ab284-8e41-47c9-bbf8-13760b7f1c99","resolution":{"observed_at":"2026-08-03T23:07:54.145111Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.14487","last_updated":"2024-04-22T18:00:01Z","snapshot_observed_at":"2026-08-05T04:13:28.474087Z","submitted_at":"2024-04-22T18:00:01Z","title":"A Strong Gravitational Lens Is Worth a Thousand Dark Matter Halos: Inference on Small-Scale Structure Using Sequential Methods","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.14487","snapshot_observed_at":"2026-08-03T23:07:54.148991Z","title":"Wagner-Carena, J","venue":null,"work_id":null,"year":2024},"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":22,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.148991Z"},"links":{"cited_paper":"/paper/2404.14487","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:dde3347dc170a76c104e56de4cfce563d140d373bff83ffe5065ae3d7b9081da","observation_id":"c803db95-3c0c-4b1b-930e-68ae1bafdc42","resolution":{"observed_at":"2026-08-03T23:07:54.148991Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T23:07:54.152832Z","title":null,"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":23,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.152832Z"},"links":{"citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:565137ffdd0eddafc604a14cb1105862c85d8793117effa6c24ecff01d994bdc","observation_id":"3e168a6d-698d-4dc7-a5ef-30e9ed1b75e8","resolution":{"observed_at":"2026-08-03T23:07:54.152832Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.3643","last_updated":"2012-01-17T21:46:57Z","snapshot_observed_at":"2026-08-03T20:29:46.044299Z","submitted_at":"2012-01-17T21:46:57Z","title":"Gravitational detection of a low-mass dark satellite at cosmological distance","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.3643","snapshot_observed_at":"2026-08-03T23:07:54.156515Z","title":"Vegetti, D","venue":null,"work_id":null,"year":2012},"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":24,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.156515Z"},"links":{"cited_paper":"/paper/1201.3643","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:bae92f4795be6adeab89e03f0de7e5f0555c543f8409c3d1f40ca62282b087af","observation_id":"b9ae2e01-58d2-40d3-a8b1-0cb9d699939d","resolution":{"observed_at":"2026-08-03T23:07:54.156515Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.3666","last_updated":"2014-06-04T11:45:52Z","snapshot_observed_at":"2026-08-03T19:05:39.954633Z","submitted_at":"2014-05-14T20:00:30Z","title":"Inference of the Cold Dark Matter substructure mass function at z=0.2 using strong gravitational lenses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.3666","snapshot_observed_at":"2026-08-03T23:07:54.160373Z","title":"Vegetti, L","venue":null,"work_id":null,"year":2017},"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":25,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.160373Z"},"links":{"cited_paper":"/paper/1405.3666","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:6c686b334cd6e4b16352eb832bc08d3080000bbb1c2951789a1fe82c6a73493e","observation_id":"27d39617-0671-4e74-86c9-7a39c338a2c1","resolution":{"observed_at":"2026-08-03T23:07:54.160373Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.01388","last_updated":"2016-01-07T03:39:18Z","snapshot_observed_at":"2026-07-06T04:42:05.827933Z","submitted_at":"2016-01-07T03:39:18Z","title":"Detection of lensing substructure using ALMA observations of the dusty galaxy SDP.81","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.01388","snapshot_observed_at":"2026-08-03T23:07:54.164351Z","title":null,"venue":null,"work_id":null,"year":2016},"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":26,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.164351Z"},"links":{"cited_paper":"/paper/1601.01388","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:f389dd2f58b371c34b304e7aa02acbcf39c568ff57d29d911c9b6bc4bca331ca","observation_id":"abe1992d-6a98-4023-8bb4-3262374011ef","resolution":{"observed_at":"2026-08-03T23:07:54.164351Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.10627","last_updated":"2020-11-20T20:37:11Z","snapshot_observed_at":"2026-07-06T10:16:31.843825Z","submitted_at":"2020-11-20T20:37:11Z","title":"An unexpected high concentration for the dark substructure in the gravitational lens SDSSJ0946+1006","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.10627","snapshot_observed_at":"2026-08-03T23:07:54.168266Z","title":"Minor, S","venue":null,"work_id":null,"year":2021},"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":27,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.168266Z"},"links":{"cited_paper":"/paper/2011.10627","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:a765067123fbb5e510e599762e2bd7901c1bb356248b00944ef962c1ec90b52d","observation_id":"15252d8d-5ee0-4866-81c3-50f5f21a84f6","resolution":{"observed_at":"2026-08-03T23:07:54.168266Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.08718","last_updated":"2021-12-04T20:34:39Z","snapshot_observed_at":"2026-08-04T05:25:21.156336Z","submitted_at":"2021-11-16T19:00:01Z","title":"Detecting low-mass haloes with strong gravitational lensing I: the effect of data quality and lensing configuration","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.08718","snapshot_observed_at":"2026-08-03T23:07:54.172041Z","title":"Despali, S","venue":null,"work_id":null,"year":2022},"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":28,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.172041Z"},"links":{"cited_paper":"/paper/2111.08718","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:3fae0cbf85da49d1a7f209e68fb3001c90b18c726a2a6e21d2c2347d9cbfdb50","observation_id":"ac1a84c2-8c79-480b-b034-68d4712ecb31","resolution":{"observed_at":"2026-08-03T23:07:54.172041Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.00749","last_updated":"2022-07-08T18:09:39Z","snapshot_observed_at":"2026-08-04T18:08:03.268230Z","submitted_at":"2021-12-01T19:00:01Z","title":"Substructure Detection Reanalyzed: Dark Perturber shown to be a Line-of-Sight Halo","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.00749","snapshot_observed_at":"2026-08-03T23:07:54.176016Z","title":null,"venue":null,"work_id":null,"year":2022},"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":29,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.176016Z"},"links":{"cited_paper":"/paper/2112.00749","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:2c22093329f5cfc9f7c57eab1cb88e8e9a7d547a7a5eebc21607f04653db0607","observation_id":"f922ddf5-f873-4dcd-9843-0f9ef61582fd","resolution":{"observed_at":"2026-08-03T23:07:54.176016Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.11090","last_updated":"2025-01-31T18:46:59Z","snapshot_observed_at":"2026-07-06T19:03:39.672411Z","submitted_at":"2024-08-20T18:00:01Z","title":"High detection significance of the dark substructure in gravitational lens SDSSJ0946+1006 by image pixel supersampling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.11090","snapshot_observed_at":"2026-08-03T23:07:54.179948Z","title":null,"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":30,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.179948Z"},"links":{"cited_paper":"/paper/2408.11090","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:e19804ba0c28f5fc78a0c16427718aa8198ddda964694e348de1f1e83df395f3","observation_id":"7afe2414-18be-4bfa-bab7-f93f473ed612","resolution":{"observed_at":"2026-08-03T23:07:54.179948Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.12987","last_updated":"2025-03-23T16:37:32Z","snapshot_observed_at":"2026-07-06T19:34:55.594468Z","submitted_at":"2024-10-16T19:32:47Z","title":"Galaxy Mass Modelling from Multi-Wavelength JWST Strong Lens Analysis: Dark Matter Substructure, Angular Mass Complexity, or Both?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.12987","snapshot_observed_at":"2026-08-03T23:07:54.183753Z","title":null,"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":31,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.183753Z"},"links":{"cited_paper":"/paper/2410.12987","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:d8f90949e320422727c6a44c3d3eb4e30b9b82642ef89649c276bbead21a6d7b","observation_id":"a7ee5344-67fa-4988-9165-eb079c63eb57","resolution":{"observed_at":"2026-08-03T23:07:54.183753Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08565","last_updated":"2024-11-13T12:25:21Z","snapshot_observed_at":"2026-08-06T04:47:29.111205Z","submitted_at":"2024-11-13T12:25:21Z","title":"The overconcentrated dark halo in the strong lens SDSS J0946+1006 is a subhalo: evidence for self interacting dark matter?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08565","snapshot_observed_at":"2026-08-03T23:07:54.187723Z","title":null,"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":32,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.187723Z"},"links":{"cited_paper":"/paper/2411.08565","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:72e91d5246496aab3d15bd5f7526f134a1e2ce54c0116ac334b5b1fa84d1eb52","observation_id":"4a9ce28c-71ac-44ea-a8c6-9316f32211c9","resolution":{"observed_at":"2026-08-03T23:07:54.187723Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.07978","last_updated":"2025-06-09T17:50:57Z","snapshot_observed_at":"2026-07-06T21:39:13.304260Z","submitted_at":"2025-06-09T17:50:57Z","title":"Not so dark, not so dense: an alternative explanation for the lensing subhalo in SDSSJ0946+1006","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.07978","snapshot_observed_at":"2026-08-03T23:07:54.191586Z","title":null,"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":33,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.191586Z"},"links":{"cited_paper":"/paper/2506.07978","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:bd2d950ab9f7280181f3af5b72a6293ac04265b33f4cb3dadf796a9eb06f4ebf","observation_id":"45238ad2-a555-4777-a345-22c206b999a8","resolution":{"observed_at":"2026-08-03T23:07:54.191586Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T23:07:54.195675Z","title":null,"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":34,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.195675Z"},"links":{"citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:189682d0346d5974e9057ecd5c0aeb5a36bec0b874f852594f4c8b5d1715eb91","observation_id":"b27adf07-9744-4294-a674-30065f8ba447","resolution":{"observed_at":"2026-08-03T23:07:54.195675Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.11031","last_updated":"2019-07-26T21:29:44Z","snapshot_observed_at":"2026-08-04T20:15:48.557905Z","submitted_at":"2019-01-30T19:00:01Z","title":"Probing dark matter structure down to $10^7$ solar masses: flux ratio statistics in gravitational lenses with line of sight halos","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.11031","snapshot_observed_at":"2026-08-03T23:07:54.199398Z","title":"Gilman, S","venue":null,"work_id":null,"year":2019},"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":35,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.199398Z"},"links":{"cited_paper":"/paper/1901.11031","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:92d56b766df7c00d17f8a832162851c12b33b6dd1fab410a59b9ca9ed36ddd7e","observation_id":"573708b3-738b-4810-ab0f-f2e634bcfe15","resolution":{"observed_at":"2026-08-03T23:07:54.199398Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0111456","last_updated":"2002-04-02T21:50:23Z","snapshot_observed_at":"2026-07-07T00:23:23.601338Z","submitted_at":"2001-11-23T13:57:42Z","title":"Direct Detection of CDM Substructure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0111456","snapshot_observed_at":"2026-08-03T23:07:54.203182Z","title":"Dalal and C","venue":null,"work_id":null,"year":2002},"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":36,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.203182Z"},"links":{"cited_paper":"/paper/astro-ph/0111456","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:5742bb66acc298cd90cef589f33f4c0705aa0dbac11f12cd4bbd556d77148672","observation_id":"5c79ef3a-16d9-494c-aa0d-afea5b0930fd","resolution":{"observed_at":"2026-08-03T23:07:54.203182Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.04182","last_updated":"2019-12-19T10:51:41Z","snapshot_observed_at":"2026-08-05T15:21:15.488057Z","submitted_at":"2019-05-10T14:09:36Z","title":"SHARP -- VII. New constraints on the dark matter free-streaming properties and substructure abundance from gravitationally lensed quasars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.04182","snapshot_observed_at":"2026-08-03T23:07:54.207016Z","title":null,"venue":null,"work_id":null,"year":2020},"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":37,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.207016Z"},"links":{"cited_paper":"/paper/1905.04182","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:48483a4c1b3a0290c1a63f7c06b9128d6f706b621a8712f998161596deab881d","observation_id":"a8a6a28f-7d13-4c28-9648-da27041c75f3","resolution":{"observed_at":"2026-08-03T23:07:54.207016Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.06983","last_updated":"2019-11-11T09:16:51Z","snapshot_observed_at":"2026-08-05T20:45:56.749196Z","submitted_at":"2019-08-19T18:00:01Z","title":"Warm dark matter chills out: constraints on the halo mass function and the free-streaming length of dark matter with 8 quadruple-image strong gravitational lenses","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.06983","snapshot_observed_at":"2026-08-03T23:07:54.211243Z","title":"Gilman, S","venue":null,"work_id":null,"year":2020},"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":38,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.211243Z"},"links":{"cited_paper":"/paper/1908.06983","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:259bf6d4db231734a2c5b7e1f572cbefd08709352e2529e745850ce5ead55b98","observation_id":"0abeee40-6296-469d-82db-e86a16787710","resolution":{"observed_at":"2026-08-03T23:07:54.211243Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.07265","last_updated":"2023-08-30T21:06:52Z","snapshot_observed_at":"2026-08-05T16:36:51.246623Z","submitted_at":"2023-01-18T02:11:04Z","title":"Pushing the Limits of Detectability: Mixed Dark Matter from Strong Gravitational Lenses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.07265","snapshot_observed_at":"2026-08-03T23:07:54.215014Z","title":null,"venue":null,"work_id":null,"year":2023},"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":39,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.215014Z"},"links":{"cited_paper":"/paper/2301.07265","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:e3e2a531afacc30a6a0a000cc2d5bfbc5946c77f8316c0ea30a42b6fc0a9bb46","observation_id":"433385c1-5dad-471b-a4b8-6a0c77f501d6","resolution":{"observed_at":"2026-08-03T23:07:54.215014Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T23:07:54.058962Z","title":"CAREER: An order of magnitude improvement in measurements of the physical properties of dark matter","venue":null,"work_id":null,"year":2023},"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":40,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.058962Z"},"links":{"citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:3b143f197b77f8fee81b3ff5424a0a820af750b627c7590c988f9290aed55aaa","observation_id":"298a9577-f84b-4166-acc4-2dd0c250bf20","resolution":{"observed_at":"2026-08-03T23:07:54.058962Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.01620","last_updated":"2024-05-02T17:50:31Z","snapshot_observed_at":"2026-08-04T00:50:28.394911Z","submitted_at":"2024-05-02T17:50:31Z","title":"JWST Lensed quasar dark matter survey II: Strongest gravitational lensing limit on the dark matter free streaming length to date","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.01620","snapshot_observed_at":"2026-08-03T23:07:54.219004Z","title":null,"venue":null,"work_id":null,"year":2024},"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":41,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.219004Z"},"links":{"cited_paper":"/paper/2405.01620","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:e3b12f2fa405a593de5289bbb6703ec90d3ec16c05c1fa99576cb6092e4985f9","observation_id":"656bf277-cd9a-4b39-b2b8-5421c089cb2d","resolution":{"observed_at":"2026-08-03T23:07:54.219004Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.05259","last_updated":"2021-09-05T23:25:44Z","snapshot_observed_at":"2026-08-02T19:07:58.564521Z","submitted_at":"2021-05-11T18:00:02Z","title":"Strong lensing signatures of self-interacting dark matter in low-mass halos","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.05259","snapshot_observed_at":"2026-08-03T23:07:54.223372Z","title":"Gilman, J","venue":null,"work_id":null,"year":2021},"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":42,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.223372Z"},"links":{"cited_paper":"/paper/2105.05259","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:3cbd51a132daef67dac5ebf184d2b286b05ec0dbcd64dffa4a0ee6904614889b","observation_id":"2d39190c-a4c3-4bce-9f8e-fe724069db63","resolution":{"observed_at":"2026-08-03T23:07:54.223372Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.13111","last_updated":"2023-05-08T18:17:13Z","snapshot_observed_at":"2026-07-06T13:35:39.787667Z","submitted_at":"2022-07-26T18:01:51Z","title":"Constraining resonant dark matter self-interactions with strong gravitational lenses","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.13111","snapshot_observed_at":"2026-08-03T23:07:54.227729Z","title":"Gilman, Y.-M","venue":null,"work_id":null,"year":2023},"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":43,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.227729Z"},"links":{"cited_paper":"/paper/2207.13111","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:e5b58181b65502fca5bce84a4ba40ea771f551f3e0d59e941a466758f344f5a4","observation_id":"7896432c-ae47-49fe-9731-fbfea27d271a","resolution":{"observed_at":"2026-08-03T23:07:54.227729Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.09493","last_updated":"2023-04-28T00:21:05Z","snapshot_observed_at":"2026-07-06T14:06:56.291161Z","submitted_at":"2022-10-18T00:29:24Z","title":"Strong lensing constraints on primordial black holes as a dark matter candidate","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.09493","snapshot_observed_at":"2026-08-03T23:07:54.231861Z","title":null,"venue":null,"work_id":null,"year":2023},"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":44,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.231861Z"},"links":{"cited_paper":"/paper/2210.09493","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:15818131b454bcdcf70ff14ff2e2777dad9459681f26b4ad29754050918f26e3","observation_id":"79bcc56a-c3f2-4b23-a3cf-366acc2756f7","resolution":{"observed_at":"2026-08-03T23:07:54.231861Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.10473","last_updated":"2020-08-10T18:05:47Z","snapshot_observed_at":"2026-07-06T08:59:42.044090Z","submitted_at":"2020-02-24T19:00:05Z","title":"Multiple Images and Flux Ratio Anomaly of Fuzzy Gravitational Lenses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.10473","snapshot_observed_at":"2026-08-03T23:07:54.236058Z","title":null,"venue":null,"work_id":null,"year":2020},"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":45,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.236058Z"},"links":{"cited_paper":"/paper/2002.10473","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:5d415a23128ddf05ecbf2eaca4311226a6382fd87eef13c15ab7852d2a035b5c","observation_id":"b25afe77-ded2-4238-8f76-e2f1204d4e7e","resolution":{"observed_at":"2026-08-03T23:07:54.236058Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.11269","last_updated":"2022-09-15T16:39:05Z","snapshot_observed_at":"2026-07-06T13:23:40.750177Z","submitted_at":"2022-06-22T18:00:00Z","title":"Quantum fluctuations masquerade as halos: Bounds on ultra-light dark matter from quadruply-imaged quasars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.11269","snapshot_observed_at":"2026-08-03T23:07:54.240133Z","title":"Laroche, D","venue":null,"work_id":null,"year":2022},"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":46,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.240133Z"},"links":{"cited_paper":"/paper/2206.11269","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:f96b9d5926bad9b09375d13644d277602eb05b090bdf1e56345629e41e30622d","observation_id":"503c8849-8af7-4aba-a55c-88a780019782","resolution":{"observed_at":"2026-08-03T23:07:54.240133Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0304292","last_updated":"2003-07-27T20:10:36Z","snapshot_observed_at":"2026-07-07T00:32:43.377098Z","submitted_at":"2003-04-15T21:17:52Z","title":"Halo Substructure And The Power Spectrum","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0304292","snapshot_observed_at":"2026-08-03T23:07:54.244091Z","title":null,"venue":null,"work_id":null,"year":2003},"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":47,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.244091Z"},"links":{"cited_paper":"/paper/astro-ph/0304292","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:27479265a8754246be110ea45c6d83bd41697ededa6893f2f5c215369a366769","observation_id":"c612b825-74ed-4a1a-9690-20b62c0a99f0","resolution":{"observed_at":"2026-08-03T23:07:54.244091Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03293","last_updated":"2022-03-09T19:00:13Z","snapshot_observed_at":"2026-07-06T12:15:54.864685Z","submitted_at":"2021-12-06T19:00:04Z","title":"The primordial matter power spectrum on sub-galactic scales","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.03293","snapshot_observed_at":"2026-08-03T23:07:54.248337Z","title":"Gilman, A","venue":null,"work_id":null,"year":2022},"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":48,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.248337Z"},"links":{"cited_paper":"/paper/2112.03293","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:c01d5c98d68f15f738c4e8de32f49f888cb01685fa520f62c39debc5e0b7c3b7","observation_id":"8d7a3de4-3e31-4881-a332-c4d77347daa5","resolution":{"observed_at":"2026-08-03T23:07:54.248337Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T23:07:54.252212Z","title":"Nierenberg, V","venue":null,"work_id":null,"year":2046},"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":49,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.252212Z"},"links":{"citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:b9a59855948d48737d283a8d7cd431caa8b203021cb3a908743f12106a725c5e","observation_id":"78438a3c-8593-4aeb-8d8c-e29e047d08e1","resolution":{"observed_at":"2026-08-03T23:07:54.252212Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.10101","last_updated":"2023-09-18T19:23:26Z","snapshot_observed_at":"2026-07-30T21:52:50.834111Z","submitted_at":"2023-09-18T19:23:26Z","title":"JWST lensed quasar dark matter survey I: Description and First Results","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.10101","snapshot_observed_at":"2026-08-03T23:07:54.255840Z","title":null,"venue":null,"work_id":null,"year":2024},"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":50,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.255840Z"},"links":{"cited_paper":"/paper/2309.10101","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:29c1175bc80562992ac5b7d27a494f0592c5abb684597180ad5d75d20fcfb2bc","observation_id":"d637b9c1-20f8-48c3-8547-7f0b269ca505","resolution":{"observed_at":"2026-08-03T23:07:54.255840Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.1176","last_updated":"2013-06-06T13:43:58Z","snapshot_observed_at":"2026-08-04T15:02:13.286282Z","submitted_at":"2013-03-05T21:00:00Z","title":"Mid-infrared microlensing of accretion disc and dusty torus in quasars: effects on flux ratio anomalies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.1176","snapshot_observed_at":"2026-08-03T23:07:54.260133Z","title":"Sluse, M","venue":null,"work_id":null,"year":2013},"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":51,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.260133Z"},"links":{"cited_paper":"/paper/1303.1176","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:fac49ad96cebc81fd93670d616dd455856b966aa9251772070968381e3a70490","observation_id":"2fbe1116-c081-4ad3-ae7e-2d6e421d13bf","resolution":{"observed_at":"2026-08-03T23:07:54.260133Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0206176","last_updated":"2002-06-11T18:58:03Z","snapshot_observed_at":"2026-07-07T00:26:54.739118Z","submitted_at":"2002-06-11T18:58:03Z","title":"Detecting dark matter substructure spectroscopically in strong gravitational lenses","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0206176","snapshot_observed_at":"2026-08-03T23:07:54.264082Z","title":null,"venue":null,"work_id":null,"year":2003},"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":52,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.264082Z"},"links":{"cited_paper":"/paper/astro-ph/0206176","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:5f0fdd3332a9935017967d81c51851b436eed86064ac0c0cda3e837e46a0addf","observation_id":"88b75f4c-c6ca-4665-bb21-a00d63d5ba35","resolution":{"observed_at":"2026-08-03T23:07:54.264082Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.06344","last_updated":"2019-12-17T00:08:11Z","snapshot_observed_at":"2026-07-06T08:15:02.222269Z","submitted_at":"2019-08-17T22:44:16Z","title":"Double dark matter vision: twice the number of compact-source lenses with narrow-line lensing and the WFC3 grism","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.06344","snapshot_observed_at":"2026-08-03T23:07:54.267981Z","title":null,"venue":null,"work_id":null,"year":2020},"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":53,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.267981Z"},"links":{"cited_paper":"/paper/1908.06344","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:e2763b5c89d03173542a48a77d5c6ac38b6329db58bc38339a65fec2dded59f4","observation_id":"533bf313-8315-4072-beec-03f8bb4a0575","resolution":{"observed_at":"2026-08-03T23:07:54.267981Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0302189","last_updated":"2003-06-09T18:36:12Z","snapshot_observed_at":"2026-07-07T00:31:16.079633Z","submitted_at":"2003-02-11T19:43:15Z","title":"Extrinsic Radio Variability of JVAS/CLASS Gravitational Lenses","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0302189","snapshot_observed_at":"2026-08-03T23:07:54.271776Z","title":null,"venue":null,"work_id":null,"year":2003},"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":54,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.271776Z"},"links":{"cited_paper":"/paper/astro-ph/0302189","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:e55ad46545526af3695f58e60f3e5495f3439cbc6f9e19c92ab5515d9275f3b4","observation_id":"11f7f2cb-15d0-4ed1-9b0d-d61feed5b7ed","resolution":{"observed_at":"2026-08-03T23:07:54.271776Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0611215","last_updated":"2007-03-16T14:17:48Z","snapshot_observed_at":"2026-07-07T01:04:23.374410Z","submitted_at":"2006-11-07T14:22:33Z","title":"High resolution imaging of the anomalous flux-ratio gravitational lens system CLASS B2045+265: Dark or luminous satellites?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0611215","snapshot_observed_at":"2026-08-03T23:07:54.275788Z","title":null,"venue":null,"work_id":null,"year":2007},"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":55,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.275788Z"},"links":{"cited_paper":"/paper/astro-ph/0611215","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:1215156d35823bb419c2272ed0dab3f604f4765da8a1c09e0898ecf001d79473","observation_id":"4914d5e0-5fdd-41a6-b0c0-56736b023c3c","resolution":{"observed_at":"2026-08-03T23:07:54.275788Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.08525","last_updated":"2016-10-26T20:00:13Z","snapshot_observed_at":"2026-07-06T05:16:11.368290Z","submitted_at":"2016-10-26T20:00:13Z","title":"Strong lensing signatures of luminous structure and substructure in early-type galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.08525","snapshot_observed_at":"2026-08-03T23:07:54.279870Z","title":"Gilman, A","venue":null,"work_id":null,"year":2017},"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":56,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.279870Z"},"links":{"cited_paper":"/paper/1610.08525","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:5fc8b95adcf25befedcf79675a3eeb939fc382dccd739ae751ecf2925d197b47","observation_id":"a0e153f3-89ac-4cf5-a2f4-55790aeffc73","resolution":{"observed_at":"2026-08-03T23:07:54.279870Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.07680","last_updated":"2018-01-10T18:30:06Z","snapshot_observed_at":"2026-08-01T11:23:02.801225Z","submitted_at":"2017-07-24T18:00:00Z","title":"Flux-ratio anomalies from discs and other baryonic structures in the Illustris simulation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.07680","snapshot_observed_at":"2026-08-03T23:07:54.283886Z","title":"Hsueh, G","venue":null,"work_id":null,"year":2018},"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":57,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.283886Z"},"links":{"cited_paper":"/paper/1707.07680","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:cac8733f7e4198d445e5b5107b01e3cac6db487584492b0dff6c47b2cbb4ca00","observation_id":"70b48bd6-9c79-4f1e-9f2c-9e9247353616","resolution":{"observed_at":"2026-08-03T23:07:54.283886Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.08895","last_updated":"2024-03-15T20:02:36Z","snapshot_observed_at":"2026-07-06T17:44:12.972220Z","submitted_at":"2024-03-13T18:36:44Z","title":"General Multipoles and Their Implications for Dark Matter Inference","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.08895","snapshot_observed_at":"2026-08-03T23:07:54.288379Z","title":null,"venue":null,"work_id":null,"year":2024},"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":58,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.288379Z"},"links":{"cited_paper":"/paper/2403.08895","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:6cb66707896a0f6c3171932d40f99d8f728f0da479ac321bf9a51caea29967ed","observation_id":"9826c5ef-6568-40af-863b-57568d448790","resolution":{"observed_at":"2026-08-03T23:07:54.288379Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03253","last_updated":"2024-08-19T16:43:51Z","snapshot_observed_at":"2026-07-06T17:40:05.941911Z","submitted_at":"2024-03-05T19:00:02Z","title":"Turbocharging constraints on dark matter substructure through a synthesis of strong lensing flux ratios and extended lensed arcs","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03253","snapshot_observed_at":"2026-08-03T23:07:54.292565Z","title":"Gilman, S","venue":null,"work_id":null,"year":2024},"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":59,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.292565Z"},"links":{"cited_paper":"/paper/2403.03253","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:17c84fcf32cd88040d86d80e41871add968b20c23968b6de8ad2e466d9ffb1a2","observation_id":"828700d4-8644-4617-a54b-f1354d699e4c","resolution":{"observed_at":"2026-08-03T23:07:54.292565Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T23:07:54.296728Z","title":"Paugnat, T","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":60,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.296728Z"},"links":{"citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:32e72a1e2824156a2b4d703125e1b27d209ca2d91603bc55a73ddc1920fd35d5","observation_id":"7003773b-7d63-4987-8217-915e3c6a71a7","resolution":{"observed_at":"2026-08-03T23:07:54.296728Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T23:07:54.300696Z","title":null,"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":61,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.300696Z"},"links":{"citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:1296100dea80a1fb006e0ea76c43c98fcd32a6ee1b21333764057a763f51f6ea","observation_id":"da1e321e-6684-4bfc-baea-45cd5ca72fa8","resolution":{"observed_at":"2026-08-03T23:07:54.300696Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.03530","last_updated":"2025-05-14T18:00:04Z","snapshot_observed_at":"2026-07-06T20:31:50.759186Z","submitted_at":"2025-02-05T19:00:02Z","title":"Elliptical multipoles for gravitational lenses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.03530","snapshot_observed_at":"2026-08-03T23:07:54.304668Z","title":"Paugnat and D","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":62,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.304668Z"},"links":{"cited_paper":"/paper/2502.03530","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:ad18a47e75dc904510dde66efcaa86d4dee3ee2c0cc66fe50279d2b41c4bec5b","observation_id":"24ec85a0-531f-4f5b-8fc7-9d32d89a70b8","resolution":{"observed_at":"2026-08-03T23:07:54.304668Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.09746","last_updated":"2018-11-13T03:04:09Z","snapshot_observed_at":"2026-07-06T06:30:16.704374Z","submitted_at":"2018-03-26T18:00:00Z","title":"Lenstronomy: multi-purpose gravitational lens modelling software package","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.09746","snapshot_observed_at":"2026-08-03T23:07:54.308787Z","title":"Birrer and A","venue":null,"work_id":null,"year":2018},"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":63,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.308787Z"},"links":{"cited_paper":"/paper/1803.09746","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:cea00c3e0d726053467513340b4c4bbdc8bc9f0d12ca19e22a01f30fcbab4722","observation_id":"c59e48f0-1a95-4c56-be08-7b348f8590c6","resolution":{"observed_at":"2026-08-03T23:07:54.308787Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.07377","last_updated":"2018-03-28T11:13:43Z","snapshot_observed_at":"2026-07-06T05:56:32.711115Z","submitted_at":"2017-08-24T12:41:46Z","title":"AutoLens: Automated Modeling of a Strong Lens's Light, Mass and Source","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.07377","snapshot_observed_at":"2026-08-03T23:07:54.316711Z","title":null,"venue":null,"work_id":null,"year":2018},"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":65,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.316711Z"},"links":{"cited_paper":"/paper/1708.07377","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:654f2ba627cf1faca656dcd993c0728c74a8feef225e9913d97f0547ade564df","observation_id":"2ec0074e-f95f-4e3f-b431-776098fea92b","resolution":{"observed_at":"2026-08-03T23:07:54.316711Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.08484","last_updated":"2024-12-09T13:23:18Z","snapshot_observed_at":"2026-07-06T18:29:49.284504Z","submitted_at":"2024-06-12T17:59:34Z","title":"Exploiting the diversity of modeling methods to probe systematic biases in strong lensing analyses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.08484","snapshot_observed_at":"2026-08-03T23:07:54.320477Z","title":"Galan, G","venue":null,"work_id":null,"year":2024},"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":66,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.320477Z"},"links":{"cited_paper":"/paper/2406.08484","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:aa66f959504403efde97c5f4597622ba0ba151dc7696e8140e25e32ee1d083dc","observation_id":"9fcae90f-d754-4bd0-9abc-30c29b19ac97","resolution":{"observed_at":"2026-08-03T23:07:54.320477Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T23:07:54.329020Z","title":"Blandford and R","venue":null,"work_id":null,"year":1986},"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":68,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.329020Z"},"links":{"citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:99b728f6cfd014b02de5d426e4b5e960fbc5b411cffe82682a70f3d35542b85f","observation_id":"329bd181-0a18-447a-bbed-d33a4f2d63bb","resolution":{"observed_at":"2026-08-03T23:07:54.329020Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T23:07:54.332854Z","title":"Schneider, J","venue":null,"work_id":null,"year":1992},"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":69,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.332854Z"},"links":{"citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:665a284082879666273d9f88c922c992449e8e3c76789b9a33b11d034195a86c","observation_id":"cb31fb9c-eac2-4b69-b0b6-7313d10fc156","resolution":{"observed_at":"2026-08-03T23:07:54.332854Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.04696","last_updated":"2022-06-09T18:00:00Z","snapshot_observed_at":"2026-07-06T13:19:12.109592Z","submitted_at":"2022-06-09T18:00:00Z","title":"STRIDES: Automated uniform models for 30 quadruply imaged quasars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.04696","snapshot_observed_at":"2026-08-03T23:07:54.336887Z","title":"Schmidt, T","venue":null,"work_id":null,"year":2023},"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":70,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.336887Z"},"links":{"cited_paper":"/paper/2206.04696","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:94e00d3917295169bfb37f4acd80b26712ae6344501e1a535f8e6cc7c4567eee","observation_id":"5094200c-f9ea-46b2-8f8b-c93763587f98","resolution":{"observed_at":"2026-08-03T23:07:54.336887Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T23:07:54.340810Z","title":null,"venue":null,"work_id":null,"year":2022},"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":71,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.340810Z"},"links":{"citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:0c1a54e7eabb94ed761712228b888ba1813ed29a3fb26c5c1a177309f5006581","observation_id":"f2d986ba-1f69-4ff3-b392-cfb052f966bd","resolution":{"observed_at":"2026-08-03T23:07:54.340810Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T23:07:54.344520Z","title":null,"venue":null,"work_id":null,"year":2024},"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":72,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.344520Z"},"links":{"citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:798dab74b92df1292f48873cc2907e15d845bfe3a8184d1fa76d8e0f3c469baa","observation_id":"96740deb-4d06-4a60-b623-8b2b5b9f9f20","resolution":{"observed_at":"2026-08-03T23:07:54.344520Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.05566","last_updated":"2018-07-15T15:39:56Z","snapshot_observed_at":"2026-08-04T23:47:24.244323Z","submitted_at":"2018-07-15T15:39:56Z","title":"SHARP - V. Modelling gravitationally-lensed radio arcs imaged with global VLBI observations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.05566","snapshot_observed_at":"2026-08-03T23:07:54.348164Z","title":"Spingola, J","venue":null,"work_id":null,"year":2018},"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":73,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.348164Z"},"links":{"cited_paper":"/paper/1807.05566","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:0f03a7c08bb7651feba72bd0067a2b075ae1f725790d8b139b1f6da485f8659b","observation_id":"a6c96285-edea-496a-ac94-2d587695b74b","resolution":{"observed_at":"2026-08-03T23:07:54.348164Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.10566","last_updated":"2023-09-26T12:49:30Z","snapshot_observed_at":"2026-07-06T13:54:53.084096Z","submitted_at":"2022-09-21T18:00:05Z","title":"Scanning For Dark Matter Subhalos in Hubble Space Telescope Imaging of 54 Strong Lenses","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.10566","snapshot_observed_at":"2026-08-03T23:07:54.351905Z","title":null,"venue":null,"work_id":null,"year":2024},"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":74,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.351905Z"},"links":{"cited_paper":"/paper/2209.10566","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:f9e769b47d03a529b9434b7c49d02ef70d01d4d0b4fc69da4186730389423242","observation_id":"5b677ed5-2afa-4298-9eef-87b05a0cf10b","resolution":{"observed_at":"2026-08-03T23:07:54.351905Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.04535","last_updated":"2024-02-28T10:47:45Z","snapshot_observed_at":"2026-07-06T16:16:18.565073Z","submitted_at":"2023-09-08T18:00:08Z","title":"Gravitational imaging through a triple source plane lens: revisiting the $\\Lambda$CDM-defying dark subhalo in SDSSJ0946+1006","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.04535","snapshot_observed_at":"2026-08-03T23:07:54.356113Z","title":null,"venue":null,"work_id":null,"year":2024},"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":75,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.356113Z"},"links":{"cited_paper":"/paper/2309.04535","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:f0ffee88e9dec404257054a67b63eadbabd7d8bfa49e654406c9f26aeb288a84","observation_id":"f3014d9c-3edb-49f6-9731-55ec7fb6676b","resolution":{"observed_at":"2026-08-03T23:07:54.356113Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T23:07:54.360019Z","title":null,"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":76,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.360019Z"},"links":{"citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:16884db9f1a0b4d86d5d4fa8125f4ccda3a43dfa70746374ebf4e18e1ec4beb9","observation_id":"db81eca1-cc92-412c-b379-a9ebed1d6383","resolution":{"observed_at":"2026-08-03T23:07:54.360019Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1007.2880","last_updated":"2010-07-16T21:54:39Z","snapshot_observed_at":"2026-07-06T02:13:00.058560Z","submitted_at":"2010-07-16T21:54:39Z","title":"The Sloan Lens ACS Survey. X. Stellar, Dynamical, and Total Mass Correlations of Massive Early-type Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1007.2880","snapshot_observed_at":"2026-08-03T23:07:54.363627Z","title":null,"venue":null,"work_id":null,"year":2010},"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":77,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.363627Z"},"links":{"cited_paper":"/paper/1007.2880","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:df3453785b1f851f5de6e27ea1fbc819b993fd102391ba07510a8ba5e2481b81","observation_id":"2a35a75f-6ff5-4ffa-ba56-32ef691455d0","resolution":{"observed_at":"2026-08-03T23:07:54.363627Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T23:07:54.367502Z","title":"Stiavelli and T","venue":null,"work_id":null,"year":2017},"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":78,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.367502Z"},"links":{"citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:582eb4a8797a09d6674c43add747f7e341474a528161c577be7ebdafe5150f81","observation_id":"db1abc62-371d-4373-9172-1f41bc1f0b25","resolution":{"observed_at":"2026-08-03T23:07:54.367502Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T23:07:54.371101Z","title":null,"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":79,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.371101Z"},"links":{"citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:e9337b54e70290261aeb51679ce6c2b680d09869f2a33535b514d0f07fc9e14a","observation_id":"f13bd256-d787-4d3b-9873-80d12bbe8195","resolution":{"observed_at":"2026-08-03T23:07:54.371101Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.09278","last_updated":"2020-09-03T23:16:30Z","snapshot_observed_at":"2026-07-06T06:52:03.002610Z","submitted_at":"2018-07-24T18:00:02Z","title":"Is every strong lens model unhappy in its own way? Uniform modelling of a sample of 13 quadruply+ imaged quasars","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.09278","snapshot_observed_at":"2026-08-03T23:07:54.374848Z","title":null,"venue":null,"work_id":null,"year":2019},"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":80,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.374848Z"},"links":{"cited_paper":"/paper/1807.09278","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:93565ef4ef2df920933bd118a8e28ece952eb2e258cbf40ee0a210f1b9540b81","observation_id":"f186def6-2539-4dd4-ae3c-267d889cdf23","resolution":{"observed_at":"2026-08-03T23:07:54.374848Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9907024","last_updated":"1999-07-02T09:23:48Z","snapshot_observed_at":"2026-07-07T01:27:04.258766Z","submitted_at":"1999-07-02T09:23:48Z","title":"Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9907024","snapshot_observed_at":"2026-08-03T23:07:54.378962Z","title":null,"venue":null,"work_id":null,"year":2001},"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":81,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.378962Z"},"links":{"cited_paper":"/paper/astro-ph/9907024","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:a7bff7bd2a658799cfcfaa0d969b0159e95de454a22e4ebb9b2bddba29e1363b","observation_id":"d5a59250-b207-4bfe-8198-7dbdf1a8297c","resolution":{"observed_at":"2026-08-03T23:07:54.378962Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.04512","last_updated":"2018-12-18T23:10:45Z","snapshot_observed_at":"2026-07-31T21:31:14.333353Z","submitted_at":"2017-12-12T20:57:28Z","title":"COLOSSUS: A python toolkit for cosmology, large-scale structure, and dark matter halos","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.04512","snapshot_observed_at":"2026-08-03T23:07:54.382907Z","title":"Diemer, ApJS239, 35 (2018), arXiv:1712.04512 [astro-ph.CO]","venue":null,"work_id":null,"year":2018},"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":82,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.382907Z"},"links":{"cited_paper":"/paper/1712.04512","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:26da0084f34db1e331a4012e51a1c3092f96f91d88c9addd0864b7f9bcdf93b9","observation_id":"79772c7a-c7b4-475b-ae36-37d7df510b79","resolution":{"observed_at":"2026-08-03T23:07:54.382907Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.03958","last_updated":"2021-02-14T18:17:54Z","snapshot_observed_at":"2026-08-04T14:20:36.764751Z","submitted_at":"2020-12-07T19:00:02Z","title":"Out of sight, out of mind? The impact of correlated clustering in substructure lensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.03958","snapshot_observed_at":"2026-08-03T23:07:54.387277Z","title":"Lazar, J","venue":null,"work_id":null,"year":2021},"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":83,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.387277Z"},"links":{"cited_paper":"/paper/2012.03958","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:f5615b1690e94e99d69c55fe9873c7462d852cde337006f0497a4e1e5ef132a1","observation_id":"00d2a9ed-c428-43e9-97f2-dbf83a28233a","resolution":{"observed_at":"2026-08-03T23:07:54.387277Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0806.1056","last_updated":"2008-10-06T23:46:38Z","snapshot_observed_at":"2026-07-06T01:40:47.458421Z","submitted_at":"2008-06-05T20:45:03Z","title":"The Sloan Lens ACS Survey. VIII. The relation between environment and internal structure of early-type galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0806.1056","snapshot_observed_at":"2026-08-03T23:07:54.391175Z","title":null,"venue":null,"work_id":null,"year":2009},"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":84,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.391175Z"},"links":{"cited_paper":"/paper/0806.1056","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:0f07e3ae7c686f3fad517df377453df26d9af5aacecdfb8684b45cb3ac8d126e","observation_id":"16d816a7-f6cb-40d1-929a-bc0c7071c4a3","resolution":{"observed_at":"2026-08-03T23:07:54.391175Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.04201","last_updated":"2025-06-04T17:46:02Z","snapshot_observed_at":"2026-07-06T21:36:40.449308Z","submitted_at":"2025-06-04T17:46:02Z","title":"Analyzing Line-of-sight selection biases in galaxy-scale strong lensing with external convergence and shear","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.04201","snapshot_observed_at":"2026-08-03T23:07:54.395247Z","title":null,"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":85,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.395247Z"},"links":{"cited_paper":"/paper/2506.04201","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:53045366af0dc9d3813dc2661a8537df4435c230c5de7cde1cbb41c7588116e1","observation_id":"c0441d70-c338-4fd1-a5a1-5cbc03897b50","resolution":{"observed_at":"2026-08-03T23:07:54.395247Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0705.0682","last_updated":"2008-12-11T07:11:34Z","snapshot_observed_at":"2026-08-05T04:14:49.926891Z","submitted_at":"2007-05-04T17:26:43Z","title":"Analytic models of plausible gravitational lens potentials","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0705.0682","snapshot_observed_at":"2026-08-03T23:07:54.399208Z","title":null,"venue":null,"work_id":null,"year":2009},"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":86,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.399208Z"},"links":{"cited_paper":"/paper/0705.0682","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:998ff4f61daa7b8dc9fe29fc3ed810d85e868bac43dfbda748b615f085cf347f","observation_id":"a65584cb-1943-4602-8261-83d4bc3b4f2d","resolution":{"observed_at":"2026-08-03T23:07:54.399208Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.07326","last_updated":"2019-01-30T17:16:10Z","snapshot_observed_at":"2026-08-06T12:55:27.927341Z","submitted_at":"2018-09-19T18:00:00Z","title":"An accurate physical model for halo concentrations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.07326","snapshot_observed_at":"2026-08-03T23:07:54.403105Z","title":"Diemer and M","venue":null,"work_id":null,"year":2019},"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":87,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.403105Z"},"links":{"cited_paper":"/paper/1809.07326","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:02218564e8267ca99dcf4df4810e9b0a54f2676e83bdd757a421901d4cb4738a","observation_id":"6067b8c8-47be-424f-96ac-c50b022fa2d4","resolution":{"observed_at":"2026-08-03T23:07:54.403105Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.13732","last_updated":"2020-09-28T00:21:46Z","snapshot_observed_at":"2026-07-06T09:15:59.937947Z","submitted_at":"2020-04-28T18:00:02Z","title":"Concentrations of Dark Haloes Emerge from Their Merger Histories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.13732","snapshot_observed_at":"2026-08-03T23:07:54.406889Z","title":"Wang, Y.-Y","venue":null,"work_id":null,"year":2020},"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":88,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.406889Z"},"links":{"cited_paper":"/paper/2004.13732","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:689d6d0d86e67893aa91fef3bf667db8bbe8a1cdd2c5ee404a20be84a442367e","observation_id":"dd2f3591-f8b9-4a6b-bbde-b5c10c78bc41","resolution":{"observed_at":"2026-08-03T23:07:54.406889Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1410.3282","last_updated":"2015-01-07T18:26:06Z","snapshot_observed_at":"2026-07-06T03:57:11.252524Z","submitted_at":"2014-10-13T12:34:10Z","title":"How well can cold-dark-matter substructures account for the observed radio flux-ratio anomalies?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1410.3282","snapshot_observed_at":"2026-08-03T23:07:54.410657Z","title":null,"venue":null,"work_id":null,"year":2015},"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":89,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.410657Z"},"links":{"cited_paper":"/paper/1410.3282","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:33f8b337f092b13b3e17b9bd9e9059ba8f2fe8595be30557f3cb1363cdfcb50d","observation_id":"634bb95e-8d8a-4c3d-977e-35d212624bdf","resolution":{"observed_at":"2026-08-03T23:07:54.410657Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.17362","last_updated":"2025-03-12T22:59:47Z","snapshot_observed_at":"2026-07-06T20:27:41.902918Z","submitted_at":"2025-01-29T00:58:43Z","title":"Dark Matter Substructure: A Lensing Perspective","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.17362","snapshot_observed_at":"2026-08-03T23:07:54.414663Z","title":"Gannon, A","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":90,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.414663Z"},"links":{"cited_paper":"/paper/2501.17362","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:5e75ea150fa5432caaecb979e76d37e2abc16b56c3fc5d4180e6110aeeaa7420","observation_id":"c9993aa6-76df-4f64-8514-373ab753ce06","resolution":{"observed_at":"2026-08-03T23:07:54.414663Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.07728","last_updated":"2025-07-27T09:03:18Z","snapshot_observed_at":"2026-08-01T20:51:32.179050Z","submitted_at":"2025-03-10T18:00:04Z","title":"Faster than SAM: An empirical model for the tidal evolution of dark matter substructure around strong gravitational lenses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.07728","snapshot_observed_at":"2026-08-03T23:07:54.418845Z","title":null,"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":91,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.418845Z"},"links":{"cited_paper":"/paper/2503.07728","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:109527fc6ca027f1a106b2387017a415aa8d7a9c3631bc8032a3eb17e50b4166","observation_id":"caf19980-43f4-49f2-8470-17119be16c38","resolution":{"observed_at":"2026-08-03T23:07:54.418845Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1008.1786","last_updated":"2010-08-10T20:00:04Z","snapshot_observed_at":"2026-07-06T02:14:02.714262Z","submitted_at":"2010-08-10T20:00:04Z","title":"Galacticus: A Semi-Analytic Model of Galaxy Formation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1008.1786","snapshot_observed_at":"2026-08-03T23:07:54.422772Z","title":null,"venue":null,"work_id":null,"year":2012},"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":92,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.422772Z"},"links":{"cited_paper":"/paper/1008.1786","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:081f0d4bee6daab80ea73ccdab5e6190994c8f706dd424faab6e306bb3fa23bb","observation_id":"7ca2c901-3427-43a7-9505-e963ddcdc46f","resolution":{"observed_at":"2026-08-03T23:07:54.422772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.07077","last_updated":"2021-06-02T16:58:08Z","snapshot_observed_at":"2026-07-06T10:14:26.318640Z","submitted_at":"2020-11-13T19:00:02Z","title":"The asymptotic tidal remnants of cold dark matter subhalos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.07077","snapshot_observed_at":"2026-08-03T23:07:54.426614Z","title":"Errani and J","venue":null,"work_id":null,"year":2021},"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":93,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.426614Z"},"links":{"cited_paper":"/paper/2011.07077","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:70f1a7109874398e2ba56da37c04e52f67bec0861fa3782533fdc62391137647","observation_id":"7d2fc3df-a856-49f1-bd1a-de3f0b137ce3","resolution":{"observed_at":"2026-08-03T23:07:54.426614Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.09597","last_updated":"2024-07-16T00:18:26Z","snapshot_observed_at":"2026-07-06T17:44:41.822709Z","submitted_at":"2024-03-14T17:37:03Z","title":"Tidal evolution of cored and cuspy dark matter halos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.09597","snapshot_observed_at":"2026-08-03T23:07:54.430795Z","title":null,"venue":null,"work_id":null,"year":2024},"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":94,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.430795Z"},"links":{"cited_paper":"/paper/2403.09597","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:8b23523476d6f4add688e18f228610bbe55307647b273dfa64187d7f91b2c8b5","observation_id":"e2d90591-de43-45fe-9ed4-769c50e77a53","resolution":{"observed_at":"2026-08-03T23:07:54.430795Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0010389","last_updated":"2001-05-29T13:43:10Z","snapshot_observed_at":"2026-07-07T00:13:35.834290Z","submitted_at":"2000-10-19T20:05:39Z","title":"Halo Formation in Warm Dark Matter Models","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0010389","snapshot_observed_at":"2026-08-03T23:07:54.434623Z","title":null,"venue":null,"work_id":null,"year":2001},"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":95,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.434623Z"},"links":{"cited_paper":"/paper/astro-ph/0010389","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:6181f839a5aedbdbcfb3c9b0cf0a3e9a9c7e5207dccf9c04b53f10db3b08a0b9","observation_id":"10e90a18-ba8f-4728-a223-93c4cf18290b","resolution":{"observed_at":"2026-08-03T23:07:54.434623Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0906.2968","last_updated":"2009-09-11T21:43:15Z","snapshot_observed_at":"2026-07-06T01:54:43.564615Z","submitted_at":"2009-06-16T16:43:40Z","title":"Sterile neutrinos: the dark side of the light fermions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0906.2968","snapshot_observed_at":"2026-08-03T23:07:54.438545Z","title":"Kusenko, Phys","venue":null,"work_id":null,"year":2009},"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":96,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.438545Z"},"links":{"cited_paper":"/paper/0906.2968","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:69609d2a56538494ffcd148fe26dafc1925962d078c5b8973a7173a73d43a132","observation_id":"19dff626-40ae-4ac2-bfed-3cff7490db9f","resolution":{"observed_at":"2026-08-03T23:07:54.438545Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.11696","last_updated":"2019-10-23T00:51:13Z","snapshot_observed_at":"2026-07-06T08:10:31.480621Z","submitted_at":"2019-07-26T17:54:13Z","title":"Hidden Treasures: sterile neutrinos as dark matter with miraculous abundance, structure formation for different production mechanisms, and a solution to the sigma-8 problem","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.11696","snapshot_observed_at":"2026-08-03T23:07:54.442323Z","title":null,"venue":null,"work_id":null,"year":2019},"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":97,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.442323Z"},"links":{"cited_paper":"/paper/1907.11696","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:d381d6f2fd8ce57ca8a42b91c20bce708e7f19eba71872aa3b1b8b614d12fbb1","observation_id":"67385d37-09bd-4c04-a0d0-b7ab1d508855","resolution":{"observed_at":"2026-08-03T23:07:54.442323Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.09777","last_updated":"2023-07-18T19:56:09Z","snapshot_observed_at":"2026-07-06T13:11:46.425668Z","submitted_at":"2022-05-19T18:00:34Z","title":"Constraints on sterile neutrino models from strong gravitational lensing, Milky Way satellites, and Lyman-$\\alpha$ forest","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.09777","snapshot_observed_at":"2026-08-03T23:07:54.446323Z","title":null,"venue":null,"work_id":null,"year":2022},"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":98,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.446323Z"},"links":{"cited_paper":"/paper/2205.09777","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:a9934f011f60330a38bfd88b223cb55dca17b5b42fec7f451f99e326f5a518d3","observation_id":"bb934f68-71cd-41fe-af54-d0eb2ac20745","resolution":{"observed_at":"2026-08-03T23:07:54.446323Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.09760","last_updated":"2021-10-19T13:39:53Z","snapshot_observed_at":"2026-08-06T22:00:54.348170Z","submitted_at":"2021-09-20T18:00:05Z","title":"Simulating the complexity of the dark matter sheet II: halo and subhalo mass functions for non-cold dark matter models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.09760","snapshot_observed_at":"2026-08-03T23:07:54.450444Z","title":"St¨ ucker, R","venue":null,"work_id":null,"year":2022},"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":99,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.450444Z"},"links":{"cited_paper":"/paper/2109.09760","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:bddcbaf7961471649f61be210f4ca1186d128ad3cac48ddca5d7c350d1b2dc0f","observation_id":"959efc6d-9146-4a91-aad2-8b022a81c3ea","resolution":{"observed_at":"2026-08-03T23:07:54.450444Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.03635","last_updated":"2025-06-14T15:46:30Z","snapshot_observed_at":"2026-07-06T19:27:52.298292Z","submitted_at":"2024-10-04T17:42:20Z","title":"COZMIC. I. Cosmological Zoom-in Simulations with Initial Conditions Beyond Cold Dark Matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.03635","snapshot_observed_at":"2026-08-03T23:07:54.454443Z","title":null,"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":100,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.454443Z"},"links":{"cited_paper":"/paper/2410.03635","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:c9744b4fb743a5f53959c562feb04f679853ad0e973b65ac814ae38de98411d2","observation_id":"873b3087-fd41-4c92-abfc-48ebc13969f2","resolution":{"observed_at":"2026-08-03T23:07:54.454443Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.01125","last_updated":"2020-06-01T11:18:49Z","snapshot_observed_at":"2026-07-06T09:01:38.630614Z","submitted_at":"2020-03-02T19:00:01Z","title":"Towards a general parametrization of the warm dark matter halo mass function","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.01125","snapshot_observed_at":"2026-08-03T23:07:54.458270Z","title":null,"venue":null,"work_id":null,"year":2020},"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":101,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.458270Z"},"links":{"cited_paper":"/paper/2003.01125","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:25a0e95c92659dfe82217d6b0275f9764a4a69e292128325244c45de4d146b0e","observation_id":"5e4db9b8-202c-420e-996e-dca67b40b972","resolution":{"observed_at":"2026-08-03T23:07:54.458270Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2511.07513","last_updated":"2026-07-01T19:58:59Z","latest_version":5,"primary_category":"astro-ph.CO","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"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":99,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":171},"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":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 100 of 171 outbound references and 12 inbound Pith citation observations for arXiv:2511.07513."}