{"as_of":"2026-08-16T19:15:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d26dd8d99ad1a1cb955d41e64e80aebf715d795f8aa9ca5ba1b689eb043b843d","coverage":[{"denominator":106,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T15:51:27.610183Z","state":"measured"},{"denominator":106,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":106,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T15:35:45.958607Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-20T22:43:50.745111Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.22178","snapshot_observed_at":"2026-08-03T17:37:13.179034Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2512.08853","last_updated":"2026-05-27T06:59:46Z","snapshot_observed_at":"2026-08-03T17:36:59.059691Z","submitted_at":"2025-12-09T17:47:06Z","title":"New light mediators and the neutrino fog: Implications from XENONnT nuclear recoil data","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-03T17:37:13.179034Z"},"links":{"cited_paper":"/paper/2509.22178","citing_paper":"/paper/2512.08853"},"observation_digest":"sha256:5f9fcb6ed0ae843f69ebf4f75077cb191bba660e136660a4a90ef97239d920af","observation_id":"c6029b69-e5f6-4e10-8538-8d35a38e3142","resolution":{"observed_at":"2026-08-03T17:37:13.179034Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.22178","snapshot_observed_at":"2026-08-02T19:56:53.124332Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2603.00554","last_updated":"2026-07-27T09:11:11Z","snapshot_observed_at":"2026-08-12T17:31:00.929635Z","submitted_at":"2026-02-28T09:05:50Z","title":"Testing light and heavy vector mediators with solar CE$\\nu$NS measurements","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-02T19:56:53.124332Z"},"links":{"cited_paper":"/paper/2509.22178","citing_paper":"/paper/2603.00554"},"observation_digest":"sha256:de32a40fb18d40b70348baba7edf12ca1852c7a7561d91ed45ea8308e91719fa","observation_id":"9d1286e0-4fc9-4f5f-b286-40d628eb2fcb","resolution":{"observed_at":"2026-08-02T19:56:53.124332Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"cited_work":{"arxiv_id":"2509.22178","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2509.22178","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"When backgrounds be- come signals: neutrino interactions in xenon-based dark matter detectors","venue":null,"work_id":"bf49d2ab-d2ec-4e70-9c50-68eaee03b5b4","year":2025},"citing_paper":{"arxiv_id":"2605.07975","last_updated":"2026-05-16T17:58:48Z","snapshot_observed_at":"2026-08-15T05:15:43.879696Z","submitted_at":"2026-05-08T16:33:47Z","title":"Phenomenological implications of the high-precision COHERENT germanium CE$\\nu$NS data","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-05-11T02:59:38.568367Z"},"links":{"cited_paper":"/paper/2509.22178","citing_paper":"/paper/2605.07975"},"observation_digest":"sha256:aa2aa48e848b622c38cc287090cbc2623d5add8814510e9d7bb6aec255dc95f7","observation_id":"c46107c3-5dae-4a14-83ea-f0707d6ca1cb","resolution":{"observed_at":"2026-06-04T02:07:04.771428Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"cited_work":{"arxiv_id":"2509.22178","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2509.22178","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"When backgrounds be- come signals: neutrino interactions in xenon-based dark matter detectors","venue":null,"work_id":"bf49d2ab-d2ec-4e70-9c50-68eaee03b5b4","year":2025},"citing_paper":{"arxiv_id":"2605.07975","last_updated":"2026-05-16T17:58:48Z","snapshot_observed_at":"2026-08-15T05:15:43.879696Z","submitted_at":"2026-05-08T16:33:47Z","title":"Phenomenological implications of the high-precision COHERENT germanium CE$\\nu$NS data","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-05-20T22:41:59.482854Z"},"links":{"cited_paper":"/paper/2509.22178","citing_paper":"/paper/2605.07975"},"observation_digest":"sha256:aabc8f8d1ffd414ad68d739c705d297b27cd7bd808462a9a1e98da4ccb0ab326","observation_id":"fc28b2cb-d369-4d70-b4d9-46e9a9907a20","resolution":{"observed_at":"2026-06-04T02:07:04.771428Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.22178","snapshot_observed_at":"2026-08-01T04:27:08.080066Z","title":"Atzori Corona, M","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.22817","last_updated":"2026-07-24T18:00:05Z","snapshot_observed_at":"2026-08-06T08:21:48.034725Z","submitted_at":"2026-07-24T18:00:05Z","title":"$\\texttt{SNuDD}$: Solar Neutrinos for Direct Detection","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-01T04:27:08.080066Z"},"links":{"cited_paper":"/paper/2509.22178","citing_paper":"/paper/2607.22817"},"observation_digest":"sha256:7f8f998b2765e6f724ddbf8a04445ed5f61a8beb62dc1056c71ec9c468d904c9","observation_id":"cf5e366d-ae74-4141-90a3-2025970e944b","resolution":{"observed_at":"2026-08-01T04:27:08.080066Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.22178","snapshot_observed_at":"2026-08-15T15:35:45.958607Z","title":"Atzori Corona, M","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.24584","last_updated":"2026-07-27T15:51:27Z","snapshot_observed_at":"2026-08-16T10:37:21.787795Z","submitted_at":"2026-07-27T15:51:27Z","title":"Invisible decay of solar neutrinos at dark matter experiments","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-15T15:35:45.958607Z"},"links":{"cited_paper":"/paper/2509.22178","citing_paper":"/paper/2607.24584"},"observation_digest":"sha256:4dc75a8db463bebe48be03c77e0d31aac2838d281eafd8faeba960ae1f169194","observation_id":"18653a2f-ce44-4a2a-b61c-744c3da1cd5d","resolution":{"observed_at":"2026-08-15T15:35:45.958607Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2509.22178/citation-record","integrity":"/paper/2509.22178/integrity","json":"/paper/2509.22178/citation-record.json","paper":"/paper/2509.22178"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2402.10446","last_updated":"2025-08-13T08:19:01Z","snapshot_observed_at":"2026-08-16T14:18:06.992394Z","submitted_at":"2024-02-16T04:38:30Z","title":"The XENONnT Dark Matter Experiment","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.10446","snapshot_observed_at":"2026-08-15T15:51:27.098803Z","title":"Aprile et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.098803Z"},"links":{"cited_paper":"/paper/2402.10446","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:cfdaa5c97b306180720b797c6e8b9080e4a1710e3e92ac3b092987656b4e4489","observation_id":"aefff8b2-d987-4903-aef8-c92640a2757c","resolution":{"observed_at":"2026-08-15T15:51:27.098803Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.02229","last_updated":"2018-06-07T12:08:33Z","snapshot_observed_at":"2026-08-16T00:42:11.309884Z","submitted_at":"2018-06-06T14:47:44Z","title":"Dark matter direct search sensitivity of the PandaX-4T experiment","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.02229","snapshot_observed_at":"2026-08-15T15:51:27.105118Z","title":"Zhang et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.105118Z"},"links":{"cited_paper":"/paper/1806.02229","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:81e67d5c1ff1ba9d284f116a28475b47af0ae28fe9570204721f1e484221c8b4","observation_id":"47bbd4c1-b65f-4c73-94a1-cac73f2dc9c6","resolution":{"observed_at":"2026-08-15T15:51:27.105118Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.09124","last_updated":"2019-11-04T00:25:15Z","snapshot_observed_at":"2026-08-11T01:25:04.852534Z","submitted_at":"2019-10-21T02:43:22Z","title":"The LUX-ZEPLIN (LZ) Experiment","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.09124","snapshot_observed_at":"2026-08-15T15:51:27.109941Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.109941Z"},"links":{"cited_paper":"/paper/1910.09124","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:1845eaabed381b0c2dffe7f2384517e0fde6bb4100cbab7b34a87260fdc86dbc","observation_id":"4842eb38-c148-49e0-b15a-d33a4c664d3b","resolution":{"observed_at":"2026-08-15T15:51:27.109941Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.05813","last_updated":"2025-01-06T12:18:37Z","snapshot_observed_at":"2026-08-16T13:36:13.300361Z","submitted_at":"2024-07-08T10:50:25Z","title":"DarkSide-20k sensitivity to light dark matter particles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.05813","snapshot_observed_at":"2026-08-15T15:51:27.114713Z","title":"Acerbi et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.114713Z"},"links":{"cited_paper":"/paper/2407.05813","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:33c5fc0c7edb4f7f9ab0e8df5979527ec8b65fc2a242b1f317ddfc39354e6ce8","observation_id":"b51f6e40-bd47-4db1-9d60-b98ea451da0a","resolution":{"observed_at":"2026-08-15T15:51:27.114713Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.08145","last_updated":"2017-07-25T18:31:41Z","snapshot_observed_at":"2026-08-15T13:52:27.411900Z","submitted_at":"2017-07-25T18:31:41Z","title":"DarkSide-20k: A 20 Tonne Two-Phase LAr TPC for Direct Dark Matter Detection at LNGS","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.08145","snapshot_observed_at":"2026-08-15T15:51:27.119175Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.119175Z"},"links":{"cited_paper":"/paper/1707.08145","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:4b692b83aff62975a7925f1178acd5b4ada41203afd20ea70d789dd5fc6a71ee","observation_id":"459ecb35-9b11-449e-bf37-923e44faaede","resolution":{"observed_at":"2026-08-15T15:51:27.119175Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.05320","last_updated":"2024-02-02T14:31:14Z","snapshot_observed_at":"2026-08-16T14:44:40.985461Z","submitted_at":"2023-11-09T12:40:48Z","title":"Dual-phase xenon time projection chambers for rare-event searches","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.05320","snapshot_observed_at":"2026-08-15T15:51:27.124128Z","title":"Baudis, Dual-phase xenon time projection chambers for rare-event searches, Phil","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.124128Z"},"links":{"cited_paper":"/paper/2311.05320","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:7a648f1a43ed76e67b6190fa378fd68f75ae1ab57b8569c3195e9f5381296f86","observation_id":"0bda19ac-1d02-4345-ae88-9995035c64ff","resolution":{"observed_at":"2026-08-15T15:51:27.124128Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.08842","last_updated":"2023-07-26T12:18:53Z","snapshot_observed_at":"2026-08-16T15:15:32.676884Z","submitted_at":"2023-07-17T21:04:11Z","title":"A view of Coherent Elastic Neutrino-Nucleus Scattering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.08842","snapshot_observed_at":"2026-08-15T15:51:27.129733Z","title":"Cadeddu, F","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.129733Z"},"links":{"cited_paper":"/paper/2307.08842","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:e245450b4a9faa304b8b0870cefde37683af81f87555c48283bf473c08b7fd65","observation_id":"fdcdbdf7-7719-4e02-ada3-2bc6aa323b50","resolution":{"observed_at":"2026-08-15T15:51:27.129733Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.16709","last_updated":"2024-05-30T09:53:34Z","snapshot_observed_at":"2026-08-16T14:48:50.092066Z","submitted_at":"2024-02-26T16:27:03Z","title":"Momentum dependent flavor radiative corrections to the coherent elastic neutrino-nucleus scattering for the neutrino charge-radius determination","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.16709","snapshot_observed_at":"2026-08-15T15:51:27.134138Z","title":"Atzori Corona, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.134138Z"},"links":{"cited_paper":"/paper/2402.16709","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:7c24a3cf5335f3b0e13036bdd0a40eeebb97fa765b3b5487d8b415610c09e0ba","observation_id":"546ab33e-8179-4a47-b675-473cd07b5535","resolution":{"observed_at":"2026-08-15T15:51:27.134138Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.09360","last_updated":"2023-08-15T17:23:59Z","snapshot_observed_at":"2026-08-16T15:47:41.016613Z","submitted_at":"2023-03-16T14:44:25Z","title":"Nuclear neutron radius and weak mixing angle measurements from latest COHERENT CsI and atomic parity violation Cs data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.09360","snapshot_observed_at":"2026-08-15T15:51:27.139002Z","title":"Atzori Corona, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.139002Z"},"links":{"cited_paper":"/paper/2303.09360","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:36512406a05a6dd15342ab835ea4f085826b1ae16867b21222ea60dee5afa87f","observation_id":"3e6c1283-0992-4c97-a595-206c8c037090","resolution":{"observed_at":"2026-08-15T15:51:27.139002Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5522","last_updated":"2013-03-22T05:51:18Z","snapshot_observed_at":"2026-08-15T00:24:14.048587Z","submitted_at":"2013-03-22T05:51:18Z","title":"The Weak Neutral Current","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5522","snapshot_observed_at":"2026-08-15T15:51:27.144617Z","title":"Erler and S","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.144617Z"},"links":{"cited_paper":"/paper/1303.5522","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:2d27095ef10411b5dd6e52b4ab7a1d0a567933fe08613a88465938884b4419dc","observation_id":"960ecf05-0885-47be-ba91-5e669a71b57f","resolution":{"observed_at":"2026-08-15T15:51:27.144617Z","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":"2026-08-15T15:51:27.150050Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.150050Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:8073d865d700b671b9fe73cbf5b06832e0174806651a0c4330451050195a4fda","observation_id":"8fe28ff2-51d2-4dac-961a-aeacbca83026","resolution":{"observed_at":"2026-08-15T15:51:27.150050Z","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":"2026-08-15T15:51:27.154566Z","title":"Atzori Corona, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.154566Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:72fe60b87fc3d0ad3fd4323004039474d25b3966332ad410494beaef07cb7b91","observation_id":"ca9ae315-62fa-41c5-9fda-e2cb4b77dbe3","resolution":{"observed_at":"2026-08-15T15:51:27.154566Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.05606","last_updated":"2020-02-26T10:12:47Z","snapshot_observed_at":"2026-08-14T18:15:31.858804Z","submitted_at":"2018-10-12T17:02:43Z","title":"Neutrino Charge Radii from COHERENT Elastic Neutrino-Nucleus Scattering","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.05606","snapshot_observed_at":"2026-08-15T15:51:27.159175Z","title":"Cadeddu, C","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.159175Z"},"links":{"cited_paper":"/paper/1810.05606","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:b0577e48c04f3c492967733abe9bea4dd3da9fa6391ea1528e32eca238f3e337","observation_id":"41356633-75d3-47c6-99d3-8f6c1f026bb7","resolution":{"observed_at":"2026-08-15T15:51:27.159175Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0210055","last_updated":"2002-10-03T13:17:47Z","snapshot_observed_at":"2026-08-12T02:52:16.912668Z","submitted_at":"2002-10-03T13:17:47Z","title":"The neutrino charge radius is a physical observable","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0210055","snapshot_observed_at":"2026-08-15T15:51:27.163676Z","title":"Bernabeu, J","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.163676Z"},"links":{"cited_paper":"/paper/hep-ph/0210055","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:e8141a0b11ee4383ab93e75bb1df9d0528cb5c41eba7fcb1eecfc713e7e10322","observation_id":"f712f02c-1b85-499d-9a90-25e630ed3f8f","resolution":{"observed_at":"2026-08-15T15:51:27.163676Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0206015","last_updated":"2002-10-02T12:59:03Z","snapshot_observed_at":"2026-08-14T13:23:02.904129Z","submitted_at":"2002-06-03T16:20:41Z","title":"On the observability of the neutrino charge radius","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0206015","snapshot_observed_at":"2026-08-15T15:51:27.168156Z","title":"Bernabeu, J","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.168156Z"},"links":{"cited_paper":"/paper/hep-ph/0206015","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:0431f86b46b76d75937bc8a17cd3447614628ea68b04d13d2745850f7232aeb5","observation_id":"52a050d5-899c-4ed1-9054-9bc8e3f4fcd7","resolution":{"observed_at":"2026-08-15T15:51:27.168156Z","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":"2026-08-15T15:51:27.172511Z","title":"Berglund and M","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.172511Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:9e45a60d17997f75b61ca030813833c38a778bfe0194fe81a400f644b0bae076","observation_id":"2a827e56-46de-49c9-9f07-8fcf6e61e495","resolution":{"observed_at":"2026-08-15T15:51:27.172511Z","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":"2026-08-15T15:51:27.176628Z","title":null,"venue":null,"work_id":null,"year":1956},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.176628Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:ca3d47c7592795dad2407ff8eadc042974de63b4e6b264e03f164eb7bb456d02","observation_id":"45203d8a-875f-4c16-8b2c-0050105ec218","resolution":{"observed_at":"2026-08-15T15:51:27.176628Z","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":"2026-08-15T15:51:27.180855Z","title":"Fricke, C","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.180855Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:ecdc868fbd48cd06f63a3c77640e99176e80f09628b70acfacf54617a5a7bdd1","observation_id":"633be438-a896-405e-a66e-0f255e765c3d","resolution":{"observed_at":"2026-08-15T15:51:27.180855Z","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":"2026-08-15T15:51:27.185470Z","title":"Angeli and K","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.185470Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:367d001d6d5d4277431f5958113fb21f3cdbc4a994bebe225b8ff10be2076aa6","observation_id":"14a7790d-d714-4884-804f-51d7bc8fb9fd","resolution":{"observed_at":"2026-08-15T15:51:27.185470Z","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":"2026-08-15T15:51:27.190272Z","title":"Fricke and K","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.190272Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:054c960f21dae6ad04eb794326e128ab3d145cef75a14da55d96b94956422ce4","observation_id":"5aa27bc4-c2cc-407c-b7f4-a02af52979a7","resolution":{"observed_at":"2026-08-15T15:51:27.190272Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.08529","last_updated":"2020-10-23T14:36:17Z","snapshot_observed_at":"2026-08-10T20:59:03.946227Z","submitted_at":"2020-07-16T18:00:01Z","title":"Coherent elastic neutrino-nucleus scattering: EFT analysis and nuclear responses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.08529","snapshot_observed_at":"2026-08-15T15:51:27.194584Z","title":"Hoferichter, J","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.194584Z"},"links":{"cited_paper":"/paper/2007.08529","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:07f6934094ae091fce0448d16fbc50461a554202babf7551745a821819703d4c","observation_id":"625c44d3-9995-4431-bcdb-cf83c8de3b22","resolution":{"observed_at":"2026-08-15T15:51:27.194584Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.01645","last_updated":"2020-07-03T22:07:19Z","snapshot_observed_at":"2026-08-14T18:42:22.622158Z","submitted_at":"2020-05-04T17:01:08Z","title":"Physics results from the first COHERENT observation of CE$\\nu$NS in argon and their combination with cesium-iodide data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.01645","snapshot_observed_at":"2026-08-15T15:51:27.200173Z","title":"Cadeddu, F","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.200173Z"},"links":{"cited_paper":"/paper/2005.01645","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:99c701149b43abb3543ab75b7a8d2850b0cd943423dbfd029f97613337b8eae6","observation_id":"797ad026-ff32-44ba-9f2a-99d6745968aa","resolution":{"observed_at":"2026-08-15T15:51:27.200173Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.10829","last_updated":"2022-07-11T09:43:22Z","snapshot_observed_at":"2026-08-16T17:19:33.292253Z","submitted_at":"2022-02-22T11:42:42Z","title":"Bounds on new physics with data of the Dresden-II reactor experiment and COHERENT","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.10829","snapshot_observed_at":"2026-08-15T15:51:27.207357Z","title":"Coloma, I","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.207357Z"},"links":{"cited_paper":"/paper/2202.10829","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:56fa9319bb802f4fb10f0881a16c934e4e450459f0eeafb261a431dc14bc7161","observation_id":"f5e935f1-fc99-428b-955d-b6b6d93658da","resolution":{"observed_at":"2026-08-15T15:51:27.207357Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.6344","last_updated":"2015-07-02T13:30:37Z","snapshot_observed_at":"2026-08-16T07:06:56.432768Z","submitted_at":"2014-03-25T13:55:29Z","title":"Neutrino electromagnetic interactions: a window to new physics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.6344","snapshot_observed_at":"2026-08-15T15:51:27.212602Z","title":"Giunti and A","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.212602Z"},"links":{"cited_paper":"/paper/1403.6344","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:67c3c89732ab6b15e0059eac7700d1b43fd63bd6828d31a47b0075ece0580004","observation_id":"a037a3cb-5570-4c1e-9095-d5b1c00016e8","resolution":{"observed_at":"2026-08-15T15:51:27.212602Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.09484","last_updated":"2023-03-14T10:52:02Z","snapshot_observed_at":"2026-08-16T16:59:13.421849Z","submitted_at":"2022-05-19T11:45:19Z","title":"Impact of the Dresden-II and COHERENT neutrino scattering data on neutrino electromagnetic properties and electroweak physics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.09484","snapshot_observed_at":"2026-08-15T15:51:27.218465Z","title":"Atzori Corona, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.218465Z"},"links":{"cited_paper":"/paper/2205.09484","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:86e0deea7e332d8ecf91c8b095190b483ee80fe72a38eb51c64bbb507ce74f0c","observation_id":"df1ef8fb-281a-484d-97cd-ddb2b78e4f5d","resolution":{"observed_at":"2026-08-15T15:51:27.218465Z","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":"2026-08-15T15:51:27.223969Z","title":"Chen, H.-C","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.223969Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:c5f0c0d46952e965de6ce822ffcf5494f088ee04005cf76d0075de49c9633004","observation_id":"dbae6839-d85e-464e-909e-6a6364a5fb83","resolution":{"observed_at":"2026-08-15T15:51:27.223969Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.4999","last_updated":"2014-06-19T10:34:58Z","snapshot_observed_at":"2026-08-14T23:29:49.556890Z","submitted_at":"2014-06-19T10:34:58Z","title":"Theory of neutrino-atom collisions: the history, present status and BSM physics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.4999","snapshot_observed_at":"2026-08-15T15:51:27.229061Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.229061Z"},"links":{"cited_paper":"/paper/1406.4999","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:06cbd94f4dac931c648efe1a603988c927b4d5450e1e38bef98466761582946b","observation_id":"8d3e1f18-b957-4fa3-a4ea-d3f4efa77974","resolution":{"observed_at":"2026-08-15T15:51:27.229061Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.05036","last_updated":"2023-03-02T09:16:44Z","snapshot_observed_at":"2026-08-16T16:46:49.822763Z","submitted_at":"2022-07-11T17:46:54Z","title":"New constraint on neutrino magnetic moment and neutrino millicharge from LUX-ZEPLIN dark matter search results","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.05036","snapshot_observed_at":"2026-08-15T15:51:27.236521Z","title":"Atzori Corona, W","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.236521Z"},"links":{"cited_paper":"/paper/2207.05036","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:f7ae74d3cb1c7847cd7b641ca63ec7b1b1c3d27e836deee9db7ca7d311160daa","observation_id":"7e0fe498-d5fb-48eb-bfcb-b35cdea8e5ce","resolution":{"observed_at":"2026-08-15T15:51:27.236521Z","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":"2026-08-15T15:51:27.240808Z","title":null,"venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.240808Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:68f36957bc09fd3d407dd695ecbfff65fa86dc40eeda7f5cbfd6afad727b42dd","observation_id":"4c1f0cc8-295c-48a2-89af-9a734d66de31","resolution":{"observed_at":"2026-08-15T15:51:27.240808Z","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":"2026-08-15T15:51:27.245129Z","title":"Huang, Relativistic many-body theory of atomic transitions","venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.245129Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:b957d14382949b32c15c773734a8283795cbab0fcb50d5d9ecbd4b91bbe459c9","observation_id":"667fac4c-58f7-44cf-82ff-7d6f2f0c5d3e","resolution":{"observed_at":"2026-08-15T15:51:27.245129Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.5294","last_updated":"2013-11-21T02:29:18Z","snapshot_observed_at":"2026-08-14T23:54:30.938219Z","submitted_at":"2013-11-21T02:29:18Z","title":"Atomic ionization of germanium due to neutrino magnetic moments","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.5294","snapshot_observed_at":"2026-08-15T15:51:27.249551Z","title":"Chen, H.-C","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.249551Z"},"links":{"cited_paper":"/paper/1311.5294","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:1546bb5485632c222319332d779ac8cf0611595ccaf231d4369bdb1da671a1e3","observation_id":"15c74a57-2325-44e8-bff5-121a9233390e","resolution":{"observed_at":"2026-08-15T15:51:27.249551Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.0574","last_updated":"2014-11-03T17:25:12Z","snapshot_observed_at":"2026-08-14T23:13:07.982722Z","submitted_at":"2014-11-03T17:25:12Z","title":"Constraining neutrino electromagnetic properties by germanium detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.0574","snapshot_observed_at":"2026-08-15T15:51:27.255752Z","title":"Chen, H.-C","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.255752Z"},"links":{"cited_paper":"/paper/1411.0574","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:c9e746bc3be006a3bbf0cbd9c91e41f9008e084d03f58e7489c41bcf586cbdcd","observation_id":"c65e8ceb-5952-4df1-a2d3-af2ff3a3df14","resolution":{"observed_at":"2026-08-15T15:51:27.255752Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.06085","last_updated":"2019-03-14T15:42:53Z","snapshot_observed_at":"2026-08-14T17:02:14.366831Z","submitted_at":"2019-03-14T15:42:53Z","title":"Discovery potential of multi-ton xenon detectors in neutrino electromagnetic properties","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.06085","snapshot_observed_at":"2026-08-15T15:51:27.260642Z","title":"Hsieh, L","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.260642Z"},"links":{"cited_paper":"/paper/1903.06085","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:47d8ba3210fe33647ea44d4a8d59fd63a6134d2499732f1a6857b7820900e208","observation_id":"932f52a7-440c-4497-986b-9df5a6a7d599","resolution":{"observed_at":"2026-08-15T15:51:27.260642Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.09355","last_updated":"2017-08-10T19:17:41Z","snapshot_observed_at":"2026-08-14T20:44:34.756689Z","submitted_at":"2017-07-28T17:54:23Z","title":"Limiting neutrino magnetic moments with Borexino Phase-II solar neutrino data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.09355","snapshot_observed_at":"2026-08-15T15:51:27.267792Z","title":"Agostini et al","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.267792Z"},"links":{"cited_paper":"/paper/1707.09355","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:ed1234d5d4cee53fcfcf7ec2dd4371a2bd116fd0adc5d9e4a78802f4f1ef0f2e","observation_id":"fbe2783a-2a37-4e90-b9c1-65b12747a7f0","resolution":{"observed_at":"2026-08-15T15:51:27.267792Z","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":"2026-08-15T15:51:27.272737Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.272737Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:bc3e7893180ed6b1b79041befa1d5f32f006080a587c77648851ca48b294c67a","observation_id":"c5e41408-5ae8-4b57-bfcc-d3c8310b1854","resolution":{"observed_at":"2026-08-15T15:51:27.272737Z","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":"2026-08-15T15:51:27.278175Z","title":"Aprile et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.278175Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:07dcb6b00f9223606e1973bb8b0d0fb82a7e05cd45918e9230bfd3f7c09eae25","observation_id":"1fd157bc-a64c-493c-924b-2864a08ece49","resolution":{"observed_at":"2026-08-15T15:51:27.278175Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.10892","last_updated":"2024-09-13T07:52:03Z","snapshot_observed_at":"2026-08-16T13:34:04.540108Z","submitted_at":"2024-07-15T16:40:46Z","title":"First Indication of Solar $^8$B Neutrino Flux through Coherent Elastic Neutrino-Nucleus Scattering in PandaX-4T","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.10892","snapshot_observed_at":"2026-08-15T15:51:27.288604Z","title":"Bo et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.288604Z"},"links":{"cited_paper":"/paper/2407.10892","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:5882de48bc7911e5004109a49ebd8528074b5d32dc5c8db3cbea5cec0a47dbf8","observation_id":"830204ad-b3fe-407a-ba10-9329f4a89a64","resolution":{"observed_at":"2026-08-15T15:51:27.288604Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.07641","last_updated":"2025-02-07T03:08:40Z","snapshot_observed_at":"2026-08-16T13:26:27.087552Z","submitted_at":"2024-08-14T16:11:30Z","title":"Exploring New Physics with PandaX-4T Low Energy Electronic Recoil Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.07641","snapshot_observed_at":"2026-08-15T15:51:27.293503Z","title":"Zeng et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.293503Z"},"links":{"cited_paper":"/paper/2408.07641","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:e1ed3ef2cc5cca3dd569078bbff5342645118dd8ac4ef427dae633d0012d4ebe","observation_id":"d0dde43e-6505-4ea0-9d10-4d497b9f0f14","resolution":{"observed_at":"2026-08-15T15:51:27.293503Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.17036","last_updated":"2025-07-01T14:32:43Z","snapshot_observed_at":"2026-07-06T19:37:52.003100Z","submitted_at":"2024-10-22T14:07:18Z","title":"Dark Matter Search Results from 4.2 Tonne-Years of Exposure of the LUX-ZEPLIN (LZ) Experiment","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.17036","snapshot_observed_at":"2026-08-15T15:51:27.299276Z","title":"Aalbers et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.299276Z"},"links":{"cited_paper":"/paper/2410.17036","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:cd7d886e06d138cc536c6e48794b21987ebb9cc60d9fb852b7a50a156cda6f3d","observation_id":"3ca5360d-2d59-4a14-b7ca-8ba48776eea7","resolution":{"observed_at":"2026-08-15T15:51:27.299276Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.11878","last_updated":"2020-12-10T15:31:16Z","snapshot_observed_at":"2026-08-13T17:56:06.264306Z","submitted_at":"2019-10-25T18:00:02Z","title":"Grand Unified Neutrino Spectrum at Earth: Sources and Spectral Components","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.11878","snapshot_observed_at":"2026-08-15T15:51:27.305280Z","title":"Vitagliano, I","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.305280Z"},"links":{"cited_paper":"/paper/1910.11878","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:74034a66a2c28d42bc7cc31b68a02a03be95249208ad7cc5d0cf8473797cb402","observation_id":"c27303ee-bf49-451a-a2fa-36461a1159ba","resolution":{"observed_at":"2026-08-15T15:51:27.305280Z","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":"2026-08-15T15:51:27.310247Z","title":"Baker and R","venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.310247Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:03b8fa118fe46bf625cda05639cd30b6aca36de17e62fac96113e4a2f54fe83e","observation_id":"5b4c684b-e9f1-43fb-8418-0b0f10740e85","resolution":{"observed_at":"2026-08-15T15:51:27.310247Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.07179","last_updated":"2016-01-26T21:00:04Z","snapshot_observed_at":"2026-08-16T16:16:45.020235Z","submitted_at":"2016-01-26T21:00:04Z","title":"Alive and well: a short review about standard solar models","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.07179","snapshot_observed_at":"2026-08-15T15:51:27.314317Z","title":"Serenelli, Alive and well: a short review about standard solar models, Eur","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.314317Z"},"links":{"cited_paper":"/paper/1601.07179","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:fd3f9a5c5f59def3e753a654ee91abef3fcd844579cf5fc497d7759753723066","observation_id":"5fd47a14-fa27-4395-b47b-0a92d59654e4","resolution":{"observed_at":"2026-08-15T15:51:27.314317Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.00756","last_updated":"2020-03-06T14:00:49Z","snapshot_observed_at":"2026-08-14T20:36:33.926692Z","submitted_at":"2017-09-03T18:53:03Z","title":"Improved measurement of $^8$B solar neutrinos with 1.5 kt y of Borexino exposure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.00756","snapshot_observed_at":"2026-08-15T15:51:27.321586Z","title":"Agostini et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.321586Z"},"links":{"cited_paper":"/paper/1709.00756","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:8367067bf41d6f386826f0e6b67b8938480a1fabe59202d8dc00c663b3720a1d","observation_id":"38edf3af-09d0-47fd-bb2c-d566811fddcd","resolution":{"observed_at":"2026-08-15T15:51:27.321586Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.11749","last_updated":"2024-11-18T17:25:22Z","snapshot_observed_at":"2026-08-13T12:24:56.437944Z","submitted_at":"2024-11-18T17:25:22Z","title":"Bounds on new neutrino interactions from the first CE$\\nu$NS data at direct detection experiments","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.11749","snapshot_observed_at":"2026-08-15T15:51:27.327215Z","title":"De Romeri, D","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.327215Z"},"links":{"cited_paper":"/paper/2411.11749","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:fe88492f72589425d7c3a41d60782b0700e9420d0dc2d6c062bae6e619c68392","observation_id":"19388806-3a1f-44c3-b5c2-948e863848a3","resolution":{"observed_at":"2026-08-15T15:51:27.327215Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.14991","last_updated":"2024-12-19T16:04:17Z","snapshot_observed_at":"2026-08-11T11:41:46.625773Z","submitted_at":"2024-12-19T16:04:17Z","title":"Neutrino electromagnetic properties and sterile dipole portal in light of the first solar CE$\\nu$NS data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.14991","snapshot_observed_at":"2026-08-15T15:51:27.332354Z","title":"De Romeri, D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.332354Z"},"links":{"cited_paper":"/paper/2412.14991","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:1375bdb17986075df76bdb774ff69236e4d7c89ff8958155b2a33ea74907830e","observation_id":"e3e52e8f-d280-4f1b-9645-d141a42868bc","resolution":{"observed_at":"2026-08-15T15:51:27.332354Z","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":"2026-08-15T15:51:27.339095Z","title":"Atzori Corona, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.339095Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:4e870e4e6b2182034af322639aad7570f794d32d31650c86eb892245509f67d1","observation_id":"86fe7fe1-1c86-4c7f-8a45-9990d5f95ae0","resolution":{"observed_at":"2026-08-15T15:51:27.339095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.18550","last_updated":"2025-07-18T08:36:36Z","snapshot_observed_at":"2026-08-15T06:43:30.259184Z","submitted_at":"2025-01-30T18:26:47Z","title":"Reactor antineutrinos CE$\\nu$NS on germanium: CONUS+ and TEXONO as a new gateway to SM and BSM physics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.18550","snapshot_observed_at":"2026-08-15T15:51:27.343373Z","title":"Atzori Corona, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.343373Z"},"links":{"cited_paper":"/paper/2501.18550","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:799b2d3598f3505e954b3871314e53ab6b421283d09a311a2e3bbf0a94c262d3","observation_id":"c8af6a4c-1a98-474d-a3af-9600f6bf1015","resolution":{"observed_at":"2026-08-15T15:51:27.343373Z","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":"ex/0607010","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T15:51:28.608032Z","title":"Aharmim et al","venue":null,"work_id":"88e8c2d1-9088-4f95-b7e8-32dfec253db7","year":2006},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.350422Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:937a849d42fd5ae2428eb4dcae310bb35563c4e2f98952927481b75388bf39b2","observation_id":"11dffdfe-fcb6-4a38-b54b-125c609c1f17","resolution":{"observed_at":"2026-08-15T15:51:28.615799Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T15:51:27.363407Z","title":"Safronova, D","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.363407Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:ead86968bd0ef37342c45d8890292d161684e291bfe4dc026f0478a6d60e1243","observation_id":"077a3b68-46e9-405c-b787-d5ce33e88a26","resolution":{"observed_at":"2026-08-15T15:51:27.363407Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.03280","last_updated":"2021-07-19T09:45:48Z","snapshot_observed_at":"2026-08-16T18:33:13.754553Z","submitted_at":"2021-04-07T17:36:01Z","title":"Muon and electron g-2 and proton and cesium weak charges implications on dark $\\mathbf{Z_d}$ models","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.03280","snapshot_observed_at":"2026-08-15T15:51:27.369604Z","title":"Cadeddu, N","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.369604Z"},"links":{"cited_paper":"/paper/2104.03280","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:d7b7b3d9569b9bd544e633f42ffcea79031f2dbcc7a370214878d01dc2c8e005","observation_id":"56f30dad-f15e-4a86-a0d0-97147d5b4e9d","resolution":{"observed_at":"2026-08-15T15:51:27.369604Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.09717","last_updated":"2022-05-20T10:40:53Z","snapshot_observed_at":"2026-08-16T17:33:42.136370Z","submitted_at":"2021-12-17T19:00:10Z","title":"Incorporating the weak mixing angle dependence to reconcile the neutron skin measurement on 208Pb by PREX-II","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.09717","snapshot_observed_at":"2026-08-15T15:51:27.375292Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.375292Z"},"links":{"cited_paper":"/paper/2112.09717","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:dc7689aeea56188d4b27e4b0f5579645672809a77e636229dd6c318f391e1d76","observation_id":"6aa97624-4342-4102-a225-509edbe9ea84","resolution":{"observed_at":"2026-08-15T15:51:27.375292Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.09743","last_updated":"2024-10-08T13:38:38Z","snapshot_observed_at":"2026-08-16T13:34:35.288087Z","submitted_at":"2024-07-13T02:16:28Z","title":"Simultaneous Extraction of the Weak Radius and the Weak Mixing Angle from Parity-Violating Electron Scattering on $^{12}\\mathrm{C}$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.09743","snapshot_observed_at":"2026-08-15T15:51:27.379536Z","title":"Cadeddu, N","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.379536Z"},"links":{"cited_paper":"/paper/2407.09743","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:af89cbd1512a40db66a2322670644c1d81c8bf05f19d48edb884920eae8cf245","observation_id":"c80f4512-1be9-49a7-a808-4cc2163cfc2e","resolution":{"observed_at":"2026-08-15T15:51:27.379536Z","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":"2026-08-15T15:51:27.384808Z","title":null,"venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.384808Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:76372dd185eeee9f4a9fe07316638707400734cee62e2c4f39f2a4557fbafb89","observation_id":"21e551a0-f7eb-418b-ab96-1491275e3442","resolution":{"observed_at":"2026-08-15T15:51:27.384808Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.5864","last_updated":"2012-07-25T01:21:40Z","snapshot_observed_at":"2026-08-16T17:53:31.921788Z","submitted_at":"2012-07-25T01:21:40Z","title":"Revisiting parity non-conservation in cesium","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.5864","snapshot_observed_at":"2026-08-15T15:51:27.391744Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.391744Z"},"links":{"cited_paper":"/paper/1207.5864","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:d47e27d6a3fd30b69559ea3f5232ba3869492153e55f494daec36ecc4337d203","observation_id":"cb631d95-8dff-4281-9855-7cfd0e63a867","resolution":{"observed_at":"2026-08-15T15:51:27.391744Z","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":"2026-08-15T15:51:27.396823Z","title":"Androic et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.396823Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:a063481f41e951a6b476519e12327a763e2d3ba0516f0c3227103c492262cdce","observation_id":"1395cf2a-787e-4d97-b924-79792dc8ac30","resolution":{"observed_at":"2026-08-15T15:51:27.396823Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ex/0504049","last_updated":"2005-04-26T19:44:49Z","snapshot_observed_at":"2026-08-05T22:49:20.370832Z","submitted_at":"2005-04-26T19:44:49Z","title":"Precision Measurement of the Weak Mixing Angle in Moller Scattering","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ex/0504049","snapshot_observed_at":"2026-08-15T15:51:27.403934Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.403934Z"},"links":{"cited_paper":"/paper/hep-ex/0504049","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:9a348ed2d8ce17950dddb42d4e23d73443cb002ff32325887ab64f01a845d38d","observation_id":"d12c97c7-0c10-459b-9890-098471431dc4","resolution":{"observed_at":"2026-08-15T15:51:27.403934Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.04385","last_updated":"2025-09-04T08:49:09Z","snapshot_observed_at":"2026-08-16T13:20:42.192500Z","submitted_at":"2024-09-06T16:22:44Z","title":"First constraint on the weak mixing angle using direct detection experiments","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.04385","snapshot_observed_at":"2026-08-15T15:51:27.409773Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.409773Z"},"links":{"cited_paper":"/paper/2409.04385","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:85c363af1c8edaa1903df577b7872e461dfd076534d7beef6630548898927452","observation_id":"15c84ce8-a985-4b34-a0ab-aec50e4470b1","resolution":{"observed_at":"2026-08-15T15:51:27.409773Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.17380","last_updated":"2023-11-07T10:52:03Z","snapshot_observed_at":"2026-08-16T14:56:26.934973Z","submitted_at":"2023-09-29T16:29:21Z","title":"Testing neutrino electromagnetic properties at current and future dark matter experiments","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.17380","snapshot_observed_at":"2026-08-15T15:51:27.414321Z","title":"Giunti and C","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.414321Z"},"links":{"cited_paper":"/paper/2309.17380","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:1e8ba25c2096ae09aef6fe2f728dc0b94474587f791e8ad4d8318700cfc6f30e","observation_id":"fd7abf8a-7c6a-4625-b6ea-ffd287e5854b","resolution":{"observed_at":"2026-08-15T15:51:27.414321Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.03122","last_updated":"2024-11-25T14:59:27Z","snapshot_observed_at":"2026-08-16T13:02:45.600515Z","submitted_at":"2024-11-05T14:13:34Z","title":"Neutrino Electromagnetic Properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.03122","snapshot_observed_at":"2026-08-15T15:51:27.418520Z","title":"Giunti, K","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.418520Z"},"links":{"cited_paper":"/paper/2411.03122","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:24c171826d9cbc69e9745b476568efe0d741dad484aba6b361bfce3e13f306ab","observation_id":"30860504-80fe-4bdc-812d-1f7a7beea356","resolution":{"observed_at":"2026-08-15T15:51:27.418520Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0008114","last_updated":"2000-08-11T16:05:09Z","snapshot_observed_at":"2026-08-15T11:30:12.602308Z","submitted_at":"2000-08-11T16:05:09Z","title":"On the charge radius of the neutrino","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0008114","snapshot_observed_at":"2026-08-15T15:51:27.423118Z","title":"Bernabeu, L","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.423118Z"},"links":{"cited_paper":"/paper/hep-ph/0008114","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:55edd72bf1b4eab100e3a4e12094c1168598593d0e2db924c2a983b1d712f468","observation_id":"80b9aed3-eade-4dca-8c2b-c806737f486b","resolution":{"observed_at":"2026-08-15T15:51:27.423118Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.00401","last_updated":"2017-10-20T08:13:16Z","snapshot_observed_at":"2026-08-14T21:14:04.476514Z","submitted_at":"2017-03-01T17:23:36Z","title":"Electromagnetic properties of massive neutrinos in low-energy elastic neutrino-electron scattering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.00401","snapshot_observed_at":"2026-08-15T15:51:27.427629Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.427629Z"},"links":{"cited_paper":"/paper/1703.00401","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:21bf9049d19669269e0e1de7b80b20a5545fd974cce0e78fba508134dac3e8b1","observation_id":"1cc48ef7-f3fa-49f2-882e-372cfb682b24","resolution":{"observed_at":"2026-08-15T15:51:27.427629Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.07730","last_updated":"2022-06-02T22:48:46Z","snapshot_observed_at":"2026-08-16T17:49:11.451607Z","submitted_at":"2021-10-14T21:17:46Z","title":"Measurement of the Coherent Elastic Neutrino-Nucleus Scattering Cross Section on CsI by COHERENT","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.07730","snapshot_observed_at":"2026-08-15T15:51:27.433422Z","title":"Akimov et al., Measurement of the Coherent Elastic Neutrino-Nucleus Scattering Cross Section on CsI by COHERENT (2021), arXiv:2110.07730 [hep-ex]","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.433422Z"},"links":{"cited_paper":"/paper/2110.07730","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:665288b6c2089d1bbb47c8298a762f324feb067919fa54a4b8afcba8776561d9","observation_id":"07302901-7f25-43dd-aaae-a560ee98a8f3","resolution":{"observed_at":"2026-08-15T15:51:27.433422Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.10630","last_updated":"2021-02-15T22:11:01Z","snapshot_observed_at":"2026-08-09T10:39:48.842335Z","submitted_at":"2020-03-24T02:57:01Z","title":"First Measurement of Coherent Elastic Neutrino-Nucleus Scattering on Argon","version":7},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.10630","snapshot_observed_at":"2026-08-15T15:51:27.438072Z","title":"Akimov et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.438072Z"},"links":{"cited_paper":"/paper/2003.10630","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:8ade54feda373958c8f3664452cd2a89167b2a8e57fe8ad902331d3c88fe3348","observation_id":"330091bd-d610-435a-a9a5-519b8dca6b97","resolution":{"observed_at":"2026-08-15T15:51:27.438072Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.12659","last_updated":"2020-07-29T13:47:50Z","snapshot_observed_at":"2026-07-06T09:31:42.788370Z","submitted_at":"2020-06-22T22:49:30Z","title":"COHERENT Collaboration data release from the first detection of coherent elastic neutrino-nucleus scattering on argon","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.12659","snapshot_observed_at":"2026-08-15T15:51:27.443282Z","title":"Akimov et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.443282Z"},"links":{"cited_paper":"/paper/2006.12659","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:173aa4f589268bbffc98ea945a266ab242d6d1da169a6313b222a8c05da04d0f","observation_id":"3efd5141-9b1d-4cb1-abbf-c2854c875d3d","resolution":{"observed_at":"2026-08-15T15:51:27.443282Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.05206","last_updated":"2025-07-31T11:24:18Z","snapshot_observed_at":"2026-08-15T00:59:02.965584Z","submitted_at":"2025-01-09T12:57:38Z","title":"Direct observation of coherent elastic antineutrino-nucleus scattering","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.05206","snapshot_observed_at":"2026-08-15T15:51:27.451152Z","title":"Ackermann et al., First observation of reactor antineutrinos by coherent scattering (2025), arXiv:2501.05206 [hep-ex]","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.451152Z"},"links":{"cited_paper":"/paper/2501.05206","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:ef27256ae5ef0ed96100d8af51296da81a4d046109390dc37200289fd16ce6a4","observation_id":"da48830e-efa5-49eb-aca5-bebb9c486980","resolution":{"observed_at":"2026-08-15T15:51:27.451152Z","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":"2026-08-15T15:51:27.455570Z","title":"Karmakar et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.455570Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:3a060931d0a0c08b894c77d25edfc366a33797c415d437ba2f4b24ba07dbe535","observation_id":"65ddbc87-1bd3-452b-9a49-b9ad8e55fcbe","resolution":{"observed_at":"2026-08-15T15:51:27.455570Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.18502","last_updated":"2025-02-21T10:55:18Z","snapshot_observed_at":"2026-08-16T12:56:23.262382Z","submitted_at":"2025-02-21T10:55:18Z","title":"New constraints on coherent elastic neutrino-nucleus scattering by the nuGeN experiment","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.18502","snapshot_observed_at":"2026-08-15T15:51:27.459327Z","title":"Belov et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.459327Z"},"links":{"cited_paper":"/paper/2502.18502","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:abb8cea0b1c14093d5271179556cd367dae622de9bfd4f3b8536d2b587b70235","observation_id":"db983031-ba2d-4425-a0f3-d2a903c416c9","resolution":{"observed_at":"2026-08-15T15:51:27.459327Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.1597","last_updated":"2010-04-07T09:25:43Z","snapshot_observed_at":"2026-08-15T15:44:02.414678Z","submitted_at":"2009-11-09T07:29:13Z","title":"Measurement of Neutrino-Electron Scattering Cross-Section with a CsI(Tl) Scintillating Crystal Array at the Kuo-Sheng Nuclear Power Reactor","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.1597","snapshot_observed_at":"2026-08-15T15:51:27.463114Z","title":"Deniz et al","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.463114Z"},"links":{"cited_paper":"/paper/0911.1597","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:32a7c1b383818f60cc0c14d6a1f1514bd8c9b32151a28b46812c60c4c86fb456","observation_id":"9a6634c3-f2a8-41fe-ab9a-50a88ef9061f","resolution":{"observed_at":"2026-08-15T15:51:27.463114Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ex/0101039","last_updated":"2001-01-22T18:00:10Z","snapshot_observed_at":"2026-07-07T03:33:18.246007Z","submitted_at":"2001-01-22T18:00:10Z","title":"Measurement of electron-neutrino electron elastic scattering","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ex/0101039","snapshot_observed_at":"2026-08-15T15:51:27.467871Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.467871Z"},"links":{"cited_paper":"/paper/hep-ex/0101039","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:17fe318f970cceb631e5f50d7bad72305bf339f0919723d9166ccaac7ecb8b9b","observation_id":"72b2ae64-5a04-4536-a506-24a331dba605","resolution":{"observed_at":"2026-08-15T15:51:27.467871Z","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":"2026-08-15T15:51:27.472409Z","title":null,"venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.472409Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:8683b2cefbc83ee7a84bfa0be22d16f5af769410072b75f5c578d56bc70aa939","observation_id":"179fc5c1-acde-48e0-8f16-da79ca423989","resolution":{"observed_at":"2026-08-15T15:51:27.472409Z","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":"2026-08-15T15:51:27.478393Z","title":"Ahrens, S","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.478393Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:4cc2a048f5bee83e430212ace6f7b1723c11b0cc9d1d0e5be62624a4b1342819","observation_id":"3ec50e41-ecdf-4062-a8e5-747ddf402206","resolution":{"observed_at":"2026-08-15T15:51:27.478393Z","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":"2026-08-15T15:51:27.482596Z","title":"Vilain et al","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.482596Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:ff82444d247c562f4cb5fa1b88ceeb402f561695a440b8023a38b3a84639fe17","observation_id":"8175a367-3daf-412d-8737-02c1413460a5","resolution":{"observed_at":"2026-08-15T15:51:27.482596Z","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":"2026-08-15T15:51:27.486543Z","title":"Vilain et al","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.486543Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:08cc8c4783d18da3c8582b76590846d751f278b50adade02b701eb1b89c17193","observation_id":"ece638b0-08bc-49db-bcdd-bd657a7107a8","resolution":{"observed_at":"2026-08-15T15:51:27.486543Z","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":"2026-08-15T15:51:27.491488Z","title":"Vilain et al","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.491488Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:3cdd0586a8294850bb061f1ed62a23c137d1f085e93fc20f491c10a5f59af08f","observation_id":"285fb507-b492-46c9-97cc-b2c5bcb0e899","resolution":{"observed_at":"2026-08-15T15:51:27.491488Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ex/9701010","last_updated":"1997-01-21T00:27:46Z","snapshot_observed_at":"2026-07-07T03:38:53.401732Z","submitted_at":"1997-01-21T00:27:46Z","title":"A Precision Measurement of Electroweak Parameters in Neutrino-Nucleon Scattering","version":1},"cited_work":{"arxiv_id":"hep-ex/9701010","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ex/9701010","snapshot_observed_at":"2026-08-15T15:51:28.159895Z","title":"A Precision Measurement of Electroweak Parameters in Neutrino-Nucleon Scattering","venue":"hep-ex","work_id":"fa9b4961-3083-4d06-9954-918b0464f0d7","year":1997},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.495504Z"},"links":{"cited_paper":"/paper/hep-ex/9701010","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:a8f677bed45bc39d1f46b3b5acf8e7c858dd379fc0fb1a284c95ec7c8614a853","observation_id":"8d40f567-bfcf-49c3-a4d2-596036731043","resolution":{"observed_at":"2026-08-15T15:51:28.166279Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1506.05387","last_updated":"2015-11-12T06:42:28Z","snapshot_observed_at":"2026-08-14T22:44:02.210897Z","submitted_at":"2015-06-17T17:21:06Z","title":"Electromagnetic neutrinos in laboratory experiments and astrophysics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.05387","snapshot_observed_at":"2026-08-15T15:51:27.500106Z","title":"Giunti, K","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.500106Z"},"links":{"cited_paper":"/paper/1506.05387","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:20af6d6df23ca5620dc2b348cf6fdb1487c1bbfb39a7b5c3717b1be5b6405335","observation_id":"b97ec4a7-bbf2-4dec-b298-c887939ab162","resolution":{"observed_at":"2026-08-15T15:51:27.500106Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.02633","last_updated":"2025-08-30T13:24:19Z","snapshot_observed_at":"2026-08-16T04:18:20.090986Z","submitted_at":"2025-05-05T13:23:45Z","title":"Neutrino magnetic moments: effective versus fundamental parameters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.02633","snapshot_observed_at":"2026-08-15T15:51:27.504671Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.504671Z"},"links":{"cited_paper":"/paper/2505.02633","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:17d09bb574de8f101319942e08a2597e8b51b06decc986e628300c7a46bb6d83","observation_id":"d2d05f98-9806-4a5f-a152-4a61ba837355","resolution":{"observed_at":"2026-08-15T15:51:27.504671Z","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":"2026-08-15T15:51:27.509051Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.509051Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:6938e21821d96874f8fb8d6c3bf8b5822edf65a3aeb7ba1e2c3dbfec7c1e083b","observation_id":"872d9c83-3fbc-4fb8-bcc7-9448cad5c1fb","resolution":{"observed_at":"2026-08-15T15:51:27.509051Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ex/0605006","last_updated":"2006-11-14T06:05:58Z","snapshot_observed_at":"2026-07-07T03:37:51.134237Z","submitted_at":"2006-05-01T04:28:24Z","title":"Search of Neutrino Magnetic Moments with a High-Purity Germanium Detector at the Kuo-Sheng Nuclear Power Station","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ex/0605006","snapshot_observed_at":"2026-08-15T15:51:27.513081Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.513081Z"},"links":{"cited_paper":"/paper/hep-ex/0605006","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:dbf500404d815a5eb3e670c86d6bd033c8363f701bc05e7607fcc0b6a1fb3ac9","observation_id":"ec88ca4c-e983-4c31-a7fd-cb32114d838e","resolution":{"observed_at":"2026-08-15T15:51:27.513081Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ex/0402015","last_updated":"2004-02-08T03:50:56Z","snapshot_observed_at":"2026-08-13T10:28:45.098774Z","submitted_at":"2004-02-08T03:50:56Z","title":"Limit On the Neutrino Magnetic Moment Using 1496 Days of Super-Kamiokande-i Solar Neutrino Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ex/0402015","snapshot_observed_at":"2026-08-15T15:51:27.517390Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.517390Z"},"links":{"cited_paper":"/paper/hep-ex/0402015","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:5fdbac3a4f112c98d926c7adf36364451c0dbf7069e38b3c2ec3027df17878f3","observation_id":"129c32f5-0cf2-4197-9850-791197769e16","resolution":{"observed_at":"2026-08-15T15:51:27.517390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ex/0502037","last_updated":"2005-05-06T12:19:39Z","snapshot_observed_at":"2026-08-08T00:40:13.019897Z","submitted_at":"2005-02-19T13:34:18Z","title":"Final results on the neutrino magnetic moment from the MUNU experiment","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ex/0502037","snapshot_observed_at":"2026-08-15T15:51:27.522307Z","title":"Daraktchieva et al","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.522307Z"},"links":{"cited_paper":"/paper/hep-ex/0502037","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:d3a8d39f70164e9fb12101c9fd932ea86df89c088fc0c06d6dab4a6c5f063455","observation_id":"17519e16-54dd-4d7e-b887-ba9eaedc0d6c","resolution":{"observed_at":"2026-08-15T15:51:27.522307Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.11891","last_updated":"2020-08-15T01:51:28Z","snapshot_observed_at":"2026-08-16T10:36:55.395624Z","submitted_at":"2020-05-25T02:36:16Z","title":"Search for exotic neutrino-electron interactions using solar neutrinos in XMASS-I","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.11891","snapshot_observed_at":"2026-08-15T15:51:27.526651Z","title":"Abe et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.526651Z"},"links":{"cited_paper":"/paper/2005.11891","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:a7239b9ed02c4ad96fb3267a2510367fb0ed70d90b2fdc4f0fd7aec185d9c6ca","observation_id":"5960066f-889b-4fb2-814a-9a19bb1e6062","resolution":{"observed_at":"2026-08-15T15:51:27.526651Z","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":"2026-08-15T15:51:27.531552Z","title":"Navas et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.531552Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:9f8b8120eae980cb83ec297a398a993611443f06b5476af4243cf680d0262240","observation_id":"a5606ce8-7fb4-4a03-b19c-5a41f7270d16","resolution":{"observed_at":"2026-08-15T15:51:27.531552Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.12257","last_updated":"2023-01-30T02:42:55Z","snapshot_observed_at":"2026-08-16T17:25:10.862824Z","submitted_at":"2022-01-28T17:17:20Z","title":"First upper limits on neutrino electromagnetic properties from the CONUS experiment","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.12257","snapshot_observed_at":"2026-08-15T15:51:27.537869Z","title":"Bonet et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.537869Z"},"links":{"cited_paper":"/paper/2201.12257","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:8e58cdb8e8f7832fabd2eb8e4aca8127c4a1a8dc7f8f8d93fe953ce103f58e3e","observation_id":"86d12a07-4634-4962-8253-adf05f1528d5","resolution":{"observed_at":"2026-08-15T15:51:27.537869Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.11330","last_updated":"2022-11-15T15:25:30Z","snapshot_observed_at":"2026-08-16T16:43:57.466227Z","submitted_at":"2022-07-22T20:47:41Z","title":"Search for New Physics in Electronic Recoil Data from XENONnT","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.11330","snapshot_observed_at":"2026-08-15T15:51:27.542635Z","title":"Aprile et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.542635Z"},"links":{"cited_paper":"/paper/2207.11330","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:86d7ec5bd935685b86b9b4bdb1b1678e2d2ce916d043f943b527b97872a6d8ce","observation_id":"b0a0fe52-8c6d-4f01-b5d9-3be4394866e4","resolution":{"observed_at":"2026-08-15T15:51:27.542635Z","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":"2026-08-15T15:51:27.547166Z","title":"Henke, E","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.547166Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:4f54fec393296d698c1402d394f41a979da30c5bf84e70b43243c254945108d1","observation_id":"ac93cae8-dfbf-4994-8694-fb086fcb5c46","resolution":{"observed_at":"2026-08-15T15:51:27.547166Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.7168","last_updated":"2014-07-31T04:00:33Z","snapshot_observed_at":"2026-08-14T23:32:27.975026Z","submitted_at":"2014-05-28T09:14:37Z","title":"Constraints on millicharged neutrinos via analysis of data from atomic ionizations with germanium detectors at sub-keV sensitivities","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.7168","snapshot_observed_at":"2026-08-15T15:51:27.551596Z","title":"Chen, H.-C","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.551596Z"},"links":{"cited_paper":"/paper/1405.7168","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:101ecc2711344b0a0815aaae82ea656d0de24180ffbe073a618cc10afd38f904","observation_id":"23a915d5-19e7-49f2-93d9-3c5571313883","resolution":{"observed_at":"2026-08-15T15:51:27.551596Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.05022","last_updated":"2021-01-21T14:13:35Z","snapshot_observed_at":"2026-08-10T21:46:01.222322Z","submitted_at":"2020-08-11T22:28:46Z","title":"Constraints on light vector mediators through coherent elastic neutrino nucleus scattering data from COHERENT","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.05022","snapshot_observed_at":"2026-08-15T15:51:27.556328Z","title":"Cadeddu, N","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.556328Z"},"links":{"cited_paper":"/paper/2008.05022","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:82f6e7bd916919718d98ac2683f99aa95097112fe78af4b784b13699b2f077c9","observation_id":"a4bb1b5d-d96e-4fb9-a90e-b04410b6eaf1","resolution":{"observed_at":"2026-08-15T15:51:27.556328Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.11002","last_updated":"2022-05-19T13:27:41Z","snapshot_observed_at":"2026-08-16T17:19:28.801234Z","submitted_at":"2022-02-22T16:08:19Z","title":"Probing light mediators and $(g-2)_{\\mu}$ through detection of coherent elastic neutrino nucleus scattering at COHERENT","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.11002","snapshot_observed_at":"2026-08-15T15:51:27.560639Z","title":"Atzori Corona, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.560639Z"},"links":{"cited_paper":"/paper/2202.11002","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:a6d40dc9c6a63fb12ec5cd5a44dfe4fd94b7f2f4996510c4212b28adb9deb7ed","observation_id":"0816b3b5-19dc-45c5-bf7f-b47aea641647","resolution":{"observed_at":"2026-08-15T15:51:27.560639Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.00466","last_updated":"2020-02-05T11:23:09Z","snapshot_observed_at":"2026-08-16T12:37:28.391613Z","submitted_at":"2019-09-01T20:12:07Z","title":"General COHERENT Constraints on Neutrino Non-Standard Interactions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.00466","snapshot_observed_at":"2026-08-15T15:51:27.565025Z","title":"Giunti, General COHERENT constraints on neutrino nonstandard interactions, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.565025Z"},"links":{"cited_paper":"/paper/1909.00466","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:3ad851ecd283a28c1e4b358a44673f27132d82f3b468bbd24153e8e79952f88a","observation_id":"b96ff136-5d59-4336-90fb-2c4c2c4628e2","resolution":{"observed_at":"2026-08-15T15:51:27.565025Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.14545","last_updated":"2021-03-12T16:33:10Z","snapshot_observed_at":"2026-08-16T19:10:08.938648Z","submitted_at":"2020-10-27T18:29:49Z","title":"Astrophysical constraints on non-standard coherent neutrino-nucleus scattering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.14545","snapshot_observed_at":"2026-08-15T15:51:27.569054Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.569054Z"},"links":{"cited_paper":"/paper/2010.14545","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:bccda16385c2bc72d5f04cd1f18068b15bbb41781e01205b80f848f683b0475c","observation_id":"d4e7cdb9-a526-4507-84f1-9e96a9cecd37","resolution":{"observed_at":"2026-08-15T15:51:27.569054Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2509.07856","last_updated":"2026-06-27T18:58:10Z","snapshot_observed_at":"2026-08-15T16:07:24.996010Z","submitted_at":"2025-09-09T15:35:29Z","title":"Oscillation-Independent Probes of Neutrino Non-Standard Interactions from Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.07856","snapshot_observed_at":"2026-08-15T15:51:27.574122Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.574122Z"},"links":{"cited_paper":"/paper/2509.07856","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:9186d948cf7135ae290e57a86bac20bf5105d5e8b59c59f821291c46ad7d97d8","observation_id":"d3a5ceb9-df5d-48ca-bbe5-e7c3a5c983da","resolution":{"observed_at":"2026-08-15T15:51:27.574122Z","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":"2026-08-15T15:51:27.578490Z","title":"Atzori Corona, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.578490Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:68c580d33cfeaad1f5a25b045a814d6f602e011a47e2071db4225776efe93d09","observation_id":"8d852134-1cab-4976-9601-09564a2db7ae","resolution":{"observed_at":"2026-08-15T15:51:27.578490Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.03501","last_updated":"2016-06-10T23:43:18Z","snapshot_observed_at":"2026-08-14T21:53:14.160756Z","submitted_at":"2016-06-10T23:43:18Z","title":"Search for a muonic dark force at BABAR","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.03501","snapshot_observed_at":"2026-08-15T15:51:27.583298Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.583298Z"},"links":{"cited_paper":"/paper/1606.03501","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:4fb2fe803d4290699e46ac0b58093e3521ba297a35b042ce8b84b324732dbb7f","observation_id":"30c83412-4aa2-4632-8e9d-5d98391702c4","resolution":{"observed_at":"2026-08-15T15:51:27.583298Z","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":"2026-08-15T15:51:27.588180Z","title":null,"venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.588180Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:ea3b5e153b110adacf635ce0023c2e2e32c94b6746bc0530129c2719100a0f4d","observation_id":"ccaa3ef7-c798-4a79-8e28-f27d46ffbc72","resolution":{"observed_at":"2026-08-15T15:51:27.588180Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.2332","last_updated":"2014-08-20T19:49:49Z","snapshot_observed_at":"2026-08-14T23:31:00.356801Z","submitted_at":"2014-06-09T20:00:53Z","title":"Neutrino Trident Production: A Powerful Probe of New Physics with Neutrino Beams","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.2332","snapshot_observed_at":"2026-08-15T15:51:27.592904Z","title":"Altmannshofer, S","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.592904Z"},"links":{"cited_paper":"/paper/1406.2332","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:23a378c19e7c6ef4e898c06e68e7e909391eabaee53897034e374364a11d8d00","observation_id":"81201e04-1f83-46bb-b567-35cec38a32e5","resolution":{"observed_at":"2026-08-15T15:51:27.592904Z","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":"2026-08-15T15:51:27.597230Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.597230Z"},"links":{"citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:620e93a300595d5edffb7a37a38ee434f95a93c53d40a6db8065c83c7c5368c5","observation_id":"020009e5-4b8f-40d5-a8e0-7a8c01579217","resolution":{"observed_at":"2026-08-15T15:51:27.597230Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.21476","last_updated":"2025-09-11T09:32:41Z","snapshot_observed_at":"2026-08-05T08:03:04.600080Z","submitted_at":"2025-05-27T17:48:30Z","title":"The anomalous magnetic moment of the muon in the Standard Model: an update","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.21476","snapshot_observed_at":"2026-08-15T15:51:27.600956Z","title":"Aliberti et al., The anomalous magnetic moment of the muon in the Standard Model: an update (2025), arXiv:2505.21476 [hep-ph]","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.600956Z"},"links":{"cited_paper":"/paper/2505.21476","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:7b9390c41f2fe9956d754a320c67775ac86995ca546f4092d24bb62b9147884c","observation_id":"0b05a4c0-1c86-480c-9ea1-ef85685535e2","resolution":{"observed_at":"2026-08-15T15:51:27.600956Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.05506","last_updated":"2024-05-29T19:41:29Z","snapshot_observed_at":"2026-08-16T14:20:18.862570Z","submitted_at":"2024-02-08T09:24:16Z","title":"Light vector mediators at direct detection experiments","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.05506","snapshot_observed_at":"2026-08-15T15:51:27.605265Z","title":"De Romeri, D","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.605265Z"},"links":{"cited_paper":"/paper/2402.05506","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:514c5de44744208b1ddadc9aa361ab5de39a27487b77d38cce3f82264480157f","observation_id":"2acd9178-257f-40e3-acf5-cc8f2937ead5","resolution":{"observed_at":"2026-08-15T15:51:27.605265Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.20026","last_updated":"2025-02-27T12:10:29Z","snapshot_observed_at":"2026-08-16T12:54:40.444726Z","submitted_at":"2025-02-27T12:10:29Z","title":"Probing light mediators with recent PandaX-4T low energy electron recoil data","version":1},"cited_work":{"arxiv_id":"2502.20026","doi":null,"metadata_source":"pith","pith_arxiv_id":"2502.20026","snapshot_observed_at":"2026-08-15T15:51:27.768010Z","title":"Probing light mediators with recent PandaX-4T low energy electron recoil data","venue":"hep-ph","work_id":"6ab4de80-5d1d-4987-a4fd-b7a89f28339e","year":2025},"citing_paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors","version":3},"reference_index":101,"source":"pdf_text","source_observed_at":"2026-08-15T15:51:27.610183Z"},"links":{"cited_paper":"/paper/2502.20026","citing_paper":"/paper/2509.22178"},"observation_digest":"sha256:7e7b76ce4ca4dd16060768a64c7001ef2bd4020b68c7a3a127ffafc9cddcbd1f","observation_id":"948e6c73-f687-4061-b27e-7f947940f69a","resolution":{"observed_at":"2026-08-15T15:51:27.775302Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2509.22178","last_updated":"2026-06-03T09:06:00Z","latest_version":3,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-16T07:07:37.518223Z","submitted_at":"2025-09-26T10:37:46Z","title":"When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":97,"verified_exact":3,"verified_fuzzy":0},"total_outbound_references":106},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 100 of 106 outbound references and 6 inbound Pith citation observations for arXiv:2509.22178."}