{"as_of":"2026-08-21T18:45:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:14bc4a856d8bb19efdab067464c2240ce492abc96abe6a02e8325c6a015ceff4","coverage":[{"denominator":24,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":24,"source":"paper_references, paper_reference_links","source_observed_at":"2026-05-25T05:40:54.900959Z","state":"measured"},{"denominator":26,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":26,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-21T06:32:19.484+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T15:35:45.941616Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-15T15:35:47.053219Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2605.22935","snapshot_observed_at":"2026-08-01T04:27:08.783634Z","title":"Kelly, N","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.22817","last_updated":"2026-07-24T18:00:05Z","snapshot_observed_at":"2026-08-20T06:23:09.688739Z","submitted_at":"2026-07-24T18:00:05Z","title":"$\\texttt{SNuDD}$: Solar Neutrinos for Direct Detection","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-01T04:27:08.783634Z"},"links":{"cited_paper":"/paper/2605.22935","citing_paper":"/paper/2607.22817"},"observation_digest":"sha256:1dfb330703952ba86e996ef3f312d1c8e2a473378c285f08e7f0e090e798f833","observation_id":"97d08819-e2fa-40cc-8e47-039c72cac7a2","resolution":{"observed_at":"2026-08-01T04:27:08.783634Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"cited_work":{"arxiv_id":"2605.22935","doi":null,"metadata_source":"pith","pith_arxiv_id":"2605.22935","snapshot_observed_at":"2026-08-15T15:35:47.053219Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","venue":"hep-ph","work_id":"16c55bae-2a6f-498a-92ba-9313b60a3a26","year":2026},"citing_paper":{"arxiv_id":"2607.24584","last_updated":"2026-07-27T15:51:27Z","snapshot_observed_at":"2026-08-18T07:00:31.088045Z","submitted_at":"2026-07-27T15:51:27Z","title":"Invisible decay of solar neutrinos at dark matter experiments","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-15T15:35:45.941616Z"},"links":{"cited_paper":"/paper/2605.22935","citing_paper":"/paper/2607.24584"},"observation_digest":"sha256:a0fd2259fcec69b6d957479e922454146847aba2c406fba09e917cd863612f5e","observation_id":"1a9ae05e-068b-4d64-a2de-22caee34b069","resolution":{"observed_at":"2026-08-15T15:35:47.058941Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2605.22935/citation-record","integrity":"/paper/2605.22935/integrity","json":"/paper/2605.22935/citation-record.json","paper":"/paper/2605.22935"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2408.00664","last_updated":"2025-02-07T18:23:08Z","snapshot_observed_at":"2026-08-19T21:01:38.991439Z","submitted_at":"2024-08-01T15:59:50Z","title":"Dark Matter Search Results from 1.54 Tonne$\\cdot$Year Exposure of PandaX-4T","version":2},"cited_work":{"arxiv_id":"2408.00664","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.00664","snapshot_observed_at":"2026-07-10T13:27:05.854218Z","title":"Dark Matter Search Results from 1.54 Tonne·Year Exposure of PandaX-4T","venue":"hep-ex","work_id":"b2d7de9e-fee6-43b7-803e-7b139e7b7be6","year":2024},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/2408.00664","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:09e0fd7ee446a1b16b65b823f6ab56e676a999d90b172bb5f3dc77eb44157d47","observation_id":"7b67782a-70a3-48b2-b9cb-6177623e7ed4","resolution":{"observed_at":"2026-05-25T05:46:39.903948Z","resolver_source":"arxiv_id","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1307.5458","last_updated":"2014-01-19T18:10:55Z","snapshot_observed_at":"2026-08-15T14:31:45.246584Z","submitted_at":"2013-07-20T20:16:11Z","title":"Implication of neutrino backgrounds on the reach of next generation dark matter direct detection experiments","version":3},"cited_work":{"arxiv_id":"1307.5458","doi":null,"metadata_source":"pith","pith_arxiv_id":"1307.5458","snapshot_observed_at":"2026-07-04T10:59:46.709810Z","title":"Implication of neutrino backgrounds on the reach of next generation dark matter direct detection experiments","venue":"hep-ph","work_id":"ba252fe3-aa82-4c2e-b056-f86f6e62cedf","year":2013},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/1307.5458","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:91182b8818f650fc4d9c39f3edf7ca45602929cb15b450a0b4ed1469f745768c","observation_id":"6218a499-2f16-4cbb-9c17-ff0e132616d4","resolution":{"observed_at":"2026-05-25T05:46:39.922070Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1408.3581","last_updated":"2014-08-15T16:20:53Z","snapshot_observed_at":"2026-08-19T08:49:50.397480Z","submitted_at":"2014-08-15T16:20:53Z","title":"Complementarity of dark matter detectors in light of the neutrino background","version":1},"cited_work":{"arxiv_id":"1408.3581","doi":null,"metadata_source":"pith","pith_arxiv_id":"1408.3581","snapshot_observed_at":"2026-07-03T16:18:38.249774Z","title":"Complementarity of dark matter detectors in light of the neutrino background","venue":"hep-ph","work_id":"b865548d-a1ef-4743-b8dd-da261262c41c","year":2014},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/1408.3581","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:c08450c031e9281e6db2e882abde264d3da55835add1388ef625533a93797e90","observation_id":"261d443b-bb3c-423a-a5cc-8256c2270416","resolution":{"observed_at":"2026-05-25T05:46:39.909242Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2109.03116","last_updated":"2021-12-16T22:36:33Z","snapshot_observed_at":"2026-08-19T20:01:30.376408Z","submitted_at":"2021-09-07T14:23:56Z","title":"Fog on the horizon: a new definition of the neutrino floor for direct dark matter searches","version":2},"cited_work":{"arxiv_id":"2109.03116","doi":null,"metadata_source":"pith","pith_arxiv_id":"2109.03116","snapshot_observed_at":"2026-07-09T12:16:13.945925Z","title":"New Definition of the Neutrino Floor for Direct Dark Matter Searches","venue":"hep-ph","work_id":"d7910e6b-b068-47f2-bb07-c67d69575c8e","year":2021},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/2109.03116","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:c8a71be8ebf2f932090890e845aaaa510789336943c0ed2b7837d6ae15dad698","observation_id":"00c61b4e-de3a-4b30-82c2-d1774b697264","resolution":{"observed_at":"2026-05-25T05:46:39.874016Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1901.08876","last_updated":"2019-01-25T14:09:04Z","snapshot_observed_at":"2026-08-18T17:37:41.042000Z","submitted_at":"2019-01-25T14:09:04Z","title":"Neutrino physics with dark matter detectors","version":1},"cited_work":{"arxiv_id":"1901.08876","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1901.08876","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Neutrino physics with dark matter detectors","venue":null,"work_id":"513d6de9-495d-42d2-b6e0-0f43f1a13260","year":2019},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/1901.08876","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:c4a8b06263e6b5fff136a5e24b495a26a9d88bb55885215affd8a06ccb2dfc08","observation_id":"65de26e5-d22f-442b-8638-d32b514ac73f","resolution":{"observed_at":"2026-05-25T05:46:39.894676Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.17827","last_updated":"2023-09-27T01:03:48Z","snapshot_observed_at":"2026-08-20T02:14:17.926492Z","submitted_at":"2023-05-28T23:37:34Z","title":"Solar neutrinos with CE$\\nu$NS and flavor-dependent radiative corrections","version":2},"cited_work":{"arxiv_id":"2305.17827","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2305.17827","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Solar neutrinos with CEνNS and flavor-dependent radiative corrections","venue":null,"work_id":"16a50748-7147-46bb-9d3f-0510181b73a7","year":2023},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/2305.17827","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:bb6d08898a87c700f81c16f75ada4bf2054f2f83e0160dd46da80630fdc20914","observation_id":"9afa9ad2-9073-43fb-9f08-84ffcf1d2eb9","resolution":{"observed_at":"2026-05-25T05:46:39.927655Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.07361","last_updated":"2022-03-14T17:55:28Z","snapshot_observed_at":"2026-08-18T17:43:19.822684Z","submitted_at":"2022-03-14T17:55:28Z","title":"Coherent elastic neutrino-nucleus scattering: Terrestrial and astrophysical applications","version":1},"cited_work":{"arxiv_id":"2203.07361","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2203.07361","snapshot_observed_at":"2026-07-04T19:10:05.464968Z","title":"Coherent elastic neutrino-nucleus scattering: Terrestrial and astrophysical applications","venue":null,"work_id":"f936cf19-a291-4d03-9e46-b5f7e30d379d","year":2022},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/2203.07361","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:80b0bdcf89f5cf136017cca284b2656e0f6c712e1e4bcf423c60661a8ba25dd4","observation_id":"8a19eebe-5143-4213-a4c7-38b0c4c94a10","resolution":{"observed_at":"2026-05-25T05:46:39.915168Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Differences in the Coherent Interactions ofν e,ν µ andν τ","venue":null,"work_id":"1178b920-cb72-4879-a90c-20ef567035d7","year":1985},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:6cdbf1e2724a40d0c26a956a43abee3fdc2d6754d6e0e1dfb6048b53693dfa4b","observation_id":"a5921b68-aac2-4442-bcde-8603b619bb76","resolution":{"observed_at":"2026-05-25T10:56:54.399719Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2011.05960","last_updated":"2021-02-15T07:16:47Z","snapshot_observed_at":"2026-08-20T10:23:19.096255Z","submitted_at":"2020-11-11T18:26:42Z","title":"Flavor-dependent radiative corrections in coherent elastic neutrino-nucleus scattering","version":2},"cited_work":{"arxiv_id":"2011.05960","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2011.05960","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Flavor-dependent radiative corrections in coherent elastic neutrino-nucleus scattering","venue":null,"work_id":"ab234150-7a18-4aef-b80f-61f98b85e9c6","year":2021},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/2011.05960","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:2357af128021958f501ccde897681d1640a4325619cbcd7d8b9eac5cb1c195e4","observation_id":"092f45c9-1c69-4241-beb4-0daa88e73ab6","resolution":{"observed_at":"2026-05-25T05:46:39.880286Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2501.05206","last_updated":"2025-07-31T11:24:18Z","snapshot_observed_at":"2026-08-19T05:43:21.857925Z","submitted_at":"2025-01-09T12:57:38Z","title":"Direct observation of coherent elastic antineutrino-nucleus scattering","version":3},"cited_work":{"arxiv_id":"2501.05206","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2501.05206","snapshot_observed_at":"2026-07-03T21:58:59.250415Z","title":"First observation of reactor antineutrinos by coherent scattering","venue":null,"work_id":"d3936b4f-95c6-460f-b21a-895cd7906d48","year":2024},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/2501.05206","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:606fb272ee6abf7af3ed6f37403d756528282f39400b2433c228a1bf046c0d20","observation_id":"edbcc29b-bcdf-4a86-9293-fccf923fc230","resolution":{"observed_at":"2026-05-25T05:46:39.933383Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.02003","last_updated":"2024-09-03T15:48:57Z","snapshot_observed_at":"2026-08-18T16:21:03.297714Z","submitted_at":"2024-09-03T15:48:57Z","title":"Implications of first neutrino-induced nuclear recoil measurements in direct detection experiments","version":1},"cited_work":{"arxiv_id":"2409.02003","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2409.02003","snapshot_observed_at":"2026-07-03T16:18:38.316414Z","title":"Implications of first neutrino-induced nuclear recoil measurements in direct detection experiments: Probing nonstandard interaction via CEνNS","venue":null,"work_id":"ba86cbc6-fefd-4ca0-9c21-1574e5baa248","year":2025},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/2409.02003","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:f968308c614d481e78e3f76029cb33c8e60a59c35ed16804f768adfa66438cac","observation_id":"fa56fdad-0a7f-4984-b040-6a7d11bea7f3","resolution":{"observed_at":"2026-05-25T05:46:39.898311Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.14206","last_updated":"2025-08-01T09:08:31Z","snapshot_observed_at":"2026-08-14T21:33:16.407355Z","submitted_at":"2024-11-21T15:15:59Z","title":"Clarity through the Neutrino Fog: Constraining New Forces in Dark Matter Detectors","version":2},"cited_work":{"arxiv_id":"2411.14206","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2411.14206","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Clarity through the Neutrino Fog: Constraining New Forces in Dark Matter Detectors","venue":null,"work_id":"25924da4-8975-4d4e-a91a-1d3f14e6ce68","year":2025},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/2411.14206","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:55a4ba5fd2de4a2bd2d9df39b089f50903dea94dafffe89295d8eb67aa313fb5","observation_id":"4ab20d84-8bcf-4d7a-8999-588d15ae1618","resolution":{"observed_at":"2026-05-25T05:46:39.892400Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.04703","last_updated":"2025-01-30T13:09:03Z","snapshot_observed_at":"2026-08-18T17:37:42.303715Z","submitted_at":"2024-09-07T03:58:07Z","title":"Constraints on neutrino non-standard interactions from COHERENT, PandaX-4T and XENONnT","version":2},"cited_work":{"arxiv_id":"2409.04703","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2409.04703","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Constraints on neutrino nonstandard interactions from COHERENT, PandaX-4T and XENONnT","venue":null,"work_id":"c10e0ae8-1643-40df-a5ee-abe4cb9295bd","year":2025},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/2409.04703","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:bfe3826f261935a89a063489abd72a4be3e91707aa55866366df67e9be7c1f3c","observation_id":"28577f42-f6bf-4d86-8330-d22953d99d28","resolution":{"observed_at":"2026-05-25T05:46:39.832016Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"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":"2411.11749","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2411.11749","snapshot_observed_at":"2026-07-04T18:20:03.255638Z","title":"Bounds on new neutrino interactions from the first CEνNS data at direct detection experiments","venue":null,"work_id":"f4f9700a-df7c-46a8-a37d-2b6e44d02836","year":2025},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/2411.11749","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:8c6d9193e54d10f72ab2edcb45e02018a1751eb1c7d8e56b256e2566a4bd1325","observation_id":"2fd8d0c2-2594-4e2d-bb61-b6fcfe12abfa","resolution":{"observed_at":"2026-05-25T05:46:39.852451Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2512.19784","last_updated":"2026-07-11T02:06:13Z","snapshot_observed_at":"2026-08-18T22:06:00.470601Z","submitted_at":"2025-12-22T19:00:01Z","title":"Shifting the neutrino fog: studying the Isospin-violating Dark Matter case","version":2},"cited_work":{"arxiv_id":"2512.19784","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2512.19784","snapshot_observed_at":"2026-07-14T01:19:57.403343Z","title":"Shifting the neutrino fog: studying the Isospin-violating Dark Matter case","venue":null,"work_id":"8ef4fc94-b4af-4f4a-bc6b-3a98260ed801","year":null},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/2512.19784","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:962ced6626d75731ef07db781df7b7957a90fdd1cac2fc05df93d5c0a99489ae","observation_id":"5fdb5109-7232-418d-8133-ab2b6739812d","resolution":{"observed_at":"2026-07-14T01:19:57.403343Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":"2603.00554","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2603.00554","snapshot_observed_at":"2026-07-28T03:23:26.927194Z","title":"Testing light and heavy vector mediators with solar CEνNS measurements","venue":null,"work_id":"da094fc6-6c0d-471d-9408-d5c79d6c98f2","year":2026},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/2603.00554","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:f3329511406e90678e1fc5b63884fe344e144431759c533e422bb435a48d31a0","observation_id":"67cc6921-4e57-46fa-854d-112b6a8fa190","resolution":{"observed_at":"2026-07-28T03:23:26.927194Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"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":"2412.14991","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.14991","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Neutrino electromagnetic properties and sterile dipole portal in light of the first solar CEνNS data","venue":null,"work_id":"d8480aad-db31-4fbf-a9bb-eabc567b474d","year":2025},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/2412.14991","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:53361698eaa727db3a6aee70941eff787e42dfed5a5fc7913656fc0e3c834c5d","observation_id":"5bc440f9-b51a-42b8-a558-2e715d1a7408","resolution":{"observed_at":"2026-05-25T05:46:39.842384Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1803.10661","last_updated":"2018-03-28T14:49:48Z","snapshot_observed_at":"2026-08-18T17:42:50.495924Z","submitted_at":"2018-03-28T14:49:48Z","title":"Updated global analysis of neutrino oscillations in the presence of eV-scale sterile neutrinos","version":1},"cited_work":{"arxiv_id":"1803.10661","doi":null,"metadata_source":"pith","pith_arxiv_id":"1803.10661","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Updated global analysis of neutrino oscillations in the presence of eV-scale sterile neutrinos","venue":"hep-ph","work_id":"cc58f563-f203-4b69-9b2a-386ed8b9e9e3","year":2018},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/1803.10661","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:283e71131795311fa052d5ee7d6bb4bdc6b820f304f17116eefd7059254e3aee","observation_id":"7f2a98ca-0132-4a86-901d-10a478e8157b","resolution":{"observed_at":"2026-05-25T05:46:39.840887Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1409.0050","last_updated":"2014-08-29T22:15:11Z","snapshot_observed_at":"2026-08-19T08:40:58.837740Z","submitted_at":"2014-08-29T22:15:11Z","title":"Solar neutrino physics with low-threshold dark matter detectors","version":1},"cited_work":{"arxiv_id":"1409.0050","doi":null,"metadata_source":"pith","pith_arxiv_id":"1409.0050","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Solar neutrino physics with low-threshold dark matter detectors","venue":"astro-ph.CO","work_id":"2d954c24-8511-4deb-a67b-662c38c361e0","year":2014},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/1409.0050","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:329dc4fa8a2f9117c9498962bc476ceb12338b5fa54c20fe3595e174de0f5fb4","observation_id":"435c2355-e453-4b49-ab6c-b30d212e557d","resolution":{"observed_at":"2026-05-25T05:46:39.836612Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.16840","last_updated":"2025-02-06T17:43:42Z","snapshot_observed_at":"2026-08-17T17:04:24.372794Z","submitted_at":"2024-11-25T19:00:01Z","title":"Solar Model Independent Constraints on the Sterile Neutrino Interpretation of the Gallium Anomaly","version":2},"cited_work":{"arxiv_id":"2411.16840","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2411.16840","snapshot_observed_at":"2026-07-01T13:45:46.667480Z","title":"Solar model independent constraints on the sterile neutrino interpretation of the Gallium Anomaly","venue":null,"work_id":"dae86271-e44d-4185-be85-2f71ca8661ff","year":2025},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/2411.16840","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:03eb1b2f0f389dbca778c3c67d834ca637b838ca35673504de8f76ee9f130179","observation_id":"aa8fb20c-1cc2-4ab5-8612-e906f3cadc54","resolution":{"observed_at":"2026-05-25T05:46:39.837168Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1140/epjc/s10052-022-10052-2","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Testing sterile neutrino mixing with present and future solar neutrino data","venue":"The European Physical Journal C","work_id":"b008cd34-fa65-4c1c-9f87-2e2837767103","year":2022},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:a5e2e395145a97c75ca3721537180d8c699e24c6939c9cf490382e3f3050062d","observation_id":"c66d8433-b1f3-4ded-ae3a-676dda017411","resolution":{"observed_at":"2026-05-25T05:45:22.932034Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-05-25T18:23:28.895845+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-25T18:23:28.895845+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.05380","last_updated":"2025-10-28T13:33:51Z","snapshot_observed_at":"2026-08-13T20:34:18.192890Z","submitted_at":"2024-10-07T18:00:02Z","title":"NuFit-6.0: Updated global analysis of three-flavor neutrino oscillations","version":2},"cited_work":{"arxiv_id":"2410.05380","doi":null,"metadata_source":"pith","pith_arxiv_id":"2410.05380","snapshot_observed_at":"2026-07-10T19:37:33.987732Z","title":"NuFit-6.0: Updated global analysis of three-flavor neutrino oscillations","venue":"hep-ph","work_id":"b906c236-cb3d-4ee1-a23a-dd60cfeacff6","year":2024},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/2410.05380","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:8df22b104ae9b839025536f18cbf1c4d071261453cad4e17d39bb6c9b6dc7591","observation_id":"8bd8d267-5bb8-4039-a94e-4c0218defcd6","resolution":{"observed_at":"2026-05-25T05:46:39.847918Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1104.1816","last_updated":"2011-08-24T08:01:11Z","snapshot_observed_at":"2026-08-21T13:32:18.688569Z","submitted_at":"2011-04-10T23:31:23Z","title":"Precision measurement of the 7Be solar neutrino interaction rate in Borexino","version":2},"cited_work":{"arxiv_id":"1104.1816","doi":null,"metadata_source":"pith","pith_arxiv_id":"1104.1816","snapshot_observed_at":"2026-07-04T20:30:08.523386Z","title":"Precision measurement of the 7Be solar neutrino interaction rate in Borexino","venue":"hep-ex","work_id":"1b6a3dec-d31f-4b33-a19a-7cb1b20bef96","year":2011},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/1104.1816","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:5fd439ba3cfd0c77558088eff7f13aaf84dccb73a0672582d5c09a2490d9ee06","observation_id":"ef916df0-c673-44a3-b8a5-ba950e8f90d3","resolution":{"observed_at":"2026-05-25T05:46:39.869002Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1202.6073","last_updated":"2015-08-03T15:27:01Z","snapshot_observed_at":"2026-08-18T17:37:33.340611Z","submitted_at":"2012-02-27T21:18:57Z","title":"Exploring nu signals in dark matter detectors","version":3},"cited_work":{"arxiv_id":"1202.6073","doi":null,"metadata_source":"pith","pith_arxiv_id":"1202.6073","snapshot_observed_at":"2026-07-03T16:18:38.324879Z","title":"Exploring nu signals in dark matter detectors","venue":"hep-ph","work_id":"f109b0bf-900d-41d5-9d43-af6fb51251ce","year":2012},"citing_paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-25T05:40:54.900959Z"},"links":{"cited_paper":"/paper/1202.6073","citing_paper":"/paper/2605.22935"},"observation_digest":"sha256:f2a5483919596fa126b304b8a027a5566dd608109672e5248d50ecee3360a347","observation_id":"bd7f46c2-7b4f-4671-91b8-aee2cb934c5e","resolution":{"observed_at":"2026-05-25T05:46:39.819531Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2605.22935","last_updated":"2026-05-21T18:09:29Z","latest_version":1,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-15T14:31:42.555863Z","submitted_at":"2026-05-21T18:09:29Z","title":"Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering"},"reference_resolution":{"displayed":24,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":22,"verified_fuzzy":1},"total_outbound_references":24},"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":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 24 of 24 outbound references and 2 inbound Pith citation observations for arXiv:2605.22935."}