{"as_of":"2026-08-23T22:05:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:be581d89803f14acf5da068209de0cdc56aa9bd42ea6ca4025a80abb840bfe75","coverage":[{"denominator":98,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":98,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T22:10:27.622657Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-23T06:30:58.430688+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":"2026-08-06T12:09:11.412824Z","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":"2026-05-16T06:57:29.004684Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.22586","snapshot_observed_at":"2026-08-06T12:09:11.412824Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.22124","last_updated":"2025-07-29T18:00:13Z","snapshot_observed_at":"2026-08-14T20:41:49.296743Z","submitted_at":"2025-07-29T18:00:13Z","title":"Supernova cooling from neutrino-devouring dark matter","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T12:09:11.412824Z"},"links":{"cited_paper":"/paper/2506.22586","citing_paper":"/paper/2507.22124"},"observation_digest":"sha256:f84b9ee51c7564136e69612a7e139b921627a5a0f088fdaea172f5ef979cd283","observation_id":"7887e927-1a31-48e2-96c6-0d749ed0ca01","resolution":{"observed_at":"2026-08-06T12:09:11.412824Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"cited_work":{"arxiv_id":"2506.22586","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2506.22586","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Richardson et al., Phys","venue":null,"work_id":"6b30bde3-ca38-4d8f-be9e-bb7548bf16c6","year":2025},"citing_paper":{"arxiv_id":"2602.07384","last_updated":"2026-03-12T08:12:34Z","snapshot_observed_at":"2026-08-14T12:13:48.128812Z","submitted_at":"2026-02-07T05:56:50Z","title":"Constraints on Fermionic Dark Matter Absorption from Radiochemical Solar-Neutrino Measurements","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-16T06:56:04.056379Z"},"links":{"cited_paper":"/paper/2506.22586","citing_paper":"/paper/2602.07384"},"observation_digest":"sha256:7108a24c18a371ba3be97dfa6a35934d6ad204b29aaafa5a0fd584b4371701b4","observation_id":"3c95baf5-94eb-4c1e-ac03-2a05153db49d","resolution":{"observed_at":"2026-05-16T06:57:29.006191Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2506.22586/citation-record","integrity":"/paper/2506.22586/integrity","json":"/paper/2506.22586/citation-record.json","paper":"/paper/2506.22586"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2207.03764","last_updated":"2023-08-02T15:16:09Z","snapshot_observed_at":"2026-07-06T13:29:08.763456Z","submitted_at":"2022-07-08T09:10:04Z","title":"First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.03764","snapshot_observed_at":"2026-08-06T22:10:19.359898Z","title":"Aalberset al.(LZ), Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:19.359898Z"},"links":{"cited_paper":"/paper/2207.03764","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:bd52b54d6d684205d44336fec8dcbd8afdc6ac4cdc5c318330c030181e7cb93d","observation_id":"ad68db87-4684-4982-84b4-968a8a0ffa63","resolution":{"observed_at":"2026-08-06T22:10:19.359898Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.17868","last_updated":"2025-02-04T19:55:15Z","snapshot_observed_at":"2026-08-16T13:15:07.492684Z","submitted_at":"2024-09-26T14:17:18Z","title":"First Search for Light Dark Matter in the Neutrino Fog with XENONnT","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.17868","snapshot_observed_at":"2026-08-06T22:10:19.385608Z","title":"Aprileet al.(XENON), Phys","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:19.385608Z"},"links":{"cited_paper":"/paper/2409.17868","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:6f56f9d229fbe59a51f2c6140817afd1b41717bc38d7682bdb54f9c596389daa","observation_id":"186dd207-128d-4100-a87a-65c494b18da9","resolution":{"observed_at":"2026-08-06T22:10:19.385608Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.10067","last_updated":"2023-08-28T09:04:59Z","snapshot_observed_at":"2026-08-16T16:07:24.673210Z","submitted_at":"2022-12-20T08:19:12Z","title":"Search for light dark matter with ionization signals in the PandaX-4T Experiment","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.10067","snapshot_observed_at":"2026-08-06T22:10:19.451728Z","title":"Liet al.(PandaX), Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:19.451728Z"},"links":{"cited_paper":"/paper/2212.10067","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:2f76027b5789f26a4b6353a46dc0396c6218ded3da1f5702189d6b358f7719e1","observation_id":"062dadd5-392a-4d1f-ac4b-8fb158cfed3d","resolution":{"observed_at":"2026-08-06T22:10:19.451728Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.02723","last_updated":"2019-10-18T17:55:07Z","snapshot_observed_at":"2026-08-22T03:31:03.183151Z","submitted_at":"2019-06-06T17:46:06Z","title":"Search for Neutrinoless Double-Beta Decay with the Complete EXO-200 Dataset","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.02723","snapshot_observed_at":"2026-08-06T22:10:19.489262Z","title":"Antonet al.(EXO-200), Phys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:19.489262Z"},"links":{"cited_paper":"/paper/1906.02723","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:432659ff4206ff4159faee324521bdb82111fb8d7835bcac754b8ba675f41dca","observation_id":"6aad8b74-9291-401e-b1ab-82eafeab8398","resolution":{"observed_at":"2026-08-06T22:10:19.489262Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.11142","last_updated":"2018-08-13T19:27:15Z","snapshot_observed_at":"2026-08-18T19:55:50.877498Z","submitted_at":"2018-05-28T19:35:13Z","title":"nEXO Pre-Conceptual Design Report","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.11142","snapshot_observed_at":"2026-08-06T22:10:19.494820Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:19.494820Z"},"links":{"cited_paper":"/paper/1805.11142","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:695361fff3a93b14449666303491764dde1f53bafbaa6dc6d42e44b1cfb42fc0","observation_id":"e65b4b1d-5795-455b-98d4-07e67d880be0","resolution":{"observed_at":"2026-08-06T22:10:19.494820Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.11893","last_updated":"2023-06-21T03:54:15Z","snapshot_observed_at":"2026-08-17T23:05:49.223821Z","submitted_at":"2023-01-27T18:10:16Z","title":"Observation of low-lying isomeric states in $^{136}$Cs: a new avenue for dark matter and solar neutrino detection in xenon detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.11893","snapshot_observed_at":"2026-08-06T22:10:19.501547Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:19.501547Z"},"links":{"cited_paper":"/paper/2301.11893","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:0f3903bf3c6f6bcd791afbde7de499ce5a9826d610c7bd68ed02f616e8639f81","observation_id":"5990d774-4b39-44d2-af90-9a3ab2a08a53","resolution":{"observed_at":"2026-08-06T22:10:19.501547Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.04604","last_updated":"2023-06-08T17:38:05Z","snapshot_observed_at":"2026-08-16T15:25:45.199416Z","submitted_at":"2023-06-07T17:12:57Z","title":"$\\beta^-$ decay $Q$-value measurement of $^{136}$Cs and its implications to neutrino studies","version":2},"cited_work":{"arxiv_id":"2306.04604","doi":null,"metadata_source":"pith","pith_arxiv_id":"2306.04604","snapshot_observed_at":"2026-08-06T22:10:34.233145Z","title":"$\\beta^-$ decay $Q$-value measurement of $^{136}$Cs and its implications to neutrino studies","venue":"nucl-ex","work_id":"c5efb322-9daf-4d6c-b87f-857e6eba40c1","year":2023},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:19.548867Z"},"links":{"cited_paper":"/paper/2306.04604","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:c3396ffd1220097b3b72664c50bfbab853c7c464f58b07b06a016a387d1d59ed","observation_id":"1b552ef3-c519-4c9a-9746-6ecf89bc12b4","resolution":{"observed_at":"2026-08-06T22:10:34.307038Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-08-06T22:10:19.615020Z","title":"Fujioka, T","venue":null,"work_id":null,"year":1967},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:19.615020Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:807e5380d1291955dd6434be4b35e53b8f14fcd0756ec118499f962c97bb30fa","observation_id":"5f180ef4-5935-439d-8c6c-7949bfffec6b","resolution":{"observed_at":"2026-08-06T22:10:19.615020Z","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":"2026-08-06T22:10:19.713034Z","title":null,"venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:19.713034Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:47643b256117644a5b4d8e71e4ce747b7abf463e371c1f2416935899828f2539","observation_id":"62c9d26a-75d9-446b-9b79-94968df43ccc","resolution":{"observed_at":"2026-08-06T22:10:19.713034Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.4952","last_updated":"2012-07-20T13:49:39Z","snapshot_observed_at":"2026-08-15T00:52:35.915444Z","submitted_at":"2012-07-20T13:49:39Z","title":"Towards High-Energy Neutrino Astronomy. A Historical Review","version":1},"cited_work":{"arxiv_id":"1207.4952","doi":null,"metadata_source":"pith","pith_arxiv_id":"1207.4952","snapshot_observed_at":"2026-08-06T22:10:34.046583Z","title":"Towards High-Energy Neutrino Astronomy. A Historical Review","venue":"astro-ph.IM","work_id":"2425c6b7-f8a9-4228-8d61-c05cd35ec0dc","year":2012},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:19.843118Z"},"links":{"cited_paper":"/paper/1207.4952","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:e6c0930dfd03b7a1ca471aeb5409dd26a680f151a25a29a9a04eaf904c5c322e","observation_id":"b03189ee-3ea3-446d-afbe-fe3de61f0a1d","resolution":{"observed_at":"2026-08-06T22:10:34.118442Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2106.16243","last_updated":"2022-02-22T20:55:55Z","snapshot_observed_at":"2026-08-16T18:13:24.027847Z","submitted_at":"2021-06-30T17:55:12Z","title":"NEXO: Neutrinoless double beta decay search beyond $10^{28}$ year half-life sensitivity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.16243","snapshot_observed_at":"2026-08-06T22:10:19.941612Z","title":"Adhikariet al.(nEXO), J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:19.941612Z"},"links":{"cited_paper":"/paper/2106.16243","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:85c1b2f00505262125258ba088426767d0b3ed5d972138958a549d962438f4d1","observation_id":"be78526a-b760-4d19-b9cb-9ed0388e8614","resolution":{"observed_at":"2026-08-06T22:10:19.941612Z","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":"2026-08-06T22:10:20.025186Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:20.025186Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:ea79b5f27294edea1cbbed30e087335b129874443f62aa91cb15332b0c5dd905","observation_id":"937a2221-87db-49b5-b1b9-c42ab21d34cf","resolution":{"observed_at":"2026-08-06T22:10:20.025186Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.00535","last_updated":"2020-09-01T16:09:56Z","snapshot_observed_at":"2026-08-18T03:56:16.959847Z","submitted_at":"2020-09-01T16:09:56Z","title":"Solar neutrino detection in liquid xenon detectors via charged-current scattering to excited states","version":1},"cited_work":{"arxiv_id":"2009.00535","doi":null,"metadata_source":"pith","pith_arxiv_id":"2009.00535","snapshot_observed_at":"2026-08-06T22:10:33.902013Z","title":"Solar neutrino detection in liquid xenon detectors via charged-current scattering to excited states","venue":"hep-ex","work_id":"d0c40834-1a12-4d05-b8ae-0a16a9f275fc","year":2020},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:20.103799Z"},"links":{"cited_paper":"/paper/2009.00535","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:7e849984265118050d221bffc45ab7eb7a89e3bdc78ed1445dfc1e5a2d505dc7","observation_id":"80771f73-e050-4d59-a8fd-d5d7dcdf7582","resolution":{"observed_at":"2026-08-06T22:10:33.938692Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.00897","last_updated":"2023-02-20T14:29:27Z","snapshot_observed_at":"2026-08-19T17:21:19.288075Z","submitted_at":"2022-07-02T18:37:49Z","title":"Search for MeV Electron Recoils from Dark Matter in EXO-200","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.00897","snapshot_observed_at":"2026-08-06T22:10:20.160087Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:20.160087Z"},"links":{"cited_paper":"/paper/2207.00897","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:d3f134040916165af1540fd28951f36466f5a5840b15bffdaf4cabdbd456abe9","observation_id":"05634c2b-310c-4c67-bd53-df2c46a7a144","resolution":{"observed_at":"2026-08-06T22:10:20.160087Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.19419","last_updated":"2024-11-29T18:53:37Z","snapshot_observed_at":"2026-08-16T13:48:03.922345Z","submitted_at":"2024-05-29T18:01:20Z","title":"Supernova electron-neutrino interactions with xenon in the nEXO detector","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.19419","snapshot_observed_at":"2026-08-06T22:10:20.215666Z","title":"Hedgeset al.(nEXO), Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:20.215666Z"},"links":{"cited_paper":"/paper/2405.19419","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:f31f6ee4ac084c7434b831dad59504d0bc6d2d14dccbdd13afe9fadbbfad4198","observation_id":"088f3f78-08a8-47f3-a607-68983c45caa3","resolution":{"observed_at":"2026-08-06T22:10:20.215666Z","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":"2026-08-06T22:10:20.244748Z","title":"Davis, Prog","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:20.244748Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:77b53c5f7b3d4758388d92a5beb057905639e18c644e43cba8b845d1ddd8ca8b","observation_id":"ac1ec157-add3-4021-b349-9db92dace5d0","resolution":{"observed_at":"2026-08-06T22:10:20.244748Z","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":"2026-08-06T22:10:20.273667Z","title":null,"venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:20.273667Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:c5a796fdd504767f2c446538b8615d8c1b9001fcde697a40550439201f57eace","observation_id":"d678644d-828d-40ab-9727-147773d381aa","resolution":{"observed_at":"2026-08-06T22:10:20.273667Z","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":"2026-08-06T22:10:20.293491Z","title":"Kirsten, J","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:20.293491Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:c12c7d404f50663762d9b7a66c6cbc6a3e20153a9ebb52e37d09d55e4f92e868","observation_id":"1db6a509-ed71-4e45-8edb-ca4fde92bad0","resolution":{"observed_at":"2026-08-06T22:10:20.293491Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ex/0012030","last_updated":"2000-12-11T18:41:12Z","snapshot_observed_at":"2026-08-19T08:22:09.226054Z","submitted_at":"2000-12-11T18:41:12Z","title":"Science and Technology of BOREXINO: A Real Time Detector for Low Energy Solar Neutrinos SOLAR NEUTRINOS","version":1},"cited_work":{"arxiv_id":"hep-ex/0012030","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ex/0012030","snapshot_observed_at":"2026-08-06T22:10:33.762208Z","title":"Science and Technology of BOREXINO: A Real Time Detector for Low Energy Solar Neutrinos SOLAR NEUTRINOS","venue":"hep-ex","work_id":"3d9f2654-4111-4e24-b374-4242e3012e70","year":2000},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:20.321255Z"},"links":{"cited_paper":"/paper/hep-ex/0012030","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:f5471de4d099c56e46f96713e2ee84ea0efef7198af68de667947e95ca789a5c","observation_id":"91c9f607-8c3e-493e-9024-bacf5f25272c","resolution":{"observed_at":"2026-08-06T22:10:33.805872Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1109.0763","last_updated":"2011-09-04T22:39:58Z","snapshot_observed_at":"2026-08-15T22:38:52.651370Z","submitted_at":"2011-09-04T22:39:58Z","title":"Combined Analysis of all Three Phases of Solar Neutrino Data from the Sudbury Neutrino Observatory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1109.0763","snapshot_observed_at":"2026-08-06T22:10:20.367274Z","title":"Aharmimet al.(SNO), Phys","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:20.367274Z"},"links":{"cited_paper":"/paper/1109.0763","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:312d57b75aed7b5b90785c919ce101644ed0691648c0a5f32e80dca3c62bd536","observation_id":"21747ff6-5193-4c42-a71f-1ef39e06dc4e","resolution":{"observed_at":"2026-08-06T22:10:20.367274Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.03501","last_updated":"2021-02-22T05:13:36Z","snapshot_observed_at":"2026-08-19T19:45:57.069582Z","submitted_at":"2019-11-08T19:07:35Z","title":"Theia: An advanced optical neutrino detector","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.03501","snapshot_observed_at":"2026-08-06T22:10:20.400545Z","title":"Askinset al.(Theia), Eur","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:20.400545Z"},"links":{"cited_paper":"/paper/1911.03501","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:62f5e3fc09a5c986ecb98106a530235a84afbbbe2f7f42785da5b3d2f443e6a9","observation_id":"6ac8f314-bea4-43fe-8390-07c15ca2a262","resolution":{"observed_at":"2026-08-06T22:10:20.400545Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.08613","last_updated":"2021-07-19T04:47:50Z","snapshot_observed_at":"2026-08-21T17:41:07.389975Z","submitted_at":"2021-07-19T04:47:50Z","title":"The Future of Solar Neutrinos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.08613","snapshot_observed_at":"2026-08-06T22:10:20.447032Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:20.447032Z"},"links":{"cited_paper":"/paper/2107.08613","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:cc01aec3db03caa4572565028565f5161718e5cb5d3bdf6f0ffdbd7f31b503cd","observation_id":"6d489c60-5016-4a6e-a069-7fcf00583f52","resolution":{"observed_at":"2026-08-06T22:10:20.447032Z","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":"2026-08-06T22:10:20.559778Z","title":"Abuslemeet al.(JUNO), JCAP10, 022 (2023), arXiv:2303.03910 [hep-ex]","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:20.559778Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:930707f218314ab47e49feb92771fa072f48941de1ef6884f3ecfd19dab56539","observation_id":"5f1c4218-ec75-4cd9-abad-5128db887a48","resolution":{"observed_at":"2026-08-06T22:10:20.559778Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.11687","last_updated":"2021-08-25T18:44:38Z","snapshot_observed_at":"2026-08-18T07:49:50.047631Z","submitted_at":"2021-04-23T16:27:17Z","title":"The SNO+ Experiment","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.11687","snapshot_observed_at":"2026-08-06T22:10:20.694806Z","title":"Albaneseet al.(SNO+), JINST16, P08059 (2021), arXiv:2104.11687 [physics.ins-det]","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:20.694806Z"},"links":{"cited_paper":"/paper/2104.11687","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:1e69b315c50089c17fbfbee91391ff7dfa41a5f55a25784dfdfe0c156eb10a5e","observation_id":"97339b3a-8a8c-48bd-a2be-5091bd24d542","resolution":{"observed_at":"2026-08-06T22:10:20.694806Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.6240","last_updated":"2011-06-30T14:22:04Z","snapshot_observed_at":"2026-08-15T04:42:25.709144Z","submitted_at":"2011-06-30T14:22:04Z","title":"Identification of the slow E3 transition 136mCs -> 136Cs with conversion electrons","version":1},"cited_work":{"arxiv_id":"1106.6240","doi":null,"metadata_source":"pith","pith_arxiv_id":"1106.6240","snapshot_observed_at":"2026-08-06T22:10:33.516895Z","title":"Identification of the slow E3 transition 136mCs -> 136Cs with conversion electrons","venue":"nucl-ex","work_id":"6fd0f296-dcbc-4e0c-9784-f2addaf83a61","year":2011},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:20.846841Z"},"links":{"cited_paper":"/paper/1106.6240","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:532a127a7663047e3054b4ea859f52aa674a1c972fd730d5bfe345bf450b0e66","observation_id":"f521e55a-a7c6-4c0a-a8da-5f88b75c2155","resolution":{"observed_at":"2026-08-06T22:10:33.580488Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.11371","last_updated":"2023-07-14T02:25:49Z","snapshot_observed_at":"2026-08-16T15:59:52.968860Z","submitted_at":"2023-01-26T19:33:05Z","title":"$^{138}{\\rm Ba}(d,\\alpha)$ study of states in $^{136}{\\rm Cs}$: Implications for new physics searches with xenon detectors","version":3},"cited_work":{"arxiv_id":"2301.11371","doi":null,"metadata_source":"pith","pith_arxiv_id":"2301.11371","snapshot_observed_at":"2026-08-06T22:10:33.354373Z","title":"$^{138}{\\rm Ba}(d,\\alpha)$ study of states in $^{136}{\\rm Cs}$: Implications for new physics searches with xenon detectors","venue":"nucl-ex","work_id":"6a3263f5-33e8-43fb-bb6b-4a7cae80fde2","year":2023},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:20.926822Z"},"links":{"cited_paper":"/paper/2301.11371","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:75ebd00bb6ecfda5101f1c3750f681e47700938fe311ffce4e64fc996383c1e2","observation_id":"b10e5d08-b6db-47d1-b327-6990f5065d93","resolution":{"observed_at":"2026-08-06T22:10:33.432182Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1611.09867","last_updated":"2017-02-13T11:56:19Z","snapshot_observed_at":"2026-08-20T20:57:16.600751Z","submitted_at":"2016-11-29T21:00:10Z","title":"A new Generation of Standard Solar Models","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.09867","snapshot_observed_at":"2026-08-06T22:10:20.989317Z","title":"Vinyoleset al., Astrophys","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:20.989317Z"},"links":{"cited_paper":"/paper/1611.09867","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:79a7cf303ca1911f43f672841f7f6b5bdfb70cc52658ba1a66d942846537f93f","observation_id":"75f69ea4-1243-4547-bbfa-7e15a3787290","resolution":{"observed_at":"2026-08-06T22:10:20.989317Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.06488","last_updated":"2021-05-14T09:18:53Z","snapshot_observed_at":"2026-08-02T15:10:20.292790Z","submitted_at":"2020-07-13T16:38:09Z","title":"Solar structure and evolution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.06488","snapshot_observed_at":"2026-08-06T22:10:21.085454Z","title":"Christensen-Dalsgaard, Living Reviews in So- lar Physics18(2021), 10.1007/s41116-020-00028-3, arXiv:2007.06488v2 [astro-ph.SR]","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:21.085454Z"},"links":{"cited_paper":"/paper/2007.06488","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:a00c9f2e35e7249bc007dbaea8df0e379c82e2485313fd448db45ca4af420658","observation_id":"e0bdcbd6-83a2-4d5a-bc98-50940112cb4b","resolution":{"observed_at":"2026-08-06T22:10:21.085454Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.06522","last_updated":"2018-04-04T14:35:15Z","snapshot_observed_at":"2026-08-18T11:05:14.417439Z","submitted_at":"2017-12-18T16:58:48Z","title":"CNO Neutrino Grand Prix: The race to solve the solar metallicity problem","version":2},"cited_work":{"arxiv_id":"1712.06522","doi":null,"metadata_source":"pith","pith_arxiv_id":"1712.06522","snapshot_observed_at":"2026-08-06T22:10:33.216003Z","title":"CNO Neutrino Grand Prix: The race to solve the solar metallicity problem","venue":"hep-ph","work_id":"3947da0b-3e0b-497b-994a-63f248eaf6c4","year":2017},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:21.181068Z"},"links":{"cited_paper":"/paper/1712.06522","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:eb6f8890cd85851f62d018447f0298993b5841d2c9d27237f5afb400303b8588","observation_id":"617da58d-804e-4297-8335-d999ca3adc29","resolution":{"observed_at":"2026-08-06T22:10:33.257995Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-08-06T22:10:21.302766Z","title":null,"venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:21.302766Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:306fc02fe7442ddde65379e5ca22edbfc518aa0356c9d896fec7460a1c2925db","observation_id":"60ab5f20-c04f-4b11-bada-29e071423d55","resolution":{"observed_at":"2026-08-06T22:10:21.302766Z","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":"2026-08-06T22:10:21.422213Z","title":null,"venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:21.422213Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:d62f9fdb09448566606c01ac4b6db4b06586a1a0c1e7b26cc02bc9c9ca003612","observation_id":"0b04c50c-3598-4ed1-b8f4-c3547ec912b4","resolution":{"observed_at":"2026-08-06T22:10:21.422213Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.03512","last_updated":"2020-01-21T07:14:31Z","snapshot_observed_at":"2026-08-20T13:31:07.925759Z","submitted_at":"2019-05-09T10:02:49Z","title":"Constraints on Flavor-Diagonal Non-Standard Neutrino Interactions from Borexino Phase-II","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.03512","snapshot_observed_at":"2026-08-06T22:10:21.545885Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:21.545885Z"},"links":{"cited_paper":"/paper/1905.03512","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:f815404ac3906b2ad027aeb0c238b3fa17823ca1e41925b49e4ac90252e277ed","observation_id":"675731a1-025b-4b1b-834a-02ce8d9439a2","resolution":{"observed_at":"2026-08-06T22:10:21.545885Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.12635","last_updated":"2020-05-09T06:57:35Z","snapshot_observed_at":"2026-08-20T12:40:00.596234Z","submitted_at":"2019-05-29T18:00:01Z","title":"Direct Detection Signals from Absorption of Fermionic Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.12635","snapshot_observed_at":"2026-08-06T22:10:21.644186Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:21.644186Z"},"links":{"cited_paper":"/paper/1905.12635","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:64b81558a69038cdf418611dd253c950f1d3bb44c6956cf7148c11fc6ab812ee","observation_id":"6fe4c4e9-a08d-4dac-8f83-bec915e054e1","resolution":{"observed_at":"2026-08-06T22:10:21.644186Z","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":"10.1007/jhep02(2020)134","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T00:03:45.533247Z","title":null,"venue":"Journal of High Energy Physics","work_id":"7a8f4189-4400-4007-a5cb-aa44add7a7e5","year":2020},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:21.711742Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:204b7f07ef93ab8bf6b7dc915c679ae0e3d9efb7570867f27a1381e7c0195e3b","observation_id":"edf53c07-3c90-4ddc-8588-811442cb05d4","resolution":{"observed_at":"2026-08-06T22:10:27.957036Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.07512","last_updated":"2019-10-11T12:41:02Z","snapshot_observed_at":"2026-08-14T16:05:07.130346Z","submitted_at":"2019-07-17T13:37:02Z","title":"Simulation of charge readout with segmented tiles in nEXO","version":2},"cited_work":{"arxiv_id":"1907.07512","doi":null,"metadata_source":"pith","pith_arxiv_id":"1907.07512","snapshot_observed_at":"2026-08-06T22:10:33.019313Z","title":"Simulation of charge readout with segmented tiles in nEXO","venue":"physics.ins-det","work_id":"5e04c526-82e3-44d8-948c-b8bad9544421","year":2019},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:21.815534Z"},"links":{"cited_paper":"/paper/1907.07512","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:3fa776b324e1a33b49036feb1b9cfe78ce7354528231737df5aba9b3d89e33a0","observation_id":"ccb119b9-f401-44c0-9b58-7a4f474ae501","resolution":{"observed_at":"2026-08-06T22:10:33.098279Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05109","last_updated":"2018-01-19T22:24:53Z","snapshot_observed_at":"2026-08-16T12:00:50.581436Z","submitted_at":"2017-10-14T00:28:40Z","title":"Characterization of an Ionization Readout Tile for nEXO","version":2},"cited_work":{"arxiv_id":"1710.05109","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.05109","snapshot_observed_at":"2026-08-06T22:10:32.882945Z","title":"Characterization of an Ionization Readout Tile for nEXO","venue":"physics.ins-det","work_id":"f94f753d-4b09-4b26-95c2-a578f807be2b","year":2017},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:21.931369Z"},"links":{"cited_paper":"/paper/1710.05109","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:76748531f0cc52e9d70cf618268d26024050577388e8dffce2e2a447f0908580","observation_id":"dc2b79f1-5aac-40f9-aa55-f2e624649ec7","resolution":{"observed_at":"2026-08-06T22:10:32.943905Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1802.06162","last_updated":"2018-05-10T17:38:17Z","snapshot_observed_at":"2026-08-14T19:45:03.299405Z","submitted_at":"2018-02-17T00:05:33Z","title":"Liquid xenon scintillation measurements and pulse shape discrimination in the LUX dark matter detector","version":2},"cited_work":{"arxiv_id":"1802.06162","doi":null,"metadata_source":"pith","pith_arxiv_id":"1802.06162","snapshot_observed_at":"2026-08-06T22:10:32.738468Z","title":"Liquid xenon scintillation measurements and pulse shape discrimination in the LUX dark matter detector","venue":"physics.ins-det","work_id":"730ed1e9-9435-42a6-98c6-6d8e3859836a","year":2018},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:22.027435Z"},"links":{"cited_paper":"/paper/1802.06162","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:b63c4ad282a5be565f5c87588ee49b689036a4211e690ed0fe2aa7e3fffe7f88","observation_id":"8bf88785-adb2-4f05-996c-3ddac2190602","resolution":{"observed_at":"2026-08-06T22:10:32.811230Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1604.01503","last_updated":"2016-08-18T04:30:45Z","snapshot_observed_at":"2026-08-14T22:02:54.226654Z","submitted_at":"2016-04-06T06:22:00Z","title":"A measurement of the time profile of scintillation induced by low energy gamma-rays in liquid xenon with the XMASS-I detector","version":3},"cited_work":{"arxiv_id":"1604.01503","doi":null,"metadata_source":"pith","pith_arxiv_id":"1604.01503","snapshot_observed_at":"2026-08-06T22:10:32.403500Z","title":"A measurement of the time profile of scintillation induced by low energy gamma-rays in liquid xenon with the XMASS-I detector","venue":"physics.ins-det","work_id":"3a992107-51a4-4943-adfb-a33bc9d43ff6","year":2016},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:22.088179Z"},"links":{"cited_paper":"/paper/1604.01503","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:49ec2d2860829346f7081abc7b4d9208969d202641b5a0bf48147546a8ca0aba","observation_id":"986635e8-f321-4e0b-a298-8a41938229f2","resolution":{"observed_at":"2026-08-06T22:10:32.593480Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-08-06T22:10:22.152276Z","title":"Kubotaet al., Phys","venue":null,"work_id":null,"year":1979},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:22.152276Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:7a144c32c089e0af0d6d5ed2d1a2e6c0fbea92335a1e013aa2950dfeefaa39f5","observation_id":"b7b45f13-1a95-4a84-bbf4-636deb690306","resolution":{"observed_at":"2026-08-06T22:10:22.152276Z","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":"2026-08-06T22:10:22.225130Z","title":"Hitachiet al., Phys","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:22.225130Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:0b00eb3745a802c37055b29e2679f8335d482e04b21eee0987ca66132f3a3edc","observation_id":"40db40a0-a08d-4c7e-9625-63db77e43208","resolution":{"observed_at":"2026-08-06T22:10:22.225130Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.03663","last_updated":"2019-06-07T04:52:02Z","snapshot_observed_at":"2026-08-14T17:05:05.884892Z","submitted_at":"2019-03-08T20:37:11Z","title":"Characterization of the Hamamatsu VUV4 MPPCs for nEXO","version":3},"cited_work":{"arxiv_id":"1903.03663","doi":null,"metadata_source":"pith","pith_arxiv_id":"1903.03663","snapshot_observed_at":"2026-08-06T22:10:32.136544Z","title":"Characterization of the Hamamatsu VUV4 MPPCs for nEXO","venue":"astro-ph.IM","work_id":"3a154542-dfc8-4a77-a6bb-3500f8f5f7a1","year":2019},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:22.307520Z"},"links":{"cited_paper":"/paper/1903.03663","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:c6438b12f1f6eba079841e5f73b1d430154101a0e8463b76f03d78a3ef8745d3","observation_id":"a0e44cb8-2d35-41ac-be34-c1d29537475f","resolution":{"observed_at":"2026-08-06T22:10:32.248550Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1806.02220","last_updated":"2019-03-13T14:55:20Z","snapshot_observed_at":"2026-08-14T19:06:52.132241Z","submitted_at":"2018-06-06T14:33:22Z","title":"VUV-sensitive Silicon Photomultipliers for Xenon Scintillation Light Detection in nEXO","version":3},"cited_work":{"arxiv_id":"1806.02220","doi":null,"metadata_source":"pith","pith_arxiv_id":"1806.02220","snapshot_observed_at":"2026-08-06T22:10:31.834885Z","title":"VUV-sensitive Silicon Photomultipliers for Xenon Scintillation Light Detection in nEXO","venue":"physics.ins-det","work_id":"9b133283-6260-4bcb-9e4b-7e12af1e727e","year":2018},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:22.378431Z"},"links":{"cited_paper":"/paper/1806.02220","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:582e3cd27d5c059d742a54046d0e17e223ff9411b768c06a35e2b444041b0ea4","observation_id":"0ff91f9d-9a57-4d9a-a0ba-ba0551f4a1d8","resolution":{"observed_at":"2026-08-06T22:10:32.010327Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2209.07765","last_updated":"2022-11-25T16:55:04Z","snapshot_observed_at":"2026-08-18T03:56:12.316700Z","submitted_at":"2022-09-16T07:50:21Z","title":"Performance of novel VUV-sensitive Silicon Photo-Multipliers for nEXO","version":2},"cited_work":{"arxiv_id":"2209.07765","doi":null,"metadata_source":"pith","pith_arxiv_id":"2209.07765","snapshot_observed_at":"2026-08-06T22:10:31.645268Z","title":"Performance of novel VUV-sensitive Silicon Photo-Multipliers for nEXO","venue":"physics.ins-det","work_id":"2c07ca09-63e8-436e-9cc2-63137eeec39e","year":2022},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:22.475427Z"},"links":{"cited_paper":"/paper/2209.07765","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:5e0030f41f48fbc7f16c337a9687b3bce86228ed294ea7eba62e2f6e54312b1a","observation_id":"894f9a5a-e1fd-4935-9197-d447a4b71f69","resolution":{"observed_at":"2026-08-06T22:10:31.740931Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-08-06T22:10:22.547882Z","title":"Tsanget al., in2021 IEEE Nuclear Science Sym- posium and Medical Imaging Conference (NSS/MIC) (2021) pp","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:22.547882Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:78851cd775eca63da27dc32be4166d8bda062c0edf8c344042cb2df0e008cfbe","observation_id":"d5bdf589-c33e-4340-85aa-46b4523d4ad2","resolution":{"observed_at":"2026-08-06T22:10:22.547882Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.04467","last_updated":"2017-03-22T16:58:37Z","snapshot_observed_at":"2026-08-15T13:40:00.615739Z","submitted_at":"2016-09-14T22:41:29Z","title":"Measurement of the Drift Velocity and Transverse Diffusion of Electrons in Liquid Xenon with the EXO-200 Detector","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.04467","snapshot_observed_at":"2026-08-06T22:10:22.634804Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:22.634804Z"},"links":{"cited_paper":"/paper/1609.04467","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:24bdf1829a96b1ba0a17cdb4641a7be76ad6672c4080c832ee62f1390a87e79f","observation_id":"f47fa12c-2f52-4068-a82d-b0c3bc372979","resolution":{"observed_at":"2026-08-06T22:10:22.634804Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.11580","last_updated":"2019-11-25T00:31:17Z","snapshot_observed_at":"2026-08-14T09:31:32.922961Z","submitted_at":"2019-11-25T00:31:17Z","title":"Measurements of electron transport in liquid and gas Xenon using a laser-driven photocathode","version":1},"cited_work":{"arxiv_id":"1911.11580","doi":null,"metadata_source":"pith","pith_arxiv_id":"1911.11580","snapshot_observed_at":"2026-08-06T22:10:31.344529Z","title":"Measurements of electron transport in liquid and gas Xenon using a laser-driven photocathode","venue":"physics.ins-det","work_id":"936ca4f9-6fac-4c9b-b6bc-a8e5cff8009a","year":2019},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:22.721612Z"},"links":{"cited_paper":"/paper/1911.11580","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:c49e3aed9d0e3691ab2af04523f0cc93cb6b720a3826a7e9a19c4bd27e0dc355","observation_id":"6159fcc3-9783-4e41-8232-7e0b661a6192","resolution":{"observed_at":"2026-08-06T22:10:31.470432Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2303.13963","last_updated":"2023-12-12T10:52:23Z","snapshot_observed_at":"2026-08-23T03:32:05.371998Z","submitted_at":"2023-03-24T12:36:27Z","title":"Electron transport measurements in liquid xenon with Xenoscope, a large-scale DARWIN demonstrator","version":2},"cited_work":{"arxiv_id":"2303.13963","doi":null,"metadata_source":"pith","pith_arxiv_id":"2303.13963","snapshot_observed_at":"2026-08-06T22:10:31.091540Z","title":"Electron transport measurements in liquid xenon with Xenoscope, a large-scale DARWIN demonstrator","venue":"physics.ins-det","work_id":"7218e87f-8c9a-460d-87b8-e4898216c21b","year":2023},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:22.804099Z"},"links":{"cited_paper":"/paper/2303.13963","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:26fb97677be7ecae6e6ab6f815adf6c3d25fa8549d4c65c5648f45d5baebf474","observation_id":"a02d7503-f349-41bf-94f7-7719a7cdb209","resolution":{"observed_at":"2026-08-06T22:10:31.187501Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1802.06039","last_updated":"2019-12-02T22:25:08Z","snapshot_observed_at":"2026-08-14T19:45:09.256612Z","submitted_at":"2018-02-16T17:26:57Z","title":"Projected WIMP sensitivity of the LUX-ZEPLIN (LZ) dark matter experiment","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.06039","snapshot_observed_at":"2026-08-06T22:10:22.902261Z","title":"Akeribet al.(LUX-ZEPLIN), Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:22.902261Z"},"links":{"cited_paper":"/paper/1802.06039","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:f4d39747496edf3d3541fda27f2f13c2a0b4d8f32b52f6cc3b6a18a0a79310dd","observation_id":"22603d73-5baf-4b49-9715-9a3cb78ed35e","resolution":{"observed_at":"2026-08-06T22:10:22.902261Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.03825","last_updated":"2020-09-09T13:58:06Z","snapshot_observed_at":"2026-08-15T01:48:15.981239Z","submitted_at":"2020-03-08T18:37:30Z","title":"Energy resolution and linearity of XENON1T in the MeV energy range","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.03825","snapshot_observed_at":"2026-08-06T22:10:22.970544Z","title":"Aprileet al.(XENON), Eur","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:22.970544Z"},"links":{"cited_paper":"/paper/2003.03825","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:1825e9af8968d5e383a0cf931f5cc57e9825eafb1137181d346f94ca93e6a015","observation_id":"6b9be5f1-81d7-4c88-abdc-45eb57404501","resolution":{"observed_at":"2026-08-06T22:10:22.970544Z","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":"2026-08-06T22:10:23.070381Z","title":"Al Kharusi, Ph.D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:23.070381Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:e9ec37f05f7a97909b939d05c714fd5c4184fcade8ebbb45c193ba9727d03a9f","observation_id":"db6fb831-64f2-4ba1-9ab2-2dc366e8f18d","resolution":{"observed_at":"2026-08-06T22:10:23.070381Z","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":"2026-08-06T22:10:23.156479Z","title":"Fast optical monte carlo sim- ulation with surface-based geometries,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:23.156479Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:e6b1b31f9d48a572b5881bf11c04deee6a9c5b80c88cff030a72a59a6558bfc5","observation_id":"8c34a279-e6bd-4e3e-8680-ebf76c72a0aa","resolution":{"observed_at":"2026-08-06T22:10:23.156479Z","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":"2026-08-06T22:10:23.292991Z","title":"Jamil, Ph.D","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:23.292991Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:de964dc52887f50d1552396ffc39b2c51db12bcda98cfd73e2931fd14beab37e","observation_id":"1f93b26e-53b1-4636-8d19-0b2528cf291c","resolution":{"observed_at":"2026-08-06T22:10:23.292991Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.1613","last_updated":"2011-06-08T18:10:11Z","snapshot_observed_at":"2026-08-16T13:39:22.288690Z","submitted_at":"2011-06-08T18:10:11Z","title":"NEST: A Comprehensive Model for Scintillation Yield in Liquid Xenon","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.1613","snapshot_observed_at":"2026-08-06T22:10:23.410352Z","title":"Szydagiset al., JINST6, P10002 (2011), arXiv:1106.1613 [physics.ins-det]","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:23.410352Z"},"links":{"cited_paper":"/paper/1106.1613","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:c92c072f2318c119bcf740e05470a9ed362642d36ac8dd586bad15c4bc5b441d","observation_id":"7ca4568a-5145-4e52-ae25-d309afe4932f","resolution":{"observed_at":"2026-08-06T22:10:23.410352Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10231","last_updated":"2021-03-24T20:33:05Z","snapshot_observed_at":"2026-08-06T10:13:59.147071Z","submitted_at":"2020-09-22T00:27:10Z","title":"Event Reconstruction in a Liquid Xenon Time Projection Chamber with an Optically-Open Field Cage","version":2},"cited_work":{"arxiv_id":"2009.10231","doi":null,"metadata_source":"pith","pith_arxiv_id":"2009.10231","snapshot_observed_at":"2026-08-06T22:10:30.816057Z","title":"Event Reconstruction in a Liquid Xenon Time Projection Chamber with an Optically-Open Field Cage","venue":"physics.ins-det","work_id":"8522d557-c53c-4095-8220-725bf15b73dc","year":2020},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:23.502201Z"},"links":{"cited_paper":"/paper/2009.10231","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:6b1e9b8c5682644ba1a9d6a781f7b6769e6d9bb5c7c02a116819c11b70955334","observation_id":"77d05900-c568-4843-aeaa-86fc4d5a87b1","resolution":{"observed_at":"2026-08-06T22:10:30.923806Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-08-06T22:10:23.589173Z","title":"Liuet al., Vacuum197, 110806 (2022)","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:23.589173Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:0d08fa9ebfb5c7ff0ecc27ff138aabef40e7fbf71339eb518d7cc515d14a2670","observation_id":"cfe99785-ba30-4d5a-8b23-9eb04185c880","resolution":{"observed_at":"2026-08-06T22:10:23.589173Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.06204","last_updated":"2017-08-21T23:42:53Z","snapshot_observed_at":"2026-08-14T21:11:15.871133Z","submitted_at":"2017-03-17T21:39:06Z","title":"A method for characterizing after-pulsing and dark noise of PMTs and SiPMs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.06204","snapshot_observed_at":"2026-08-06T22:10:23.675396Z","title":"Butcheret al., Nucl","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:23.675396Z"},"links":{"cited_paper":"/paper/1703.06204","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:f9b7b7b234dc6f3f4ac635bef42e0986722514891b0698cff686cb20ef718ead","observation_id":"a098a97a-41bd-4683-8c85-1648df67db08","resolution":{"observed_at":"2026-08-06T22:10:23.675396Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.09634","last_updated":"2024-09-25T19:58:03Z","snapshot_observed_at":"2026-08-18T21:17:13.404721Z","submitted_at":"2024-02-15T00:25:29Z","title":"Stimulated Secondary Emission of Single Photon Avalanche Diodes","version":2},"cited_work":{"arxiv_id":"2402.09634","doi":null,"metadata_source":"pith","pith_arxiv_id":"2402.09634","snapshot_observed_at":"2026-08-06T22:10:30.627195Z","title":"Stimulated Secondary Emission of Single Photon Avalanche Diodes","venue":"physics.ins-det","work_id":"c0a6adbb-7424-4c0b-af93-587b01810080","year":2024},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:23.769112Z"},"links":{"cited_paper":"/paper/2402.09634","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:03bc1cbcf7a3041ebe611fb7088ba0478975f21eb54ca0f874188292d3efb724","observation_id":"dd8a8689-8758-448c-bb9c-caf24e4d4359","resolution":{"observed_at":"2026-08-06T22:10:30.670794Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.15991","last_updated":"2025-02-21T23:00:20Z","snapshot_observed_at":"2026-08-17T22:13:57.968844Z","submitted_at":"2025-02-21T23:00:20Z","title":"Characterization of external cross-talk from silicon photomultipliers in a liquid xenon detector","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.15991","snapshot_observed_at":"2026-08-06T22:10:23.831517Z","title":"Gallacheret al., (2025), arXiv:2502.15991 [physics.ins-det]","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:23.831517Z"},"links":{"cited_paper":"/paper/2502.15991","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:083c8bca35ec3a6bea071421a814707d030353c3219f1821c94ba6437c598967","observation_id":"ff7473ab-844f-47e3-b635-d79a43acadf4","resolution":{"observed_at":"2026-08-06T22:10:23.831517Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1007.1727","last_updated":"2013-06-24T14:20:41Z","snapshot_observed_at":"2026-08-13T20:03:05.337756Z","submitted_at":"2010-07-10T15:48:35Z","title":"Asymptotic formulae for likelihood-based tests of new physics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1007.1727","snapshot_observed_at":"2026-08-06T22:10:23.900778Z","title":"Cowan, K","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:23.900778Z"},"links":{"cited_paper":"/paper/1007.1727","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:ce52714addc608cf0a03b10f90ee79220d7e812d25fac32686a0a5a253bd7507","observation_id":"756ed8db-366a-4db5-a1cb-9e5a32e9e1ab","resolution":{"observed_at":"2026-08-06T22:10:23.900778Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.08796","last_updated":"2020-11-17T18:29:31Z","snapshot_observed_at":"2026-08-21T20:27:47.432986Z","submitted_at":"2020-07-17T07:39:46Z","title":"Projected WIMP Sensitivity of the XENONnT Dark Matter Experiment","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.08796","snapshot_observed_at":"2026-08-06T22:10:23.974632Z","title":"Aprileet al.(XENON), (2020), arXiv:2007.08796 [physics.ins-det]","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:23.974632Z"},"links":{"cited_paper":"/paper/2007.08796","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:27847b3a88e7870ef095efca37e5834677ba753767db0b156ca83291968096ce","observation_id":"3b3c8451-2b47-4040-b6ca-95c97b6a2dc8","resolution":{"observed_at":"2026-08-06T22:10:23.974632Z","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":"2026-08-06T22:10:24.104515Z","title":"Kib´ ediet al., Nucl","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:24.104515Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:b22d244c96f4a91469c894104282512ba94856cb6e0c7e4be75026589b672d7e","observation_id":"69886553-0220-42d5-aea5-6764f72fafe6","resolution":{"observed_at":"2026-08-06T22:10:24.104515Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.06835","last_updated":"2016-04-16T04:50:59Z","snapshot_observed_at":"2026-08-14T22:17:31.087475Z","submitted_at":"2015-12-21T20:55:30Z","title":"Cosmogenic Backgrounds to 0{\\nu}{\\beta}{\\beta} in EXO-200","version":2},"cited_work":{"arxiv_id":"1512.06835","doi":null,"metadata_source":"pith","pith_arxiv_id":"1512.06835","snapshot_observed_at":"2026-08-06T22:10:30.321757Z","title":"Cosmogenic Backgrounds to 0{\\nu}{\\beta}{\\beta} in EXO-200","venue":"nucl-ex","work_id":"879cdbfc-4196-44f1-8131-55d2569405d6","year":2015},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:24.213744Z"},"links":{"cited_paper":"/paper/1512.06835","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:f673cd378a77dabeab38bc67a77ccaa0f3ae07f272abd0af5f2f534234b1e288","observation_id":"b7680730-6f8f-4dab-92a9-708ec7e784da","resolution":{"observed_at":"2026-08-06T22:10:30.439534Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1704.05042","last_updated":"2017-11-06T16:38:02Z","snapshot_observed_at":"2026-08-15T11:16:06.653481Z","submitted_at":"2017-04-17T17:35:50Z","title":"Searches for Double Beta Decay of $^{134}$Xe with EXO-200","version":2},"cited_work":{"arxiv_id":"1704.05042","doi":null,"metadata_source":"pith","pith_arxiv_id":"1704.05042","snapshot_observed_at":"2026-08-06T22:10:30.149142Z","title":"Searches for Double Beta Decay of $^{134}$Xe with EXO-200","venue":"hep-ex","work_id":"e0e1ed10-a9ce-45a7-8bd1-eb7d7ef70931","year":2017},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:24.300806Z"},"links":{"cited_paper":"/paper/1704.05042","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:da6792e9e6c8fdab4b7a0613f008b9e5e376a9442d3afb56351e077598844eaf","observation_id":"1b22ae78-a681-4e88-963d-8d1577d24f8f","resolution":{"observed_at":"2026-08-06T22:10:30.221147Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-08-06T22:10:24.387027Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:24.387027Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:d277b3193ac749c10042844410b94aff3bc09de8b714c5396ce7484eb578fa24","observation_id":"643b991d-1b8e-496f-96ec-262979196663","resolution":{"observed_at":"2026-08-06T22:10:24.387027Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.14636","last_updated":"2023-07-27T05:56:32Z","snapshot_observed_at":"2026-08-16T15:12:56.329924Z","submitted_at":"2023-07-27T05:56:32Z","title":"Final results of Borexino on CNO solar neutrinos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.14636","snapshot_observed_at":"2026-08-06T22:10:24.505271Z","title":"Basilicoet al.(BOREXINO), Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:24.505271Z"},"links":{"cited_paper":"/paper/2307.14636","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:80277e99689b6673059a45d9eccfbe348fba54bdd84f4b23561e0be53b9da0f6","observation_id":"2a141e19-4f9b-4a9d-872a-bff7be9c0a21","resolution":{"observed_at":"2026-08-06T22:10:24.505271Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T22:10:36.537622Z","title":"Agostiniet al.(BOREXINO), Nature562, 505 (2018)","venue":null,"work_id":"537c186e-a96f-43cf-bfa1-2e396febafbe","year":2018},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:24.555938Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:40e283b45346e4f6de0dc0e4842b970adda8834493d881d2c4fd8f7d5cde6e72","observation_id":"820b777b-6e51-48d2-84a6-aadc6aba1d4c","resolution":{"observed_at":"2026-08-06T22:10:36.628874Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"nucl-ex/0512025","last_updated":"2006-03-20T18:45:08Z","snapshot_observed_at":"2026-08-03T06:27:19.283750Z","submitted_at":"2005-12-20T04:12:57Z","title":"The (t,3He) and (3He,t) reactions as probes of Gamow-Teller strength","version":2},"cited_work":{"arxiv_id":"nucl-ex/0512025","doi":null,"metadata_source":"pith","pith_arxiv_id":"nucl-ex/0512025","snapshot_observed_at":"2026-08-06T22:10:30.004911Z","title":"The (t,3He) and (3He,t) reactions as probes of Gamow-Teller strength","venue":"nucl-ex","work_id":"783984c2-7db4-4948-98aa-2e80b17b0456","year":2005},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:24.608014Z"},"links":{"cited_paper":"/paper/nucl-ex/0512025","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:b93d6a225bd43ba5dd7f1e95f4acee80fd06256aa923d6160048724b1f6cad23","observation_id":"fbe11e64-7003-4014-a876-86a4e52c8f16","resolution":{"observed_at":"2026-08-06T22:10:30.062823Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1503.08095","last_updated":"2015-03-27T14:47:24Z","snapshot_observed_at":"2026-08-14T22:54:39.802662Z","submitted_at":"2015-03-27T14:47:24Z","title":"Neutrino-nucleus reactions and their role for supernova dynamics and nucleosynthesis","version":1},"cited_work":{"arxiv_id":"1503.08095","doi":null,"metadata_source":"pith","pith_arxiv_id":"1503.08095","snapshot_observed_at":"2026-08-06T22:10:29.868573Z","title":"Neutrino-nucleus reactions and their role for supernova dynamics and nucleosynthesis","venue":"nucl-th","work_id":"5630afb5-e192-4aab-b05b-08bf10ab5087","year":2015},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:24.689864Z"},"links":{"cited_paper":"/paper/1503.08095","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:3a993617de614a735a4fc9531a3d4cf1dced07525ca5c830ba5fb3284803f06f","observation_id":"3fc48bc1-7535-4434-8ec7-49b5f017ae05","resolution":{"observed_at":"2026-08-06T22:10:29.934220Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-08-06T22:10:36.326687Z","title":"Ejiri, J","venue":null,"work_id":"ea89dcd1-c6f5-437d-b421-23addecd3988","year":2019},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:24.740822Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:dbc778b9698b9a2237797a61b173b63f48ed03003864a675038b7c322a310239","observation_id":"0b5df3cd-6404-4aea-954c-9c9d59897436","resolution":{"observed_at":"2026-08-06T22:10:36.430317Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-08-06T22:10:36.143335Z","title":"Puppeet al., Phys","venue":null,"work_id":"d9c33764-38ad-4e24-b536-4033fb547873","year":2011},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:24.791700Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:07a1de8e914bd74eebd86cd986d546168142765670303ad49874733609afc2c5","observation_id":"9d7cd1e4-d231-4011-8a09-eaf7b5732e6b","resolution":{"observed_at":"2026-08-06T22:10:36.239236Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-08-06T22:10:24.846476Z","title":"Aprileet al.(XENON), Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:24.846476Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:885eeb9843d9d21bfdaf3d71beb05fab74fd9785de6458a8374c322c6bca8e45","observation_id":"a1c02c4f-222f-4c7e-b408-67d3cc945e41","resolution":{"observed_at":"2026-08-06T22:10:24.846476Z","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":"2026-08-06T22:10:24.898994Z","title":"Boet al.(PandaX), Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:24.898994Z"},"links":{"cited_paper":"/paper/2407.10892","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:386aa92ada609bc596cd0fc72d6482cace37290526d81816976f5f2fcd3bfd27","observation_id":"8ad153ee-5c4b-4200-b9dd-2ec4224cc2fb","resolution":{"observed_at":"2026-08-06T22:10:24.898994Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.07045","last_updated":"2024-07-02T13:42:23Z","snapshot_observed_at":"2026-08-16T14:27:46.372767Z","submitted_at":"2024-01-13T11:16:53Z","title":"Measurement of Solar $pp$ Neutrino Flux using Electron Recoil Data from PandaX-4T Commissioning Run","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.07045","snapshot_observed_at":"2026-08-06T22:10:24.965206Z","title":"Luet al.(PandaX), Chin","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:24.965206Z"},"links":{"cited_paper":"/paper/2401.07045","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:36841d67c82bdb757cb84fb7a5e0c1f37168f85dd497aa9767c227d4779b5028","observation_id":"9d9459c5-e27f-4aed-b518-2ab4cbc6dc43","resolution":{"observed_at":"2026-08-06T22:10:24.965206Z","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":"2026-08-06T22:10:25.033936Z","title":"Aalberset al.(XLZD), (2024), arXiv:2410.17137 [hep- ex]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:25.033936Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:0e6d5dd9c1ef0bc56365cb6c77c26bfed83e377213728171807a698fc53c34b9","observation_id":"b61e825f-32e6-483c-8690-ecfb14b9d902","resolution":{"observed_at":"2026-08-06T22:10:25.033936Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.07169","last_updated":"2019-02-16T17:01:20Z","snapshot_observed_at":"2026-08-14T18:50:16.884848Z","submitted_at":"2018-07-18T22:03:25Z","title":"CNO Solar Neutrinos in Next-Generation Dark Matter Experiments","version":2},"cited_work":{"arxiv_id":"1807.07169","doi":null,"metadata_source":"pith","pith_arxiv_id":"1807.07169","snapshot_observed_at":"2026-08-06T22:10:29.544045Z","title":"CNO Solar Neutrinos in Next-Generation Dark Matter Experiments","venue":"astro-ph.SR","work_id":"7f2b077d-cc50-45af-9be3-af3f7782cd2d","year":2018},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:25.102244Z"},"links":{"cited_paper":"/paper/1807.07169","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:fcaab71cdacff6dbac6ec5736e37b4633bbab748a3998610027d79ece7114656","observation_id":"0fae270b-396e-495d-b3ab-bfe2ba5d554a","resolution":{"observed_at":"2026-08-06T22:10:29.616003Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-08-06T22:10:35.995300Z","title":"Barlow, Nucl","venue":null,"work_id":"2e67652f-9f45-4c1b-8c65-3842c863cb35","year":1990},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:25.162710Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:063ad5c00e24a16618ffcc4a08b6d7bd0449c221b0152e9cd185e2e4e49709ba","observation_id":"d7136955-7144-4ea0-ae54-02d8f2ab7872","resolution":{"observed_at":"2026-08-06T22:10:36.058783Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.15115","last_updated":"2021-07-22T12:40:17Z","snapshot_observed_at":"2026-08-15T22:24:25.312674Z","submitted_at":"2020-06-26T17:21:23Z","title":"Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.15115","snapshot_observed_at":"2026-08-06T22:10:25.231157Z","title":"Agostiniet al.(BOREXINO), Nature587, 577 (2020), arXiv:2006.15115 [hep-ex]","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:25.231157Z"},"links":{"cited_paper":"/paper/2006.15115","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:703d914f149bc3fba5de662b9fd6ce89e091b6674c39811f50f82e167448595a","observation_id":"62a59e76-3519-4e2b-a302-2cf60ccaf164","resolution":{"observed_at":"2026-08-06T22:10:25.231157Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T22:10:35.796761Z","title":"Pereira and others","venue":null,"work_id":"9ccabc2e-73f2-4113-b8d1-c138b5ce5e39","year":2023},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:25.296925Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:0609e9113885fbac748a535883892ad2176baf0293528eff6e60adc3fb0af239","observation_id":"deb291d9-de07-4e32-af0d-3212ec6f2cdc","resolution":{"observed_at":"2026-08-06T22:10:35.883720Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1405.6190","last_updated":"2015-10-01T02:26:25Z","snapshot_observed_at":"2026-08-14T23:32:54.273574Z","submitted_at":"2014-05-23T19:41:05Z","title":"7Be Solar Neutrino Measurement with KamLAND","version":2},"cited_work":{"arxiv_id":"1405.6190","doi":null,"metadata_source":"pith","pith_arxiv_id":"1405.6190","snapshot_observed_at":"2026-08-06T22:10:29.354811Z","title":"7Be Solar Neutrino Measurement with KamLAND","venue":"hep-ex","work_id":"b61ee4ab-ddd3-491f-bbe6-54953b2715ef","year":2014},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:25.378192Z"},"links":{"cited_paper":"/paper/1405.6190","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:d5d422113426ed6053fb2e79d3ac7602e0680a176a591f56b6a4af09982a896a","observation_id":"234013ed-0e78-4262-9366-be3fe8fe679f","resolution":{"observed_at":"2026-08-06T22:10:29.435521Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-08-06T22:10:35.591846Z","title":"Grevesse and A","venue":null,"work_id":"2247eff9-5a20-45f3-960d-9479ebbe9957","year":1998},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:25.435815Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:5bb6509990573146542bb886095043aab416a0cfb90a0d77011cbb3c4fcb6ba4","observation_id":"468daf7a-2452-4376-b774-6af9c0b3ced2","resolution":{"observed_at":"2026-08-06T22:10:35.688555Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-08-06T22:10:35.393066Z","title":"Grevesse, M","venue":null,"work_id":"75dbbf14-a594-461f-98eb-e6f1818f71c5","year":2010},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:25.483653Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:68743904ae08ce34524990db21b42a152f987840c8d830567ad142c4af21c78f","observation_id":"b050f51a-9251-492d-b4a4-b0334054e8a0","resolution":{"observed_at":"2026-08-06T22:10:35.483585Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-08-06T22:10:35.231020Z","title":"Sukhoruchkin and Z","venue":null,"work_id":"6b01af4d-d1bc-4398-94d6-25eff30108bb","year":2009},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:25.567277Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:a87d205af1de25792e3fbf5b52646b8ca5b949f7ed81e9763b8fd2f3e1dd0be4","observation_id":"b323fd55-ba14-4f1e-a39a-18d782d92361","resolution":{"observed_at":"2026-08-06T22:10:35.311938Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-08-06T22:10:35.031638Z","title":"Liet al., Chinese Physics C45, 074104 (2021)","venue":null,"work_id":"c258826f-8566-4072-9b89-e18f352130da","year":2021},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:25.639254Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:b846ba6395f60347863305cd634639ddfbf2ea1cac04bb4651a7883e684c2189","observation_id":"30fdaa45-027c-4d32-81d9-432ac499d945","resolution":{"observed_at":"2026-08-06T22:10:35.110930Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-08-06T22:10:34.806483Z","title":"Zhanget al., Chinese Physics C45, 074107 (2021)","venue":null,"work_id":"d853a50f-9897-4d97-86f0-73b7351d68bd","year":2021},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:25.698647Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:1bd487ca46946a8282ca4e5af977fbaffe125bbdeb8b95c5461433cd2b7b4da4","observation_id":"dc15bb77-3109-4175-ad74-9cf71db1790c","resolution":{"observed_at":"2026-08-06T22:10:34.890652Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1408.2745","last_updated":"2015-06-02T18:25:55Z","snapshot_observed_at":"2026-08-19T11:05:49.669808Z","submitted_at":"2014-08-12T15:29:26Z","title":"Search for physics beyond the standard model in final states with a lepton and missing transverse energy in proton-proton collisions at sqrt(s) = 8 TeV","version":2},"cited_work":{"arxiv_id":"1408.2745","doi":null,"metadata_source":"pith","pith_arxiv_id":"1408.2745","snapshot_observed_at":"2026-08-06T22:10:29.214275Z","title":"Search for physics beyond the standard model in final states with a lepton and missing transverse energy in proton-proton collisions at sqrt(s) = 8 TeV","venue":"hep-ex","work_id":"781ace78-eaf9-4353-8e8c-7be2013b2297","year":2014},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:25.820360Z"},"links":{"cited_paper":"/paper/1408.2745","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:d3b8ed2df09ef54256cf825d7137bb508811da8669b91ac2e3c0ceafd47e7d07","observation_id":"faaf6bd8-5022-4016-b136-f3e3d67e8d01","resolution":{"observed_at":"2026-08-06T22:10:29.279369Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-08-06T22:10:26.002130Z","title":"Ma, (2024), arXiv:2404.06419 [hep-ph]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:26.002130Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:4e42306bd004ac903a1b55e1c07eae390599405a45e9ee36086ecca78f7c30da","observation_id":"9b356719-4481-461a-8ec1-27551ca9ec55","resolution":{"observed_at":"2026-08-06T22:10:26.002130Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.02266","last_updated":"2021-11-03T14:59:10Z","snapshot_observed_at":"2026-08-18T21:23:51.039122Z","submitted_at":"2021-11-03T14:59:10Z","title":"Search for physics beyond the standard model in final states with two or three soft leptons and missing transverse momentum in proton-proton collisions at $\\sqrt{s} = 13~\\text{TeV}$","version":1},"cited_work":{"arxiv_id":"2111.02266","doi":null,"metadata_source":"pith","pith_arxiv_id":"2111.02266","snapshot_observed_at":"2026-08-06T22:10:28.926840Z","title":"Search for physics beyond the standard model in final states with two or three soft leptons and missing transverse momentum in proton-proton collisions at $\\sqrt{s} = 13~\\text{TeV}$","venue":"hep-ex","work_id":"87a36bc4-c2ae-4d2b-899e-cc3afa75e6b4","year":2021},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:26.152272Z"},"links":{"cited_paper":"/paper/2111.02266","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:7a49c468068217e07d0c89e462995a2a3bc0b5558bb76cc8f11c9803cd7270d1","observation_id":"8e648fa0-ba51-44fa-8254-d5278bdc4d22","resolution":{"observed_at":"2026-08-06T22:10:29.008032Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.05609","last_updated":"2019-09-24T02:05:02Z","snapshot_observed_at":"2026-08-20T00:04:20.585156Z","submitted_at":"2019-06-13T11:41:01Z","title":"Search for a heavy charged boson in events with a charged lepton and missing transverse momentum from $pp$ collisions at $\\sqrt{s} = 13$ TeV with the ATLAS detector","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.05609","snapshot_observed_at":"2026-08-06T22:10:26.307718Z","title":"Aadet al.(ATLAS), Phys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:26.307718Z"},"links":{"cited_paper":"/paper/1906.05609","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:d541197414e7299ee68fc1db3fcacd8e7cde5c2a50f1315af7d635f200feafdf","observation_id":"b69734f7-49d7-4bb1-86da-ed55d04d4529","resolution":{"observed_at":"2026-08-06T22:10:26.307718Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1309.4091","last_updated":"2013-12-11T22:08:21Z","snapshot_observed_at":"2026-08-18T20:02:25.625555Z","submitted_at":"2013-09-16T20:00:01Z","title":"Constraining Light Dark Matter with Diffuse X-Ray and Gamma-Ray Observations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1309.4091","snapshot_observed_at":"2026-08-06T22:10:26.481359Z","title":"Essiget al., JHEP11, 193 (2013), arXiv:1309.4091 [hep-ph]","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:26.481359Z"},"links":{"cited_paper":"/paper/1309.4091","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:f5f7f6879be59fff51f6333c506e48373f7a909bfca9fc21c1dcece8fe41a6a4","observation_id":"55439c90-d041-415b-b352-135dfca410fa","resolution":{"observed_at":"2026-08-06T22:10:26.481359Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.19594","last_updated":"2024-03-07T20:19:04Z","snapshot_observed_at":"2026-08-16T15:28:03.713906Z","submitted_at":"2023-05-31T06:33:37Z","title":"Measurement of the Electron-Neutrino Charged-Current Cross Sections on ${}^{127}$I with the COHERENT NaI$\\nu$E detector","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.19594","snapshot_observed_at":"2026-08-06T22:10:26.661040Z","title":"Anet al.(COHERENT), Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:26.661040Z"},"links":{"cited_paper":"/paper/2305.19594","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:3bdc6e901feb8adabaeafc3aa55bafa9207bd00f2b2a6ee51449784633c9bec3","observation_id":"f3f30ed6-2e6a-4644-8055-47d9bb4ffafd","resolution":{"observed_at":"2026-08-06T22:10:26.661040Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.01537","last_updated":"2021-12-21T15:11:35Z","snapshot_observed_at":"2026-08-16T17:51:59.936426Z","submitted_at":"2021-10-04T16:12:49Z","title":"Kiloton-scale xenon detectors for neutrinoless double beta decay and other new physics searches","version":2},"cited_work":{"arxiv_id":"2110.01537","doi":null,"metadata_source":"pith","pith_arxiv_id":"2110.01537","snapshot_observed_at":"2026-08-06T22:10:28.741527Z","title":"Kiloton-scale xenon detectors for neutrinoless double beta decay and other new physics searches","venue":"physics.ins-det","work_id":"90c00ef0-436a-4f1a-9d1b-1e6ad7a8ae6b","year":2021},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:26.820372Z"},"links":{"cited_paper":"/paper/2110.01537","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:57ec849c0957513d78e86e42a10dd54d5bb8602e304f448d4d572401b028cb12","observation_id":"35b08c5f-7f16-4dd0-8beb-8ec45aaea754","resolution":{"observed_at":"2026-08-06T22:10:28.802314Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2402.03596","last_updated":"2024-12-06T11:53:22Z","snapshot_observed_at":"2026-08-21T12:00:03.628570Z","submitted_at":"2024-02-06T00:12:06Z","title":"PandaX-xT: a Multi-ten-tonne Liquid Xenon Observatory at the China Jinping Underground Laboratory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.03596","snapshot_observed_at":"2026-08-06T22:10:26.990447Z","title":"Abdukerimet al.(PandaX-xT), Sci","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:26.990447Z"},"links":{"cited_paper":"/paper/2402.03596","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:435e8bfb7eadd528949849140950bb12668c9c535f3af4cb039bfb9b0eb625e3","observation_id":"c0cd2397-eb84-488e-be06-753797ddf4eb","resolution":{"observed_at":"2026-08-06T22:10:26.990447Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.14354","last_updated":"2022-07-11T22:36:04Z","snapshot_observed_at":"2026-08-16T17:11:29.148474Z","submitted_at":"2022-03-27T17:32:25Z","title":"GPU-based optical simulation of the DARWIN detector","version":2},"cited_work":{"arxiv_id":"2203.14354","doi":null,"metadata_source":"pith","pith_arxiv_id":"2203.14354","snapshot_observed_at":"2026-08-06T22:10:28.473981Z","title":"GPU-based optical simulation of the DARWIN detector","venue":"physics.ins-det","work_id":"afc3dbb8-12f1-4270-abaa-756d5d51fad1","year":2022},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:27.106416Z"},"links":{"cited_paper":"/paper/2203.14354","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:fb2172489bd27f074d2eb629771c107d4d6ee3300a7eaab6870105f3e7e52929","observation_id":"31a673a3-475d-46a9-8880-4e0cc6837715","resolution":{"observed_at":"2026-08-06T22:10:28.624911Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-08-06T22:10:34.622004Z","title":"Origin-x — origin-x.llnl.gov,","venue":null,"work_id":"148de3e7-ac4c-4d0c-b76c-c5492881849c","year":2025},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:27.260214Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:26a4b7de14643cb24e2c922f4f95832101ca0a83e4f409aced5503abfa75e902","observation_id":"b1d3a925-1723-47e9-8c09-f31211d51f5a","resolution":{"observed_at":"2026-08-06T22:10:34.712327Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.19050","last_updated":"2024-04-29T18:41:21Z","snapshot_observed_at":"2026-08-18T18:02:59.777062Z","submitted_at":"2024-04-29T18:41:21Z","title":"Report from the Workshop on Xenon Detector $0\\nu\\beta\\beta$ Searches: Steps Towards the Kilotonne Scale","version":1},"cited_work":{"arxiv_id":"2404.19050","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.19050","snapshot_observed_at":"2026-08-06T22:10:28.150747Z","title":"Report from the Workshop on Xenon Detector $0\\nu\\beta\\beta$ Searches: Steps Towards the Kilotonne Scale","venue":"nucl-ex","work_id":"e0cd7119-e316-4e34-b01b-d03f7c6495f7","year":2024},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:27.380668Z"},"links":{"cited_paper":"/paper/2404.19050","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:bd13605024714ea692a84b59e4f63db84a4c9e42f8602326a8c6dda2e7099f86","observation_id":"3beabd4f-c8f0-4499-9e83-357a4693161d","resolution":{"observed_at":"2026-08-06T22:10:28.283585Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1807.03817","last_updated":"2018-07-10T18:33:06Z","snapshot_observed_at":"2026-08-15T23:13:35.528306Z","submitted_at":"2018-07-10T18:33:06Z","title":"Interplay of the LHC and non-LHC Dark Matter searches in the Effective Field Theory approach","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.03817","snapshot_observed_at":"2026-08-06T22:10:27.481456Z","title":"Belyaevet al., Phys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:27.481456Z"},"links":{"cited_paper":"/paper/1807.03817","citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:3f0674e3caa7ba108b3c40c406959d0b38348858bd7c1439e93cedc2e68b3405","observation_id":"c90536bf-2d9e-46ed-91bc-cc265cf208c1","resolution":{"observed_at":"2026-08-06T22:10:27.481456Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T22:10:34.461662Z","title":null,"venue":null,"work_id":"51c35abc-d81d-4b4a-bc62-0b2c5297a742","year":1990},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:27.622657Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:d97dde776891271bead135d76c7d88fb89a79b007e5d88cbcbe91180500ab4ec","observation_id":"bba34c07-d782-4e8b-82c1-42c826999909","resolution":{"observed_at":"2026-08-06T22:10:34.539024Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-08-06T22:10:24.453422Z","title":"817, Data extracted using the NNDC On-Line Data Service from the ENSDF database, file revised as of Nov","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter","version":1},"reference_index":1992,"source":"pdf_text","source_observed_at":"2026-08-06T22:10:24.453422Z"},"links":{"citing_paper":"/paper/2506.22586"},"observation_digest":"sha256:3bdd5c904e72b18879eedd9c2d74a1a3f6e8ac7cded4a9792755ee8befeb47da","observation_id":"31fbfe5a-004a-4939-8baa-2afffd2d10f5","resolution":{"observed_at":"2026-08-06T22:10:24.453422Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2506.22586","last_updated":"2025-06-27T19:07:45Z","latest_version":1,"primary_category":"nucl-ex","snapshot_observed_at":"2026-08-17T02:46:27.759589Z","submitted_at":"2025-06-27T19:07:45Z","title":"Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter"},"reference_resolution":{"displayed":98,"state_counts":{"malformed_identifier":0,"metadata_mismatch":11,"parse_uncertain":0,"unresolved":57,"verified_exact":19,"verified_fuzzy":11},"total_outbound_references":98},"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":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"thesis":"As of 23 August 2026, this Paper Citation Record lists 98 of 98 outbound references and 2 inbound Pith citation observations for arXiv:2506.22586."}