{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:A2TAAQKZC2S5ISCLCUYKXD6DYS","short_pith_number":"pith:A2TAAQKZ","schema_version":"1.0","canonical_sha256":"06a600415916a5d4484b1530ab8fc3c4858f7f7a64837f046cefe2a52432451a","source":{"kind":"arxiv","id":"1802.06162","version":2},"attestation_state":"computed","paper":{"title":"Liquid xenon scintillation measurements and pulse shape discrimination in the LUX dark matter detector","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.ins-det","authors_text":"A. Bernstein, A. Currie, A. Dobi, A. Fan, A.J. Bailey, A. Lindote, A. Manalaysay, A.St.J. Murphy, B.G. Lenardo, B.N. Edwards, B.P. Tennyson, C. Chan, C. Ghag, C.M. Ignarra, C. Nehrkorn, C.R. Hall, C. Rhyne, C. Silva, C. Zhang, D. Byram, D.J. Taylor, D. Khaitan, D.M. Mei, D.N. McKinsey, D.P. Hogan, D.Q. Huang, D.R. Tiedt, E. Druszkiewicz, E.K. Pease, E.M. Boulton, E.P. Bernard, F.L.H. Wolfs, F. Neves, H.M. Ara\\'ujo, H.N. Nelson, J.A. Morad, J. Balajthy, J.E. Cutter, J. Genovesi, J. Liao, J. Mock, J.R. Verbus, J.T. White, J. Xu, K.C. Oliver-Mallory, K.J. Palladino, K. Kamdin, K. Kazkaz, K. O'Sullivan, K.T. Lesko, K. Yazdani, L. Tvrznikova, M.C. Carmona-Benitez, M.F. Marzioni, M.G.D. Gilchriese, M. Horn, M.I. Lopes, M. Moongweluwan, M. Solmaz, M.S. Witherell, M. Szydagis, M. Tripathi, P.A. Terman, P. Beltrame, P. Br\\'as, P. Sorensen, R.C. Webb, R.G. Jacobsen, R.J. Gaitskell, R. Knoche, R.L. Mannino, S.A. Hertel, S. Alsum, S. Fiorucci, S.J. Haselschwardt, S.K. Young, S.R. Fallon, S. Shaw, S. Uvarov, T.A. Shutt, The LUX Collaboration: D.S. Akerib, T.J.R. Davison, T.J. Sumner, T.J. Whitis, T.P. Biesiadzinski, U. Utku, V.N. Solovov, V. Velan, W.C. Taylor, W.H. To, W. Ji, X. Bai","submitted_at":"2018-02-17T00:05:33Z","abstract_excerpt":"Weakly Interacting Massive Particles (WIMPs) are a leading candidate for dark matter and are expected to produce nuclear recoil (NR) events within liquid xenon time-projection chambers. We present a measurement of the scintillation timing characteristics of liquid xenon in the LUX dark matter detector and develop a pulse shape discriminant to be used for particle identification. To accurately measure the timing characteristics, we develop a template-fitting method to reconstruct the detection times of photons. Analyzing calibration data collected during the 2013-16 LUX WIMP search, we provide "},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1802.06162","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.ins-det","submitted_at":"2018-02-17T00:05:33Z","cross_cats_sorted":[],"title_canon_sha256":"73b874d8537e6e28c603d18703a51941524d4110d10c260ca90030fc27342617","abstract_canon_sha256":"7ee6843d7364fb04fc371b0021f9b9060e454960f66e2dba68f0cd28e8fb1ef4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:12:53.203506Z","signature_b64":"8gXgFm1WvjheIL+rbYIY4qPgYTot274WCsQdAw+7DVzFXnY1cZV9W4GzFCUXQ4AKEQBSmehRHFrJjFgNytfXAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"06a600415916a5d4484b1530ab8fc3c4858f7f7a64837f046cefe2a52432451a","last_reissued_at":"2026-05-18T00:12:53.202783Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:12:53.202783Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Liquid xenon scintillation measurements and pulse shape discrimination in the LUX dark matter detector","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.ins-det","authors_text":"A. Bernstein, A. Currie, A. Dobi, A. Fan, A.J. Bailey, A. Lindote, A. Manalaysay, A.St.J. Murphy, B.G. Lenardo, B.N. Edwards, B.P. Tennyson, C. Chan, C. Ghag, C.M. Ignarra, C. Nehrkorn, C.R. Hall, C. Rhyne, C. Silva, C. Zhang, D. Byram, D.J. Taylor, D. Khaitan, D.M. Mei, D.N. McKinsey, D.P. Hogan, D.Q. Huang, D.R. Tiedt, E. Druszkiewicz, E.K. Pease, E.M. Boulton, E.P. Bernard, F.L.H. Wolfs, F. Neves, H.M. Ara\\'ujo, H.N. Nelson, J.A. Morad, J. Balajthy, J.E. Cutter, J. Genovesi, J. Liao, J. Mock, J.R. Verbus, J.T. White, J. Xu, K.C. Oliver-Mallory, K.J. Palladino, K. Kamdin, K. Kazkaz, K. O'Sullivan, K.T. Lesko, K. Yazdani, L. Tvrznikova, M.C. Carmona-Benitez, M.F. Marzioni, M.G.D. Gilchriese, M. Horn, M.I. Lopes, M. Moongweluwan, M. Solmaz, M.S. Witherell, M. Szydagis, M. Tripathi, P.A. Terman, P. Beltrame, P. Br\\'as, P. Sorensen, R.C. Webb, R.G. Jacobsen, R.J. Gaitskell, R. Knoche, R.L. Mannino, S.A. Hertel, S. Alsum, S. Fiorucci, S.J. Haselschwardt, S.K. Young, S.R. Fallon, S. Shaw, S. Uvarov, T.A. Shutt, The LUX Collaboration: D.S. Akerib, T.J.R. Davison, T.J. Sumner, T.J. Whitis, T.P. Biesiadzinski, U. Utku, V.N. Solovov, V. Velan, W.C. Taylor, W.H. To, W. Ji, X. Bai","submitted_at":"2018-02-17T00:05:33Z","abstract_excerpt":"Weakly Interacting Massive Particles (WIMPs) are a leading candidate for dark matter and are expected to produce nuclear recoil (NR) events within liquid xenon time-projection chambers. We present a measurement of the scintillation timing characteristics of liquid xenon in the LUX dark matter detector and develop a pulse shape discriminant to be used for particle identification. To accurately measure the timing characteristics, we develop a template-fitting method to reconstruct the detection times of photons. Analyzing calibration data collected during the 2013-16 LUX WIMP search, we provide "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1802.06162","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1802.06162","created_at":"2026-05-18T00:12:53.202904+00:00"},{"alias_kind":"arxiv_version","alias_value":"1802.06162v2","created_at":"2026-05-18T00:12:53.202904+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1802.06162","created_at":"2026-05-18T00:12:53.202904+00:00"},{"alias_kind":"pith_short_12","alias_value":"A2TAAQKZC2S5","created_at":"2026-05-18T12:32:13.499390+00:00"},{"alias_kind":"pith_short_16","alias_value":"A2TAAQKZC2S5ISCL","created_at":"2026-05-18T12:32:13.499390+00:00"},{"alias_kind":"pith_short_8","alias_value":"A2TAAQKZ","created_at":"2026-05-18T12:32:13.499390+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/A2TAAQKZC2S5ISCLCUYKXD6DYS","json":"https://pith.science/pith/A2TAAQKZC2S5ISCLCUYKXD6DYS.json","graph_json":"https://pith.science/api/pith-number/A2TAAQKZC2S5ISCLCUYKXD6DYS/graph.json","events_json":"https://pith.science/api/pith-number/A2TAAQKZC2S5ISCLCUYKXD6DYS/events.json","paper":"https://pith.science/paper/A2TAAQKZ"},"agent_actions":{"view_html":"https://pith.science/pith/A2TAAQKZC2S5ISCLCUYKXD6DYS","download_json":"https://pith.science/pith/A2TAAQKZC2S5ISCLCUYKXD6DYS.json","view_paper":"https://pith.science/paper/A2TAAQKZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1802.06162&json=true","fetch_graph":"https://pith.science/api/pith-number/A2TAAQKZC2S5ISCLCUYKXD6DYS/graph.json","fetch_events":"https://pith.science/api/pith-number/A2TAAQKZC2S5ISCLCUYKXD6DYS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/A2TAAQKZC2S5ISCLCUYKXD6DYS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/A2TAAQKZC2S5ISCLCUYKXD6DYS/action/storage_attestation","attest_author":"https://pith.science/pith/A2TAAQKZC2S5ISCLCUYKXD6DYS/action/author_attestation","sign_citation":"https://pith.science/pith/A2TAAQKZC2S5ISCLCUYKXD6DYS/action/citation_signature","submit_replication":"https://pith.science/pith/A2TAAQKZC2S5ISCLCUYKXD6DYS/action/replication_record"}},"created_at":"2026-05-18T00:12:53.202904+00:00","updated_at":"2026-05-18T00:12:53.202904+00:00"}