{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:EANAOLAD5IBIPJ4V2ORGFKND2H","short_pith_number":"pith:EANAOLAD","schema_version":"1.0","canonical_sha256":"201a072c03ea0287a795d3a262a9a3d1c7f52f8ab7c199cf777e79e4358bb691","source":{"kind":"arxiv","id":"1712.05696","version":1},"attestation_state":"computed","paper":{"title":"Calibration, event reconstruction, data analysis and limits calculation for the LUX dark matter experiment","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. H. Faham, C. Lee, 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, D. S. Akerib, 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. E. Y. Dobson, J. Genovesi, 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. Reichhart, L. Tvrznikova, M. C. Carmona-Benitez, M. F. Marzioni, M. G. D. Gilchriese, M. Hanhardt, M. Horn, M. I. Lopes, M. Moongweluwan, M. Solmaz, M. S. Witherell, M. Szydagis, M. Tripathi, N. A. Larsen, 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. B. Cahn, S. Fiorucci, S. J. Haselschwardt, S. K. Young, S. R. Fallon, S. Shaw, S. Uvarov, T. A. Shutt, T. J. R. Davison, T. J. Sumner, T. J. Whitis, T. P. Biesiadzinski, V. M. Gehman, V. N. Solovov, V. Velan, W. C. Taylor, W. H. To, W. Ji, X. Bai","submitted_at":"2017-12-15T15:03:32Z","abstract_excerpt":"The LUX experiment has performed searches for dark matter particles scattering elastically on xenon nuclei, leading to stringent upper limits on the nuclear scattering cross sections for dark matter. Here, for results derived from ${1.4}\\times 10^{4}\\;\\mathrm{kg\\,days}$ of target exposure in 2013, details of the calibration, event-reconstruction, modeling, and statistical tests that underlie the results are presented. Detector performance is characterized, including measured efficiencies, stability of response, position resolution, and discrimination between electron- and nuclear-recoil popula"},"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":"1712.05696","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.ins-det","submitted_at":"2017-12-15T15:03:32Z","cross_cats_sorted":[],"title_canon_sha256":"0aff033af3dbfda439cda8687c3fac1912faf4d58f75cf6bf46baa4134f8c44e","abstract_canon_sha256":"538cc85bb8de73c902afc1761f85a93fc94741b7082f380216c61c835595f6a9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:14:10.910013Z","signature_b64":"eSy7U6fi0MAUzFIRZTJn8+TlzPxhFKaT34HUM49osrwc1Lh+TdFbU2vg+20Q4wVVxOjDMfs/PoymMhbK/aC7Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"201a072c03ea0287a795d3a262a9a3d1c7f52f8ab7c199cf777e79e4358bb691","last_reissued_at":"2026-05-18T00:14:10.909434Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:14:10.909434Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Calibration, event reconstruction, data analysis and limits calculation for the LUX dark matter experiment","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. H. Faham, C. Lee, 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, D. S. Akerib, 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. E. Y. Dobson, J. Genovesi, 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. Reichhart, L. Tvrznikova, M. C. Carmona-Benitez, M. F. Marzioni, M. G. D. Gilchriese, M. Hanhardt, M. Horn, M. I. Lopes, M. Moongweluwan, M. Solmaz, M. S. Witherell, M. Szydagis, M. Tripathi, N. A. Larsen, 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. B. Cahn, S. Fiorucci, S. J. Haselschwardt, S. K. Young, S. R. Fallon, S. Shaw, S. Uvarov, T. A. Shutt, T. J. R. Davison, T. J. Sumner, T. J. Whitis, T. P. Biesiadzinski, V. M. Gehman, V. N. Solovov, V. Velan, W. C. Taylor, W. H. To, W. Ji, X. Bai","submitted_at":"2017-12-15T15:03:32Z","abstract_excerpt":"The LUX experiment has performed searches for dark matter particles scattering elastically on xenon nuclei, leading to stringent upper limits on the nuclear scattering cross sections for dark matter. Here, for results derived from ${1.4}\\times 10^{4}\\;\\mathrm{kg\\,days}$ of target exposure in 2013, details of the calibration, event-reconstruction, modeling, and statistical tests that underlie the results are presented. Detector performance is characterized, including measured efficiencies, stability of response, position resolution, and discrimination between electron- and nuclear-recoil popula"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1712.05696","kind":"arxiv","version":1},"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":"1712.05696","created_at":"2026-05-18T00:14:10.909533+00:00"},{"alias_kind":"arxiv_version","alias_value":"1712.05696v1","created_at":"2026-05-18T00:14:10.909533+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1712.05696","created_at":"2026-05-18T00:14:10.909533+00:00"},{"alias_kind":"pith_short_12","alias_value":"EANAOLAD5IBI","created_at":"2026-05-18T12:31:12.930513+00:00"},{"alias_kind":"pith_short_16","alias_value":"EANAOLAD5IBIPJ4V","created_at":"2026-05-18T12:31:12.930513+00:00"},{"alias_kind":"pith_short_8","alias_value":"EANAOLAD","created_at":"2026-05-18T12:31:12.930513+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/EANAOLAD5IBIPJ4V2ORGFKND2H","json":"https://pith.science/pith/EANAOLAD5IBIPJ4V2ORGFKND2H.json","graph_json":"https://pith.science/api/pith-number/EANAOLAD5IBIPJ4V2ORGFKND2H/graph.json","events_json":"https://pith.science/api/pith-number/EANAOLAD5IBIPJ4V2ORGFKND2H/events.json","paper":"https://pith.science/paper/EANAOLAD"},"agent_actions":{"view_html":"https://pith.science/pith/EANAOLAD5IBIPJ4V2ORGFKND2H","download_json":"https://pith.science/pith/EANAOLAD5IBIPJ4V2ORGFKND2H.json","view_paper":"https://pith.science/paper/EANAOLAD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1712.05696&json=true","fetch_graph":"https://pith.science/api/pith-number/EANAOLAD5IBIPJ4V2ORGFKND2H/graph.json","fetch_events":"https://pith.science/api/pith-number/EANAOLAD5IBIPJ4V2ORGFKND2H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EANAOLAD5IBIPJ4V2ORGFKND2H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EANAOLAD5IBIPJ4V2ORGFKND2H/action/storage_attestation","attest_author":"https://pith.science/pith/EANAOLAD5IBIPJ4V2ORGFKND2H/action/author_attestation","sign_citation":"https://pith.science/pith/EANAOLAD5IBIPJ4V2ORGFKND2H/action/citation_signature","submit_replication":"https://pith.science/pith/EANAOLAD5IBIPJ4V2ORGFKND2H/action/replication_record"}},"created_at":"2026-05-18T00:14:10.909533+00:00","updated_at":"2026-05-18T00:14:10.909533+00:00"}