Search Results - "Kamdin, K."

Results from a Search for Dark Matter in the Complete LUX Exposure by Akerib, D S, Alsum, S, Araújo, H M, Bai, X, Bailey, A J, Balajthy, J, Beltrame, P, Bernard, E P, Bernstein, A, Biesiadzinski, T P, Boulton, E M, Bramante, R, Brás, P, Byram, D, Cahn, S B, Carmona-Benitez, M C, Chan, C, Chiller, A A, Chiller, C, Currie, A, Cutter, J E, Davison, T J R, Dobi, A, Dobson, J E Y, Druszkiewicz, E, Edwards, B N, Faham, C H, Fiorucci, S, Gaitskell, R J, Gehman, V M, Ghag, C, Gibson, K R, Gilchriese, M G D, Hall, C R, Hanhardt, M, Haselschwardt, S J, Hertel, S A, Hogan, D P, Horn, M, Huang, D Q, Ignarra, C M, Ihm, M, Jacobsen, R G, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, N A, Lee, C, Lenardo, B G, Lesko, K T, Lindote, A, Lopes, M I, Manalaysay, A, Mannino, R L, Marzioni, M F, McKinsey, D N, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J A, Murphy, A St J, Nehrkorn, C, Nelson, H N, Neves, F, O'Sullivan, K, Oliver-Mallory, K C, Palladino, K J, Pease, E K, Phelps, P, Reichhart, L, Rhyne, C, Shaw, S, Shutt, T A, Silva, C, Solmaz, M, Solovov, V N, Sorensen, P, Stephenson, S, Sumner, T J, Szydagis, M, Taylor, D J, Taylor, W C, Tennyson, B P, Terman, P A, Tiedt, D R, To, W H, Tripathi, M, Tvrznikova, L, Uvarov, S, Verbus, J R, Webb, R C, White, J T, Whitis, T J, Witherell, M S, Wolfs, F L H, Xu, J, Yazdani, K, Young, S K

“…We report constraints on spin-independent weakly interacting massive particle (WIMP)-nucleon scattering using a 3.35×10^{4}  kg day exposure of the Large…”
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Results of a Search for Sub-GeV Dark Matter Using 2013 LUX Data by Akerib, D S, Alsum, S, Araújo, H M, Bai, X, Balajthy, J, Beltrame, P, Bernard, E P, Bernstein, A, Biesiadzinski, T P, Boulton, E M, Boxer, B, Brás, P, Burdin, S, Byram, D, Carmona-Benitez, M C, Chan, C, Cutter, J E, Davison, T J R, Druszkiewicz, E, Fallon, S R, Fan, A, Fiorucci, S, Gaitskell, R J, Genovesi, J, Ghag, C, Gilchriese, M G D, Gwilliam, C, Hall, C R, Haselschwardt, S J, Hertel, S A, Hogan, D P, Horn, M, Huang, D Q, Ignarra, C M, Jacobsen, R G, Jahangir, O, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Knoche, R, Korolkova, E V, Kravitz, S, Kudryavtsev, V A, Lenardo, B G, Lesko, K T, Liao, J, Lin, J, Lindote, A, Lopes, M I, Manalaysay, A, Mannino, R L, Marangou, N, Marzioni, M F, McKinsey, D N, Mei, D-M, Moongweluwan, M, Morad, J A, Murphy, A St J, Naylor, A, Nehrkorn, C, Nelson, H N, Neves, F, Oliver-Mallory, K C, Palladino, K J, Pease, E K, Riffard, Q, Rischbieter, G R C, Rhyne, C, Rossiter, P, Shaw, S, Shutt, T A, Silva, C, Solmaz, M, Solovov, V N, Sorensen, P, Sumner, T J, Szydagis, M, Taylor, D J, Taylor, W C, Tennyson, B P, Terman, P A, Tiedt, D R, To, W H, Tripathi, M, Tvrznikova, L, Utku, U, Uvarov, S, Velan, V, Webb, R C, White, J T, Whitis, T J, Witherell, M S, Wolfs, F L H, Woodward, D, Xu, J, Yazdani, K, Zhang, C

“…The scattering of dark matter (DM) particles with sub-GeV masses off nuclei is difficult to detect using liquid xenon-based DM search instruments because the…”
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The LUX-ZEPLIN (LZ) experiment by Akimov, D.Yu, Angelides, N., Araújo, H.M., Armstrong, J.E., Balashov, S., Baxter, A., Belle, J., Bhatti, A., Birrittella, B., Boulton, E.M., Branson, S., Bugaev, V.V., Campbell, J.S., Chiller, A.A., Colling, D., Coughlen, R., Curran, D., da Cunha, J.P., Dardin, S., Davison, T.J.R., de Viveiros, L., Dobson, J.E.Y., Edberg, T.K., Elnimr, M.M., Fruth, T., Gaitskell, R.J., Garcia, D., Geffre, A., Ghag, C., Gibson, E., Gilchriese, M.G.D., Hans, S., Harrison, A., Holtom, E., Ignarra, C.M., Irving, M.N., Johnson, M., Jones, W.G., Kim, W.T., Kocher, C.D., Kravitz, S.W., Kumpan, A.V., Kyre, S., Lee, H.S., Lee, C., Lenardo, B.G., Leonard, R., Lesko, K.T., Liu, Y., Liao, J., Lin, J., Linehan, R., Liu, R., Loniewski, C., Lucero, D., Lynch, C., Manenti, L., McKinsey, D.N., McLaughlin, J., Mei, D.-M., Meng, Y., Naim, D., Nehrkorn, C., Nelson, H.N., Nikkel, J.A., Nilima, A., Oliver-Mallory, K.C., Pagenkopf, D., Palmaccio, V.M., Palmer, J., Pangilinan, M., Penning, B.P., Pereira, G., Peterson, I.B., Piepke, A., Pierson, S., Powell, S., Ratcliff, B.N., Rosero, R., Rynders, D., Sarychev, M., Severson, M., Silva, C., Smith, R.J., Stephenson, S., Studley, R., Sundarnath, K., Szydagis, M., Terman, P.A., Thomas, K.J., Tiedt, D.R., Tronstad, D.R., Tull, C.E., Walcott, S., Wang, L., Wei, W.-Z., Witherell, M.S., Xiang, X., Xiao, Q., Yeh, M.

“…We describe the design and assembly of the LUX-ZEPLIN experiment, a direct detection search for cosmic WIMP dark matter particles. The centerpiece of the…”
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The LUX-ZEPLIN (LZ) radioactivity and cleanliness control programs by Alquahtani, A., Anderson, T. J., Armstrong, J. E., Bai, X., Baxter, A., Bernard, E. P., Bernstein, A., Bhatti, A., Boast, K. E., Bramante, R., Branson, S., Bugaev, V. V., Burdin, S., Cabrita, R., Carels, C., Carlsmith, D. L., Carmona-Benitez, M. C., Chan, C., Cherwinka, J. J., Chott, N. I., Curran, D., Currie, A., Dahl, C. E., Decheine, N., Dobi, A., Druszkiewicz, E., Flaecher, H., Fruth, T., Gantos, N. J., Gehman, V. M., Hasselkus, C., Hertel, S. A., Huang, D. Q., Jahangir, O., Jeffery, S. N., Johnson, J., Kamaha, A., Khaleeq, M., Khurana, I., Kim, Y. D., Korolkova, E. V., Kras, J., Kudryavtsev, V. A., Lambert, A. R., Larsen, N. A., Leason, E. A., Li, J., Liu, R., Lopes, M. I., Lyle, J. M., Lynch, C., MarrLaundrie, P., Martin, T. J., McKinsey, D. N., Mizrachi, E., Molash, D., Neves, F., Nikkel, J. A., Nilima, A., Olcina, I., Olevitch, M. A., Pagenkopf, D., Pal, S., Palladino, K. J., Pereira, C., Piepke, A., Pierson, S., Powell, S., Reichenbacher, J., Sabarots, L., Sazzad, A. B. M. R., Shutt, G. W., Silk, J. J., Silva, C., Skulski, W., Smith, A. R., Smith, R. E., Solovov, V. N., Sosnovtsev, V. V., Stancu, I., Stifter, K., Studley, R., Sutcliffe, P., Taylor, W. C., Taylor, R., Temples, D., Thomson, J. A., Tomás, A., Verbus, J. R., Vietanen, T., Walcott, S., Wang, W., Migneault, J., White, R. G., Wilson, K., Witherell, M. S., Wolfs, F. L. H., Xu, J., Yeh, M., Zarzhitsky, P.

“…LUX-ZEPLIN (LZ) is a second-generation direct dark matter experiment with spin-independent WIMP-nucleon scattering sensitivity above 1.4 × 10 - 48 cm 2 for a…”
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Current Status and Future Prospects of the SNO+ Experiment by Asahi, S., Auty, D. J., Back, A. R., Barnard, Z., Barros, N., Beier, E. W., Biller, S. D., Bonventre, R., Braid, D., Caden, E., Caravaca, J., Carvalho, J., Cavalli, L., Chauhan, D., Chkvorets, O., Clark, K., Coulter, I. T., Cressy, D., Darrach, C., Davis-Purcell, B., Depatie, M. M., Descamps, F., Dunger, J., Falk, E., Ford, R., Grullon, S., Hallman, D., Hans, S., Hartnell, J., Harvey, P., Hedayatipour, M., Heintzelman, W. J., Helmer, R. L., Hreljac, B., Hu, J., Iida, T., Jackson, C. M., Jelley, N. A., Jillings, C., Kamdin, K., Kaptanoglu, T., Kaspar, J., Keener, P., Khaghani, P., Klein, J. R., Knapik, R., Kormos, L. L., Korte, S., Labe, K., Lam, I., Land, B. J., Langrock, S., Lefeuvre, G. M., Leming, E. J., Lidgard, J., Liu, Y., Maio, A., Manecki, S., Maneira, J., Marzec, E., Mastbaum, A., McDonald, A. B., Mekarski, P., Mohan, Y., Mony, E., Mottram, M. J., Novikov, V., O’Keeffe, H. M., O’Sullivan, E., Pershing, T., Prior, G., Prouty, J. C., Quirk, S., Reichold, A., Rose, J., Schumaker, M. A., Schwendener, M. H., Seddighin, M., Segui, L., Seibert, S., Shokair, T. M., Sibley, L., Sinclair, J. R., Sörensen, A., Sonley, T., Stringer, M. I., Svoboda, R., Tatar, J., Tian, L., Tseng, J., Vázquez-Jáuregui, E., Virtue, C., von Krosigk, B., Walker, J. M. G., Waterfield, J., White, R. F., Winchester, T. J., Wright, A., Yeh, M., Zhao, T.

“…SNO+ is a large liquid scintillator-based experiment located 2 km underground at SNOLAB, Sudbury, Canada. It reuses the Sudbury Neutrino Observatory detector,…”
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Simulations of events for the LUX-ZEPLIN (LZ) dark matter experiment by Alsum, S.K., Angelides, N., Araújo, H.M., Arthurs, M., Bai, X., Balajthy, J., Balashov, S., Baxter, A., Bernard, E.P., Birch, H.J., Boast, K.E., Boxer, B., Buckley, J.H., Bugaev, V.V., Busenitz, J.K., Cabrita, R., Carels, C., Carmona-Benitez, M.C., Cole, A., Cottle, A., Cutter, J.E., Viveiros, L. de, Druszkiewicz, E., Fan, A., Fayer, S., Fruth, T., Ghag, C., Gibson, E., Gokhale, S., van der Grinten, M.G.D., Harrison, A., Hertel, S.A., Hor, J.Y-K., Huang, D.Q., Ignarra, C.M., Ji, W., Kaboth, A.C., Kazkaz, K., Kocher, C.D., Korley, L., Korolkova, E.V., Kras, J., Kraus, H., Kravitz, S., Kudryavtsev, V.A., Leason, E.A., Lee, J., Lesko, K.T., Levy, C., Li, J., Liao, J., Liao, F.-T., Lin, J., Liu, R., Loniewski, C., Lopes, M.I., Lorenzon, W., Luitz, S., Manalaysay, A., Manenti, L., McLaughlin, J., Meng, Y., Miller, E.H., Mizrachi, E., Morad, J.A., Morrison, E., Nehrkorn, C., Nilima, A., Oliver-Mallory, K.C., Parveen, N., Piepke, A., Pushkin, K., Richards, A., Rutherford, G., Sazzad, A.B.M.R., Schnee, R.W., Seymour, D., Shaw, S., Silk, J.J., Smith, R., Stancu, I., Stevens, A., Stifter, K., Swanson, N., Tan, M., Taylor, R., Temples, D.J., Tiedt, D.R., Timalsina, M., Tripathi, M., Tvrznikova, L., Vaitkus, A., Wang, J.J., Wang, W., Webb, R.C., Whitis, T.J., Woodward, D., Xiang, X., Yeh, M., Zarzhitsky, P.

“…The LUX-ZEPLIN dark matter search aims to achieve a sensitivity to the WIMP-nucleon spin-independent cross-section down to (1–2)×10−12 pb at a WIMP mass of 40 …”
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Limits on Spin-Dependent WIMP-Nucleon Cross Section Obtained from the Complete LUX Exposure by Akerib, D. S., Alsum, S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Brás, P., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chiller, A. A., Chiller, C., Currie, A., Cutter, J. E., Davison, T. J. R., Dobi, A., Dobson, J. E. Y., Druszkiewicz, E., Edwards, B. N., Faham, C. H., Fallon, S. R., Fiorucci, S., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gilchriese, M. G. D., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Jacobsen, R. G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D.-M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., O’Sullivan, K., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T. A., Silva, C., Solmaz, M., Solovov, V. N., Sorensen, P., Stephenson, S., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W. C., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Velan, V., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Xu, J., Yazdani, K., Young, S. K., Zhang, C.

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Measurement of the gamma ray background in the Davis cavern at the Sanford Underground Research Facility by Akerlof, C.W., Angelides, N., Araújo, H.M., Armstrong, J.E., Arthurs, M., Bai, X., Baxter, A., Biekert, A., Biesiadzinski, T.P., Boast, K.E., Boxer, B., Buckley, J.H., Busenitz, J.K., Carels, C., Carmona-Benitez, M.C., Chan, C., Cottle, A., Dahl, C.E., Edberg, T.K., Fiorucci, S., Flaecher, H., Gaitskell, R.J., Ghag, C., Gilchriese, M.G.D., Hall, C.R., Harrison, J., Haselschwardt, S.J., Hertel, S.A., Horn, M., Ignarra, C.M., Jahangir, O., Johnson, J., Khazov, A., Kim, W.T., Kocher, C.D., Korley, L., Korolkova, E.V., Kraus, H., Kravitz, S.W., Kreczko, L., Krikler, B., Kudryavtsev, V.A., Leason, E.A., Lee, J., Leonard, D.S., Lesko, K.T., Levy, C., Li, J., Liao, J., Liao, F.-T., Lin, J., Lindote, A., Lippincott, W.H., Liu, R., Liu, X., López Paredes, B., Lorenzon, W., Luitz, S., Majewski, P.A., Manenti, L., Marangou, N., Meng, Y., Miller, E.H., Morad, J.A., Mount, B.J., Naim, D., Nedlik, C., Nelson, H.N., Neves, F., Nilima, A., Oliver-Mallory, K.C., Palladino, K.J., Pease, E.K., Penning, B.P., Pereira, G., Pushkin, K., Reichenbacher, J., Rischbieter, G.R.C., Rossiter, P., Rutherford, G., Sazzad, A.B.M.R., Seymour, D., Shaw, S., Solmaz, M., Solovov, V.N., Sorensen, P., Stancu, I., Stevens, A., Stifter, K., Szydagis, M., Taylor, W.C., Taylor, R., Tomás, A., Tripathi, M., Tvrznikova, L., Uvarov, S., Vacheret, A., Watson, J.R., Whitis, T.J., Yin, J.

“…Deep underground environments are ideal for low background searches due to the attenuation of cosmic rays by passage through the earth. However, they are…”
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Results of a Search for Sub-GeV Dark Matter Using 2013 LUX Data by Akerib, D. S., Alsum, S., Araújo, H. M., Bai, X., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Boxer, B., Brás, P., Burdin, S., Byram, D., Carmona-Benitez, M. C., Chan, C., Cutter, J. E., Davison, T. J. R., Druszkiewicz, E., Fallon, S. R., Fan, A., Fiorucci, S., Gaitskell, R. J., Genovesi, J., Ghag, C., Gilchriese, M. G. D., Gwilliam, C., Hall, C. R., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Jacobsen, R. G., Jahangir, O., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Korolkova, E. V., Kravitz, S., Kudryavtsev, V. A., Lenardo, B. G., Lesko, K. T., Liao, J., Lin, J., Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marangou, N., Marzioni, M. F., McKinsey, D. N., Mei, D. -M., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Naylor, A., Nehrkorn, C., Nelson, H. N., Neves, F., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Riffard, Q., Rischbieter, G. R. C., Rhyne, C., Rossiter, P., Shaw, S., Shutt, T. A., Silva, C., Solmaz, M., Solovov, V. N., Sorensen, P., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W. C., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Utku, U., Uvarov, S., Velan, V., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Woodward, D., Xu, J., Yazdani, K., Zhang, C.

“…The scattering of dark matter (DM) particles with sub-GeV masses off nuclei is difficult to detect using liquid xenon-based DM search instruments because the…”
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Results of a Search for Sub-GeV Dark Matter Using 2013 LUX Data by Akerib, D. S., Alsum, S., Araújo, H. M., Bai, X., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Boxer, B., Brás, P., Burdin, S., Byram, D., Carmona-Benitez, M. C., Chan, C., Cutter, J. E., Davison, T. J. R., Druszkiewicz, E., Fallon, S. R., Fan, A., Fiorucci, S., Gaitskell, R. J., Genovesi, J., Ghag, C., Gilchriese, M. G. D., Gwilliam, C., Hall, C. R., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Jacobsen, R. G., Jahangir, O., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Korolkova, E. V., Kravitz, S., Kudryavtsev, V. A., Lenardo, B. G., Lesko, K. T., Liao, J., Lin, J., Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marangou, N., Marzioni, M. F., McKinsey, D. N., Mei, D. -M., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Naylor, A., Nehrkorn, C., Nelson, H. N., Neves, F., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Riffard, Q., Rischbieter, G. R. C., Rhyne, C., Rossiter, P., Shaw, S., Shutt, T. A., Silva, C., Solmaz, M., Solovov, V. N., Sorensen, P., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W. C., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Utku, U., Uvarov, S., Velan, V., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Woodward, D., Xu, J., Yazdani, K., Zhang, C., LUX Collaboration

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LUX trigger efficiency by Akerib, D. S., Alsum, S., Araújo, H. M., Bai, X., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., B. Boxer, Brás, P., S. Burdin, Byram, D., Carmona-Benitez, M. C., Chan, C., Cutter, J. E., Davison, T. J.R., Druszkiewicz, E., Fallon, S. R., Fan, A., Fiorucci, S., Gaitskell, R. J., Genovesi, J., Ghag, C., Gilchriese, M. G.D., E. Grace, C. Gwilliam, Hall, C. R., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Jacobsen, R. G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., E.V. Korolkova, S. Kravitz, V.A. Kudryavtsev, Lenardo, B. G., Lesko, K. T., Liao, J., J. Lin, Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marangou, N., Marzioni, M. F., McKinsey, D. N., Mei, D. -M., Moongweluwan, M., Morad, J. A., Murphy, A. St.J., Nehrkorn, C., Nelson, H. N., Neves, F., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., G. Rischbieter, Rhyne, C., P. Rossiter, Shaw, S., Shutt, T. A., Silva, C., Solmaz, M., Solovov, V. N., Sorensen, P., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W. C., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Utku, U., Uvarov, S., Velan, V., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L.H., D. Woodward, Xu, J., Yazdani, K., Zhang, C.

“…The Large Underground Xenon experiment (LUX) searches for dark matter using a dual-phase xenon detector. LUX uses a custom-developed trigger system for event…”
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Chromatographic separation of radioactive noble gases from xenon by Akerib, D. S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Bramante, R., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chiller, A. A., Chiller, C., Coffey, T., Currie, A., Cutter, J. E., Davison, T. J. R., Dobi, A., Dobson, J. E. Y., Druszkiewicz, E., Edwards, B. N., Faham, C. H., Fiorucci, S., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G. D., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Ihm, M., Jacobsen, R. G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D. -M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., O’Sullivan, K., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Pech, K., Phelps, P., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T. A., Silva, C., Solovov, V. N., Sorensen, P., Stephenson, S., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Yazdani, K., Young, S. K., Zhang, C.

“…The Large Underground Xenon (LUX) experiment operates at the Sanford Underground Research Facility to detect nuclear recoils from the hypothetical Weakly…”
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Two distinct components of the delayed single electron background signals in liquid xenon emission detectors by Sorensen, P, Kamdin, K

“…2018 JINST 13 P02032 Single electron background signals with millisecond timescales are known to follow ionizing events in liquid/gas xenon emission detectors…”
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Improved Dark Matter Search Sensitivity Resulting from LUX Low-Energy Nuclear Recoil Calibration by LUX Collaboration, Akerib, D. S, Alsum, S, Araújo, H. M, Bai, X, Balajthy, J, Bang, J, Baxter, A, Bernard, E. P, Bernstein, A, Biesiadzinski, T. P, Boulton, E. M, Boxer, B, Brás, P, Burdin, S, Byram, D, Carmona-Benitez, M. C, Chan, C, Cutter, J. E, de Viveiros, L, Druszkiewicz, E, Fan, A, Fiorucci, S, Gaitskell, R. J, Ghag, C, Gilchriese, M. G. D, Gwilliam, C, Hall, C. R, Haselschwardt, S. J, Hertel, S. A, Hogan, D. P, Horn, M, Huang, D. Q, Ignarra, C. M, Jacobsen, R. G, Jahangir, O, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Korolkova, E. V, Kravitz, S, Kudryavtsev, V. A, Leason, E, Lesko, K. T, Liao, J, Lin, J, Lindote, A, Lopes, M. I, Manalaysay, A, Mannino, R. L, Marangou, N, McKinsey, D. N, Mei, D. -M, Morad, J. A, Murphy, A. St. J, Naylor, A, Nehrkorn, C, Nelson, H. N, Neves, F, Nilima, A, Oliver-Mallory, K. C, Palladino, K. J, Rhyne, C, Riffard, Q, Rischbieter, G. R. C, Rossiter, P, Shaw, S, Shutt, T. A, Silva, C, Solmaz, M, Solovov, V. N, Sorensen, P, Sumner, T. J, Swanson, N, Szydagis, M, Taylor, D. J, Taylor, R, Taylor, W. C, Tennyson, B. P, Terman, P. A, Tiedt, D. R, To, W. H, Tvrznikova, L, Utku, U, Vacheret, A, Vaitkus, A, Velan, V, Webb, R. C, White, J. T, Whitis, T. J, Witherell, M. S, Wolfs, F. L. H, Woodward, D, Xiang, X, Xu, J, Zhang, C

“…Dual-phase xenon time projection chamber (TPC) detectors have demonstrated superior search sensitivities to dark matter over a wide range of particle masses…”
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Constraints on Effective Field Theory Couplings Using 311.2 days of LUX Data by Akerib, D. S, Alsum, S, Araújo, H. M, Bai, X, Balajthy, J, Bang, J, Baxter, A, Bernard, E. P, Bernstein, A, Biesiadzinski, T. P, Boulton, E. M, Boxer, B, Brás, P, Burdin, S, Byram, D, Carmona-Benitez, M. C, Chan, C, Cutter, J. E, de Viveiros, L, Druszkiewicz, E, Fan, A, Fiorucci, S, Gaitskell, R. J, Ghag, C, Gilchriese, M. G. D, Gwilliam, C, Hall, C. R, Haselschwardt, S. J, Hertel, S. A, Hogan, D. P, Horn, M, Huang, D. Q, Ignarra, C. M, Jacobsen, R. G, Jahangir, O, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Korolkova, E. V, Kravitz, S, Kudryavtsev, V. A, Leason, E, Lenardo, B. G, Lesko, K. T, Liao, J, Lin, J, Lindote, A, Lopes, M. I, Manalaysay, A, Mannino, R. L, Marangou, N, McKinsey, D. N, Mei, D. -M, Morad, J. A, Murphy, A. St. J, Naylor, A, Nehrkorn, C, Nelson, H. N, Neves, F, Nilima, A, Oliver-Mallory, K. C, Palladino, K. J, Rhyne, C, Riffard, Q, Rischbieter, G. R. C, Rossiter, P, Shaw, S, Shutt, T. A, Silva, C, Solmaz, M, Solovov, V. N, Sorensen, P, Sumner, T. J, Swanson, N, Szydagis, M, Taylor, D. J, Taylor, R, Taylor, W. C, Tennyson, B. P, Terman, P. A, Tiedt, D. R, To, W. H, Tvrznikova, L, Utku, U, Vacheret, A, Vaitkus, A, Velan, V, Webb, R. C, White, J. T, Whitis, T. J, Witherell, M. S, Wolfs, F. L. H, Woodward, D, Xiang, X, Xu, J, Zhang, C

“…Phys. Rev. D 104, 062005 (2021) We report here the results of an Effective Field Theory (EFT) WIMP search analysis using LUX data. We build upon previous LUX…”
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Investigation of background electron emission in the LUX detector by Akerib, D. S, Alsum, S, Araújo, H. M, Bai, X, Balajthy, J, Baxter, A, Bernard, E. P, Bernstein, A, Biesiadzinski, T. P, Boulton, E. M, Boxer, B, Brás, P, Burdin, S, Byram, D, Carmona-Benitez, M. C, Chan, C, Cutter, J. E, de Viveiros, L, Druszkiewicz, E, Fan, A, Fiorucci, S, Gaitskell, R. J, Ghag, C, Gilchriese, M. G. D, Gwilliam, C, Hall, C. R, Haselschwardt, S. J, Hertel, S. A, Hogan, D. P, Horn, M, Huang, D. Q, Ignarra, C. M, Jacobsen, R. G, Jahangir, O, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Korolkova, E. V, Kravitz, S, Kudryavtsev, V. A, Leason, E, Lenardo, B. G, Lesko, K. T, Liao, J, Lin, J, Lindote, A, Lopes, M. I, Manalaysay, A, Mannino, R. L, Marangou, N, McKinsey, D. N, Mei, D. M, Moongweluwan, M, Morad, J. A, Murphy, A. St. J, Naylor, A, Nehrkorn, C, Nelson, H. N, Neves, F, Nilima, A, Oliver-Mallory, K. C, Palladino, K. J, Pease, E. K, Riffard, Q, Rischbieter, G. R. C, Rhyne, C, Rossiter, P, Shaw, S, Shutt, T. A, Silva, C, Solmaz, M, Solovov, V. N, Sorensen, P, Sumner, T. J, Szydagis, M, Taylor, D. J, Taylor, R, Taylor, W. C, Tennyson, B. P, Terman, P. A, Tiedt, D. R, To, W. H, Tvrznikova, L, Utku, U, Uvarov, S, Vacheret, A, Velan, V, Webb, R. C, White, J. T, Whitis, T. J, Witherell, M. S, Wolfs, F. L. H, Woodward, D, Xu, J, Zhang, C

“…Phys. Rev. D 102, 092004 (2020) Dual-phase xenon detectors, as currently used in direct detection dark matter experiments, have observed elevated rates of…”
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Improved Modeling of $\beta$ Electronic Recoils in Liquid Xenon Using LUX Calibration Data by The LUX Collaboration, Akerib, D. S, Alsum, S, Araújo, H. M, Bai, X, Balajthy, J, Baxter, A, Bernard, E. P, Bernstein, A, Biesiadzinski, T. P, Boulton, E. M, Boxer, B, Brás, P, Burdin, S, Byram, D, Carmona-Benitez, M. C, Chan, C, Cutter, J. E, de Viveiros, L, Druszkiewicz, E, Fan, A, Fiorucci, S, Gaitskell, R. J, Ghag, C, Gilchriese, M. G. D, Gwilliam, C, Hall, C. R, Haselschwardt, S. J, Hertel, S. A, Hogan, D. P, Horn, M, Huang, D. Q, Ignarra, C. M, Jacobsen, R. G, Jahangir, O, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Korolkova, E. V, Kravits, S, Kudryavtsev, V. A, Leason, E, Lenardo, B. G, Lesko, K. T, Liao, J, Lin, J, Lindote, A, Lopes, M. I, Manalaysay, A, Mannino, R. L, Marangou, N, Marzioni, M. F, McKinsey, D. N, Mei, D. M, Moongweluwan, M, Morad, J. A, Murphy, A. St. J, Naylor, A, Nehrkorn, C, Nelson, H. N, Neves, F, Nilima, A, Oliver-Mallory, K. C, Palladino, K. J, Pease, E. K, Riffard, Q, Rischbieter, G. R. C, Rhyne, C, Rossiter, P, Shaw, S, Shutt, T. A, Silva, C, Solmaz, M, Solovov, V. N, Sorensen, P, Sumner, T. J, Szydagis, M, Taylor, D. J, Taylor, R, Taylor, W. C, Tennyson, B. P, Terman, P. A, Tiedt, D. R, To, W. H, Tripathi, M, Tvrznikova, L, Utku, U, Uvarov, S, Vacheret, A, Velan, V, Webb, R. C, White, J. T, Whitis, T. J, Witherell, M. S, Wolfs, F. L. H, Woodward, D, Xu, J, Zhang, C

“…Journal of Instrumentation, Volume 15, February 2020 We report here methods and techniques for creating and improving a model that reproduces the scintillation…”
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Liquid xenon scintillation measurements and pulse shape discrimination in the LUX dark matter detector by The LUX Collaboration, Akerib, D. S, Alsum, S, Araújo, H. M, Bai, X, Bailey, A. J, Balajthy, J, Beltrame, P, Bernard, E. P, Bernstein, A, Biesiadzinski, T. P, Boulton, E. M, Brás, P, Byram, D, Carmona-Benitez, M. C, Chan, C, Currie, A, Cutter, J. E, Davison, T. J. R, Dobi, A, Druszkiewicz, E, Edwards, B. N, Fallon, S. R, Fan, A, Fiorucci, S, Gaitskell, R. J, Genovesi, J, Ghag, C, Gilchriese, M. G. D, Hall, C. R, Haselschwardt, S. J, Hertel, S. A, Hogan, D. P, Horn, M, Huang, D. Q, Ignarra, C. M, Jacobsen, R. G, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Knoche, R, Lenardo, B. G, Lesko, K. T, Liao, J, Lindote, A, Lopes, M. I, Manalaysay, A, Mannino, R. L, Marzioni, M. F, McKinsey, D. N, Mei, D. M, Mock, J, Moongweluwan, M, Morad, J. A, Murphy, A. St. J, Nehrkorn, C, Nelson, H. N, Neves, F, O'Sullivan, K, Oliver-Mallory, K. C, Palladino, K. J, Pease, E. K, Rhyne, C, Shaw, S, Shutt, T. A, Silva, C, Solmaz, M, Solovov, V. N, Sorensen, P, Sumner, T. J, Szydagis, M, Taylor, D. J, Taylor, W. C, Tennyson, B. P, Terman, P. A, Tiedt, D. R, To, W. H, Tripathi, M, Tvrznikova, L, Utku, U, Uvarov, S, Velan, V, Verbus, J. R, Webb, R. C, White, J. T, Whitis, T. J, Witherell, M. S, Wolfs, F. L. H, Xu, J, Yazdani, K, Young, S. K, Zhang, C

“…Phys. Rev. D 97, 112002 (2018) Weakly Interacting Massive Particles (WIMPs) are a leading candidate for dark matter and are expected to produce nuclear recoil…”
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Position Reconstruction in LUX by LUX Collaboration, Akerib, D. S, Alsum, S, Araújo, H. M, Bai, X, Bailey, A. J, Balajthy, J, Beltrame, P, Bernard, E. P, Bernstein, A, Biesiadzinski, T. P, Boulton, E. M, Brás, P, Byram, D, Cahn, S. B, Carmona-Benitez, M. C, Chan, C, Currie, A, Cutter, J. E, Davison, T. J. R, Dobi, A, Druszkiewicz, E, Edwards, B. N, Fallon, S. R, Fan, A, Fiorucci, S, Gaitskell, R. J, Genovesi, J, Ghag, C, Gilchriese, M. G. D, Hall, C. R, Hanhardt, M, Haselschwardt, S. J, Hertel, S. A, Hogan, D. P, Horn, M, Huang, D. Q, Ignarra, C. M, Jacobsen, R. G, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, N. A, Lenardo, B. G, Lesko, K. T, Lindote, A, Lopes, M. I, Manalaysay, A, Mannino, R. L, Marzioni, M. F, McKinsey, D. N, Mei, D. M, Mock, J, Moongweluwan, M, Morad, J. A, Murphy, A. St. J, Nehrkorn, C, Nelson, H. N, Neves, F, O'Sullivan, K, Oliver-Mallory, K. C, Palladino, K. J, Pease, E. K, Rhyne, C, Shaw, S, Shutt, T. A, Silva, C, Solmaz, M, Solovov, V. N, Sorensen, P, Sumner, T. J, Szydagis, M, Taylor, D. J, Taylor, W. C, Tennyson, B. P, Terman, P. A, Tiedt, D. R, To, W. H, Tripathi, M, Tvrznikova, L, Uvarov, S, Velan, V, Verbus, J. R, Webb, R. C, White, J. T, Whitis, T. J, Witherell, M. S, Wolfs, F. L. H, Xu, J, Yazdani, K, Young, S. K, Zhang, C

“…Journal of Instrumentation, Volume 13, February 2018, P02001 The $(x, y)$ position reconstruction method used in the analysis of the complete exposure of the…”
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3D Modeling of Electric Fields in the LUX Detector by LUX Collaboration, Akerib, D. S, Alsum, S, Araújo, H. M, Bai, X, Bailey, A. J, Balajthy, J, Beltrame, P, Bernard, E. P, Bernstein, A, Biesiadzinski, T. P, Boulton, E. M, Brás, P, Byram, D, Cahn, S. B, Carmona-Benitez, M. C, Chan, C, Currie, A, Cutter, J. E, Davison, T. J. R, Dobi, A, Druszkiewicz, E, Edwards, B. N, Fallon, S. R, Fan, A, Fiorucci, S, Gaitskell, R. J, Genovesi, J, Ghag, C, Gilchriese, M. G. D, Hall, C. R, Hanhardt, M, Haselschwardt, S. J, Hertel, S. A, Hogan, D. P, Horn, M, Huang, D. Q, Ignarra, C. M, Jacobsen, R. G, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, N. A, Lenardo, B. G, Lesko, K. T, Lindote, A, Lopes, M. I, Manalaysay, A, Mannino, R. L, Marzioni, M. F, McKinsey, D. N, Mei, D. M, Mock, J, Moongweluwan, M, Morad, J. A, Murphy, A. St. J, Nehrkorn, C, Nelson, H. N, Neves, F, O'Sullivan, K, Oliver-Mallory, K. C, Palladino, K. J, Pease, E. K, Rhyne, C, Shaw, S, Shutt, T. A, Silva, C, Solmaz, M, Solovov, V. N, Sorensen, P, Sumner, T. J, Szydagis, M, Taylor, D. J, Taylor, W. C, Tennyson, B. P, Terman, P. A, Tiedt, D. R, To, W. H, Tripathi, M, Tvrznikova, L, Uvarov, S, Velan, V, Verbus, J. R, Webb, R. C, White, J. T, Whitis, T. J, Witherell, M. S, Wolfs, F. L. H, Xu, J, Yazdani, K, Young, S. K, Zhang, C

“…JINST 12, no. 11, P11022 (2017) This work details the development of a three-dimensional (3D) electric field model for the LUX detector. The detector took data…”
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