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2. Chromatographic separation of radioactive noble gases from xenon

Author

Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Boulton, EM, Bramante, R, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chiller, AA, Chiller, C, Coffey, T, Currie, A, Cutter, JE, Davison, TJR, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edwards, BN, Faham, CH, Fiorucci, S, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, CR, Hanhardt, M, Haselschwardt, SJ, Hertel, SA, Hogan, DP, Horn, M, Huang, DQ, Ignarra, CM, Ihm, M, Jacobsen, RG, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Lindote, A, Lopes, MI, Manalaysay, A, Mannino, RL, Marzioni, MF, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, JA, Murphy, A St J, Nehrkorn, C, Nelson, HN, Neves, F, O’Sullivan, K, Oliver-Mallory, KC, Palladino, KJ, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Rhyne, C, Shaw, S, Shutt, TA, Silva, C, Solovov, VN, Sorensen, P, Stephenson, S, Sumner, TJ, Szydagis, M, Taylor, DJ, Taylor, W, Tennyson, BP, Terman, PA, Tiedt, DR, To, WH, Tripathi, M, Tvrznikova, L, Uvarov, S, Verbus, JR, Webb, RC, White, JT, Whitis, TJ, Witherell, MS, Wolfs, FLH, Yazdani, K, Young, SK, and Zhang, C

Subjects
Chromatography, Xenon, Particle and Plasma Physics, Gas Separation, Krypton, Dark Matter, Molecular, Nuclear, Adsorption, physics.ins-det, Nuclear & Particles Physics, Atomic, Astronomical and Space Sciences
Abstract

The Large Underground Xenon (LUX) experiment operates at the Sanford Underground Research Facility to detect nuclear recoils from the hypothetical Weakly Interacting Massive Particles (WIMPs) on a liquid xenon target. Liquid xenon typically contains trace amounts of the noble radioactive isotopes 85Kr and 39Ar that are not removed by the in situ gas purification system. The decays of these isotopes at concentrations typical of research-grade xenon would be a dominant background for a WIMP search experiment. To remove these impurities from the liquid xenon, a chromatographic separation system based on adsorption on activated charcoal was built. 400 kg of xenon was processed, reducing the average concentration of krypton from 130 ppb to 3.5 ppt as measured by a cold-trap assisted mass spectroscopy system. A 50 kg batch spiked to 0.001 g/g of krypton was processed twice and reduced to an upper limit of 0.2 ppt.

Published
2018

3. DE-ESCALATION OF TYROSINE KINASE INHIBITOR THERAPY IS SAFE IN CHRONIC MYELOID LEUKAEMIA IN DURABLE MOLECULAR RESPONSE (>= MR3 FOR >= 12 MONTHS): INITIAL RESULTS IN THE BRITISH DESTINY STUDY

Author

Clark, R, Polydoros, F, Apperley, J, Pocock, C, Smith, G, Salim, R, Coffey, T, O'Brien, S, Foroni, L, Copland, M, Bristol Myers Squibb, National Institute for Health Research, and Leuka

Subjects
Science & Technology, Immunology, Hematology, Life Sciences & Biomedicine, 1102 Cardiovascular Medicine And Haematology
Published
2016

4. The LUX Experiment

Author

Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Bernard, E, Bernstein, A, Bradley, A, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Coffey, T, Currie, A, De Viveiros, L, Dobi, A, Dobson, J, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Flores, C, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, C, Hertel, SA, Horn, M, Huang, DQ, Ihm, M, Jacobsen, RG, Kazkaz, K, Knoche, R, Larsen, NA, Lee, C, Lindote, A, Lopes, MI, Malling, DC, Mannino, R, McKinsey, DN, Mei, DM, Mock, J, Moongweluwan, M, Morad, J, Murphy, ASJ, Nehrkorn, C, Nelson, H, Neves, F, Ott, RA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Solovov, VN, Sorensen, P, O'Sullivan, K, Sumner, TJ, Szydagis, M, Taylor, D, Tennyson, B, Tiedt, DR, Tripathi, M, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, JT, Witherell, MS, Wolfs, FLH, Woods, M, and Zhang, C

Subjects
WIMP, Direct detection, Dark matter, Liquid xenon detectors
Abstract

We present the status and prospects of the LUX experiment, which employs approximately 300 kg of two-phase xenon to search for WIMP dark matter interactions. The LUX detector was commissioned at the surface laboratory of the Sanford Underground Research Facility in Lead, SD, between December 2011 and February 2012 and the detector has been operating underground since January, 2013. These proceedings review the results of the commissioning run as well as the status of underground data-taking through the summer of 2013.

Published
2015

5. The LUX Experiment

Author

Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Bernard, E, Bernstein, A, Bradley, A, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Coffey, T, Currie, A, de Viveiros, L, Dobi, A, Dobson, J, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Flores, C, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, C, Hertel, SA, Horn, M, Huang, DQ, Ihm, M, Jacobsen, RG, Kazkaz, K, Knoche, R, Larsen, NA, Lee, C, Lindote, A, Lopes, MI, Malling, DC, Mannino, R, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J, Murphy, A St J, Nehrkorn, C, Nelson, H, Neves, F, Ott, RA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Solovov, VN, Sorensen, P, O'Sullivan, K, Sumner, TJ, Szydagis, M, Taylor, D, Tennyson, B, Tiedt, DR, Tripathi, M, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, JT, Witherell, MS, Wolfs, FLH, Woods, M, and Zhang, C

Subjects
WIMP, Direct detection, Dark matter, Liquid xenon detectors
Abstract

We present the status and prospects of the LUX experiment, which employs approximately 300 kg of two-phase xenon to search for WIMP dark matter interactions. The LUX detector was commissioned at the surface laboratory of the Sanford Underground Research Facility in Lead, SD, between December 2011 and February 2012 and the detector has been operating underground since January, 2013. These proceedings review the results of the commissioning run as well as the status of underground data-taking through the summer of 2013.

Published
2015

6. First results from the LUX dark matter experiment at the Sanford underground research facility

Author

Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Bedikian, S, Bernard, E, Bernstein, A, Bolozdynya, A, Bradley, A, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Clark, K, Coffey, T, Currie, A, Curioni, A, Dazeley, S, de Viveiros, L, Dobi, A, Dobson, J, Dragowsky, EM, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Flores, C, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, C, Hanhardt, M, Hertel, SA, Horn, M, Huang, DQ, Ihm, M, Jacobsen, RG, Kastens, L, Kazkaz, K, Knoche, R, Kyre, S, Lander, R, Larsen, NA, Lee, C, Leonard, DS, Lesko, KT, Lindote, A, Lopes, MI, Lyashenko, A, Malling, DC, Mannino, R, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J, Morii, M, Murphy, A St J, Nehrkorn, C, Nelson, H, Neves, F, Nikkel, JA, Ott, RA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Skulski, W, Sofka, CJ, Solovov, VN, Sorensen, P, Stiegler, T, O'Sullivan, K, Sumner, TJ, Svoboda, R, Sweany, M, Szydagis, M, Taylor, D, Tennyson, B, Tiedt, DR, Tripathi, M, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, JT, White, D, Witherell, MS, Wlasenko, M, and Wolfs, FLH

Subjects
General Physics, Engineering, hep-ex, Physical Sciences, astro-ph.CO, physics.ins-det, Mathematical Sciences, LUX Collaboration, astro-ph.IM
Abstract

The Large Underground Xenon (LUX) experiment is a dual-phase xenon time-projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota). The LUX cryostat was filled for the first time in the underground laboratory in February 2013. We report results of the first WIMP search data set, taken during the period from April to August 2013, presenting the analysis of 85.3 live days of data with a fiducial volume of 118 kg. A profile-likelihood analysis technique shows our data to be consistent with the background-only hypothesis, allowing 90% confidence limits to be set on spin-independent WIMP-nucleon elastic scattering with a minimum upper limit on the cross section of 7.6 × 10(-46) cm(2) at a WIMP mass of 33 GeV/c(2). We find that the LUX data are in disagreement with low-mass WIMP signal interpretations of the results from several recent direct detection experiments.

Published
2014

7. Direct search for dark matter with two-phase xenon detectors: Current status of LUX and plans for LZ

Author

Akerib, D. S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Bernard, E., Bernstein, A., Bradley, A., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chapman, J. J., Chiller, A. A., Chiller, C., Coffey, T., Currie, A., Viveiros, L., Dobi, A., Dobson, J., Druszkiewicz, E., Edwards, B., Faham, C. H., Fiorucci, S., Flores, C., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G. D., Hall, C., Hertel, S. A., Horn, M., Huang, D. Q., Ihm, M., Jacobsen, R. G., Kazkaz, K., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B., Lesko, K. T., Lindote, A., Lopes, M. I., Malling, D. C., Man-Nino, R., Mckinsey, D. N., Mei, D. -M, Mock, J., Moongweluwan, M., Morad, J., Murphy, A. St J., Nehrkorn, C., Nelson, H., Neves, F., Ott, R. A., Pangilinan, M., Parker, P. D., Pease, E. K., Pech, K., Phelps, P., Reichhart, L., Shutt, T., Claudio Silva, Solovov, V. N., Sorensen, P., O Sullivan, K., Sumner, T. J., Szydagis, M., Tay-Lor, D., Tennyson, B., Tiedt, D. R., Tripathi, M., Uvarov, S., Verbus, J. R., Walsh, N., Webb, R., White, J. T., Witherell, M. S., Wolfs, F. L. H., Woods, M., and Zhang, C.

Abstract

The search for dark matter reaches back generations and remains one of the most compelling endeavors in the hunt for physics beyond the Standard Model. Experiments attempting to directly detect WIMP dark matter have made re-markable progress in increasing sensitivity to elastic scattering of WIMPs on nuclei. The LUX experiment is a 370-kg, two-phase, xenon TPC currently running at SURF, 4850 feet below Lead, SD. LUX recently completed its first science run and was sensitive to spin independent WIMP scattering at cross sections below 10-45 cm2 for WIMP masses of approximately 20 to 80 GeV. Preparations for the final science run of LUX are currently underway, with final results expected in 2015. We will present results from and current status of the LUX experiment, as well as plans for a follow-on, multi-ton-scale xenon experiment at SURF.

Published
2014

8. After LUX: The LZ program

Author

Malling, DC, Akerib, DS, Araujo, HM, Bai, X, Bedikian, S, Bernard, E, Bernstein, A, Bradley, A, Cahn, SB, Carmona-Benitez, MC, Carr, D, Chapman, JJ, Clark, K, Classen, T, Coffey, T, Curioni, A, Currie, A, Dazeley, S, Viveiros, LD, Dragowsky, M, Druszkiewicz, E, Faham, CH, Fiorucci, S, Gaitskell, RJ, Gibson, KR, Hall, C, Hanhardt, M, Holbrook, B, Ihm, M, Jacobsen, RG, Kastens, L, Kazkaz, K, Lander, R, Larsen, N, Lee, C, Leonard, D, Lesko, K, Lindote, A, Lopes, MI, Lyashenko, A, Majewski, P, Mannino, R, McKinsey, DN, Mei, D-M, Mock, J, Morii, M, Murphy, ASJ, Nelson, H, Neves, F, Nikkel, JA, Pangilinan, M, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Skulski, W, Solovov, V, Sorensen, P, Spaans, J, Stiegler, T, Sumner, TJ, Svoboda, R, Sweany, M, Szydagis, M, Thomson, J, Tripathi, M, Verbus, JR, Walsh, N, Webb, R, White, JT, Wlasenko, M, Wolfs, FLH, Woods, M, and Zhang, C

Subjects
astro-ph.CO, astro-ph.IM
Abstract

The LZ program consists of two stages of direct dark matter searches using liquid Xe detectors. The first stage will be a 1.5-3 tonne detector, while the last stage will be a 20 tonne detector. Both devices will benefit tremendously from research and development performed for the LUX experiment, a 350 kg liquid Xe dark matter detector currently operating at the Sanford Underground Laboratory. In particular, the technology used for cryogenics and electrical feedthroughs, circulation and purification, low-background materials and shielding techniques, electronics, calibrations, and automated control and recovery systems are all directly scalable from LUX to the LZ detectors. Extensive searches for potential background sources have been performed, with an emphasis on previously undiscovered background sources that may have a significant impact on tonne-scale detectors. The LZ detectors will probe spin-independent interaction cross sections as low as 5E-49 cm2 for 100 GeV WIMPs, which represents the ultimate limit for dark matter detection with liquid xenon technology.

Published
2011

9. After LUX: The LZ program

Author

Malling, DC, Chapman, JJ, Faham, CH, Fiorucci, S, Gaitskell, RJ, Pangilinan, M, Verbus, JR, Akerib, DS, Bradley, A, Carmona-Benitez, MC, Clark, K, Coffey, T, Dragowsky, M, Gibson, KR, Lee, C, Phelps, P, Shutt, T, Araújo, HM, Currie, A, Sumner, TJ, Bai, X, Hanhardt, M, Bedikian, S, Bernard, E, Cahn, SB, Kastens, L, Larsen, N, Lyashenko, A, McKinsey, DN, Nikkel, JA, Bernstein, A, Carr, D, Dazeley, S, Kazkaz, K, Sorensen, P, Classen, T, Holbrook, B, Lander, R, Mock, J, Svoboda, R, Sweany, M, Szydagis, M, Thomson, J, Tripathi, M, Walsh, N, Woods, M, de Viveiros, L, Lindote, A, Lopes, MI, Neves, F, Silva, C, Solovov, V, Druszkiewicz, E, Skulski, W, Wolfs, FLH, Hall, C, Leonard, D, Ihm, M, Jacobsen, RG, Lesko, K, Majewski, P, Mannino, R, Stiegler, T, Webb, R, White, JT, Mei, DM, Spaans, J, Zhang, C, Morii, M, Wlasenko, M, Murphy, ASJ, Reichhart, L, and Nelson, H

Subjects
astro-ph.CO, astro-ph.IM
Abstract

© Proceedings of the 2011 Meeting of the Division of Particles and Fields of the American Physical Society, DPF 2011. All rights reserved. The LZ program consists of two stages of direct dark matter searches using liquid Xe detectors. The first stage will be a 1.5-3 tonne detector, while the last stage will be a 20 tonne detector. Both devices will benefit tremendously from research and development performed for the LUX experiment, a 350 kg liquid Xe dark matter detector currently operating at the Sanford Underground Laboratory. In particular, the technology used for cryogenics and electrical feedthroughs, circulation and purification, low-background materials and shielding techniques, electronics, calibrations, and automated control and recovery systems are all directly scalable from LUX to the LZ detectors. Extensive searches for potential background sources have been performed, with an emphasis on previously undiscovered background sources that may have a significant impact on tonne-scale detectors. The LZ detectors will probe spin-independent interaction cross sections as low as 5 × 10-49 cm2 for 100 GeV WIMPs, which represents the ultimate limit for dark matter detection with liquid xenon technology.

Published
2011

10. After LUX: The LZ program

Author

Malling, DC, Chapman, JJ, Faham, CH, Fiorucci, S, Gaitskell, RJ, Pangilinan, M, Verbus, JR, Akerib, DS, Bradley, A, Carmona-Benitez, MC, Clark, K, Coffey, T, Dragowsky, M, Gibson, KR, Lee, C, Phelps, P, Shutt, T, Araújo, HM, Currie, A, Sumner, TJ, Bai, X, Hanhardt, M, Bedikian, S, Bernard, E, Cahn, SB, Kastens, L, Larsen, N, Lyashenko, A, McKinsey, DN, Nikkel, JA, Bernstein, A, Carr, D, Dazeley, S, Kazkaz, K, Sorensen, P, Classen, T, Holbrook, B, Lander, R, Mock, J, Svoboda, R, Sweany, M, Szydagis, M, Thomson, J, Tripathi, M, Walsh, N, Woods, M, de Viveiros, L, Lindote, A, Lopes, MI, Neves, F, Silva, C, Solovov, V, Druszkiewicz, E, Skulski, W, Wolfs, FLH, Hall, C, Leonard, D, Ihm, M, Jacobsen, RG, Lesko, K, Majewski, P, Mannino, R, Stiegler, T, Webb, R, White, JT, Mei, DM, Spaans, J, Zhang, C, Morii, M, Wlasenko, M, Murphy, ASJ, Reichhart, L, and Nelson, H

Subjects
astro-ph.CO, astro-ph.IM
Abstract

© Proceedings of the 2011 Meeting of the Division of Particles and Fields of the American Physical Society, DPF 2011. All rights reserved. The LZ program consists of two stages of direct dark matter searches using liquid Xe detectors. The first stage will be a 1.5-3 tonne detector, while the last stage will be a 20 tonne detector. Both devices will benefit tremendously from research and development performed for the LUX experiment, a 350 kg liquid Xe dark matter detector currently operating at the Sanford Underground Laboratory. In particular, the technology used for cryogenics and electrical feedthroughs, circulation and purification, low-background materials and shielding techniques, electronics, calibrations, and automated control and recovery systems are all directly scalable from LUX to the LZ detectors. Extensive searches for potential background sources have been performed, with an emphasis on previously undiscovered background sources that may have a significant impact on tonne-scale detectors. The LZ detectors will probe spin-independent interaction cross sections as low as 5 × 10-49 cm2 for 100 GeV WIMPs, which represents the ultimate limit for dark matter detection with liquid xenon technology.

Published
2011

11. After LUX: The LZ Program

Author

Malling, D. C., Akerib, D. S., Araujo, H. M., Bai, X., Bedikian, S., Bernard, E., Bernstein, A., Bradley, A., Cahn, S. B., Carmona-Benitez, M. C., Carr, D., Chapman, J. J., Clark, K., Classen, T., Coffey, T., Curioni, A., Currie, A., Dazeley, S., de Viveiros, L., Dragowsky, M., Druszkiewicz, E., Faham, C. H., Fiorucci, S., Gaitskell, R. J., Gibson, K. R., Hall, C., Hanhardt, M., Holbrook, B., Ihm, M., Jacobsen, R. G., Kastens, L., Kazkaz, K., Lander, R., Larsen, N., Lee, C., Leonard, D., Lesko, K., Lindote, A., Lopes, M. I., Lyashenko, A., Majewski, P., Mannino, R., McKinsey, D. N., Mei, D. -M., Mock, J., Morii, M., Murphy, A. St J., Nelson, H., Neves, F., Nikkel, J. A., Pangilinan, M., Phelps, P., Reichhart, L., Shutt, T., Silva, C., Skulski, W., Solovov, V., Sorensen, P., Spaans, J., Stiegler, T., Sumner, T. J., Svoboda, R., Sweany, M., Szydagis, M., Thomson, J., Tripathi, M., Verbus, J. R., Walsh, N., Webb, R., White, J. T., Wlasenko, M., Wolfs, F. L. H., Woods, M., and Zhang, C.

Subjects
Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, Instrumentation and Methods for Astrophysics (astro-ph.IM)
Abstract

The LZ program consists of two stages of direct dark matter searches using liquid Xe detectors. The first stage will be a 1.5-3 tonne detector, while the last stage will be a 20 tonne detector. Both devices will benefit tremendously from research and development performed for the LUX experiment, a 350 kg liquid Xe dark matter detector currently operating at the Sanford Underground Laboratory. In particular, the technology used for cryogenics and electrical feedthroughs, circulation and purification, low-background materials and shielding techniques, electronics, calibrations, and automated control and recovery systems are all directly scalable from LUX to the LZ detectors. Extensive searches for potential background sources have been performed, with an emphasis on previously undiscovered background sources that may have a significant impact on tonne-scale detectors. The LZ detectors will probe spin-independent interaction cross sections as low as 5E-49 cm2 for 100 GeV WIMPs, which represents the ultimate limit for dark matter detection with liquid xenon technology., Conference proceedings from APS DPF 2011. 9 pages, 6 figures

Published
2011
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12. A bulk 2D Pauli Limited Superconductor

Author

Coffey, T., Martin, C., Agosta, C. C., Kinoshota, Tatsue, and Tokumoto, M.

Subjects
Superconductivity (cond-mat.supr-con), Condensed Matter - Superconductivity, FOS: Physical sciences
Abstract

We present a nearly perfect Pauli-limited critical field phase diagram for the anisotropic organic superconductor \$\alpha$-(ET)$_2$NH$_4$(SCN)$_4$ when the applied magnetic field is oriented parallel to the conducting layers. The critical fields (${H_{c_2}$) were found by use of penetration depth measurements. Because ${H_{c_2}$ is Pauli-limited, the size of the superconducting energy gap can be calculated. The role of spin-orbit scattering and many-body effects play a role in explaining our measurements., Comment: 4 pages, 5 figures. V5, corrections were made to the text, present data was included

Published
2003
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13. A Detailed Look at the First Results from the Large Underground Xenon (LUX) Dark Matter Experiment

Author

Matthew Szydagis, Akerib, D. S., Araujo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Bernard, E., Bernstein, A., Bradley, A., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chapman, J. J., Chiller, A. A., Chiller, C., Coffey, T., Currie, A., Viveiros, L., Dobi, A., Dobson, J., Druszkiewicz, E., Edwards, B., Faham, C. H., Fiorucci, S., Flores, C., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G. D., Carter Hall, Hertel, S. A., Horn, M., Huang, D. Q., Ihm, M., Jacobsen, R. G., Kazkaz, K., Knoche, R., Larsen, N. A., Lee, C., Lindote, A., Lopes, M. I., Malling, D. C., Mannino, R., Mckinsey, D. N., Mei, D. M., Mock, J., Moongweluwan, M., Morad, J., Murphy, A. St J., Nehrkorn, C., Nelson, H., Neves, F., Ott, R. A., Pangilinan, M., Parker, P. D., Pease, E. K., Pech, K., Phelps, P., Reichhart, L., Shutt, T., Silva, C., Solovov, V. N., Sorensen, P., O Sullivan, K., Taylor, D., Tennyson, B., Tiedt, D. R., Tripathi, M., Uvarov, S., Verbus, J. R., Walsh, N., Webb, R., White, J. T., Witherell, M. S., Wolfs, F. L. H., Woods, M., and Zhang, C.

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