Related papers: Light WIMP search in XMASS

Direct Detection Limits on Heavy Dark Matter

Multiply-interacting massive particles (MIMPs) are heavy (>10^10 GeV/c^2) dark matter particles that interact strongly with regular matter, but may have evaded detection due to the low number density required to make up the local dark…

High Energy Physics - Phenomenology · Physics 2022-01-12 Michael Clark , Amanda Depoian , Bahaa Elshimy , Abigail Kopec , Rafael F. Lang , Shengchao Li , Juehang Qin

First Dark Matter Limits from the COUPP 4kg Bubble Chamber at a Deep Underground Site

The COUPP 4 kg bubble chamber employs 4.0 kg of CF$_3$I as a WIMP scattering target for use as a dark matter direct detection search. This thesis reports the first experimental results from operating this bubble chamber at the deep…

Cosmology and Nongalactic Astrophysics · Physics 2024-01-17 Drew Fustin

CDMSlite: A Search for Low-Mass WIMPs using Voltage-Assisted Calorimetric Ionization Detection in the SuperCDMS Experiment

SuperCDMS is an experiment designed to directly detect Weakly Interacting Massive Particles (WIMPs), a favored candidate for dark matter ubiquitous in the Universe. In this paper, we present WIMP-search results using a calorimetric…

Instrumentation and Detectors · Physics 2014-02-05 R. Agnese , A. J. Anderson , M. Asai , D. Balakishiyeva , R. Basu Thakur , D. A. Bauer , J. Billard , A. Borgland , M. A. Bowles , D. Brandt , P. L. Brink , R. Bunker , B. Cabrera , D. O. Caldwell , D. G. Cerdeno , H. Chagani , J. Cooley , B. Cornell , C. H. Crewdson , P. Cushman , M. Daal , P. C. F. Di Stefano , T. Doughty , L. Esteban , S. Fallows , E. Figueroa-Feliciano , G. L. Godfrey , S. R. Golwala , J. Hall , H. R. Harris , S. A. Hertel , T. Hofer , D. Holmgren , L. Hsu , M. E. Huber , A. Jastram , O. Kamaev , B. Kara , M. H. Kelsey , A. Kennedy , M. Kiveni , K. Koch , B. Loer , E. Lopez Asamar , R. Mahapatra , V. Mandic , C. Martinez , K. A. McCarthy , N. Mirabolfathi , R. A. Moffatt , D. C. Moore , P. Nadeau , R. H. Nelson , K. Page , R. Partridge , M. Pepin , A. Phipps , K. Prasad , M. Pyle , H. Qiu , W. Rau , P. Redl , A. Reisetter , Y. Ricci , T. Saab , B. Sadoulet , J. Sander , K. Schneck , R. W. Schnee , S. Scorza , B. Serfass , B. Shank , D. Speller , A. N. Villano , B. Welliver , D. H. Wright , S. Yellin , J. J. Yen , B. A. Young , J. Zhang

Liquid xenon scintillation measurements and pulse shape discrimination in the LUX dark matter detector

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…

Instrumentation and Detectors · Physics 2018-06-20 The LUX Collaboration , D. S. Akerib , S. Alsum , H. M. Araújo , X. Bai , A. J. Bailey , J. Balajthy , P. Beltrame , E. P. Bernard , A. Bernstein , T. P. Biesiadzinski , E. M. Boulton , P. Brás , D. Byram , M. C. Carmona-Benitez , C. Chan , A. Currie , J. E. Cutter , T. J. R. Davison , A. Dobi , E. Druszkiewicz , B. N. Edwards , S. R. Fallon , A. Fan , S. Fiorucci , R. J. Gaitskell , J. Genovesi , C. Ghag , M. G. D. Gilchriese , C. R. Hall , S. J. Haselschwardt , S. A. Hertel , D. P. Hogan , M. Horn , D. Q. Huang , C. M. Ignarra , R. G. Jacobsen , W. Ji , K. Kamdin , K. Kazkaz , D. Khaitan , R. Knoche , B. G. Lenardo , K. T. Lesko , J. Liao , A. Lindote , M. I. Lopes , A. Manalaysay , R. L. Mannino , M. F. Marzioni , D. N. McKinsey , D. M. Mei , J. Mock , M. Moongweluwan , J. A. Morad , A. St. J. Murphy , C. Nehrkorn , H. N. Nelson , F. Neves , K. O'Sullivan , K. C. Oliver-Mallory , K. J. Palladino , E. K. Pease , C. Rhyne , S. Shaw , T. A. Shutt , C. Silva , M. Solmaz , V. N. Solovov , P. Sorensen , T. J. Sumner , M. Szydagis , D. J. Taylor , W. C. Taylor , B. P. Tennyson , P. A. Terman , D. R. Tiedt , W. H. To , M. Tripathi , L. Tvrznikova , U. Utku , S. Uvarov , V. Velan , J. R. Verbus , R. C. Webb , J. T. White , T. J. Whitis , M. S. Witherell , F. L. H. Wolfs , J. Xu , K. Yazdani , S. K. Young , C. Zhang

Search for Light Dark Matter-Electron Scatterings in the PandaX-II Experiment

We report constraints on light dark matter through its interactions with shell electrons in the PandaX-II liquid xenon detector with a total 46.9 tonne$\cdot$day exposure. To effectively search for these very low energy electron recoils,…

High Energy Physics - Experiment · Physics 2021-05-31 Chen Cheng , Pengwei Xie , Abdusalam Abdukerim , Wei Chen , Xun Chen , Yunhua Chen , Xiangyi Cui , Yingjie Fan , Deqing Fang , Changbo Fu , Mengting Fu , Lisheng Geng , Karl Giboni , Linhui Gu , Xuyuan Guo , Ke Han , Changda He , Di Huang , Yan Huang , Yanlin Huang , Zhou Huang , Xiangdong Ji , Yonglin Ju , Shuaijie Li , Qing Lin , Huaxuan Liu , Jianglai Liu , Liqiang Liu , Xiaoying Lu , Wenbo Ma , Yugang Ma , Yajun Mao , Yue Meng , Nasir Shaheed , Kaixiang Ni , Jinhua Ning , Xuyang Ning , Xiangxiang Ren , Changsong Shang , Guofang Shen , Lin Si , Andi Tan , Anqing Wang , Hongwei Wang , Meng Wang , Qiuhong Wang , Siguang Wang , Wei Wang , Xiuli Wang , Zhou Wang , Mengmeng Wu , Shiyong Wu , Weihao Wu , Jingkai Xia , Mengjiao Xiao , Xiang Xiao , Binbin Yan , Jijun Yang , Yong Yang , Chunxu Yu , Jumin Yuan , Ying Yuan , Xinning Zeng , Dan Zhang , Tao Zhang , Li Zhao , Qibin Zheng , Jifang Zhou , Ning Zhou , Xiaopeng Zhou

Searching for Heavy Dark Matter near the Planck Mass with XENON1T

Multiple viable theoretical models predict heavy dark matter particles with a mass close to the Planck mass, a range relatively unexplored by current experimental measurements. We use 219.4 days of data collected with the XENON1T experiment…

High Energy Physics - Experiment · Physics 2023-07-06 E. Aprile , K. Abe , S. Ahmed Maouloud , L. Althueser , B. Andrieu , E. Angelino , J. R. Angevaare , V. C. Antochi , D. Antón Martin , F. Arneodo , L. Baudis , A. L. Baxter , M. Bazyk , L. Bellagamba , R. Biondi , A. Bismark , E. J. Brookes , A. Brown , S. Bruenner , G. Bruno , R. Budnik , T. K. Bui , C. Cai , J. M. R. Cardoso , D. Cichon , A. P. Cimental Chavez , M. Clark , A. P. Colijn , J. Conrad , J. J. Cuenca-García , J. P. Cussonneau , V. D'Andrea , M. P. Decowski , P. Di Gangi , S. Di Pede , S. Diglio , K. Eitel , A. Elykov , S. Farrell , A. D. Ferella , C. Ferrari , H. Fischer , M. Flierman , W. Fulgione , C. Fuselli , P. Gaemers , R. Gaior , A. Gallo Rosso , M. Galloway , F. Gao , R. Glade-Beucke , L. Grandi , J. Grigat , H. Guan , M. Guida , R. Hammann , A. Higuera , C. Hils , L. Hoetzsch , N. F. Hood , J. Howlett , M. Iacovacci , Y. Itow , J. Jakob , F. Joerg , A. Joy , N. Kato , M. Kara , P. Kavrigin , S. Kazama , M. Kobayashi , G. Koltman , A. Kopec , F. Kuger , H. Landsman , R. F. Lang , L. Levinson , I. Li , S. Li , S. Liang , S. Lindemann , M. Lindner , K. Liu , J. Loizeau , F. Lombardi , J. Long , J. A. M. Lopes , Y. Ma , C. Macolino , J. Mahlstedt , A. Mancuso , L. Manenti , F. Marignetti , T. Marrodán Undagoitia , K. Martens , J. Masbou , D. Masson , E. Masson , S. Mastroianni , M. Messina , K. Miuchi , K. Mizukoshi , A. Molinario , S. Moriyama , K. Morå , Y. Mosbacher , M. Murra , J. Müller , K. Ni , U. Oberlack , B. Paetsch , J. Palacio , Q. Pellegrini , R. Peres , C. Peters , J. Pienaar , M. Pierre , V. Pizzella , G. Plante , T. R. Pollmann , J. Qi , J. Qin , D. Ramírez García , R. Singh , L. Sanchez , J. M. F. dos Santos , I. Sarnoff , G. Sartorelli , J. Schreiner , D. Schulte , P. Schulte , H. Schulze Eißing , M. Schumann , L. Scotto Lavina , M. Selvi , F. Semeria , P. Shagin , S. Shi , E. Shockley , M. Silva , H. Simgen , A. Takeda , P. -L. Tan , A. Terliuk , D. Thers , F. Toschi , G. Trinchero , C. Tunnell , F. Tönnies , K. Valerius , G. Volta , C. Weinheimer , M. Weiss , D. Wenz , C. Wittweg , T. Wolf , V. H. S. Wu , Y. Xing , D. Xu , Z. Xu , M. Yamashita , L. Yang , J. Ye , L. Yuan , G. Zavattini , M. Zhong , T. Zhu

Underground Commissioning of LUX

LUX is a dual-phase xenon TPC designed for the direct detection of dark matter. Using 370 kg of xenon, LUX is capable of setting a WIMP-nucleon cross section limit at 2 x 10^-46 cm^2 after 300 days of running. LUX will surpass all existing…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 Michael Woods

Light Dark Matter Search with SOIPIX

We propose a light dark matter search experiment using an SOI pixel detector (SOIPIX). The event-driven SOIPIX can be a powerful tool for detecting light WIMPs because of its low energy threshold (< 1 keV) and high timing resolution (few…

Instrumentation and Detectors · Physics 2015-07-28 Naoya Oka , Kentaro Miuchi , Takeshi G. Tsuru , Ayaki Takeda , Hideaki Matsumura

Expected Sensitivity to Galactic/Solar Axions and Bosonic Super-WIMPs based on the Axio-electric Effect in Liquid Xenon Dark Matter Detectors

We present systematic case studies to investigate the sensitivity of axion searches by liquid xenon detectors, using the axio-electric effect (analogue of the photoelectric effect) on xenon atoms. Liquid xenon is widely considered to be one…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 K. Arisaka , P. Beltrame , C. Ghag , J. Kaidi , K. Lung , A. Lyashenko , R. D. Peccei , P. Smith , K. Ye

DARWIN/XLZD: a future xenon observatory for dark matter and other rare interactions

The DARWIN/XLZD experiment is a next-generation dark matter detector with a multi-ten-ton liquid xenon time projection chamber at its core. Its principal goal will be to explore the experimentally accessible parameter space for Weakly…

Instrumentation and Methods for Astrophysics · Physics 2024-05-01 Laura Baudis

A Search of Low-Mass WIMPs with p-type Point Contact Germanium Detector in the CDEX-1 Experiment

The CDEX-1 experiment conducted a search of low-mass (< 10 GeV/c2) Weakly Interacting Massive Particles (WIMPs) dark matter at the China Jinping Underground Laboratory using a p-type point-contact germanium detector with a fiducial mass of…

High Energy Physics - Experiment · Physics 2016-10-25 W. Zhao , Q. Yue , K. J. Kang , J. P. Cheng , Y. J. Li , H. T. Wong , S. T. Lin , J. P. Chang , J. H. Chen , Q. H. Chen , Y. H. Chen , Z. Deng , Q. Du , H. Gong , X. Q. Hao , H. J. He , Q. J. He , H. X. Huang , T. R. Huang , H. Jiang , H. B. Li , J. Li , J. Li , J. M. Li , X. Li , X. Y. Li , Y. L. Li , F. K. Lin , S. K. Liu , L. C. Lü , H. Ma , J. L. Ma , S. J. Mao , J. Q. Qin , J. Ren , J. Ren , X. C. Ruan , V. Sharma , M. B. Shen , L. Singh , M. K. Singh , A. K. Soma , J. Su , C. J. Tang , J. M. Wang , L. Wang , Q. Wang , S. Y. Wu , Y. C. Wu , Z. Z. Xianyu , R. Q. Xiao , H. Y. Xing , F. Z. Xu , Y. Xu , X. J. Xu , T. Xue , L. T. Yang , S. W. Yang , N. Yi , C. X. Yu , H. Yu , X. Z. Yu , M. Zeng , X. H. Zeng , Z. Zeng , L. Zhang , Y. H. Zhang , M. G. Zhao , Z. Y. Zhou , J. J. Zhu , W. B. Zhu , X. Z. Zhu , Z. H. Zhu

Limits on light WIMPs with a germanium detector at 177 eVee threshold at the China Jinping Underground Laboratory

The China Dark Matter Experiment reports results on light WIMP dark matter searches at the China Jinping Underground Laboratory with a germanium detector array with a total mass of 20 g. The physics threshold achieved is 177 eVee ("ee"…

High Energy Physics - Experiment · Physics 2014-08-20 S. K. Liu , Q. Yue , K. J. Kang , J. P. Cheng , H. T. Wong , Y. J. Li , S. T. Lin , J. P. Chang , N. Chen , Q. H. Chen , Y. H. Chen , Y. C. Chuang , Z. Deng , Q. Du , H. Gong , X. Q. Hao , H. J. He , Q. J. He , H. X. Huang , T. R. Huang , H. Jiang , H. B. Li , J. M. Li , J. Li , J. Li , X. Li , X. Q. Li , X. Y. Li , Y. L. Li , H. Y. Liao , F. K. Lin , L. C. Lü , H. Ma , S. J. Mao , J. Q. Qin , J. Ren , J. Ren , X. C. Ruan , M. B. Shen , L. Singh , M. K. Singh , A. K. Soma , J. Su , C. J. Tang , C. H. Tseng , J. M. Wang , L. Wang , Q. Wang , S. Y. Wu , Y. C. Wu , Y. C. Wu , Z. Z. Xianyu , R. Q. Xiao , H. Y. Xing , F. Z. Xu , Y. Xu , X. J. Xu , T. Xue , C. W. Yang , L. T. Yang , S. W. Yang , N. Yi , C. X. Yu , H. Yu , X. Z. Yu , X. H. Zeng , Z. Zeng , L. Zhang , Y. H. Zhang , M. G. Zhao , W. Zhao , Z. Y. Zhou , J. J. Zhu , W. B. Zhu , X. Z. Zhu , Z. H. Zhu

New Measurement of the Relative Scintillation Efficiency of Xenon Nuclear Recoils Below 10 keV

Liquid xenon is an important detection medium in direct dark matter experiments, which search for low-energy nuclear recoils produced by the elastic scattering of WIMPs with quarks. The two existing measurements of the relative…

Astrophysics · Physics 2010-05-19 E. Aprile , L. Baudis , B. Choi , K. L. Giboni , K. E. Lim , A. Manalaysay , M. E. Monzani , G. Plante , R. Santorelli , M. Yamashita

The BDX-MINI detector for Light Dark Matter search at JLab

This paper describes the design and performance of a compact detector, BDX-MINI, that incorporates all features of a concept that optimized the detection of light dark matter produced by electrons in a beam dump. It represents a reduced…

Instrumentation and Detectors · Physics 2021-03-17 M. Battaglieri , P. Bisio , M. Bondí , A. Celentano , P. L. Cole , M. De Napoli , R. De Vita , L. Marsicano , G. Ottonello , F. Parodi , N. Randazzo , E. S. Smith , D. Snowden-Ifft , M. Spreafico , T. Whitlatch , M. H. Wood

Constraints on low-mass WIMPs from the EDELWEISS-III dark matter search

We present the results of a search for elastic scattering from galactic dark matter in the form of Weakly Interacting Massive Particles (WIMPs) in the 4-30 GeV/$c^2$ mass range. We make use of a 582 kg-day fiducial exposure from an array of…

Cosmology and Nongalactic Astrophysics · Physics 2016-05-10 EDELWEISS Collaboration , E. Armengaud , Q. Arnaud , C. Augier , A. Benoît , A. Benoît , L. Bergé , T. Bergmann , J. Billard , J. Blümer , T. de Boissière , G. Bres , A. Broniatowski , V. Brudanin , P. Camus , A. Cazes , M. Chapellier , F. Charlieux , L. Dumoulin , K. Eitel , D. Filosofov , N. Foerster , N. Fourches , G. Garde , J. Gascon , G. Gerbier , A. Giuliani , M. Grollier , M. Gros , L. Hehn , S. Hervé , G. Heuermann , V. Humbert , M. De Jésus , Y. Jin , S. Jokisch , A. Juillard , C. Kéfélian , M. Kleifges , V. Kozlov , H. Kraus , V. A. Kudryavtsev , H. Le-Sueur , J. Lin , M. Mancuso , S. Marnieros , A. Menshikov , X. -F. Navick , C. Nones , E. Olivieri , P. Pari , B. Paul , M. -C. Piro , D. V. Poda , E. Queguiner , M. Robinson , H. Rodenas , S. Rozov , V. Sanglard , B. Schmidt , S. Scorza , B. Siebenborn , D. Tcherniakhovski , L. Vagneron , M. Weber , E. Yakushev , X. Zhang

Exclusion limits on the WIMP-nucleon cross-section from the Cryogenic Dark Matter Search

The Cryogenic Dark Matter Search (CDMS) employs low-temperature Ge and Si detectors to search for Weakly Interacting Massive Particles (WIMPs) via their elastic-scattering interactions with nuclei while discriminating against interactions…

Astrophysics · Physics 2012-08-27 CDMS Collaboration

Low Mass WIMP Searches with a Neutrino Experiment: A Proposal for Further MiniBooNE Running

A proposal submitted to the FNAL PAC is described to search for light sub-GeV WIMP dark matter at MiniBooNE. The possibility to steer the beam past the target and into an absorber leads to a significant reduction in neutrino background,…

High Energy Physics - Experiment · Physics 2012-11-14 A. A. Aguilar-Arevalo , B. Batell , R. Cooper , P. deNiverville , R. Dharmapalan , Z. Djurcic , R. Ford , F. G. Garcia , G. T. Garvey , J. Grange , S. Habib , W. Huelsnitz , C. Jiang , R. A. Johnson , W. Ketchum , T. Kobilarcik , W. C. Louis , W. Marsh , D. McKeen , G. B. Mills , J. Mirabal , C. D. Moore , P. Nienaber , Z. Pavlovic , D. Perevalov , C. C. Polly , M. Pospelov , H. Ray , A. Ritz , B. P. Roe , I. Stancu , R. Tayloe R. Van de Water , D. A. Wickremasinghe

Dark matter search by exclusive studies of X-rays following WIMPs nuclear interactions

It is shown that weakly interacting massive particles (WIMPs), which are possible cold dark matter candidates, can be studied by exclusive measurements of X-rays following WIMPs nuclear interactions. Inner-shell atomic electrons are ionized…

High Energy Physics - Phenomenology · Physics 2009-11-11 H. Ejiri , Ch. C. Moustakidis , J. D. Vergados

First dark matter search results from the PandaX-I experiment

We report on the first dark-matter (DM) search results from PandaX-I, a low threshold dual-phase xenon experiment operating at the China Jinping Underground Laboratory. In the 37-kg liquid xenon target with 17.4 live-days of exposure, no DM…

High Energy Physics - Experiment · Physics 2014-09-05 PandaX Collaboration , Mengjiao Xiao , Xiang Xiao , Li Zhao , Xiguang Cao , Xun Chen , Yunhua Chen , Xiangyi Cui , Deqing Fang , Changbo Fu , Karl L. Giboni , Haowei Gong , Guodong Guo , Jie Hu , Xingtao Huang , Xiangdong Ji , Yonglin Ju , Siao Lei , Shaoli Li , Qing Lin , Huaxuan Liu , Jianglai Liu , Xiang Liu , Wolfgang Lorenzon , Yugang Ma , Yajun Mao , Kaixuan Ni , Kirill Pushkin , Xiangxiang Ren , Michael Schubnell , Manbing Shen , Scott Stephenson , Andi Tan , Greg Tarle , Hongwei Wang , Jimin Wang , Meng Wang , Xuming Wang , Zhou Wang , Yuehuan Wei , Shiyong Wu , Pengwei Xie , Yinghui You , Xionghui Zeng , Hua Zhang , Tao Zhang , Zhonghua Zhu

Identification of Radiopure Titanium for the LZ Dark Matter Experiment and Future Rare Event Searches

The LUX-ZEPLIN (LZ) experiment will search for dark matter particle interactions with a detector containing a total of 10 tonnes of liquid xenon within a double-vessel cryostat. The large mass and proximity of the cryostat to the active…

Instrumentation and Detectors · Physics 2017-09-28 D. S. Akerib , C. W. Akerlof , D. Yu. Akimov , S. K. Alsum , H. M. Araújo , I. J. Arnquist , M. Arthurs , X. Bai , A. J. Bailey , J. Balajthy , S. Balashov , M. J. Barry , J. Belle , P. Beltrame , T. Benson , E. P. Bernard , A. Bernstein , T. P. Biesiadzinski , K. E. Boast , A. Bolozdynya , B. Boxer , R. Bramante , P. Brás , J. H. Buckley , V. V. Bugaev , R. Bunker , S. Burdin , J. K. Busenitz , C. Carels , D. L. Carlsmith , B. Carlson , M. C. Carmona-Benitez , C. Chan , J. J. Cherwinka , A. A. Chiller , C. Chiller , A. Cottle , R. Coughlen , W. W. Craddock , A. Currie , C. E. Dahl , T. J. R. Davison , A. Dobi , J. E. Y. Dobson , E. Druszkiewicz , T. K. Edberg , W. R. Edwards , W. T. Emmet , C. H. Faham , S. Fiorucci , T. Fruth , R. J. Gaitskell , N. J. Gantos , V. M. Gehman , R. M. Gerhard , C. Ghag , M. G. D. Gilchriese , B. Gomber , C. R. Hall , S. Hans , K. Hanzel , S. J. Haselschwardt , S. A. Hertel , S. Hillbrand , C. Hjemfelt , M. D. Hoff , B. Holbrook , E. Holtom , E. W. Hoppe , J. Y-K. Hor , M. Horn , D. Q. Huang , T. W. Hurteau , C. M. Ignarra , R. G. Jacobsen , W. Ji , A. Kaboth , K. Kamdin , K. Kazkaz , D. Khaitan , A. Khazov , A. V. Khromov , A. M. Konovalov , E. V. Korolkova , M. Koyuncu , H. Kraus , H. J. Krebs , V. A. Kudryavtsev , A. V. Kumpan , S. Kyre , C. Lee , H. S. Lee , J. Lee , D. S. Leonard , R. Leonard , K. T. Lesko , C. Levy , F. -T. Liao , J. Lin , A. Lindote , R. E. Linehan , W. H. Lippincott , X. Liu , M. I. Lopes , B. Lopez Paredes , W. Lorenzon , S. Luitz , P. Majewski , A. Manalaysay , L. Manenti , R. L. Mannino , D. J. Markley , T. J. Martin , M. F. Marzioni , C. T. McConnell , D. N. McKinsey , D. -M. Mei , Y. Meng , E. H. Miller , E. Mizrachi , J. Mock , M. E. Monzani , J. A. Morad , B. J. Mount , A. St. J. Murphy , C. Nehrkorn , H. N. Nelson , F. Neves , J. A. Nikkel , J. O'Dell , K. O'Sullivan , I. Olcina , M. A. Olevitch , K. C. Oliver-Mallory , K. J. Palladino , E. K. Pease , A. Piepke , S. Powell , R. M. Preece , K. Pushkin , B. N. Ratcliff , J. Reichenbacher , L. Reichhart , C. A. Rhyne , A. Richards , J. P. Rodrigues , H. J. Rose , R. Rosero , P. Rossiter , J. S. Saba , M. Sarychev , R. W. Schnee , M. Schubnell , P. R. Scovell , S. Shaw , T. A. Shutt , C. Silva , K. Skarpaas , W. Skulski , M. Solmaz , V. N. Solovov , P. Sorensen , V. V. Sosnovtsev , I. Stancu , M. R. Stark , S. Stephenson , T. M. Stiegler , K. Stifter , T. J. Sumner , M. Szydagis , D. J. Taylor , W. C. Taylor , D. Temples , P. A. Terman , K. J. Thomas , J. A. Thomson , D. R. Tiedt , M. Timalsina , W. H. To , A. Tomás , T. E. Tope , M. Tripathi , L. Tvrznikova , J. Va'vra , A. Vacheret , M. G. D. van der Grinten , J. R. Verbus , C. O. Vuosalo , W. L. Waldron , R. Wang , R. Watson , R. C. Webb , W. -Z. Wei , M. While , D. T. White , T. J. Whitis , W. J. Wisniewski , M. S. Witherell , F. L. H. Wolfs , D. Woodward , S. Worm , J. Xu , M. Yeh , J. Yin , C. Zhang