Matthew Szydagis
University at Albany, SUNY
120 Papers
724 Citations
Matthew Szydagis is an academic researcher from University at Albany, SUNY. The author has contributed to research in topics: Dark matter & Xenon. The author has an hindex of 32, co-authored 90 publications. Previous affiliations of Matthew Szydagis include University of California, Davis & State University of New York System.
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Papers
Extending light WIMP searches to single scintillation photons in LUX
D. S. Akerib,S. Alsum,Henrique Araujo,X. Bai,J. Balajthy,A. Baxter,P. Beltrame,Ethan Bernard,Adam Bernstein,T. P. Biesiadzinski,E. M. Boulton,B. Boxer,P. Brás,Sergey Burdin,D. Byram,M. C. Carmona-Benitez,C. Chan,J. E. Cutter,L. de Viveiros,E. Druszkiewicz,S. R. Fallon,A. Fan,S. Fiorucci,R. J. Gaitskell,J. Genovesi,C. Ghag,M. G. D. Gilchriese,Carl Gwilliam,C. R. Hall,S. J. Haselschwardt,S. A. Hertel,D. P. Hogan,M. Horn,D. Q. Huang,C. M. Ignarra,R. G. Jacobsen,O. Jahangir,W. Ji,K. Kamdin,K. Kazkaz,D. Khaitan,Elena Korolkova,S. Kravitz,V. A. Kudryavtsev,E. Leason,B. G. Lenardo,K. T. Lesko,J. Liao,J. Lin,A. Lindote,M.I. Lopes,B. Lopez Paredes,A. Manalaysay,R. L. Mannino,N. Marangou,M. F. Marzioni,Daniel McKinsey,Dongming Mei,M. Moongweluwan,J. A. Morad,A. St. J. Murphy,A. Naylor,C. Nehrkorn,H. N. Nelson,F. Neves,A. Nilima,K. C. Oliver-Mallory,K. J. Palladino,E. K. Pease,Q. Riffard,G. R. C. Rischbieter,C. Rhyne,P. Rossiter,S. Shaw,T. A. Shutt,Catarina Silva,M. Solmaz,V. N. Solovov,P. Sorensen,T. J. Sumner,Matthew Szydagis,D. J. Taylor,Robert A. Taylor,W. C. Taylor,B. P. Tennyson,P. A. Terman,D. R. Tiedt,W. H. To,Mani Tripathi,L. Tvrznikova,U. Utku,S. Uvarov,Antonin Vacheret,V. Velan,R. C. Webb,J. T. White,T. J. Whitis,Michael S. Witherell,F. L. H. Wolfs,D. Woodward,Jilei Xu,Chao Zhang +101 more
TL;DR: In this paper, the authors exploit the double photoelectron emission effect observed in some photomultiplier models at vacuum ultraviolet wavelengths to lower the energy threshold of liquid xenon time projection chambers.
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Position reconstruction in LUX
D. S. Akerib,D. S. Akerib,D. S. Akerib,S. Alsum,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,P. Beltrame,Ethan Bernard,Ethan Bernard,Adam Bernstein,T. P. Biesiadzinski,T. P. Biesiadzinski,T. P. Biesiadzinski,E. M. Boulton,E. M. Boulton,P. Brás,D. Byram,Sidney Cahn,M. C. Carmona-Benitez,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,A. Fan,S. Fiorucci,S. Fiorucci,R. J. Gaitskell,J. Genovesi,C. Ghag,M. G. D. Gilchriese,C. R. Hall,M. Hanhardt,S. J. Haselschwardt,S. A. Hertel,S. A. Hertel,S. A. Hertel,D. P. Hogan,M. Horn,M. Horn,D. Q. Huang,C. M. Ignarra,C. M. Ignarra,R. G. Jacobsen,W. Ji,W. Ji,W. Ji,K. Kamdin,Kareem Kazkaz,D. Khaitan,R. Knoche,N. A. Larsen,B. G. Lenardo,B. G. Lenardo,K. T. Lesko,A. Lindote,M.I. Lopes,A. Manalaysay,R. L. Mannino,R. L. Mannino,M. F. Marzioni,Daniel McKinsey,Daniel McKinsey,Daniel McKinsey,Dongming Mei,J. Mock,M. Moongweluwan,J. A. Morad,A. St. J. Murphy,C. Nehrkorn,H. N. Nelson,F. Neves,K. O’Sullivan,K. O’Sullivan,K. O’Sullivan,K. C. Oliver-Mallory,K. J. Palladino,K. J. Palladino,K. J. Palladino,E. K. Pease,E. K. Pease,C. Rhyne,S. Shaw,S. Shaw,T. A. Shutt,T. A. Shutt,C. Silva,M. Solmaz,V. N. Solovov,P. Sorensen,T. J. Sumner,Matthew Szydagis,D. J. Taylor,W. C. Taylor,B. P. Tennyson,P. A. Terman,D. R. Tiedt,W. H. To,W. H. To,W. H. To,Mani Tripathi,L. Tvrznikova,L. Tvrznikova,L. Tvrznikova,S. Uvarov,V. Velan,J.R. Verbus,R. C. Webb,J. T. White,T. J. Whitis,T. J. Whitis,T. J. Whitis,M. S. Witherell,F.L.H. Wolfs,Jilei Xu,K. Yazdani,Sarah Young,Chao Zhang +124 more
TL;DR: In this article, the (x, y) position reconstruction method used in the analysis of the complete exposure of the Large Underground Xenon (LUX) experiment is presented, based on a statistical test that makes use of an iterative method to recover the photomultiplier tube (PMT) light response directly from the calibration data.
Liquid xenon scintillation measurements and pulse shape discrimination in the LUX dark matter detector
D. S. Akerib,S. Alsum,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,P. Beltrame,Ethan Bernard,Adam 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,Blair Edwards,S. R. Fallon,A. Fan,S. Fiorucci,R. J. Gaitskell,J. Genovesi,C. Ghag,Murdock 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,Daniel McKinsey,Dongming 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,Catarina Silva,M. Solmaz,V. N. Solovov,P. Sorensen,T. J. Sumner,Matthew Szydagis,D. J. Taylor,W. C. Taylor,B. P. Tennyson,P. A. Terman,D. R. Tiedt,W. H. To,Mani Tripathi,L. Tvrznikova,U. Utku,S. Uvarov,V. Velan,J.R. Verbus,R. C. Webb,J. T. White,T. J. Whitis,Michael S. Witherell,F. L. H. Wolfs,Jilei Xu,K. Yazdani,Sarah Young,Chao Zhang +91 more
TL;DR: In this article, the authors measured a singlet-to-triplet scintillation ratio for electron recoils (ER) in the LUX WIMP detector.
•Posted Content
The Present and Future of Searching for Dark Matter with LUX and LZ
TL;DR: The LUX detector achieved a maximal spin-independent 90% C.L. limit of 2 x 10^-46 cm^2 at 50 GeV/c^2 for its 332 live-day run as discussed by the authors.
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