U Texas
12 Papers
1 Citations
U Texas is an academic researcher. The author has contributed to research in topics: Computer science & Muon collider. The author has an hindex of 2, co-authored 4 publications.
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Papers
Design and simulated performance of calorimetry systems for the ECCE detector at the electron ion collider
F. Bock,Neslihan Becerici Schmidt,P. K. Wang,N. Santiesteban,T. Horn,J. Huang,J. G. Lajoie,C. M. Camacho,J. K. Adkins,Y. Akiba,Areej Albataineh,M. J. Amaryan,Ionut Christian Arsene,C. Ayerbe Gayoso,J. B. Bae,Xinzhan Bai,M. D. Baker,M. Bashkanov,R. Bellwied,Fatiha Benmokhtar,V. V. Berdnikov,Jan C. Bernauer,W. U. Boeglin,M. Borysova,E. J. Brash,P. Brindza,W. J. Briscoe,M. L. Brooks,S. Bueltmann,Masroor H. S. Bukhari,Alexander Bylinkin,R. Capobianco,W. C. Chang,Yongjin Cheon,K. X. Chen,Kai-yu Cheng,M. Chiu,Tatsuya Chujo,Zvi Hirsh Citron,Ethan Cline,E.O. Cohen,Thomas Michael Cormier,Y. Corrales Morales,Chandler W. Cotton,J. Crafts,Christopher Crawford,S. Creekmore,C.Cuevas,J. Cunningham,G. David,Charles Thomas Dean,M. Demarteau,S. Diehl,Norihiro Doshita,R. Dupre,John Matthew Durham,R. Dzhygadlo,Raymond James Ehlers,L. El Fassi,Alex R. Emmert,Rolf Ent,C. Fanelli,R. Fatemi,S. Fegan,M. Finger,J. E. Frantz,Manfred Friedman,Ivica Friščić,D. R. Gangadharan,S. Gardner,K. Gates,F. J.M. Geurts,R. Gilman,D. I. Glazier,E. Glimos,Y. Goto,N. Grau,Stacie Greene,A. Q. Guo,L. Guo,Sung-Kee Ha,J. S. Haggerty,T. B. Hayward,X. C. He,Or Hen,Douglas Higinbotham,M. Hoballah,A. Hoghmrtsyan,P. Hsu,G. M. Huber,Alek Hutson,Kyung-Yup Hwang,C. E. Hyde,M. Inaba,T. Iwata,H. S. Jo,K. S. Joo,N. Kalantarians,G. Kalicy,Kiyoshi Kawade,S. Kay,A. Kim,B. Kim,C. O. Kim,M. Kim,Y. Kim,E. Kistenev,V. G. Klimenko,S. Ko,I. Korover,Wolfgang Korsch,Georgios Krintiras,S. E. Kuhn,C.M. Kuo,T. Kutz,David J. Lawrence,S. Lebedev,H. Lee,J. S. H. Lee,S. W. Lee,Y. Lee,W. Li,W. Li,X. Li,Y. F. Liang,S. Lim,C. Lin,Da Xien Lin,K. Liu,M. X. Liu,K. Livingston,Nilanga Liyanage,W. J. Llope,Constantinos Loizides,E. Long,R Rongguo Lu,Z. Lu,W. A. Lynch,Swarna P. Mantry,D. Marchand,Michal Marcisovsky,Christina Markert,Pete Markowitz,H. Marukyan,P. L. McGaughey,M. Mihovilovic,Ross Milner,Alexander Milov,Yoshiki Miyachi,H. Mkrtchyan,P. Monaghan,R. A. Montgomery,D. P. Morrison,A. Movsisyan,Michael Murray,Kiyoshi Nagai,J. L. Nagle,I. Nakagawa,Christine Nattrass,D. Nguyen,S. Niccolai,Rachid Nouicer,G. Nukazuka,M. Nycz,V. A. Okorokov,Susan Oresic,J. D. Osborn,C.O’. Shaughnessy,S. Paganis,Z. Papandreou,S. F. Pate,M. Patel,Christoph Paus,G. G. Penman,M. Grosse Perdekamp,Dennis Perepelitsa,H. Pereira Da Costa,K. Peters,W. Phelps,E. Piasetzky,C. Pinkenburg,I. Prochazka,T. F. Protzman,Martin Purschke,J. Putschke,J.R. Pybus,Renuka Rajput-Ghoshal,J. Rasson,Brian Raue,Kenneth Francis Read,Ketil Røed,Rolf K. Reed,Joerg Reinhold,E. Renner,James Canton Richards,C. Riedl,Timothy Thomas Rinn,J. Roche,Gunther Roland,Guy Ron,M. Rosati,Christophe Royon,J.H. Ryu,Sevil Salur,R. Santos,M. Sarsour,J. Schambach,A. Schmidt,Cornelius Schwarz,J. Schwiening,R. Seidl,Anne Marie Sickles,Paul Simmerling,Simon Širca,D. Sharma,Zhifeng Shi,T. A. Shibata,C. W. Shih,S Shimizu,U. Shrestha,Karl Slifer,K. Smith,D. Sokhan,R. A. Soltz,W. E. Sondheim,J. Song,I. I. Strakovsky,P. Steinberg,P.V. Stepanov,Justin Stevens,J. Strube,P. Sun,X Sun,K. Suresh,V. Tadevosyan,W. Tang,S. Araya,S. Tarafdar,Liliana Teodorescu,Deloris S. Thomas,Anthony Robert Timmins,L. Tomášek,Nikita Trotta,Richard Trotta,Trine Spedstad Tveter,Ejiro Naomi Umaka,A. Usman,H. W. Van Hecke,C. B. Van Hulse,Julia Velkovska,E. Voutier,Q. Wang,Yu Wang,D. P. Watts,N. Wickramaarachchi,Larry Weinstein,Mark Ian Williams,C.P. Wong,L. Wood,M. Wood,C. L. Woody,Boleslaw Wyslouch,Z.G. Xiao,Yasunori Yamazaki,Y. Yang,Z. Ye,H. Yoo,M. Yurov,Nicholas Zachariou,W. A. Zajc,W. Zha,J.-L. Zhang,J.X. Zhang,Yi Zhang,Y. Zhao,Yerevan,Armenia,Institute of Applied Physics,A. Sinica,Taipei,Taiwan,A. University,Sioux Falls,Sd,Usa,Ben-Gurion University of the Negev Beer-Sheva,Israel,B. N. Laboratory,Upton,Ny,Usa University College London,Uxbridge,Uk,Canisius College,Buffalo,Central China Normal University,Wuhan,China.,Charles University,Prague,Czech Republic,China China Institute of Atomic Energy,Fangshan,Beijing,Christopher Newport University,Newport News,Va,C. University,N. York,Catholic University of America,Dc Washington,Czech Technical University,Duquesne University,Pittsburgh,Pa,D. University,N. Durham,Florida International University,Miami,Fl,Georgia State University,Atlanta,Ga,U Glasgow,Glasgow,Gsi GmbH,Darmstadt,Germany,The George Washington University,Washington,Dc,H. University,Hampton,Hebrew University,Jerusalem,Isreal,U. Paris-Saclay,CNRSIN2p3,IJCLab,Orsay,France.,Irfu,Cea,Gif-sur-Yvette France,Chinese Academy of Sciences,Lanzhou,I. S. University,Iowa City,Ia,J. University,Jazan,Sadui Arabia,Thomas Jefferson National Accelerator Facility,James Madison University,Harrisonburg,K. University,Kobe,Japan.,Kyungpook National University,Daegu,R Korea,Los Alamos National Laboratory,L. Alamos,Nm,Lawrence Berkeley National Lab.,Berkeley,Ca,Lehigh University,Bethlehem,L. Laboratory,Livermore,Morehead State University,Morehead,Ky,M. I. O. Technology,Cambridge,Ma,M. S. University,Mississippi State,Mš,National Cheng Kung University,Tainan,National Central University,Chungli,Nihon University,Tokyo,N. University,Las Cruces,National Research Nuclear University MEPhI,Moscow,Russian Federation,Nuclear Research Center - Negev,Beer-Sheva,National Tsing Hua University,Hsinchu,National Taiwan Normal University,Old Dominion University,Norfolk,Ohio University,Athens,Oh,Oak Ridge National Laboratory,Oak Ridge,Tn,P. N. N. Laboratory,Richland,Wa,Pusan National University,Busan,R. University,Houston,Tx,Riken Nishina Center,Wako,Saitama,The State University of New Jersey,Piscataway,Nj,Center for Space Science,S. Brook,S. B. University,RIKEN-BNL Research Center,Shandong Qingdao,Shandong,Seoul National University,Seoul,Sejong University,S. University,Matsumoto,Nagano,S. University,Suwon,T. University,Tel Aviv,U. O. Science,Technology of China,Hefei,China Tsinghua University,Tsukuba University of Technology,Tsukuba,Ibaraki,U. C. A. Boulder,Boulder,Co,U. Connecticut,Storrs,Ct,Universityof Georgia,GA Dahlonega,U. Houston,U. Illinois,Urbana,Il,Unviersity of Kansas,Lawrence,Ks,U Kentucky,Lexington,U Ljubljana,Ljubljana,Slovenia,University of New Hampshire,Durham,Nh,Universityof Oslo,Oslo,Norway,U. O. Regina,Regina,Sk,Canada,University of Seoul,U Tsukuba,U Texas,Austin,Texas,U Tennessee,Knoxville,U Virginia,Charlottesville,V. University,Nashville,V. Tech,Blacksburg,Virginia Union University,Richmond,Wayne State University,Detroit,Mi,Weizmann Institute of Science,Rehovot,T William,Mary,Williamsburg,Y. University,Yamagata,Yarmouk University,Irbid,Jordan,Y. University,University of York,York,University of Zagreb,Zagreb,Croatia +504 more
Abstract: We describe the design and performance the calorimeter systems used in the ECCE detector design to achieve the overall performance specifications cost-effectively with careful consideration of appropriate technical and schedule risks. The calorimeter systems consist of three electromagnetic calorimeters, covering the combined pseudorapdity range from -3.7 to 3.8 and two hadronic calorimeters. Key calorimeter performances which include energy and position resolutions, reconstruction efficiency, and particle identification will be presented.
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The universal shape of the X-ray variability power spectrum of AGN up to z~3
Maurizio Paolillo,I. E. Papadakis,W. N. Brandt,Franz E. Bauer,Giorgio Lanzuisi,Viola Allevato,Ohad Shemmer,X. C. Zheng,D. De Cicco,Roberto Gilli,Bin Luo,M. Thomas,Paolo Tozzi,Fabio Vito,Y. Q. X. D. D. F. Pancini'',U. Federico,Italy.,I. A. D. Capodimonte,Naples,Infn -- Unita di Napoli,D. Physics,Institute of Theoretical,C. Physics,Universityof Crete,Heraklion,Greece,Institute of Astrophysics,Forth,D. Astronomy,Astrophysics,T. O. S. University,University Park,USA.,Institute for Gravitation,The Cosmos,Instituto de Astrof'isica,Centro de Astroingenier'ia,Facultad de F'isica,P. U. C. D. Chile,Santiago,Chile,Millennium Institute of Astrophysics,S. S. Institute,Boulder,Colorado.,I. A. D. Bologna,Scuola normale superiore,Pisa,U Texas,Denton,L. Observatory,Leiden University,Leiden,The Netherlands.,School of Astronomy,S. Science,N. University,China.,Key Laboratory of Optical Astronomy,I. Arcetri,Firenze,Cas Key Laboratory for Research in Galaxies,Cosmology,U. O. Science,Technology of China,Hefei,S. Sciences +66 more
- 16 Feb 2023
TL;DR: In this paper , the ensemble X-ray variability properties of active galactic nuclei (AGN) over a large range of timescales (20 ks, T + 14 yrs), redshift, luminosity, and BH masses were studied.
SDSS spectroscopic survey of stars
Zeljko Ivezic,David J. Schlegel,A. Uomoto,Nicholas A. Bond,Timothy C. Beers,C. Allende Prieto,R. Wilhelm,Y. Sun Lee,T. Sivarani,Mario Juric,Robert H. Lupton,Berkeley Lbl,U Princeton,U Texas,Texas Tech.,Santa Cruz Uc,Flagstaff Naval Observ.,U Drexel +17 more
- 01 Jan 2007
TL;DR: In this paper, the authors show that stellar parameters, such as effective temperature, gravity and metallicity from SDSS spectra, show a good correlation with the position of a star in the g-r vs. u-g color-color diagram, thereby demonstrating their robustness and potential for photometric parameter estimation methods.
TA-RNN: an Attention-based Time-aware Recurrent Neural Network Architecture for Electronic Health Records
Mohammad Al Olaimat,Serdar Bozdag,the Alzheimer's Disease Neuroimaging Initiative Dept. Science,Engineering,U Texas,Denton,Usa,Dept . o f Mathematics,BioDiscovery Institute +8 more
TL;DR: This study proposes two interpretable DL architectures based on RNN, namely Time-Aware RNN (TA-RNN) and TA-RNN-Autoencoder (TA-RNN-AE) to predict patient's clinical outcome in EHR at next visit and multiple visits ahead, respectively.
1
Studies of beam heating of proton beam profile monitor SEM's
Z. Pavlovich,Thomas H. Osiecki,Sacha E Kopp,U Texas +3 more
- 01 May 2005
TL;DR: In this paper, the expected temperature rise of proton beam profile monitors due to beam heating is studied. But the authors only consider the NuMI beam, where the per-pulse intensity is quite high; for completeness the calculations are also performed for other beam energies and intensities.