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Insertion of STC into TRT at the Department of Physics, Oxford
Credit: CERN

Dr. Kimberly Palladino

Associate Professor

Sub department

  • Particle Physics

Research groups

  • LUX-ZEPLIN
kimberly.palladino@physics.ox.ac.uk
Telephone: 273301
Denys Wilkinson Building, room 622
  • About
  • Publications

LUX-ZEPLIN (LZ) Conceptual Design Report

(2015)

Authors:

The LZ Collaboration, DS Akerib, CW Akerlof, D Yu Akimov, SK Alsum, HM Araújo, X Bai, AJ Bailey, J Balajthy, S Balashov, MJ Barry, P Bauer, P Beltrame, EP Bernard, A Bernstein, TP Biesiadzinski, KE Boast, AI Bolozdynya, EM Boulton, R Bramante, JH Buckley, VV Bugaev, R Bunker, S Burdin, JK Busenitz, C Carels, DL Carlsmith, B Carlson, MC Carmona-Benitez, M Cascella, C Chan, JJ Cherwinka, AA Chiller, C Chiller, WW Craddock, A Currie, JE Cutter, JP da Cunha, CE Dahl, S Dasu, TJR Davison, L de Viveiros, A Dobi, JEY Dobson, E Druszkiewicz, TK Edberg, BN Edwards, WR Edwards, MM Elnimr, WT Emmet, CH Faham, S Fiorucci, P Ford, VB Francis, C Fu, RJ Gaitskell, NJ Gantos, VM Gehman, RM Gerhard, C Ghag, MGD Gilchriese, B Gomber, CR Hall, A Harris, SJ Haselschwardt, SA Hertel, MD Hoff, B Holbrook, E Holtom, DQ Huang, TW Hurteau, CM Ignarra, RG Jacobsen, W Ji, X Ji, M Johnson, Y Ju, K Kamdin, K Kazkaz, D Khaitan, A Khazov, AV Khromov, AM Konovalov, EV Korolkova, H Kraus, HJ Krebs, VA Kudryavtsev, AV Kumpan, S Kyre, NA Larsen, C Lee, BG Lenardo, KT Lesko, F-T Liao, J Lin, A Lindote, WH Lippincott, J Liu, X Liu, MI Lopes, W Lorenzon, S Luitz, P Majewski, DC Malling, AG Manalaysay, L Manenti, RL Mannino, DJ Markley, TJ Martin, MF Marzioni, DN McKinsey, D-M Mei, Y Meng, EH Miller, J Mock, ME Monzani, JA Morad, A St J Murphy, HN Nelson, F Neves, JA Nikkel, FG O'Neill, J O'Dell, K O'Sullivan, MA Olevitch, KC Oliver-Mallory, KJ Palladino, M Pangilinan, SJ Patton, EK Pease, A Piepke, S Powell, RM Preece, K Pushkin, BN Ratcliff, J Reichenbacher, L Reichhart, C Rhyne, JP Rodrigues, HJ Rose, R Rosero, JS Saba, M Sarychev, RW Schnee, MSG Schubnell, PR Scovell, S Shaw, TA Shutt, C Silva, K Skarpaas, W Skulski, VN Solovov, P Sorensen, VV Sosnovtsev, I Stancu, MR Stark, S Stephenson, TM Stiegler, TJ Sumner, K Sundarnath, M Szydagis, DJ Taylor, W Taylor, BP Tennyson, PA Terman, KJ Thomas, JA Thomson, DR Tiedt, WH To, A Tomás, M Tripathi, CE Tull, L Tvrznikova, S Uvarov, J Va'vra, MGD van der Grinten, JR Verbus, CO Vuosalo, WL Waldron, L Wang, RC Webb, W-Z Wei, M While, DT White, TJ Whitis, WJ Wisniewski, MS Witherell, FLH Wolfs, E Woods, D Woodward, SD Worm, M Yeh, J Yin, SK Young, C Zhang
More details from the publisher
Details from ArXiV

Energy and Flux Measurements of Ultra-High Energy Cosmic Rays Observed During the First ANITA Flight

(2015)

Authors:

H Schoorlemmer, K Belov, A Romero-Wolf, D García-Fernández, V Bugaev, SA Wissel, P Allison, J Alvarez-Muñiz, SW Barwick, JJ Beatty, DZ Besson, WR Binns, WR Carvalho, C Chen, P Chen, JM Clem, A Connolly, PF Dowkontt, MA DuVernois, RC Field, D Goldstein, PW Gorham, C Hast, CL Heber, T Huege, S Hoover, MH Israel, A Javaid, J Kowalski, J Lam, JG Learned, KM Liewer, JT Link, E Lusczek, S Matsuno, BC Mercurio, C Miki, P Miočinović, K Mulrey, J Nam, CJ Naudet, J Ng, RJ Nichol, K Palladino, BF Rauch, J Roberts, K Reil, B Rotter, M Rosen, L Ruckman, D Saltzberg, D Seckel, D Urdaneta, GS Varner, AG Vieregg, D Walz, F Wu, E Zas
More details from the publisher

Design of the MiniCLEAN dark matter search veto detector subsystem

Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment Elsevier 781 (2015) 78-85

Authors:

Robert Abruzzio, Benjamin Buck, Stephen Jaditz, James Kelsey, Jocelyn Monroe, Kimberly Palladino
More details from the publisher
More details
Details from ArXiV

Improving photoelectron counting and particle identification in scintillation detectors with Bayesian techniques

Astroparticle Physics Elsevier 65 (2015) 40-54

Authors:

M Akashi-Ronquest, P-A Amaudruz, M Batygov, B Beltran, M Bodmer, MG Boulay, B Broerman, B Buck, A Butcher, B Cai, T Caldwell, M Chen, Y Chen, B Cleveland, K Coakley, K Dering, FA Duncan, JA Formaggio, R Gagnon, D Gastler, F Giuliani, M Gold, VV Golovko, P Gorel, K Graham, E Grace, N Guerrero, V Guiseppe, AL Hallin, P Harvey, C Hearns, R Henning, A Hime, J Hofgartner, S Jaditz, CJ Jillings, C Kachulis, E Kearns, J Kelsey, JR Klein, M Kuźniak, A LaTorre, I Lawson, O Li, JJ Lidgard, P Liimatainen, S Linden, K McFarlane, DN McKinsey, S MacMullin, A Mastbaum, R Mathew, AB McDonald, D-M Mei, J Monroe, A Muir, C Nantais, K Nicolics, JA Nikkel, T Noble, E O’Dwyer, K Olsen, GD Orebi Gann, C Ouellet, K Palladino, P Pasuthip, G Perumpilly, T Pollmann, P Rau, F Retière, K Rielage, R Schnee, S Seibert, P Skensved, T Sonley, E Vázquez-Jáuregui, L Veloce, J Walding, B Wang, J Wang, M Ward, C Zhang
More details from the publisher
Details from ArXiV

Energy and flux measurements of ultra-high energy cosmic rays observed during the first ANITA flight

Proceedings of Science 30-July-2015 (2015)

Authors:

H Schoorlemmer, K Belov, A Romero-Wolf, D García-Fernández, V Bugaev, SA Wissel, P Allison, J Alvarez-Muñiz, SW Barwick, JJ Beatty, DZ Besson, WR Binns, WR Carvalho, C Chen, P Chen, JM Clem, A Connolly, PF Dowkontt, MA DuVernois, RC Field, D Goldstein, PW Gorham, C Hast, CL Heber, T Huege, S Hoover, MH Israel, A Javaid, J Kowalski, J Lam, JG Learned, KM Liewer, JT Link, E Lusczek, S Matsuno, BC Mercurio, C Miki, P Miocinović, K Mulrey, J Nam, CJ Naudet, J Ng, RJ Nichol, K Palladino, BF Rauch, J Roberts, K Reil, B Rotter, M Rosen, L Ruckman, D Saltzberg, D Seckel, D Urdaneta, GS Varner, AG Vieregg, D Walz, F Wu, E Zas

Abstract:

The first flight of the Antarctic Impulsive Transient Antenna (ANITA) experiment recorded 14 radio signals that were emitted by downward going cosmic-ray induced air showers. The dominant contribution to the radiation comes from the deflection of positrons and electrons in the geomagnetic field and is beamed in a cone around the direction of motion of the air shower. This radiation is reflected from the ice and subsequently detected by the ANITA experiment at a flight altitude of -36 km. In this contribution, we estimate the cosmic-ray energy of the 14 individual events and find a mean energy of 2:9-1018 eV. By simulating the ANITA flight, we calculate its exposure for ultra-high energy cosmic rays (UHECRs) and we estimate for the first time the cosmic-ray flux derived only from radio observations.

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