Steve Biller: Publications

Neutral current and day night measurements from the pure D2O phase of SNO

Nuclear and Particle Physics Proceedings Elsevier 118 (2003) 3-14

Authors:

AL Hallin, EW Beier, SD Biller, MG Boulay, MG Bowler, TJ Bowles, SJ Brice, TV Bullard, J Cameron, YD Chan, X Chen, M Chen, BT Cleveland, GA Cox, X Dai, F Dalnoki-Veress, PJ Doe, G Doucas, MR Dragowsky, CA Duba, FA Duncan, M Dunford, JA Dunmore, ED Earle, SR Elliott, HC Evans, GT Ewan, J Farine, H Fergani, JA Formaggio, MM Fowler, K Frame, W Frati, N Gagnon, K Graham, DR Grant, RL Hahn, ED Hallman, AS Hamer, WB Handler, CK Hargrove, PJ Harvey, R Hazama, KM Heeger, WJ Heintzelman, J Heise, RL Helmer, A Hime, M Howe, P Jagam, NA Jelley, K Kazkaz, PT Keener, JR Klein, T Kutter, CCM Kyba, J Law, IT Lawson, KT Lesko, JR Leslie, I Levine, S Luoma, S Majerus, HB Mak, J Maneira, J Manor, AD Marino, N McCauley, AB McDonald, G McGregor, GG Miller, CW Nally, AJ Noble, EB Norman, CE Okada, JL Orrell, SM Oser, AWP Poon, BC Robertson, RGH Robertson, SSE Rosendahl, VL Rusu, KK Schaffer, MH Schwendener, JJ Simpson, CJ Sims, D Sinclair, P Skensved, MWE Smith, T Spreitzer, N Starinsky, RG Stokstad, LC Stonehill, R Tafirout, N Tagg, R Van Berg, RG Van de Water, CJ Virtue, CE Waltham, DL Wark, N West, JB Wilhelmy, JF Wilkerson, JR Wilson, P Wittich, JM Wouters, M Yeh

More details from the publisher

More details

Science capabilities of the VERITAS array of 10 m imaging atmospheric Cherenkov gamma-ray detectors

Proceedings of SPIE - The International Society for Optical Engineering 4834 (2002) 276-287

Authors:

D Kieda, SD Biller, P Boyle, IH Bond, SM Bradbury, JH Buckley, DA Carter-Lewis, S Criswell, W Cui, P Dowkontt, C Duke, A Falcone, DJ Fegan, SJ Fegan, JP Finley, L Fortson, JA Gaidos, S Gammell, K Gibbs, J Hall, AM Hillas, J Holder, D Horan, M Kertzman, J Knapp, F Krennrich, S LeBohec, J Lloyd-Evans, P Moriarity, D M̈ller, P Ogden, R Ong, D Petry, J Quinn, PT Reynolds, HJ Rose, M Schroedter, J Smith, GH Sembrowski, SP Swordy, VV Vassiliev, SP Wakely, G Walker, TC Weekes

Abstract:

The Very Energetic Radiation Imaging Telescope Array System (VERITAS) is an array of seven 10m aperture telescopes used for gamma-ray astronomy in the 50 GeV to 50 TeV (1 TeV= 1012 electron Volt) energy range. The gamma rays are detected by measuring the optical Cherenkov light emitted by the cascade of electromagnetic particles that is generated by interactions of the high energy gamma-ray with the Earth's Atmosphere. This paper describes the science goals of the VERITAS array, a description of the array, and expected performance of the instrument.

More details from the publisher

Direct evidence for neutrino flavor transformation from neutral-current interactions in the Sudbury Neutrino Observatory

Physical Review Letters 89 (2002) article 011301 6 pages

Authors:

NA Jelley, Q.R.Ahmad, R.C.Allen, T.C.Andersen

More details from the publisher

More details

Measurement of Day and Night Neutrino Energy Spectra at SNO and Constraints on Neutrino Mixing Parameters

Physical Review Letters 89 (2002) 011302 5pp

Authors:

SD Biller, Q.R. Ahmad, R.C. Allen, T.C. Anderson

More details from the publisher

More details

VERITAS: The Very Energetic Radiation Imaging Telescope Array System

Astroparticle Physics 17:2 (2002) 221-243

Authors:

TC Weekes, H Badran, SD Biller, I Bond, S Bradbury, J Buckley, D Carter-Lewis, M Catanese, S Criswell, W Cui, P Dowkontt, C Duke, DJ Fegan, J Finley, L Fortson, J Gaidos, GH Gillanders, J Grindlay, TA Hall, K Harris, AM Hillas, P Kaaret, M Kertzman, D Kieda, F Krennrich, MJ Lang, S LeBohec, R Lessard, J Lloyd-Evans, J Knapp, B McKernan, J McEnery, P Moriarty, D Muller, P Ogden, R Ong, D Petry, J Quinn, NW Reay, PT Reynolds, J Rose, M Salamon, G Sembroski, R Sidwell, P Slane, N Stanton, SP Swordy, VV Vassiliev, SP Wakely

Abstract:

The Very Energetic Radiation Imaging Telescope Array System (VERITAS) represents an important step forward in the study of extreme astrophysical processes in the universe. It combines the power of the atmospheric Cherenkov imaging technique using a large optical reflector with the power of stereoscopic observatories using arrays of separated telescopes looking at the same shower. The seven identical telescopes in VERITAS, each of aperture 10 m, will be deployed in a filled hexagonal pattern of side 80 m; each telescope will have a camera consisting of 499 pixels with a field of view of 3.5°. VERITAS will substantially increase the catalog of very high energy (E > 100 GeV) γ-ray sources and greatly improve measurements of established sources. © 2002 Elsevier Science B.V. All rights reserved.

More details from the publisher

More details

Steve Biller

Sub department

Neutral current and day night measurements from the pure D2O phase of SNO

Authors:

Science capabilities of the VERITAS array of 10 m imaging atmospheric Cherenkov gamma-ray detectors

Authors:

Abstract:

Direct evidence for neutrino flavor transformation from neutral-current interactions in the Sudbury Neutrino Observatory

Authors:

Measurement of Day and Night Neutrino Energy Spectra at SNO and Constraints on Neutrino Mixing Parameters

Authors:

VERITAS: The Very Energetic Radiation Imaging Telescope Array System

Authors:

Abstract:

FIND US

CONTACT US

Steve Biller

Sub department

Research groups

Neutral current and day night measurements from the pure D2O phase of SNO

Authors:

Science capabilities of the VERITAS array of 10 m imaging atmospheric Cherenkov gamma-ray detectors

Authors:

Abstract:

Direct evidence for neutrino flavor transformation from neutral-current interactions in the Sudbury Neutrino Observatory

Authors:

Measurement of Day and Night Neutrino Energy Spectra at SNO and Constraints on Neutrino Mixing Parameters

Authors:

VERITAS: The Very Energetic Radiation Imaging Telescope Array System

Authors:

Abstract: