Zobrazeno 1 - 10
of 101
pro vyhledávání: '"D D, Driscoll"'
Autor:
Richard Scalzo, Douglas Gingrich, A. Jarvis, J. Ball, R. A. Ong, David A. Williams, John Kildea, D. D. Driscoll, N. Akhter, Reshmi Mukherjee, C. Mueller, D. Bramel, Jeffrey Zweerink, K. Ragan, T. Lindner, P. Fortin, D. S. Hanna, J. Carson, Corbin Covault
Publikováno v:
Astroparticle Physics. 34:674-678
We present results of very-high-energy gamma-ray observations (Eγ > 160 GeV) of two high-frequency-peaked BL Lac (HBL) objects, 1ES 1218 + 304 and H 1426 + 428, with the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE). Both sources are
Autor:
A. Jarvis, J. Ball, R. A. Ong, Reshmi Mukherjee, C. Mueller, D. D. Driscoll, D. S. Hanna, Douglas Gingrich, John Kildea, T. Lindner, David A. Williams, K. Ragan, J. Carson, P. Fortin, T. Aune, Corbin Covault, Jeffrey Zweerink
Publikováno v:
The Astrophysical Journal. 722:862-870
Gamma-ray bursts (GRBs) are the most powerful explosions known in the universe. Sensitive measurements of the high-energy spectra of GRBs can place important constraints on the burst environments and radiation processes. Until recently, there were no
Autor:
John Kildea, R. A. Ong, Corbin Covault, K. Ragan, Douglas Gingrich, D. S. Hanna, David A. Williams, J. Carson, Reshmi Mukherjee, P. Fortin, Jeffrey Zweerink, C. Mueller, D. D. Driscoll, T. Lindner, A. Jarvis, J. Ball
Publikováno v:
The Astrophysical Journal. 693:1128-1132
The Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE) is a ground-based telescope that uses the wave-front-sampling technique to detect very high energy (VHE) gamma rays. STACEE's sensitivity in the energy range near 100 GeV permits useful
Autor:
Corbin Covault, Douglas Gingrich, David A. Williams, John Kildea, D. S. Hanna, Jeffrey Zweerink, D. Bramel, D. D. Driscoll, K. Ragan, T. Lindner, Reshmi Mukherjee, J. Carson, C. Mueller, A. Jarvis, J. Ball, Richard Scalzo, P. Fortin, R. A. Ong
Publikováno v:
Astroparticle Physics. 28:338-347
Using the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE), we have observed the BL Lac objects 3C 66A and OJ 287. These are members of the class of low-frequency-peaked BL Lac objects (LBLs) and are two of the three LBLs predicted by Cos
Autor:
Miguel Daal, C. Savage, Laura Baudis, A. Lu, M. Pyle, R. Hennings-Yeomans, Darren Grant, Ronald R. Ross, Thushara Perera, Bernard Sadoulet, S. J. Yellin, H. N. Nelson, Betty A. Young, S. Leclercq, M. R. Dragowsky, K. M. Sundqvist, C. N. Bailey, Vuk Mandic, N. Mirabolfathi, R. H. Nelson, D. D. Driscoll, M. J. Attisha, R. Ferril, P. Cushman, Sunil Golwala, Donald J. Holmgren, D. O. Caldwell, S. Kamat, D. A. Bauer, J. Sander, D. N. Seitz, J. P. F. Thompson, D. S. Akerib, Blas Cabrera, Bruno Serfass, R. Bunker, J. Yoo, Chihway Chang, R. J. Gaitskell, Jodi Cooley, R. L. Dixon, R. Mahapatra, R. W. Schnee, G. Wang, M. B. Crisler, A. Reisetter, W. Rau, P. Meunier, P. P. Brusov, E. J. Ramberg, Jeffrey P. Filippini, P. L. Brink, R. W. Ogburn, L. Duong, Martin E. Huber
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 173:137-140
The published CDMS analyses have used the shape of the phonon signal rising edge to reject low-ionization-yield surface events which produce acoustic phonons more quickly than bulk events do. To achieve better WIMP sensitivity with future larger expo
Autor:
R. Mahapatra, Tarek Saab, M. J. Attisha, M. B. Crisler, H. N. Nelson, R. Ferril, John M. Martinis, Donald J. Holmgren, R. H. Nelson, M. C. Perillo Isaac, Astrid Tomada, G. Smith, R. Bunker, J. Alvaro-Dean, A. Lu, Alexander Bolozdynya, M. Haldeman, L. Duong, Martin E. Huber, J. P. F. Thompson, A. L. Spadafora, P. Meunier, J. Hellmig, Thushara Perera, D. O. Caldwell, R. L. Dixon, G. Wang, D. N. Seitz, S. Kamat, J. P. Castle, R. J. Gaitskell, M. S. Armel, S. J. Yellin, J. Sander, Bernard Sadoulet, R. W. Ogburn, Betty A. Young, T. A. Shutt, J. Emes, J. Perales, D. A. Bauer, R. W. Schnee, Ronald R. Ross, C. Savage, Laura Baudis, C. L. Chang, M. Kurylowicz, M. Hennessey, Vuk Mandic, D. D. Driscoll, Sunil Golwala, A. K. Davies, P. Cushman, A. Reisetter, W. Rau, D. S. Akerib, Blas Cabrera, Sae Woo Nam, R. M. Clarke, P. L. Brink, N. Mirabolfathi
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 520:116-119
In the past year and a half, the Cryogenic Dark Matter Search (CDMS) collaboration has been active at the Soudan mine in installing a system for running ZIP detectors that will be used to search for dark matter in the form of Weakly Interacting Massi
Autor:
R. J. Gaitskell, L. Bogdanova, V. N. Trofimov, D. D. Driscoll, S. Kamat, Thushara Perera, D. S. Akerib, M. R. Dragowsky, R. W. Schnee, G. Wang
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 520:163-166
100-g silicon detectors (known as “ZIPs,” Z-resolving Ionization and Phonon detectors) developed by the Cryogenic Dark Matter Search Experiment have been tested at charge bias voltages of up to 200 V/cm, significantly above their usual operating
Publikováno v:
Physica E: Low-dimensional Systems and Nanostructures. 21:708-711
Scanning gate measurements have been performed on a shallow two-dimensional electron gas in a Ga[Al]As heterostructure in the quantum Hall regime at 300 mK . This technique uses the local electrostatic potential induced by the conducting tip of a sca
Autor:
M. S. Armel-Funkhouser, P. Meunier, V. Mandi, Thushara Perera, S. J. Yellin, A. R. Smith, G. Wang, Tarek Saab, C. L. Chang, Donald J. Holmgren, J. P. Castle, S. Eichblatt, Betty A. Young, Ronald R. Ross, M. B. Crisler, W. Rau, A. H. Sonnenschein, R. J. Gaitskell, David S. Abrams, Alexander Bolozdynya, J. Sander, Sae Woo Nam, Martin E. Huber, John M. Martinis, D. A. Bauer, P. L. Brink, J. Hellmig, D. D. Driscoll, A. Lu, R. Bunker, R. L. Dixon, Blas Cabrera, R. W. Schnee, H. N. Nelson, Sunil Golwala, S. Kamat, Laura Baudis, D. S. Akerib, T. A. Shutt, M. C. Perillo Isaac, R. M. Clarke, Bernard Sadoulet, A. L. Spadafora, D. O. Caldwell, E. E. Haller
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 124:185-188
The Cryogenic Dark Matter Search (CDMS) uses low-temperature Ge and Si detectors to search for Weakly Interacting Massive Particles (WIMPs) via their elastic-scattering interaction with atomic nuclei while discriminating against interactions of backg
Autor:
Thushara Perera, S. J. Yellin, J. Sander, C. N. Bailey, Chihway Chang, R. H. Nelson, Sunil Golwala, M. J. Attisha, Tarek Saab, P. Meunier, S. Leclercq, M. R. Dragowsky, J. P. F. Thompson, N. Mirabolfathi, E. J. Ramberg, R. Ferril, S. Kamat, D. O. Caldwell, Betty A. Young, R. J. Gaitskell, D. S. Akerib, K. M. Sundqvist, Donald J. Holmgren, R. W. Ogburn, Jeffrey P. Filippini, P. L. Brink, H. N. Nelson, M. B. Crisler, J. Yoo, Ronald R. Ross, R. Hennings-Yeomans, M. Pyle, Darren Grant, Vuk Mandic, L. Duong, Miguel Daal, Martin E. Huber, P. P. Brusov, D. N. Seitz, D. A. Bauer, R. Mahapatra, A. Reisetter, A. Lu, Bernard Sadoulet, G. Wang, C. Savage, Laura Baudis, R. Bunker, R. L. Dixon, Blas Cabrera, Jodi Cooley, R. W. Schnee, D. D. Driscoll, P. Cushman, Bruno Serfass
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 559:387-389
We present the techniques and results of the calibrations and surface-event rejection cut for the current CDMS-II data set, along with proposals for future analysis of CDMS-II data.