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An aging study of triple GEMs in Ar鈥揅O2

Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment Elsevier 478:1-2 (2002) 263-266

Authors:

L Guirl, S Kane, J May, J Miyamoto, I Shipsey

The Nature of the Progenitor of the Type II-P Supernova 1999em**Based on observations at the William Herschel Telescope on La Palma and the Canada-France-Hawaii Telescope.

The Astrophysical Journal American Astronomical Society 565:2 (2002) 1089-1100

Authors:

Stephen J Smartt, Gerard F Gilmore, Christopher A Tout, Simon T Hodgkin

Observations of the Hubble Deep Field South with the Infrared Space Observatory - I. Observations, data reduction and mid-infrared source counts

(2002)

Authors:

S Oliver, RG Mann, R Carballo, A Franceschini, M Rowan-Robinson, M Kontizas, A Dapergolas, E Kontizas, A Verma, D Elbaz, GL Granato, L Silva, D Rigopoulou, JI Gonzalez-Serrano, S Serjeant, A Efstathiou, PP van der Werf

Observations of the Hubble Deep Field South with the Infrared Space Observatory - II. Associations and star formation rates

(2002)

Authors:

RG Mann, S Oliver, R Carballo, A Franceschini, M Rowan-Robinson, AF Heavens, M Kontizas, D Elbaz, A Dapergolas, E Kontizas, GL Granato, L Silva, D Rigopoulou, JI Gonzalez-Serrano, A Verma, S Serjeant, A Efstathiou, PP van der Werf

Report of Snowmass 2001 Working Group E2 : Electron-positron Colliders from the $蠁$ to the Z

ArXiv hep-ex/0201047 (2002)

Authors:

Z Zhao, G Eigen, G Burdman, W Marciano, D Hitlin, M Mandelkern, A Soffer, D Cassel, L Gibbons, K Moenig, J Butler, P Kasper, R Kutschke, P Mackenzie, S Pordes, R Ray, T Sen, D Bettoni, R Calabrese, C Bloise, D Kaplan, N Katayama, Y Okada, Y Ohnishi, H Yamamoto, A Gritsan, S Dytman, J Lee, I Shipsey, Y Maravin, FJ Decker, G Hiller, P Kim, D Leith, S Petrak, S Robertson, A Roodman, J Seeman, M Artuso, S Stone, X Lou, M Luke, W Johns

Abstract:

We report on the status and plans of experiments now running or proposed for electron-positron colliders at energies between the $\phi$ and the Z. The $e^{+}e^{-}$ B and charm factories we considered were PEP-II/BABAR, KEKB/Belle, superKEK, SuperBABAR, and CESR-c/CLEO-c. We reviewed the programs at the $\phi$ factory at Frascati and the proposed PEP-N facility at Stanford Linear Accelerator Center. We studied the prospects for B physics with a dedicated linear collider Z factory, associated with the TESLA high energy linear collider. In all cases, we compared the physics reach of these facilities with that of alternative experiments at hadron colliders or fixed target facilities.