Publication
An update from STAR—using strangeness to probe relativistic heavy ion collisions
Helen Caines, (for the STAR Collaboration), J Adams, C Adler, Z Ahammed, J Amonett, B D Anderson, M Anderson, D Arkhipkin, G S Averichev, J Balewski, O Barannikova, L S Barnby, J Baudot, S Bekele, V V Belaga, R Bellwied, J Berger, H Bichsel, A Billmeier, L C Bland, C O Blyth, B E Bonner, A Boucham, A Brandin, A Bravar, R V Cadman, X Z Cai, M Calderón de la Barca Sánchez, A Cardenas, J Carroll, J Castillo, M Castro, D Cebra, P Chaloupka, S Chattopadhyay, H F Chen, Y Chen, S P Chernenko, M Cherney, A Chikanian, B Choi, W Christie, J P Coffin, T M Cormier, M M Corral, J G Cramer, H J Crawford, A A Derevschikov, L Didenko, T Dietel, X Dong, J E Draper, V B Dunin, J C Dunlop, V Eckardt, L G Efimov, V Emelianov, J Engelage, G Eppley, B Erazmus, P Fachini, V Faine, J Faivre, R Fatemi, K Filimonov, P Filip, E Finch, Y Fisyak, D Flierl, K J Foley, J Fu, C A Gagliardi, N Gagunashvili, J Gans, L Gaudichet, M Germain, F Geurts, V Ghazikhanian, J E Gonzalez, O Grachov, V Grigoriev, D Grosnick, M Guedon, S M Guertin, E Gushin, T J Hallman, D Hardtke, J W Harris, M Heinz, T W Henry, S Heppelmann, T Herston, B Hippolyte, A Hirsch, E Hjort, G W Hoffmann, M Horsley, H Z Huang, S L Huang, T J Humanic, G Igo, A Ishihara, P Jacobs, W W Jacobs, M Janik, I Johnson, P G Jones, E G Judd, S Kabana, M Kaneta, M Kaplan, D Keane, J Kiryluk, A Kisiel, J Klay, S R Klein, A Klyachko, D D Koetke, T Kollegger, A S Konstantinov, M Kopytine, L Kotchenda, A D Kovalenko, M Kramer, P Kravtsov, K Krueger, C Kuhn, A I Kulikov, G J Kunde, C L Kunz, R Kh Kutuev, A A Kuznetsov, M A C Lamont, J M Landgraf, S Lange, C P Lansdell, B Lasiuk, F Laue, J Lauret, A Lebedev, R Lednický, V M Leontiev, M J LeVine, C Li, Q Li, S J Lindenbaum, M A Lisa, F Liu, L Liu, Z Liu, Q J Liu, T Ljubicic, W J Llope, H Long, R S Longacre, M Lopez-Noriega, W A Love, T Ludlam, D Lynn, J Ma, Y G Ma, D Magestro, R Majka, R Manweiler, S Margetis, C Markert, L Martin, J Marx, H S Matis, Yu A Matulenko, T S McShane, F Meissner, Yu Melnick, A Meschanin, M Messer, M L Miller, Z Milosevich, N G Minaev, J Mitchell, C F Moore, V Morozov, M M de Moura, M G Munhoz, J M Nelson, P Nevski, V A Nikitin, L V Nogach, B Norman, S B Nurushev, G Odyniec, A Ogawa, V Okorokov, M Oldenburg, D Olson, G Paic, S U Pandey, Y Panebratsev, S Y Panitkin, A I Pavlinov, T Pawlak, V Perevoztchikov, W Peryt, V A Petrov, J Pluta, N Porile, J Porter, A M Poskanzer, E Potrebenikova, D Prindle, C Pruneau, J Putschke, G Rai, G Rakness, O Ravel, R L Ray, S V Razin, D Reichhold, J G Reid, G Renault, F Retiere, A Ridiger, H G Ritter, J B Roberts, O V Rogachevski, J L Romero, A Rose, C Roy, L J Ruan, V Rykov, I Sakrejda, S Salur, J Sandweiss, I Savin, J Schambach, R P Scharenberg, N Schmitz, L S Schroeder, A Schüttauf, K Schweda, J Seger, D Seliverstov, P Seyboth, E Shahaliev, M Shao, K E Shestermanov, S S Shimanskii, F Simon, G Skoro, N Smirnov, R Snellings, P Sorensen, J Sowinski, H M Spinka, B Srivastava
Journal of Physics G Nuclear and Particle Physics, December 2003, Institute of Physics Publishing
DOI: 10.1088/0954-3899/30/1/005