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Table 2: Sizes of the smaller partition in the seg- mented network in case of massive node failure with difierent fanouts (m)
2006
Cited by 7
Table 1. Interprocessor communication networks for a massively parallel machine (CRAY T3E-1200) with 512 processors and two Linux based PC clusters with 32 (Zampano) and 40 (MPCB) processors.
Table 3-2. VLSI neural network Chips
1996
"... In PAGE 38: ...Table3 -1. Analog VLSI vs.... ..."
Table 1: slave structure 5. PROBLEM AND CAUSES The parallel e ciency of this rst version is very dis- appointing. Several causes can be found for this lack of e ciency : communications are still huge and very frequent regarding to the computation load; commu- nications in themselves are slow and unstable on an Ethernet network comparatively to networks intercon- necting processors of massively parallel machines; each
1996
"... In PAGE 2: ... If convergence is assumed, convergence loops are over and slaves give their results back to the master. Table1 shows the structure of a slave.... ..."
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Table 1: slave structure 5. PROBLEM AND CAUSES The parallel e ciency of this rst version is very dis- appointing. Several causes can be found for this lack of e ciency : communications are still huge and very frequent regarding to the computation load; commu- nications in themselves are slow and unstable on an Ethernet network comparatively to networks intercon- necting processors of massively parallel machines; each
1996
"... In PAGE 2: ... If convergence is assumed, convergence loops are over and slaves give their results back to the master. Table1 shows the structure of a slave.... ..."
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Table 1 Massive Out ows
"... In PAGE 17: ...2. MOLECULAR BIPOLAR OUTFLOW PROPERTIES In Table1 , I have tabulated the sources toward which massive out ows have been detected. These are listed in order of increasing RA.... In PAGE 20: ...ED CHUR CHWELL Table1 (continued). Source RA(1950) DEC(1950) D LHII LIR Refs Notes kpc L L S140 (IRS1) 22 17 41.... ..."
Table 4. Massive Star Photometry
"... In PAGE 8: ....3. Photometry of High-Mass Stars In addition to the low-mass members of the Ori region, we have also studied the massive stars. In Table4 we present new Stromgren photometry of one O star and eighteen B stars courtesy of colleagues at the Copenhagen Astronomical Observatory. This table includes all of the stars classi ed as spectral type O or B0{B5 in the Positions and Proper Motions Catalog (PPM Roeser amp; Bastian 1988) within 5 of Ori, except Bellatrix.... In PAGE 9: ... (1994). We report their photometry in Table4 with the others. 3.... ..."
Table 5: Massive Comparison. 20
2007
Table 5: Massive Comparison. 20
2007
Table 3: Massive supersymmetry representations of N =8
1996
"... In PAGE 11: ...short supermultiplets which we assume to be the maximum spin J =2,superspinL=0 multiplet (1; 8; 27; 48; 42) appearing in Table3 . The bound state interpretation requires that the a = 1 black holes preserving q = 2 supersymmetries appear in the product of two a = p3 representations.... ..."
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