El experimento AMS-02 como un observatorio de rayos gamma ...
El experimento AMS-02 como un observatorio de rayos gamma ...
El experimento AMS-02 como un observatorio de rayos gamma ...
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2m ¢¡¤£ ¡ ! ¡ %$(¦¢ )¢¢ 2pvwF<strong>un</strong>cion <strong>de</strong> dispersion angular (32 GeV)Probabilidad/grados0.160.140.120.1σ 68(32 GeV)0.080.060.040.<strong>02</strong>00 0.05 0.1 0.15 0.2 0.25 0.3Residuo angular ψ (grados)798:2;="D BK^Xaqp [d^`PLhPdalHr2LW\H\aqp [d^wN¤^¡|dKQxN¤We L9qN(H\K%r2LWYr"K2LH\U_[(LQ,N §VK¡H\U_L~N¦QSN \K^Xaqp [d^ je ¢ ¤`”¦LQ"]¤N¤Qx[¤WhPL¡ £¢¥¤§A©CF<strong>un</strong>cion <strong>de</strong> dispersion p<strong>un</strong>tual (32 GeV)Probabilidad/sr0.10.08P(ψ,32 GeV,todo x)0.060.040.<strong>02</strong>00 0.<strong>02</strong> 0.04 0.06 0.08 0.1 0.12 0.14Residuo angular ψ(grados)[¤^798:2;=} r"acX\N‰PjLQ L^ \K^XaqpN¤^|KQS[PjLƒPda LWZL^"XacN*L^EUWZLQxNP¤anWZL\X\Xaqp[dWVa |dan^N¤Q9”ŽQSN§"A©C 2D =[¤WVMONŽUdp[d^PLQp[d^wWZL\X\[¤^2HVUWVKacPjNePdanWZL\X\Xaqp
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