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Table A.1:

r-process elemental abundances in metal-poor stars and the Sun for radioactive dating.
Object Reference [Fe/H] A(Eu) A(Hf) A(Os) A(Ir) A(Th) A(U)
HD 115444 Cowan et al. (1999) -2.7 -1.5       -2.1  
HD 115444 Westin et al. (2000) -2.9 $-1.63\pm 0.07$   $-0.55\pm 0.11$   $-2.23\pm 0.11$ <-2.6
CS 22892-052 Cowan et al. (1999) -3.1 -0.9       -1.6  
CS 22892-052 Sneden et al. (2000a)a -3.1 $-0.89\pm 0.12$ $-0.90\pm 0.14$ $-0.10\pm 0.38$   $-1.55\pm 0.08$  
CS 22892-052 Sneden et al. (2000a) -3.1 $-0.93\pm 0.09$   $-0.05\pm 0.10$ $+0.00\pm 0.26$ $-1.60\pm 0.07$  
CS 22892-052 Sneden et al. (2003) -3.1 $-0.95\pm 0.03$ $-0.98\pm 0.10$ $+0.02\pm 0.13$ $-0.10\pm 0.10$ $-1.57\pm 0.10$ <-2.3
BD +17 3248 Cowan et al. (2002) -2.0 $-0.67\pm 0.05$   $+0.45\pm 0.10$ $+0.30\pm 0.13$ $-1.18\pm 0.10$ $-2.0:\pm 0.30$
HD 221170 Ivans et al. (2006) -2.18 $-0.86\pm 0.07$ $-0.94\pm 0.04$ $+0.16\pm 0.10$ $+0.02\pm 0.13$ $-1.46\pm 0.05$  
CS 31082-001 Hill et al. (2002) -2.90 $-0.63\pm 0.04$ $-0.59\pm 0.17$ $+0.43\pm 0.12$ $+0.20\pm 0.09$ $-0.98\pm 0.02$ $-1.92\pm 0.11$
M51 K341 Sneden et al. (2000b) -2.32 $-0.88\pm 0.09$       $-1.47\pm 0.10$  
M51 K462 Sneden et al. (2000b) -2.25 $-0.61\pm 0.09$       $-1.26\pm 0.10$  
M51 K583 Sneden et al. (2000b) -2.34 $-1.22\pm 0.09$       $-1.7:\pm 0.10$  
M4 L1411 Yong et al. (2008) -1.23   +0.08     -0.68  
M4 L1501 Yong et al. (2008) -1.29   -0.02     -0.63  
M4 L1514 Yong et al. (2008) -1.22   +0.03     -0.83  
M4 L2406 Yong et al. (2008) -1.30   -0.12     -0.88  
M4 L2617 Yong et al. (2008) -1.20   +0.08     -0.48  
M4 L3209 Yong et al. (2008) -1.25   +0.03     -0.68  
M4 L3413 Yong et al. (2008) -1.23   -0.02     -0.58  
M4 L4511 Yong et al. (2008) -1.22   +0.03     -0.63  
M4 L4611 Yong et al. (2008) -1.09   +0.18     -0.68  
M5 IV-81 Yong et al. (2008) -1.28   -0.12     -0.58  
M5 IV-82 Yong et al. (2008) -1.33   -0.22     -0.68  
HD 108577 Johnson & Bolte (2001) -2.38 $ -1.48\pm 0.02$       $-1.99\pm 0.07$  
HD 115444 Johnson & Bolte (2001) -3.15 $ -1.81\pm 0.03$       $-2.36\pm 0.07$  
HD 186478 Johnson & Bolte (2001) -2.61 $ -1.56\pm 0.06$       $-2.26\pm 0.07$  
BD +82856 Johnson & Bolte (2001) -2.12 $ -1.16\pm 0.06$       $-1.66\pm 0.10$  
M92VII-18 Johnson & Bolte (2001) -2.29 $ -1.48\pm 0.09$       $-1.97\pm 0.07$  
Sun Grevesse & Sauval (1998) +0.0     $+1.45\pm 0.10$ $+1.35\pm 0.10$    
Sun Mucciarelli et al. (2008) +0.0 $+0.52\pm 0.03$          
Sun Caffau et al. (2008) +0.0   $+0.87\pm 0.04$     $+0.08\pm 0.03$  

a Sneden et al. analysed two different spectra for CS 22892-052 providing two independent measurements. For this reason the object/reference combination is listed twice.

Source LaTeX | All tables | In the text

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