Online material for 'Impact of $\textit{T}$- and $\rho$-dependent decay rates and new (n,$\gamma$) cross sections on the $\textit{s}$ process in low-mass asymptotic giant branch stars'

Online material for the article titled 'Impact of $\textit{T}$- and $\rho$-dependent decay rates and new (n,$\gamma$) cross sections on the $\textit{s}$ process in low-mass AGB stars'.

Files:

• srf.tar.gz: Surface isotopic abundance data tables of seven stellar models of low-mass AGB stars from Karakas & Lugaro (2016) for three nuclear networks. The sources of the reaction rates in the different sets are described in Table 2 of the article. Each file includes 1) The essential features of the models in the header: initial mass (M), initial mass fraction of helium (Y), initial metallicity (Z), and the nucleosynthesis set; 2) The mass number (A), atomic number (Z) and neutron number (N) for 328 isotopes that includes in our nuclear network; 3) Initial normalised number abundances (from Apslund et. al. 2009) used in the post-processing calculations; 4) Surface normalised number abundances calculated at each thermal pulse steps; 5) Final normalised number abundances computed at the last time step.
  
  

  Filename	Mass ($\mathrm{M_{\odot}}$)	Metallicity	Set
  srf_m3z007_set0.dat	3	0.007	0
  srf_m4z007_set0.dat	4	0.007	0
  srf_m2z014_set0.dat	2	0.014	0
  srf_m3z014_set0.dat	3	0.014	0
  srf_m4z014_set0.dat	4	0.014	0
  srf_m3z030_set0.dat	3	0.03	0
  srf_m4z030_set0.dat	4	0.03	0
  srf_m3z007_set1.dat	3	0.007	1
  srf_m4z007_set1.dat	4	0.007	1
  srf_m2z014_set1.dat	2	0.014	1
  srf_m3z014_set1.dat	3	0.014	1
  srf_m4z014_set1.dat	4	0.014	1
  srf_m3z030_set1.dat	3	0.03	1
  srf_m4z030_set1.dat	4	0.03	1
  srf_m3z007_set2.dat	3	0.007	2
  srf_m4z007_set2.dat	4	0.007	2
  srf_m2z014_set2.dat	2	0.014	2
  srf_m3z014_set2.dat	3	0.014	2
  srf_m4z014_set2.dat	4	0.014	2
  srf_m3z030_set2.dat	3	0.03	2
  srf_m4z030_set2.dat	4	0.03	2

• sy.tar.gz: Stellar yield data tables of seven stellar models of low-mass AGB stars from Karakas & Lugaro (2016) for three nuclear networks. The sources of the reaction rates in the different sets are described in Table 2 of the article. Each file includes 1) The essential features of the models in the header: initial mass (M), initial mass fraction of helium (Y), initial metallicity (Z), and the nucleosynthesis set; 2) The mass number (A), atomic number (Z) and neutron number (N) for 328 isotopes that includes in our nuclear network; 3) Stellar yields expressed in units of solar mass calculated by the method described in Section 2.3 of the article.
  
  

  Filename	Mass ($\mathrm{M_{\odot}}$)	Metallicity	Set
  sy_m3z007_set0.dat	3	0.007	0
  sy_m4z007_set0.dat	4	0.007	0
  sy_m2z014_set0.dat	2	0.014	0
  sy_m3z014_set0.dat	3	0.014	0
  sy_m4z014_set0.dat	4	0.014	0
  sy_m3z030_set0.dat	3	0.03	0
  sy_m4z030_set0.dat	4	0.03	0
  sy_m3z007_set1.dat	3	0.007	1
  sy_m4z007_set1.dat	4	0.007	1
  sy_m2z014_set1.dat	2	0.014	1
  sy_m3z014_set1.dat	3	0.014	1
  sy_m4z014_set1.dat	4	0.014	1
  sy_m3z030_set1.dat	3	0.03	1
  sy_m4z030_set1.dat	4	0.03	1
  sy_m3z007_set2.dat	3	0.007	2
  sy_m4z007_set2.dat	4	0.007	2
  sy_m2z014_set2.dat	2	0.014	2
  sy_m3z014_set2.dat	3	0.014	2
  sy_m4z014_set2.dat	4	0.014	2
  sy_m3z030_set2.dat	3	0.03	2
  sy_m4z030_set2.dat	4	0.03	2