this is for holding javascript data
ef (OU) work on section 2
about 10 years ago
Commit id: dd53e7b1091f8a78d61fef406a59852ecd55da1c
deletions | additions
diff --git a/section2.tex b/section2.tex
new file mode 100644
index 0000000..fc906e5
--- /dev/null
+++ b/section2.tex
...
\section{Population Synthesis parameters}
\label{sec:population_synthesis_parameters}
\paragraph{SFR, IMF and z}
\label{par:sfr_imf_and_z}
The authors assume a constant Star Formation Rate (0-12Gyr) and a time independent IMF \cite{soderhjelm}. Because the metallicity parameter for [Fe/H] in the BSE code is constant for the duration of the run (i.e. it is age-independent and uniform) the authors combined several runs with different upper and lower IMF limits in order to mimic the observed [Fe/H] distributions.
% paragraph sfr_imf_and_z (end)
\paragraph{$f(a, q, e)$}
\label{par:_f_a_q_e_}
For the binary runs the authors make simplifying first assumption that the function $f(a,q,e)$ is separable and assign 3 independent functions to $f(a)$, $f(q)$ and $f(e)$ respectively.
% paragraph _f_a_q_e_ (end)
% section population_synthesis_parameters (end)
