\begin{table}%t3 \caption{\label{tab:snrs}Detailed view of the various contributors to the noise budget, given in photo-electrons persecond over the 6--20~$\mu$m wavelength range for \darwin/TPF in the Emma X-array configuration.} %\centerline {\begin{tabular}{l c c c c} \hline \hline & M0V -- 05pc & K0V -- 10~pc & G2V -- 15~pc & F0V -- 20~pc \\ \hline Optimum baseline [m] & 25 & 22 & 22 & 11 \\ Planetary modulation efficiency & 0.57 & 0.58 & 0.58 & 0.58 \\ Planetary coupling efficiency & 0.76 & 0.76 & 0.76 & 0.75 \\ \hline\noalign{\smallskip} Stellar signal [e-/s] & $2.6 \times 10^7$ & $2.1 \times 10^7$ & $1.3 \times 10^7$ & $2.1 \times 10^7$ \\ Planetary signal [e-/s] & 5.52 & 1.39 & 0.62 & 0.35 \\ Photon noise [e-/s] & 0.459 & 0.388 & 0.358 & 0.365 \\ - Geometric leakage [e-/s] & 0.304 & 0.179 & 0.101 & 0.078 \\ - Null-floor leakage [e-/s] & 0.019 & 0.017 & 0.013 & 0.017 \\ - 3-zodi signal [e-/s] & 0.077 & 0.078 & 0.075 & 0.121 \\ - Local zodiacal signal [e-/s] & 0.260 & 0.260 & 0.260 & 0.260 \\ - Detected thermal [e-/s] & 0.101 & 0.101 & 0.101 & 0.101 \\ - Detected stray light [e-/s] & 0.166 & 0.166 & 0.166 & 0.166 \\ Dark current [e-/s] & 0.063 & 0.063 & 0.063 & 0.063 \\ Detector noise [e-/s] & 0.063 & 0.063 & 0.063 & 0.063 \\ Instability noise [e-/s] & 0.025 & 0.014 & 0.008 & 0.012 \\ - First order phase term [e-/s] & 0.021 & 0.008 & 0.002 & 0.001 \\ - Second order phase-amplitude [e-/s] & 0.014 & 0.012 & 0.007 & 0.012 \\ Total noise [e-/s] & 0.460 & 0.388 & 0.358 & 0.365 \\ Integrated $SNR$ (one rotation) & 16.0 & 4.4 & 2.1 & 1.1\\ Integration time for $SNR = 5$~[h] & 1.36 & 17.9 & 81.8 & 285\\ \hline \end{tabular}} \medskip The final SNRs are computed over a single rotation of 50~000~s and for four targets representative of the target catalogue (see main text for further information). \end{table}