\begin{table}%t5 \caption[]{\label{tab:feros}Log of the FEROS observations of V1130~Tau. } { \begin{tabular}{ccrr} \hline \hline\noalign{\smallskip} HJD$-$2\,400\,000\tablefootmark{a} & Phase &$t_{\rm exp}$\tablefootmark{b} & $S/N$\tablefootmark{c}\\ \noalign{\smallskip} \hline \noalign{\smallskip} 51188.6379 & 0.1675 & 600 & 223 \\ % Cpf283610027.fits 200 900 701 1.00 0.00 6036.0 6057.0 51207.5446 & 0.8344 & 600 & 171 \\ % Cpf355210027.fits 200 900 701 0.99 0.01 6036.0 6057.0 51207.5662 & 0.8615 & 600 & 170 \\ % Cpf355410027.fits 200 900 701 0.99 0.01 6036.0 6057.0 51208.5852 & 0.1370 & 600 & 162 \\ % Cpf359310027.fits 200 900 701 0.99 0.01 6036.0 6057.0 51209.5918 & 0.3971 & 600 & 200 \\ % Cpf363010027.fits 200 900 701 0.99 0.00 6036.0 6057.0 51211.5630 & 0.8645 & 600 & 84 \\ % Cpf371310027.fits 200 900 701 1.00 0.01 6036.0 6057.0 51212.6064 & 0.1706 & 600 & 176 \\ % Cpf375910027.fits 200 900 701 1.00 0.01 6036.0 6057.0 51385.9274 & 0.1288 & 600 & 142 \\ % Cpf852110027.fits 200 900 701 1.00 0.01 6036.0 6057.0 51386.9327 & 0.3872 & 600 & 170 \\ % Cpf857810027.fits 200 900 701 1.00 0.01 6036.0 6057.0 51390.8696 & 0.3154 & 600 & 241 \\ % Cpf872210027.fits 200 900 701 1.00 0.00 6036.0 6057.0 51391.9171 & 0.6266 & 600 & 225 \\ % Cpf877810027.fits 200 900 701 1.00 0.00 6036.0 6057.0 51392.8746 & 0.8252 & 720 & 237 \\ % Cpf889410027.fits 200 900 701 0.99 0.00 6036.0 6057.0 51562.5335 & 0.1992 & 600 & 243 \\ % Cpf343110027.fits 200 900 701 1.00 0.00 6036.0 6057.0 51562.5962 & 0.2777 & 600 & 281 \\ % Cpf343310027.fits 200 900 701 1.00 0.00 6036.0 6057.0 51562.6289 & 0.3187 & 600 & 244 \\ % Cpf343610027.fits 200 900 701 1.00 0.00 6036.0 6057.0 51977.4958 & 0.6371 & 630 & 181 \\ % Cpf579910027.fits 200 900 701 1.00 0.01 6036.0 6057.0 51978.4897 & 0.8812 & 600 & 179 \\ % Cpf585710027.fits 200 900 701 0.99 0.01 6036.0 6057.0 51981.4927 & 0.6402 & 600 & 166 \\ % Cpf611610027.fits 200 900 701 1.00 0.01 6036.0 6057.0 \hline \end{tabular} } \tablefoot{\tablefoottext{a}{Refers to mid-exposure.} \tablefoottext{b}{Exposure time in seconds.} \tablefoottext{c}{Signal-to-noise ratio measured around 6070 {\AA}. At the shorter wavelengths used for the radial velocity measurements it is somewhat lower.}} \end{table}