\begin{table}%t5
\caption{\label{tab-summary2}Source fluxes $[$mCrab$]$.}
\par
\small%\centerline
 {
\begin{tabular}{l|rrrrrrrrrr}
\hline\hline
&&&&&&&&&& \\[-8pt]
{\large Object Name}& \multicolumn{10}{c}{\large Flux $[$mCrab$]$$^{a,b}$}\\
  & \multicolumn{3}{c}{25--100 keV} & \multicolumn{3}{c}{100--200 keV}& \multicolumn{3}{c}{200--600 keV} & 600--1000 keV \\
      & \multicolumn{1}{c}{SPI} & \multicolumn{1}{c}{ISGRI} & \multicolumn{1}{c}{SPI(B08)} 
      & \multicolumn{1}{c}{SPI} & \multicolumn{1}{c}{ISGRI} & \multicolumn{1}{c}{SPI(B08)} 
      & \multicolumn{1}{c}{SPI} & \multicolumn{1}{c}{ISGRI} & \multicolumn{1}{c}{SPI(B08)} & \multicolumn{1}{c}{SPI} \\
\hline
Crab &1000.0 $\pm$ 2.0&1000.0 $\pm$ 2.0&1000.0 $\pm$ 2.0&1000.0 $\pm$ 3.4&1000.0 $\pm$ 3.5&1000.0 $\pm$ 3.7&1000.0 $\pm$ 11.8&1000.0 $\pm$ 18.6&1000.0 $\pm$ 8.3&1000.0 $\pm$ 43.2 
\\
Vela Pulsar &10.0 $\pm$ 0.4&7.2 $\pm$ 0.1&9.8 $\pm$ 0.7&11.6 $\pm$ 1.3&10.2 $\pm$ 0.9&12.6 $\pm$ 2.1&5.6 $\pm$ 5.3&0.0$+$19.0&13.9 $\pm$ 4.9&23.0 $\pm$ 18.5
\\
NGC 4151 &35.4 $\pm$ 2.4&32.7 $\pm$ 0.7&31.3 $\pm$ 2.1&43.8 $\pm$ 7.4&34.6 $\pm$ 2.5&22.9 $\pm$ 6.8&28.2 $\pm$ 36.4&0.0$+$132.5&46.9 $\pm$ 14.1&101.4 $\pm$ 111 
\\
NGC 4945 &18.7 $\pm$ 1.1&16.4 $\pm$ 0.3&18.3 $\pm$ 1.1&21.4 $\pm$ 3.7&21.5 $\pm$ 1.2&14.3 $\pm$ 4.0&0.5 $\pm$ 27.1&0.0$+$53.2&20.2 $\pm$ 8.3&5.8 $\pm$ 53.8 
\\
Cen A &40.7 $\pm$ 1.1&36.0 $\pm$ 0.3&40.5 $\pm$ 1.3&59.7 $\pm$ 3.7&53.7 $\pm$ 1.2&56.9 $\pm$ 4.6&55.9 $\pm$ 20.7&87.7 $\pm$ 24.2&70.1 $\pm$ 9.8&12.9 $\pm$ 48.7 
\\
XTE J1550-564&36.1 $\pm$ 0.6&41.6 $\pm$ 0.3&23.5 $\pm$ 0.7&55.2 $\pm$ 1.7&70.2 $\pm$ 0.9&30.2 $\pm$ 2.5&48.8 $\pm$ 8.4&51.5 $\pm$ 12.1&18.8 $\pm$ 5.5&6.7 $\pm$ 24.4 
\\
4U 1630-47&36.5 $\pm$ 1.6&1.8 $\pm$ 0.2$^c$&30.5 $\pm$ 1.3&19.7 $\pm$ 6.0&0.8 $\pm$ 0.3$^c$&21.7 $\pm$ 2.4&2.2 $\pm$ 23.3&19.9 $\pm$ 13.2$^c$&21.4 $\pm$ 5.3&0.0$+$164.2 
\\
Swift J1656.3-3302&3.7 $\pm$ 2.2&--\ \ \  $^d$& 6.0 $\pm$ 1.1&8.0 $\pm$ 3.4&--\ \ \  $^d$&  5.0 $\pm$ 1.9 &15.2 $\pm$ 7.8&--\ \ \  $^d$&  17.6 $\pm$ 4.0&24.6 $\pm$ 12.9 
\\
OAO 1657-415&66.6 $\pm$ 0.6&51.5 $\pm$ 1.3&51.3 $\pm$ 0.7&15.0 $\pm$ 1.3&7.6 $\pm$ 0.6&10.3 $\pm$ 2.2&15.0 $\pm$ 8.0&0.0$+$24.9&13.8 $\pm$ 4.8&2.3 $\pm$ 26.6 
\\
GX 339-4&34.1 $\pm$ 0.5&11.5 $\pm$ 0.2&38.4 $\pm$ 1.4&32.6 $\pm$ 1.4&12.1 $\pm$ 0.5&35.6 $\pm$ 2.4&30.1 $\pm$ 13.8&0.0$+$30.3&30.0 $\pm$ 5.2&66.1 $\pm$ 27.4 
\\
4U 1700-377&171.7 $\pm$ 0.8&162.3 $\pm$ 3.6&146.3 $\pm$ 1.4&36.0 $\pm$ 1.0&40.9 $\pm$ 1.6&35.5 $\pm$ 2.2&13.6 $\pm$ 8.1&23.4 $\pm$ 17.2&6.4 $\pm$ 4.8&0.0$+$62.7 
\\
IGR J17091-3624&5.2 $\pm$ 0.8&6.1 $\pm$ 0.1&8.9 $\pm$ 0.6&7.2 $\pm$ 5.0&6.3 $\pm$ 0.3&5.6 $\pm$ 2.0&18.5 $\pm$ 8.8&2.7 $\pm$ 13.4&9.8 $\pm$ 4.4&8.7 $\pm$ 19.6 
\\
GX 354-0&34.2 $\pm$ 0.5&23.4 $\pm$ 0.1&24.4 $\pm$ 0.5&10.5 $\pm$ 1.1&5.4 $\pm$ 0.2&7.6 $\pm$ 1.8&0.7 $\pm$ 10.0&1.0 $\pm$ 10.5&7.9 $\pm$ 4.1&7.4 $\pm$ 21.4 
\\
1E 1740.7-2942&52.8 $\pm$ 0.9&32.7 $\pm$ 0.1&51.1 $\pm$ 1.2&43.0 $\pm$ 2.3&35.0 $\pm$ 0.3&48.3 $\pm$ 1.6&18.5 $\pm$ 10.9&22.1 $\pm$ 6.1&39.2 $\pm$ 3.6&7.8 $\pm$ 34.9 
\\
IGR J17464-3213&13.3 $\pm$ 0.6&15.1 $\pm$ 0.1&15.6 $\pm$ 0.7&6.9 $\pm$ 1.1&9.9 $\pm$ 0.2&11.2 $\pm$ 1.6&2.2 $\pm$ 4.4&6.8 $\pm$ 6.3&9.9 $\pm$ 3.6&41.6 $\pm$ 23.1 
\\
GRS 1758-258&68.8 $\pm$ 0.7&66.6 $\pm$ 0.2&70.8 $\pm$ 0.9&84.6 $\pm$ 2.1&82.2 $\pm$ 0.5&83.4 $\pm$ 1.6&41.1 $\pm$ 7.2&49.3 $\pm$ 6.0&47.4 $\pm$ 3.6&51.2 $\pm$ 18.0 
\\
Ginga 1826-24&75.8 $\pm$ 0.5&73.1 $\pm$ 0.3&74.6 $\pm$ 0.5&30.3 $\pm$ 0.9&34.2 $\pm$ 0.4&33.6 $\pm$ 1.9&18.4 $\pm$ 5.7&0.0$+$19.8&24.5 $\pm$ 3.9&38.3 $\pm$ 22.4
\\
GRS 1915+105&189.1 $\pm$ 0.8&187.8 $\pm$ 0.5&150.1 $\pm$ 0.9&73.2 $\pm$ 2.2&60.5 $\pm$ 0.5&61.8 $\pm$ 2.3&38.8 $\pm$ 8.7&40.9 $\pm$ 10.2&38.6 $\pm$ 5.2&53.9 $\pm$ 27.2 
\\
Cyg X-1&841.0 $\pm$ 1.5&871.6 $\pm$ 1.7&843.8 $\pm$ 1.0&873.7 $\pm$ 3.1&907.6 $\pm$ 3.1&769.9 $\pm$ 3.1&575.5 $\pm$ 9.8&581.3 $\pm$ 16.1&500.6 $\pm$ 6.9&386.4 $\pm$ 37.3
\\
Cyg X-3&117.7 $\pm$ 0.6&111.7 $\pm$ 0.6&101.2 $\pm$ 0.8&34.9 $\pm$ 1.4&25.3 $\pm$ 0.5&25.0 $\pm$ 2.9&26.4 $\pm$ 7.6&21.0 $\pm$ 21.8&14.8 $\pm$ 6.2&52.6 $\pm$ 31.0 
\\
Estim. Syst. Error$^e$      & --0.9 & --0.1 &  --\ \ \   & --0.1 & --0.4 &  --\ \ \  & --0.1 & --1.2 &  --\ \ \   & --0.1 \\
\hline
\end{tabular}}
\medskip
$^a$~For the columns ``SPI'' and ``ISGRI'' fluxes are expressed as fractions of the Crab fluxes for the individual instrument given in Table~\ref{tab-crab}. In the columns ``SPI (B08)'' we give the fluxes obtained by Bouchet et~al. (\cite{bouchet08}) (B08) for the available energy ranges          (see B08 for their definition of the unit ``mCrab''). \\
$^b$~The statistical errors shown in this table do not take into account the uncertainty of the Crab flux on which the flux values are normalised. \\
$^c$~Spectrum very probably flawed by source contamination from  IGR~J16358-472; therefore not included in Fig.~\ref{fig-agree-spi-isgri}. \\
$^d$~ISGRI spectral fit failed, see Sect.~\ref{sec-SwiftJ}; therefore not included in Fig.~\ref{fig-agree-spi-isgri}. \\
$^e$~See Sect. \ref{sec-control1}.
\end{table}