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Three of the lensing pipelines (I3, DE, KM) that are included in the
cluster STEP results, also competed in the GREAT10 challenge.
The comparison between the GREAT10 and CSTEP results is shown in
Figure %\ref{fig:gt10}. The results are roughly consistent between
the two challenges for I3 and KM showing that both pipelines are
robust, and demonstrate similar levels of shape measurement bias
for a wide variety of sources and PSF types. Both I3 and KM are
among the best performing lensing pipelines for both CSTEP and
GREAT10.
\begin{figure}
\centering % this centres figure in column
\includegraphics[width=0.45\textwidth]{fig/QMC_gt10.pdf}
\includegraphics[width=0.45\textwidth]{fig/MC_gt10.pdf}
\caption{This figure shows the average shape measurement bias
as measured on all images for galaxy objects SNR $>$ 20 on
CSTEP data and the shape measurement bias as measured by the
same lensing pipelines on the GREAT10 data \citep{GREAT10}. The
top panel shows the shape measurement bias Q,M as measured using
a Q,M,C fit. The bottom panel shows the shape measurement bias
M,C as measured using a M,C fit.}
\label{fig:gt10}
\end{figure}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\begin{table*}
\centering
\begin{tabular}{|c|c|c|c|c|c|c|c|}
\hline
Pipeline & Qsel & Msel & Csel & Q & M & C \\
\hline
DE & -0.088 $\pm$ 0.017 & 0.928 $\pm$ 0.002 & -0.0014 $\pm$ 0.0002 & -0.094 $\pm$ 0.009 & 0.924 $\pm$ 0.001 & -0.0004 $\pm$ 0.0001 \\
\hline
PF & -0.033 $\pm$ 0.040 & 0.988 $\pm$ 0.005 & -0.0004
$\pm$ 0.0003 & -0.058 $\pm$ 0.038 & 0.963 $\pm$ 0.005 &
-0.0008 $\pm$ 0.0003 \\
\hline
GM & 0.236 $\pm$ 0.032 & 0.944 $\pm$ 0.004 & 0.0006
$\pm$ 0.0003 & 0.153 $\pm$ 0.034 & 0.991 $\pm$ 0.004 &
-0.0001 $\pm$ 0.0003 \\
\hline
MJ & 0.083 $\pm$ 0.035 & 0.901 $\pm$ 0.004 & 0.0015 $\pm$
0.0003 & 0.106 $\pm$ 0.043 & 0.867 $\pm$ 0.006 & 0.0016
$\pm$ 0.0004 & 0.81 \\
\hline
PK & -0.029 $\pm$ 0.016 & 0.946 $\pm$ 0.002 & 0.0006 $\pm$
0.0001 & -0.022 $\pm$ 0.016 & 0.945 $\pm$ 0.002 & 0.0003
$\pm$ 0.0001 \\
\hline
I3 & -0.042 $\pm$ 0.016 & 0.983 $\pm$ 0.002 & 0.0000
$\pm$ 0.0001 & -0.051 $\pm$ 0.017 & 0.982 $\pm$ 0.002 &
0.0001 $\pm$ 0.0002 \\
\hline
IM & -0.020 $\pm$ 0.058 & 1.275 $\pm$ 0.008 & -0.0066
$\pm$ 0.0005 & -0.035 $\pm$ 0.066 & 1.098 $\pm$ 0.009 &
-0.0080 $\pm$ 0.0006 \\
\hline
KM & -0.050 $\pm$ 0.010 & 0.981 $\pm$ 0.001 & 0.0007 $\pm$
0.0001 & -0.040 $\pm$ 0.010 & 0.973 $\pm$ 0.001 & 0.0004
$\pm$ \\
\hline
\end{tabular}
\caption{ The Q, M, C results for objects SNR $>$ 20. The
values reported are the reults of a Q,M,C fit after
correcting for selection effects (Qsel, Msel, Csel) and not
correcting for selection effects (Q, M, C).}
\label{table:QMC_sel}
\end{table*}
\begin{table*}
\centering
\begin{tabular}{|c|c|c|c|c| }
\hline
Pipeline & Msel & Csel & M & C \\
\hline
DEIMOS & 0.915 $\pm$ 0.002 & -0.0013 $\pm$ 0.0002 & 0.911
$\pm$ 0.001 & -0.0002 $\pm$ 0.0001 \\
\hline
PFDNT & 0.983 $\pm$ 0.005 & -0.0004 $\pm$ 0.0003 & 0.956
$\pm$ 0.005 & -0.0007 $\pm$ 0.0003 \\
\hline
GaussianMix & 0.976 $\pm$ 0.004 & 0.0003 $\pm$ 0.0003 &
1.012 $\pm$ 0.004 & -0.0003 $\pm$ 0.0003 \\
\hline
MJ & 0.913 $\pm$ 0.004 & 0.0014 $\pm$ 0.0003 & 0.881 $\pm$ 0.006 & 0.0015 $\pm$ 0.0004 \\
\hline
PKSB & 0.942 $\pm$ 0.002 & 0.0007 $\pm$ 0.0001 & 0.942 $\pm$
0.002 & 0.0004 $\pm$ 0.0001 \\
\hline
im3shape & 0.977 $\pm$ 0.002 & 0.0001 $\pm$ 0.0001 & 0.975 $\pm$ 0.002 & 0.0002 $\pm$ 0.0002 \\
\hline
IMCAT & 1.272 $\pm$ 0.007 & -0.0066 $\pm$ 0.0005 & 1.093 $\pm$ 0.008 & -0.0079 $\pm$ 0.0006 \\
\hline
ksbm & 0.975 $\pm$ 0.001 & 0.0008 $\pm$ 0.0001 & 0.967 $\pm$ 0.001 & 0.0005 $\pm$ 0.0001 \\
\hline
\end{tabular}
\caption{ The M, C results for objects SNR $>$ 20. The
values reported are the reults of a M,C fit after
correcting for selection effects (Msel, Csel) and not
correcting for selection effects (M, C).}
\label{table:MC_sel}
\end{table*}