\begin{table}%t6
\par
\caption {\label{globsmet}Classification of inner bulge globular clusters in terms of metallicity
and HB morphology (R~=~Red, B~=~Blue).  }
\par
 {\begin{tabular}{lllllllrrr}
\hline
\hline
Cluster & $E(B-V)$ & \phantom{-}$d_{\odot}$ &
[Fe/H] &
\phantom{-}$v_r$  &
HB &
$\phantom{--}$Ref.  \\
 &  & (kpc) &  &
(km~s$^{-1}$) &
 &  \\
\hline
\noalign{\bf Metal-poor}
Terzan 4 & 1.8 & 8.3 & --1.6 & --50 & B & 1, 2, 3 \\
Terzan 9 & 1.95    & 4.9 & --1.0 & --  & B & 4  \\
\noalign{\bf Moderately metal-poor, BHB}\\
HP~1     & 1.21        & 6.4  & --1.0 & 46 & B & 5, 6  \\
NGC~6522 & 0.45        & 7.4 & --0.86 & --25 & B & 7, 27 \\
NGC~6558 & 0.38        & 7.7 & --0.97 & --197  & B  & 8, 9 \\
Al~3     &0.36         & 6    & --1.3 & -- & B &  10 \\
Terzan 10 & 2.4       &  4.8    &  --1.0    & --    & B & 2, 11 \\
NGC~6540 &0.60 & 3.5 &--1.0 & --  & B & 12 \\
\noalign{\bf Moderately metal-poor, RHB}\\
Terzan 2 & 1.6 & 6.6 & --0.5 & --  & R & 2, 13 \\
Terzan 6 & 2.3 & 5.4 & --0.5 & --  & R & 2, 14 \\
UKS 1 &3.6 &10 & --0.78 &+57 & R & 11, 15 \\
ESO456-SC38 & 0.90 &5.5 &--0.5 &--  & R & 2,11 \\
Terzan 1 & 2.5 & 5.2 &--1.3 &114 & R & 16, 17 \\
Palomar 6 &1.36 & 6.40 &--1.0 & 180 & R & 18 \\
Djorgovski 1 &1.70  &5.6 &--0.4 &--  &R & 2, * \\
\noalign{\bf Metal-rich}\\[-3mm]
NGC~6528 &0.46 & 7.7 & --0.1 &212 & R & 19, 20 \\
NGC~6553 &0.7 & 5.1 &--0.2 &-2 & R & 2, 21 \\
Terzan 5 &2.39 &5.6 &--0.3 &-93 & R & 2, 3, 22 \\
Liller 1 & 3.7 & 6 & --0.3 &+64 & R & 20, 23 \\
\noalign{\bf Moderately metal-poor, BHB, located in the ring  6$^{\circ}$ -- 12$^{\circ}$}\\
NGC~6325 & 0.89 &   6.9  &   --1.17 & 29.8  & B & 7, 24, 25 \\
NGC~6355 & 0.75 &   8.8  &  --1.3   & --176.9  &  B  & 7, 24, 25 \\
NGC~6453 & 0.61 &   11.2 &   --1.53 & --83.7  & B & 7, 25 \\
NGC~6626 & 0.40 &   5.7  &  --1.0   & 17.0  &     B & 25 \\
NGC~6642 & 0.41 &   7.2  &  --1.3   & --57.2  &  B  &  7, 26  \\
%NGC~6284 &  &   14.7 &  -1.32  &   &  B    & 7,22 \\
\noalign{\smallskip} \hline \end{tabular}}
\par
\smallskip
References: 1 Ortolani et~al. (\cite{Ortolani97}a);
2 Barbuy et~al. (\cite{Barbuy98}); 3 Origlia \& Rich (\cite{Origlia04}); 4 Ortolani et~al. (\cite{Ortolani99}a);
5 Ortolani et~al. (\cite{Ortolani97}b); 6 Barbuy et~al. (\cite{Barbuy06}a); 7 Piotto et~al. (\cite{Piotto02});
8 Rich et~al. (\cite{Rich98}); 9 Barbuy et~al. (\cite{Barbuy07}); 10 Ortolani et~al. (\cite{Ortolani06}); 
11 Ortolani et~al. (\cite{Ortolani97}c); 12 Bica et~al. (\cite{Bica94}); 
13 Ortolani et~al. (\cite{Ortolani97}d);
14 Barbuy et~al. (\cite{Barbuy97}); 15 Origlia et~al. (\cite{Origlia05});  
16 Ortolani et~al. (\cite{Ortolani99}b); 17~Idiart et~al. (\cite{Idiart02}); 
18 Lee et~al. (\cite{Lee04});
19 Zoccali et~al. (\cite{Zoccali04}); 20~Ortolani et~al. (\cite{Ortolani07}); 21 Alves-Brito et~al. (\cite{AlvesBrito06});
22 Ortolani et~al. (\cite{Ortolani96}); 23 Origlia et~al. (2002); 24 Ortolani et~al. (\cite{Ortolani03});
25 Harris (\cite{Harris96}); 26 Barbuy et~al. (\cite{Barbuy06}b); 27 Present work;
 * Note that Davidge (\cite{Davidge00})
obtained [Fe/H]~=~--2.2 for Djorgovski~1.
\end{table}