\begin{table}%t1
\caption{List of sources in the {\em INTEGRAL}
Galactic bulge monitoring program, ordered by Galactic longitude
(from left to right in the Hammer-Aitoff projection, i.e.,
from 180$^{\circ}$$-$0$^{\circ}$, 360$^{\circ}$$-$180$^{\circ}$).}
\label{sourcelist}
\small%%\centering

\par
\begin{tabular}{l|lllrrlll}
\hline\hline
\multicolumn{1}{l|}{Source} &
\multicolumn{1}{l}{Type} &
\multicolumn{1}{l}{Ref.} &
\multicolumn{1}{l}{Fig.} &
\multicolumn{1}{c}{l$_{\rm II}$} &
\multicolumn{1}{c}{b$_{\rm II}$} &
\multicolumn{1}{c}{RA} &
\multicolumn{1}{c}{Dec} &
\multicolumn{1}{l}{Comment} \\
\hline
GX~17+2                 & LMXB, B, Z         & 1    & \ref{xrb} &  16.432 & $-$0.710 & 18 16 01.4 & $-$14 02 11 & \\
SAX~J1818.6$-$1703      & ?,T                & 1    & &  14.078 &  $-$0.710 & 18 18 39    & $-$17 03.1    & \\
GX~13+1                 & LMXB, B, A         & 1    & \ref{xrb} &  13.517 &    +0.106 & 18 14 31.55 & $-$17 09 26.7 & \\
PKS~1830$-$211          & AGN, QSO           & 1    & &  12.166 &  $-$5.712 & 18 33 39.89 & $-$21 03 39.8 & \\
SGR~1806$-$20           & SGR                & 1    & &   9.996 &  $-$0.242 & 18 08 39.32 & $-$20 24 39.5 & \\
SAX~J1805.5$-$2031      & ?,T                & 2    & &   9.554 &    +0.340 & 18 05 34    & $-$20 30.8    & \\
IGR~J18027$-$2016       & HMXB, T, XP        & 1    & &   9.417 &    +1.044 & 18 02 39.9  & $-$20 17 13   & SAX~J1802.7$-$2017 \\
GS~1826$-$24            & LMXB, B            & 1    & \ref{xrb}, \ref{misc2} &   9.272 &  $-$6.088 & 18 29 28.2  & $-$23 47 49   & Ginga~1826$-$24 \\
GX~9+1                  & LMXB, A            & 1    & \ref{misc} &   9.077 &    +1.154 & 18 01 32.3  & $-$20 31 44   & \\
GX~9+9                  & LMXB, A            & 1    & &   8.513 &    +9.038 & 17 31 44.2  & $-$16 57 42   & 3A~1728$-$169 \\
1RXS~J175113.3$-$201214 & ?                  & 1    & &   8.145 &    +3.408 & 17 51 13.4  & $-$20 12 14   & \\
H1745$-$203              & LMXB, G, B         & 1, 3  & &   7.729 &    +3.798 & 17 48 53.40 & $-$20 21 43.0 & in NGC~6440 \\
IGR~J17597$-$2201       & LMXB, B, D         & 1    & &   7.581 &    +0.775 & 17 59 46    & $-$22 00.9    & XTE~J1759$-$220 \\
XTE~J1818$-$245         & LMXB?, T           & 4    & \ref{misc} &   7.441 &  $-$4.196 & 18 18 25.2  & $-$24 32 31   & \\
1RXS~J174607.8$-$213333 & ?                  & 5    & &   6.367 &    +3.734 & 17 46 07.80 & $-$21 33 33.0 & \\
GX~5$-$1                & LMXB, Z            & 1    & \ref{misc}, \ref{GX_5-1_isgri_jmx}, \ref{GX_5-1_jmx_isgri_cd} &   5.077 &  $-$1.019 & 18 01 08.2  & $-$25 04 45   & \\
V1223~Sgr               & CV                 & 1    & &   4.958 & $-$14.355 & 18 55 02.24 & $-$31 09 48.5 & 1H 1853$-$312 \\
GRS~1758$-$258          & LMXB, BHC          & 1    & \ref{bhc} &   4.508 &  $-$1.361 & 18 01 12.3  & $-$25 44 36   & \\
IGR~J17544$-$2619       & HMXB?, T           & 1    & \ref{misc}, \ref{OMC_lightcurve} &   3.235 &  $-$0.338 & 17 54 25.7  & $-$26 19 58   & \\
H1820$-$303              & LMXB, G, B, A      & 1    & \ref{xrb} &   2.788 &  $-$7.913 & 18 23 40.45 & $-$30 21 40.1 & 4U~1820$-$303; in NGC~6624 \\
IGR~J17331$-$2406       & ?,T                & 6    & &   2.607 &    +4.927 & 17 33 08    & $-$24 06.8    & \\
GX~3+1                  & LMXB, B, A         & 1    & \ref{xrb} &   2.294 &    +0.794 & 17 47 56.0  & $-$26 33 49   & \\
GX~1+4                  & Symb, XP           & 1, 7  & \ref{misc}, \ref{misc2} &   1.937 &    +4.795 & 17 32 02.16 & $-$24 44 44.0 & \\
XTE~J1807$-$294         & LMXB, T, XP        & 1    & &   1.935 &  $-$4.273 & 18 06 59.8  & $-$29 24 30   & \\
AX~J1749.2$-$2725       & HMXB, XP           & 5    & &   1.699 &    +0.108 & 17 49 11.6  & $-$27 25 36   & \\
AX~J1749.1$-$2733       & HMXB?              & 8    & &   1.585 &    +0.051 & 17 49 09.0  & $-$27 33 14   & \\
XB~1832$-$330           & LMXB, G, B, T      & 1    & \ref{xrb} &   1.531 & $-$11.372 & 18 35 44.1  & $-$32 59 29   & in NGC~6652 \\ 
SLX~1735$-$269          & LMXB, B            & 1    & \ref{xrb} &   0.785 &    +2.398 & 17 38 16.00 & $-$27 00 16.0 & \\
XTE~J1748$-$288         & LMXB, T, BHC       & 9    & &   0.676 &  $-$0.222 & 17 48 05.06 & $-$28 28 25.8 & \\
IGR~J17475$-$2822       & Mol cloud?         & 1    & &   0.601 &  $-$0.040 & 17 47 12    & $-$28 26.6    & \\      
EXMS~B1709$-$232        & ?                  & 10    & &   0.594 &    +9.269 & 17 12 31    & $-$23 21.2    & \\      
IGR~J17507$-$2856       & ?,T                & 11   & &   0.576 &  $-$0.959 & 17 50 44    & $-$28 56.3    & \\
Oph~Cluster             & Cluster            & 1    & &   0.564 &    +9.272 & 17 12 26.0  & $-$23 22 33   & \\
IGR~J17419$-$2802       & ?,T                & 12   & &   0.345 &    +1.164 & 17 41 56.0  & $-$28 01 54   & \\
1E~1743.1$-$2843        & LMXB               & 1    & \ref{misc} &   0.251 &  $-$0.026 & 17 46 19.20 & $-$28 44 07.0 & \\
SAX~J1747.0$-$2853      & LMXB, B, T         & 1    & \ref{xrb} &   0.207 &  $-$0.239 & 17 47 02.60 & $-$28 52 58.9 & \\
IGR~J17407$-$2808       & ?,T                & 13   & &   0.115 &    +1.341 & 17 40.7     & $-$28 08      & \\
SLX~1737$-$282          & LMXB, B            & 1    & \ref{xrb} & 359.995 &    +1.201 & 17 40 57.00 & $-$28 18 36.0 & \\
IGR~J17456$-$2901       & ?                  & 1    & & 359.930 &  $-$0.048 & 17 45 38.5  & $-$29 01 15   & AX~J1745.6$-$2900, Sgr A* \\
V2400~Oph               & CV                 & 1    & & 359.867 &    +8.739 & 17 12 36.45 & $-$24 14 44.6 & RX~J1712.6$-$2414 \\
XTE~J1817$-$330         & LMXB, T, BHC       & 14   & \ref{bhc} & 359.817 & $-$7.996 & 18 17 43.54 & $-$33 01 07.8 & \\
XTE~J1739$-$285         & LMXB, T, B         & 1, 15 & \ref{xrb} & 359.714 &    +1.298 & 17 39 53.95 & $-$28 29 46.8 & \\
GRS~1741.9$-$2853       & LMXB, T, B         & 5, 16, 17 & \ref{xrb} & 359.612 &    +0.734 & 17 41 50    & $-$28 52 42   & AX~J1745.0$-$2855 \\
SAX~J1744.7$-$2916      & ?                  & 18   & & 359.600 &  $-$0.009 & 17 44 42    & $-$29 16.9    & \\
KS~1741$-$293           & LMXB, T, B         & 1    & \ref{xrb} & 359.584 &  $-$0.087 & 17 44 58    & $-$29 20.2    & \\
1A~1742$-$294           & LMXB, B            & 1    & \ref{xrb}, \ref{1A_1742-294_isgri_jmx} & 359.559 &  $-$0.389 & 17 46 05.5  & $-$29 30 55   & \\
SLX~1744$-$299/300      & LMXB, B            & 1    & \ref{xrb} & 359.296 &  $-$0.889 & 17 47 25.9  & $-$29 59 58   & \\
1E~1740.7$-$2942        & LMXB, BHC          & 1    & \ref{bhc} & 359.116 &  $-$0.106 & 17 43 54.83 & $-$29 44 42.6 & \\
GRS~1734$-$292          & AGN, Sy1           & 1    & & 358.844 &    +1.395 & 17 37 24.3  & $-$29 10 48   & GRS~1734$-$294 in [1] \\
GRS~1747$-$312          & LMXB, G, T, B      & 1, 19 & & 358.555 &  $-$2.168 & 17 50 45.5  & $-$31 17 32   & in Terzan~6\\
IGR~J17460$-$3047       & ?                  & 1    & & 358.494 &  $-$1.094 & 17 46 19    & $-$30 47.5    & Artefact in [26] \\
IGR~J17391$-$3021       & HMXB, NS, Be?, T   & 1    & & 358.068 &    +0.445 & 17 39 11.58 & $-$30 20 37.6 & XTE~J1739$-$302 \\
IGR~J17285$-$2922       & BHC?, T            & 1    & & 357.630 &    +2.923 & 17 28.5     & $-$29 22      & \\         
H1743$-$322              & LMXB, T, BHC       & 1    & \ref{bhc} & 357.255 &  $-$1.833 & 17 46 15.61  & $-$32 13 59.9    & IGR~J17464$-$3213 \\     
IGR~J17488$-$3253       & ?                  & 1    & & 356.962 &  $-$2.662 & 17 48 54.71 & $-$32 54 44.0 & \\
3A~1822$-$371           & LMXB, XP, D        & 1, 20 & \ref{misc} & 356.850 & $-$11.291 & 18 25 46.8  & $-$37 06 19   & \\  
SLX~1746$-$331          & LMXB?, BHC         & 5, 9 & & 356.807 &  $-$2.973 & 17 49 48.50 & $-$33 12 18.3 & \\
XTE~J1710$-$281         & LMXB, T, B         & 1    & & 356.357 &    +6.922 & 17 10 12.3  & $-$28 07 54   & \\
4U~1722$-$30            & LMXB, G, B, A      & 1    & \ref{xrb} & 356.320 &    +2.298 & 17 27 33.2  & $-$30 48 07   & XB~1724$-$30; in Terzan~2 \\
IGR~J17200$-$3116       & ?,T                & 1    & & 355.022 &    +3.346 & 17 20 06.10 & $-$31 17 02.0 & 1RXS~J172006.1$-$311702 \\
MXB~1730$-$335          & LMXB, G, B, T      & 1    & \ref{xrb} & 354.841 &  $-$0.158 & 17 33 24.10 & $-$33 23 16.0 & The Rapid Burster; in Liller 1 \\
XTE~J1720$-$318         & LMXB, T, BHC       & 1    & & 354.597 &    +3.087 & 17 19 58    & $-$31 46.8    & \\  
GX~354$-$0              & LMXB, B, A         & 1    & \ref{xrb}, \ref{GX354-0_isgri_jmx} & 354.302 &  $-$0.150 & 17 31 57.4  & $-$33 50 05   & 4U 1728$-$337 \\  
\hline
IGR~J17254$-$3257       & LMXB?, B           & 1, 21 & & 354.280 &    +1.472 & 17 25 25.50 & $-$32 57 17.5 & 1RXS~J172525.5$-$325717 \\
1A~1744$-$361           & LMXB, T, B, A?     & 1, 22 & & 354.140 &  $-$4.204 & 17 48 19.22 & $-$36 07 16.6 & XTE~J1748$-$361\\
1H~1746$-$370           & LMXB, G, B, A      & 1    & & 353.531 &  $-$5.005 & 17 50 12.7  & $-$37 03 08   & in NGC~6441 \\
XTE~J1743$-$363         & ?,T                & 1    & \ref{misc} & 353.392 &  $-$3.402 & 17 43 00.0  & $-$36 20 41   & \\
4U~1705$-$32            & LMXB, B            & 1    & & 352.794 &    +4.681 & 17 08 54.40 & $-$32 18 57.5 & \\
IGR~J17252$-$3616       & HMXB, XP, T        & 23, 24 & \ref{misc} & 351.510 &  $-$0.356 & 17 25 14    & $-$36 16.4   & EXO~1722$-$363 \\
IGR~J17098$-$3628       & ?,T                & 25   & \ref{misc}, \ref{misc2} & 349.555 &    +2.066 & 17 09 48    & $-$36 28.2    & \\ 
IGR~J17091$-$3624       & BHC?               & 1    & & 349.519 &    +2.215 & 17 09 06    & $-$36 24.7    & \\
GX~349+2                & LMXB, Z            & 1    & \ref{misc} & 349.104 &    +2.748 & 17 05 44.5  & $-$36 25 23   & Sco X-2 \\  
SAX~J1712.6$-$3739      & LMXB, T, B         & 1    & & 348.935 &    +0.928 & 17 12 34.00 & $-$37 38 36.0 & \\
4U~1700$-$377           & HMXB               & 1    & \ref{misc}, \ref{misc2} & 347.754 &    +2.173 & 17 03 56.77 & $-$37 50 38.9 & \\
GRO~J1655$-$40          & LMXB, T, BH, D     & 9    & \ref{bhc} & 344.982 &    +2.456 & 16 54 00.14 & $-$39 50 44.9 & \\
OAO~1657$-$415          & HMXB, XP           & 1    & \ref{misc} & 344.354 &    +0.311 & 17 00 47.9  & $-$41 40 23   & \\
\hline
\end{tabular}
\smallskip
 NOTE: The source type and the reference from where this information is taken are given.
We further provide the Galactic as well as the J2000.0 equatorial coordinates; these
are taken from the SIMBAD Astronomical Database (except for the sources detected
by {\em ASCA}, i.e., the "AX~J'' sources, which are taken from Sakano et~al.\ \cite{Sakano2002}).
For some sources we give alternative names frequently used in the literature.
Source type classification (after Bird et~al.\ \cite{Bird2006}): ? = unknown type, A = atoll source (neutron
star), AGN = active galactic nucleus, B = burster (neutron star), Be =
B-type emission-line star, BH = black hole (dynamically confirmed),
BHC = black-hole candidate, Cluster = cluster of galaxies, CV =
cataclysmic variable, D = dipping source, G = globular cluster source,
HMXB = high-mass X-ray binary, LMXB = low-mass X-ray binary, Mol cloud
= molecular cloud, NS = neutron star, QSO = quasar, SGR = soft
gamma-ray repeater, Sy = Seyfert galaxy, Symb = Symbiotic binary, T~=
transient source, XP = X-ray pulsar (neutron star), Z = Z-type source
(neutron star). References:
[1]~Bird et~al.\ (\cite{Bird2006}); [2]~Lowes et~al.\ (\cite{Lowes2002}); [3]~Forman et~al.\ (\cite{Forman1976});
[4]~Levine et~al.\ (\cite{Levine2005}); [5]~Revnivtsev et~al.\ (\cite{Revnivtsev2004a});
[6]~Lutovinov et~al.\ (\cite{Lutovinov2004}); [7]~Chakrabarty \&\ Roche (\cite{Chakrabarty1997});
[8]~in~'t~Zand (\cite{Zand2005}); [9]~McClintock \&\ Remillard (\cite{McClintock2006});
[10]~Reynolds et~al.\ (\cite{Reynolds1999}); [11]~Grebenev \&\ Sunyaev (\cite{Grebenev2004b});
[12]~Grebenev et~al.\ (\cite{Grebenev2005c}); [13]~Kretschmar et~al.\ (\cite{Kretschmar2004});
[14]~Remillard et~al.\ (2006); [15]~Brandt et~al.\ (\cite{Brandt2005});
[16]~Cocchi et~al.\ (\cite{Cocchi1999}); [17]~Muno et~al.\ (\cite{Muno2003b});
[18]~in~'t~Zand et~al.\ (\cite{Zand1997}); [19]~in~'t~Zand et~al.\ (\cite{Zand2003});
[20]~Jonker \&\ van der Klis (\cite{Jonker2001});
[21]~Brandt et~al.\ (\cite{Brandt2006}); [22]~Bhattacharyya et~al.\ (\cite{Bhattacharyya2006});
[23]~Zurita Heras et~al.\ (\cite{Zurita2006}); [24]~Thompson et~al.\ (\cite{Thompson2006});
[25]~Grebenev et~al.\ (\cite{Grebenev2005a}); [26]~Bird et~al.\ (\cite{Bird2004}). 
\end{table}