Table 5: Compilation of information for each of the JEM-X mosaic images per season and for the whole program (Fig. 4). We report the season which is refered to, the INTEGRAL revolutions corresponding to the season, the total number of single pointings (ScWs), the total exposure time at the center of each mosaic ( $t_{\rm exp}$ ), the effective exposure time ( $t_{\rm eff}$ ) when taking into account vignetting and other effects inherent to the JEM-X instrument (see Lund et al. 2003), and the list of sources which are detected above the 3 $\sigma$ level in the 3-10 keV and 10-25 keV bands during a season or in the average over the whole program. When the detection significance is lower than 3 or a source is not detected we indicate it with (-). The ordering of the sources is the same as in Table 1.
Season 1 2 3 all

Revs 287-307 347-370 406-429 287-429

# ScWs 132 118 141 391

$t_{\rm exp}$ (ks) $\simeq$ 200 $\simeq$ 180 $\simeq$ 195 $\simeq$ 578

$t_{\rm eff}$ (ks) $\simeq$ 135 $\simeq$ 122 $\simeq$ 130 $\simeq$ 379

Source Detection significances [3-10]/[10-25] keV

GX 5-1 150/62 174/82 158/79 276/97

GRS 1758-258 8.4/14 8.4/14 8.5/12 14/17

GX 3+1 150/71 135/57 154/76 259/94

GX 1+4 3.8/6.9 7.5/10 8.6/11.1 11/15

SLX 1735-269 8.3/9.9 11/8.4 7.3/15 15/11

1E 1743.1-2843 9.0/7.7 10/8.6 5.6/4.1 14/9.2

SAX J1747.0-2853 -/- 9.0/- 23/14 16/7.4

SLX 1737-282 4.7/4.0 -/- 3.9/5.1 7.3/6.6

XTE J1739-285 -/- 20/13 21/12 24/10

1A 1742-294 28/24 39/28 25/31 57/38

SLX 1744-229/300 18/12 15/11 12/10 26/15

1E 1740.7-2942 20/24 19/32 -/- 22/29

GRS 1747-312 -/- 7.6/4.4 5.7/4.0 8.0/3.9

GRS 1734-292 -/- -/- -/- 4.6/5.3

H1743-322 -/- 18/8.9 -/- 9.3/3.7

4U 1722-30 14/13 14/11 11/7.0 23/14

MXB 1730-335 4.4/- 5.1/3.4 -/- 5.7/-

GX 354-0 44/29 32/20 41/28 72/35

**Table 5:** Compilation of information for each of the JEM-X mosaic images per season and for the whole program (Fig. 4). We report the season which is refered to, the *INTEGRAL* revolutions corresponding to the season, the total number of single pointings (ScWs), the total exposure time at the center of each mosaic ( $t_{\rm exp}$ ), the effective exposure time ( $t_{\rm eff}$ ) when taking into account vignetting and other effects inherent to the JEM-X instrument (see Lund et al. 2003), and the list of sources which are detected above the 3 $\sigma$ level in the 3-10 keV and 10-25 keV bands during a season or in the average over the whole program. When the detection significance is lower than 3 or a source is not detected we indicate it with (-). The ordering of the sources is the same as in Table 1.
Season	1	2	3	all
Revs	287-307	347-370	406-429	287-429
# ScWs	132	118	141	391
$t_{\rm exp}$ (ks)	$\simeq$ 200	$\simeq$ 180	$\simeq$ 195	$\simeq$ 578
$t_{\rm eff}$ (ks)	$\simeq$ 135	$\simeq$ 122	$\simeq$ 130	$\simeq$ 379
Source	Detection significances [3-10]/[10-25] keV
GX 5-1	150/62	174/82	158/79	276/97
GRS 1758-258	8.4/14	8.4/14	8.5/12	14/17
GX 3+1	150/71	135/57	154/76	259/94
GX 1+4	3.8/6.9	7.5/10	8.6/11.1	11/15
SLX 1735-269	8.3/9.9	11/8.4	7.3/15	15/11
1E 1743.1-2843	9.0/7.7	10/8.6	5.6/4.1	14/9.2
SAX J1747.0-2853	-/-	9.0/-	23/14	16/7.4
SLX 1737-282	4.7/4.0	-/-	3.9/5.1	7.3/6.6
XTE J1739-285	-/-	20/13	21/12	24/10
1A 1742-294	28/24	39/28	25/31	57/38
SLX 1744-229/300	18/12	15/11	12/10	26/15
1E 1740.7-2942	20/24	19/32	-/-	22/29
GRS 1747-312	-/-	7.6/4.4	5.7/4.0	8.0/3.9
GRS 1734-292	-/-	-/-	-/-	4.6/5.3
H1743-322	-/-	18/8.9	-/-	9.3/3.7
4U 1722-30	14/13	14/11	11/7.0	23/14
MXB 1730-335	4.4/-	5.1/3.4	-/-	5.7/-
GX 354-0	44/29	32/20	41/28	72/35

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