Table 2:

The list of X-ray sources detected by SuperAGILE in the period July 2007 - April 2009.

Name	RA	Dec	Average detected flux	Total exposure	Max. sign.	Type	Orbital	Note
	(deg)	(deg)	(mCrab)	(ks)	()		data
SMC X-1	19.271	-73.443	87	140	4.4	HMXB	N
1A 0114+650	19.511	65.292	13	380	5.9	HMXB	N	5-h flare
X Per	58.846	31.045	55	45	4.5	HMXB	Y
SGR 0501+4516	75.278	45.276	-	-	-	SGR	N	Short bursts
LMC X-4	83.207	-66.370	50	400	10.1	HMXB	N
Crab	83.628	22.020	1000	2477	76.4	PWN	Y
Vela X-1	135.512	-40.557	603	1523	47.6	HMXB	Y
GRO J1008-57	152.441	-58.291	56	220	6.0	HMXB	N
Mkn 421	166.114	38.209	40	140	9.4	BL	N
1A 1118-61	170.238	-61.917	475	447	47.6	HMXB	Y
Cen X-3	170.300	-60.638	173	1859	21.3	HMXB	Y
1E 1145.1-6141	176.869	-61.953	44	1010	9.4	HMXB	Y
NGC 4151	182.636	39.405	17	115	6.9	Sy	N
GX 301-2	186.657	-62.770	390	3315	129.9	HMXB	Y
3C 273	187.278	2.052	24	740	21.3	QSO	N
Cen A	201.365	-43.019	60	200	6.6	RG	Y
1E1547.0-5408	237.725	-54.307	-	-	-	AXP	N	Short bursts
4U 1608-522	243.179	-52.423	126	130	8.22	LMXB	Y
Sco X-1	244.979	-15.640	1666	3594	103.0	LMXB	Y
4U 1624-490	247.011	-49.198	139	8	4.6	LMXB	N
IGR J16318-4848	247.966	-48.808	165	360	22.6	HMXB	Y
4U 1626-67	248.070	-67.461	53	2600	11.7	LMXB	Y
4U 1636-536	250.231	-53.751	68	380	8.5	LMXB	Y
GX 340+0	251.448	-45.611	85	908	18.5	LMXB	Y
Her X-1	254.458	35.342	200	122	5.3	HMXB	N
OAO 1657-415	255.199	-41.673	96	530	27.1	HMXB	Y
GX 339-4	255.706	-48.789	105	868	11.3	LMXB	Y
4U 1700-377	255.986	-37.844	357	1179	35.8	HMXB	Y
GX 349+2	256.435	-36.423	117	3110	21.4	LMXB	Y
4U 1702-429	256.563	-43.035	63	561	10.8	LMXB	Y
4U 1705-440	257.226	-44.102	78	805	14.5	LMXB	Y
GX 354-0	262.989	-33.834	61	1977	18.6	LMXB	Y
GX 1+4	263.009	-24.745	64	805	7.8	LMXB	Y
4U 1735-444	264.742	-44.450	47	272	11.8	LMXB	N
1E1740.7-2942	265.978	-29.745	47	1251	11.2	LMXB	Y
IGR J17464-3213	266.565	-32.233	134	536	23.1	LMXB	Y
IGR J17473-2721	266.825	-27.344	37	129	5.3	LMXB	N	X-ray burst
GX 3+1	266.983	-26.563	40	276	10.0	LMXB	Y
AX J1749.1-2639	267.300	-26.647	196	1097	37.2	HMXB	Y
SAX J1750.8-2900	267.600	-29.038	67	137	21.8	LMXB	N	X-ray burst
SWIFTJ1753.5-0127	268.368	-1.453	116	158	6.0	LMXB	N
GX 5-1	270.284	-25.079	137	2621	33.4	LMXB	Y
GRS 1758-258	270.301	-25.743	100	791	28.2	LMXB	N
GX 9+1	270.385	-20.529	50	1260	8.4	LMXB	N
SAX J1808.4-3658	272.115	-36.979	-	-	-	LMXB	N	X-ray burst
SGR 1806-20	272.164	-20.411	-	-	-	SGR	N	Short bursts
SAX J1810.8-2609	272.685	-26.150	35	376	8.4	LMXB	Y
GX 13+1	273.631	-17.157	46	371	5.5	LMXB	Y
1M 1812-121	273.800	-12.083	45	708	7.8	LMXB	Y
GX 17+2	274.006	-14.036	122	2705	22.4	LMXB	Y
4U 1820-303	275.919	-30.361	80	3099	26.6	LMXB	Y
3A 1822-371	276.445	-37.105	53	1016	7.9	LMXB	Y
Ginga 1826-24	277.367	-23.796	84	3316	17.3	LMXB	Y
Ginga 1843+009	281.412	0.891	95	125	5.2	HMXB	N
HETE J1900.1-2455	285.036	-24.920	60	210	7.6	LMXB	Y
GRS 1915+105	288.798	10.946	347	4361	66.8	LMXB	Y
4U 1954+31	298.926	32.097	64	279	13.8	LMXB	Y
Cyg X-1	299.590	35.202	714	7923	161.4	HMXB	Y
EXO 2030+375	308.063	37.638	92	1976	28.7	HMXB	Y
Cyg X-3	308.107	40.958	165	6290	32.8	HMXB	Y
Cyg X-2	326.172	38.322	59	3793	16.1	LMXB	Y

Notes. Average flux (mCrab, 20-60 keV), total exposure and maximum detection significance are based on daily averages. A ``Y'' in the ``orbital data'' column specifies that the source was also detected on an orbital timescale, while the Note column identifies specific integrations (e.g., short transients). The source type is identified according to the following classes: HMXB - High mass X-ray binary; LMXB - Low mass X-ray binary; SGR - soft gamma repeater; PWN - pulsar wind nebula; Sy - Seyfert galaxy; BL - BL Lac; RG - radio galaxy; AXP - Anomalous X-ray pulsar.