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Table 2

The catalog of sources detected during the INTEGRAL/IBIS 7-year all-sky survey.

Id Name RA Dec F 17 − 60   keV* Type Ref.** Notes***
(deg) (deg) erg   cm-2s-1

1 IGR J00040+7020 1.008 70.322 0.87 ± 0.13 AGN 153,116 Sy2 z=0.096;
2 IGR J00234+6141 5.723 61.700 0.79 ± 0.10 CV 43,50
3 TYCHO SNR 6.334 64.150 0.92 ± 0.10 SNR
4 SWIFT J0025.8+6818 6.387 68.362 1.01 ± 0.12 AGN Sy2 z=0.012;
5 V709 Cas 7.205 59.300 5.85 ± 0.11 CV 36
6 IGR J00291+5934 7.254 59.563 31.29 ± 0.32R261:264        LMXB       
7 IGR J00335+6126 8.397 61.448 0.67 ± 0.10 AGN 149,134 Sy1.5 z=0.105; =IGR J00333+6122
8 87GB003300.9+593328 8.977 59.827 1.40 ± 0.11 AGN 1 Blazar z = 0.086;
9 IGR J00370+6122 9.286 61.386 0.68 ± 0.10        HMXB        45
10 MRK 348 12.181 31.947 9.69 ± 0.52 AGN Sy2 z = 0.01514; NGC 262;
11 1WGA J0053.8-722 13.526  −72.468 2.88 ± 0.50        HMXB       
12 Gamma Cas 14.176 60.712 4.75 ± 0.11 Star
13 SMC X-1 19.299  −73.449 43.96 ± 0.49        HMXB       
14 1A 0114+650 19.516 65.289 13.44 ± 0.12        HMXB       
15 4U0115+63 19.625 63.746 179.47 ± 0.52R667:675        HMXB       
377.17 ± 0.56R238
16 IGR J01363+6610 24.060 66.188 22.07 ± 2.69R185        HMXB        14,52
17 ESO 297- G 018 24.639  −40.020 4.97 ± 0.71 AGN Sy2 z = 0.0252;
18 4U 0142+61 26.630 61.738 2.86 ± 0.16 AXP
19 RJ 0146.9+6121 26.744 61.351 1.71 ± 0.16        HMXB       
20 IGR J01528-0326 28.208  −3.450 1.71 ± 0.19 AGN 55 Sy2 z = 0.01668; MCG -01-05-047;
21 NGC 788 30.277  −6.819 5.17 ± 0.17 AGN Sy2 z = 0.0136;
22 Mrk 1018 31.612  −0.297 1.15 ± 0.18 AGN Sy1 z = 0.04264;
23 IGR J02086-1742 32.141  −17.659 1.33 ± 0.26 AGN 152,192,173 Sy1 z = 0.129;
24 IGR J02095+5226 32.392 52.458 2.64 ± 0.32 AGN Sy1 z = 0.0492; LEDA 138501; 1ES 0206+522;
25 MRK 590 33.640  −0.767 1.12 ± 0.17 AGN Sy1 z = 0.026542;
26 IGR J02164+5126 34.113 51.441 2.21 ± 0.36 AGN 134,135 Sy2 z = 0.422;
27 QSO B0212+73 34.494 73.802 1.78 ± 0.31 AGN z = 2.367; SWIFTJ0218.0+7348;
28 MRK 1040 37.063 31.316 4.01 ± 0.54 AGN Sy1 z = 0.016338; NGC 931
29 IGR J02343+3229 38.599 32.475 3.03 ± 0.43 AGN 144,139 Sy2 z = 0.016195; NGC 973;
30 NGC 0985 38.657  −8.788 1.84 ± 0.19 AGN Sy1.8 z = 0.043143;
31 IGR J02403+6113 40.090 61.222 1.75 ± 0.24        HMXB        V* V615 Cas
32 NGC 1052 40.267  −8.236 1.73 ± 0.20 AGN Sy2 z = 0.004930;
33 NGC 1068 40.687  −0.010 2.11 ± 0.21 AGN Sy2 z = 0.003786;
34 IGR J02448+1442 41.220 14.710 3.02 ± 0.62
35 4U 0241+61 41.262 62.464 3.72 ± 0.25 AGN Sy1 z = 0.044557;
36 IGR J02466-4222 41.644  −42.360 2.88 ± 0.52R446:452 AGN 77,134 XBONG z = 0.0696; MCG -07-06-018;
37 IGR J02501+5440 42.547 54.678 2.02 ± 0.31 AGN 116 Sy2 z = 0.015; =IGR J02504+5443;
LEDA 166445
38 IGR J02524-0829 43.115  −8.486 1.46 ± 0.24 AGN 113 Sy2 z = 0.016758; MCG-02-08-014;
39 NGC 1142 43.804  −0.186 5.16 ± 0.26 AGN Sy2 z = 0.028847; NGC 1144;
40 V* XY Ari 44.038 19.441 2.89 ± 0.52 CV DQ Her type;
41 NGC 1194 45.955  −1.104 1.57 ± 0.32 AGN Sy1 z = 0.013333;
42 PERSEUS CLUSTER 49.973 41.509 3.77 ± 0.24 Cluster Thermal emission dominates;
43 1H 0323+342 51.140 34.168 2.85 ± 0.46R25:300 AGN 28,59 NL Sy1 z = 0.0629;
2MASX J032441.19+341045.9;
44 IGR J03249+4041 51.225 40.698 1.28 ± 0.24 AGN 199 Sy2 z = 0.0476; interacting galaxies
LEDA 097012 and 2MASX J03251221+4042021;
=SWIFT J0324.9+4044; =PBC J0325.1+4042;
=RX J0325.2+4042;
45 GK Per 52.777 43.880 2.51 ± 0.25 CV
46 IGR J03334+3718 53.362 37.313 2.02 ± 0.23 AGN 60,77,144 Sy1 z = 0.05583;
47 NGC 1365 53.428  −36.170 3.74 ± 0.71 AGN Sy1 z = 0.005559;
48 V0332+53 53.751 53.172 562.40 ± 0.49R269:288        HMXB       
49 NRAO 140 54.125 32.308 1.90 ± 0.25 AGN z = 1.258497;
50 ESO 548-81 55.513  −21.241 3.43 ± 0.67 AGN Sy1 z = 0.01448; =SWIFT J0342.0-2115
51 4U 0352+30 58.849 31.036 43.00 ± 0.27        HMXB        X Per;
52 SWIFTJ0407.3+0342 61.837 3.748 2.45 ± 0.39 AGN Sy2 z = 0.089; 3C 105;
53 3C111 64.581 38.013 6.12 ± 0.26 AGN Sy1 z = 0.0485;
54 IGR J04236+0408 65.923 4.136 1.98 ± 0.28 AGN Sy2 z = 0.046149; 2MASX J04234080+0408017;
55 3C 120 68.319 5.350 5.51 ± 0.24 AGN Sy1 z = 0.0331;
56 RX J0440.9+4431 70.270 44.530 1.36 ± 0.22        HMXB        141
57 UGC03142 70.945 28.972 3.65 ± 0.31 AGN Sy1 z = 0.021828; 1RXS J044350.8+285845
58 LEDA 168563 73.044 49.531 2.98 ± 0.24 AGN Sy1 z = 0.029; 1RXS J045205.0+493248;
59 CGCG 420-015 73.362 4.062 1.63 ± 0.19 AGN Sy2 z = 0.02939;
60 ESO 033-G002 74.001  −75.538 1.50 ± 0.22 AGN Sy2 z = 0.018426;
61 IGR J04571+4527 74.290 45.450 1.45 ± 0.22 CV 173 non-magnetic CV; 1RXS J045707.4+452751;
62 IGR J05007-7047 75.203  −70.775 1.46 ± 0.20        HMXB        2 IGR J05009-7044;
63 LEDA 075258 75.537 3.531 0.98 ± 0.17 AGN Sy1 z = 0.01599;
64 V1062 Tau 75.617 24.732 5.64 ± 0.69R102 CV
65 XSS J05054-2348 76.439  −23.840 4.75 ± 0.39 AGN Sy2 z = 0.0350;
66 IRAS 05078+1626 77.705 16.513 6.25 ± 0.22 AGN Sy1 z = 0.017879;
67 4U 0513-40 78.534  −40.069 3.37 ± 0.44        LMXB       
68 AKN 120 79.026  −0.140 4.26 ± 0.17 AGN Sy1 z = 0.0323;
69 ESO 362-18 79.898  −32.658 3.60 ± 0.31 AGN z = 0.012666; SWIFTJ0519.5-3140
70 PICTOR A 79.957  −45.779 3.53 ± 0.65 AGN Sy1 z = 0.035058;
71 PKS0521-36 80.690  −36.470 1.69 ± 0.34 AGN Blazar z = 0.05534; RBS 0644; QSO B0521-365
72 RX J0525.3+2413 81.390 24.220 1.20 ± 0.19 CV 142
73 TV COL 82.356  −32.818 4.94 ± 0.29 CV DQ Her type
74 IGR J05305-6559 82.636  −65.984 1.16 ± 0.19 C76;
75 PKS 0528+134 82.739 13.563 1.15 ± 0.22 AGN? z = 2.07;
76 LMC X-4 83.210  −66.367 25.53 ± 0.19        HMXB        C74;
77 Crab 83.632 22.016 1430.00 ± 0.18 PSR
78 A 0535+262 84.735 26.324 319.59 ± 16.47R831        HMXB       
718.84 ± 0.83R352
79 LMC X-1 84.912  −69.748 4.69 ± 0.19        HMXB       
80 QSO J0539-2839 84.976  −28.665 1.34 ± 0.27 AGN z = 3.103997; SWIFTJ0539.9-2839;
81 PSR 0540-69 85.005  −69.338 2.33 ± 0.18 PSR
82 BY Cam 85.713 60.868 3.50 ± 0.60 CV 36
83 NGC 2110 88.047  −7.456 12.67 ± 0.32 AGN Sy2 z = 0.007579;
84 MCG 8-11-11 88.801 46.437 8.87 ± 0.41 AGN Sy1 z = 0.020484;
85 IRAS 05589+2828 90.601 28.461 3.79 ± 0.21 AGN Sy1 z = 0.033; =SWIFT J0602.2+2829;
86 IGR J06058-2755 91.471  −27.931 1.54 ± 0.32 AGN 173 Sy 1.5 z = 0.090; 1RXS J060548.1-275439;
87 ESO 005- G 004 92.575  −86.554 3.99 ± 0.59R99 AGN Sy2 z = 0.006384;
88 MRK 3 93.908 71.036 6.82 ± 0.29 AGN Sy2 z = 0.013443;
89 4U 0614+091 94.282 9.139 27.93 ± 0.41        LMXB       
90 IGR J06233-6436 95.847  −64.605 1.22 ± 0.22 AGN Sy1 z = 0.128889; PMN J0623-6436
91 IGR J06239-6052 95.936  −60.974 1.64 ± 0.28 AGN 111 Sy2 z = 0.04052; ESO 121-IG 028
92 ESO490-IG026 100.060  −25.890 2.89 ± 0.60 AGN Sy1.2 z = 0.0248; =SWIFT J0640.4-2554
93 IGR J06415+3251 100.380 32.850 3.66 ± 0.41 AGN 143 Sy2 z = 0.017195; =Swift J0641.3+3257;
94 MRK 6 103.048 74.423 4.07 ± 0.26 AGN Sy1 z = 0.018676;
95 2E 0655.8-0708 104.557  −7.218 4.65 ± 0.38        HMXB       
96 IGR J07264-3553 111.595  −35.900 2.31 ± 0.48 AGN Sy2 z = 0.029624; LEDA 096373;
97 SWIFT J0732.5-1331 113.120  −13.490 2.08 ± 0.34 CV 115,133,129 DQ Her type
98 EXO 0748-676 117.146  −67.754 32.06 ± 0.33        LMXB       
99 IGR J07563-4137 119.055  −41.638 1.18 ± 0.17 AGN 44,2 Sy2 z = 0.021; =IGR J07565-4139;
100 IGR J07597-3842 119.934  −38.727 2.92 ± 0.19 AGN 13,8 Sy1.2 z = 0.04;
101 ESO 209-G012 120.496  −49.734 1.64 ± 0.16 AGN Sy1 z = 0.039587;
102 Vela pulsar 128.835  −45.182 9.98 ± 0.11 PSR
103 4U 0836-429 129.354  −42.894 21.50 ± 0.12        LMXB       
104 FAIRALL 1146 129.621  −35.983 1.68 ± 0.18 AGN Sy1 z = 0.031789;
105 IGR J08390-4833 129.728  −48.556 0.92 ± 0.12 CV 118,157
106 S5 0836+71 130.340 70.902 2.89 ± 0.22 AGN 1 z = 2.1720;
107 IGR J08557+6420 133.944 64.349 1.35 ± 0.27 AGN 173 Likely Sy2 z = 0.037; SWIFT J0855.6+6425;
108 Vela X-1 135.531  −40.555 307.11 ± 0.13        HMXB       
109 IGR J09026-4812 135.648  −48.221 1.91 ± 0.12 AGN 154 Sy1 z = 0.0391;
110 IRAS 09149-6206 139.043  −62.330 1.98 ± 0.21 AGN Sy1 z = 0.05715;
111 X 0918-548 140.102  −55.196 4.22 ± 0.15        LMXB       
112 SWIFT J0920.8-0805 140.213  −8.086 2.80 ± 0.58 AGN Sy2 z = 0.019827; MCG-01-24-012;
113 IGR J09251+5219 141.274 52.331 4.86 ± 1.01 AGN Sy1 z = 0.035398; Mrk 110;
114 IGR J09253+6929 141.321 69.488 1.27 ± 0.23 AGN 127 Sy1.5 z = 0.039;
115 NGC 2992 146.431  −14.335 5.56 ± 0.39 AGN Sy1 z = 0.00771;
116 MCG-5-23-16 146.916  −30.947 11.52 ± 0.39 AGN Sy2 z = 0.008226; ESO 434-G040;
117 IGR J09522-6231 148.025  −62.523 1.20 ± 0.17 AGN 77,101,116 Sy1.9 z = 0.252; =IGR J09523-6231
118 NGC 3081 149.859  −22.816 4.45 ± 0.42 AGN Sy2 z = 0.007956;
119 GRO J1008-57 152.447  −58.298 19.48 ± 0.31R200:203        HMXB        184
43.28 ± 3.29R372
120 IGR J10095-4248 152.449  −42.800 2.03 ± 0.27 AGN ESO 263-G013; Sy2 z = 0.032859;
121 IGR J10100-5655 152.529  −56.914 1.23 ± 0.14        HMXB        62,8
122 IGR J10109-5746 152.753  −57.795 1.59 ± 0.14 CV 23,67 RXP J101103.0-574810; Symbiotic binary
123 NGC 3227 155.876 19.867 8.30 ± 0.69 AGN Sy1 z = 0.00365;
124 NGC 3281 157.935  −34.855 4.65 ± 0.47 AGN Sy2 z = 0.011475;
125 3U 1022-55 159.401  −56.801 12.38 ± 0.58R529:530        HMXB       
126 IGR J10386-4947 159.676  −49.789 1.29 ± 0.20 AGN 20 SWIFT J1038.8-4942; Sy1 z = 0.060;
127 IGR J10404-4625 160.124  −46.391 2.29 ± 0.27 AGN 44,4 LEDA 93974; Sy2 z = 0.024027;
128 eta Car 161.189  −59.719 0.87 ± 0.13 Star
129 IGR J10447-6027 161.196  −60.454 0.88 ± 0.13 128,196 2MASSJ10445192-6025115;
130 Mrk 421 166.114 38.209 28.12 ± 0.22 AGN Blazar z = 0.03;
131 NGC 3516 166.698 72.569 4.28 ± 0.30 AGN Sy1 z = 0.008816;
132 IGR J11187-5438 169.580  −54.660 0.74 ± 0.14 XRB 139
133 IGR J11203+4531 170.090 45.530 5.27 ± 0.75R74:76
134 Cen X-3 170.306  −60.628 68.04 ± 0.13        HMXB       
135 IGR J11215-5952 170.429  −59.869 4.86 ± 0.40R197:198        HMXB        12,56,165 SFXT
15.07 ± 0.82R88
79.95 ± 4.16R308
136 IGR J11305-6256 172.779  −62.945 3.69 ± 0.13        HMXB        34,4,120
137 IGR J11321-5311 173.047  −53.200 49.33 ± 3.80R330 58
138 IGR J11361-6003 174.030  −60.060 0.72 ± 0.13 AGN 116 LINER Sy2 z = 0.014; =IGR J11366-6002;
139 NGC 3783 174.739  −37.766 11.71 ± 1.44 AGN Sy1 z = 0.009647;
140 IGR J11395-6520 174.858  −65.406 9.16 ± 0.93R88:90 RS CVn? HD 101379;
141 IGR J11435-6109 176.031  −61.106 4.04 ± 0.13        HMXB        14,18,120,179
142 IGR J11459-6955 176.478  −69.924 1.13 ± 0.20 AGN 173 Sy 1.2, z = 0.244; SWIFT J1145.6-6956;
2MASS J11455362-6954017;
143 A 1145.1-6141 176.870  −61.956 27.16 ± 0.13        HMXB        C144;
144 4U 1145-619 177.000  −62.207 3.28 ± 0.13        HMXB        C143;
145 IGR J12009+0648 180.240 6.810 1.55 ± 0.24 AGN Sy2 z = 0.035948;
2MASX J12005792+0648226;
146 IGR J12026-5349 180.686  −53.823 3.15 ± 0.17 AGN 23,2,158 WKK0560; Sy2 z = 0.028368;
147 NGC 4051 180.781 44.525 2.67 ± 0.21 AGN Sy1 z = 0.00216;
148 NGC 4138 182.352 43.672 1.76 ± 0.20 AGN Sy1 z = 0.002955;
149 NGC 4151 182.634 39.408 30.52 ± 0.18 AGN Sy1 z = 0.003262;
150 IGR J12107+3822 182.681 38.381 1.14 ± 0.18 AGN 137,173 Sy1.5 z = 0.0229; SWIFT J1210.7+3819;
151 1ES 1210-646 183.269  −64.917 1.19 ± 0.14        HMXB        168
152 IGR J12134-6015 183.374  −60.265 0.63 ± 0.13 1RXS J121324.5-601458;
153 NGC 4235 184.291 7.191 0.95 ± 0.19 AGN Sy1 z = 0.007772;
154 NGC 4253 184.592 29.825 1.47 ± 0.23 AGN Sy1 z = 0.012662; =QSO B1215+300;
155 NGC 4258 184.747 47.309 1.31 ± 0.26 AGN LINER Sy1.9 z = 0.001541; =M 106;
156 PKS 1219+04 185.588 4.230 1.35 ± 0.17 AGN z = 0.965001;
157 MRK 50 185.860 2.676 1.31 ± 0.16 AGN Sy1 z = 0.023196;
158 NGC 4388 186.444 12.664 17.76 ± 0.24 AGN Sy2 z = 0.008426;
159 NGC 4395 186.462 33.565 1.33 ± 0.19 AGN Sy1 z = 0.00101;
160 GX 301-2 186.651  −62.772 259.13 ± 0.13        HMXB       
161 XSS J12270-4859 186.978  −48.907 1.95 ± 0.23 CV 63
162 3C273 187.271 2.050 18.52 ± 0.15 AGN z = 0.15834;
163 IGR J12349-6434 188.724  −64.565 4.44 ± 0.14 SymbStr 17,68 V* RT Cru;
164 NGC 4507 188.908  −39.905 11.52 ± 0.34 AGN Sy2 z = 0.011771;
165 ESO 506-G027 189.727  −27.308 4.02 ± 0.71 AGN Sy2 z = 0.025208;
166 IGR J12391-1612 189.792  −16.186 3.03 ± 0.31 AGN 23,2 LEDA 170194; Sy2 z = 0.0367;
XSS 12389-1614;
167 NGC 4593 189.910  −5.347 5.51 ± 0.16 AGN Sy1 z = 0.0090;
168 WKK 1263 190.356  −57.841 1.79 ± 0.14 AGN Sy1.5 z = 0.024; =IGR J12415-5750
169 IGR J12480-5829 192.020  −58.497 0.84 ± 0.14 AGN 152,161,173 Sy1.9 z = 0.028; =IGR J1248.2-5828;
170 4U 1246-588 192.386  −59.090 4.29 ± 0.14        LMXB        40,110
171 NGC 4748 193.052  −13.415 1.25 ± 0.25 AGN Sy1 z = 0.013753;
172 3C279 194.030  −5.779 1.24 ± 0.18 AGN z = 0.53620;
173 2S 1254-690 194.392  −69.296 2.87 ± 0.17        LMXB        41
174 Coma 194.865 27.938 2.22 ± 0.20 Cluster
175 4U 1258-61 195.322  −61.602 1.97 ± 0.13        HMXB        V* V850 Cen
176 1RXP J130159.6-635806 195.495  −63.969 2.55 ± 0.13        HMXB        51 C177;
177 PSR B1259-63 195.699  −63.836 1.17 ± 0.13        HMXB        C176;
178 IGR J13042-0534 196.054  −5.574 0.96 ± 0.20 AGN Sy2 z = 0.003696; NGC 4941;
1RXS J130413.2-053304;
179 NGC 4939 196.095  −10.336 1.59 ± 0.24 AGN Sy2 z = 0.010374;
180 NGC 4945 196.364  −49.470 18.43 ± 0.19 AGN Sy2 z = 0.001908;
181 ESO 323-G077 196.607  −40.423 2.26 ± 0.22 AGN Sy2 z = 0.014904;
182 IGR J13091+1137 197.270 11.619 2.98 ± 0.27 AGN 23,2 NGC 4992; Sy2 z = 0.025201;
183 IGR J13109-5552 197.689  −55.865 1.84 ± 0.15 AGN 23,116 PMN J1310-5552; Sy1 z = 0.104;
184 IGR J13149+4422 198.743 44.389 1.53 ± 0.29 AGN 164,139 Mrk 248; Sy2 z = 0.036698;
185 IGR J13168-7157 199.210  −71.951 0.84 ± 0.17 AGN 172,173 Sy1.5 z = 0.0705; SWIFT J1316.9-7155l;
1RXS J131651.8-715537;
186 IGR J13186-6257 199.650  −62.947 1.15 ± 0.13 HMXB? 131,136
187 MCG-03-34-064 200.602  −16.728 2.50 ± 0.47 AGN Sy2 z = 0.017092;
188 Cen A 201.363  −43.019 63.63 ± 0.19 AGN Sy2 z = 0.001830;
189 4U 1323-619 201.643  −62.136 12.38 ± 0.13        LMXB       
190 IGR J13290-6323 202.268  −63.392 3.23 ± 0.50R92
191 ESO 383-G018 203.332  −34.030 1.58 ± 0.21 AGN Sy2 z = 0.013;
192 MCG-6-30-15 203.990  −34.288 3.87 ± 0.21 AGN ESO 383-G035; Sy1 z = 0.007892;
193 NGC 5252 204.564 4.528 6.66 ± 0.22 AGN Sy2 z = 0.022219;
194 MRK 268 205.420 30.395 1.72 ± 0.28 AGN Sy2 z = 0.040408;
195 IGR J13466+1921 206.670 19.360 1.60 ± 0.30 1RXS J134628.5+192310
196 4U 1344-60 206.894  −60.615 5.85 ± 0.13 AGN Sy1.5 z = 0.013;
197 IC 4329A 207.333  −30.309 17.95 ± 0.25 AGN Sy1 z = 0.016024; =ESO 445-50
198 LEDA 49418 208.567  −37.779 0.90 ± 0.18 AGN Sy2 z = 0.051602;
199 IGR J14003-6326 210.204  −63.414 1.19 ± 0.13 PWN 57,136,194 ms pulsar
200 Circinus galaxy 213.290  −65.342 16.80 ± 0.14 AGN Sy2 z = 0.001421;
201 NGC 5506 213.312  −3.220 14.68 ± 0.32 AGN Sy2 z = 0.006068;
202 IGR J14175-4641 214.296  −46.671 1.13 ± 0.16 AGN 23,8 Sy2 z = 0.076;
203 NGC 5548 214.541 25.155 2.75 ± 0.46 AGN Sy1 z = 0.01668;
204 ESO 511-G030 214.885  −26.633 2.46 ± 0.30 AGN Sy1 z = 0.022242;
205 4U 1416-62 215.303  −62.698 1.11 ± 0.13        HMXB       
206 H 1426+428 217.070 42.660 2.18 ± 0.34 AGN Blazar z = 0.129; 1ES1426+428
207 IGR J14298-6715 217.388  −67.251 1.17 ± 0.15        LMXB        57,116
208 NGC 5643 218.169  −44.174 1.02 ± 0.15 AGN Sy2 z = 0.003943;
209 IGR J14331-6112 218.273  −61.221 0.92 ± 0.13        HMXB        57,116
210 NGC 5728 220.599  −17.253 4.40 ± 0.51 AGN Sy2 z = 0.009467;
211 IGR J14471-6414 221.528  −64.284 0.88 ± 0.14 AGN 57,116 Sy1.2 z = 0.053;
212 IGR J14471-6319 221.834  −63.289 0.78 ± 0.13 AGN 23,8 Sy2 z = 0.038;
213 IGR J14488-4009 222.201  −40.152 0.85 ± 0.16
214 IGR J14493-5534 222.311  −55.589 1.47 ± 0.14 AGN 101 2MASX J14491283-5536194;
215 IGR J14515-5542 222.887  −55.691 1.62 ± 0.14 AGN 62,8 WKK 4374; Sy2 z = 0.018;
216 IGR J14536-5522 223.421  −55.363 1.26 ± 0.14 CV 62,63,156 Polar
217 IGR J14552-5133 223.846  −51.571 1.28 ± 0.15 AGN 23,8 WKK 4438; Sy1 z = 0.016;
218 IGR J14561-3738 224.055  −37.632 1.14 ± 0.16 AGN 101 ESO 386- G 034; Sy2 z = 0.024;
219 IC 4518A 224.427  −43.125 2.11 ± 0.15 AGN Sy2 z = 0.016261;
220 Mrk 841 226.005 10.438 3.07 ± 0.44 AGN Sy1 z = 0.03642;
221 IGR J15094-6649 227.382  −66.816 1.71 ± 0.16 CV 23,63
222 PSR 1509-58 228.480  −59.145 12.67 ± 0.14 PSR
223 SWIFT J1513.8-8125 228.567  −81.415 1.42 ± 0.29 AGN 132,173 Sy1.2 z = 0.0684; 2MASX J15144217-8123377;
224 4U 1516-569 230.167  −57.168 7.72 ± 0.13        LMXB       
225 IGR J15360-5750 234.014  −57.806 1.36 ± 0.14 AGN? 23,195 =IGR J15359-5750;
226 IGR J15414-5030 235.350  −50.512 0.87 ± 0.13 CV? 136 Galactic source; =IGR J15415-5029;
227 4U 1538-522 235.600  −52.385 23.42 ± 0.13        HMXB       
228 XTE J1543-568 236.011  −56.748 14.97 ± 1.12R468        HMXB       
16.12 ± 0.82R37:38
229 4U 1543-624 236.964  −62.578 3.15 ± 0.16        LMXB       
230 NY Lup 237.052  −45.472 6.04 ± 0.14 CV 1RXS J154814.5-452845
231 NGC 5995 237.104  −13.758 3.12 ± 0.24 AGN Sy2 z = 0.025091;
232 XTE J1550-564 237.751  −56.474 328.23 ± 0.46R54:60        LMXB       
233 IGR J15529-5029 238.233  −50.490 0.61 ± 0.12 CV? 136 Galactic source
234 IGR J15539-6142 238.468  −61.676 0.78 ± 0.16 AGN 57,102 ESO 136-6; Sy2 z = 0.014997;
235 ESO 389- G 002 238.693  −37.604 1.00 ± 0.19 AGN 173 Sy2 z = 0.0194; =IGR J15549-3740;
236 4U 1556-605 240.363  −60.716 1.18 ± 0.16        LMXB       
237 IGR J16058-7253 241.470  −72.900 1.71 ± 0.23 SWIFT J1605.9-7250?; IRAS F15596-7245?;
238 WKK 6092 242.981  −60.637 1.68 ± 0.16 AGN Sy1 z = 0.016; =IGR J16119-6036
239 4U 1608-522 243.177  −52.425 21.69 ± 0.12        LMXB       
240 IGR J16167-4957 244.162  −49.975 2.10 ± 0.12 CV 86,36 1RXS J161637.2-495847;
241 IGR J16175-5059 244.357  −50.972 0.59 ± 0.12 PSR PSR J1617-5055
242 IGR J16185-5928 244.635  −59.468 1.25 ± 0.15 AGN 23,8 WKK 6471; Sy1 z = 0.035;
243 IGR J16195-2807 244.871  −28.151 3.23 ± 0.28        LMXB        44,108,197 SyXB; =IGR J16194-2810;
1RXS J161933.6-280736;
244 IGR J16195-4945 244.893  −49.755 2.38 ± 0.12        HMXB        86,83 AX J161929-4945;
245 Sco X-1 244.981  −15.637 1142.08 ± 0.20        LMXB       
246 IGR J16207-5129 245.194  −51.505 3.92 ± 0.12        HMXB        86,83
247 SWIFT J1626.6-5156 246.659  −51.938 17.47 ± 1.33R398:407        LMXB        78
248 4U 1624-49 247.002  −49.209 5.10 ± 0.12        LMXB       
249 IGR J16283-4838 247.034  −48.652 1.08 ± 0.12        HMXB        125,105
250 IGR J16287-5021 247.175  −50.343 0.86 ± 0.12        LMXB        124,173
251 IGR J16293-4603 247.311  −46.076 0.59 ± 0.12        LMXB        197 SyXB?
252 IGR J16318-4848 247.953  −48.819 35.22 ± 0.12        HMXB        84,85
253 IGR J16320-4751 248.013  −47.876 20.35 ± 0.12        HMXB        87,25 AX J1631.9-4752
254 4U 1626-67 248.076  −67.466 20.63 ± 0.24        LMXB       
255 IGR J16336-4733 248.396  −47.559 10.08 ± 0.12 C256;
256 4U 1630-47 248.503  −47.391 31.58 ± 0.12        LMXB        C255,258;
257 ESO 137-G34 248.790  −58.088 1.40 ± 0.15 AGN Sy2 z = 0.009113;
258 IGR J16358-4726 248.992  −47.407 19.58 ± 0.83R54:57        HMXB        88,89,193 C256;
63.25 ± 7.87R185
259 Triangulum A 249.567  −64.347 1.55 ± 0.22 Cluster z = 0.051;
260 IGR J16385-2057 249.630  −20.920 1.15 ± 0.19 AGN 1RXSJ163830.9-205520; Sy1 z = 0.0269;
261 AX J163904-4642 249.768  −46.707 5.53 ± 0.12        HMXB        90
262 4U 1636-536 250.230  −53.751 38.49 ± 0.13        LMXB       
263 IGR J16418-4532 250.465  −45.534 5.23 ± 0.12        HMXB        91,37
264 GX 340+0 251.449  −45.616 41.27 ± 0.12        LMXB       
265 IGR J16465-4507 251.648  −45.118 6.64 ± 0.48R222:224        HMXB        11,93 C266;
13.63 ± 0.75R232:233
266 IGR J16479-4514 252.015  −45.207 5.17 ± 0.12        HMXB        92,93,197 2MASS J16480656-4512068;
267 IGR J16482-3036 252.058  −30.591 3.12 ± 0.14 AGN 44,4 2MASX J16481523-3035037; Sy1 z = 0.031;
268 IGR J16493-4348 252.362  −43.819 2.58 ± 0.12        HMXB        106,117 2MASS J16492695-4349090;
269 IGR J16500-3307 252.493  −33.113 1.76 ± 0.13 CV 44,116,197 IP; 1RXS J164955.1-330713;
270 NGC 6221 253.120  −59.215 1.59 ± 0.18 AGN Sy2 z = 0.004750;
May contain flux from ESO 138-G1;
271 NGC 6240 253.305 2.429 4.19 ± 0.31 AGN LIRG z = 0.024323;
272 MKN 501 253.464 39.751 6.47 ± 0.32 AGN BL Lac z = 0.033640;
273 GRO J1655-40 253.499  −39.844 15.55 ± 0.13        LMXB       
274 IGR J16547-1916 253.682  −19.275 1.07 ± 0.17 CV 173,198 IP; RXS J165443.5-191620;
275 IGR J16558-5203 254.032  −52.078 2.41 ± 0.13 AGN 86,8 Sy1.2 z = 0.054;
276 IGR J16562-3301 254.073  −33.045 2.16 ± 0.12 AGN 112 BL Lac; SWIFT J1656.3-3302;
277 Her X-1 254.455 35.343 118.05 ± 0.29        LMXB       
278 AX J1700.2-4220 255.082  −42.335 1.98 ± 0.12        HMXB        63
279 OAO 1657-415 255.199  −41.656 93.57 ± 0.12        HMXB       
280 XTE J1701-462 255.232  −46.197 5.81 ± 0.13        LMXB        outburst activity rev.400-550
281 IGR J17009+3559 255.250 35.990 1.65 ± 0.29 AGN 140,173 XBONG z = 0.113;
282 GX 339-4 255.705  −48.792 69.48 ± 0.13        LMXB       
283 IGR J17036+3734 255.910 37.570 1.56 ± 0.30
284 4U 1700-377 255.984  −37.842 299.44 ± 0.11        HMXB       
285 GX 349+2 256.431  −36.421 60.56 ± 0.11        LMXB       
286 IGR J17062-6143 256.556  −61.715 1.72 ± 0.23 151 =SWIFT J1706.6-6146
287 4U 1702-429 256.566  −43.037 22.65 ± 0.13        LMXB       
288 1RXS J170849.0-400910 257.214  −40.142 1.55 ± 0.12 AXP
289 4U 1705-32 257.223  −32.322 2.72 ± 0.10        LMXB       
290 4U 1705-440 257.234  −44.102 27.83 ± 0.13        LMXB       
291 IGR J17091-3624 257.308  −36.408 6.20 ± 0.11        LMXB        94,24 C293;
292 XTE J1709-267 257.386  −26.658 19.10 ± 0.72R171:172        LMXB       
293 IGR J17098-3628 257.438  −36.460 27.64 ± 0.42R298:305 103,185 C291;
294 XTE J1710-281 257.549  −28.128 3.56 ± 0.10        LMXB       
295 RX J1713.7-3946 257.991  −39.862 0.57 ± 0.12 SNR G347.3-0.5;
296 Oph cluster 258.114  −23.347 5.29 ± 0.11 Cluster
297 4U 1708-40 258.120  −40.858 1.06 ± 0.12        LMXB       
298 V2400 Oph 258.149  −24.244 3.59 ± 0.10 CV
299 SAX J1712.6-3739 258.153  −37.645 5.90 ± 0.11        LMXB       
300 KS 1716-389 259.003  −38.879 2.16 ± 0.38R36:63        HMXB        48,49,197 XTE J1716-389;
301 NGC 6300 259.244  −62.830 5.12 ± 0.26 AGN Sy2 z = 0.003706;
302 IGR J17195-4100 259.911  −41.023 2.82 ± 0.12 CV 86,36 1RXS J171935.6-410054;
303 IGR J17197-3010 259.930  −30.180 0.50 ± 0.09
304 XTE J1720-318 259.993  −31.753 33.49 ± 0.49R56:63        LMXB       
305 IGR J17200-3116 260.022  −31.294 2.39 ± 0.09        HMXB        86,8 1RXS J172006.1-311702;
306 IGR J17204-3554 260.087  −35.900 0.82 ± 0.10 AGN 44,27
307 IGR J17233-2837 260.850  −28.620 0.82 ± 0.08
308 EXO 1722-363 261.295  −36.282 11.04 ± 0.09        HMXB       
309 IGR J17254-3257 261.354  −32.953 2.17 ± 0.08        LMXB        86,70 1RXS J172525.5-325717;
310 IGR J17269-4737 261.681  −47.647 17.95 ± 2.01R364 XRB 73 XTE J1726-476;
311 4U 1724-30 261.888  −30.804 27.16 ± 0.08        LMXB        Terzan 2;
312 IGR J17285-2922 262.163  −29.370 5.07 ± 0.51R119:122 LMXB? 86,35 XTE J1728-295;
313 IGR J17303-0601 262.579  −5.971 4.24 ± 0.21 CV 86,72 1RXS J173021.5-055933;
314 GX 9+9 262.934  −16.952 15.64 ± 0.13        LMXB       
315 GX 354-0 262.988  −33.833 62.19 ± 0.08        LMXB       
316 IGR J17320-1914 263.001  −19.195 1.23 ± 0.11 CV 36 V2487 Oph;
317 GX 1+4 263.011  −24.747 80.62 ± 0.08        LMXB       
318 IGR J17331-2406 263.291  −24.142 0.58 ± 0.08 64,195
319 RapidBurster 263.349  −33.387 5.01 ± 0.08        LMXB       
320 IGR J17350-2045 263.740  −20.754 0.92 ± 0.10
321 IGR J17353-3539 263.830  −35.663 1.10 ± 0.09 HMXB? 124 Galactic source
322 IGR J17353-3257 263.848  −32.934 1.45 ± 0.08 HMXB? 22,136 =IGR J17354-3255;
323 GRS 1734-292 264.371  −29.139 7.36 ± 0.08 AGN 29 Sy1 z = 0.021400;
324 IGR J17379-3747 264.465  −37.774 11.13 ± 1.36R165 178 Burster;
325 SLX 1735-269 264.571  −26.991 15.45 ± 0.08        LMXB       
326 4U 1735-444 264.748  −44.453 32.73 ± 0.15        LMXB       
327 IGR J17391-3021 264.812  −30.355 1.34 ± 0.08        HMXB        6,15 XTE J1739-302;
328 GRS 1736-297 264.899  −29.736 4.79 ± 0.43R479:484        LMXB        29
6.35 ± 0.51R408:409
329 XTE J1739-285 264.975  −28.496 2.15 ± 0.07        LMXB        5 C331;
330 IGR J17402-3656 265.087  −36.936 1.00 ± 0.09 HMXB? 136 =IGR J17404-3655;
331 SLX 1737-282 265.168  −28.313 5.59 ± 0.07        LMXB        C329,47,334;
332 IGR J17407-2808 265.175  −28.133 2.11 ± 0.07        HMXB        16,10 C331; 2RXP J174040.9-280852;
333 2E 1739.1-1210 265.484  −12.188 2.25 ± 0.16 AGN IGR J17418-1212; Sy1 z = 0.037;
334 IGR J17419-2802 265.485  −28.031 6.37 ± 0.45R425:426 61 C331,332;
9.41 ± 0.58R361:362
10.56 ± 0.67R409
335 IGR J17427-3018 265.696  −30.301 0.39 ± 0.08 AX J1742.6-3022
336 XTE J1743-363 265.753  −36.377 3.01 ± 0.09        HMXB        10,182,197 SFXT?
337 1E 1740.7-294 265.976  −29.748 44.53 ± 0.07        LMXB        C340,344;
338 IGR J17445-2747 266.082  −27.772 3.85 ± 0.33R165:173 44
339 IGR J17448-3231 266.190  −32.528 0.56 ± 0.08 SNR 136 C345;
340 KS 1741-293 266.242  −29.337 6.02 ± 0.07        LMXB        C337;
341 GRS 1741.9-2853 266.250  −28.917 4.35 ± 0.07        LMXB        186 C342,343,346,347;
342 IGR J17456-2901 266.401  −29.026 8.16 ± 0.07 NucStrCl 79,76 C340,341,343,346,347; =AX J1745.6-2901;
Nuclear stellar cluster;
343 1E 1742.8-2853 266.500  −28.914 8.36 ± 0.07        LMXB        C341,342,346,347;
344 A 1742-294 266.517  −29.508 19.00 ± 0.07        LMXB        C337;
345 IGR J17464-3213 266.564  −32.237 22.46 ± 0.08        LMXB        95 H1743-322/XTE J1746-322;
346 1E 1743.1-2843 266.580  −28.735 6.82 ± 0.07        LMXB        C347,343;
347 SAX J1747.0-2853 266.761  −28.883 4.75 ± 0.07        LMXB        C341,342,343,346;
348 IGR J17464-2811 266.817  −28.180 2.25 ± 0.07        LMXB        148,147 C351; Neutron star LMXB
349 SLX 1744-299/300 266.834  −30.010 10.37 ± 0.07        LMXB        C344;
350 IGR J17473-2721 266.841  −27.352 91.27 ± 0.57R667:725        LMXB        74,123
351 IGR J17475-2822 266.864  −28.364 3.22 ± 0.07 MolCld 21 C348; SgrB2;
352 IGR J17475-2253 266.901  −22.862 1.33 ± 0.08 AGN 137 Sy1 z = 0.0463;
353 GX 3+1 266.983  −26.563 15.84 ± 0.07        LMXB        C359;
354 A 1744-361 267.052  −36.133 16.99 ± 0.60R181:185        LMXB        181
355 4U 1745-203 267.217  −20.359 15.26 ± 0.68R120        LMXB       
356 IGR J17488-3253 267.223  −32.907 1.52 ± 0.08 AGN 86,8 Sy1 z = 0.020;
357 AX J1749.1-2733 267.275  −27.550 1.70 ± 0.07        HMXB        114,183 C358;
358 AX J1749.2-2725 267.292  −27.421 1.43 ± 0.07        HMXB        188 C357;
359 GRO J1750-27 267.300  −26.647 1.76 ± 0.07        HMXB        C353;
360 IGR J17497-2821 267.415  −28.360 3.81 ± 0.07        LMXB        121,169
361 SLX 1746-331 267.477  −33.201 9.14 ± 0.27R106:112        LMXB        BH X-ray transient
362 4U 1746-37 267.548  −37.046 3.14 ± 0.09        LMXB       
363 SAX J1750.8-2900 267.600  −29.038 50.96 ± 1.11R670:674        LMXB        160 C365;
364 IGR J17505-2644 267.636  −26.744 0.81 ± 0.07
365 IGR J17507-2856 267.677  −28.909 3.53 ± 0.48R236:237 104 C363;
366 GRS 1747-313 267.689  −31.284 1.73 ± 0.08        LMXB        29 Terzan 6;
367 XTE J1751-305 267.816  −30.616 10.56 ± 0.79R299        LMXB        189 ms-pulsar
21.98 ± 0.92R546
368 IGR J17513-2011 267.820  −20.184 1.36 ± 0.09 AGN 44,8 Sy1.9 z = 0.047;
369 SWIFT J1753.5-0127 268.361  −1.452 87.62 ± 0.17        LMXB        155
370 AX J1754.2-2754 268.495  −28.026 0.45 ± 0.07        LMXB        176,177
371 IGR J17544-2619 268.619  −26.325 0.97 ± 0.08        HMXB        54,31
372 IGR J17585-3057 269.636  −30.956 0.80 ± 0.08
373 IGR J17586-2129 269.658  −21.327 1.35 ± 0.09 HMXB? 136
374 IGR J17597-2201 269.946  −22.026 5.65 ± 0.09        LMXB        96,97,175,197 XTE J1759-220;
375 V2301 OPH 270.170 8.190 1.33 ± 0.28 CV AM Herculis
376 GX 5-1 270.283  −25.075 69.29 ± 0.08        LMXB       
377 GRS 1758-258 270.302  −25.743 81.48 ± 0.08        LMXB       
378 GX 9+1 270.385  −20.527 22.84 ± 0.09        LMXB        C379;
379 IGR J18027-2016 270.666  −20.283 6.03 ± 0.10        HMXB        98,99,163 C378; IGR/SAX J18027-2017;
380 IGR J18027-1455 270.692  −14.910 2.39 ± 0.12 AGN 86,31 RXS J180245.2-145432; Sy1 z = 0.0350;
381 IGR J18048-1455 271.180  −14.925 0.95 ± 0.12        LMXB        44,116
382 XTE J1807-294 271.770  −29.430 9.09 ± 0.40R50:63        LMXB       
383 SGR 1806-20 272.162  −20.404 3.74 ± 0.10 SGR
384 XTE J1810-189 272.585  −19.070 43.76 ± 1.00R660:674        LMXB        190 Burster;
385 V4722 Sgr 272.685  −26.150 35.89 ± 0.33R594:606        LMXB       
386 PSR J1811-1925 272.862  −19.423 1.07 ± 0.10 PSR/PWN SNR G11.2-0.3;
387 IGR J18134-1636 273.370  −16.650 0.89 ± 0.12
388 IGR J18135-1751 273.397  −17.858 1.51 ± 0.11 SNR/PWN 46,171 HESS J1813-178;
389 GX 13+1 273.629  −17.155 16.12 ± 0.11        LMXB       
390 M 1812-12 273.780  −12.094 38.10 ± 0.13        LMXB       
391 IGR J18151-1052 273.790  −10.880 0.65 ± 0.13        HMXB        140,166
392 GX 17+2 274.006  −14.035 77.26 ± 0.13        LMXB       
393 IGR J18162+4953 274.060 49.890 7.53 ± 1.18 CV V* AM Her;
394 IGR J18170-2511 274.295  −25.142 1.14 ± 0.09 CV 134 IP; (=IGR J18173-2509);
395 IGR J18175-1530 274.400  −15.470 0.59 ± 0.12
396 XTE J1817-330 274.431  −33.020 48.27 ± 0.25R406:426        LMXB       
397 XTE J1818-245 274.597  −24.546 3.88 ± 0.09 LMXB?
398 SAX J1818.6-1703 274.699  −17.033 1.87 ± 0.12        HMXB        33,116,180
399 AX J1820.5-1434 275.112  −14.564 1.84 ± 0.13        HMXB       
400 IGR J18214-1318 275.340  −13.299 2.03 ± 0.13        HMXB        44,150
401 IGR J18218+6421 275.466 64.363 1.33 ± 0.25 AGN Sy1 z = 0.297; 7C 1821+6419;
402 IGR J18219-1347 275.500  −13.790 0.71 ± 0.13
403 4U 1820-303 275.921  −30.362 46.74 ± 0.10        LMXB       
404 IC 4709 276.081  −56.369 3.58 ± 0.31 AGN IGR J18244-5622; z = 0.016905;
405 XTE J1824-141 276.110  −14.440 0.98 ± 0.13 HMXB? 162 X-Ray Pulsar; =IGR J18246-1425;
406 IGR J18249-3243 276.206  −32.738 0.94 ± 0.10 AGN 9,134 Sy1 z = 0.355; PKS 1821-327?;
407 4U 1822-000 276.312 0.007 2.13 ± 0.15        LMXB       
408 IGR J18256-1035 276.434  −10.585 0.83 ± 0.13
409 4U 1822-371 276.447  −37.106 36.95 ± 0.12        LMXB       
410 IGR J18257-0707 276.480  −7.145 1.13 ± 0.14 AGN 44,120 Sy1 z = 0.037; =IGRJ18259-0706;
411 LS 5039 276.554  −14.861 0.91 ± 0.13        HMXB       
412 IGR J18293-1213 277.340  −12.220 0.74 ± 0.13
413 GS 1826-24 277.367  −23.798 112.29 ± 0.11        LMXB       
414 AX J183039-1002 277.660  −10.049 0.98 ± 0.13 AGN? 126
415 IGR J18308-1232 277.700  −12.530 1.14 ± 0.13 CV 136
416 IGR J18325-0756 278.112  −7.938 9.15 ± 0.38R62:66 100
11.42 ± 0.38R429:432
417 SNR 021.5-00.9 278.394  −10.572 4.16 ± 0.13 SNR
418 PKS 1830-211 278.421  −21.068 3.20 ± 0.12 AGN z = 2.507;
419 IGR J18354-2417 278.850  −24.290 0.58 ± 0.12 1WGA J1835.4-2418
420 RX J1832-33 278.933  −32.990 13.24 ± 0.12        LMXB       
421 AX J1838.0-0655 279.503  −6.911 2.78 ± 0.14 SNR/PWN 47 HESS J1837-069;
422 ESO 103-G035 279.632  −65.422 6.82 ± 0.38 AGN Sy2 z = 0.013249;
423 Ser X-1 279.991 5.041 15.16 ± 0.13        LMXB       
424 IGR J18410-0535 280.262  −5.577 1.34 ± 0.13        HMXB        19 AX J1841.0-0536;
425 1E 1841-045 280.329  −4.938 3.78 ± 0.13 PSR/PWN
426 3C390.3 280.578 79.763 5.09 ± 0.31 AGN Sy1 z = 0.056159;
427 ESO 140-43 281.225  −62.365 3.06 ± 0.33 AGN Sy1 z = 0.014113;
428 AX J1845.0-0433 281.253  −4.574 2.08 ± 0.13        HMXB        40
429 GS 1843+00 281.404 0.868 4.62 ± 0.12        HMXB       
430 IGR J18462-0223 281.567  −2.387 34.17 ± 2.91R610 HMXB? 119,191
431 PSR J1846-0258 281.613  −2.983 2.32 ± 0.12 PSR/PWN 170 AXP?
432 IGR J18470-7831 281.757  −78.533 1.42 ± 0.28 AGN z = 0.0743;
433 A 1845-024 282.048  −2.426 13.82 ± 1.31R229:233        HMXB       
434 IGR J18483-0311 282.071  −3.172 5.87 ± 0.12        HMXB        71,109,163 SFXT
435 IGR J18486-0047 282.104  −0.787 1.35 ± 0.12 AGN? 136 strong radio source, high X-ray abs.;
436 IGR J18490-0000 282.258  −0.013 1.63 ± 0.12 PWN 38,139,174,197
437 4U 1850-087 283.265  −8.702 7.55 ± 0.14        LMXB       
438 IGR J18539+0727 283.500 7.488 25.14 ± 0.86R62 LMXB? 30,24
439 ESO 25-2 283.759  −78.877 1.66 ± 0.28 AGN Sy1 z = 0.028743;
440 4U 1849-31 283.761  −31.155 9.23 ± 0.18 CV V1223 Sgr;
441 XTE J1855-026 283.870  −2.601 14.78 ± 0.12        HMXB       
442 IGR J18559+1535 283.987 15.629 1.97 ± 0.14 AGN 32,8 2E 1853.7+1534; Sy1 z = 0.084;
443 2E 1849.2-7832 284.346  −78.491 2.53 ± 0.29 AGN z = 0.042;
444 IGR J18578-3405 284.469  −34.096 5.89 ± 0.80R408 AGN?
445 XTE J1858+034 284.673 3.437 75.34 ± 0.32R186:193        HMXB       
446 HETE J19001-2455 285.039  −24.917 24.38 ± 0.19        LMXB       
447 XTE J1901+014 285.415 1.447 3.25 ± 0.11 HMXB? 69
448 4U 1901+03 285.917 3.207 115.17 ± 0.24R48:70        HMXB       
449 IGR J19072-2046 286.820  −20.770 1.14 ± 0.20 CV V1082 Sgr
450 SGR 1900+14 286.839 9.322 1.31 ± 0.10 SGR
451 IGR J19077-3925 286.890  −39.380 1.14 ± 0.20 AGN 173 Sy1.9 z = 0.073;
452 XTE J1908+094 287.219 9.374 0.94 ± 0.10        LMXB       
453 4U 1907+097 287.406 9.833 19.10 ± 0.11        HMXB       
454 IGR J19108+0917 287.641 9.312 0.50 ± 0.10
455 X 1908+075 287.701 7.595 18.14 ± 0.10        HMXB       
456 Aql X-1 287.814 0.584 12.57 ± 0.11        LMXB        187
457 SS 433 287.957 4.979 11.61 ± 0.10        HMXB       
458 IGR J19140+0951 288.526 9.885 12.76 ± 0.11        HMXB        53,42,163 =IGR J19140+098;
459 GRS 1915+105 288.801 10.947 388.69 ± 0.11        LMXB       
460 4U 1916-053 289.686  −5.247 11.90 ± 0.15        LMXB       
461 IGR J19193+0754 289.820 7.908 0.51 ± 0.10 high systematic noise from GRS 1915+105;
462 IGR J19194-2956 289.860  −29.950 1.38 ± 0.22 AGN 173 Sy 1.5/1.8 z = 0.166822; PKS 1916-300;
1RXS J191928.5-295808
463 ESO141-G055 290.309  −58.671 3.59 ± 0.38 AGN Sy1 z = 0.036649;
464 SWIFT J1922.7-1716 290.615  −17.300 6.83 ± 0.82R371 65
465 IGR J19267+1325 291.613 13.368 0.62 ± 0.12 CV 138 1RXS J192626.8+132153
466 IGR J19302+3411 292.550 34.190 1.30 ± 0.22 AGN 144 Sy1 z = 0.06326; =SWIFTJ1930.5+3414
467 1H 1934-063 294.422  −6.240 1.43 ± 0.19 AGN Sy1 z = 0.010254;
468 RX J1940.2-1025 295.050  −10.446 3.65 ± 0.22 CV 36 V1432 Aql;
469 IGR J19405-3016 295.062  −30.264 1.49 ± 0.26 AGN 116 z = 0.052;
470 NGC 6814 295.685  −10.331 4.53 ± 0.22 AGN Sy1 z = 0.005214;
471 IGR J19443+2117 296.000 21.310 1.07 ± 0.17 AGN? 167,136 =RX J1943.9+2118;
=SWIFT J194353.0+212119;
472 XSS J19459+4508 296.887 44.883 1.53 ± 0.21 AGN 23,2 =IGR J19473+4452; Sy2 z = 0.0539;
2MASX J19471938+4449425;
473 KS 1947+300 297.397 30.211 7.95 ± 0.18        HMXB       
474 3C403 298.024 2.445 0.88 ± 0.19 AGN Sy2 z = 0.059;
475 4U 1954+319 298.933 32.094 14.49 ± 0.17        HMXB       
476 Cyg X-1 299.588 35.202 1209.26 ± 0.16        HMXB       
477 IGR J19583+1941 299.600 19.690 0.94 ± 0.20
478 Cygnus A 299.863 40.736 6.13 ± 0.16 AGN Sy2 z = 0.056146; =3C 405.0;
479 SWIFT J2000.6+3210 300.101 32.166 3.07 ± 0.17        HMXB        65,66 IGR J20006+3210;
480 ESO 399-IG 020 301.738  −34.548 1.25 ± 0.25 AGN Sy1 z = 0.024951;
481 NGC 6860 302.192  −61.099 3.10 ± 0.64 AGN Sy1 z = 0.014884;
482 IGR J20159+3713 303.980 37.230 1.23 ± 0.14 SNR SNR G074.9+01.2; SWIFT J2015.9+3715
483 IGR J20187+4041 304.647 40.706 1.84 ± 0.13 AGN 26,39 IGR J2018+4043; Sy2 z = 0.0144;
2MASX J20183871+4041003;
484 IGR J20216+4359 305.409 43.996 1.04 ± 0.14 AGN 146 Sy2 z = 0.017;
485 IGR J20286+2544 307.140 25.746 3.55 ± 0.24 AGN 9,7 MCG +04-48-002; Sy2 z = 0.014206;
486 EXO 2030+375 308.062 37.638 126.68 ± 0.13        HMXB       
487 Cyg X-3 308.108 40.959 189.07 ± 0.12        HMXB       
488 SWIFT J2037.2+4151 309.300 41.850 0.75 ± 0.12
489 4C +74.26 310.576 75.141 3.49 ± 0.48 AGN Sy1 z = 0.103999;
490 MRK 509 311.036  −10.727 5.90 ± 0.43 AGN Sy1 z = 0.034397; =QSO B2041-1054;
491 SWIFT J2044.0+2832 311.042 28.510 2.02 ± 0.23 AGN 132 Sy1 z = 0.05; RX J2044.0+2833;
492 IGR J20569+4940 314.215 49.679 1.00 ± 0.14 161 3A 2056+493; Blazar or microQSO;
493 SAX J2103.5+4545 315.901 45.753 13.15 ± 0.13        HMXB       
494 S5 2116+81 318.736 82.045 2.84 ± 0.53 AGN Sy1 z = 0.086;
495 IGR J21178+5139 319.441 51.650 1.45 ± 0.14 AGN 9 2MASX J21175311+5139034;
496 IGR J21196+3333 319.910 33.560 1.43 ± 0.21 AGN 173 Sy1.5 z = 0.051; 1RXS J211928.4+333259;
497 IGR J21237+4218 320.960 42.316 1.40 ± 0.15 CV V2069 Cyg;
498 IGR J21247+5058 321.161 50.973 10.75 ± 0.14 AGN 86,3 Sy1 z = 0.02;
499 IGR J21277+5656 321.930 56.943 3.21 ± 0.16 AGN 32 Sy1 z = 0.014;
500 4U 2127+119 322.502 12.172 6.73 ± 0.71        LMXB       
501 IGR J21335+5105 323.449 51.122 3.58 ± 0.14 CV 36
502 IGR J21343+4738 323.625 47.614 2.01 ± 0.28R25:200        HMXB        146 USNO-B1.0 1376-0511904;
1RXS J213419.6+473810;
503 IGR J21358+4729 323.970 47.490 1.42 ± 0.15 AGN Sy1 z = 0.02523; 1RXS J213555.0+472823;
504 SS Cyg 325.711 43.574 4.39 ± 0.17 CV
505 Cyg X-2 326.170 38.319 33.49 ± 0.22        LMXB       
506 NGC 7172 330.490  −31.864 6.19 ± 0.45 AGN Sy2 z = 0.008616;
507 BL Lac 330.645 42.267 1.63 ± 0.22 AGN 1 Blazar z = 0.0688;
508 4U 2206+543 331.992 54.513 12.28 ± 0.15        HMXB       
509 FO Aqr 334.402  −8.301 3.53 ± 0.63R25 CV
510 IGR J22292+6646 337.316 66.774 1.07 ± 0.16 AGN 150,173 Sy1.5 z = 0.113; =IGR J22292+6647;
511 NGC 7314 338.890  −26.021 2.73 ± 0.43 AGN Sy1 z = 0.004790;
512 IGR J22367-1231 339.176  −12.539 2.13 ± 0.38 AGN Sy1 z = 0.024043; MRK 915;
513 IGR J22517+2218 342.939 22.316 2.70 ± 0.47R316:337 AGN 109 z = 3.668; =MG3 J225155+2217;
514 MR 2251-178 343.465  −17.616 5.28 ± 0.31 AGN Sy1 0.063980;
515 3C 454.3 343.490 16.143 10.27 ± 0.36 AGN 1 z = 0.859001;
516 NGC 7465 345.505 15.965 2.46 ± 0.36 AGN Sy2 z = 0.006565;
517 NGC 7469 345.825 8.879 4.55 ± 0.52 AGN Sy1 z = 0.01588;
518 MRK 926 346.166  −8.689 3.62 ± 0.41 AGN Sy1 z = 0.047156;
519 IGR J23206+6431 350.152 64.513 0.89 ± 0.11 AGN 146 Sy1 z = 0.07173;
520 Cas A 350.846 58.813 5.19 ± 0.11 SNR
521 IGR J23523+5844 358.079 58.745 0.84 ± 0.10 AGN 146 Sy2 z = 0.162;

Notes.

(†)

For the column descriptions see Sect. 4.

(‡)

The positional accuracy of sources detected by IBIS/ISGRI depends on the source significance (Gros et al. 2003). The estimated 68% confidence intervals for sources detected at 5–6, 10, and  > 20σ are 2.1′, 1.5′, and  < 0.8′, respectively (K07).

(*)

Source flux was measured on the 7-year time-averaged map or over the indicated spacecraft revolution interval RXXX:XXX. Flux is expressed in units of 10-11erg cm-2s-1.

(**)

(1) Donato et al. (2005); (2) Sazonov et al. (2005); (3) Masetti et al. (2004); (4) Masetti et al. (2006a); (5) Brandt et al. (2005); (6) Sunyaev et al. (2003a); (7) Masetti et al. (2006b); (8) Masetti et al. (2006c); (9) Bassani et al. (2006); (10) Sguera et al. (2006); (11) Lutovinov et al. (2004b); (12) Lubinski et al. (2005); (13) den Hartog et al. (2004a); (14) Grebenev et al. (2004b); (15) Smith & Hartigan (2006); (16) Kretschmar et al. (2004); (17) Chernyakova et al. (2005a); (18) in ’t Zand & Heise (2004); (19) Rodriguez et al. (2004); (20) Morelli et al. (2006); (21) Revnivtsev et al. (2004a); (22) Kuulkers et al. (2006); (23) Revnivtsev et al. (2006); (24) Lutovinov & Revnivtsev (2003); (25) Lutovinov et al. (2005b); (26) Bykov et al. (2004); (27) Bassani et al. (2005); (28) Zhou et al. (2007); (29) Pavlinskii et al. (1992); (30) Lutovinov et al. (2003a); (31) in ’t Zand (2005); (32) Bikmaev et al. (2006a); (33) Negueruela & Smith (2006); (34) Produit et al. (2004); (35) Barlow et al. (2005); (36) Barlow et al. (2006); (37) Walter et al. (2006); (38) Molkov et al. (2004); (39) Bykov et al. (2006); (40) Liu et al. (2000); (41) Liu et al. (2001); (42) Rodriguez et al. (2005); (43) Den Hartog et al. (2005); (44) Bird et al. (2006); (45) den Hartog et al. (2004b); (46) Ubertini et al. (2005); (47) Malizia et al. (2005); (48) Aleksandrovich et al. (1995); (49) Cornelisse et al. (2006); (50) Bikmaev et al. (2006b); (51) Chernyakova et al. (2005b); (52) Reig et al. (2005); (53) Hannikainen et al. (2003); (54) Sunyaev et al. (2003b); (55) Burenin et al. (2006b); (56) Negueruela et al. (2005); (57) Keek et al. (2006); (58) Krivonos et al. (2005a); (59) Abdo et al. (2009); (60) Burenin et al. (2006a); (61) Grebenev et al. (2005e); (62) Kuiper et al. (2006a); (63) Masetti et al. (2006e); (64) Lutovinov et al. (2004a); (65) Tueller et al. (2005b); (66) Halpern (2006); (67) Masetti et al. (2006d); (68) Masetti et al. (2005); (69) Karasevet al. (2007b); (70) Brandt et al. (2006a); (71) Chernyakova et al. (2003); (72) Gänsicke et al. (2005); (73) Turler et al. (2005a); (74) Grebenev et al. (2005d); (75) Gotz et al. (2006); (76) Krivonos et al. (2007a); (77) Sazonov et al. (2007); (78) Rea et al. (2006); (79) Bélanger et al. (2006); (80) Palmer et al. (2005); (81) Torres et al. (2005); (82) Sguera et al. (2007); (83) Tomsick et al. (2006); (84) Revnivtsev et al. (2003b); (85) Courvoisier et al. (2003); (86) Walter et al. (2004); (87) Tomsick et al. (2003); (88) Revnivtsev et al. (2003c); (89) Patel et al. (2004); (90) Bodaghee et al. (2006); (91) Tomsick et al. (2004); (92) Molkov et al. (2003a); (93) Lutovinov et al. (2005c); (94) Kuulkers et al. (2003); (95) Revnivtsev et al. (2003a); (96) Lutovinov et al. (2003c); (97) Lutovinov et al. (2005a); (98) Revnivtsev et al. (2004b); (99) Augello et al. (2003); (100) Lutovinov et al. (2003b); (101) Sazonov et al. (2008); (102) Masetti et al. (2007b); (103) Grebenev et al. (2005a); (104) Grebenev & Sunyaev (2004b); (105) Beckmann et al. (2005); (106) Grebenev et al. (2005c); (107) Kuiper et al. (2005); (108) Masetti et al. (2007a); (109) Bassani et al. (2007); (110) Bassa et al. (2006); (111) Revnivtsev et al. (2007); (112) Burenin et al. (2007); (113) Bikmaev et al. (2008b); (114) Karasev et al. (2007a); (115) Landi et al. (2007); (116) Masetti et al. (2008a); (117) Nespoli et al. (2008); (118) Kniazev et al. (2008); (119) Grebenev et al. (2007a); (120) Tomsick et al. (2008b); (121) Soldi et al. (2006); (122) Masetti et al. (2008b); (123) Altamirano et al. (2008); (124) Rodriguez et al. (2009); (125) Soldi et al. (2005); (126) Bassani et al. (2009); (127) Parisi et al. (2008); (128) Leyder et al. (2008); (129) Brunschweiger et al. (2009); (130) Tomsick et al. (2008a); (131) Landi et al. (2008); (132) Tueller et al. (2010); (133) Butters et al. (2007); (134) Masetti et al. (2009); (135) Watson et al. (2009); (136) Tomsicket al. (2009); (137) Mescheryakov et al. (2009); (138) Steeghs et al. (2008); (139) Rodriguez et al. (2008); (140) Krivonos et al. (2009); (141) Reig & Roche (1999); (142) Torres et al. (2007); (143) Winter et al. (2008); (144) Burenin et al. (2008); (145) Im et al. (2007); (146) Bikmaev et al. (2008a); (147) Wijnands (2006); (148) Brandt et al. (2006b); (149) Kuiper et al. (2006b); (150) Butler et al. (2009); (151) Cackett et al. (2006); (152) Bird et al. (2010); (153) Masetti et al. (2006f); (154) Zurita Heras et al. (2009); (155) Cadolle Bel et al. (2007); (156) Potter et al. (2010); (157) Revnivtsev et al. (2009); (158) Fisher et al. (1995); (159) Enya et al. (2002); (160) Markwardt & Swank (2008); (161) Landi et al. (2010); (162) Markwardt (2008); (163) Torrejón et al. (2010); (164) Krivonos et al. (2007b); (165) Sidoli et al. (2006); (166) Burenin et al. (2009); (167) Landi et al. (2009); (168) Masetti et al. (2010a); (169) Paizis et al. (2007); (170) Kuiper & Hermsen (2009); (171) Dean & Hill (2008); (172) Kniazev et al. (2010); (173) Masetti et al. (2010b); (174) Terrier et al. (2008); (175) Brandt et al. (2007); (176) Chelovekov & Grebenev (2007a); (177) Chelovekov & Grebenev (2007b); (178) Chelovekov et al. (2007); (179) Grebenev et al. (2004c); (180) Grebenev & Sunyaev (2005); (181) Grebenev et al. (2004a); (182) Grebenev & Sunyaev (2004a); (183) Grebenev & Sunyaev (2007); (184) Grebenev et al. (2005g); (185) Grebenev et al. (2007b); (186) Sunyaev et al. (1991); (187) Molkov et al. (2003b); (188) Karasev et al. (2009); (189) Grebenev et al. (2005b); (190) Chelovekov & Grebenev (2010); (191) Grebenev et al. (2010); (192) Rodriguez et al. (2010); (193) Chaty et al. (2008); (194) Renaud et al. (2010); (195) Malizia et al. (2010); (196) Fiocchi et al. (2010); (197) Ratti et al. (2010); (198) Lutovinov et al. (2010a); (199) Lutovinov et al. (2010b).

(***)

The spatial confusion with the source XXX is indicated as CXXX. The measured flux of sources being in spatial confusion should be taken with the caution.

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