Äîêóìåíò âçÿò èç êýøà ïîèñêîâîé ìàøèíû. Àäðåñ îðèãèíàëüíîãî äîêóìåíòà : http://hea-www.harvard.edu/QEDT/Papers/crss5_t2.ps Äàòà èçìåíåíèÿ: Thu Aug 1 22:09:14 1996 Äàòà èíäåêñèðîâàíèÿ: Mon Oct 1 23:58:54 2012 Êîäèðîâêà: Ïîèñêîâûå ñëîâà: m 81

Table
2.
Optical
Identifications
X­ray
Optical
Survey
Name
S
0:5\Gamma2
keV
RA
(J2000)
Dec
`
RA
(J2000)
Dec
O\GammaX
E
O
O\GammaE
ID
z
Notes
erg
s
\Gamma1
cm
\Gamma2
h
m
s
ffi
0
00
0
h
m
s
ffi
0
00
00
CRSS0007.3+2042
0.48\Theta10
\Gamma13
00
07
21.9
+20
42
04
13.6
00
07
21.7
+20
42
02
2.6
18.53
18.78
0.24
QSO
0.7686
CRSS0007.5+2034
0.34\Theta10
\Gamma13
00
07
33.4
+20
34
46
12.7
00
07
33.8
+20
34
39
9.1
15.29
17.81
2.52
M(e)
CRSS0007.7+2050
0.29\Theta10
\Gamma13
00
07
43.0
+20
50
39
12.2
00
07
42.7
+20
50
39
4.0*
--
20.76
--
QSO
1.3964
CRSS0008.0+2043
0.23\Theta10
\Gamma13
00
08
02.0
+20
43
56
4.9
00
08
02.4
+20
44
11
16.8
17.68
17.93
0.26
QSO
1.3813
CRSS0008.4+2034
0.16\Theta10
\Gamma12
00
08
26.4
+20
34
34
7.6
00
08
26.5
+20
34
32
1.8*
16.34
16.84
0.50
QSO
0.3886
CRSS0008.4+2042
0.20\Theta10
\Gamma13
00
08
09.3
+20
42
10
2.2
00
08
29.5
+20
42
00
9.6*
19.28
19.85
0.57
QSO
1.7099
CRSS0008.4+2035
0.24\Theta10
\Gamma13
00
08
29.7
+20
34
01
7.8
00
08
29.8
+20
34
00
1.9
18.25
21.41
3.16
M
CRSS0008.6+2046
0.24\Theta10
\Gamma13
00
08
40.6
+20
45
57
6.6
00
08
40.9
+20
46
00
5.1
--
20.72
--
QSO
0.7524
CRSS0008.9+2050
0.68\Theta10
\Gamma12
00
08
54.0
+20
50
26
11.7
00
08
54.1
+20
50
36
10.5*
11.26
14.83
3.57
M(e)
CRSS0009.0+2041
0.20\Theta10
\Gamma13
00
09
01.3
+20
41
33
9.7
00
09
01.7
+20
41
35
6.6*
19.04
21.83
2.79
NLXG
0.1895
HII
1
CRSS0029.1+2616
0.34\Theta10
\Gamma13
00
29
07.5
+26
16
22
13.2
No
optical
counterpart
CRSS0029.7+2606
0.20\Theta10
\Gamma13
00
29
44.7
+26
06
37
11.9
00
29
44.0
+26
06
27
13.8
18.88
19.26
0.38
QSO
1.0938
CRSS0030.2+2611
0.51\Theta10
\Gamma13
00
30
17.3
+26
11
43
6.4
00
30
17.4
+26
11
38
4.9
14.84
16.26
1.42
NLXG
0.0773
HII
1
CRSS0030.5+2618
0.15\Theta10
\Gamma12
00
30
33.4
+26
18
16
6.2
00
30
34.0
+26
18
08
11.1y
19.44
--
--
Gal
0.516
Cluster
2
00
30
33.3
26
18
10
5.9*
19.75
--
--
Gal?
0.52:
CRSS0030.6+2620
0.19\Theta10
\Gamma12
00
30
39.5
+26
20
53
8.1
00
30
39.6
+26
20
54
1.7*
16.87
17.31
0.44
QSO
0.4925
CRSS0030.7+2616
0.20\Theta10
\Gamma13
00
30
47.2
+26
16
50
9.3
00
30
47.9
+26
16
47
9.4
18.45
--
--
NLXG
0.2465
Sy2
1
CRSS0030.8+2628
0.20\Theta10
\Gamma13
00
30
48.7
+26
28
26
13.9
00
30
48.8
+26
28
31
5.7
19.15
19.64
0.49
QSO
1.3722
CRSS1406.2+2830
0.65\Theta10
\Gamma13
14
06
16.2
+28
30
50
10.3
14
06
15.6
+28
30
52
8.8*
19.66
--
--
Gal
0.546
CRSS1406.7+2827
0.25\Theta10
\Gamma13
14
06
44.3
+28
27
21
3.5
14
06
44.3
+28
27
25
4.7
--
20.57
--
QSO
0.878
CRSS1406.7+2838
0.28\Theta10
\Gamma13
14
06
47.3
+28
38
54
11.9
14
06
48.0
+28
38
53
8.9
--
22.10
--
NLXG
0.3309
HII
1
CRSS1406.9+2834
0.15\Theta10
\Gamma12
14
06
54.3
+28
34
14
6.7
14
06
54.0
+28
34
17
4.3*
12.77
16.73
3.96
Gal
0.118
Cluster
3
14
06
53.8
+28
34
08
9.0*
--
21.49
--
Gal
0.118
CRSS1407.3+2818
0.19\Theta10
\Gamma12
14
07
19.4
+28
18
11
10.3
14
07
19.4
+28
18
14
2.8
17.23
17.76
1.12
QSO
1.1207
CRSS1407.3+2814
0.36\Theta10
\Gamma13
14
07
20.3
+28
14
56
13.2
14
07
20.2
+28
14
50
6.4y
16.88
18.00
1.12
QSO
0.7284
4
14
07
20.5
+28
14
58
2.6*
--
21.42
--
?
CRSS1407.6+2825
0.24\Theta10
\Gamma13
14
07
38.9
+28
25
12
8.9
14
07
38.4
+28
25
15
6.8
18.95
19.73
0.78
QSO
1.2220
CRSS1407.7+2830
0.34\Theta10
\Gamma12
14
07
45.2
+28
30
24
10.3
14
07
45.4
+28
30
28
4.8*
18.40
18.81
0.42
QSO
0.6424
CRSS1407.7+2824
0.42\Theta10
\Gamma13
14
07
45.6
+28
24
33
10.6
14
07
45.3
+28
24
35
4.0
--
21.49
--
QSO
1.1272
CRSS1407.8+2833
0.35\Theta10
\Gamma13
14
07
51.7
+28
33
14
12.7
14
07
50.8
+28
33
21
14.3*
--
21.96
--
N/O
14
07
51.7
+28
33
31
16.3*
--
22.09
--
N/O
1

X­ray
Optical
Survey
Name
S
0:5\Gamma2
keV
RA
(J2000)
Dec
`
RA
(J2000)
Dec
O­X
E
O
O\GammaE
ID
z
Notes
erg
s
\Gamma1
cm
\Gamma2
h
m
s
ffi
0
00
0
h
m
s
ffi
0
00
00
CRSS1412.5+4355
0.22\Theta10
\Gamma12
14
12
31.6
+43
55
41
14.7
14
12
31.6
+43
55
35
5.1*
15.86
17.03
1.17
NLXG
0.0945
Sy1.8
1
CRSS1413.0+4406
0.28\Theta10
\Gamma13
14
13
04.3
+44
06
59
9.8
No
optical
counterpart
CRSS1413.3+4405
0.52\Theta10
\Gamma13
14
13
20.0
+44
05
31
7.0
14
13
19.9
+44
05
35
4.6
17.19
--
--
NLXG
0.1363
Sy1.5
1
CRSS1413.4+4358
0.30\Theta10
\Gamma13
14
13
28.8
+43
58
06
4.1
14
13
28.9
+43
58
07
1.7*
19.81
20.19
0.39
QSO
0.9497
CRSS1413.8+4406
0.46\Theta10
\Gamma13
14
13
48.4
+44
06
43
5.9
14
13
48.3
+44
06
46
3.7*
19.06
--
--
QSO
0.9784
CRSS1413.8+4402
0.28\Theta10
\Gamma13
14
13
53.1
+44
02
27
2.1
14
13
53.0
+44
02
30
3.9*
19.58
--
--
QSO
1.3469
CRSS1413.9+4352
0.43\Theta10
\Gamma13
14
13
59.6
+43
52
06
8.4
No
optical
counterpart
CRSS1414.2+4354
0.53\Theta10
\Gamma13
14
14
14.3
+43
54
16
7.7
14
14
14.2
+43
54
14
1.9*
19.09
19.72
0.62
QSO
1.1968
CRSS1415.0+4402
0.29\Theta10
\Gamma13
14
14
59.5
+44
02
10
13.0
14
15
00.2
+44
02
11
8.0*
17.60
--
--
NLXG
0.1363
Sy1.5
1
CRSS1415.0+1119
0.51\Theta10
\Gamma13
14
15
04.8
+11
19
39
14.8
14
15
04.6
+11
19
41
3.6
19.03
20.06
1.03
QSO
0.5383
CRSS1415.1+1140
0.26\Theta10
\Gamma13
14
15
11.1
+11
40
01
12.6
14
15
11.2
+11
40
03
2.7*
19.36
19.87
0.52
QSO
2.3534
CRSS1415.2+1123
0.23\Theta10
\Gamma13
14
15
15.7
+11
23
44
10.1
14
15
15.9
+11
23
44
2.6*
19.17
19.93
0.76
QSO
1.2303
CRSS1415.2+1119
0.61\Theta10
\Gamma13
14
15
16.6
+11
19
34
13.0
14
15
17.5
+11
19
21
18.7
16.87
18.16
1.29
G
5
CRSS1415.3+1137
0.46\Theta10
\Gamma13
14
15
23.7
+11
37
38
9.1
No
optical
counterpart
CRSS1415.5+1127
0.20\Theta10
\Gamma13
14
15
30.9
+11
27
11
4.7
14
15
31.1
+11
27
13
3.6*
--
21.51
--
QSO
1.4117
CRSS1415.5+1131
0.15\Theta10
\Gamma12
14
15
31.5
+11
32
00
3.8
14
15
31.5
+11
31
57
3.5*
18.38
19.91
1.53
QSO
0.2565
CRSS1415.5+1128
0.25\Theta10
\Gamma13
14
15
32.1
+11
28
53
3.9
14
15
32.0
+11
28
50
3.4
19.74
21.79
2.05
QSO
0.3595
CRSS1415.6+1127
0.41\Theta10
\Gamma13
14
15
38.0
+11
27
46
3.4
No
optical
counterpart
CRSS1415.6+1124
0.62\Theta10
\Gamma13
14
15
39.8
+11
24
12
6.0
14
15
40.1
+11
24
03
10.1*
17.59
--
4.77
M(e)
CRSS1415.7+1116
0.26\Theta10
\Gamma13
14
15
44.5
+11
16
29
13.7
14
15
44.4
+11
16
26
2.5*
18.84
19.19
0.34
QSO
1.2567
CRSS1415.9+1139
0.34\Theta10
\Gamma13
14
15
56.5
+11
39
09
9.6
No
optical
counterpart
CRSS1416.0+1142
0.40\Theta10
\Gamma13
14
16
02.2
+11
42
45
12.9
No
optical
counterpart
CRSS1416.2+1136
0.52\Theta10
\Gamma13
14
16
12.6
+11
36
17
9.0
14
16
13.1
+11
36
07
12.4
19.50
22.22
2.72
?
CRSS1416.2+1131
0.20\Theta10
\Gamma13
14
16
15.4
+11
31
10
7.3
14
16
15.9
+11
31
09
7.2
--
21.69
--
QSO
1.4287
CRSS1416.3+1129
0.22\Theta10
\Gamma13
14
16
19.5
+11
29
53
8.2
No
optical
counterpart
CRSS1416.3+1137
0.21\Theta10
\Gamma13
14
16
21.0
+11
37
53
11.2
14
16
20.7
+11
37
37
15.3
19.28
20.77
1.50
BL
7
CRSS1416.3+1124
0.20\Theta10
\Gamma13
14
16
23.0
+11
24
42
10.7
14
16
23.5
+11
24
40
7.4*
--
20.95
--
QSO
1.6729
BAL
CRSS1416.3+1140
0.52\Theta10
\Gamma13
14
16
23.7
+11
40
21
13.8
14
16
23.5
+11
40
27
6.7*
17.37
18.57
1.21
G
7
CRSS1418.3+0637
0.19\Theta10
\Gamma12
14
18
20.9
+06
37
49
14.6
14
18
21.3
+06
37
46
6.4*
16.91
17.41
0.50
QSO
0.3285
2

X­ray
Optical
Survey
Name
S
0:5\Gamma2
keV
RA
(J2000)
Dec
`
RA
(J2000)
Dec
O­X
E
O
O\GammaE
ID
z
Notes
erg
s
\Gamma1
cm
\Gamma2
h
m
s
ffi
0
00
0
h
m
s
ffi
0
00
00
CRSS1419.2+5429
0.33\Theta10
\Gamma13
14
19
16.1
+54
29
32
7.4
14
19
16.2
+54
29
42
10.2
19.29
19.90
0.61
QSO
0.7217
CRSS1419.2+5414
0.50\Theta10
\Gamma13
14
19
16.7
+54
14
17
9.9
14
19
17.1
+54
14
16
3.3*
16.67
19.55
2.88
Gal
0.226
CRSS1419.3+5424
0.21\Theta10
\Gamma13
14
19
18.3
+54
24
31
4.2
14
19
19.0
+54
24
33
5.8*
19.81
20.45
0.64
QSO
0.785
CRSS1419.5+5428
0.27\Theta10
\Gamma13
14
19
32.6
+54
28
21
5.4
14
19
31.8
+54
28
19
7.7*
15.27
17.05
1.77
G
8
14
19
32.6
54
28
12
8.4*
--
21.65
--
?
CRSS1419.8+5433
0.31\Theta10
\Gamma13
14
19
51.6
+54
33
57
10.1
14
19
52.6
+54
33
55
8.6*
19.52
21.31
1.79
QSO
0.3668
CRSS1419.8+5419
0.27\Theta10
\Gamma13
14
19
53.3
+54
19
25
4.1
14
19
53.8
+54
19
20
6.1
11.06
12.44
1.38
N/O
Bright
Star
CRSS1419.9+5430
0.49\Theta10
\Gamma13
14
19
54.9
+54
30
18
7.2
14
19
54.1
+54
30
14
7.9
17.45
17.93
0.48
QSO
2.2573
CRSS1420.1+5426
0.11\Theta10
\Gamma12
14
20
09.2
+54
26
38
4.5
14
20
09.4
+54
26
38
2.1
19.03
20.24
1.21
QSO
0.5830
CRSS1428.0+4244
0.32\Theta10
\Gamma13
14
27
59.8
+42
44
15
6.9
14
28
00.2
+42
44
10
6.8
15.07
17.62
2.55
M(e)
CRSS1428.3+4231
0.32\Theta10
\Gamma13
14
28
20.3
+42
31
34
10.0
14
28
20.4
+42
31
38
3.8*
17.72
18.27
0.55
QSO
2.1705
CRSS1429.0+0122
0.47\Theta10
\Gamma13
14
29
04.5
+01
22
29
4.4
14
29
04.4
+01
22
30
2.3*
19.19
20.00
0.81
QSO
0.4158
CRSS1429.0+0120
0.43\Theta10
\Gamma13
14
29
04.7
+01
20
29
2.5
14
29
04.7
+01
20
17
11.9y
16.56
18.26
1.70
NLXG
0.1016
HII
1;9
14
29
05.1
+01
20
32
6.8*
16.78
17.95
1.17
F
CRSS1429.1+0128
0.41\Theta10
\Gamma13
14
29
11.8
+01
28
09
10.5
14
29
11.8
+01
28
00
9.3
--
21.35
--
QSO
1.1312
CRSS1429.2+0121
0.26\Theta10
\Gamma13
14
29
17.9
+01
20
56
4.4
14
29
17.7
+01
21
00
4.7
18.18
18.95
0.78
QSO
1.1269
CRSS1429.0+4230
0.89\Theta10
\Gamma13
14
29
01.5
+42
30
53
11.0
14
29
01.8
+42
30
54
3.1
9.90
11.16
1.25
F
CRSS1429.1+4241
0.62\Theta10
\Gamma13
14
29
06.4
+42
41
10
6.2
No
optical
counterpart
CRSS1429.7+4240
0.13\Theta10
\Gamma12
14
29
45.1
+42
40
58
13.3
14
29
45.1
+42
40
54
4.0
15.25
16.87
1.61
QSO
1.6719
CRSS1514.7+3641
0.48\Theta10
\Gamma13
15
14
47.1
+36
41
50
9.9
15
14
47.0
+36
41
50
1.4
19.02
20.08
1.06
QSO
1.2193
CRSS1514.3+5621
0.50\Theta10
\Gamma12
15
14
22.9
+56
21
29
12.8
15
14
22.9
+56
21
33
3.5*
13.91
16.09
2.19
M(e)
CRSS1515.0+3649
0.18\Theta10
\Gamma12
15
15
03.5
+36
49
48
4.5
15
15
03.4
+36
49
50
2.2
7.66
8.30
0.64
N/O
Bright
Star
CRSS1515.0+3657
0.16\Theta10
\Gamma12
15
15
05.0
+36
57
26
7.5
15
15
05.0
+36
57
21
4.0
19.41
20.47
1.06
QSO
0.2530
CRSS1514.4+5627
0.37\Theta10
\Gamma13
15
14
30.0
+56
26
59
14.0
15
14
29.6
+56
27
07
8.9
--
20.69
--
NLXG
0.4463
CRSS1515.4+3652
0.82\Theta10
\Gamma13
15
15
26.8
+36
51
56
8.7
15
15
26.7
+36
52
03
7.3*
19.98
20.68
0.70
QSO
0.8931
CRSS1515.5+3655
0.11\Theta10
\Gamma12
15
15
35.2
+36
55
54
11.2
15
15
35.4
+36
55
49
5.2*
18.72
19.53
0.81
QSO
0.8120
CRSS1515.1+5628
0.57\Theta10
\Gamma13
15
15
10.2
+56
28
30
10.6
15
15
10.1
+56
28
34
4.7
--
20.06
--
QSO
0.7229
CRSS1515.7+5610
0.37\Theta10
\Gamma13
15
15
47.1
+56
10
32
9.4
15
15
47.5
+56
10
33
3.3
19.25
20.29
1.04
QSO
0.2956
CRSS1516.3+5611
0.23\Theta10
\Gamma13
15
16
22.1
+56
11
53
9.1
15
16
22.0
+56
11
50
2.7*
--
20.59
--
QSO
1.1675
CRSS1516.4+5612
0.25\Theta10
\Gamma13
15
16
26.2
+56
12
46
8.5
15
16
26.0
+56
12
50
4.0
--
21.61
--
M
CRSS1516.8+5617
0.32\Theta10
\Gamma13
15
16
53.4
+56
17
45
8.5
No
optical
counterpart
CRSS1517.0+5623
0.85\Theta10
\Gamma13
15
17
03.8
+56
23
40
10.3
15
17
03.6
+56
23
38
2.1*
19.36
20.38
1.02
QSO
0.4341
CRSS1517.6+5619
0.80\Theta10
\Gamma13
15
17
39.6
+56
19
24
14.6
15
17
39.4
+56
19
15
8.9
13.99
15.50
1.51
G
3

X­ray
Optical
Survey
Name
S
0:5\Gamma2
keV
RA
(J2000)
Dec
`
RA
(J2000)
Dec
O­X
E
O
O\GammaE
ID
z
Notes
erg
s
\Gamma1
cm
\Gamma2
h
m
s
ffi
0
00
0
h
m
s
ffi
0
00
00
CRSS1545.4+4838
0.37\Theta10
\Gamma13
15
45
26.4
+48
38
27
8.5
15
45
26.5
+48
38
21
6.5*
--
20.94
--
QSO
0.9374
CRSS1545.5+4858
0.38\Theta10
\Gamma13
15
45
34.6
+48
58
13
11.5
15
45
34.6
+48
58
16
3.2*
19.39
19.54
0.16
QSO
0.6660
CRSS1545.5+4847
0.35\Theta10
\Gamma13
15
45
36.1
+48
47
19
1.1
15
45
35.9
+48
47
13
6.3
18.85
19.93
1.08
QSO
1.4027
CRSS1545.9+4849
0.58\Theta10
\Gamma13
15
45
55.7
+48
49
37
4.9
15
45
55.6
+48
49
29
8.1*
18.68
20.93
2.25
QSO
0.1542
CRSS1546.4+4849
0.32\Theta10
\Gamma13
15
46
25.3
+48
49
53
9.7
15
46
25.4
+48
49
58
5.0
18.84
19.99
1.15
F
CRSS1604.8+2549
0.36\Theta10
\Gamma13
16
04
51.8
+25
49
58
12.2
16
04
51.9
+25
49
58
2.0
19.78
20.96
1.17
QSO
0.4258
CRSS1604.9+2545
0.38\Theta10
\Gamma13
16
04
56.0
+25
45
26
13.1
16
04
55.7
+25
45
20
6.9
16.44
17.51
1.07
G
CRSS1605.2+2602
0.28\Theta10
\Gamma13
16
05
12.8
+26
02
42
12.6
No
optical
counterpart
CRSS1605.2+2541
0.40\Theta10
\Gamma13
16
05
17.0
+25
41
17
12.6
16
05
17.2
+25
41
19
3.4*
18.47
18.88
0.40
QSO
1.0708
CRSS1605.6+2543
0.44\Theta10
\Gamma13
16
05
39.8
+25
43
10
8.9
16
05
39.9
+25
43
10
1.8
18.93
20.21
1.28
NLXG
0.2779
HII
1
CRSS1603.8+2602
0.41\Theta10
\Gamma13
16
05
58.5
+25
54
05
3.7
16
05
58.7
+25
54
07
3.5*
--
20.55
--
NLXG
0.1510
CRSS1606.6+2542
0.23\Theta10
\Gamma13
16
06
35.9
+25
42
41
14.9
16
06
36.1
+25
42
45
4.1*
18.53
19.03
0.50
QSO
1.4356
CRSS1618.0+0617
0.18\Theta10
\Gamma12
16
18
04.6
+06
17
17
13.7
16
18
04.7
+06
17
07
9.7*
13.62
15.74
2.13
M(e)
CRSS1618.4+0558
0.35\Theta10
\Gamma13
16
18
26.6
+05
58
22
12.0
16
18
27.3
+05
58
15
12.7*
19.29
20.45
1.17
QSO
0.4060
CRSS1620.1+1724
0.65\Theta10
\Gamma12
16
20
11.3
+17
24
28
12.7
16
20
11.3
+17
24
27
1.2*
15.21
15.67
0.46
QSO
0.114
PG1617+175
10
CRSS1653.3+3951
0.91\Theta10
\Gamma13
16
53
23.8
+39
51
21
7.8
16
53
23.7
+39
51
24
3.1
--
20.50
--
QSO
0.6920
CRSS1654.5+3954
0.21\Theta10
\Gamma12
16
54
30.8
+39
54
21
11.3
16
54
30.8
+39
54
20
0.8*
18.49
19.23
0.73
QSO
0.3398
CRSS1703.9+6045
0.10\Theta10
\Gamma12
17
03
55.6
+60
45
08
5.6
17
03
55.7
+60
45
11
2.7
17.81
19.69
1.88
QSO
0.284
MS1703.2+6049
11
CRSS1704.1+6047
0.66\Theta10
\Gamma13
17
04
05.9
+60
47
49
5.0
17
04
06.1
+60
47
53
4.6*
17.25
18.12
0.87
QSO
1.3615
CRSS1704.6+6036
0.23\Theta10
\Gamma13
17
04
39.7
+60
36
54
8.5
17
04
39.0
+60
36
49
7.7
18.50
21.35
2.85
M
CRSS1705.3+6049
0.27\Theta10
\Gamma13
17
05
17.8
+60
49
53
6.4
17
05
18.3
+60
49
54
3.7
19.95
21.83
1.88
NLXG
0.5724
Sy2?
1
CRSS1705.3+6044
0.24\Theta10
\Gamma13
17
05
22.9
+60
44
55
5.1
17
05
23.7
+60
44
57
6.0*
18.79
19.29
0.50
QSO
1.4164
CRSS1705.4+6031
0.61\Theta10
\Gamma13
17
05
27.2
+60
31
10
14.5
17
05
26.4
+60
31
03
9.7*
17.22
18.19
0.97
QSO
0.3747
CRSS1705.5+6042
0.55\Theta10
\Gamma12
17
05
34.9
+60
42
16
7.0
17
05
34.7
+60
42
15
1.6
18.09
20.36
2.28
BL
0.280
MS1704.9+6046
11
CRSS1706.4+6042
0.22\Theta10
\Gamma13
17
06
26.2
+60
42
59
13.1
17
06
26.6
+60
42
45
14.3y
18.05
18.74
0.69
QSO
1.1416
12
17
06
26.0
+60
43
01
2.9*
19.39
21.24
1.85
N/O
17
06
27.5
+60
42
55
10.0*
18.14
20.17
2.03
N/O
4

X­ray
Optical
Survey
Name
S
0:5\Gamma2
keV
RA
(J2000)
Dec
`
RA
(J2000)
Dec
O­X
E
O
O\GammaE
ID
z
Notes
erg
s
\Gamma1
cm
\Gamma2
h
m
s
ffi
0
00
arcmin
h
m
s
ffi
0
00
arcsec
CRSS2235.3+1340
0.98\Theta10
\Gamma13
22
35
18.2
+13
40
09
12.8
22
35
18.3
+13
40
07
2.4*
19.22
19.89
0.67
QSO
1.021
Q2232+134
13
CRSS2249.5+1425
0.34\Theta10
\Gamma12
22
49
30.5
+14
25
11
14.2
22
49
30.5
+14
25
09
1.5*
11.93
13.16
1.23
F
CRSS2250.0+1407
0.44\Theta10
\Gamma13
22
50
01.2
+14
07
34
14.2
22
50
01.2
+14
07
40
5.4*
19.83
20.92
1.09
QSO
1.1594
CRSS2250.1+1414
0.94\Theta10
\Gamma13
22
50
06.6
+14
14
58
6.7
22
50
06.3
+14
14
54
6.4
10.57
11.43
0.87
F
CRSS2250.4+1431
0.79\Theta10
\Gamma12
22
50
24.1
+14
31
43
11.1
22
50
24.2
+14
31
44
1.7
11.71
13.65
1.94
G
CRSS2250.8+1429
0.47\Theta10
\Gamma13
22
50
51.2
+14
29
23
11.1
22
50
51.4
+14
29
29
6.8
15.83
17.93
2.10
M(e)
CRSS2250.9+1419
0.34\Theta10
\Gamma13
22
50
59.5
+14
19
20
8.3
22
50
59.5
+14
19
20
0.7
16.71
19.32
2.61
M(e)
CRSS2251.0+1418
0.49\Theta10
\Gamma13
22
51
01.6
+14
18
32
9.0
22
51
01.8
+14
18
26
6.1
18.54
19.02
0.48
QSO
0.9624
CRSS2324.7+2315
0.39\Theta10
\Gamma13
23
24
43.1
+23
15
37
12.5
23
24
43.8
+23
15
37
9.3
18.55
18.98
0.42
QSO
1.8282
CRSS2324.8+2321
0.77\Theta10
\Gamma13
23
24
49.9
+23
21
02
8.3
23
24
50.5
+23
21
06
9.6
19.14
19.68
0.54
QSO
0.4474
CRSS2325.1+2330
0.45\Theta10
\Gamma13
23
25
09.2
+23
30
14
6.0
23
25
09.6
+23
30
16
6.1
10.56
12.63
2.07
F
1.
Detailed
identification
from
Boyle
et
al.
1995b.
2.
Optical
spectra
of
both
objects
consistent
with
z
=
0:52
galaxies,
although
spectrum
of
the
galaxy
closer
to
the
X­ray
source
position
has
low
signal­to­noise
ratio.
A
CCD
image
indicates
the
presence
of
a
rich
cluster.
3.
Galaxy
cluster
on
Palomar
sky
survey
plate.
4.
The
closest
optical
counterpart
is
a
faint
source
with
an
ambiguous
optical
spectrum.
However,
the
most
likely
identification
of
the
X­ray
source
in
the
QSO
6
arcsec
from
the
X­ray
position.
5.
The
a
posteriori
probability
of
finding
an
of
this
magnitude
or
brighter
within
a
20
arcsec
radius
is
¸
0:02.
It
is
therefore
possible
that
this
is
not
the
correct
counterpart
of
the
X­ray
source,
but
it
is
the
only
object
identified
eithin
the
20arcsec
error
radius
down
to
the
photographic
plate
limit.
6.
Continuum
object
7.
The
a
posteriori
probability
of
finding
an
of
this
magnitude
or
brighter
within
a
20
arcsec
radius
is
¸
0:03.
It
is
therefore
possible
that
this
is
not
the
correct
counterpart
of
the
X­ray
source,
however
the
only
other
optical
source
within
the
error
circle
is
a
faint
E
=
19:7
galaxy,
18arcsec
from
the
X­ray
source
position.
8.
Although
the
probability
of
finding
a
such
a
bright
star
within
the
error
radius
is
very
low
!
0:01,
a
second
(almost
equidistant)
faint
candidate
was
observed
spectroscopically,
but
no
strong
emission
lines
were
found.
9.
Although
an
F
star
was
found
to
closer
to
the
X­ray
source
position,
the
low
probability
of
identifying
a
starburst
galaxy
within
12
arcsec
makes
it
the
more
probably
X­ray
source
counterpart.
10.
Schmidt
and
Green
(1983)
11.
Stocke
et
al.
(1991)
12.
The
QSO
observed
is
not
the
closest
object
to
the
X­ray
source
position.
Two
faint
objects
were
found
closer
to
the
X­ray
position
but
were
not
observed.
13.
Crampton,
Cowley
and
Hartwick
(1987)
5