Tully list
In 1985, Tully determined a local dominant supercluster plane, and found the Pisces–Cetus Supercluster Complex.[22]
More information #, Coordinates ...
# |
Coordinates |
Distance |
Diameter |
Notes |
(h−1 Mpc) |
1 |
17.0h 80° |
90 |
140 |
|
2 |
21.0h −7° |
100 |
136 |
|
3 |
8.6h +13° |
150 |
150 |
|
4 |
21.5h +5° |
170 |
173 |
|
5 |
14.3h +52° |
180 |
158 |
Boötes Void |
6 |
23.0h −16° |
190 |
171 |
|
7 |
12.8h +14° |
190 |
174 |
|
8 |
10.0h +35° |
250 |
170 |
|
9 |
2.6h −11° |
280 |
229 |
|
10 |
8.7h +58° |
310 |
243 |
|
11 |
16.8h +5° |
310 |
270 |
|
Close
B&B Abell-derived list
In a 1985 study of Abell clusters, 29 voids were determined, in the sphere z<0.1 around Earth.[23]
More information #, Coordinates ...
# |
Coordinates |
Distance |
Diameter |
Notes |
(h−1 Mpc) |
1 |
0.0h +20° |
293 |
100 |
|
2 |
0.3h 0° |
276 |
100 |
|
3 |
0.7h +10° |
284 |
100 |
|
4 |
2.0h −13° |
275 |
150 |
|
5 |
8.0h +60° |
300 |
100 |
|
6 |
9.0h +18° |
220 |
100 |
|
7 |
9.0h +67° |
180 |
120 |
|
8 |
9.2h +26° |
137 |
140 |
|
9 |
9.5h +45° |
262 |
200 |
|
10 |
9.8h 0° |
285 |
110 |
|
11 |
9.8h +35° |
219 |
110 |
|
12 |
10.8h −10° |
293 |
120 |
|
13 |
12.0h +14° |
206 |
110 |
|
14 |
12.3h 0° |
276 |
100 |
|
15 |
12.4h −12° |
272 |
150 |
|
16 |
12.5h +32° |
237 |
100 |
|
17 |
12.9h +64° |
105 |
110 |
|
18 |
13.6h +35° |
154 |
200 |
Boötes Void |
19 |
13.8h +20° |
297 |
110 |
|
20 |
14.2h −4° |
265 |
210 |
|
21 |
14.7h +70° |
283 |
160 |
|
22 |
15.2h +42° |
286 |
140 |
|
23 |
16.0h +7° |
295 |
110 |
|
24 |
16.4h +41° |
291 |
130 |
|
25 |
16.5h +59° |
110 |
100 |
|
26 |
17.2h +58° |
237 |
100 |
|
27 |
22.2h −2° |
155 |
130 |
|
28 |
22.5h 5° |
284 |
160 |
|
29 |
23.5h −7° |
203 |
120 |
|
Close
SSRS1 list
A redshift survey of galaxies in the southern sky in 1988, out to a distance of 120 Mpc/h, revealed some voids.[24]
More information #, Coordinates ...
# |
Coordinates |
Distance (V) |
Dimensions W × H × D (h−1 Mpc) |
Constellation |
Notes |
1 |
1.5h −50° |
3000 km/s |
30 × 30 × 40 |
Phoenix/Eridanus |
Located just behind the galaxy concentration in Eridanus-Fornax-Dorado |
2 |
21h −25° |
5000 km/s |
30 × 30 × 30 |
Capricornus/Microscopium |
|
3 |
23.5h −35° |
6000 km/s |
70 × 30 × 50 |
Sculptor/Grus |
|
4 |
4h −40° |
9000 km/s |
50 × 100 × 50 |
Horologium/Eridanus |
|
Close
SSRS2 list
In 1994, a redshift survey in the southern sky identified 18 voids, 11 of which are major voids.[19]
More information #, Coordinates ...
# |
Coordinates |
Distance (r) |
Diameter (h−1 Mpc) |
Constellation |
Notes |
1 |
1h 33m −16° 45′ |
85.7 |
54.3 |
Cetus |
major void |
2 |
3h 34m −28° 50′ |
99.7 |
56.2 |
Fornax |
major void SRSS1 Void 4 |
3 |
22h 25m −14° 46′ |
107.2 |
60.8 |
Aquarius |
major void |
4 |
21h 43m −14° 40′ |
66.7 |
35.6 |
Capricornus |
major void |
5 |
23h 48m −24° 39′ |
53.0 |
34.8 |
Aquarius/Sculptor |
major void SRSS1 Void 3 (Sculptor Void) |
6 |
3h 56m −20° 11′ |
56.5 |
32.0 |
Eridanus |
major void |
7 |
3h 17m −11° 40′ |
77.2 |
25.5 |
Eridanus |
major void |
8 |
23h 20m −12° 32′ |
83.9 |
27.8 |
Aquarius |
major void |
9 |
3h 06m −13° 47′ |
114.6 |
39.0 |
Eridanus |
major void |
10 |
0h 26m −9° 17′ |
104.7 |
34.8 |
Cetus |
major void |
11 |
0h 21m −29° 43′ |
112.8 |
42.9 |
Sculptor |
major void |
12 |
23h 03m −32° 35′ |
74.8 |
25.0 |
Piscis Austrinus/Sculptor |
|
13 |
1h 23m −19° 36′ |
31.0 |
22.1 |
Cetus |
SRSS1 Void 1 |
14 |
21h 28m −29° 28′ |
87.2 |
21.3 |
Piscis Austrinus/Microscopium |
|
15 |
21h 24m −33° 17′ |
116.1 |
27.3 |
Microscopium |
|
16 |
21h 43m −18° 41′ |
36.5 |
20.3 |
Capricornus |
|
17 |
3h 42m −21° 21′ |
32.1 |
19.0 |
Eridanus |
|
18 |
4h 18m −8° 42′ |
85.9 |
21.1 |
Eridanus |
|
Close
1994 EEDTA Whole Sky Survey
A 1994 census lists a total of 27 supervoids within a cube of 740 Mpc a side, centered on us (z=0.1 distant sphere).[25]
More information #, Coordinates (B1950.0) ...
# |
Coordinates (B1950.0) |
Distance (Mpc/h) |
Diameter (Mpc/h) [Note 1] |
Notes |
1 |
19.0° −57.1° |
134 |
88 |
|
2 |
28.2° −12.3° |
207 |
96 |
|
3 |
34.8° −61.9° |
216 |
72 |
|
4 |
36.6° −33.5° |
241 |
86 |
|
5 |
37.8° −36.1° |
129 |
92 |
|
6 |
46.0° −21.4° |
236 |
72 |
|
7 |
62.0° −8.0° |
248 |
100 |
|
8 |
71.2° −38.3° |
201 |
76 |
|
9 |
121.7° −1.5° |
96 |
112 |
Southern Local Supervoid |
10 |
130.0° +49.3° |
246 |
144 |
|
11 |
140.4° +10.5° |
160 |
92 |
|
12 |
146.9° +27.4° |
227 |
106 |
|
13 |
153.1° −11.4° |
246 |
94 |
|
14 |
159.9° +1.2° |
167 |
68 |
|
15 |
161.6° −32.2° |
241 |
98 |
|
16 |
167.4° +22.8° |
222 |
74 |
|
17 |
186.9° −15.6° |
216 |
94 |
|
18 |
196.8° +9.5° |
119 |
102 |
|
19 |
204.8° +35.7° |
119 |
108 |
|
20 |
214.6° +13.6° |
216 |
78 |
Boötes Void (Great Void) |
21 |
216.7° +56.5° |
143 |
116 |
|
22 |
219.8° +57.9° |
246 |
96 |
|
23 |
220.2° +33.9° |
219 |
72 |
|
24 |
256.1° −4.8° |
61 |
104 |
Northern Local Supervoid |
25 |
353.0° −59.4° |
198 |
74 |
|
26 |
356.6° +22.2° |
246 |
80 |
|
27 |
358.9° −33.1° |
241 |
70 |
|
Close
Galactic Anti-Center IRAS search
In a 1995 study of IRAS data looking for large-scale structure in the Galactic Anticenter in the Zone of Avoidance, four voids were discovered.[26]
More information #, Coordinates (B1950.0) ...
Close
IRAS list
Analysis of the IRAS redshift survey in 1997 revealed 24 voids, 12 of which were termed "significant"[27]
More information #, Supergalactic Coordinates (r,X,Y,Z) ...
# |
Supergalactic Coordinates (r,X,Y,Z) |
Diameter (h−1 Mpc) |
Data |
Notes |
1 |
(55.2,−10.4,−53.8,6.1) |
51.0 |
|
significant void |
2 |
(49.6,−25.3,31.4,−28.9) |
43.8 |
|
significant void |
3 |
(46.0,−24.8,26.7,28.1) |
44.5 |
|
significant void |
4 |
(46.5,8.7,24.7,38.4) |
45.0 |
|
significant void (Local Void) |
5 |
(32.0,−13.0,−23.9,−16.9) |
36.0 |
|
significant void |
6 |
(51.5,17.0,−32.2,36.4) |
41.4 |
|
significant void |
7 |
(57.1,31.2,44.9,16.5) |
43.5 |
|
significant void |
8 |
(60.4,−25.8,−22.7,−49.7) |
39.5 |
|
significant void |
9 |
(49.8,35.9,−25.6,−23.0) |
36.0 |
|
significant void |
10 |
(63.3,−48.0,−40.9,6.0) |
33.6 |
|
significant void (Sculptor Void) |
11 |
(48.6,11.8,46.6,−6.9) |
32.0 |
|
significant void |
12 |
(49.9,−15.6,−35.7,31.3) |
31.5 |
|
significant void |
13 |
(62.8,14.2,29.3,−53.7) |
40.3 |
|
|
14 |
(19.0,0.7,−16.4,9.6) |
28.8 |
|
|
15 |
(37.6,32.4,−17.0,8.6) |
30.4 |
|
Perseus–Pisces Void |
Close