Table 1

Radio astronomy stations operating in the Asia-Pacific Region

Country

Site

Longitude

(East)

Latitude

(North)

Operating Frequency (M/GHz)

Diameter
(m)

Remarks

Australia

Parkes

148 15' 44"

–33 00' 00"

440 M

640-704 M

1.2-1.8 G

2.2-2.5 G

2.6-3.6 G

4.5-5.1 G

5.9-6.8 G

8.1-8.7 G

12-15 G

21-24 G

64

S,VLBI

Mopra

149 05' 58"

–31 16' 04"

1.2-1.8 G

1.8-3.0 G

4.4-6.7 G

8.0-9.2 G

16-25 G

83.5-116 G

22

S,VLBI

ATCA (Narrabri)

149 32' 56"

–30 59' 52"

1.25-1.78 G

2.2-2.5 G

4.4-6.7 G

8.0-9.2 G

16-25 G

83.5-106 G

6 22m

I, VLBI

Tidbinbilla

148 58' 59"

–35 24' 18"

1.61-1.705 G

2.2-2.3 G

8.1-8.6 G

19-24.3 G

70m, 34m

S,VLBI

Hobart (Mt. Pleasant)

147 26' 21"

42 48' 18"

1.4 G

2.2 G

4.8 G

6.7 G

8.4 G

12.2 G

22.0 G

(bw=500 MHz)

26

S,VLBI

Ceduna

133.81

-31.87

2.2 G

4.8 G

6.7 G

8.4 G

12.2 G

22.0 G

(bw=500 MHz)

30

S,VLBI

MOST

149.42

-35.37

841.5-844.5 M

2 x (778m x 12m)

I

China

Shanghai

121.2

31.1

1.62-1.68 G

2.15-2.45 G

4.7-5.1 G

8.1-9.0 G

22.1-22.6 G

25

S, VLBI

Urmuqi

87.18

43.5

314-340 M

605-615 M

1.38-1.70 G

2.15-2.45 G

4.75-5.15 G

8.18-8.67 G

22-24 G

25

S, VLBI

MSRT

116 58'

40 33'

229-235 M

28 x 9m

I

MIYUN50

116 58'

40 33'

229-235 M

294.3-359.7 M

549.9-672.1 M

1-2 G

2.07-2.53 G

4.5-5.5 G

7.56-92.4  G

3.5-16.5 G

50

S, VLBI

Delingha

97 44'

37 22'

22-24 G

85-120 G

13.7

S

India

GMRT

74 03'

19 06'

37.5-1670 M

30 x 45m

I

ORT

76 40'

11 23'

325 M

530m x 30m

S

RRI mm-Telescope

77 38'

12 58'

6-8 G
40-50 G
75-120 G

10.4

S

T-Array

77 27'

13 36'

33.5-34.5 M

1 km x 0.5 km

I

Solar Heliograph

77 27'

13 36'

30-150 M

1.28 km x 0.441 km

I

IPS Array-Rajkot

70 56'

22 18'

103 M

?

S

Mauritius

MRT

57 44'

-20 08'

149-155 M

2 km x 1 km

I

Japan

Nobeyama

138 28' 32"

35 56' 29"

1.4-1.427 G
1.66-1.669 G
4.7-5.14 G
15.35-15.4 G
20-24 G
26-50 G
72-116 G

45

S

Nobeyama

138 28'

35 56'

85 – 116 G
126-152 G
213-237 G
325-365 G

10 x 6m

I

Nobeyama Heliograph

138 28'

35 56'

17 G
33.8 G

84 x 0.8m

I

Mizusawa

141 07' 56"

39 08' 00"

2.15-2.35 G
8.13-8.6 G
19.5-25.0 G
43-45 G

10

S,VLBI

VERA-Mizusawa

141 07' 57"

39 08' 01"

2.2-2.4 G
8.1-9.0 G
21.5-23.8 G

42.5-44.5 G
85-87 G

20

S,VLBI

VERA-Kagoshima

130 26' 24"

31 44' 52"

2.2-2.4 G
8.1-9.0 G
21.5-23.8 G

42.5-44.5 G
85-87 G

20

S,VLBI

VERA-Ogasawara

142 13' 00"

27 05' 31"

2.2-2.4 G
8.1-9.0 G
21.5-23.8 G

42.5-44.5 G
85-87 G

20

S,VLBI

VERA-Ishigakijima

124 10' 06"

24 24' 38"

2.2-2.4 G
8.1-9.0 G
21.5-23.8 G

42.5-44.5 G
85-87 G

20

S,VLBI

Kashima

140 39' 58"

35 57' 03"

1.45-1.75 G
2.25-2.35 G
4.6-5.1 G
7.86-8.68 G
10.2-10.7 G
14.4-15.4 G
21.9-22.4 G
23.5-24.0 G
42.9-43.4 G

34

S

Usuda

138 21' 57"

36 07' 45"

1.4-1.75 G
2.2-2.3 G
4.7-5.14 G
8-9 G
21.9-22.9 G

64

S

Nishi-Harima

133 00' 41"

33 32' 39"

18-250 M

?

S

Toyokawa

137 22' 09"

34 50' 05"

322-332 M

1012 m2

S

Fujigane

138 36' 42"

35 25' 36"

322-332 M

1500 m2

S

Sugadaira

138 19' 16"

36 31' 12"

322-332 M

1100 m2

S

Kiso

137 37' 49"

35 47' 34"

322-332 M

1405 m2

S

Zao

140 31' 59"

38 06' 07"

322-332 M

Four arrays

S

Hiraiso

140 37' 31"

36 22' 17"

25-70 M
70-500 M
1.4-1.6 G
2.8 G

Log-periodic
10
6
2

S
S
S
S

Nishi-Waseda

139 43' 20"

35 42' 25"

10.65 G

2.4 x 64

S

Nasu

139 59'

36 55' 30"

1.4 G

20 x 5

S

Nagoya

136 58'

35 09'

110-116 G

4

S

Mt.Fuji

138 43' 38"

35 21' 44"

325-350 G
440-500 G
800-830 G

1.2

S

Tomakomai

141 36' 00"

42 40' 19"

2, 8, 22, 43 G

11

S,VLBI

Gifu

136 44' 22"

35 28' 03"

?

11

S

Yamaguchi

131 33' 35"

34 12' 48"

?

32

S

Korea

Taejon

127 22' 18"

36 23' 54"

43-175 G

13.7

S, VLBI

K-SRBL

127.37

36.40

245, 410 M

1-18 G

2 x 2m

S

KVN-Yonsei

126 56' 35"

37 33' 44"

2-115 G

20

S, VLBI

KVN-Ulsan

129 15' 04"

35 32' 33"

2-115 G

20

S, VLBI

KVN-Tamna

126 27' 43"

33 17' 18"

2-115 G

20

S, VLBI

Seoul

126 57' 19"

37 27' 15"

85-115G
200-270G

6

S

Ichon (RRL)

127 32' 58"

37 09' 01"

30M-2.5G

6, 10

S

Taiwan

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New Zealand

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NOTE – S refers to stations were single-dish operations are made, I stands for Interferometer, and VLBI refers to stations used exclusively for very long baseline interferometry.