A Herschel view of the far-infrared properties of submillimetre galaxies

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Volume 539 (March 2012)

A&A, 539 (2012) A155

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Table 11

Mid- and far-infrared properties of our lensed-SMG sample.

Reference submm source and its counterpart

PEP/HerMES multi-wavelength counterpart

field

name

submm position^a

counterpart position

infrared position

Δr

S₂₄

S₁₀₀

S₁₆₀

S₂₅₀

S₃₅₀

S₅₀₀

Dec

″

μJy

mJy

A1835

SMMJ14011+0252

14 01 04.96

+02 52 23.50 S

14 01 04.97

+02 52 24.60

14 01 04.97

+02 52 24.54

0.1

883.4 ± 14.5

11.6 ± 0.8

33.5 ± 1.4

61.7 ± 6.0

63.1 ± 3.8

48.5 ± 4.0

A1835

SMMJ14009+0252

14 00 57.55

+02 52 48.60 S

14 00 57.57

+02 52 49.10

14 00 57.58

+02 52 48.95

0.2

297.7 ± 13.7

4.9 ± 0.7

27.7 ± 1.9

66.4 ± 6.0

65.8 ± 3.8

53.7 ± 4.2

A2219

SMMJ16403+4644

16 40 19.40

+46 44 01.00 S

16 40 19.50

+46 44 00.50

16 40 19.46

+46 44 00.81

0.5

729.7 ± 7.6

17.1 ± 0.9

35.6 ± 1.9

50.5 ± 5.8

44.9 ± 3.6

34.7 ± 6.5

MS1054

SMMJ10570-0334

10 57 02.20

-03 36 04.00 S

.........

10 57 02.50

-03 36 02.52

4.7

253.1 ± 12.0

...

10.6 ± 2.1

15.2 ± 1.2

17.0 ± 1.1

...

CL0024

SMMJ00266+1708

00 26 34.10

+17 08 32.00 S

00 26 34.06

+17 08 33.10

00 26 34.09

+17 08 34.16

1.1

283.4 ± 15.4

4.7 ± 0.7

24.5 ± 2.2

52.8 ± 7.2

61.3 ± 4.5

44.6 ± 4.7

MS0451

SMMJ04542-0301

04 54 12.50

-03 01 04.00 S

.........

04 54 12.73

-03 01 09.25

...

169.9 ± 10.5

14.6 ± 1.2

40.6 ± 7.7

76.0 ± 15.1

94.4 ± 8.8

84.1 ± 11.5

A2390

SMMJ21536+1742

21 53 38.20

+17 42 16.00 S

21 53 38.35

+17 42 20.70

21 53 38.51

+17 42 17.73

3.8

382.7 ± 8.0

3.8 ± 0.9

11.9 ± 2.1

52.4 ± 12.7

54.8 ± 7.1

47.5 ± 7.2

A2218

SMMJ16354+6611

16 35 41.20

+66 11 44.00 S

16 35 41.20

+66 11 44.00

16 35 40.73

+66 11 42.96

3.1

411.8 ± 156.3

1.0 ± 0.7

13.6 ± 1.2

20.5 ± 6.0

25.7 ± 3.0

17.4 ± 3.3

A2218

SMMJ16355+66120C

16 35 50.96

+66 12 05.50 S

16 35 50.96

+66 12 05.50

16 35 50.75

+66 12 06.31

1.5

280.2 ± 26.2

4.9 ± 0.7

18.5 ± 1.6

37.8 ± 6.0

35.9 ± 3.1

...

A2218

SMMJ16355+66122B

16 35 54.10

+66 12 23.80 S

16 35 54.10

+66 12 23.80

16 35 53.91

+66 12 22.43

1.8

2709.2 ± 129.0

9.4 ± 0.9

28.1 ± 1.9

78.1 ± 6.0

70.2 ± 7.2

74.7 ± 3.5

A2218

SMMJ16355+66123A

16 35 55.18

+66 12 37.20 S

16 35 55.18

+66 12 37.20

16 35 54.96

+66 12 37.04

1.4

2955.0 ± 123.4

5.9 ± 1.1

21.3 ± 2.0

53.7 ± 6.0

47.1 ± 3.1

26.9 ± 3.5

A2218

SMMJ16355+6611

16 35 55.20

+66 11 50.00 S

16 35 55.20

+66 11 50.00

16 35 55.00

+66 11 50.62

1.4

4724.5 ± 182.7

26.4 ± 0.8

51.0 ± 1.5

42.1 ± 6.0

37.2 ± 3.0

14.9 ± 3.3

A370

SMMJ02399-0136

02 39 51.90

-01 35 59.00 S

02 39 51.88

-01 35 58.00

02 39 51.86

-01 35 58.45

0.5

1231.0 ± 11.6

13.0 ± 0.8

30.1 ± 1.8

65.7 ± 6.1

72.0 ± 3.9

62.8 ± 4.6

A370

SMMJ02399-0134

02 39 56.40

-01 34 27.00 S

02 39 56.51

-01 34 27.10

02 39 56.58

-01 34 26.10

1.4

2402.0 ± 10.9

45.8 ± 0.8

111.1 ± 1.9

125.8 ± 6.1

89.8 ± 3.9

41.7 ± 4.4

A1689

SMMJ13115-1208

13 11 29.10

-01 20 49.00 S

13 11 29.14

-01 20 46.50

13 11 29.14

-01 20 46.47

0.1

329.8 ± 12.8

3.3 ± 0.4

7.6 ± 0.8

...

16.1 ± 4.1

17.3 ± 4.4

Notes.

^(a)

After the position, we indicate the (sub)mm observation from which the multi-wavelength identification has been made, S: SCUBA, L: Laboca, A: AzTEC and M: MAMBO.

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