Planck intermediate results. XV. A study of anomalous microwave emission in Galactic clouds

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201322612e]

Table 3

List of 98 candidate AME regions. Names are given by the central Galactic coordinates.

EM_ff

τ ₂₅₀

T _d

β _d

ΔT_CMB

A _sp

σ _AME

ν _sp

G ₀

Notes

Name

[°]

[cm^-6 pc]

[× 10⁵]

[K]

[ μK_CMB]

[10²⁰ cm^-2]

[GHz]

[Jy]

[× 10⁴]

G004.24+18.09 ^a .....

1.0 ± 1.8

1.0 ± 0.1

17.1 ± 0.3

1.70 ± 0.05

−16 ± 1

6.2 ± 0.4

15.6

29.0 ± 0.9

0.00

0.88 ± 0.09

5.3 ± 0.7

16.2 ± 3.4

1.35

LDN137/141

G005.40+36.50 ^a .....

1.5 ± 1.5

0.9 ± 1.5

2.5 ± 0.3

14.0 ± 0.3

1.99 ± 0.06

40 ± 2

2.1 ± 0.1

18.7

25.9 ± 2.3

0.00

0.27 ± 0.04

1.7 ± 0.3

8.0 ± 1.9

1.09

LDN134

G008.51−00.31^a .....

1338 ± 643

30.0 ± 4.7

19.1 ± 0.7

2.02 ± 0.08

198 ± 220

54 ± 28

1.9

...

1.7 ± 0.3

46 ± 54

1.3 ± 1.5

0.16

Synch. Faint SNR8.3−0.0; 1.2 Jy @ 1 GHz

G010.19−00.32^a .....

1.2 ± 0.5

2067 ± 502

37.8 ± 5.1

19.7 ± 0.6

2.05 ± 0.07

335 ± 189

80 ± 23

3.4

26.0 ± 2.1

1.01

2.0 ± 0.4

67 ± 42

1.1 ± 0.7

0.25

Kes62. Synch. SNR9.9−0.8; 6.7 Jy @ 1 GHz

G012.80−00.19^a .....

1.7 ± 0.7

2414 ± 473

46.4 ± 13.5

19.5 ± 1.2

2.03 ± 0.10

344 ± 230

85 ± 31

2.7

26.0 ± 2.2

0.47

1.9 ± 0.7

71 ± 39

1.0 ± 0.6

0.14

W33. Synch. Several weak SNRs

G015.06−00.69^a .....

0.4 ± 0.2

7472 ± 506

29.5 ± 3.4

20.6 ± 0.5

2.10 ± 0.11

533 ± 251

77 ± 40

1.9

...

2.6 ± 0.4

60 ± 44

0.9 ± 0.7

0.22

M17

G017.00+00.85 ^a .....

0.6 ± 0.3

869 ± 130

22.3 ± 10.8

18.2 ± 1.6

2.08 ± 0.18

75 ± 109

68 ± 12

5.3

35.0 ± 6.2

0.03

1.3 ± 0.7

58 ± 18

3.2 ± 1.3

0.87

M16, W37

G023.47+08.19 ^a .....

1.5 ± 1.2

1.6 ± 1.0

4.8 ± 0.5

13.9 ± 0.2

1.97 ± 0.07

33 ± 4

4.2 ± 0.5

8.5

23.0 ± 5.7

0.00

0.26 ± 0.02

3.2 ± 0.6

9.8 ± 2.5

1.38

LDN462

G028.79+03.49^a .....

0.3 ± 0.1

512 ± 38

3.3 ± 0.2

22.9 ± 0.3

1.49 ± 0.05

−100 ± 27

0.6 ± 3.0

0.2

...

5.1 ± 0.4

−0.7 ± 3.8

−0.1 ± 0.4

1.77

W40

G030.77−00.03^a .....

1.1 ± 0.2

4730 ± 255

46.2 ± 3.3

21.4 ± 0.3

1.93 ± 0.06

603 ± 180

194 ± 22

8.5

28.5 ± 0.4

0.37

3.4 ± 0.3

166 ± 29

1.5 ± 0.3

0.76

W43

G035.20−01.74^a .....

713 ± 129

13.0 ± 1.8

19.0 ± 0.5

1.74 ± 0.12

4 ± 101

21 ± 11

2.0

...

1.6 ± 0.3

16 ± 14

1.4 ± 1.2

0.06

W48

G037.79−00.11^b .....

1.3 ± 0.3

1768 ± 348

27.0 ± 8.5

19.7 ± 1.3

1.90 ± 0.10

184 ± 157

61 ± 18

3.4

25.5 ± 2.8

0.35

2.0 ± 0.8

49 ± 29

1.3 ± 0.8

0.36

W47. Synch. Several weak SNRs

G040.52+02.53^a .....

0.6 ± 0.3

231 ± 37

2.4 ± 0.5

20.6 ± 1.0

1.67 ± 0.15

9 ± 37

1.0 ± 4.1

0.2

...

2.7 ± 0.8

1.1 ± 4.9

0.3 ± 1.3

0.09

W45

G043.20−00.10^a .....

1.1 ± 0.3

1433 ± 100

18.4 ± 5.1

19.4 ± 1.1

1.88 ± 0.09

187 ± 74

50.5 ± 9.4

5.4

26.0 ± 2.2

1.23

1.9 ± 0.6

39 ± 12

1.8 ± 0.6

0.37

W49

G045.47+00.06^a .....

1.8 ± 0.6

748 ± 70

9.1 ± 0.6

21.4 ± 0.4

1.63 ± 0.07

97 ± 67

39.1 ± 6.6

5.9

27.3 ± 0.8

0.80

3.3 ± 0.3

33.4 ± 9.5

2.2 ± 0.7

0.75

NRAO601 - SNR in SIMBAD

G053.63+00.19^a .....

1.9 ± 0.7

625 ± 49

5.9 ± 0.6

20.4 ± 0.4

1.70 ± 0.07

44 ± 38

17.0 ± 4.6

3.7

27.0 ± 1.1

0.57

2.5 ± 0.3

14.2 ± 6.1

1.6 ± 0.7

0.30

W52

G059.42−00.21^a .....

1.1 ± 0.5

294 ± 27

6.8 ± 2.3

18.3 ± 1.2

1.92 ± 0.12

−26 ± 22

18.0 ± 2.6

7.0

26.8 ± 1.3

0.37

1.3 ± 0.5

14.6 ± 3.9

2.6 ± 0.8

0.71

W55

G061.47+00.11^a .....

1.2 ± 0.8

328 ± 23

2.4 ± 0.8

21.8 ± 1.6

1.59 ± 0.12

4 ± 22

4.7 ± 2.5

1.9

...

3.7 ± 1.7

3.9 ± 3.8

0.8 ± 0.7

0.58

HII LBN061.50+00.29. SH2-88

G062.98+00.05^a .....

1.2 ± 1.5

201 ± 14

3.5 ± 1.1

18.9 ± 1.1

1.82 ± 0.10

38 ± 12

9.8 ± 1.3

7.5

25.7 ± 2.5

0.25

1.6 ± 0.6

8.1 ± 2.0

2.3 ± 0.7

1.45

S89

G068.16+01.02^a .....

0.8 ± 0.5

187 ± 13

0.9 ± 0.2

20.6 ± 0.9

1.89 ± 0.20

40 ± 12

0†

...

2.7 ± 0.7

0.0 ± 2.0

0.0 ± 1.2

0.22

S98

G071.59+02.85^a .....

1.0 ± 0.4

286 ± 51

2.0 ± 1.2

19.9 ± 2.5

1.75 ± 0.24

−5 ± 34

9.2 ± 5.0

1.8

...

2.2 ± 1.6

7.8 ± 6.3

3.0 ± 2.5

0.06

S101

G075.81+00.39^a .....

0.7 ± 0.8

423 ± 50

4.4 ± 0.7

19.3 ± 0.7

1.72 ± 0.08

118 ± 36

12.4 ± 4.9

2.5

26.8 ± 1.3

1.07

1.8 ± 0.4

9.0 ± 6.1

2.0 ± 1.4

0.11

HII GAL075.84+00.40. SH2-105. Cyg 2N

G076.38−00.62^a .....

138 ± 42

1.8 ± 0.8

20.8 ± 2.3

2.20 ± 0.36

52 ± 39

0†

...

2.8 ± 1.9

2.2 ± 8.1

0.4 ± 1.5

0.35

S106

G081.59+00.01^a .....

1.0 ± 0.6

3726 ± 304

7.1 ± 2.0

24.1 ± 1.6

1.67 ± 0.10

140 ± 139

32 ± 25

1.3

...

6.9 ± 2.7

25 ± 29

0.8 ± 1.0

0.21

HII DR23. Near Cygnus X

G093.02+02.76^a .....

0.8 ± 0.3

614 ± 49

2.9 ± 0.3

20.4 ± 0.4

1.58 ± 0.09

−23 ± 35

5.9 ± 3.8

1.6

...

2.5 ± 0.3

4.7 ± 4.7

1.1 ± 1.2

0.18

HII GAL093.06+2.81

G094.47−01.53^a .....

0.8 ± 0.3

270 ± 33

0.6 ± 0.3

20.9 ± 2.6

1.79 ± 0.40

−3 ± 23

1.5 ± 2.4

0.6

...

2.9 ± 2.2

1.3 ± 3.0

1.0 ± 2.5

0.07

HII LBN094.79−01.77. LDN1059

G098.00+01.47^a .....

0.5 ± 0.1

155 ± 14

0.9 ± 0.3

19.2 ± 1.2

1.73 ± 0.12

5 ± 9

7.6 ± 1.2

6.1

35.1 ± 6.3

0.47

1.8 ± 0.7

6.1 ± 1.6

6.3 ± 1.9

0.46

RNe GM1-12, DNe TGU H582

G099.60+03.70^a .....

544 ± 24

0.6 ± 0.2

21.5 ± 1.4

2.09 ± 0.22

−41 ± 16

1.4 ± 2.3

0.6

...

3.4 ± 1.4

0.1 ± 2.3

0.1 ± 1.3

0.33

Tr 37 cluster. Large complex incl. LDN1111

G102.88−00.69^a .....

0.6 ± 0.1

372 ± 27

1.3 ± 0.3

20.7 ± 0.9

1.64 ± 0.13

−60 ± 17

5.4 ± 2.1

2.5

32.3 ± 3.9

0.02

2.7 ± 0.7

4.6 ± 2.7

2.1 ± 1.3

0.38

HII G102.9−00.7. LDN1161/1163

G107.20+05.20^a .....

1.0 ± 0.3

258 ± 19

3.0 ± 0.3

20.2 ± 0.4

1.87 ± 0.08

59 ± 17

16.3 ± 1.6

9.9

29.2 ± 1.1

1.03

2.4 ± 0.3

13.9 ± 2.1

2.7 ± 0.5

0.94

AME-G107.2+5.2¹ .....

G109.01+00.00^b .....

1.1 ± 1.9

51 ± 11

1.3 ± 0.4

19.5 ± 1.1

1.81 ± 0.16

−18 ± 9

3.7 ± 2.4

1.5

...

1.9 ± 0.6

2.3 ± 1.9

1.4 ± 1.2

0.10

DNe TGU H684. Near HII LBN108.80−00.98

G110.25+02.58^ab .....

0.8 ± 0.1

296 ± 23

1.0 ± 0.3

25.6 ± 2.1

1.52 ± 0.10

−42 ± 18

6.9 ± 2.0

3.4

40 ± 10

5.41

9.7 ± 4.7

4.5 ± 2.8

0.8 ± 0.5

0.24

HII G110.2+02.5. LBN110.11+02.44

G118.09+04.96^a .....

0.8 ± 0.2

1295 ± 22

1.4 ± 0.1

24.0 ± 0.4

1.81 ± 0.09

26 ± 16

0†

...

6.6 ± 0.7

−1.1 ± 3.5

−0.2 ± 0.5

0.49

Weak SNR NGC 7822

G123.13−06.27^a .....

0.4 ± 0.1

182 ± 13

0.7 ± 0.1

20.5 ± 0.4

1.65 ± 0.09

11 ± 6

2.0 ± 1.1

1.8

...

2.6 ± 0.3

1.5 ± 1.1

1.4 ± 1.1

0.37

S184

G133.27+09.05 ^ab .....

1.3 ± 0.5

25 ± 3

4.5 ± 0.3

14.5 ± 0.2

1.83 ± 0.06

8 ± 8

3.4 ± 0.4

8.5

24.3 ± 4.1

0.08

0.32 ± 0.03

2.7 ± 0.9

6.2 ± 2.2

0.13

LDN1358/1355/1357

G133.74+01.22^a .....

0.6 ± 0.2

2155 ± 116

3.3 ± 0.8

25.3 ± 1.5

1.67 ± 0.08

53 ± 56

14.8 ± 9.8

1.5

...

9.2 ± 3.3

10 ± 10

0.5 ± 0.5

0.97

G142.35+01.35 ^a .....

1.9 ± 1.7

0 ± 10

4.4 ± 1.3

16.8 ± 0.9

1.76 ± 0.10

37 ± 10

6.7 ± 0.7

9.5

24.8 ± 3.5

0.07

0.8 ± 0.3

5.3 ± 2.1

3.6 ± 1.5

0.45

DNe TGU H942

G151.62−00.28^a .....

1.0 ± 0.7

348 ± 30

1.3 ± 0.1

21.0 ± 0.4

1.38 ± 0.08

8 ± 23

3.6 ± 2.3

1.5

...

3.0 ± 0.3

2.8 ± 2.9

1.5 ± 1.6

0.21

HII SH2-209

G158.40−20.60^a .....

0 ± 11

3.6 ± 0.2

15.5 ± 0.1

1.74 ± 0.06

56 ± 11

5.3 ± 0.3

16.3

26.6 ± 1.6

0.26

0.49 ± 0.03

4.4 ± 1.3

6.9 ± 2.2

1.69

LDN1450/1452

G160.26 − 18.62 ^abc .....

1.5 ± 0.7

66 ± 6

4.6 ± 0.3

17.4 ± 0.2

1.92 ± 0.06

51 ± 8

13.3 ± 0.8

17.4

27.8 ± 0.3

0.04

0.98 ± 0.07

12.0 ± 1.2

4.4 ± 0.7

0.70

Perseus AME-G160.26−18.62¹ .....

G160.60 − 12.05 ^a .....

1.4 ± 0.2

379 ± 19

0.5 ± 0.2

21.7 ± 1.6

2.01 ± 0.16

−8 ± 10

8.3 ± 1.6

5.1

50 ± 17

0.00

3.7 ± 1.7

3.8 ± 1.9

2.6 ± 1.3

0.33

NGC 1499 (California nebula)

G166.44−24.08^ac .....

1.4 ± 1.2

11.2 ± 1.5

0.5 ± 0.0

22.7 ± 0.4

1.77 ± 0.06

14 ± 1

0.9 ± 0.2

4.3

20.8 ± 8.5

0.00

4.7 ± 0.6

0.5 ± 0.2

0.3 ± 0.2

0.58

Pleiades²

G173.56−01.76^a .....

0.5 ± 0.1

401 ± 32

0.4 ± 0.2

22.7 ± 2.1

1.68 ± 0.17

−17 ± 15

2.1 ± 2.6

0.8

...

4.8 ± 2.7

1.9 ± 2.9

1.6 ± 2.5

0.39

NGC 1893

G173.62+02.79^abc .....

0.7 ± 0.2

194 ± 16

3.9 ± 0.2

18.7 ± 0.2

1.64 ± 0.04

−6 ± 12

7.9 ± 1.4

5.6

26.2 ± 1.9

1.22

1.47 ± 0.09

6.5 ± 1.9

2.2 ± 0.7

0.36

S235, AME-G173.6+2.8¹ .....

G180.80+04.30 ^a .....

1.2 ± 0.6

0.7 ± 1.8

0.7 ± 0.1

17.7 ± 0.5

1.73 ± 0.12

−14 ± 7

2.9 ± 0.2

13.2

25.5 ± 2.7

0.00

1.08 ± 0.17

2.6 ± 0.5

6.9 ± 1.6

1.13

LDN1557

G182.36+00.22^ab .....

1.0 ± 0.5

3.6 ± 1.5

1.9 ± 0.6

16.3 ± 1.0

1.78 ± 0.12

64 ± 6

2.4 ± 0.5

4.5

26.9 ± 1.2

0.36

0.7 ± 0.2

2.0 ± 1.1

3.6 ± 2.0

0.14

HII LBN182.30+00.07 & RNe/DNe

G190.00+00.46^a .....

0.5 ± 0.1

278 ± 19

3.5 ± 0.2

19.4 ± 0.2

1.67 ± 0.05

46 ± 15

11.5 ± 1.6

7.4

27.7 ± 0.3

0.58

1.83 ± 0.12

9.7 ± 2.1

2.6 ± 0.7

0.91

NGC 2174/2175

G192.34 − 11.37 ^a .....

1.5 ± 0.9

8 ± 6

1.4 ± 0.4

17.3 ± 1.0

1.93 ± 0.12

25 ± 5

9.1 ± 0.7

12.3

30.2 ± 2.0

0.00

0.9 ± 0.3

7.6 ± 1.0

11.7 ± 2.3

2.46

LDN1582/1584

G192.60−00.06^a .....

1.1 ± 0.6

65 ± 8

1.0 ± 0.3

20.8 ± 1.5

1.83 ± 0.14

−7 ± 10

3.8 ± 0.9

4.3

27.2 ± 0.9

0.50

2.9 ± 1.3

3.2 ± 1.2

1.6 ± 0.7

0.12

S255

G201.62+01.63 ^a .....

0.8 ± 0.4

161 ± 16

1.4 ± 0.2

18.0 ± 0.6

2.11 ± 0.17

90 ± 12

9.6 ± 1.3

7.4

27.4 ± 0.7

0.06

1.2 ± 0.2

7.9 ± 1.5

6.3 ± 1.5

0.88

LPH96 201.6+1.6. LDN1608/1609³ .....

G203.24+02.08 ^a .....

1.6 ± 0.9

103 ± 9

3.8 ± 1.0

16.9 ± 0.9

1.77 ± 0.09

19 ± 10

7.8 ± 0.9

8.3

30.3 ± 2.1

0.02

0.8 ± 0.2

6.6 ± 1.9

4.3 ± 1.4

0.55

HII G203.2+02.1. LDN1613. Cone nebula.

G204.70 − 11.80 ^c .....

23 ± 6

2.1 ± 0.2

16.5 ± 0.3

1.84 ± 0.06

7 ± 7

6.6 ± 0.9

7.4

30.1 ± 1.9

0.00

0.70 ± 0.09

5.8 ± 1.2

9.5 ± 2.5

1.23

LDN1622

G208.80−02.65^a .....

0.9 ± 0.6

124 ± 8

0.8 ± 0.2

19.0 ± 0.8

1.64 ± 0.13

12 ± 10

1.8 ± 0.9

2.0

...

1.7 ± 0.4

1.6 ± 1.5

2.2 ± 2.1

0.26

S280

G209.01−19.38^a .....

0.3 ± 0.1

4278 ± 226

14.8 ± 1.2

21.2 ± 0.3

2.13 ± 0.09

371 ± 102

32 ± 18

1.8

...

3.1 ± 0.3

24 ± 19

0.5 ± 0.4

1.13

M42 (Orion nebula)

G211.98 − 01.17 ^a .....

0.8 ± 0.2

164 ± 10

0.8 ± 0.1

20.4 ± 0.4

1.65 ± 0.09

59 ± 8

4.8 ± 0.9

5.5

27.3 ± 0.8

0.14

2.5 ± 0.3

3.9 ± 1.1

3.4 ± 1.1

0.94

HII LBN211.65−01.51

G213.71−12.60^ab .....

0.6 ± 0.1

68 ± 5

2.7 ± 0.2

20.1 ± 0.2

1.73 ± 0.05

13 ± 8

7.6 ± 0.5

14.9

27.0 ± 1.1

3.93

2.31 ± 0.17

6.5 ± 1.0

1.4 ± 0.3

1.45

RNe NGC 2170. Mon R2

G218.05−00.38^ab .....

1.2 ± 1.2

10.3 ± 1.4

0.8 ± 0.3

19.9 ± 1.4

1.51 ± 0.12

−13 ± 5

3.7 ± 0.4

9.4

25.9 ± 2.3

0.52

2.2 ± 0.9

3.3 ± 1.1

4.1 ± 1.5

2.60

Mon R2. LDN1650

G219.18 − 08.93 ^a .....

0.5 ± 0.5

0.6 ± 1.1

1.7 ± 0.1

16.2 ± 0.2

1.86 ± 0.04

0 ± 2

2.0 ± 0.1

18.9

23.3 ± 5.2

0.00

0.64 ± 0.04

1.5 ± 0.2

2.9 ± 0.6

1.64

RNe LBN1015, DNe TGU H1544/1546

G231.83 − 02.00 ^a .....

1.4 ± 1.0

13.7 ± 1.0

1.7 ± 0.2

16.8 ± 0.4

1.50 ± 0.07

36 ± 6

3.4 ± 0.3

11.4

26.5 ± 1.6

0.03

0.79 ± 0.12

2.9 ± 1.1

6.5 ± 2.7

0.60

DNe TGU H1593

G234.20 − 00.20 ^ab .....

0.8 ± 0.7

87 ± 5

2.5 ± 0.2

18.5 ± 0.3

1.63 ± 0.07

−46 ± 8

8.2 ± 0.6

14.5

26.3 ± 1.8

0.05

1.38 ± 0.14

6.8 ± 1.3

4.3 ± 1.0

1.25

HII LBN1050

G239.40 − 04.70 ^a .....

1.6 ± 0.5

80 ± 4

1.4 ± 0.1

17.3 ± 0.4

1.89 ± 0.14

18 ± 8

5.2 ± 0.5

9.9

30.7 ± 2.5

0.00

0.93 ± 0.14

4.5 ± 0.9

6.2 ± 1.5

0.95

LDN1667. HII LBN1059. V VY Cma

G243.16+00.42^a .....

0.3 ± 0.1

171 ± 10

0.4 ± 0.1

21.5 ± 1.1

1.83 ± 0.16

−2 ± 6

3.6 ± 0.8

4.2

29.5 ± 1.4

0.00

3.4 ± 1.0

3.0 ± 1.0

2.8 ± 1.0

0.56

NGC 2467

G247.60 − 12.40 ^ab .....

1.2 ± 0.9

10.3 ± 1.4

0.5 ± 0.0

18.8 ± 0.5

1.59 ± 0.13

−5 ± 4

3.6 ± 0.3

14.0

27.3 ± 0.8

0.00

1.6 ± 0.2

3.0 ± 0.6

8.3 ± 1.9

0.79

DNe TGU H1630

G253.80−00.20^ab .....

0.9 ± 0.5

227 ± 13

2.2 ± 0.2

19.3 ± 0.3

1.63 ± 0.07

61 ± 13

10.2 ± 1.1

9.5

28.7 ± 0.6

0.31

1.81 ± 0.15

8.8 ± 1.7

4.3 ± 1.0

0.57

Gum 10. RNe BRAN124/126

G259.30 − 13.50 ^a .....

1.1 ± 0.6

33.0 ± 2.0

0.3 ± 0.0

19.8 ± 0.4

1.68 ± 0.07

7 ± 3

2.9 ± 0.3

10.5

27.9 ± 0.2

0.00

2.1 ± 0.3

2.7 ± 0.4

7.1 ± 1.5

1.10

BRAN34. DNe TGU H1667

G260.50+00.40^a .....

243 ± 16

2.9 ± 0.4

18.7 ± 0.6

1.70 ± 0.07

58 ± 14

6.4 ± 1.9

3.3

23.9 ± 4.6

0.10

1.5 ± 0.3

4.8 ± 2.4

2.1 ± 1.1

0.15

Vela-D mol cloud. BRAN166

G265.15+01.45^a .....

0.5 ± 0.5

360 ± 41

2.5 ± 0.3

21.7 ± 0.8

1.48 ± 0.16

−125 ± 100

8.2 ± 9.0

0.9

...

3.7 ± 0.8

1.8 ± 7.3

0.3 ± 1.4

0.12

RCW36

G267.95−01.06^a .....

0.3 ± 0.1

3170 ± 165

3.6 ± 0.9

24.0 ± 1.4

1.98 ± 0.09

195 ± 67

24 ± 13

1.9

...

6.6 ± 2.3

19 ± 14

0.9 ± 0.7

0.70

RCW38

G270.27+00.84^a .....

0.9 ± 0.6

106 ± 24

4.7 ± 0.5

18.0 ± 0.4

1.71 ± 0.10

−32 ± 28

7.5 ± 3.4

2.2

24.3 ± 4.1

0.34

1.18 ± 0.16

6.3 ± 4.6

2.2 ± 1.7

0.04

RCW41

G274.01−01.15^a .....

0.1 ± 0.1

332 ± 18

0.4 ± 0.0

25.7 ± 1.0

1.65 ± 0.17

−37 ± 10

2.7 ± 1.6

1.6

...

10.1 ± 2.4

1.8 ± 2.0

0.7 ± 0.7

0.41

HII Gum26. RNe BRAN261/258

G282.02−01.16^a .....

1.1 ± 0.6

1726 ± 82

6.6 ± 0.6

23.1 ± 0.5

1.47 ± 0.05

8 ± 61

29.8 ± 6.8

4.4

28.9 ± 0.8

0.56

5.3 ± 0.7

23.5 ± 8.8

1.3 ± 0.5

0.43

RCW46

G284.30−00.30^ab .....

0.7 ± 0.2

4534 ± 249

6.7 ± 0.6

24.2 ± 0.6

1.71 ± 0.10

215 ± 135

47 ± 20

2.4

31.9 ± 3.6

0.64

7.0 ± 1.0

35 ± 22

1.0 ± 0.7

0.49

RCW49, NGC 3247⁴

G287.48−00.63^a .....

0.7 ± 0.1

8492 ± 322

6.3 ± 0.4

25.8 ± 0.4

1.89 ± 0.10

350 ± 134

52 ± 27

2.0

...

10.2 ± 0.9

35 ± 30

0.6 ± 0.5

0.84

RCW53, NGC 3372 (Carina nebula)

G289.80−01.15^a .....

1.1 ± 1.4

1250 ± 111

2.2 ± 1.0

25.2 ± 2.9

1.42 ± 0.15

−76 ± 96

0†

...

8.9 ± 6.2

−8 ± 23

−0.8 ± 2.3

0.12

Gum35, RCW54

G291.63−00.52^a .....

0.5 ± 0.1

4456 ± 215

3.7 ± 0.3

26.2 ± 0.5

1.74 ± 0.08

193 ± 94

34 ± 17

1.9

...

11.2 ± 1.3

24 ± 19

0.8 ± 0.7

0.51

RCW57, NGC 3603/3576

G293.35 − 24.47 ^b .....

15.2 ± 0.8

0.4 ± 0.1

18.1 ± 0.5

1.50 ± 0.07

30 ± 3

1.4 ± 0.2

8.9

23.7 ± 4.8

0.00

1.2 ± 0.2

1.1 ± 0.3

4.7 ± 1.7

0.41

DNe TGU H1811/1810/1815

G294.98−01.71^a .....

0.6 ± 0.3

1033 ± 66

2.3 ± 1.0

23.3 ± 2.4

1.62 ± 0.16

62 ± 50

12.6 ± 6.2

2.0

33.6 ± 5.1

0.63

5.6 ± 3.4

9.1 ± 8.7

1.1 ± 1.1

0.10

RCW62

G298.60−00.20^a .....

0.8 ± 0.1

2169 ± 103

6.8 ± 1.6

22.0 ± 1.2

1.73 ± 0.07

137 ± 59

28.1 ± 8.8

3.2

26.6 ± 1.6

0.82

4.0 ± 1.3

22 ± 10

1.2 ± 0.6

0.23

Several DNe. HII GAL298.56−00.11

G305.27+00.15^a .....

0.6 ± 0.1

3090 ± 145

17.4 ± 1.5

21.1 ± 0.4

2.08 ± 0.08

417 ± 83

78 ± 12

6.3

29.1 ± 1.0

0.92

3.1 ± 0.3

65 ± 14

1.2 ± 0.3

0.74

RCW74

G311.94+00.12^a .....

2655 ± 174

21.3 ± 1.9

21.7 ± 0.4

1.71 ± 0.05

25 ± 121

67 ± 15

4.2

25.4 ± 2.8

0.51

3.6 ± 0.4

53 ± 19

1.1 ± 0.4

0.18

Several DNe. HII GAL311.89+00.10

G317.51−00.11^b .....

2226 ± 141

19.0 ± 1.6

20.7 ± 0.4

1.78 ± 0.06

178 ± 95

56 ± 12

4.6

27.7 ± 0.4

0.67

2.8 ± 0.3

47 ± 15

1.4 ± 0.5

0.15

Several DNe. HII GAL317.60−00.36

G318.49 − 04.28 ^a .....

1.0 ± 0.3

102 ± 17

2.9 ± 0.3

17.2 ± 0.3

1.99 ± 0.11

46 ± 15

8.0 ± 1.5

5.2

30.8 ± 2.6

0.00

0.92 ± 0.10

6.6 ± 2.1

4.0 ± 1.4

0.58

RNe GN15.11.0. DNe TGU H1978

G320.27−00.27^ab .....

1.5 ± 1.2

1349 ± 91

10.5 ± 1.0

22.6 ± 0.5

1.66 ± 0.05

134 ± 64

53.3 ± 7.9

6.8

27.3 ± 0.8

0.69

4.6 ± 0.6

44.3 ± 10.0

1.6 ± 0.4

0.63

HII GAL320.23−00.29. Several DNe.

G322.15+00.61^a .....

36 ± 56

3.9 ± 1.1

18.7 ± 1.1

1.92 ± 0.26

33 ± 56

16.0 ± 6.5

2.5

32.5 ± 4.2

0.26

1.5 ± 0.6

13 ± 10

3.5 ± 3.1

0.09

RCW92

G327.30−00.50^a .....

1.3 ± 0.8

2882 ± 212

18.1 ± 7.5

20.2 ± 1.7

2.08 ± 0.17

190 ± 127

46 ± 19

2.4

29.3 ± 1.2

0.68

2.3 ± 1.2

40 ± 23

1.1 ± 0.7

0.32

HII GAL327.30−00.60. Several DNe

G336.90+00.00^a .....

1.5 ± 0.5

4543 ± 308

29.6 ± 2.8

22.7 ± 0.5

1.82 ± 0.06

−91 ± 182

79 ± 27

2.9

27.6 ± 0.5

1.01

4.8 ± 0.7

67 ± 33

0.7 ± 0.3

0.14

Kes39. Weak SNR G337.0−00.1; 1.5 Jy @ 1 GHz

G343.48−00.04^a .....

1491 ± 177

35.4 ± 11.5

18.6 ± 1.2

1.94 ± 0.11

61 ± 117

54 ± 16

3.4

24.9 ± 3.3

0.55

1.4 ± 0.6

43 ± 21

1.3 ± 0.7

0.29

HII GAL343.4−00.0. Several DNe.

G344.75+23.97 ^b .....

12.1 ± 0.8

0.3 ± 0.0

20.3 ± 0.4

1.86 ± 0.07

−7 ± 2

1.4 ± 0.2

6.0

26.9 ± 1.2

0.00

2.4 ± 0.3

1.2 ± 0.3

2.1 ± 0.6

1.45

MBM 121/122. Synch.

G345.40−00.94^a .....

66 ± 113

5.7 ± 3.8

19.3 ± 2.8

2.38 ± 0.49

221 ± 110

48 ± 10

4.6

33.2 ± 4.8

0.86

1.8 ± 1.6

43 ± 17

3.9 ± 2.1

0.24

RCW117

G348.73−00.75^a .....

0.7 ± 0.5

1956 ± 176

4.2 ± 1.1

22.9 ± 2.1

2.08 ± 0.41

−24 ± 122

10 ± 15

0.7

...

5.0 ± 2.8

7 ± 19

0.4 ± 1.0

0.11

RCW122

G351.29+00.68^a .....

0.5 ± 0.2

3071 ± 239

13.1 ± 1.8

22.3 ± 0.7

2.04 ± 0.12

290 ± 169

25 ± 23

1.1

...

4.3 ± 0.9

17 ± 30

0.3 ± 0.6

0.18

Extension to the west of AME-G353.05+16.90

G351.31+17.28 ^a .....

161 ± 12

0.9 ± 0.4

25.4 ± 2.6

1.69 ± 0.15

4 ± 13

7.5 ± 1.4

5.3

28.5 ± 0.4

0.01

9.4 ± 5.7

6.5 ± 2.2

1.1 ± 0.4

0.24

HII LBN1105/1104. Several DNe

G351.65−01.23^a .....

1.8 ± 1.7

443 ± 222

11.8 ± 4.2

19.7 ± 1.4

2.20 ± 0.26

291 ± 150

49 ± 24

2.1

28.5 ± 0.4

1.38

2.0 ± 0.9

41 ± 31

1.9 ± 1.5

0.05

Kes52

G353.05+16.90 ^bc .....

0.9 ± 0.5

11 ± 2

6.5 ± 1.0

21.0 ± 0.7

1.78 ± 0.05

121 ± 13

22.2 ± 0.7

29.8

30.5 ± 2.3

0.23

3.0 ± 0.6

20.0 ± 1.9

1.5 ± 0.2

0.80

ρ Ophiuchi AME-G353.05+16.90¹ .....

G353.16+00.74^a .....

0.4 ± 0.1

5725 ± 307

16.4 ± 5.2

21.7 ± 1.5

2.13 ± 0.12

576 ± 155

85 ± 26

3.2

32.5 ± 4.1

0.28

3.6 ± 1.5

71 ± 31

1.2 ± 0.6

0.40

HII GAL353.19+0.67. HII NGC 6357

G353.97+15.79 ^a .....

31 ± 6

4.7 ± 1.5

18.7 ± 1.2

1.69 ± 0.10

−23 ± 9

10.8 ± 1.0

10.9

26.6 ± 1.5

0.11

1.5 ± 0.6

9.0 ± 2.9

2.3 ± 0.8

0.72

In Ophiuchus

G355.44+00.11^a .....

1.9 ± 0.6

1444 ± 478

41.6 ± 13.1

18.3 ± 1.1

2.12 ± 0.12

338 ± 198

69 ± 23

2.9

26.1 ± 2.0

0.22

1.3 ± 0.5

56 ± 39

1.4 ± 1.0

0.25

Synch. SNR G355.6−0.0; 3 Jy @ 1 GHz

G355.63+20.52 ^a .....

1.7 ± 0.8

12 ± 2

2.2 ± 0.2

16.1 ± 0.3

2.01 ± 0.10

60 ± 6

7.1 ± 0.5

13.3

26.9 ± 1.2

0.00

0.61 ± 0.06

5.9 ± 0.7

9.0 ± 1.8

1.70

In Ophiuchus

Notes. The detection method used for each source is indicated by the superscript letter after the name. Fitted parameters are based on the aperture photometry (see Sect. 3.4). Regions that show significant (>5σ) AME have boldface names, except for those with a high potential UCH ii contribution (). Values for ν_sp and are only given if σ_AME > 2. In four cases, A_sp was fixed at zero (see Sect. 3.5), these are marked with a dagger. Note that EM_ff is an effective emission measure integrated over the aperture.

^(a)

Detected in bandmerged catalogue.

^(b)

Detected in component subtracted map.

^(c)

Previously known source from the literature.

Reference.

⁽¹⁾

Planck Collaboration XX (2011);

⁽²⁾

Génova-Santos et al. (2011);

⁽³⁾

Finkbeiner et al. (2002); Dickinson et al. (2006);

⁽⁴⁾

Dickinson et al. (2007).

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