Exploring the physical properties of local star-forming ULIRGs from the ultraviolet to the infrared

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Volume 523 (November-December 2010)

A&A, 523 (2010) A78

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Table A.3

Photometric data – mid-infrared to far-infrared. All fluxes are in Jy.

Galaxy

12 μm

25 μm

60 μm

100 μm

15 μm

24 μm

70 μm

160 μm

350 μm

450 μm

850 μm

IRAS 00199-7426

0.0963

6.59E-2^a

3.26E-1^a

4.16E0^a

6.42E0^a

9.00E-2^b

–

IRAS 01494-1845

0.1579

1.72E-2^a

7.58E-2^a

1.29E0^a

1.85E0^a

2.10E-2^b

6.67E-2^b

–

IRAS Z02376-0054

0.4097

1.85E-3^b

4.76E-3^b

2.00E-1^c

6.90E-1^c

1.34E-2^b

4.38E-3^b

–

6.65E-2^c

–

IRAS 04114-5117

0.1245

1.32E-2^a

7.40E-2^a

2.09E0^a

3.23E0^a

1.72E-2^b

7.14E-2^b

2.77E0^d

1.65E0^d

–

IRAS 06009-7716

0.1169

2.75E-2^a

1.18E-1^a

1.42E0^a

2.11E0^a

3.48E-2^b

9.54E-2^b

1.63E0^d

8.46E-1^d

–

IRAS F08208+3211

0.3957

1.76E-3^b

5.50E-3^b

2.27E-1^a

5.20E-1^c

1.49E-3^b

4.98E-3^b

–

3.62E-1^d

7.60E-2^c

–

IRAS F10156+3705

0.4897

1.62E-3^b

3.34E-3^b

2.06E-1^a

4.71E-1^a

1.49E-3^b

2.96E-3^b

–

3.66E-1^d

7.86E-2^c

–

IRAS 10565+2448

0.0431

2.00E-1^e

1.27E0^e

1.21E1^e

1.50E1^e

2.99E-1^b

9.86E-1^d

9.59E0^d

6.66E0^d

1.24E0^c

–

6.10E-2^f

IRAS 12112+0305

0.0726

5.93E-2^b

4.68E-1^b

8.18E0^e

9.46E0^e

9.30E-2^b

3.50E-1^b

–

2.81E-1^g

4.90E-2^f

IRAS 13120-5453

0.0307

4.40E-1^e

2.98E0^e

4.11E1^e

5.23E1^e

6.42E-1^b

2.70E0^b

3.13E1^d

–

IRAS 16334+4630

0.1909

1.58E-2^b

7.99E-2^b

1.19E0^a

2.09E0^a

2.10E-2^b

6.90E-2^b

1.57E0^d

9.40E-1^d

–

IRAS 17208-0014

0.043

1.78E-1^b

1.61E0^e

3.21E1^e

3.61E1^e

2.55E-1^b

1.21E0^d

1.91E1^d

–

1.07E0^h

1.55E-1^h

IRAS 19297-0406

0.0857

6.02E-2^b

5.17E-1^b

7.32E0^e

8.62E0^e

9.87E-2^b

3.93E-1^d

6.64E0^d

4.47E0^d

–

IRAS 19458+0944

0.0999

3.73E-2^b

2.53E-1^b

3.95E0ⁱ

7.11E0ⁱ

5.46E-2^b

1.70E-1^d

3.32E0^d

–

IRAS 20414-1651

0.087

2.51E-2^b

2.64E-1^b

4.36E0^a

5.25E0^a

3.89E-2^b

2.20E-1^b

–

IRAS 22491-1808

0.0772

4.37E-2^b

5.40E-1^e

5.54E0^e

4.64E0^e

7.90E-2^b

4.09E-1^d

4.68E0^d

2.04E0^d

–

1.90E-2^h

Notes.

^(a)

– IRAS FSC (Moshir & et al. 1990);

^(b)

– Computed from IRS spectrum;

^(c)

– Yang et al. (2007);

^(d)

– Computed using post-BCD products provided by the Spitzer Science Center, as described in Marshall et al. (2007);

^(e)

– Sanders et al. (2003);

^(f)

– Dunne et al. (2000);

^(g)

– Rigopoulou et al. (1996);

^(h)

– Klaas et al. (2001);

⁽ⁱ⁾

– IRAS PSC. Extra ISO photometry: IRAS 00199-7426 – F_ν(10 μm) = 5.70E − 1, F_ν(120 μm) = 7.50E0, F_ν(150 μm) = 5.34E0, F_ν(180 μm) = 4.21E0, F_ν(200 μm) = 3.00E0 (Klaas et al. 2001); IRAS 01494-1845 – F_ν(170 μm) = 1.49E0 (Stickel et al. 2004); IRAS 13120-5453 – F_ν(170 μm) = 3.05E1 (Stickel et al. 2004).

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