Table 6: Source luminosities calculated from the integrated "normal-galaxy'' spectrum (Lagache Lum.), Stickel's formula (Stickel Lum.) and the best fit Dale spectrum (Dale Lum.) with its $\alpha$ value. The H $\alpha$ luminosities, uncorrected for extinction (hence the ">'' sign in the corresponding SFR), are also given. The K luminosity is directly derived from the K magnitude. The "q'' parameter is the logarithmic ratio of IR to radio flux, following Helou et al. (1985).
ID z Lagache Lum. Stickel L. Dale L. (and $\alpha$ ) H $\alpha$ L. K Lum. SFR(IR) SFR(H $\alpha$ ) q

( $10^{10}~L_{\odot}$ ) ( $10^{10}~L_{\odot}$ ) ( $10^{10} L_{\odot}$ ) ( $10^{6}~L_{\odot}$ ) ( $10^{9}~L_{\odot}$ ) $M_{\odot}/$ yr^-1 $10^{-2}~M_{\odot}~$ yr^-1

0 0.145 52.3 73.0 95.3 (1.69) 222 5.87 68 >675 2.30

1 0.030 1.5 1.3 1.8 (1.83) 4.9 0.70 1.9 >15 2.69

2 0.063 6.4 4.6 6.1 (2.07) 3.2 2.32 8.3 >9.7 2.60

3 0.063 4.9 5.2 2.54 6.4 >16

4 0.063 4.6 3.4 5.2 (2.52) 2.2 4.97 6.0 >6.7 2.32

5 0.288 100.8 70.5 113.6 (2.35) 131

6 0.073 5.6 4.4 7.2 (2.52) 11.3 2.80 7.3 >34

7 0.063 3.6 3.8 12.8 2.14 4.7 >39 2.35

9 0.053 2.4 2.8 3.14 3.1 >8.5

11 0.063 3.6 3.0 1.39 4.7 >9.1

12 0.063 3.8 8.2 0.93 4.9 >25 2.66

14 0.07 4.1 4.8 7.9 (2.25) 5.3

15 0.23 48.6 4.23 63

16 0.090 6.8 8.5 13.3 (2.13) 23.6 3.02 8.8 >72 2.22

18 0.067 6.0 3.3 2.22 7.8 >10

20 0.01 0.1 0.13

21 0.064 3.2 3.6 1.61 4.1 >11

23 0.063 3.1 5.9 0.89 4.0 >18

24 0.086 5.7 8.5 1.89 7.4 >26

26 0.077 4.3 1.7 1.28 5.6 >5.2

31 0.063 2.6 1.9 1.15 3.4 >5.8

33 0.133 12.4 16.1

35 0.137 11.9 32.5 5.30 15.5 >99

38 0.107 6.9 6.7 9.0 >20

39 0.269 47.6 2.23 62

40^a 0.45 122.9 0.17 160 2000

41 0.12 8.6 1.22 11.1

43 0.21 27.5 21.1 7.23 36 >64

49 0.127 9.8 3.39 12.7

^a Data from Chapman et al. (2002), main component, reddening corrected H $\beta$ luminosity.

**Table 6:** Source luminosities calculated from the integrated "normal-galaxy'' spectrum (Lagache Lum.), Stickel's formula (Stickel Lum.) and the best fit Dale spectrum (Dale Lum.) with its $\alpha$ value. The H $\alpha$ luminosities, uncorrected for extinction (hence the ">'' sign in the corresponding SFR), are also given. The K luminosity is directly derived from the K magnitude. The "q'' parameter is the logarithmic ratio of IR to radio flux, following Helou et al. (1985).
ID	z	Lagache Lum.	Stickel L.	Dale L. (and $\alpha$ )	H $\alpha$ L.	K Lum.	SFR(IR)	SFR(H $\alpha$ )	q
		( $10^{10}~L_{\odot}$ )	( $10^{10}~L_{\odot}$ )	( $10^{10} L_{\odot}$ )	( $10^{6}~L_{\odot}$ )	( $10^{9}~L_{\odot}$ )	$M_{\odot}/$ yr^-1	$10^{-2}~M_{\odot}~$ yr^-1
0	0.145	52.3	73.0	95.3 (1.69)	222	5.87	68	>675	2.30
1	0.030	1.5	1.3	1.8 (1.83)	4.9	0.70	1.9	>15	2.69
2	0.063	6.4	4.6	6.1 (2.07)	3.2	2.32	8.3	>9.7	2.60
3	0.063	4.9			5.2	2.54	6.4	>16
4	0.063	4.6	3.4	5.2 (2.52)	2.2	4.97	6.0	>6.7	2.32
5	0.288	100.8	70.5	113.6 (2.35)			131
6	0.073	5.6	4.4	7.2 (2.52)	11.3	2.80	7.3	>34
7	0.063	3.6	3.8		12.8	2.14	4.7	>39	2.35
9	0.053	2.4			2.8	3.14	3.1	>8.5
11	0.063	3.6			3.0	1.39	4.7	>9.1
12	0.063	3.8			8.2	0.93	4.9	>25	2.66
14	0.07	4.1	4.8	7.9 (2.25)			5.3
15	0.23	48.6				4.23	63
16	0.090	6.8	8.5	13.3 (2.13)	23.6	3.02	8.8	>72	2.22
18	0.067	6.0			3.3	2.22	7.8	>10
20	0.01	0.1					0.13
21	0.064	3.2			3.6	1.61	4.1	>11
23	0.063	3.1			5.9	0.89	4.0	>18
24	0.086	5.7			8.5	1.89	7.4	>26
26	0.077	4.3			1.7	1.28	5.6	>5.2
31	0.063	2.6			1.9	1.15	3.4	>5.8
33	0.133	12.4					16.1
35	0.137	11.9			32.5	5.30	15.5	>99
38	0.107	6.9			6.7		9.0	>20
39	0.269	47.6				2.23	62
40^a	0.45	122.9				0.17	160	2000
41	0.12	8.6				1.22	11.1
43	0.21	27.5			21.1	7.23	36	>64
49	0.127	9.8				3.39	12.7

Source LaTeX | All tables | In the text

	1 Introduction
	2 Complementary observations
	3 Identifications: method and results
	4 Optical properties of identified sources
	5 Mid and far-IR properties
	6 The radio-FIR relation
	7 Star formation rates
	8 Discussion and conclusions
	References
	Online Material