Table 6: Results from model SEDs for known cluster galaxies in Cl 0024+1654. The columns list: LW3 identification number; best-fit SED model; number of data points in the observed SED; $\chi ^2$ of the fit; rejection probability of the fit; other acceptable models (rejection probability 95% or less); 15 $\mu$ m k-correction; luminosity at 15 $\mu$ m (h=0.7, $\Omega _{\rm m}=0.3$ , $\Omega _l=0.7$ ) using the transformation from Boselli et al. (1998), and k-corrected using best-fit SED; total infrared luminosity including the k-correction using the best-fit SED and computed using the transformation from Elbaz et al. (2002); SFR from total IR luminosity using the transformation of Kennicutt (1998); position in the V-I vs. I colour-magnitude diagram (Fig. 7) where "MS'' stands for "Main Sequence'', "BO'' for "Butcher-Oemler'', "U'' for "Unknown''; EW [O II] line from Czoske et al. (2001); SFR computed from the [O II] emission line using the transformation to the optical SFR; ratio infrared to optical SFR.
id. Best-fit $\sharp$ of $\chi ^2$ Rejection Other SED k-corr. $L_{15~\mu {\rm m}}$ $L_{\rm IR}$ SFR[IR] Colour EW[O II] SFR[O II] SFR[IR]/

model data points Probability models ( ${L}_\odot$ ) ( ${L}_\odot$ ) ( ${M}_\odot$ yr^-1) Fig. 8 (Å) ( ${M}_\odot$ yr^-1) SFR[O II]

05 S 12 17.8 96.2 None 1.45 2.03e+09 9.56e+10 16 U - - -

08 SB+1 15 23.4 97.6 None 1.80 9.66e+09 4.54e+11 77 BO - - -

10 S 4 1.9 79.8 S, SB+1 1.46 2.21e+09 1.04e+11 18 BO - - -

18 S 11 3.9 13.4 E, S, SB+1 1.46 7.85e+09 3.69e+11 63 BO - - -

21 S 7 5.4 74.7 SB+1, S 1.46 2.11e+09 9.93e+10 17 BO - - -

22 S 11 7.6 52.6 S, SB+1 1.46 3.96e+09 1.87e+11 32 BO 17.5 4.9 6.5

24 S 4 1.2 79.8 E, SB+1, S 1.42 2.07e+09 9.74e+10 17 MS 5.0 0.8 21.3

26 S 4 1.4 79.8 S, SB+1 1.73 4.51e+09 2.17e+11 36 - - - -

27 SB+1 8 6.7 87.8 SB 1.80 5.50e+09 2.59e+11 44 MS - - -

1s S 10 8.6 71.4 E, E, S, SB+1 1.73 1.96e+09 9.23e+10 16 BO 9.6 1.0 16.0

3s SB+1 4 1.3 79.8 S, SB+1, E 1.80 1.59e+09 7.48e+10 13 MS - - -

4s E 20 9.4 7.3 E, S, SB+1 0.78 9.87e+08 4.66e+10 8 MS - - -

**Table 6:** Results from model SEDs for known cluster galaxies in Cl 0024+1654. The columns list: LW3 identification number; best-fit SED model; number of data points in the observed SED; $\chi ^2$ of the fit; rejection probability of the fit; other acceptable models (rejection probability 95% or less); 15 $\mu$ m k-correction; luminosity at 15 $\mu$ m (h=0.7, $\Omega _{\rm m}=0.3$ , $\Omega _l=0.7$ ) using the transformation from Boselli et al. (1998), and k-corrected using best-fit SED; total infrared luminosity including the k-correction using the best-fit SED and computed using the transformation from Elbaz et al. (2002); SFR from total IR luminosity using the transformation of Kennicutt (1998); position in the V-I vs. I colour-magnitude diagram (Fig. 7) where "MS'' stands for "Main Sequence'', "BO'' for "Butcher-Oemler'', "U'' for "Unknown''; EW [O II] line from Czoske et al. (2001); SFR computed from the [O II] emission line using the transformation to the optical SFR; ratio infrared to optical SFR.
id.	Best-fit	$\sharp$ of	$\chi ^2$	Rejection	Other SED	k-corr.	$L_{15~\mu {\rm m}}$	$L_{\rm IR}$	SFR[IR]	Colour	EW[O II]	SFR[O II]	SFR[IR]/
	model	data points		Probability	models		( ${L}_\odot$ )	( ${L}_\odot$ )	( ${M}_\odot$ yr^-1)	Fig. 8	(Å)	( ${M}_\odot$ yr^-1)	SFR[O II]
05	S	12	17.8	96.2	None	1.45	2.03e+09	9.56e+10	16	U	-	-	-
08	SB+1	15	23.4	97.6	None	1.80	9.66e+09	4.54e+11	77	BO	-	-	-
10	S	4	1.9	79.8	S, SB+1	1.46	2.21e+09	1.04e+11	18	BO	-	-	-
18	S	11	3.9	13.4	E, S, SB+1	1.46	7.85e+09	3.69e+11	63	BO	-	-	-
21	S	7	5.4	74.7	SB+1, S	1.46	2.11e+09	9.93e+10	17	BO	-	-	-
22	S	11	7.6	52.6	S, SB+1	1.46	3.96e+09	1.87e+11	32	BO	17.5	4.9	6.5
24	S	4	1.2	79.8	E, SB+1, S	1.42	2.07e+09	9.74e+10	17	MS	5.0	0.8	21.3
26	S	4	1.4	79.8	S, SB+1	1.73	4.51e+09	2.17e+11	36	-	-	-	-
27	SB+1	8	6.7	87.8	SB	1.80	5.50e+09	2.59e+11	44	MS	-	-	-
1s	S	10	8.6	71.4	E, E, S, SB+1	1.73	1.96e+09	9.23e+10	16	BO	9.6	1.0	16.0
3s	SB+1	4	1.3	79.8	S, SB+1, E	1.80	1.59e+09	7.48e+10	13	MS	-	-	-
4s	E	20	9.4	7.3	E, S, SB+1	0.78	9.87e+08	4.66e+10	8	MS	-	-	-

Source LaTeX | All tables | In the text

	1 Introduction
	2 The cluster
	3 Observations, data reduction and source detection
	4 Results
	5 Spatial, dynamical and colour properties of the 15 $\mu$ m cluster galaxies
	6 Comparison of Cl 0024+1654 with other clusters observed by ISO
	7 Conclusions
	Appendix A: Additional notes on some mid-infrared sources
	References