Table 4: The list of 7 $\mu$ m sources with source flux exceeding 5 $\sigma$ of the local noise, and having 15 $\mu$ m counterparts. From left to right: 15 $\mu$ m source identification number as listed in Table 2; signal and precision of flux in ADU; flux and precision in mJy; Right Ascension, Declination; nature of the source; and finally the [7 $\mu$ m]/[15 $\mu$ m] colour ratio.
Source ID Signal Precision Flux Precision RA Dec Notes [7 $\mu$ m]/[15 $\mu$ m]

(ADU) ( $\pm$ ADU) (mJy) ( $\pm$ mJy) (J2000) (J2000)

03 1.461 0.219 1.685 0.253 00 26 27.0 +17 09 08.2 Star 5.7

14 1.276 0.191 1.468 0.220 00 26 36.5 +17 07 41.0 Star 4.2

29 3.806 0.571 4.427 0.664 00 26 47.9 +17 08 11.1 Star 3.7

**Table 4:** The list of 7 $\mu$ m sources with source flux exceeding 5 $\sigma$ of the local noise, and having 15 $\mu$ m counterparts. From left to right: 15 $\mu$ m source identification number as listed in Table 2; signal and precision of flux in ADU; flux and precision in mJy; Right Ascension, Declination; nature of the source; and finally the [7 $\mu$ m]/[15 $\mu$ m] colour ratio.
Source ID	Signal	Precision	Flux	Precision	RA	Dec	Notes	[7 $\mu$ m]/[15 $\mu$ m]
	(ADU)	( $\pm$ ADU)	(mJy)	( $\pm$ mJy)	(J2000)	(J2000)
03	1.461	0.219	1.685	0.253	00 26 27.0	+17 09 08.2	Star	5.7
14	1.276	0.191	1.468	0.220	00 26 36.5	+17 07 41.0	Star	4.2
29	3.806	0.571	4.427	0.664	00 26 47.9	+17 08 11.1	Star	3.7

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