Table 2: The primary list of sources detected at 15 $\mu $m. The columns are (from left to right): source identification number in order of increasing Right Ascension; source flux and precision before calibration (in ADUgs); source flux and precision after calibration (in mJy); Right Ascension and Declination of the infrared source (J2000); redshift and name of the optical counterpart, if known. The redshift of source ISO_Cl0024_02 was taken from Schmidt et al. (1986). All other redshifts are from Czoske et al. (2001) or provided by T. Treu (private communication). The names of the stars are from HEASARC.

Source ID		 Signal Precision Flux Precision RA Dec z Name of optical
ISO_Cl0024 (ADU) ($\pm$ADU) (mJy) ($\pm$mJy) (J2000) (J2000) if known counterpart if known

01		 0.634 0.090 0.786 0.120 00 26 24.3 +17 08 18.0 Star TYC 1180-82-1
02 0.472 0.060 0.577 0.090 00 26 26.3 +17 09 39.0 0.959 PC 0023+1653
03 0.256 0.060 0.298 0.080 00 26 27.0 +17 09 11.7 Star N3231320329
04 0.298 0.060 0.352 0.080 00 26 30.8 +17 09 44.8 -  
05 0.184 0.060 0.205 0.080 00 26 30.7 +17 09 03.5 0.3935  
06 0.230 0.060 0.264 0.080 00 26 30.9 +17 10 29.4 -  
07 0.217 0.060 0.247 0.080 00 26 31.0 +17 09 37.4 -  
08 0.610 0.090 0.755 0.120 00 26 31.0 +17 10 15.6 0.4005  
09 0.286 0.060 0.336 0.080 00 26 31.5 +17 10 21.4 0.2132  
10 0.191 0.060 0.214 0.080 00 26 31.8 +17 10 03.5 0.4000  
11 0.220 0.060 0.251 0.080 00 26 35.5 +17 09 59.1 0.5558  
12 0.182 0.060 0.202 0.080 00 26 35.9 +17 10 36.4 0.3860  
13 0.210 0.060 0.238 0.080 00 26 35.9 +17 11 39.9 -  
14 0.293 0.060 0.346 0.080 00 26 36.6 +17 07 44.4 Star EO903-0219757
15 0.170 0.060 0.186 0.080 00 26 36.6 +17 10 25.4 -  
16 0.260 0.060 0.302 0.080 00 26 37.7 +17 11 33.4 -  
17 0.253 0.060 0.293 0.080 00 26 38.9 +17 08 03.9 -  
18 0.634 0.090 0.786 0.120 00 26 40.4 +17 09 28.7 0.394  
19 0.187 0.060 0.208 0.080 00 26 40.6 +17 11 44.9 -  
20 0.262 0.060 0.305 0.080 00 26 40.7 +17 09 54.0 0.7125  
21 0.191 0.060 0.213 0.080 00 26 41.3 +17 11 01.4 0.3924  
22 0.334 0.060 0.398 0.080 00 26 41.8 +17 09 52.9 0.3935  
23 0.282 0.060 0.331 0.080 00 26 42.7 +17 09 41.6 -  
24 0.189 0.060 0.211 0.080 00 26 42.8 +17 08 48.5 0.3954  
25 0.200 0.060 0.225 0.080 00 26 42.9 +17 08 31.7 0.9174  
26 0.324 0.060 0.385 0.080 00 26 43.1 +17 08 25.1 0.3961  
27 0.373 0.060 0.449 0.080 00 26 43.2 +17 09 11.7 0.3932  
28 0.120 0.060 0.122 0.080 00 26 45.5 +17 08 30.8 -  
29 0.946 0.110 1.191 0.140 00 26 47.9 +17 08 12.0 Star EO903-0219375
30 0.489 0.070 0.598 0.090 00 26 48.0 +17 09 15.7 -  

Source LaTeX | All tables | In the text

Article Contents
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
List of tables
List of figures