Table 3: Catalog of the deep ISOCAM-detected sources in CFRS fields 1300+00 and 1415+52.
                B450 V606 I814      
CFRS ID z m450 m606 m814 $M_{\rm AB}$(B) $M_{\rm AB}$(K) $L_{\rm IR}(10^{10}~L_\odot$) B/T $\chi^2$ B/T $\chi^2$ B/T $\chi^2$ Typea Qb Int/Mc
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15) (16) (17)
No redshift identification
03.0028 - - 21.16 19.30 - - - - - $\rm0.71_{-0.02}^{+0.01}$ 1.078 $\rm0.73_{-0.01}^{+0.01}$ 1.047      
03.0115 - - 21.15 19.53 - - - - - $\rm0.13_{-0.01}^{+0.01}$ 1.588 $\rm0.22_{-0.01}^{+0.01}$ 1.474      
03.0121 - - 21.40 19.76 - - - - - $\rm0.20_{-0.07}^{+0.02}$ 1.947 $\rm0.18_{-0.02}^{+0.01}$ 1.413      
03.0346 - 23.77 - 21.52 - - - $\rm0.72_{-0.06}^{+0.10}$ 1.089 - - $\rm0.43_{-0.01}^{+0.01}$ 2.375      
14.0324 - - 22.85 21.47 - - -   - $\rm0.27_{-0.05}^{+0.13}$ 1.0156 $\rm0.38_{-0.05}^{+0.05}$ 1.0075      
14.0405 - - 22.26 20.38 - - -   - $\rm0.36_{-0.04}^{+0.06}$ 1.0004 $\rm0.19_{-0.02}^{+0.02}$ 1.0183      
$z \leq 0.4$
03.0355 0.0870 19.06 - 16.91 -19.31 - 1.52 $\pm$ 0.32 $\rm0.34^{-0.02}_{+0.02}$ 1.183 - - $\rm0.70^{-0.01}_{+0.00}$ 1.383      
03.0364 0.2513 20.97 - 18.95 -20.30 -22.14 4.56 $\pm$ 0.81 $\rm0.00^{-0.00}_{+0.01}$ 1.520 - - $\rm0.03^{-0.00}_{+0.00}$ 1.787      
03.0365 0.2187 21.10 - 18.89 -19.57 -21.68 4.26 $\pm$ 0.87 $\rm0.18^{-0.02}_{+0.02}$ 1.374 - - $\rm0.00^{-0.00}_{+0.00}$ 1.420      
03.0443 0.1178 20.37 - 19.12 -19.15 - 0.78 $\pm$ 0.16 $\rm0.72^{-0.07}_{+0.05}$ 0.952 - - $\rm0.70^{-0.02}_{+0.02}$ 1.093      
03.0495 0.2614 - 20.38 19.25 -19.82 - 5.38 $\pm$ 1.22 - - $\rm0.32^{-0.01}_{+0.01}$ 2.174 $\rm0.40^{-0.06}_{+0.07}$ 1.906      
03.0569 0.1810 - 22.41 21.27 -16.73 -20.01 1.67 $\pm$ 0.37 - - - - - -      
03.0578 0.2200 - 21.59 20.93 -18.64 -19.52 1.58 $\pm$ 0.36 - - $\rm0.13^{-0.01}_{+0.02}$ 1.084 $\rm0.21^{-0.05}_{+0.05}$ 0.989      
03.0711 0.2620 - 21.34 20.51 -18.55 -20.44 2.51 $\pm$ 0.58 - - $\rm0.00^{-0.00}_{+0.00}$ 1.298 $\rm0.00^{-0.00}_{+0.00}$ 1.136      
03.0949 0.0330 19.40 - 17.56 -16.86 - 0.18 $\pm$ 0.02 $\rm0.24^{-0.08}_{+0.03}$ 0.897 - - $\rm0.13^{-0.07}_{+0.12}$ 1.225      
03.1299 0.1760 - 19.66 18.76 -19.94 - 5.02 $\pm$ 1.23 - - $\rm0.13^{-0.02}_{+0.02}$ 3.688 $\rm0.10^{-0.01}_{+0.07}$ 1.005      
03.1311 0.1760 - 20.30 19.36 -18.86 -21.69 2.09 $\pm$ 0.49 - - $\rm0.00^{-0.00}_{+0.00}$ 1.562 $\rm0.04^{-0.01}_{+0.01}$ 1.327      
14.0435 0.0684 - 18.71 17.91 -18.30 - 0.14 $\pm$ 0.02 - - $\rm0.00^{-0.00}_{+0.00}$ 1.481 $\rm0.00^{-0.00}_{+0.00}$ 1.395      
14.1257 0.2927 - 21.24 20.16 -19.44 -22.45 15.97 $\pm$ 2.15 - - $\rm0.00^{-0.00}_{+0.00}$ 1.859 $\rm0.00^{-0.00}_{+0.00}$ 1.490      
14.1329 0.3750 - 20.21 19.19 -21.00 - 13.03 $\pm$ 2.47 - - $\rm0.43^{-0.01}_{+0.02}$ 1.976 $\rm0.48^{-0.02}_{+0.01}$ 1.816      
14.9025 0.1550 - 19.57 18.69 -19.77 - 1.69 $\pm$ 0.39 - - $\rm0.00^{-0.00}_{+0.00}$ 3.280 $\rm0.07^{-0.00}_{+0.00}$ 2.186      
0.4 < z < 1.2
03.0035 0.8804 24.06 22.69 21.12 -21.87 -23.70 171.47 $\pm$ 23.41 - - $\rm0.28^{-0.08}_{+0.06}$ 1.349 $\rm0.31^{-0.06}_{+0.04}$ 0.993 Sab (3.6) 2 R?
03.0062 0.8252 - 22.26 20.90 -21.84 -23.00 111.73 $\pm$ 13.74 - - $\rm0.00^{-0.00}_{+0.00}$ 1.545 $\rm0.01^{-0.01}_{+0.01}$ 1.439 Sbc (3.0) 1  
03.0085 0.6100 - 22.58 21.51 -19.98 -21.09 29.55 $\pm$ 2.67 - - $\rm0.00^{-0.00}_{+0.01}$ 1.274 - - Sd (5.1) 2  
03.0445 0.5300 22.84 - 20.40 -21.25 - 21.28$\pm$4.27 $\rm 1.00^{-0.03}_{+0.00}$ 0.992 - - $\rm0.01^{-0.00}_{+0.00}$ 1.038 Sbc (3.9) 2 R?
03.0507 0.4660 - 21.33 20.48 -20.47 -21.23 11.57 $\pm$ 2.71 - - $\rm0.07^{-0.01}_{+0.12}$ 1.325 $\rm0.24^{-0.04}_{+0.08}$ 1.227 Sab (3.2) 2  
03.0523 0.6508 23.03 22.00 20.99 -20.93 -21.73 68.65 $\pm$ 4.36 $\rm0.34^{-0.29}_{+0.55}$ 0.931 $\rm0.53^{-0.03}_{+0.04}$ 1.789 $\rm0.42^{-0.05}_{+0.05}$ 1.292 C/T 1 M 2
03.0533 0.8290 - 22.30 21.02 -21.38 -22.28 170.04 $\pm$ 23.67 - - $\rm0.00^{-0.00}_{+0.00}$ 1.096 $\rm0.00^{-0.00}_{+0.00}$ 1.170 Irr 1 R
03.0570 0.6480 - 22.67 21.69 -20.12 -20.58 29.97 $\pm$ 2.75 - - $\rm0.03^{-0.03}_{+0.05}$ 1.242 $\rm0.42^{-0.08}_{+0.06}$ 1.111 C 1  
03.0603 1.0480 - 21.26 20.37 -23.01 -23.71 435.58 $\pm$ 83.86 - - $\rm0.43^{-0.01}_{+0.01}$ 1.464 $\rm0.73^{-0.01}_{+0.01}$ 1.290 C 1 R
03.0615 1.0480 - 22.52 21.51 -21.66 -22.77 344.69 $\pm$ 62.39 - - $\rm0.35^{-0.03}_{+0.04}$ 1.390 $\rm0.33^{-0.03}_{+0.02}$ 1.306 C 3  
03.0776 0.8830 - 23.28 22.05 -20.69 -20.98 107.84 $\pm$ 14.25 - - $\rm0.00^{-0.00}_{+0.08}$ 0.992 $\rm0.04^{-0.04}_{+0.09}$ 1.061 C 1  
03.0916d 1.0300 22.64 - 21.17 -22.23 - 503.26 $\pm$ 68.64 - - - - - - C 1  
03.0932 0.6478 23.54 - 21.18 -20.73 -22.85 97.18 $\pm$ 6.95 - - - - $\rm0.00^{-0.00}_{+0.01}$ 1.046 Sbc (7.0) 1  
03.1309 0.6170 - 21.65 20.77 -21.49 -23.00 89.28 $\pm$ 6.32 - - - - - -   4 M 1
03.1349 0.6155 - 21.67 20.38 -21.15 -22.63 56.77 $\pm$ 3.38 - - $\rm0.28^{-0.01}_{+0.01}$ 1.179 $\rm0.39^{-0.09}_{+0.08}$ 0.873 Sab (4.5) 1 I2
03.1522 0.5870 25.73 - 21.74 -19.59 -21.96 46.13 $\pm$ 3.02 - - - - $\rm0.22^{-0.16}_{+0.28}$ 0.994 S (9.0) 1  
03.1540 0.6898 22.95 - 20.61 -21.27 - 90.23 $\pm$ 9.19 $\rm0.64^{-0.64}_{+0.36}$ 0.932 - - $\rm0.52^{-0.04}_{+0.06}$ 1.223 C 1 R?
03.9003 0.6189 22.58 - 20.47 -21.24 - 54.74 $\pm$ 3.73 $\rm0.13^{-0.02}_{+0.04}$ 1.863 - - $\rm0.00^{-0.00}_{+0.00}$ 2.017 Irr 1 M 2
14.0302 0.5830 22.78 - 20.44 -20.98 -22.70 56.94 $\pm$ 3.17 $\rm0.28^{-0.18}_{+0.16}$ 1.005 - - $\rm0.22^{-0.03}_{+0.04}$ 1.069 Sab (3.0) 2 R?
14.0393 0.6016 23.07 - 20.94 -21.64 -22.30 55.15 $\pm$ 3.57 - - - - $\rm0.04^{-0.01}_{+0.01}$ 1.157 Sbc (3.6) 1  
14.0446 0.6030 - 21.15 19.88 -21.95 - 56.87 $\pm$ 3.29 - - $\rm0.00^{-0.00}_{+0.00}$ 1.243 $\rm0.00^{-0.00}_{+0.00}$ 1.363 Sd (6.8) 1  
14.0547 1.1963 - 22.02 21.17 -23.12 -23.88 186.03 $\pm$ 43.71 - - - - - -   4 M 1
14.0600e 1.0385 - 22.03 21.13 -22.04 - 369.49 $\pm$ 61.12 - - - - - - Irr 1  
14.0663 0.7434 - 21.98 20.51 -21.65 - 148.43 $\pm$ 18.98 - - $\rm0.02^{-0.01}_{+0.01}$ 1.241 $\rm0.15^{-0.01}_{+0.01}$ 1.155 Sbc (3.1) 2  
14.0711 1.1180 - 22.30 21.24 -22.50 -23.18 463.42 $\pm$ 96.59 - - $\rm0.42^{-0.16}_{+0.06}$ 1.166 $\rm0.03^{-0.03}_{+0.05}$ 1.228 Irr 1 M 2
14.0725 0.5820 - 22.86 21.66 -19.47 -21.26 24.12 $\pm$ 3.27 - - $\rm0.00^{-0.00}_{+0.01}$ 1.027 $\rm0.00^{-0.00}_{+0.00}$ 1.091 Irr 3  
14.0814 0.9995 - 23.56 22.04 -20.73 -22.02 163.02 $\pm$ 84.25 - - $\rm0.01^{-0.01}_{+0.02}$ 1.076 $\rm0.00^{-0.00}_{+0.01}$ 1.159 Irr 3 R?
14.0998 0.4300 23.02 21.27 20.09 -20.32 -22.17 26.08 $\pm$ 4.24 $\rm0.08^{-0.08}_{+0.32}$ 0.867 $\rm0.00^{-0.00}_{+0.00}$ 1.891 $\rm0.00^{-0.00}_{+0.00}$ 1.582 Irr 3 M 2
14.1042 0.8916 - 22.75 20.98 -21.60 -23.07 99.37 $\pm$ 10.51 $\rm0.21^{-0.21}_{+0.28}$ 1.008 $\rm0.01^{-0.01}_{+0.00}$ 1.189 $\rm0.31^{-0.01}_{+0.01}$ 1.352 C 1 M 2
14.1129 0.8443 - 22.59 21.36 -21.86 -22.81 123.68 $\pm$ 15.89 - - - - - -   4 M 1
14.1139 0.6600 22.40 21.20 20.24 -22.02 -23.47 118.00 $\pm$ 11.36 - - - - - -   4 M 1
14.1157 1.0106 - 22.44 19.95 -23.11 - 1786f - - - - - -   4 M 1
14.1190 0.7544 - 21.97 20.57 -21.58 - 92.43 $\pm$ 9.42 - - $\rm0.02^{-0.01}_{+0.01}$ 1.309 $\rm0.03^{-0.00}_{+0.00}$ 1.373 Sd (2.6) 2 R?
14.1305 0.8069 - 23.29 21.59 -20.73 - 67.30 $\pm$ 7.23 - - - - - -   4 M 1
14.1350 1.0054 - 22.70 21.43 -21.44 - 297.35 $\pm$ 139.92 - - $\rm0.01^{-0.01}_{+0.01}$ 1.085 $\rm0.00^{-0.00}_{+0.00}$ 1.171 Irr 2  
14.1415 0.7486 - 22.47 20.67 -21.48 - 87.44 $\pm$ 9.98 - - $\rm0.23^{-0.02}_{+0.03}$ 1.076 $\rm0.42^{-0.02}_{+0.01}$ 1.142 C 2 R
a Galaxy type - E/S0: 0.8 < B/T $\leq$ 1, S0: 0.5 < B/T $\leq$ 0.8, Sab: 0.15 < B/T $\leq$ 0.5, Sbc: 0 < B/T $\leq$ 0.15, Sd: B/T = 0, C: compact, T: tadpole, Irr: irregular. Note that disk scale length $R_{\rm d}$ is given in parentheses in unit of kiloparsec for spiral type galaxies.
b Quality factor - 1: secure, 2: possibly secure, 3: insecure, 4: undetermined.
c Interaction/Merging - M 1: obvious merging, M 2: possible merging, I1: obvious interaction, I2: possible interaction, R: relics of merger/interaction.
d This object is too compact to obtain structural parameters.
e Structural parameters are not successfully derived for this object from the two-dimensional structure fitting because of its clumpy light distribution and imagery close to the CCD chip border.
f Infrared luminosity is estimated according to an obscured AGN model.
Notes: Structural parameters are not provided for the merging systems with multiple distinctly separated components.

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