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Table 4:

Stars in N88A observed with the S27 camera (Field 2) in the Ks-band (numbers refer to Fig. 4).

Id.
$\alpha$(2000) $\delta$(2000) $K^{\rm dao}$ err $K^{\rm psf}$ $L^{\rm ap}$ K-L
57 1 24 8.88 -73 8 56.00 14.64 0.003   14.36 $\pm$ 0.05  
34 1 24 7.94 -73 9 5.69 18.45 0.070      
35 1 24 7.64 -73 9 5.42 18.73 0.050      
37 1 24 7.83 -73 9 4.56 16.43 0.032 16.66 $\pm$ 0.15    
38 1 24 8.30 -73 9 3.85 18.46 0.060      
40 1 24 8.21 -73 9 3.80 18.40 0.065      
41 1 24 7.93 -73 9 3.99 14.99 0.010 15.05 $\pm$ 0.10 14.1 $\pm$ 0.10 0.95
42 1 24 7.85 -73 9 3.82 16.11 0.047 16.60 $\pm$ 0.30    
43 1 24 8.21 -73 9 3.30 17.62 0.066      
44 1 24 8.23 -73 9 3.05 17.76 0.060      
45 1 24 8.16 -73 9 3.14 17.12 0.044      
47 1 24 7.93 -73 9 3.19 15.62 0.036 15.99 $\pm$ 0.20    
49 1 24 8.16 -73 9 2.70 17.41 0.061      
51 1 24 7.49 -73 9 2.29 18.27 0.040      
52 1 24 7.88 -73 9 1.90 18.65 0.061      
L1-C 1 24 7.95 -73 9 3.80 $\geq$18.5 0.024   13.98 $\pm$ 0.20 $\geq$4.52

Notes.  $^{\rm dao}$, $^{\rm psf}$ and $^{\rm ap}$ magnitudes derived using DAOPHOT, the PSF of star $\char93 $57, and an aperture respectively.


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