Table 3
Parameters for the detected sources.
| Source | ΔRA (″) | ΔDec (′) | Mag (contrast) | resσbf | resσbfconv | σx | σy | Θ | Extended? |
|---|---|---|---|---|---|---|---|---|---|
| F444W | |||||||||
| C2 | −5.16 ± 0.01 | 1.185 ± 0.007 | 13.84 ± 0.05 | 0.047 | 0.044 | 5 | 5 | 89.6 | Y |
| C3 | −4.756 ± 0.003 | −1.859 ± 0.003 | 12.92 ± 0.02 | 0.041 | 0.040 | 1.5 | 1.2 | 48.3 | Y |
| C4 | −4.1464 ± 0.0006 | −4.4279 ± 0.0005 | 11.078 ± 0.005 | 0.083 | 0.079 | 0.14 | 2.1 | −46.9 | N |
| C5 | 2.71 ± 0.01 | −7.03 ± 0.01 | 14.75 ± 0.07 | 0.029 | 0.029 | 1.9 | 1.3 | −87.1 | Y |
| C6 | 1.14 ± 0.01 | −8.37 ± 0.01 | 15.2 ± 0.1 | 0.023 | 0.023 | 0.35 | 0.36 | 15.5 | Y? |
| F200W | |||||||||
| C3 | −4.730 ± 0.003 | −1.862 ± 0.002 | 16.34 ± 0.05 | 0.0998 | 0.0998 | 0.26 | 0.11 | 74.2 | Y |
Notes. Parameters for the sources detected in the F444W (C2, C3, C4, C5, and C6) and F200W (C3) field of views. In the second and third column we list the coordinates for each companion and in the fourth column their contrasts with respect to the star. In the fifth and sixth columns are shown the standard deviations calculated on the residual images from left and right column of Figure B.1 and B.2. Finally, the last columns list the elongation and orientation of the convolved PSF.
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