Table 3: Absolute magnitudes for the resolved host galaxies.
object MU MB/mB Mg MR MI/mI MF814W MJ $M_{K{\rm s}}$ rB[''] rI['']
FDF0809 [disk] -21.02 -20.02/24.62 -21.32 -22.02 -22.22/21.79 -22.26 -22.62 -23.62 0.24 0.32
FDF0809 [bulge] -24.12 -22.52/24.63 -22.52 -23.12 -23.12/21.43 -23.34 -22.62 -23.32 0.21 0.26
FDF1837 [bulge] -21.99 -19.95/26.32 -19.69 -21.09< -22.23/24.04< - - - 0.30 0.11
FDF1837 [disk] -21.79 -19.78/26.49 -21.36 -21.66< -22.48/23.79< - - - 0.26 0.12
FDF2229 [bulge] -23.40 -22.35/23.81 -22.62 -23.14< -23.09/23.07< - - - 0.31 0.13
FDF2229 [disk] -23.63 -21.88/24.28 -22.06 -23.11 -23.37/22.79< - - - 0.38 0.13
FDF6007 [bulge] - -21.60/25.20 -20.81 -22.15< -22.31/24.49 - - - 0.50 0.67
FDF6007 [disk] - -21.10/25.70 -20.78 -21.74 -21.76/25.04 - - - 0.44 0.54
We marked the magnitudes for objects for which the radii indicate that the galaxy is only marginally resolved. For a full result table, see Appendix A. For further information, see discussion in the text.

Source LaTeX | All tables | In the text