|Object no.||Offset ( )||b ( )||U (mag)||R (mag)||LU/LU* at z = 2|
|1a||0.7 E||8.4 N||8.4||0.10|
|2a||4.1 W||2.4 N||4.7||>26.4||0.03|
|3a||6.4 W||3.4 S||7.2||1.87|
|4a||3.4 E||4.8 S||5.8||>26.4||0.10|
|5a||5.3 E||5.2 S||7.4||>26.4||0.03|
|1b||0.0 E||6.4 N||6.4||>27.3||<0.03|
|2b||1.0 W||5.4 S||5.5||24.81 0.10||0.31|
|3b||6.9 E||5.0 S||8.5||25.64 0.20||0.11|
|4b||8.2 E||6.4 S||10.4||25.55 0.07||22.25 0.02||0.13|
|5b||3.3 W||8.2 S||8.9||25.53 0.08||24.79 0.10||0.13|
|6b||5.6 W||7.7 S||9.5||26.03 0.12||26.41 0.40||0.08|
|7b||8.8 W||1.7 S||8.9||26.73 0.21||24.88 0.10||0.04|
|8b||0.7 E||0.3 S||0.8||26.92 0.10||-||0.04|
|Objects near Q1108 are in the upper 5 rows, and near Q1408 in the bottom 8 rows. The magnitudes are corrected for Galactic extinction. The last column gives the luminosity fraction relative to a U* galaxy at z=2, which has an apparent magnitude . The uncertainties are 0.01 for this fraction.|
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