& 167 & +7 –7\
$F_{tot}$ \[mJy\] & total belt flux density & 2.77 & +0.19 –0.07 & & 2.57 & +0.09 –0.08 & & 2.72 & +0.12 –0.08 & & 2.74 & +0.09 –0.10\
$\Delta$x$_c$ \[\] & RA offset of ring & 0.15 & +0.04 –0.04 & & 0.09 & +0.03 –0.03 & & 0.15 & +0.05 –0.04 & & 0.12 & +0.04 –0.04\
$\Delta$y$_c$ \[\] & Dec offset of ring & 0.05 & +0.04 –0.04 & & 0.05 & +0.03 –0.03& & 0.06 & +0.04 –0.04 & & 0.08 & +0.03 –0.03\
$i$ \[\] & inclination & 31 & +3 –3 & & 28 & +3 –3 & & 31 & +2 –3 & & 30 & +3 –3\
P.A. \[\] & position angle & 98 & +4 –3 & & 97 & +6 –6 & & 98 & +4 –4 & & 95 & +5 –5

Best-Fit Disk Parameters by Minimizing Other Contamination
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Since ALMA is sampling the sky with many different baselines (i.e., spatial scales) through interferometry, we can better assess the properties of the bright source by generating a map with only the long baseline data ($>$80 $k\lambda$ = 31) where any extended structure 