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Table 1:

Sample of SMGs with redshift and MIPS photometry or 3$\sigma $upper limits (in mJy).
Name z 24 $\mu $m 70 $\mu $m 160 $\mu $m
SMM J163658.78+405728.1 1.2 0.45 <4.9 <30
SMM J030227.73+000653.5 1.4 0.23 <8.8 -
MM J163639+4056 1.5 0.23 <5.5 <21
MM J163650+4057 2.4 1.02 <5.5 <22
SMM J09429+4659 2.4 0.19 <6.8 <23
MM J163706+4053 2.4 0.41 <5.1 <17
MM J105155+5723 2.7 0.18 <2.2 <16
SMM J105207.56+571904.7 2.7 0.24 <2.0 <13
SMM J00266+1708 2.7 0.32 - -
MM J154127+6616 2.8 0.24 - -
SMM J02399-0136 2.8 1.24 $15^{\dagger}$ 16
SMM J09431+4700 3.4 1.04 <7.2 <22

$^{\dagger}$ Tentative detection: brightest source pixel appears ${\sim}8''$ off from NED position.


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