Table 1:

Flux densities measured from the MIPS and Herschel maps.

ID
RA Dec Flux24 Flux100 Flux160 Flux250 Flux350 Flux500
  [deg] [deg] [mJy] [mJy] [mJy] [mJy] [mJy] [mJy]

HLS01
104.72828 -55.88917 0.40 $\pm$ 0.01 $ \ldots$ $ \ldots$ 21.1 $\pm$ 2.5 10.0 $\pm$ 3.5 <7.8b
HLS02 104.46419 -56.02209 0.15 $\pm$ 0.01 $ \ldots$ $ \ldots$ 10.1 $\pm$ 2.4 16.2 $\pm$ 3.5 14.4 $\pm$ 4.0
HLS03 104.48783 -56.03070 0.39 $\pm$ 0.02 $ \ldots$ $ \ldots$ 9.0 $\pm$ 2.4 9.5 $\pm$ 3.4 <7.8b
HLS04 104.45727 -55.91533 0.39 $\pm$ 0.01 $ \ldots$ $ \ldots$ 18.6 $\pm$ 2.8 13.2 $\pm$ 3.6 <7.8b
HLS05 104.60260 -55.92013 0.71 $\pm$ 0.02 75.4 $\pm$ 1.3 164.4 $\pm$ 5.1 168.9 $\pm$ 6.2 120.0 $\pm$ 4.1 58.4 $\pm$ 4.4
HLS06 104.64300 -55.90990 0.40 $\pm$ 0.01 9.9 $\pm$ 1.2 28.4 $\pm$ 2.4 44.6 $\pm$ 2.8 39.0 $\pm$ 3.5 25.2 $\pm$ 4.0
HLS07 104.60545 -55.89051 0.29 $\pm$ 0.01 7.0 $\pm$ 1.3 7.8 $\pm$ 2.1 8.2 $\pm$ 2.8 <8.4b <7.8b
HLS08 104.63628 -55.98351 0.135 $\pm$ 0.003 2.7 $\pm$ 1.1 4.6 $\pm$ 2.1 <6.0b <8.4b <7.8b
HLS09 104.55591 -55.87279 0.65 $\pm$ 0.02 $ \ldots$ $ \ldots$ 23.2 $\pm$ 2.6 12.9 $\pm$ 3.5 <7.8b
HLS10 104.54350 -55.98005 0.53 $\pm$ 0.02 16.7 $\pm$ 1.4 22.6 $\pm$ 2.1 13.9 $\pm$ 2.4 <8.4b <7.8b
HLS11 104.56008 -55.95848 0.47 $\pm$ 0.01 7.4 $\pm$ 1.1 15.1 $\pm$ 2.1 33.1 $\pm$ 2.7 36.9 $\pm$ 3.5 18.8 $\pm$ 4.1
HLS12 104.62997 -55.94386 0.046 $\pm$ 0.003 <2.4b 4.3 $\pm$ 2.1 7.8 $\pm$ 2.5 11.4 $\pm$ 3.4 <7.8b
HLS13 104.60567 -55.94490 0.28 $\pm$ 0.01 2.9 $\pm$ 1.1 5.5 $\pm$ 2.0 10.1 $\pm$ 2.5 19.6 $\pm$ 3.5 <7.8b
HLS14 104.64689 -55.88658 0.136 $\pm$ 0.004 3.0 $\pm$ 1.2 4.4 $\pm$ 2.1 <6.0b <8.4b <7.8b
HLS15 104.73730 -55.88516 0.16 $\pm$ 0.02 $ \ldots$ $ \ldots$ 11.1 $\pm$ 2.7 15.3 $\pm$ 3.8 11.7 $\pm$ 3.7
HLS16 104.58575 -55.93920 0.83 $\pm$ 0.02 25.3 $\pm$ 1.3 51.3 $\pm$ 2.5 47.7 $\pm$ 2.6 24.0 $\pm$ 3.6 10.2 $\pm$ 3.7
HLS17 104.64463 -56.00850 0.71 $\pm$ 0.02 24.7 $\pm$ 1.2 56.5 $\pm$ 3.4 49.2 $\pm$ 3.4 35.5 $\pm$ 3.7 17.9 $\pm$ 3.7
HLS18Aa 104.65471 -55.95193 0.49 $\pm$ 0.01 7.0 $\pm$ 1.2 24.5 $\pm$ 2.1 65.3 $\pm$ 2.8 98.6 $\pm$ 3.9 101.4 $\pm$ 4.0
HLS18Ba 104.65861 -55.95057 0.36 $\pm$ 0.01 3.8 $\pm$ 1.1 14.0 $\pm$ 2.5 <6.0b <8.4b <7.8b

HLS19

104.59877 -55.87833 1.10 $\pm$ 0.03 $ \ldots$ $ \ldots$ 40.9 $\pm$ 2.9 21.6 $\pm$ 4.0 9.4 $\pm$ 3.7

Notes. The 500 $\mu $m map was corrected for SZ contamination before extracting the photometry. These measurements have not been corrected for the amplification due to gravitational lensing. (a) Multiple images of the highly lensed galaxy (Gonzalez et al. 2009); (b) upper limits correspond to statistical 3-$\sigma $ noise levels of each map.


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