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Table 5:

SCUBA, MAMBO and AzTEC counterparts found in our $z\geq 3.5$ sample.
ID SCUBA MAMBO/AzTEC $z_{\rm phot}$ $z_{\rm min 90\%}$ $z_{\rm max 90\%}$ $z_{\rm phot}$ $z_{\rm radio-IR}$ S850 S1200/1100 d
(this paper) name name (this paper)     (P06) (D09) [mJy] [mJy] [arcsec]
#588 ... .../AzGN12 4.28 3.69 4.74 ... ... ... 3.07 5.2
#3850 ... .../AzGN20N 4.17 3.41 9.29 ... ... ... 2.79 2.3
#5367 ... .../AzGN27N 4.35 3.90 4.88 ... ... ... 2.31 6.5
#14505 ... GN1200.9/AzGN28 3.56 2.92 10.06 ... ... ... 2.7/2.31 4.1/4.2
#522 ... GN1200.5/AzGN06 3.93 3.06 5.23 ... ... ... 3.8/4.13 2.9/1.1
#7785 ... GN1200.46/... 3.97 3.90 4.04 ... ... ... 2.1a 4.5
#11304 ... GN1200.13/... 4.14 3.55 8.10 ... ... ... 2.2 0.8
#6099 GN03 ... 5.25 2.95 10.0 2.0 1.9 1.8 ... 2.5
#10176 GN09 .../AzGN31 5.818 3.55 10.0 2.4 13.42 8.9 2.13 3.9/5.3
#5157 GN11 ... 4.74 4.11 7.40 2.3 2.45 7.0 ... 2.4
#8520 GN12 .../AzGN08 3.68 3.34 3.83 3.1 3.20 8.6 3.83 5.16/8.7
#6463 GN18 ... 9.437/4.215 3.7 10.0 2.2 2.50 3.2 ... 3.2
#15541 GN20 GN1200.1/AzGN01 3.949 3.69 4.11 2.95 4.055 20.3 9.3/10.69 1.3/1.9/1.4
#13857 GN20.2a ... 3.746 3.27 4.04 2.83 4.051 9.9 ... 6.2
In the columns we report: the ID number of the objects (this paper); the names from the sub-mm surveys; photometric redshift estimated in this paper and their 90% confidence intervals; photometric redshifts by Pope et al. (2006, P06); radio-IR redshifts by Daddi et al. (2009, D09) - with the two spectroscopic values in boldface -; the SCUBA, MAMBO and AzTEC fluxes. The last column is the distances between the proposed IRAC-4.5 ${\mu }$m counterparts and the sub-mm positions.
a Not deboosted flux.

Source LaTeX | All tables | In the text

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