Open Access

Table 1.

Main properties of our sample of 22 DSFGs.

ID Redshift Mass Masscore SFR SFRcore Type (c) Morphology (d)
(CANDELS) log10(M*/M) log10(M*/M) M yr−1 M yr−1
11887 1.539 (b) 10.5 ± 0.1 9.59 ± 0.07 38 ± 24 5 ± 3 Type I Lop
13098 1.720 (a) 10.6 ± 0.1 10.22 ± 0.04 73 ± 63 62 ± 9 Type II wLop
13107 2.21 ± 0.02 10.1 ± 0.1 9.43 ± 0.06 29 ± 21 10 ± 2 Type II Lop
13776 2.297 (b) 11.4 ± 0.1 10.86 ± 0.05 340 ± 214 114 ± 64 Type II SMGc+Lop
13932 2.48 ± 0.02 10.2 ± 0.1 8.91 ± 0.07 35 ± 20 3 ± 1 Type I wLop
14559 2.020 ± 0.004 (a) 10.2 ± 0.1 9.59 ± 0.07 44 ± 25 10 ± 3 Type I ...
15036 1.60 ± 0.01 (a) 10.5 ± 0.1 10.02 ± 0.03 36 ± 22 3 ± 2 Type III ...
15371 1.921 (b) 11.0 ± 0.1 10.61 ± 0.03 197 ± 125 26 ± 13 Type III wLop
16544 2.73 ± 0.03 (a) 11.4 ± 0.1 10.89 ± 0.03 269 ± 186 97 ± 31 Type I SMGc+wLop
18278 1.805 (a) 11.5 ± 0.1 10.84 ± 0.06 254 ± 168 72 ± 23 Type II SMGc+Lop
18694 2.80 ± 0.01 11.1 ± 0.1 10.22 ± 0.05 415 ± 244 52 ± 9 Type I Lop
21190 1.68 ± 0.01 (a) 11.0 ± 0.1 10.48 ± 0.07 106 ± 95 94 ± 20 Type II SMGc
23205 2.14 ± 0.01 (a) 11.40 ± 0.05 10.78 ± 0.03 138 ± 87 21 ± 10 Type III ...
23510 2.51 ± 0.02 (a) 10.4 ± 0.2 9.51 ± 0.15 141 ± 106 27 ± 6 Type I wLop
23581 2.83 ± 0.02 11.3 ± 0.1 11.01 ± 0.06 259 ± 152 87 ± 38 Type I SMGc+Lop
25604 1.673 (b) 11.1 ± 0.1 10.75 ± 0.02 24 ± 18 3 ± 4 Type III ...
26188 2.87 ± 0.02 10.8 ± 0.1 10.10 ± 0.05 257 ± 178 34 ± 11 Type I wLop
29608 1.64 ± 0.03 10.7 ± 0.1 9.72 ± 0.09 342 ± 181 84 ± 11 Type I SMGc+wLop
30012 1.53 ± 0.01 (a) 11.0 ± 0.1 10.62 ± 0.03 49 ± 42 6 ± 3 Type III ...
30186 1.85 (a) 11.7 ± 0.1 11.29 ± 0.03 550 ± 436 136 ± 57 Type I SMGc+wLop
31125 2.08 ± 0.02 11.60 ± 0.05 10.90 ± 0.03 237 ± 156 25 ± 18 Type III ...
31281 1.634 (b) 10.80 ± 0.05 10.35 ± 0.03 36 ± 35 0.9 ± 0.5 Type III ...

Notes.

(a)

Grism based redshift.

(b)

Spectroscopic redshift.

(c)

Type I: Star-forming disk and star-forming core; Type II: star-forming disk and quiescent (Q) core; Type III: quiescent core and star-forming disk

(d)

“SMGc” and “(w)Lop” stand for sub-millimeter galaxy counterpart and (weakly) lopsided, respectively.

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