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Table A.3:

Properties of SMGs derived from the SED modeling.
    SFR ($M_\odot$ yr-1) SSFR $\log M_*$ $M_{\rm burst}/M_*$ M*/LK $\log M_{\rm d}$ $\log L_{\rm IR}$ $T_{\rm d}$ AV    
SMG z SED UV IR Radio (Gyr-1) ($M_\odot$) (%) ( $M_\odot/L_\odot$) ($M_\odot$) ($L_\odot$) (K) (mag) q AGN?
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15) (16)
SMMJ030227.73+000653.5 1.408 825 7.91 713 1190 4.81 11.17 25.5 0.42 8.54 12.62 52.6 1.81 2.29 rad
SMMJ030231.81+001031.3 1.316 433 0.68 224 211 7.81 10.46 71.1 1.36 9.10 12.11 25.6 4.38 2.54 ...
SMMJ030236.15+000817.1 2.435 91 4.18 1152 810 3.33 11.54 1.1 0.55 8.62 12.83 41.3 0.27 2.67 mIR,rad
SMMJ105151.69+572636.0 1.147 134 0.30 248 457 0.92 11.43 1.5 0.65 8.97 12.16 34.4 4.00 2.25 rad
SMMJ105155.47+572312.7 2.686 837 12.95 589 1110 1.91 11.49 12.5 0.66 8.90 12.54 38.7 2.29 2.24 mIR
SMMJ105158.02+571800.2 2.239 314 16.77 373 1561 0.44 11.93 0.6 0.60 9.15 12.34 33.2 1.12 1.89 rad
SMMJ105200.22+572420.2 0.689 163 0.26 118 59 0.74 11.20 4.5 1.56 8.72 11.84 33.2 2.58 2.82 ...
SMMJ105201.25+572445.7 2.148 935 2.58 798 1044 3.40 11.37 18.1 0.95 9.01 12.67 45.1 2.91 2.40 mIR
SMMJ105207.49+571904.0 2.689 2195 3.81 1559 6679 1.93 11.91 12.5 1.18 8.80 12.96 45.1 2.85 1.88 rad
SMMJ105225.79+571906.4 2.372 217 18.89 329 2310 0.75 11.64 0.0 0.49 8.96 12.28 33.2 1.16 1.67 rad
SMMJ105227.58+572512.4 2.142 410 4.73 376 564 0.57 11.82 1.9 0.78 8.79 12.34 38.7 1.71 2.34 ...
SMMJ105227.77+572218.2 1.956 515 1.55 447 473 0.89 11.70 4.5 1.16 9.01 12.42 33.2 2.17 2.49 ...
SMMJ105230.73+572209.5 2.611 1255 45.92 975 1942 0.72 12.13 3.8 0.68 9.18 12.75 38.7 1.51 2.22 ...
SMMJ105238.19+571651.1 1.852 919 21.87 659 734 4.54 11.16 28.8 0.37 8.85 12.58 38.7 2.13 2.47 ...
SMMJ105238.30+572435.8 3.036 1558 7.40 1169 1921 0.69 12.23 3.9 0.85 9.04 12.83 45.1 1.86 2.30 spec
SMMJ123549.44+621536.8 2.203 237 29.23 335 1144 0.70 11.68 0.0 0.51 9.18 12.29 33.2 1.11 1.98 X,rad
SMMJ123553.26+621337.7 2.098 1460 6.05 1223 802 5.73 11.33 31.8 0.42 8.85 12.85 52.6 2.99 2.70 SB
SMMJ123555.14+620901.7 1.875 332 11.94 358 2252 0.61 11.76 1.0 0.61 8.98 12.32 33.2 1.41 1.72 X,mIR,rad
SMMJ123600.10+620253.5 2.710 3733 6.49 3066 6407 8.92 11.54 51.6 0.29 8.52 13.25 71.5 3.64 2.20 rad
SMMJ123600.15+621047.2 1.994 1449 3.04 1102 1602 2.53 11.64 15.2 0.89 9.03 12.81 38.7 2.80 2.35 SB,rad
SMMJ123606.72+621550.7 2.416 448 30.23 354 454 1.27 11.45 6.9 0.65 8.92 12.32 33.2 1.15 2.41 X,spec,mIR
SMMJ123606.85+621021.4 2.509 1291 12.59 1153 1531 1.17 11.99 5.6 0.79 9.34 12.83 33.2 1.58 2.39 X,rad
SMMJ123616.15+621513.7 2.578 968 2.91 754 1179 0.80 11.97 4.5 1.12 9.04 12.64 33.2 2.17 2.32 X
SMMJ123618.33+621550.5 1.865 339 2.20 325 1585 0.66 11.70 2.4 1.10 9.25 12.28 28.5 2.33 1.83 SB,rad
SMMJ123621.27+621708.4 1.988 330 5.65 266 1797 0.32 11.91 1.5 1.30 9.43 12.19 24.4 1.92 1.69 SB,rad
SMMJ123622.65+621629.7 2.466 1981 6.78 1438 1403 1.72 11.92 10.8 0.90 8.90 12.92 45.1 2.40 2.53 X
SMMJ123629.13+621045.8 1.013 202 0.69 176 207 0.35 11.70 1.5 1.53 9.07 12.01 24.4 2.13 2.45 X
SMMJ123632.61+620800.1 1.993 1067 17.30 973 1107 4.52 11.33 22.7 0.45 8.45 12.75 71.5 1.70 2.46 X,spec,mIR,rad
SMMJ123634.51+621241.0 1.219 309 4.49 289 901 0.64 11.66 2.4 1.06 8.93 12.23 28.5 2.16 2.02 SB,rad
SMMJ123635.59+621424.1 2.005 1921 14.81 1740 1087 7.23 11.38 37.1 0.25 8.45 13.01 71.5 2.31 2.72 X,spec,mIR
SMMJ123636.75+621156.1 0.557 11 0.94 21 24 0.69 10.47 0.8 0.67 9.36 11.08 15.2 1.04 2.44 X,spec
SMMJ123707.21+621408.1 2.484 361 4.01 338 905 0.38 11.95 1.3 0.92 8.95 12.29 33.2 1.65 2.09 X,rad
SMMJ123711.98+621325.7 1.992 371 2.50 337 658 1.72 11.29 8.0 0.61 8.64 12.29 45.1 2.30 2.23 X,rad
SMMJ123712.05+621212.3 2.914 150 4.96 247 604 0.20 12.10 0.0 1.32 9.53 12.16 24.4 1.91 2.13 X,spec,rad
SMMJ123716.01+620323.3 2.037 879 567.07 1091 1399 1.28 11.93 0.0 0.31 8.74 12.80 45.1 0.18 2.41 X,spec
SMMJ123721.87+621035.3 0.979 76 2.44 91 96 0.33 11.44 0.6 0.80 9.77 11.72 16.9 1.12 2.49 X,spec
SMMJ131201.17+424208.1 3.405 4375 37.82 3748 1992 16.26 11.36 88.3 0.18 8.14 13.34 113.3 3.08 2.79 spec
SMMJ131208.82+424129.1 1.544 787 3.75 551 560 1.75 11.50 10.9 0.74 8.70 12.51 45.1 1.99 2.51 spec
SMMJ131212.69+424422.5 2.805 2095 2.18 1470 2710 2.22 11.82 14.4 1.29 8.89 12.93 38.7 3.44 2.25 spec,rad
SMMJ131215.27+423900.9 2.565 2361 3387.93 80 1498 0.04 12.32 0.0 0.32 9.90 11.67 15.4 0.00 1.24 spec,mIR
SMMJ131222.35+423814.1 2.565 600 512.57 510 569 0.88 11.76 0.0 0.31 8.75 12.47 33.2 0.10 2.47 spec,mIR
SMMJ131225.20+424344.5 1.038 238 8.94 252 205 2.26 11.05 7.2 0.36 8.42 12.17 38.7 1.46 2.60 ...
SMMJ131225.73+423941.4 1.554 742 5.47 661 5188 3.94 11.22 19.1 0.59 8.62 12.59 45.1 2.14 1.62 rad
SMMJ131228.30+424454.8 2.931 1572 16.32 1131 1482 2.43 11.67 15.3 0.61 8.30 12.82 61.3 1.75 2.40 ...
SMMJ131231.07+424609.0 2.713 1212 1.42 910 966 5.13 11.25 31.8 0.66 8.70 12.72 45.1 3.95 2.49 ...
SMMJ131232.31+423949.5 2.320 2457 8.41 1660 1635 1.60 12.02 10.8 0.87 8.47 12.99 61.3 2.40 2.52 mIR
SMMJ131239.14+424155.7 2.242 1271 3.75 1068 795 3.32 11.51 17.9 0.80 9.01 12.79 38.7 2.87 2.64 ...
SMMJ141741.81+522823.0 1.150 948 13.50 770 274 0.75 12.01 3.8 0.72 8.48 12.65 45.1 1.28 2.97 mIR
SMMJ141742.04+523025.7 0.661 403 11.08 267 216 2.02 11.12 13.8 0.40 8.23 12.19 45.1 1.74 2.61 ...
SMMJ141750.50+523101.0 2.128 343 5.31 241 808 1.91 11.10 12.5 0.66 8.58 12.15 38.7 2.29 1.99 ...
SMMJ141800.40+512820.3 1.913 1999 17.45 1095 1424 0.39 12.44 3.3 0.80 8.61 12.80 52.6 0.89 2.40 ...
SMMJ141802.87+523011.1 2.127 1325 10.95 1127 552 11.82 10.98 63.5 0.74 8.34 12.82 61.3 2.87 2.83 ...
SMMJ141809.00+522803.8 2.712 1213 6.24 551 1641 0.33 12.23 3.3 0.83 8.64 12.51 45.1 1.09 2.04 ...
SMMJ141813.54+522923.4 3.484 243 6.65 240 3967 1.16 11.31 4.2 0.60 8.86 12.15 33.2 1.35 1.30 spec,rad
SMMJ163627.94+405811.2 3.180 1332 18.32 1095 3210 6.32 11.24 34.0 0.65 8.82 12.80 45.1 2.41 2.05 spec
SMMJ163631.47+405546.9 2.283 1325 10.28 865 1646 1.77 11.69 12.5 0.96 8.94 12.70 38.7 2.62 2.24 spec
SMMJ163639.01+405635.9 1.495 250 7.51 1101 1002 6.49 11.23 4.8 0.53 8.94 12.81 32.7 1.46 2.56 mIR,rad
SMMJ163650.43+405734.5 2.378 1147 73.43 1191 4030 3.24 11.57 10.1 0.33 8.93 12.84 45.1 1.12 1.99 spec,mIR,rad
SMMJ163658.19+410523.8 2.454 1769 4.97 1485 1801 2.55 11.77 13.8 0.80 9.04 12.94 45.1 2.45 2.43 ...

 

Table A.3: Properties of SMGs derived from the SED modeling.
    SFR ($M_\odot$ yr-1) SSFR $\log M_*$ $M_{\rm burst}/M_*$ M*/LK $\log M_{\rm d}$ $\log L_{\rm IR}$ $T_{\rm d}$ AV    
SMG z SED UV IR radio (Gyr-1) ($M_\odot$) (%) ( $M_\odot/L_\odot$) ($M_\odot$) ($L_\odot$) (K) (mag) q AGN?
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15) (16)
SMMJ163658.78+405728.1 1.190 129 8.41 171 274 0.56 11.49 0.9 0.59 9.13 11.10 24.4 1.14 2.31 ...
SMMJ163704.34+410530.3 0.840 205 2.50 157 74 2.22 10.85 13.1 0.92 9.13 11.96 33.2 2.43 2.84 ...
SMMJ163706.51+405313.8 2.374 2020 9.63 1478 1344 1.83 11.91 10.9 0.76 9.06 12.94 45.1 1.99 2.56 spec
SMMJ221724.69+001242.1 0.510 154 14.71 43 62 0.21 11.31 3.4 0.63 9.36 11.40 15.9 0.69 2.36 ...
SMMJ221725.97+001238.9 3.094 2499 2.29 1935 1353 2.10 11.96 12.5 1.58 9.38 13.05 38.7 3.27 2.67 ...
SMMJ221733.02+000906.0 0.926 447 0.72 381 333 0.88 11.64 4.5 1.56 9.16 12.35 33.2 2.58 2.58 ...
SMMJ221733.12+001120.2 0.652 31 2.77 59 62 0.28 11.33 4.7 1.79 9.13 11.54 21.8 1.27 2.49 rad
SMMJ221733.91+001352.1 2.555 875 17.73 731 954 0.78 11.97 3.8 0.79 9.01 12.63 38.7 1.69 2.40 ...
SMMJ221735.15+001537.2 3.098 594 8.51 536 1627 2.28 11.37 10.0 0.68 8.94 12.49 38.7 1.93 2.03 ...
SMMJ221735.84+001558.9 3.089 1969 7.43 1668 1450 6.49 11.41 35.0 0.30 8.35 12.99 71.5 2.98 2.58 ...
SMMJ221737.39+001025.1 2.614 2991 13.32 2641 2484 7.05 11.57 37.1 0.29 8.47 13.19 71.5 2.70 2.54 ...
SMMJ221804.42+002154.4 2.517 1474 15.50 1239 908 6.30 11.29 33.5 0.55 8.85 12.86 52.6 2.11 2.65 mIR
SMMJ221806.77+001245.7 3.623 8825 29.59 7774 11225 20.81 11.57 109.9 0.23 8.25 13.66 113.3 3.76 2.36 rad
SMMJ030226.17+000624.5 0.080 3 0.06 2 4 0.07 10.53 0.4 1.08 8.28 10.11 11.4 0.33 2.24 rad
SMMJ030238.62+001106.3 0.276 14 0.04 36 44 59.74 8.78 113.3 0.36 8.32 11.32 25.5 4.22 2.43 spec,rad
SMMJ030244.82+000632.3 0.176 6 0.59 11 7 0.37 10.46 0.0 0.76 8.22 10.80 20.1 1.44 2.69 ...
SMMJ123651.76+621221.3 0.298 6 0.12 14 7 1.02 10.13 0.9 0.98 8.91 10.90 13.3 1.93 2.79 ...
mean 2.002 1065 68.35 873 1429 3.51 11.71 15.6 0.75 9.02 12.71 40.1 2.03 2.34 ...
median 2.148 825 6.78 659 1087 1.72 11.54 7.2 0.68 8.91 12.58 38.7 1.99 2.40 ...
std dev 0.851 1271 395.38 1066 1731 7.44 0.55 23.2 0.36 0.36 0.60 18.3 0.95 0.34 ...
min 0.080 3 0.04 2 4 0.04 8.78 0.0 0.18 8.14 10.11 11.4 0.00 1.24 ...
max 3.623 8825 3387.93 7774 11225 59.74 12.44 113.3 1.79 9.90 13.66 113.3 4.38 2.97 ...

Notes. Column (1): SMG name. Column (2): redshift (Chapman et al. 2005). Column (3): total star formation rate (SFR) for 0.15-120 $M_\odot$ stars averaged over the last 50 Myr derived from the SED model. Column (4): SFR from UV emission interpolated from the SED template (using Kennicutt 1998). Column (5): SFR from IR emission (Column 12) used in all analysis throughout the paper (using Kennicutt 1998). Column (6): SFR from radio emission derived directly from the radio data (using Bell 2003). Column (7): specific SFR  $\equiv\mbox{SFR}_{\rm IR}/M_*$. Column (8): stellar mass. Column (9): Ratio of the mass of gas converted to star during the recent starburst episode to the total stellar mass. There are values greater than 100%, because the starburst episode is ongoing; 0% means that non-starburst template was adopted. Column (10): stellar mass to light ratio (luminosity at rest-frame K was intepolated using the best SED model). Column (11): dust mass. Column (12): total 8-1000 $\mu $m infrared luminosity. Column (13): dust temperature. Column (14): Average extinction $ A_V=2.5\log$(V-band starlight unextinguished / V-band starlight observed). Column (15): IR-radio correlation parameter (Sect. 5.4.1). Column (16): AGN flag - X: X-ray identified AGN; SB: X-ray identified starburst (Alexander et al. 2005); spec: spectroscopically identified AGN or QSO (Chapman et al. 2005); mIR: mid-IR identified AGN (Sect. 5.4.2); rad: radio datapoint is more than 3$\sigma$ above the starburst model (Sect. 5.4.2). The horizontal line divides the z>0.5 and z<0.5 samples.


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