Table 5.
Best-fit SED parameters and 1σ uncertainties.
| ID | zphot | log(LIR) (a) | SFR (b) | Td | log(Md) | log(ℳ) (c) | log(MISM) (d) |
|---|---|---|---|---|---|---|---|
| (L⊙) | (M⊙ yr−1) | (K) | (M⊙) | (M⊙) | (M⊙) | ||
| 0 | 1.06 |
12.27 |
179 |
26.6 |
8.73 |
11.53 |
11.30 |
| 1 | 2.42 |
12.53 |
320 |
27.0 |
9.16 |
10.56 |
11.58 |
| 2 | 3.05 |
12.30 |
191 |
27.6 |
8.95 |
10.86 |
11.38 |
| 3 | 1.543 (e) | 12.06 |
109 |
22.8 |
8.98 |
10.59 |
11.47 |
| 4 | 0.43 |
11.01 |
9 |
20.9 |
7.90 |
10.58 |
10.61 |
| 5 | 1.74 |
12.20 |
151 |
25.0 |
8.93 |
11.32 |
11.38 |
| 6 | 1.45 |
11.88 |
71 |
28.7 |
8.22 |
10.95 |
10.77 |
| 7 | 2.14 |
12.07 |
110 |
32.7 |
8.19 |
10.61 |
10.75 |
| 8 | 1.545 (e) | 12.60 |
381 |
32.0 |
8.69 |
11.06 |
11.35 |
| 9 | 2.21 |
11.81 |
61 |
23.4 |
8.76 |
10.60 |
11.03 |
| 10 | 1.27 |
12.24 |
164 |
27.2 |
8.68 |
11.03 |
10.98 |
| 11 | 2.43 |
12.31 |
195 |
30.7 |
8.63 |
11.26 |
11.17 |
| 12 | 1.40 |
12.12 |
126 |
28.0 |
8.52 |
11.09 |
11.06 |
| 13 | 2.63 |
12.34 |
207 |
27.0 |
9.00 |
10.46 |
11.42 |
| 14 | 2.30 |
12.43 |
255 |
33.5 |
8.51 |
10.23 |
11.09 |
| 15 | 2.45 |
11.68 |
44 |
24.0 |
8.60 |
11.21 |
10.99 |
| 16 | 1.02 |
10.71 |
4 |
14.4 |
8.62 |
10.67 |
11.16 |
| 17 | 0.98 |
12.02 |
99 |
28.6 |
8.28 |
10.89 |
10.94 |
Notes.
8–1000 μm (rest-frame) luminosity derived by fitting the FIR SED with a single-temperature modified black-body model.
SFR derived from LIR, assuming the relationship in Kennicutt (1998) modified for a Chabrier IMF, i.e. SFR[M⊙ yr−1] = 9.5 × 10−11 LIR[L⊙].
Stellar mass derived from fitting the Pan-STARRS-WIRCam-IRAC SED with the models of Bruzual & Charlot (2003).
ISM mass derived from the ALMA 233 GHz flux density (Table 1) and using Eq. (2) (Scoville et al. 2016).
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