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Table B.3.

Submillimeter galaxies.

Galaxy Name vmax lflat(b)(d) l* M*(c) (e) log(LTIR(f)) (a) Mgas(a)
(km s−1) (kpc) (kpc) (1010 M) (M yr−1) (L) (M yr−1) (109 M)
SMM J02399-013 590 0.10 3.5 10.0 2294 13.1;–;13.4;13.0;– 1927.0 318.5
SMM J09431+470 295 0.10 0.9 10.0 1746 12.9;–;13.0;–;– 1117.4 39.1
SMM J105141+57 457 0.10 2.1 10.0 1296 12.8;–;–;–;13.1 423.4 98.2
SMM J123549+62 442 0.10 0.6 24.0 1794 13.0;–;–;–;– 71.8 17.1
SMM J123634+62 343 0.10 2.8 10.0 930 12.7;–;–;12.7;– 737.8 117.0
SMM J123707+62 317 0.10 1.9 24.0 1016 12.7;–;–;12.8;– 135.5 45.6
SMM J131201+42 430 0.10 2.1 10.0 1340 12.8;12.9;–;–;– 589.6 99.5
SMM J131232+42 346 0.10 1.4 10.0 1016 12.7;–;–;–;– 257.4 41.5
SMM J163650+40 523 0.10 1.6 46.0 1772 12.9;12.7;–;–;– 59.1 50.8
SMM J163658+41 590 0.10 0.5 52.0 2248 13.1;12.9;–;–;– 28.5 16.0

Notes.

(a)

calculated quantities; the mean CO(1-0)–H2 conversion factor is αCO = 1.4 ± 0.7 M(K km s−1 pc2)−1 (Vollmer et al. 2017).

(b)

assumed quantities; all other columns are input quantities from Genzel et al. (2010).

(c)

we assumed M* = 1011 M for galaxies whose mass is not given in Genzel et al. (2010).

(d)

A rotation curve of the form vrot = vmax(1 − exp(−R/lflat)) was assumed.

(e)

Twice the SFRs from Genzel et al. (2010) who used /LTIR = 1.0 × 10−10 M yr−1.

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