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Table 5

Rest-frame FIR/submm and UV/optical sizes of our 3 GHz detected SMGs.

Source ID FIR/submm sizea UV/opt. sizeb

AzTEC1 c < (<5.2 kpc)
(2.1 × 1.4 kpc2)c ...
c ...
(2.8 × 2.1 kpc2)c ...
d ...
( kpc2)d ...
AzTEC2 (10.1 kpc) ...
AzTEC3 e < (<4.8 kpc)
( kpc2)e ...
AzTEC4 f < (<5.0 kpc)
[(3.9 ± 1.3) × (2.6 ± 1.3) kpc2]f ...
f ...
[(6.5 ± 2.6) × (4.5 ± 3.9) kpc2]f ...
AzTEC5 g (1.0 ± 0.8 kpc)
( kpc2)g ...
AzTEC6 ...
AzTEC7 (10.1 kpc) ...
AzTEC8 f < (<6.0 kpc)
[(4.6 ± 1.5) × (3.9 ± 2.3) kpc2]f ...
f ...
[(7.7 ± 3.9) × (3.1 ± 6.2) kpc2]f ...
AzTEC9 (10.0 kpc) ...
AzTEC11-N (10.4 kpc) ...
AzTEC11-S (10.4 kpc) ...
AzTEC12 (9.9 kpc) ...
AzTEC15 (9.3 kpc) (10.0 ± 1.6 kpc)
AzTEC17a (7.3 kpc) ...
AzTEC19a (7.2 kpc) ...
AzTEC21a h ...
( kpc2)h ...
AzTEC24b ...
AzTEC27 i ...

Notes. Besides the angular sizes, the physical sizes are given in parentheses when a spectroscopic or photometric redshift is available.

(a)

The upper FWHM size limits for AzTEC2–15 at observed-frame 890 μm are from Younger et al. (2007, 2009), while those for AzTEC17a, 19a, and 24b refer to observed-frame 1.3 mm (Miettinen et al. 2015) and represent half of the beam major axis FWHM.

(b)

The diameter at rest-frame UV/optical derived from the effective radii from Toft et al. (2014; see text for details).

(c)

The FWHM size derived from SMA 890 μm data by Younger et al. (2008) when modelling the source as a Gaussian (upper value) or elliptical disk (lower value).

(d)

The FWHM size measured from the ALMA 870 μm image (Miettinen et al., in prep.) using JMFIT.

(e)

A deconvolved FWHM size derived through ALMA 1 mm observations by Riechers et al. (2014).

(f)

The FWHM size derived from SMA 870 μm data by Younger et al. (2010) when modelling the source as a Gaussian (upper value) or elliptical disk (lower value).

(g)

The FWHM size measured from the ALMA 994 μm image (Miettinen et al., in prep.) using JMFIT.

(h)

The observed-frame 1.3 mm FWHM size of AzTEC21a derived here using JMFIT.

(i)

The major axis FWHM at 1.3 mm from Miettinen et al. (2015).

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