Table 3.
Far-infrared dust continuum observations (ALMA band 6) and rest-frame UV/optical ground-based observations.
| Target | Synthesised beam | RMS | S1.3mm(b) | LIR(c) | Reff, FIR(d) | HAWK-I | PSF | Reff, UV/opt(e) |
|---|---|---|---|---|---|---|---|---|
| Size (″)/PA (° ) | ((a)) | (μJy) | (1011 L⊙) | (kpc) | band | (″) | (kpc) | |
| J1322+0423 | 1.59 × 1.39/−89 | 12 | < 48 | < 2.59 | – | H | 0.49 | 2.01 ± 0.10 |
| J0146–0220 | 0.63 × 0.56/−74 | 15 | 148 ± 10 | 8.06 ± 2.90 | – | Ks | 0.37 | 2.59 ± 0.10 ( † ) |
| J1415+2036 | 1.71 × 1.38/+24 | 15 | < 64 | < 3.40 | – | Ks | 0.38 | 1.24 ± 0.68 |
| J1249+1550 | 1.65 × 1.54/+56 | 17 | 155 ± 10 | 8.54 ± 3.01 | 5.0 ± 2.0 | Ks | 0.28 | 1.04 ± 0.05 |
| J0006+2452 | 1.70 × 1.30/+9 | 18 | 510 ± 30 | 28.3 ± 9.8 | 3.5 ± 0.9 | Ks | 0.39 | 2.23 ± 0.35 ( † ) |
| J0850+1549 | 0.72 × 0.59/−3 | 13 | 106 ± 20 | 5.90 ± 2.04 | 1.8 ± 0.5 | R(f) | 0.71 | 1.46 ± 0.18 |
| J1220–0051 | 1.60 × 1.33/−80 | 16 | 172 ± 12 | 9.57 ± 3.30 | 2.4 ± 1.0 | H | 0.61 | 1.51 ± 0.22 |
| J0950+0523 | 1.07 × 0.76/+57 | 14 | 331 ± 20 | 18.5 ± 6.3 | 2.0 ± 0.7 | Ks | 0.36 | < 0.74 |
| J1220+0842 | 0.62 × 0.61/−27 | 25 | < 102 | < 5.69 | – | H | 0.44 | 1.64 ± 0.24 |
| J1157+0113 | 0.63 × 0.58/−89 | 11 | 251 ± 40 | 14.1 ± 4.8 | – | H | 0.38 | 1.07 ± 0.14 |
| J0121+0025 | 1.57 × 1.14/+63 | 10 | 122 ± 30 | 7.12 ± 2.15 | 3.6 ± 0.8 | R(g) | 0.55 | 0.79 ± 0.15 |
| J1316+2614 | 1.70 × 1.33/+8 | 11 | 124 ± 20 | 7.37 ± 2.09 | 1.7 ± 0.8 | Ks | 0.30 | < 0.55 |
Notes.
Far-infrared fluxes; for the non-detections we considered 4σ upper limits (Sect. 3.3).
Infrared luminosities derived from S1.3mm assuming the MBB function (Sect. 3.3).
Far-infrared dust continuum effective radii measured in the uv plane only for the resolved galaxies using the 1.3 mm band 6 visibilities (Sect. 3.3).
Rest-frame UV or optical effective radii measured, respectively, from HAWK-I seeing-limited H-band or AO Ks-band observations (Sect. 3.4).
( † )For J0146–0220 and J0006+2452, the HAWK-I AO Ks-band observations reveal a main bright and compact (unresolved) component and a more extended diffuse component. The rest-frame optical effective radii of the bright compact component, respectively, are < 0.78 kpc and < 0.80 kpc.
CFHT MegaCam seeing-limited R-band observations were used to derive the rest-frame UV effective radius of J0850+1549 (Sect. 3.4).
Subaru seeing-limited R-band observations were used to derive the rest-frame UV effective radius of J0121+0025 as described in Marques-Chaves et al. (2021).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.