Simpson, J. M.J. M.Simpson0000-0001-8751-8360Swinbank, A. M.A. M.SwinbankSmail, I.I.SmailAlexander, D. M.D. M.AlexanderBrandt, W. N.W. N.BrandtBertoldi, F.F.BertoldiDe Breuck, C.C.De BreuckChapman, S. C.S. C.ChapmanCoppin, K. E. K.K. E. K.Coppinda Cunha, E.E.da CunhaDanielson, A. L. R.A. L. R.DanielsonDannerbauer, H.H.DannerbauerGreve, T. R.T. R.GreveHodge, J. A.J. A.HodgeIvison, R. J.R. J.IvisonKarim, A.A.KarimKnudsen, K. K.K. K.KnudsenPOGGIANTI, Bianca MariaBianca MariaPOGGIANTISchinnerer, E.E.SchinnererThomson, A. P.A. P.ThomsonWalter, F.F.WalterWardlow, J. L.J. L.WardlowWeiss, A.A.Weissvan der Werf, P. P.P. P.van der Werf2020-09-082020-09-082017http://hdl.handle.net/20.500.12386/27219In this study we undertake a multi-wavelength analysis of the ALMA-detected submm galaxies from the catalog presented by Hodge et al. (2013, J/ApJ/768/91) (see also Karim et al. 2013MNRAS.432....2K). To briefly summarize the observations, we obtained 120 s integrations of 122 of the original 126 LESS submm sources, initially identified using the LABOCA camera on the APEX telescope (Weiss et al. 2009, J/ApJ/707/1201). These Cycle 0 observations used the compact configuration, yielding a median synthesized beam of ~1.6"x1.2". The observing frequency was matched to the original LESS survey, 344 GHz (Band 7), and we reach a typical rms across our velocity-integrated maps of 0.4 mJy/beam. (3 data files).enDatabase10.26093/cds/vizier.17880125http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/ApJ/788/1252017yCat..17880125SFIS/05 - ASTRONOMIA E ASTROFISICA