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An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: Near-infrared morphologies and stellar sizes
Chian-Chou Chen, Ian Smail, A. M. Swinbank +19
We analyse HST WFC3/-band observations of a sample of 48 ALMA-detected submillimeter galaxies (SMGs) in the Extended Chandra Deep Field South field, to study their stellar…
The SCUBA-2 Cosmology Legacy Survey: ALMA resolves the rest-frame far-infrared emission of sub-millimeter galaxies
J. M. Simpson, Ian Smail, A. M. Swinbank +26
We present high-resolution (0.3'') ALMA 870um imaging of 52 sub-millimeter galaxies (SMGs) in the Ultra Deep Survey (UDS) field and investigate the size and morphology of the sub-m…
Molecular gas content in strongly-lensed z~1.5-3 star-forming galaxies with low IR luminosities
M. Dessauges-Zavadsky, M. Zamojski, D. Schaerer +10
To extend the molecular gas measurements to typical star-forming galaxies (SFGs) with SFR < 40 Msun yr^{-1} and M* < 2.5x10^{10} Msun at z~1.5-3, we have observed CO emission with…
An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: radio properties and the far-infrared/radio correlation
A. P. Thomson, R. J. Ivison, J. M. Simpson +18
We present a study of the radio properties of 870m-selected submillimetre galaxies (SMGs), observed at high resolution with ALMA in the Extended Chandra Deep Field South. From o…
A 10 deg Lyman- survey at z=8.8 with spectroscopic follow-up: strong constraints on the LF and implications for other surveys
Jorryt Matthee, David Sobral, Mark Swinbank +6
Candidate galaxies at redshifts of are now being found in extremely deep surveys, probing very small areas. As a consequence, candidates are very faint, making spectros…
A submillimeter galaxy illuminating its circumgalactic medium: Ly-alpha scattering in a cold, clumpy outflow
J. E. Geach, R. G. Bower, D. M. Alexander +17
We report the detection at 850um of the central source in SSA22-LAB1, the archetypal Lyman-alpha Blob (LAB), a 100kpc-scale radio-quiet emission-line nebula at z=3.1. The flux dens…