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Galaxy And Mass Assembly (GAMA)
Simon P. Driver, the GAMA team
The GAMA survey aims to deliver 250,000 optical spectra (3--7Ang resolution) over 250 sq. degrees to spectroscopic limits of r_{AB} <19.8 and K_{AB}<17.0 mag. Complementary imaging…
Revised masses of dust and gas of SLUGS FIR bright galaxies based on a recent CO survey
E. R. Seaquist, Lihong Yao, L. Dunne +1
Recent CO measurements of an essentially complete sub-sample of galaxies from the SCUBA Local Universe Survey (SLUGS) are used to examine their implications for dust and gas masses…
A census of metals at high and low redshifts and the connection between submillimetre sources and spheroid formation
L. Dunne, S. A. Eales, M. G. Edmunds
Deep surveys in many wavebands have shown that the rate at which stars were forming was at least a factor of 10 higher at z > 1 than today. Heavy elements (metals) are produced by…
The Canada-UK Deep Submillimeter Survey V: The Submillimeter Properties of Lyman-Break Galaxies
T. M. A. Webb, S. Eales, S. Foucaud +9
We have used 850m maps obtained as part of the Canada-UK Deep Submillimeter Survey (CUDSS) to investigate the sub-mm properties of Lyman-break galaxies (LBGs). We used three sam…
High spatial resolution observations of CUDSS14A: a SCUBA-selected Ultraluminous galaxy at high redshift
W. K. Gear, S. J. Lilly, J. A. Stevens +4
We present a high-resolution millimetre interferometric image of the brightest SCUBA-selected galaxy from the Canada-UK deep SCUBA survey (CUDSS). We make a very clear detection at…
Constraining the Radio-Submm Redshift Indicator using data from the SCUBA Local Universe Galaxy Survey
L. Dunne, D. L. Clements, S. A. Eales
Many of the faint submm sources uncovered by deep SCUBA surveys still remain unidentified at most, if not all other wavelengths. The most successful method so far of obtaining accu…