GALEX-GAMA

GALEX Galaxy And Mass Assembly

The figure below shows the GALEX MIS tiling for the coverage of the three GAMA subfields G9 (top), G12 (center) and G15 (lower). Existing or already accepted future MIS pointings are plotted in solid circles and the MIS pointings tp be observed by us are plotted as dashed circles.




The figure below shows: Lower panel: predicted 5 sigma photometric and spectroscopic limits of approved survey observations of GAMA fields across the optical - submm spectral range, in comparison with the predicted photometric limit of GALEX (open circles) in MIS mode and a typical source spectrum. Upper panel: corresponding angular resolution of survey observations, in relation to the angular size of a 1kpc structure at z=0.1.