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.