Changes
prime focus detector = mosaic of 4 x H4RG-10 HgCdTe arrays with 10 micron pixels (flight spares from the WFIRST mission)
filters: z, Y, J, H, selected narrow bands ([FeII]、Paβ、HeI, used in parallel with broadband to reduce OH contamination)
'''Science Drivers:'''
''Main programme (50% of total time, mostly in winter): '' microlensing detection in the Galactic bulge (50% of total time) to search for exoplanets ''Secondary programmes (comprising the remaining 50% of the time):''
exoplanet transits
variable stars
transients (with ToO override over-ride capability)
'''Schedule:'''
