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The Roman Space Telescope’s observing program during the first five years will consist of:
Core Community Surveys (CCS) with the Wide Field Instrument (WFI):
These are surveys that will be defined by the astronomical community and will include a High Latitude Wide Area Survey (~17 months), a High Latitude Time Domain Survey (~6 months), and a Galactic Bulge Time Domain Survey (~15 months).
General Astrophysics Surveys with the WFI that will be competitively selected, including the Galactic Plane Survey
A technology demonstration program with the Coronagraph Instrument.