Simulations may be need to evaluate whether observations with a given array are relevant or not for the expected science goal. There are 3 basic questions in this respect:
Case (3) is not treated separately by IMAGER, because Observatories like ALMA and NOEMA provide their own tools to figure out the expected noise level. In Case (1), an approximate noise level can be derived using the /WEIGHT FULL option, but it is based on a generic estimate for the system temperature. A user specified noise level (e.g. the one indicated by the Observatory tool) can be accounted for in Case (2).