| 5 | 7 | 1. We plan to start with simulated CABB output files, which should be available by 2007 Oct. Many of the CABB output formats have been written already, by various observatory systems (MOPS, Parkes DFBs) using the ATNF's standard RPFITS library; the changes to Miriad mainly relate to handling the larger number of IFs and spectral channels within the data files. Shortly after the first test data starts appearing (Nov 2007) it will be possible to read it into Miriad and do basic processing of subsections of the full bandwidth. At this stage interactive review and flagging of the UV data will be necessary. Some changes to the data selection subroutines and the INVERT task may be needed before images can be formed. |
