Recent Results from the EVN Mk IV Data Processor at JIVE

Recent achievements at the EVN Mk IV data processor at JIVE include decreasing the read-out time for the whole correlator to 0.25 s (or 0.125 s for half the correlator), improving the end quality of user data (e.g., applying an improved 2-bit van Vleck correction), developing new astronomical capabilities (e.g., oversampling to ×4, wider-field mapping), and strengthening liaison procedures with PIs (e.g., pipelining, the EVN Archive facility). At the same time, the move to a disk-based EVN and regular incorporation of FTP fringe-checks is well underway, resulting in more reliable data quality. We will review these developments, highlighting how they may broaden the kinds of astronomy you can do. We’ll also go over some measures you can take to help you get the most out of these new/improved features.