Large synthesis arrays in radio astronomy operating at low frequencies require wide-field imaging using a full 3-D Fourier transform rather than the conventional 2-D approximation. This presents computational and algorithmic challenges. We discuss some solutions adopted in AIPS++

© 2001 Optical Society of America

PDF Article


You do not have subscription access to this journal. Citation lists with outbound citation links are available to subscribers only. You may subscribe either as an OSA member, or as an authorized user of your institution.

Contact your librarian or system administrator
Login to access OSA Member Subscription