The future of radio astronomy will require instruments with large collecting areas for higher sensitivity, wide fields of view for faster survey speeds, and efficient computing and data rates relative to current capabilities.We describe the first successful deployment of the E-field Parallel Imaging Correlator (EPIC) on the LWA station in Sevilleta, New Mexico, USA (LWASV). EPIC is a solution to the computational problem of large interferometers. By gridding and spatially Fourier transforming channelized electric fields from the antennas in real time, EPIC removes the explicit cross-multiplication of all pairs of antenna voltages to synthesize an aperture, reducing the computational scaling from O(n2a ) to O(ng log2 ng), where na is the number of antennas and ng is the number of grid points. Not only does this save computational costs for dense arrays but it produces very high time resolution images in real time. The GPUbased implementation uses existing LWA-SV hardware and the high performance streaming framework, Bifrost. We examine the practical details of the EPIC deployment and verify the imaging performance by detecting a meteor impact on the atmosphere using continuous all-sky imaging at 50 ms time resolution.
- Instrumentation: interferometers
- Techniques: interferometric
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science