1 code implementation • 7 Jan 2021 • Samir Choudhuri, Philip Bull, Hugh Garsden
We also investigate the possibility of signal loss due to decoherence effects when non-redundant visibilities are averaged together, finding that the decoherence is worst when bright point sources pass through the beam, and that its magnitude varies significantly between baseline groups and types of primary beam variation.
Cosmology and Nongalactic Astrophysics Instrumentation and Methods for Astrophysics
1 code implementation • 2 Aug 2017 • Miles D. Cranmer, Benjamin R. Barsdell, Danny C. Price, Jayce Dowell, Hugh Garsden, Veronica Dike, Tarraneh Eftekhari, Alexander M. Hegedus, Joseph Malins, Kenneth S. Obenberger, Frank Schinzel, Kevin Stovall, Gregory B. Taylor, Lincoln J. Greenhill
Computing blocks in the library are designed for applications such as interferometry, pulsar dedispersion and timing, and transient search pipelines.
Instrumentation and Methods for Astrophysics Distributed, Parallel, and Cluster Computing Instrumentation and Detectors
