activity
20012023
most citedTowards a model of full-sky Galactic synchrotron intensity and linear polarisation: a re-analysis of the Parkes data

135 citations · 259 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2023★ 2 cited

The SARAO MeerKAT 1.3 GHz Galactic Plane Survey

S. Goedhart, W. D. Cotton, F. Camilo +127

We present the SARAO MeerKAT Galactic Plane Survey (SMGPS), a 1.3 GHz continuum survey of almost half of the Galactic Plane (251° 358°and 2° 61°at $|b| \le 1.…

astro-ph.IM2018★ 10 cited

Baseline-dependent sampling and windowing for radio interferometry: data compression, field-of-interest shaping and outer field suppression

M. Atemkeng, O. Smirnov, C. Tasse +4

Traditional radio interferometric correlators produce regular-gridded samples of the true -distribution by averaging the signal over constant, discrete time-frequency intervals…

astro-ph.IM2016★ 16 cited

Using baseline-dependent window functions for data compression and field-of-interest shaping in radio interferometry

M. T. Atemkeng, O. M. Smirnov, C. Tasse +2

In radio interferometry, observed visibilities are intrinsically sampled at some interval in time and frequency. Modern interferometers are capable of producing data at very high t…

astro-ph.IM2016★ 37 cited

Engineering and Science Highlights of the KAT-7 Radio Telescope

A. R. Foley, T. Alberts, R P. Armstrong +100

The construction of the KAT-7 array in the Karoo region of the Northern Cape in South Africa was intended primarily as an engineering prototype for technologies and techniques appl…

astro-ph.IM2010★ 9 cited

Square Kilometre Array: a concept design for Phase 1

M. A. Garrett, J. M. Cordes, D. R. Deboer +3

The SKA at mid and low frequencies will be constructed in two distinct phases, the first being a subset of the second. This document defines the main scientific goals and baseline…

astro-ph2004★ 17 cited

A polarized synchrotron template for CMBP experiments after WMAP data

G. Bernardi, E. Carretti, R. Fabbri +4

We build template maps for the polarized Galactic--synchrotron emission on large angular scales (FWHM =~7), in the 20-90 GHz microwave range, by using WMAP data. The method…