596 citations
- Commonwealth Scientific and Industrial Research OrganisationAU284 papers
- Australia Telescope National FacilityAU193 papers
- Centre National de la Recherche ScientifiqueFR158 papers
- Astronomy and SpaceAU120 papers
- The University of SydneyAU120 papers
- International Centre for Radio Astronomy ResearchAU114 papers
- Institut d'Astrophysique de ParisFR103 papers
- Australian National UniversityAU100 papers
- Curtin UniversityAU92 papers
- Space Telescope Science InstituteUS88 papers
- California Institute of TechnologyUS84 papers
- European Southern ObservatoryCL84 papers
6 papers · 2 filters
A wide-band, active antenna system for long wavelength radio astronomy
Brian C. Hicks, Nagini Paravastu-Dalal, Kenneth P. Stewart +9
We describe an "active" antenna system for HF/VHF (long wavelength) radio astronomy that has been successfully deployed 256-fold as the first station (LWA1) of the planned Long Wav…
Noise in the Cross-Power Spectrum of the Vela Pulsar
C. R. Gwinn, M. D. Johnson, J. E. Reynolds +12
We compare the noise in interferometric measurements of the Vela pulsar from ground- and space-based antennas with theoretical predictions. The noise depends on both the flux densi…
Fast Holographic Deconvolution: a new technique for precision radio interferometry
Ian Sullivan, Miguel Morales, Bryna Hazelton +48
We introduce the Fast Holographic Deconvolution method for analyzing interferometric radio data. Our new method is an extension of A-projection/software-holography/forward modeling…
The EoR Sensitivity of the Murchison Widefield Array
A. P. Beardsley, B. J. Hazelton, M. F. Morales +48
Using the final 128 antenna locations of the Murchison Widefield Array (MWA), we calculate its sensitivity to the Epoch of Reionization (EoR) power spectrum of red- shifted 21 cm e…
A new layout optimization technique for interferometric arrays, applied to the MWA
A. P. Beardsley, B. J. Hazelton, M. F. Morales +46
Antenna layout is an important design consideration for radio interferometers because it determines the quality of the snapshot point spread function (PSF, or array beam). This is…
High Resolution Rapid Response observations of compact radio sources with the Ceduna Hobart Interferometer (CHI)
Jay M. Blanchard, James E. J. Lovell, Roopesh Ojha +3
Context. Frequent, simultaneous observations across the electromagnetic spectrum are essential to the study of a range of astrophysical phenomena including Active Galactic Nuclei.…