DiFX: a software correlator for very long baseline interferometry using multiprocessor computing environments
We describe the development of an FX‐style correlator for very long baseline interferometry
(VLBI), implemented in software and intended to run in multiprocessor computing …
(VLBI), implemented in software and intended to run in multiprocessor computing …
DiFX-2: a more flexible, efficient, robust, and powerful software correlator
AT Deller, WF Brisken, CJ Phillips… - Publications of the …, 2011 - iopscience.iop.org
Software correlation, where a correlation algorithm written in a high-level language such as
C++ is run on commodity computer hardware, has become increasingly attractive for small …
C++ is run on commodity computer hardware, has become increasingly attractive for small …
The SFXC software correlator for very long baseline interferometry: algorithms and implementation
A Keimpema, MM Kettenis, SV Pogrebenko… - Experimental …, 2015 - Springer
In this paper a description is given of the SFXC software correlator, developed and
maintained at the Joint Institute for VLBI in Europe (JIVE). The software is designed to run on …
maintained at the Joint Institute for VLBI in Europe (JIVE). The software is designed to run on …
SWARM: a 32 GHz correlator and VLBI beamformer for the submillimeter array
RA Primiani, KH Young, A Young, N Patel… - Journal of …, 2016 - World Scientific
A 32 GHz bandwidth VLBI capable correlator and phased array has been designed and
deployed at the Smithsonian Astrophysical Observatory's Submillimeter Array (SMA). The …
deployed at the Smithsonian Astrophysical Observatory's Submillimeter Array (SMA). The …
A scalable correlator architecture based on modular FPGA hardware, reuseable gateware, and data packetization
ABSTRACT A new generation of radio telescopes is achieving unprecedented levels of
sensitivity and resolution, as well as increased agility and field of view, by employing high …
sensitivity and resolution, as well as increased agility and field of view, by employing high …
[HTML][HTML] The IRAM interferometer on Plateau de Bure
S Guilloteau, J Delannoy, D Downes… - … (ISSN 0004-6361) …, 1992 - adsabs.harvard.edu
The IRAM interferometer on Plateau de Bure has three 15 m diameter antennas presently
equipped with low noise receivers for the 80-115 GHz band. Baselines extend 160m north …
equipped with low noise receivers for the 80-115 GHz band. Baselines extend 160m north …
The shapes of cross-correlation interferometers
E Keto - The Astrophysical Journal, 1997 - iopscience.iop.org
Cross-correlation imaging interferometers designed in the shape of a curve of constant width
offer better sensitivity and imaging characteristics than other designs because they sample …
offer better sensitivity and imaging characteristics than other designs because they sample …
A digital correlator upgrade for the Arcminute MicroKelvin Imager
J Hickish, N Razavi-Ghods, YC Perrott… - Monthly Notices of …, 2018 - academic.oup.com
Abstract The Arcminute Microkelvin Imager (AMI) telescopes located at the Mullard Radio
Astronomy Observatory near Cambridge have been significantly enhanced by the …
Astronomy Observatory near Cambridge have been significantly enhanced by the …
Long-baseline optical and infrared stellar interferometry
M Shao, MM Colavita - Annual Review of Astronomy and …, 1992 - annualreviews.org
The field of modern long-baseline optical 1 stel1ar interferometry has made enormous
strides since the first independent-element Michelson stellar interferometer in 1974 …
strides since the first independent-element Michelson stellar interferometer in 1974 …
The ALMA Interferometric Pipeline Heuristics
We describe the calibration and imaging heuristics developed and deployed in the Atacama
Large Millimeter/submillimeter Array (ALMA) interferometric data processing pipeline, as of …
Large Millimeter/submillimeter Array (ALMA) interferometric data processing pipeline, as of …