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A Decade of Developing Radio-Astronomy Instrumentation using CASPER Open-Source Technology

TLDR
The ongoing state of software development is described, as CASPER looks to support a broader range of programming environments and hardware and ensure compatibility with the latest vendor tools.
Abstract
The Collaboration for Astronomy Signal Processing and Electronics Research (CASPER) has been working for a decade to reduce the time and cost of designing, building and deploying new digital radio-astronomy instruments. Today, CASPER open-source technology powers over 45 scientific instruments worldwide, and is used by scientists and engineers at dozens of academic institutions. In this paper we catalog the current offerings of the CASPER collaboration, and instruments past and present built by CASPER users and developers. We describe the ongoing state of software development, as CASPER looks to support a broader range of programming environments and hardware and ensure compatibility with the latest vendor tools.

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Probing Radio Intensity at High-Z from Marion: 2017 Instrument

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References
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A two-solar-mass neutron star measured using Shapiro delay

TL;DR: Radio timing observations of the binary millisecond pulsar J1614-2230 that show a strong Shapiro delay signature are presented and the pulsar mass is calculated to be (1.97 ± 0.04)M⊙, which rules out almost all currently proposed hyperon or boson condensate equations of state.
Journal ArticleDOI

The five-hundred-meter aperture spherical radio telescope (fast) project

TL;DR: Wang et al. as discussed by the authors proposed the Five Hundred Meter Aperture Spherical Radio Telescope (FAST) to build the largest single-dish radio telescope in the world.
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