CASM-256 is a new 256-antenna radio array at Owens Valley that uses real-time digital beamforming to search for fast radio bursts and galactic transients over a huge sky area.
https://download.tek.com/datasheet/ RSA7100B Datasheet-EN US 37W-61645-5.pdf The CHIME Collaboration, Amiri, M., Bandura, K., et al
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A 2 GHz bandwidth RFI monitor was commissioned at DRAO for transient detection and radio environment characterization, with a new method derived for calculating gain drift effects on integrated data.
The primary beam of the Tianlai array is shown to be factorizable into independent E-W and N-S components, with E-W profiles measured from the Sun and N-S obtained via sky model fitting.
citing papers explorer
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The 256-antenna Coherent All-Sky Monitor
CASM-256 is a new 256-antenna radio array at Owens Valley that uses real-time digital beamforming to search for fast radio bursts and galactic transients over a huge sky area.
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Wideband RFI Monitor Requirements, Design, and Commissioning at DRAO
A 2 GHz bandwidth RFI monitor was commissioned at DRAO for transient detection and radio environment characterization, with a new method derived for calculating gain drift effects on integrated data.
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Measuring Tianlai's primary beam using sky model
The primary beam of the Tianlai array is shown to be factorizable into independent E-W and N-S components, with E-W profiles measured from the Sun and N-S obtained via sky model fitting.