1. Design and Development of a Wide-Field Fully Cryogenic Phased Array Feed for Arecibo
- Author
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Karl F. Warnick, German Cortes-Medellin, Donald B. Campbell, Stephen C. Parshley, Jakob W. Kunzler, M. Burnett, Amit Vishwas, D. Anish Roshi, Brian D. Jeffs, Erich Nygaard, and Phil Perillat
- Subjects
Noise temperature ,Phased array feed ,010308 nuclear & particles physics ,business.industry ,Phased array ,Computer science ,020206 networking & telecommunications ,02 engineering and technology ,01 natural sciences ,Wide field ,Instantaneous bandwidth ,Dual polarized ,Radio telescope ,Optics ,0103 physical sciences ,0202 electrical engineering, electronic engineering, information engineering ,business - Abstract
Brigham Young University (BYU), in collaboration with Cornell University, is developing the Advanced Cryogenic L-band Phased Array Camera for Arecibo (ALPACA) as a user provided facility instrument on the Arecibo 305 m radio telescope. This instrument will consist of a fully cryogenic 69-element phased array feed (PAF) and real-time digital beamformer back end capable of producing 40 simultaneous dual polarized beams with approximately 305 MHz of instantaneous bandwidth at 1.4 GHz. The target design goal is to operate with a system noise temperature of 25 K. We report on simulation results and a preliminary overview of the design and progress of the instrument’s development.
- Published
- 2020
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