http://arxiv.org/abs/1609.09376
The primary antenna elements and receivers are two of the most important components in a synthesis telescope. Together they are responsible for locking onto an astronomical source in both direction and frequency, capturing its radiation, and converting it into signals suitable for digitization and correlation. The properties and performance of antennas and receivers can affect the quality of the synthesized images in a number of fundamental ways. In this lecture, their most relevant design and performance parameters are reviewed, with emphasis on the current ALMA and VLA systems. We discuss in detail the shape of the primary beam and the components of aperture efficiency, and we present the basics of holography, pointing, and servo control. On receivers, we outline the use of amplifiers and mixers both in the cryogenic front-end and in the room temperature back-end signal path. The essential properties of precision local oscillators (LOs), phase lock loops (PLLs), and LO modulation techniques are also described. We provide a demonstration of the method used during ALMA observations to measure the receiver and system sensitivity as a function of frequency. Finally, we offer a brief derivation and numerical simulation of the radiometer equation.
T. Hunter and P. Napier
Fri, 30 Sep 16
19/75
Comments: 31 pages, 13 figures, 153 references; to appear in the Proceedings of the 2014 Synthesis Imaging Workshop held in Socorro, NM on May 13-20, 2014
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