CaltechAUTHORS
  A Caltech Library Service

A unique wide band receiver, warm electronics, for the FAST telescope

Smith, Stephen and Weinreb, Sander (2016) A unique wide band receiver, warm electronics, for the FAST telescope. In: Progress in Electromagnetic Research Symposium (PIERS). IEEE , Piscataway, NJ, p. 1666. ISBN 978-1-5090-6093-1. http://resolver.caltech.edu/CaltechAUTHORS:20180524-143529944

Full text is not posted in this repository. Consult Related URLs below.

Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:20180524-143529944

Abstract

A unique wide band receiver for radio astronomy has been designed and constructed. Receivers used for radio astronomy consist of two parts, the front end cold electronics and the back end warm electronics. While the cold electronics provides for a low noise amplifier and receiver calibrations, the warm electronics provides analog signal processing that shapes and filters the signals before digitizing. The following describes the unique features of the warm electronics receiver built by Caltech for installation on China's Five hundred meter Aperture Spherical Telescope (FAST).


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1109/PIERS.2016.7734751DOIArticle
Additional Information:© 2016 IEEE.
Record Number:CaltechAUTHORS:20180524-143529944
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20180524-143529944
Official Citation:S. Smith and S. Weinreb, "A unique wide band receiver, warm electronics, for the FAST telescope," 2016 Progress in Electromagnetic Research Symposium (PIERS), Shanghai, 2016, pp. 1666-1666. doi: 10.1109/PIERS.2016.7734751
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:86594
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:24 May 2018 22:00
Last Modified:24 May 2018 22:00

Repository Staff Only: item control page