Share Email Print
cover

Proceedings Paper

Automated calibration and imaging with the Allen Telescope Array
Author(s): Garrett K. Keating; William C. Barott; Melvyn Wright
Format Member Price Non-Member Price
PDF $17.00 $21.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

Planned instruments such as the Atacama Large Millimeter Array (ALMA), the Large Synoptic Survey Telescope (LSST) and the Square Kilometer Array (SKA) will measure their data in petabytes. Innovative approaches in signal processing, computing hardware, algorithms, and data handling are necessary. The Allen Telescope Array (ATA) is a 42-antenna aperture synthesis array equipped with broadband, dual polarization receivers from 0.5 to 11 GHz. Four independent IF bands feed 4 spectral cross correlators and 3 beamformers. In this paper we describe the automated data processing to handle the high data rate and RFI in close to real time at the ATA.

Paper Details

Date Published: 19 July 2010
PDF: 8 pages
Proc. SPIE 7740, Software and Cyberinfrastructure for Astronomy, 774016 (19 July 2010); doi: 10.1117/12.857928
Show Author Affiliations
Garrett K. Keating, Radio Astronomy Lab., Univ. of California, Berkeley (United States)
William C. Barott, Embry-Riddle Aeronautical Univ. (United States)
Melvyn Wright, Radio Astronomy Lab., Univ. of California, Berkeley (United States)


Published in SPIE Proceedings Vol. 7740:
Software and Cyberinfrastructure for Astronomy
Nicole M. Radziwill; Alan Bridger, Editor(s)

© SPIE. Terms of Use
Back to Top