DSN Transient Observatory-Reference-Cited by-同舟云学术

DSN Transient Observatory

Published:2016-12 Issue:04 Volume:05 Page:1641012
ISSN:2251-1717
Container-title:Journal of Astronomical Instrumentation
language:en
Short-container-title:J. Astron. Instrum.

Author:

Kuiper T. B. H.¹,Monroe R. M.¹,White L. A.¹,Miro C. Garcia²,Levin S. M.¹,Majid W. A.¹,Soriano M.¹

Affiliation:

1. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109, USA

2. NASA Madrid Deep Space Comm. Complex, INTA/ISDEFE, Madrid, Spain

Abstract

The Deep Space Network (DSN) Transient Observatory (DTO) is a signal processing facility that can monitor up to four DSN downlink bands for astronomically interesting signals. The monitoring is done commensally with reception of deep space mission telemetry. The initial signal processing is done with two CASPER a ROACH1 boards, each handling one or two baseband signals. Each ROACH1 has a 10 GBe interface with a GPU-equipped Debian Linux workstation for additional processing. The initial science programs include monitoring Mars for electrostatic discharges, radio spectral lines, searches for fast radio bursts and pulsars and SETI. The facility will be available to the scientific community through a peer review process.

Funder

Jet Propulsion Laboratory

Publisher

World Scientific Pub Co Pte Lt

Subject

Astronomy and Astrophysics,Instrumentation

Link

https://www.worldscientific.com/doi/pdf/10.1142/S2251171716410129

Reference11 articles.

1. Evidence for the depletion of ammonia in the Uranus atmosphere

2. The Search for Extraterrestrial Intelligence in Earth's Solar Transit Zone

3. DSS-28: a novel wide bandwidth radio telescope devoted to educational outreach

Cited by 1 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. The 17–27 GHz Dual Horn Receiver on the NASA 70 m Canberra Antenna;Journal of Astronomical Instrumentation;2019-11-13