scholarly journals Australian East?West Baseline Interferometer Observations at 2·3 GHz

1972 ◽  
Vol 25 (4) ◽  
pp. 461
Author(s):  
JS Gubbay ◽  
AJ Legg ◽  
DS Robertson

In 1967 the two Australian stations of the NASA?JPL Deep Space Network, DSS41 at Island Lagoon near Woomera and DSS42 at Tidbinbilla near Canberra, were operated as an intensity interferometer (Gubbay and Robertson 1967). At the operating frequency of 2�3 GHz, the baseline is 9 � 106 wavelengths in extent and runs 15� south of east from DSS41. In the work reported by Gubbay and Robertson, the flux from the radio source 3C 273 was found to be partially correlated. This note concerns later measurement over the same baseline using an intermediate interferometer (Clark 1968).

Author(s):  
Edwin Goh ◽  
Hamsa Shwetha Venkataram ◽  
Mark Hoffmann ◽  
Mark D. Johnston ◽  
Brian Wilson

IEEE Access ◽  
2021 ◽  
Vol 9 ◽  
pp. 39985-39994
Author(s):  
Alex Sabol ◽  
Ryan Alimo ◽  
Farhad Kamangar ◽  
Ramtin Madani

2012 ◽  
Vol 60 (7) ◽  
pp. 3481-3484
Author(s):  
V. V. Srinivasan ◽  
C. Kumar ◽  
D. Bhatnagar ◽  
V. K. Lakshmeesha ◽  
S. Pal

Author(s):  
Bruce E. MacNeal ◽  
Douglas S. Abraham ◽  
Rolf C. Hastrup ◽  
Janet P. Wu ◽  
Richard J. Machuzak ◽  
...  

2006 ◽  
Vol 649 (1) ◽  
pp. 561-561 ◽  
Author(s):  
P. T. Kondratko ◽  
L. J. Greenhill ◽  
J. M. Moran ◽  
J. E. J. Lovell ◽  
T. B. H. Kuiper ◽  
...  

2015 ◽  
Vol 11 (A29B) ◽  
pp. 367-369
Author(s):  
Lawrence Teitelbaum ◽  
Walid Majid ◽  
Manuel M. Franco ◽  
Daniel J. Hoppe ◽  
Shinji Horiuchi ◽  
...  

AbstractMillisecond pulsars (MSPs) are a class of radio pulsars with extremely stable rotation. Their excellent timing stability can be used to study a wide variety of astrophysical phenomena. In particular, a large sample of these pulsars can be used to detect low-frequency gravitational waves. We have developed a precision pulsar timing backend for the NASA Deep Space Network (DSN), which will allow the use of short gaps in tracking schedules to time pulses from an ensemble of MSPs. The DSN operates clusters of large dish antennas (up to 70-m in diameter), located roughly equidistant around the Earth, for communication and tracking of deep-space spacecraft. The backend system will be capable of removing entirely the dispersive effects of propagation of radio waves through the interstellar medium in real-time. We will describe our development work, initial results, and prospects for future observations over the next few years.


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