Interferometers and Aperture Synthesis

Author(s):  
Thomas L. Wilson ◽  
Kristen Rohlfs ◽  
Susanne Hüttemeister
Keyword(s):  
1974 ◽  
Vol 114 (12) ◽  
pp. 655 ◽  
Author(s):  
V.N. Sintsov ◽  
A.F. Zapryagaev
Keyword(s):  

2020 ◽  
Vol 79 (15) ◽  
pp. 1327-1347
Author(s):  
M. V. Nechyporuk ◽  
V. V. Pavlikov ◽  
A. D. Sobkolov ◽  
E. O. Tserne ◽  
Valerii K. Volosyuk ◽  
...  

1971 ◽  
Vol 15 ◽  
pp. 173-175 ◽  
Author(s):  
L. L. E. Braes ◽  
G. K. Miley

Dr. KELLOGG has just described some exciting new observations of X-ray sources made with the UHURU satellite. We shall now move some nine orders of magnitude in wavelength to the opposite end of the electromagnetic spectrum and report measurements of weak radio emission from some of the objects he mentioned. For the detection of weak sources most radio telescopes are not noise limited, but are confusion limited by their low resolution. The aperture synthesis technique minimizes this problem because it enables one to pinpoint the position of weak sources to the order of one second of arc.


1986 ◽  
Vol 7 ◽  
pp. 345-353
Author(s):  
J V Wall ◽  
C R Benn ◽  
G Grueff ◽  
M Vigotti

AbstractRadio, optical and infrared data are combined to study the nature of mJy-sources found in the 5C12 aperture-synthesis survey. The optical counterparts are QSOs, giant elliptical galaxies of the 3CR type, and blue galaxies. We find that the blue galaxies are a mixed group; the suggestion of a new blue population of evolving spirals at mJy levels is not supported by our data.


2012 ◽  
Vol 9 (6) ◽  
pp. 1021-1025 ◽  
Author(s):  
Guanli Yi ◽  
Fei Hu ◽  
Rong Jin ◽  
Da Li ◽  
Hong Yang ◽  
...  

2003 ◽  
Vol 55 (1) ◽  
pp. 103-119 ◽  
Author(s):  
Kotaro Kohno ◽  
Baltasar Vila-Vilaró ◽  
Seiichi Sakamoto ◽  
Ryohei Kawabe ◽  
Sumio Ishizuki ◽  
...  

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