The large adaptive reflector: a 200-m diameter wideband centimeter- to meter-wave radio telescope

Author(s):  
Brent Carlson ◽  
Luc Bauwens ◽  
Leonid Belostotski ◽  
Elizabeth Cannon ◽  
Ya-Ying Chang ◽  
...  
Keyword(s):  
2007 ◽  
Vol 378 (3) ◽  
pp. 995-1006 ◽  
Author(s):  
D. Moss ◽  
N. Seymour ◽  
I. M. McHardy ◽  
T. Dwelly ◽  
M. J. Page ◽  
...  
Keyword(s):  

1992 ◽  
Vol 128 ◽  
pp. 193-194
Author(s):  
A. A. Deshpande ◽  
V. Radhakrishnan

AbstractWe report measurement of pulse profiles at 34.5 MHz of 8 pulsars using the Decameter-wave Radio Telescope at Gauribidanur, India. The dispersion measures of these pulsars range from 3 to 35 pc cm–3. None of the pulsars show any significant interpulse emission at this frequency which conflicts with earlier claims from 25-MHz observations (Bruck and Ustimenko 1976, Bruck and Ustimenko 1977a, Bruck and Ustimenko 1979). The intrinsic pulse width of PSR 1919+21 at 34.5 MHz appears to be smaller than at higher frequencies. These observations were made during the period 1984-86 and were reported by Deshpande (1987).


2016 ◽  
Vol 26 (s1) ◽  
pp. 346-356 ◽  
Author(s):  
Nandini Gupta ◽  
Geetha Andrew ◽  
Monika R. Jain ◽  
Hari Balakrishna ◽  
Vivek Sanadhya ◽  
...  

1991 ◽  
Vol 9 (1) ◽  
pp. 60-61
Author(s):  
Jing-Sheng Wang

AbstractNew radio and optical telescopes installed in recent years in China are summarised. These include the 2.16-m optical telescope, the solar magnetic field telescope, the Miyun synthesis radio telescope, the 1.26-m infrared telescope (Beijing Astronomical Observatory), the 25-m radio telescope as the first station of China’s VLBI network, the 1.56-m astrometric telescope (Shanghai Observatory), and the 13.7-m millimetre wave radio telescope.


1989 ◽  
Vol 35 (6) ◽  
pp. 342-348 ◽  
Author(s):  
A A Deshpande ◽  
R K Shevgaonkar ◽  
Ch V Sastry

Author(s):  
O.E.H. Rydbeck ◽  
B Ronnang ◽  
B. Hansson ◽  
J. Ellder ◽  
A Hjalmarson ◽  
...  

2002 ◽  
Vol 199 ◽  
pp. 343-344
Author(s):  
N.G. Kantharia ◽  
D. Anish Roshi

A pilot project to observe recombination lines of hydrogen and carbon from Galactic HII regions near 20cm (n = 168) and 49cm (n = 220) using the 30-station correlator at the Giant Metre-wave Radio Telescope was undertaken. The preliminary results from observations of the HII regions W3 and S106 are presented here.


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