Linear Polarization Measurements of Radio Sources at 18-CM Wavelength.

1964 ◽  
Vol 139 ◽  
pp. 758 ◽  
Author(s):  
D. Morris ◽  
V. Radhakrishnan ◽  
G. A. Seielstad
1999 ◽  
Vol 135 (3) ◽  
pp. 571-577 ◽  
Author(s):  
E. L.H. Zukowski ◽  
P. P. Kronberg ◽  
T. Forkert ◽  
R. Wielebinski

2004 ◽  
Vol 218 ◽  
pp. 135-136
Author(s):  
J. L. Han ◽  
R. N. Manchester ◽  
A. G. Lyne ◽  
G. J. Qiao

Pulsars are among the most highly polarized sources in the universe. The NVSS has cataloged 2 million radio sources with linear polarization measurements, from which we have selected 253 sources, with polarization percentage greater than 25%, as targets for pulsar searches. We believe that such a sample is not biased by selection effects against ultra-short spin or orbit periods. Using the Parkes 64-m telescope, we conducted searches with sample intervals of 50 μs and 80 μs, sensitive to submillisecond pulsars. Unfortunately we did not find any new pulsars.


1969 ◽  
Vol 19 (10) ◽  
pp. 1281-1289 ◽  
Author(s):  
J. Honzátko ◽  
J. Kajfosz

2015 ◽  
Vol 806 (1) ◽  
pp. 112 ◽  
Author(s):  
K. M. Huffenberger ◽  
D. Araujo ◽  
C. Bischoff ◽  
I. Buder ◽  
Y. Chinone ◽  
...  

1967 ◽  
Vol 20 (4) ◽  
pp. 407 ◽  
Author(s):  
RX McGee ◽  
FF Gardner ◽  
BJ Robinson

A survey for the hydroxyl line radiation has been made in the directions of 30 radio sources (most of them thermal) with the 210 ft telescope of beamwidth 12'� 2 and the multichannel line receiver of bandwidths 10 and 37 kHz. The line at frequency 1665�401 MHz was observed for all sources and the other three lines at 1612, 1667, and 1720 MHz were observed for 10 of the more important sources. The latter were investigated for circular and linear polarization.


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