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Fig. 3


Signal-to-noise ratio and elevation angle comparison between 25 m Ur, 25 m On, and 15 m Ht radio telescopes from 4:00–7:30 UTC on December 29, 2013 (TX: DSS-63). Left panel shows that although Ht (in pink) has a lower collecting area, it achieves higher S/N levels than Ur (in blue) and similar S/N levels than On (in green). Right panel shows the elevation angle of each antenna during the same time period from which the correlation with the S/N levels of each station is evident.

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