Measured between March - May 2015

Reciver
Frequency
[GHz]
HPBW
[arcsec]
Main Beam
Effic [%]
Aperture
Effic [%]
Calib.
source
EL comments

S100 86 19.0+-0.4 43+-1 35+-1 Saturn 23.1 - 28.7
110 17.1+-0.4 38+-1 23+-1 Saturn 26.8 - 29.4
115 16.7+-0.3 36+-2 21+-1 Saturn 21.3 - 24.6

TZ1(H) 86 20.4+-0.4 49+-2 34+-1 Saturn 24.6 - 34.4
110 16.6+-0.4 41+-3 26+-2 Saturn 35.0 - 35.1
115 15.1+-0.3 39+-3 27+-2 Saturn 35.0 - 34.3

TZ1(V) 86 20.4+-0.4 48+-2 34+-2 Saturn 24.6 - 34.4
110 16.6+-0.4 42+-3 27+-2 Saturn 35.0 - 35.1
115 15.6+-0.3 40+-2 27+-2 Saturn 35.0 - 34.3

TZ2(H) 86 19.5+-0.5 45+-1 34+-1 Saturn 24.6 - 27.7
110 17.0+-0.4 39+-3 24+-2 Saturn 34.6 - 33.5
115 16.0+-0.4 38+-3 23+-2 Saturn 32.7 - 30.8

TZ2(V) 86 19.6+-0.4 44+-1 33+-1 Saturn 24.6 - 27.7
110 16.9+-0.4 41+-3 25+-2 Saturn 34.6 - 33.5
115 16.3+-0.4 39+-3 23+-2 Saturn 32.7 - 30.8

T70(H) 75 21.7+-0.4 48+-2 38+-1 Saturn 33.6 - 34.6
86 20.7+-0.5 45+-1 30+-1 Saturn 26.2 - 29.0

T70(V) 75 21.6+-0.4 48+-2 39+-1 Saturn 33.6 - 34.6
86 20.7+-0.5 46+-1 31+-1 Saturn 26.2 - 29.0

FOREST 115 16.0+-0.4 39+-3 24+-2 Saturn 18.6 - 25.6 an average of Beam 1H and 1V

The error of the efficiencies is mainly due to uncertainty of brightness temperature of the planet.

  1. Brightness Temperatures (Tb) of the Source (We used temperatures compiled by Shibata 1990)
    Saturn
  2. Diameter of the Planet
    The value is taken from the ASTRONOMICAL ALMANAC.
  3. References

2015-05-26