Measured between December 2012 - April 2013

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

S40 43 39.6+-0.1 76+-5 56+-4 Jupiter 31 - 30
3C279 30 - 31
49 34.2+-0.3 74+-5 56+-4 Jupiter 65 - 68
3C279 34 - 37

S80 86 19.1+-0.1 34+-2 27+-2 Saturn 71 - 69
3C279 41 - 44
110 16.0+-0.2 27+-2 19+-1 Saturn 59 - 55
3C279 27 - 31

S100 86 18.5+-0.1 39+-3 33+-2 Saturn 71 - 69
3C279 41 - 44
110 15.2+-0.2 36+-3* 28+-2 Saturn 59 - 55
3C279 27 - 31
115 15.3+-0.8 27+-2 19+-1 Saturn 47 - 43
3C279 34 - 38

TZ(H) 86 19.2+-0.2 36+-3 28+-2 Saturn 57 - 60
3C279 41 - 60
110 16.1+-0.1 31+-2 21+-2 Saturn 39 - 42
3C279 40 - 43
115 15.4+-0.1 31+-2 19+-2 Saturn 44 - 46
3C279 44 - 46

TZ(V) 86** --- --- --- --- ---
--- ---
110 16.1+-0.1 31+-2 21+-2 Saturn 39 - 42
3C279 40 - 43
115 15.4+-0.1 31+-2 19+-2 Saturn 44 - 46
3C279 44 - 46

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 Jupiter
  2. Diameter of the Planet
    The value is taken from the ASTRONOMICAL ALMANAC.
    For example, the diameter of Saturn, 17.791 (arcsec), was used for the measurements of TZ1 (April 1, 2013).
  3. References

2013-05-30