These are pictures of the equipment used in the antenna gain
calibration project carried out by Jim Gibson and Jack Welch of UC
Berkeley in September, 2000. The idea is to use a 5.5x7.5 cm
rectangular horn of known gain mounted on the side of one of the HCRO 6m
antennas (Antenna 1), and to switch between this horn and the main
antenna. The absolute gain of Antenna 1 can then be measured by making
interferometric measurememts of a strong source while switching. Once
the antenna gain is determined, it can be used to establish the absolute
flux of Jupiter. The aim of the project is to determine the antenna gains
to an accuracy of ~1%, and then to measure the flux density of primary
flux calibrators (mainly planets) to this accuracy.
Click on the thumbnail to see the full picture.


