... Modelling the infrared and sub-millimetre sky fluxes and atmospheric transmission at the SouthPole, and examining their sensitivity to temperature, water vapour content and aerosol level, we reach the following conclusions: . ...
... Bill Holzapfel (Berkeley) - SZ effect in galaxy clusters ---> OVRO/BIMA observing experience; SouthPole projects =========================================================================== Tony Wong twong_at_atnf.<!--nospam-->csiro.au CSIRO Australia ...
... The primary purpose of the observing run was obtaining photometry of the South Galactic Pole (SGP) so observations of Neptune were restricted to an hour each night when the SGP was low in the sky. ...
... interferometer operating in the frequency band 26-36 GHz (the DASI project) is expected to become operational at the Southpole around November 1999; this experiment expects to measure the degree scale CMB anisotropy with a sensitivity of about 10 micro ...
... Figure 1 shows the same region of sky as viewed by HIPASS and B85. s of a 2400 deg2 region centred upon the South Celestial Pole, including The velocity range encompassed here is vlsr = 85 - 400 km s-1 . ...
... To detect and map the vertical field of the Galaxy, we have carried out a survey of Faraday rotation toward 500 polarized extragalactic sources behind each of the North and South Galactic Poles, carried out with the WSRT and ATCA, respectively. ...