Sampled over l range of 160-170 or .25-1.15 degrees
Mount includes rotation of aperture plane along line of sight
Slide 15
Wilkinson Microwave Anisotropy Probe
Launched 2001 to map CMB radiation with higher resolution, sensitivity, and accuracy than COBE
http://map.gsfc.nasa.gov/m_mm/sg_earlyuniv.html
Slide 16
http://cosmology.berkeley.edu/group/cmb/image/maxima_map.gif
Millimeter Anisotropy eXperiment Imaging Array
angular power spectrum with a unique set of "acoustic peaks" between the angular scales of 2 degrees and 10'
can provide precise estimates of cosmological constants
Slide 17
Part of the first European mission to study the “birth” of the Universe
Construction to be finished in 2005
Launched in the same rocket with Herschel in 2007
Will observe the Cosmic Microwave Background (left over radiation from the Big Bang)
Slide 18
PLANK
http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=34875
http://www.dsri.dk/planck/
http://spaceflightnow.com/news/n0006/13planck/
Slide 19
An 8-meter precision submillimeter-wave telescope
Distant galaxy clusters through detection of their Sunyaev-Zel’dovich effect (SZE)
Dark Energy will be observed in great detail
1,000 Bolometers (heat detectors) measure the temperature differences up to 10 millionths of a degree
Mapping large areas of the sky will be very beneficial to modern astronomers
Slide 20
The South Pole Telescope
http://astro.uchicago.edu/spt/
http://www.spaceflightnow.com/news/n0301/29polescope/
Slide 21
Will be built as an Inferometer, due to the changing weather patterns and the basic noise of the instruments that are experienced
Uses radio signals received by each antenna
Construction finished in 1999 now in Tenerife
http://www.mrao.cam.ac.uk/telescopes/vsa/
Slide 22
Very Small Array
www.jb.man.ac.uk/tech/ technology/array-top.jpg
www.mrao.cam.ac.uk/ telescopes/vsa/ext-array.jpg
www.mpifr-bonn.mpg.de/ ./ teleskope/vsa_art1.jpg
Slide 23