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dc.contributor.author Lawrence, C. R. en_US
dc.date.accessioned 2004-09-17T18:13:19Z
dc.date.available 2004-09-17T18:13:19Z
dc.date.issued 2002-08-24 en_US
dc.identifier.citation IR Space Telescopes and Instruments en_US
dc.identifier.citation Waikoloa, HI, USA en_US
dc.identifier.clearanceno 02-2189 en_US
dc.identifier.uri http://hdl.handle.net/2014/10076
dc.description.abstract Planck, scheduled for launch in 2007, will be the third space mission to observe the cosmic microwave background (CMB). Two cryogenic instruments and an off-axis telescope will provide an unprecedented combination of sensitivity, angular resolution, and frequency coverage. Planck is designed to measure the temperature anisotropies of the CMB to limits set not by the instruments, but rather by the Universe itself. In addition, it will measure the E-type polarization of the CMB, and provide all-sky surveys at nine frequencies between 30 and 857GHz. en_US
dc.format.extent 3583639 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other cosmic microwave background all-sky surveys cryogenics infrared telescopes radiometers bolometers en_US
dc.title The Planck Mission en_US


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