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SUMMARY:The future of 21cm intensity mapping: New paradigm\, or not worth 
 the trouble? - Phil Bull
DTSTART:20181119T130000Z
DTEND:20181119T140000Z
UID:TALK111952@talks.cam.ac.uk
CONTACT:Tobias Baldauf
DESCRIPTION:21cm intensity mapping is a promising method for conducting la
 rge-scale structure surveys over extremely large cosmic volumes\, and out 
 to high redshift. A series of difficult (and interesting!) technical chall
 enges must be solved before its promise can be fully realised\, however. I
  will give an overview of recent progress in building\, calibrating\, and 
 simulating 21cm experiments and the surveys they will conduct\, and weigh 
 the pros and cons of the method compared with simply building larger spect
 roscopic galaxy surveys.
LOCATION:CMS\, Pav. B\, CTC Common Room (B1.19) [Potter Room]
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