This collaborative program will conduct a multi-year project to make precise measurements of the large scale structure of the universe using recently developed 21 cm intensity mapping techniques. The program will create spectral maps of 500 square degrees, spanning the frequency range 700 to 900 MHz (0.58 < z < 1). The principal goal is to measure the baryon acoustic oscillation feature at these redshifts in an innovative program which is complementary to, and competitive with, optical galaxy surveys. The acoustic scale provides a standard ruler which measures the Universe's expansion, providing an observational handle on Dark Energy.

Broader impacts of the work include training of graduate student, and outreach to the public via a planetarium show called "The Hydrogen Sky" produced in English, French and Chinese, and distributed worldwide. Additional outreach activities include tours of the night sky through the Universe in the Park program in Wisconsin and teaching electronics to under-represented groups through CMU's Summer Academy for Math and Science.

Agency
National Science Foundation (NSF)
Institute
Division of Astronomical Sciences (AST)
Application #
1211781
Program Officer
joan wrobel
Project Start
Project End
Budget Start
2012-08-01
Budget End
2015-12-31
Support Year
Fiscal Year
2012
Total Cost
$288,837
Indirect Cost
Name
University of Wisconsin Madison
Department
Type
DUNS #
City
Madison
State
WI
Country
United States
Zip Code
53715