Abstract
The six-meter Atacama Cosmology Telescope (ACT) in Chile was built to measure the cosmic microwave background (CMB) at arcminute angular scales. We are building a new polarization sensitive receiver for ACT (ACTPol). ACTPol will characterize the gravitational lensing of the CMB and aims to constrain the sum of the neutrino masses with ~ 0.05 eV precision, the running of the spectral index of inflation-induced fluctuations, and the primordial helium abundance to better than 1 %. Our observing fields will overlap with the SDSS BOSS survey at optical wavelengths, enabling a variety of cross-correlation science, including studies of the growth of cosmic structure from Sunyaev-Zel'dovich observations of clusters of galaxies as well as independent constraints on the sum of the neutrino masses. We describe the science objectives and the initial receiver design.
Original language | English (US) |
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Title of host publication | Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V |
DOIs | |
State | Published - 2010 |
Event | Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V - San Diego, CA, United States Duration: Jun 29 2010 → Jul 2 2010 |
Publication series
Name | Proceedings of SPIE - The International Society for Optical Engineering |
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Volume | 7741 |
ISSN (Print) | 0277-786X |
Other
Other | Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V |
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Country/Territory | United States |
City | San Diego, CA |
Period | 6/29/10 → 7/2/10 |
All Science Journal Classification (ASJC) codes
- Electronic, Optical and Magnetic Materials
- Condensed Matter Physics
- Computer Science Applications
- Applied Mathematics
- Electrical and Electronic Engineering
Keywords
- B-modes
- Cosmic Microwave Background
- Cryogenics
- Gravitational Lensing
- Neutrino Mass
- Optical Design
- Polarization
- Transition-Edge-Sensor Detector Arrays