Niemack, M. D., Ade, Peter A. R.  ORCID: https://orcid.org/0000-0002-5127-0401, Aguirre, J., Barrientos, F., Beall, J. A., Bond, J. R., Britton, J., Cho, H. M., Das, S., Devlin, M. J., Dicker, S., Dunkley, J., Dünner, R., Fowler, J. W., Hajian, A., Halpern, M., Hasselfield, M., Hilton, G. C., Hilton, M., Hubmayr, J., Hughes, J. P., Infante, L., Irwin, K. D., Jarosik, N., Klein, J., Kosowsky, A., Marriage, T. A., McMahon, J., Menanteau, F., Moodley, K., Nibarger, J. P., Nolta, M. R., Page, L. A., Partridge, B., Reese, E. D., Sievers, J., Spergel, D. N., Staggs, S. T., Thornton, R., Tucker, Carole Elizabeth  ORCID: https://orcid.org/0000-0002-1851-3918, Wollack, E. and Yoon, K. W.
      2010.
      
      ACTPol: a polarization-sensitive receiver for the Atacama Cosmology Telescope.
      Presented at: Millimeter, submillimeter, and far-infrared detectors and instrumentation for astronomy V,
      San Diego, CA, USA,
      29 June-2 July 2010.
      
      Proceedings of the SPIE conference on Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V  held in San Diego CA 29 June 2010.
      
      Proceedings of SPIE
      
       
      
        (7741)
      
      Bellingham, WA: 
      SPIE,
      77411S.
      10.1117/12.857464
    
  
  
       
       
     
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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.
| Item Type: | Conference or Workshop Item (Paper) | 
|---|---|
| Date Type: | Publication | 
| Status: | Published | 
| Schools: | Schools > Physics and Astronomy | 
| Subjects: | Q Science > QB Astronomy | 
| Uncontrolled Keywords: | Galaxy groups and clusters; Helium; Polarization; Receivers; Telescopes | 
| Publisher: | SPIE | 
| ISBN: | 9780819482310 | 
| ISSN: | 0277-786X | 
| Last Modified: | 20 Oct 2022 09:47 | 
| URI: | https://orca.cardiff.ac.uk/id/eprint/33127 | 
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