First season quiet observations: Measurements of cosmic microwave background polarization power spectra at 43 GHz in the multipole range 25 ≤ ℓ ≤ 475
The Q/U Imaging ExperimenT (QUIET) employs coherent receivers at 43GHz and 94GHz, operating on the Chajnantor plateau in the Atacama Desert in Chile, to measure the anisotropy in the polarization of the cosmic microwave background (CMB). QUIET primarily targets the B modes from primordial gravitatio...
المؤلفون الرئيسيون: | Bischoff, C, Brizius, A, Buder, I, Chinone, Y, Cleary, K, Dumoulin, R, Kusaka, A, Monsalve, R, Næss, S, Newburgh, L, Reeves, R, Smith, K, Wehus, I, Zuntz, J, Zwart, J, Bronfman, L, Bustos, R, Church, SE, Dickinson, C, Eriksen, H, Ferreira, P, Gaier, T, Gundersen, J, Hasegawa, M, Hazumi, M |
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التنسيق: | Journal article |
اللغة: | English |
منشور في: |
Institute of Physics Publishing
2011
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مواد مشابهة
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First Season QUIET Observations: Measurements of CMB Polarization Power
Spectra at 43 GHz in the Multipole Range 25 <= ell <= 475
حسب: Collaboration, QUIET, وآخرون
منشور في: (2010) -
SECOND SEASON QUIET OBSERVATIONS: MEASUREMENTS OF THE COSMIC MICROWAVE BACKGROUND POLARIZATION POWER SPECTRUM AT 95 GHz
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منشور في: (2012) -
THE Q/U IMAGING EXPERIMENT INSTRUMENT
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منشور في: (2013) -
Fast and precise map-making for massively multi-detector CMB experiments
حسب: Sutton, D, وآخرون
منشور في: (2009) -
The Q/U imaging experiment instrument
حسب: QUIET Collaboration, وآخرون
منشور في: (2013)