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...
Príomhchruthaitheoirí: | 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 |
---|---|
Formáid: | Journal article |
Teanga: | English |
Foilsithe / Cruthaithe: |
Institute of Physics Publishing
2011
|
Míreanna comhchosúla
Míreanna comhchosúla
-
First Season QUIET Observations: Measurements of CMB Polarization Power
Spectra at 43 GHz in the Multipole Range 25 <= ell <= 475
de réir: Collaboration, QUIET, et al.
Foilsithe / Cruthaithe: (2010) -
SECOND SEASON QUIET OBSERVATIONS: MEASUREMENTS OF THE COSMIC MICROWAVE BACKGROUND POLARIZATION POWER SPECTRUM AT 95 GHz
de réir: Araujo, D, et al.
Foilsithe / Cruthaithe: (2012) -
THE Q/U IMAGING EXPERIMENT INSTRUMENT
de réir: Bischoff, C, et al.
Foilsithe / Cruthaithe: (2013) -
Fast and precise map-making for massively multi-detector CMB experiments
de réir: Sutton, D, et al.
Foilsithe / Cruthaithe: (2009) -
The Q/U imaging experiment instrument
de réir: QUIET Collaboration, et al.
Foilsithe / Cruthaithe: (2013)