Fast and precise map-making for massively multi-detector CMB experiments
Future cosmic microwave background (CMB) polarisation experiments aim to measure an unprecedentedly small signal - the primordial gravity wave component of the polarisation field B-mode. To achieve this, they will analyse huge datasets, involving years worth of time-ordered data (TOD) from massively...
Главные авторы: | Sutton, D, Zuntz, J, Ferreira, P, Brown, M, Eriksen, H, Johnson, B, Kusaka, A, Naess, S, Wehus, I |
---|---|
Формат: | Journal article |
Язык: | English |
Опубликовано: |
2009
|
Схожие документы
-
A CMB Gibbs sampler for localized secondary anisotropies
по: Bull, P, и др.
Опубликовано: (2014) -
Map-making in small field modulated CMB polarisation experiments:
approximating the maximum-likelihood method
по: Sutton, D, и др.
Опубликовано: (2009) -
What the small angle CMB really tells us about the curvature of the
Universe
по: Clifton, T, и др.
Опубликовано: (2009) -
First Season QUIET Observations: Measurements of CMB Polarization Power
Spectra at 43 GHz in the Multipole Range 25 <= ell <= 475
по: Collaboration, QUIET, и др.
Опубликовано: (2010) -
Noise estimation in CMB time-streams and fast map-making. Application to the BOOMERanG98 data
по: Prunet, S, и др.
Опубликовано: (2001)