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...
Prif Awduron: | Sutton, D, Zuntz, J, Ferreira, P, Brown, M, Eriksen, H, Johnson, B, Kusaka, A, Naess, S, Wehus, I |
---|---|
Fformat: | Journal article |
Iaith: | English |
Cyhoeddwyd: |
2009
|
Eitemau Tebyg
-
A CMB Gibbs sampler for localized secondary anisotropies
gan: Bull, P, et al.
Cyhoeddwyd: (2014) -
Map-making in small field modulated CMB polarisation experiments:
approximating the maximum-likelihood method
gan: Sutton, D, et al.
Cyhoeddwyd: (2009) -
What the small angle CMB really tells us about the curvature of the
Universe
gan: Clifton, T, et al.
Cyhoeddwyd: (2009) -
First Season QUIET Observations: Measurements of CMB Polarization Power
Spectra at 43 GHz in the Multipole Range 25 <= ell <= 475
gan: Collaboration, QUIET, et al.
Cyhoeddwyd: (2010) -
Noise estimation in CMB time-streams and fast map-making. Application to the BOOMERanG98 data
gan: Prunet, S, et al.
Cyhoeddwyd: (2001)