A MULTI-LEVEL SOLVER FOR GAUSSIAN CONSTRAINED COSMIC MICROWAVE BACKGROUND REALIZATIONS

被引:13
作者
Seljebotn, D. S. [1 ]
Mardal, K. -A. [2 ,3 ]
Jewell, J. B. [4 ]
Eriksen, H. K. [1 ]
Bull, P. [1 ]
机构
[1] Univ Oslo, Inst Theoret Astrophys, NO-0315 Oslo, Norway
[2] Univ Oslo, Dept Informat, NO-0316 Oslo, Norway
[3] Simula Res Lab, Ctr Biomed Comp, NO-1325 Lysaker, Norway
[4] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
基金
欧洲研究理事会;
关键词
cosmic background radiation; methods: numerical; methods: statistical; POWER SPECTRUM; BAYESIAN-ANALYSIS; ALGORITHMS; MAPS;
D O I
10.1088/0067-0049/210/2/24
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a multi-level solver for drawing constrained Gaussian realizations or finding the maximum likelihood estimate of the cosmic microwave background sky, given noisy sky maps with partial sky coverage. The method converges substantially faster than existing Conjugate Gradient (CG) methods for the same problem. For instance, for the 143 GHz Planck frequency channel, only three multi-level W-cycles result in an absolute error smaller than 1 mu K in any pixel. Using 16 CPU cores, this translates to a computational expense of 6 minutes wall time per realization, plus 8 minutes wall time for a power-spectrum-dependent precomputation. Each additional W-cycle reduces the error by more than an order of magnitude, at an additional computational cost of 2 minutes. For comparison, we have never been able to achieve similar absolute convergence with conventional CG methods for this high signal-to-noise data set, even after thousands of CG iterations and employing expensive preconditioners. The solver is part of the Commander 2 code, which is available with an open source license at http://commander.bitbucket.org/.
引用
收藏
页数:13
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