Estimating the bispectrum of the Very Small Array data

被引:16
作者
Smith, S
Rocha, G
Challinor, A
Battye, RA
Carreira, P
Cleary, K
Davies, RD
Davis, RJ
Dickinson, C
Genova-Santos, R
Grainge, K
Gutiérrez, CM
Hafez, YA
Hobson, MP
Jones, ME
Kneissl, R
Lancaster, K
Lasenby, A
Leahy, JP
Maisinger, K
Pooley, GG
Rajguru, N
Rebolo, R
Rubiño-Martin, JA
Molina, PS
Saunders, RDE
Savage, RS
Scott, P
Slosar, A
Taylor, AC
Titterington, D
Waldram, E
Watson, RA
机构
[1] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England
[2] Univ Manchester, Jodrell Bank Observ, Manchester M13 9PL, Lancs, England
[3] Inst Astrofis Canarias, Tenerife 38200, Spain
[4] Univ Oxford, Dept Phys, Nucl & Astrophys Lab, Oxford OX1 3RH, England
[5] Univ Porto, Ctr Astrofis, P-4150762 Oporto, Portugal
[6] CSIC, Madrid, Spain
关键词
methods : data analysis; cosmic microwave background; cosmology : observations;
D O I
10.1111/j.1365-2966.2004.07885.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We estimate the bispectrum of the Very Small Array data from the compact and extended configuration observations released in 2002 December, and compare our results with those obtained from Gaussian simulations. There is a slight excess of large bispectrum values for two individual fields, but this does not appear when the fields are combined. Given our expected level of residual point sources, we do not expect these to be the source of the discrepancy. Using the compact configuration data, we put an upper limit of 5400 on the value of f (NL), the nonlinear coupling parameter, at 95 per cent confidence. We test our bispectrum estimator using non-Gaussian simulations with a known bispectrum, and recover the input values.
引用
收藏
页码:887 / 902
页数:16
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