On foreground removal from the Wilkinson Microwave Anisotropy Probe data by an internal linear combination method:: Limitations and implications

被引:209
作者
Eriksen, HK
Banday, AJ
Górski, KM
Lilje, PB
机构
[1] Univ Oslo, Inst Theoret Astrophys, N-0315 Oslo, Norway
[2] Max Planck Inst Astrophys, D-85741 Garching, Germany
[3] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[4] Univ Warsaw Observ, PL-00478 Warsaw, Poland
[5] Univ Oslo, Ctr Math Applicat, N-0316 Oslo, Norway
[6] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
关键词
cosmic microwave background; cosmology : observations; methods : numerical;
D O I
10.1086/422807
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the Internal Linear Combination (ILC) method presented by the Wilkinson Microwave Anisotropy Probe (WMAP) science team, with the goal of determining whether it may be used for cosmological purposes, as a template-free alternative to existing foreground-correction methods. We conclude that the method does have the potential to do just that, but great care must be taken both in implementation and in a detailed understanding of limitations caused by residual foregrounds, which can still affect cosmological results. As a first step we demonstrate how to compute the ILC weights both accurately and efficiently by means of Lagrange multipliers, and we apply this method to the observed data to produce a new version of the ILC map. This map has 12% lower variance than the ILC map of the WMAP team, primarily because of less noise. Next we describe how to generate Monte Carlo simulations of the ILC map and find that these agree well with the observed map on angular scales up to lapproximate to200, using a conservative sky cut. Finally we make two comments to the ongoing debates concerning the large-scale properties of the WMAP data. First, we note that the Galactic southeastern quadrant is associated with notably different ILC weights than the other three quadrants, possibly indicating a foreground-related anisotropy. Second, we study the properties of the quadrupole and octopole (amplitude, alignment, and planarity) and reproduce the previously reported results that the quadrupole and octopole are strongly aligned and that the octopole is moderately planar. Even more interestingly, we find that the l=5 mode is spherically symmetric at about 3 sigma, and that the l=6 mode is planar at the 2 sigma level. However, we also assess the impact of residual foregrounds on these statistics, and find that the ILC map is not clean enough to allow for cosmological conclusions. Alternative methods must be developed to study these issues further.
引用
收藏
页码:633 / 646
页数:14
相关论文
共 25 条
[1]   FLUCTUATIONS IN THE GALACTIC SYNCHROTRON RADIATION .1. IMPLICATIONS FOR SEARCHES FOR FLUCTUATIONS OF COSMOLOGICAL ORIGIN [J].
BANDAY, AJ ;
WOLFENDALE, AW .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1991, 248 (04) :705-714
[2]   First-year Wilkinson Microwave Anisotropy Probe (WMAP) observations:: Foreground emission [J].
Bennett, CL ;
Hill, RS ;
Hinshaw, G ;
Nolta, MR ;
Odegard, N ;
Page, L ;
Spergel, DN ;
Weiland, JL ;
Wright, EL ;
Halpern, M ;
Jarosik, N ;
Kogut, A ;
Limon, M ;
Meyer, SS ;
Tucker, GS ;
Wollack, E .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2003, 148 (01) :97-117
[3]   First-year Wilkinson Microwave Anisotropy Probe (WMAP) observations:: Preliminary maps and basic results [J].
Bennett, CL ;
Halpern, M ;
Hinshaw, G ;
Jarosik, N ;
Kogut, A ;
Limon, M ;
Meyer, SS ;
Page, L ;
Spergel, DN ;
Tucker, GS ;
Wollack, E ;
Wright, EL ;
Barnes, C ;
Greason, MR ;
Hill, RS ;
Komatsu, E ;
Nolta, MR ;
Odegard, N ;
Peiris, HV ;
Verde, L ;
Weiland, JL .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2003, 148 (01) :1-27
[4]  
BIELEWICZ P, 2004, UNPUB MNRAS
[5]   SEPARATION OF FOREGROUND RADIATION FROM COSMIC MICROWAVE BACKGROUND ANISOTROPY USING MULTIFREQUENCY MEASUREMENTS [J].
BRANDT, WN ;
LAWRENCE, CR ;
READHEAD, ACS ;
PAKIANATHAN, JN ;
FIOLA, TM .
ASTROPHYSICAL JOURNAL, 1994, 424 (01) :1-21
[6]   Non-Gaussianity of the derived maps from the first-year Wilkinson Microwave Anisotropy Probe data [J].
Chiang, LY ;
Naselsky, PD ;
Verkhodanov, OV ;
Way, MJ .
ASTROPHYSICAL JOURNAL, 2003, 590 (02) :L65-L68
[7]   Phase correlations in cosmic microwave background temperature maps [J].
Coles, P ;
Dineen, P ;
Earl, J ;
Wright, D .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2004, 350 (03) :989-1004
[8]   Significance of the largest scale CMB fluctuations in WMAP [J].
de Oliveira-Costa, A ;
Tegmark, M ;
Zaldarriaga, M ;
Hamilton, A .
PHYSICAL REVIEW D, 2004, 69 (06) :12
[9]  
Efstathiou G, 2004, MON NOT R ASTRON SOC, V348, P885, DOI [10.1111/j.1365-2966.2004.07409.x, 10.1111/j.1365-2966.2004.O7409.x]
[10]   Asymmetries in the cosmic microwave background anisotropy field [J].
Eriksen, HK ;
Hansen, FK ;
Banday, AJ ;
Górski, KM ;
Lilje, PB .
ASTROPHYSICAL JOURNAL, 2004, 605 (01) :14-20