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The Wilkinson Microwave Anisotropy Probe,
Lyman Page,
arXiv:astro-ph/0306381,
Carnegie Observatories Astrophysics Series, Vol. 2: Measuring and Modeling the Universe.
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Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Are There Cosmic Microwave Background Anomalies?,
C. L. Bennett et al.,
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Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Sky Maps, Systematic Errors, and Basic Results,
N. Jarosik et al.,
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Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Planets and Celestial Calibration Sources,
J. L. Weiland et al.,
192
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Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters,
D. Larson et al.,
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Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Foreground Emission,
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Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation,
E. Komatsu et al.
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192
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[WMAP:2010qai] - [2-7]
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Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results,
G. Hinshaw et al.
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180
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Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Foreground Emission,
B. Gold et al.
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180
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[WMAP:2008fkv] - [2-9]
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Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectra,
M. R. Nolta et al.
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180
arXiv:0803.0593.
[WMAP:2008ttx] - [2-10]
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Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data,
J. Dunkley et al.
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180
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[WMAP:2008rhx] - [2-11]
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Five-Year Wilkinson Microwave Anisotropy Probe (WMAP)Observations: Beam Maps and Window Functions,
R. S. Hill et al.
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180
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[WMAP:2008fkt] - [2-12]
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Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation,
E. Komatsu et al.
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180
arXiv:0803.0547.
[WMAP:2008lyn] - [2-13]
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Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam Profiles, Data Processing, Radiometer Characterization and Systematic Error Limits,
N. Jarosik et al.
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170
arXiv:astro-ph/0603452.
http://\lambda.gsfc.nasa.gov/product/map/dr2/pub_papers/threeyear/syserr/wmap_3yr_syserr.pdf.
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Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Results,
G. Hinshaw et al.
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170
arXiv:astro-ph/0603451.
http://\lambda.gsfc.nasa.gov/product/map/dr2/pub_papers/threeyear/temperature/wmap_3yr_temp.pdf.
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Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis,
L. Page et al.
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170
arXiv:astro-ph/0603450.
http://\lambda.gsfc.nasa.gov/product/map/dr2/pub_papers/threeyear/polarization/wmap_3yr_pol.pdf.
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Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Cosmology,
D.N. Spergel et al.
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170
arXiv:astro-ph/0603449.
http://\lambda.gsfc.nasa.gov/product/map/dr2/pub_papers/threeyear/parameters/wmap_3yr_param.pdf.
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Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Three Year Explanatory Supplement,
M. Limon et al.
(WMAP),
http://\lambda.gsfc.nasa.gov/product/map/dr2/pub_papers/threeyear/supplement/wmap_3yr_supplement.pdf.
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First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Inflation,
H. V. Peiris et al.
(WMAP),
148
arXiv:astro-ph/0302225.
[WMAP:2003syu] - [2-19]
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First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: On-Orbit Radiometer Characterization,
N. Jarosik et al.
(WMAP),
148
arXiv:astro-ph/0302224.
[WMAP:2003tll] - [2-20]
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First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Tests of Gaussianity,
E. Komatsu et al.
(WMAP),
148
arXiv:astro-ph/0302223.
[WMAP:2003xez] - [2-21]
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First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing Methods and Systematic Errors Limits,
G. Hinshaw et al.
(WMAP),
148
arXiv:astro-ph/0302222.
[WMAP:2003gdj] - [2-22]
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First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Interpretation of the TT and TE Angular Power Spectrum Peaks,
L. Page et al.
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148
arXiv:astro-ph/0302220.
[WMAP:2003tof] - [2-23]
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First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Parameter Estimation Methodology,
L. Verde et al.
(WMAP),
148
arXiv:astro-ph/0302218.
[WMAP:2003pyh] - [2-24]
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First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectrum,
G. Hinshaw et al.
(WMAP),
148
arXiv:astro-ph/0302217.
[WMAP:2003zzr] - [2-25]
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First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Signal Contamination from Sidelobe Pickup,
C. Barnes et al.
(WMAP),
148
arXiv:astro-ph/0302215.
[WMAP:2003hea] - [2-26]
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First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam Profiles and Window Functions,
L. Page et al.
(WMAP),
148
arXiv:astro-ph/0302214.
[WMAP:2003pvn] - [2-27]
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Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization,
A. Kogut et al.
(WMAP),
148
arXiv:astro-ph/0302213.
[WMAP:2003ggs] - [2-28]
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First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters,
D. N. Spergel et al.
(WMAP),
148
arXiv:astro-ph/0302209.
[WMAP:2003elm] - [2-29]
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First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Emission,
C. Bennett et al.
(WMAP),
148
arXiv:astro-ph/0302208.
[WMAP:2003cmr] - [2-30]
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First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results,
C. L. Bennett et al.
(WMAP),
148
arXiv:astro-ph/0302207.
[WMAP:2003ivt] - [2-31]
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Design, Implementation and Testing of the MAP Radiometers,
N. Jarosik et al.,
145
arXiv:astro-ph/0301164.
[Jarosik:2003xka] - [2-32]
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The Optical Design and Characterization of the Microwave Anisotropy Probe,
L. Page et al.,
585
arXiv:astro-ph/0301160.
[Page:2003bc] - [2-33]
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The MAP Satellite Feed Horns,
C. Barnes et al.,
143
arXiv:astro-ph/0301159.
[Barnes:2002ama] - [2-34]
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The Microwave Anisotropy Probe (MAP) Mission,
C. L. Bennett et al.
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583
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[WMAP:2003ogi] - [2-35]
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CMB Anisotropy Correlation Function and Topology from Simulated Maps for MAP,
Changbom Park et al.,
506
arXiv:astro-ph/9711057.
[Park:1997ad]
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First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Explanatory Supplement,
M. Limon et al.,
http://\lambda.gsfc.nasa.gov/product/map/pub_papers/firstyear/supplement/WMAP_supplement.pdf.
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Comparing and combining Wilkinson Microwave Anisotropy (WMAP) probe results and Large Scale Structure,
Licia verde,
arXiv:astro-ph/0306272,
Davis Inflation Meeting, 2003.
[Verde:2003rj] - [4-2]
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WMAP First Year Results,
E. L. Wright,
arXiv:astro-ph/0306132.
The Cosmic Microwave Background and its Polarization, New Astronomy Reviews.
[Wright:2003qm] - [4-3]
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WMAP Polarization Results,
A. Kogut,
arXiv:astro-ph/0306048.
'The Cosmic Microwave Background and its Polarization', New Astronomy Reviews.
[Kogut:2003td] - [4-4]
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Future Cosmic Microwave Background Experiments,
Mark Halpern, Douglas Scott,
arXiv:astro-ph/9904188,
ASP, San Francisco, 1999.
[Halpern:1999ng]
LAMBDA, Legacy Archive for Microwave Background Data Analysis
