First‐YearWilkinson Microwave Anisotropy Probe(WMAP) Observations: Temperature‐Polarization Correlation
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Cosmological parameters from SDSS and WMAPClarifying inflation models: The precise inflationary potential from effective field theory and the WMAP dataHigh resolution foreground cleaned CMB map from WMAPPlanck intermediate results. XLVII. Planck constraints on reionization historySuperimposed oscillations in the WMAP data?Searching for CPT violation with cosmic microwave background data from WMAP and BOOMERANGCharged-Particle Decay and Suppression of Primordial Power on Small ScalesHigh-redshift galaxy populations.On the origin of near-infrared extragalactic background light anisotropy.Initial conditions of the universe: how much isocurvature is allowed?Constraints from the Wilkinson microwave anisotropy probe on decaying cold dark matter.The standard cosmological modelReanalysis of the spectrum of the z = 10 galaxyUncorrelated universe: Statistical anisotropy and the vanishing angular correlation function in WMAP years 1–3Commission 28: GalaxiesInstrument, method, brightness, and polarization maps from the 2003 flight of BOOMERanGTemperature and polarization angular power spectra of Galactic dust radiation at 353 GHz as measured by ArcheopsFirst detection of polarization of the submillimetre diffuse galactic dust emission by ArcheopsThe conventions for the polarization angleA Lyman αemitter atz= 6.5 found with slitless spectroscopyPlanck intermediate results XLIX. Parity-violation constraints from polarization dataAn alternative to the cosmological “concordance model”Planck 2015 results. XVI. Isotropy and statistics of the CMBPRESENT STATUS OF PRIMORDIAL NUCLEOSYNTHESIS AFTER WMAP: RESULTS FROM A NEW BBN CODEUltrahigh energy neutrinos from population III stars: Concept and constraintsTHE PRIMEVAL STRUCTURE TELESCOPEGravitational-wave background from compact objects embedded in active galactic nuclei accretion disksStochastic gravitational-wave background from cosmological supernovaeSDSS galaxy bias from halo mass-bias relation and its cosmological implicationsPrimordial Non-Gaussianity in the Cosmic Microwave BackgroundAn upper limit to polarized submillimetre emission in Arp 220Effects of a Decaying Cosmological FluctuationThe impact of Galactic synchrotron emission on CMB anisotropy measurements. I. Angular power spectrum analysis of total intensity all-sky surveysTrade-off between angular resolution and straylight contamination in the PLANCK Low Frequency InstrumentGalaxy evolution in the infrared: comparison of a hierarchical galaxy formation model with Spitzer dataThe first generation of star-forming haloesTracing the first stars with fluctuations of the cosmic infrared backgroundThe formation of the first low-mass stars from gas with low carbon and oxygen abundances
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First‐YearWilkinson Microwave Anisotropy Probe(WMAP) Observations: Temperature‐Polarization Correlation
description
article
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована у вересні 2003
@uk
ലേഖനം
@ml
name
First‐YearWilkinson Microwave Anisotropy Probe
@nl
First‐YearWilkinson Microwave ...... ature‐Polarization Correlation
@en
type
label
First‐YearWilkinson Microwave Anisotropy Probe
@nl
First‐YearWilkinson Microwave ...... ature‐Polarization Correlation
@en
prefLabel
First‐YearWilkinson Microwave Anisotropy Probe
@nl
First‐YearWilkinson Microwave ...... ature‐Polarization Correlation
@en
P2093
P356
P1476
First‐YearWilkinson Microwave ...... ature‐Polarization Correlation
@en
P2093
C. L. Bennett
D. N. Spergel
E. L. Wright
E. Wollack
G. Hinshaw
G. S. Tucker
M. Halpern
P304
P356
10.1086/377219
P577
2003-09-01T00:00:00Z
P5875
P818
astro-ph/0302213
P819
2003ApJS..148..161K