L. Page

发表

Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Polarization

M. Halpern, Edward J. Wollack, B. Gold, 2007, The Astrophysical Journal.

FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION

Edward J. Wollack, E. L. Wright, D. Larson, 2008, 0803.0547.

The Optical Design and Characterization of the Microwave Anisotropy Probe

Edward J. Wollack, U. Chicago, G. Hinshaw, 2003, astro-ph/0301160.

Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, & Basic Results

Edward J. Wollack, D. Larson, J. Dunkley, 2008, 0803.0732.

Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, & Basic Results

Edward J. Wollack, J. Dunkley, G. Hinshaw, 2008, 0803.0732.

First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature-Polarization Correlation

Edward J. Wollack, G. Hinshaw, N. Jarosik, 2003 .

Wilkinson Microwave Anisotropy Probe (WMAP) first year observations: TE polarization

Edward J. Wollack, Princeton, G. Hinshaw, 2003, astro-ph/0302213.

First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing Methods and Systematic Error Limits

Edward J. Wollack, U. Chicago, G. Hinshaw, 2003, astro-ph/0302222.

Cosmic Microwave Background Observations with a Compact Heterogeneous 150 GHz Interferometer in Chile

M. Halpern, L. Page, W. Doriese, 2004, astro-ph/0403137.

First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Interpretation of the TT and TE Angular Power Spectrum Peaks

Edward J. Wollack, G. Hinshaw, M. Nolta, 2003, astro-ph/0302220.

A Measurement of the Angular Power Spectrum of the Microwave Background Made from the High Chilean Andes

J. Puchalla, M. Nolta, L. Page, 1999, astro-ph/9905100.

Prospects for polarized foreground removal

L. Verde, H. K. Eriksen, C. Dickinson, 2008, 0811.3915.

SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: GALACTIC FOREGROUND EMISSION

Edward J. Wollack, E. L. Wright, J. Dunkley, 2010, 1001.4555.

Accepted for Publication in the Astrophysical Journal Supplement Series

Edward J. Wollack, E. L. Wright, J. Dunkley, 2004 .

A measurement of the large-scale cosmic microwave background anisotropy at 1. 8 millimeter wavelength

S. Meyer, L. Page, E. Cheng, 1991 .

Millimeter-submillimeter wavelength filter system.

B. Golubovic, L. Page, Edward S. Cheng, 1994, Applied optics.

Five-Year Wilkinson Microwave Anisotropy Probe ( WMAP 1 ) Observations : Angular Power Spectra

J. Dunkley, G. Hinshaw, M. Nolta, 2008 .

SUBMITTED TO The Astrophysical Journal Preprint typeset using L ATEX style emulateapj v. 11/12/01 FIRST YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: INTERPRETATION OF THE TT AND TE ANGULAR POWER SPECTRUM PEAKS

M. Halpern, Edward J. Wollack, S. S. Meyer, 2022 .

A Detection of Bright Features in the Microwave Background

J. Puchalla, S. Meyer, L. Page, 1996, astro-ph/9604155.

A measurement of the medium-scale anisotropy in the cosmic microwave background radiation

J. Puchalla, S. Meyer, L. Page, 1993, astro-ph/9305022.

FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: BAYESIAN ESTIMATION OF COSMIC MICROWAVE BACKGROUND POLARIZATION MAPS

J. Dunkley, G. Hinshaw, M. Nolta, 2008, 0811.4280.

Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Polarization

Edward J. Wollack, J. Dunkley, M. Nolta, 2007, The Astrophysical Journal.

Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Cosmology

Edward J. Wollack, L. Verde, J. Dunkley, 2006, astro-ph/0603449.