MODELING EXTRAGALACTIC FOREGROUNDS AND SECONDARIES FOR UNBIASED ESTIMATION OF COSMOLOGICAL PARAMETERS FROM PRIMARY COSMIC MICROWAVE BACKGROUND ANISOTROPY

HIGH-RESOLUTION VERY LARGE ARRAY IMAGING OF SLOAN DIGITAL SKY SURVEY STRIPE 82 AT 1.4 GHz

(2011) J. A. Hodge et al.   ASTRONOMICAL JOURNAL

Planckearly results. IX.XMM-Newtonfollow-up for validation ofPlanckcluster candidates

(2011) et al.   ASTRONOMY & ASTROPHYSICS

Planckearly results. XIII. Statistical properties of extragalactic radio sources in thePlanckEarly Release Compact Source Catalogue

(2011) et al.   ASTRONOMY & ASTROPHYSICS

Planckearly results. X. Statistical analysis of Sunyaev-Zeldovich scaling relations for X-ray galaxy clusters

(2011) et al.   ASTRONOMY & ASTROPHYSICS

Planckearly results. XVIII. The power spectrum of cosmic infrared background anisotropies

(2011) et al.   ASTRONOMY & ASTROPHYSICS

Planckearly results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample

(2011) et al.   ASTRONOMY & ASTROPHYSICS

THE ATACAMA COSMOLOGY TELESCOPE: COSMOLOGICAL PARAMETERS FROM THE 2008 POWER SPECTRUM

(2011) J. Dunkley et al.   ASTROPHYSICAL JOURNAL

A MEASUREMENT OF THE DAMPING TAIL OF THE COSMIC MICROWAVE BACKGROUND POWER SPECTRUM WITH THE SOUTH POLE TELESCOPE

(2011) R. Keisler et al.   ASTROPHYSICAL JOURNAL

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

(2011) B. Gold et al.   ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES

Statistical properties of polarized radio sources at high frequency and their impact on cosmic microwave background polarization measurements

(2011) R. A. Battye et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 1011 solar masses

(2011) Alexandre Amblard et al.   NATURE

SIMULATIONS OF THE SUNYAEV-ZEL'DOVICH POWER SPECTRUM WITH ACTIVE GALACTIC NUCLEUS FEEDBACK

(2010) N. Battaglia et al.   ASTROPHYSICAL JOURNAL

ANGULAR POWER SPECTRA OF THE MILLIMETER-WAVELENGTH BACKGROUND LIGHT FROM DUSTY STAR-FORMING GALAXIES WITH THE SOUTH POLE TELESCOPE

(2010) N. R. Hall et al.   ASTROPHYSICAL JOURNAL

MEASUREMENTS OF SECONDARY COSMIC MICROWAVE BACKGROUND ANISOTROPIES WITH THE SOUTH POLE TELESCOPE

(2010) M. Lueker et al.   ASTROPHYSICAL JOURNAL

IMPACT OF CLUSTER PHYSICS ON THE SUNYAEV-ZEL'DOVICH POWER SPECTRUM

(2010) Laurie D. Shaw et al.   ASTROPHYSICAL JOURNAL

SIMULATIONS OF THE MICROWAVE SKY

(2010) Neelima Sehgal et al.   ASTROPHYSICAL JOURNAL

EXTRAGALACTIC MILLIMETER-WAVE SOURCES IN SOUTH POLE TELESCOPE SURVEY DATA: SOURCE COUNTS, CATALOG, AND STATISTICS FOR AN 87 SQUARE-DEGREE FIELD

(2010) J. D. Vieira et al.   ASTROPHYSICAL JOURNAL

SHARPENING THE PRECISION OF THE SUNYAEV-ZEL'DOVICH POWER SPECTRUM

(2009) Laurie D. Shaw et al.   ASTROPHYSICAL JOURNAL

BLAST: CORRELATIONS IN THE COSMIC FAR-INFRARED BACKGROUND AT 250, 350, AND 500 μm REVEAL CLUSTERING OF STAR-FORMING GALAXIES

(2009) Marco P. Viero et al.   ASTROPHYSICAL JOURNAL

RESIDUAL GAS MOTIONS IN THE INTRACLUSTER MEDIUM AND BIAS IN HYDROSTATIC MEASUREMENTS OF MASS PROFILES OF CLUSTERS

(2009) Erwin T. Lau et al.   ASTROPHYSICAL JOURNAL

STELLAR AND TOTAL BARYON MASS FRACTIONS IN GROUPS AND CLUSTERS SINCE REDSHIFT 1

(2009) S. Giodini et al.   ASTROPHYSICAL JOURNAL

FIVE-YEARWILKINSON MICROWAVE ANISOTROPY PROBEOBSERVATIONS: SOURCE CATALOG

(2009) E. L. Wright et al.   ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES

Statistics of the Sunyaev-Zel'dovich effect power spectrum

(2009) Michael W. Peel et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

Component separation methods for the PLANCK mission

(2008) S. M. Leach et al.   ASTRONOMY & ASTROPHYSICS

Toward a Halo Mass Function for Precision Cosmology: The Limits of Universality

(2008) Jeremy Tinker et al.   ASTROPHYSICAL JOURNAL

Biases on the cosmological parameters and thermal Sunyaev-Zel'dovich residuals

(2008) Nicolas Taburet et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

Impact of point source clustering on cosmological parameters with CMB anisotropies

(2008) Paolo Serra et al.   PHYSICAL REVIEW D