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Orientation bias of optically selected galaxy clusters and its impact on stacked weak-lensing analyses

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Planckearly results. II. The thermal performance ofPlanck

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Astronomy & Astrophysics 536 A2 (2011)
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Planckearly results. XVI. ThePlanckview of nearby galaxies

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Planckearly results. XXV. Thermal dust in nearby molecular clouds

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Astronomy & Astrophysics 536 A25 (2011)
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Planckearly results. VII. The Early Release Compact Source Catalogue

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Astronomy & Astrophysics 536 A7 (2011)
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Planckearly results. XX. New light on anomalous microwave emission from spinning dust grains

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

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Larger, faster, better: Current trends in cosmological simulations

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THE ATACAMA COSMOLOGY TELESCOPE: DYNAMICAL MASSES AND SCALING RELATIONS FOR A SAMPLE OF MASSIVE SUNYAEV-ZEL'DOVICH EFFECT SELECTED GALAXY CLUSTERS $^,$

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Optical and Sunyaev–Zel'dovich observations of a new sample of distant rich galaxy clusters in the ROSAT All Sky

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RECENT DEVELOPMENTS IN ASTROPHYSICAL AND COSMOLOGICAL EXPLOITATION OF MICROWAVE SURVEYS

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Detection of warm and diffuse baryons in large scale structure from the cross correlation of gravitational lensing and the thermal Sunyaev-Zeldovich effect

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Parametrization effects in the analysis of AMI Sunyaev-Zel’dovich observations★

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A simple empirically motivated template for the thermal Sunyaev-Zel’dovich effect

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The dynamical state and mass–concentration relation of galaxy clusters

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Planckearly results. XV. Spectral energy distributions and radio continuum spectra of northern extragalactic radio sources

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Closing the loop: a self-consistent model of optical, X-ray and Sunyaev-Zel'dovich scaling relations for clusters of Galaxies

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Scaling Relations for Galaxy Clusters: Properties and Evolution

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The Atacama Cosmology Telescope: dynamical masses for 44 SZ-selected galaxy clusters over 755 square degrees

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Clusters of galaxies in thePlancksurvey

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Planckearly results. XXIV. Dust in the diffuse interstellar medium and the Galactic halo

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Planckearly results. III. First assessment of the Low Frequency Instrument in-flight performance

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Planck2013 results. I. Overview of products and scientific results

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The pre-launchPlanckSky Model: a model of sky emission at submillimetre to centimetre wavelengths

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ON THE CLUSTER PHYSICS OF SUNYAEV–ZEL’DOVICH AND X-RAY SURVEYS. IV. CHARACTERIZING DENSITY AND PRESSURE CLUMPING DUE TO INFALLING SUBSTRUCTURES

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Planckintermediate results

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THE MASS-RICHNESS RELATION OF MaxBCG CLUSTERS FROM QUASAR LENSING MAGNIFICATION USING VARIABILITY

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Planckearly results. IV. First assessment of the High Frequency Instrument in-flight performance

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IMPACT OF SYSTEMATICS ON SZ-OPTICAL SCALING RELATIONS

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A comparative study of local galaxy clusters - II. X-ray and SZ scaling relations

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WMAPOBSERVATIONS OFPLANCKESZ CLUSTERS

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What can the spatial distribution of galaxy clusters tell about their scaling relations?

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THE ATACAMA COSMOLOGY TELESCOPE: RELATION BETWEEN GALAXY CLUSTER OPTICAL RICHNESS AND SUNYAEV-ZEL'DOVICH EFFECT

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Constraints on AGN feedback from its Sunyaev–Zel'dovich imprint on the cosmic background radiation

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The XXL Survey

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Scaling relations for galaxy clusters in the Millennium-XXL simulation

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

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Planck/SDSS cluster mass and gas scaling relations for a volume-complete redMaPPer sample

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Cosmology with the pairwise kinematic SZ effect: calibration and validation using hydrodynamical simulations

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