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20062024
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 27.5k across the 138 of their papers we have counts for

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78 papers · 1 filter

astro-ph.CO2021★ 7 cited

A Simulation-Based Method for Correcting Mode Coupling in CMB Angular Power Spectra

J. S. -Y. Leung, J. Hartley, J. M. Nagy +67

Modern CMB analysis pipelines regularly employ complex time-domain filters, beam models, masking, and other techniques during the production of sky maps and their corresponding ang…

astro-ph.CO2021★ 4 cited

The XFaster Power Spectrum and Likelihood Estimator for the Analysis of Cosmic Microwave Background Maps

A. E. Gambrel, A. S. Rahlin, X. Song +64

We present the XFaster analysis package. XFaster is a fast, iterative angular power spectrum estimator based on a diagonal approximation to the quadratic Fisher matrix estimator. X…

astro-ph.CO2021★ 26 cited

Euclid preparation: XII. Optimizing the photometric sample of the Euclid survey for galaxy clustering and galaxy-galaxy lensing analyses

Euclid Collaboration, A. Pocino, I. Tutusaus +157

The accuracy of photometric redshifts (photo-zs) particularly affects the results of the analyses of galaxy clustering with photometrically-selected galaxies (GCph) and weak lensin…

astro-ph.CO2021★ 2 cited

A Constraint on Primordial -Modes from the First Flight of the SPIDER Balloon-Borne Telescope

SPIDER Collaboration, P. A. R. Ade, M. Amiri +68

We present the first linear polarization measurements from the 2015 long-duration balloon flight of SPIDER, an experiment designed to map the polarization of the cosmic microwave b…

astro-ph.CO2021★ 22 cited

Euclid: Effect of sample covariance on the number counts of galaxy clusters

A. Fumagalli, A. Saro, S. Borgani +93

Aims. We investigate the contribution of shot-noise and sample variance to the uncertainty of cosmological parameter constraints inferred from cluster number counts in the context…

astro-ph.CO2020

Euclid: Forecasts for -cut Point Statistics

P. L. Taylor, T. Kitching, V. F. Cardone +92

Modelling uncertainties at small scales, i.e. high in the power spectrum , due to baryonic feedback, nonlinear structure growth and the fact that galaxies are biased trac…