activity
19962024
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 26.5k across the 181 of their papers we have counts for

collaborators

180 papers

astro-ph.CO2024

LoVoCCS. II. Weak Lensing Mass Distributions, Red-Sequence Galaxy Distributions, and Their Alignment with the Brightest Cluster Galaxy in 58 Nearby X-ray-Luminous Galaxy Clusters

Shenming Fu, Ian Dell'Antonio, Zacharias Escalante +31

The Local Volume Complete Cluster Survey (LoVoCCS) is an on-going program to observe nearly a hundred low-redshift X-ray-luminous galaxy clusters (redshifts and X-ray…

astro-ph.CO2024★ 1 cited

On the Detectability of the Moving Lens Signal in CMB Experiments

Selim C. Hotinli, Elena Pierpaoli

Upcoming cosmic microwave background (CMB) experiments are expected to detect new signals probing interaction of CMB photons with intervening large-scale structure. Among these the…

astro-ph.CO2023★ 5 cited

Transverse velocities and matter gradient correlations: a new signal and a new challenge to moving-lens analyses

Selim C. Hotinli, Elena Pierpaoli, Simone Ferraro +1

An observer that is moving towards a high-density region sees, on average, a higher matter density and more foreground-emitting sources ahead than behind themself. Consequently, th…

astro-ph.CO2022★ 6 cited

Is the Rees-Sciama effect detectable by the next generation of cosmological experiments?

Simone Ferraro, Emmanuel Schaan, Elena Pierpaoli

Non-linear growth of structure causes the gravitational potentials to grow with time, and this leaves an imprint on the small-scale temperature fluctuations of the Cosmic Microwave…

astro-ph.CO2022★ 12 cited

Snowmass 2021 CMB-S4 White Paper

Kevork Abazajian, Arwa Abdulghafour, Graeme E. Addison +353

This Snowmass 2021 White Paper describes the Cosmic Microwave Background Stage 4 project CMB-S4, which is designed to cross critical thresholds in our understanding of the origin a…

astro-ph.CO2022★ 39 cited

Snowmass2021 CMB-HD White Paper

HD Collaboration, Simone Aiola, Yashar Akrami +61

CMB-HD is a proposed millimeter-wave survey over half the sky that would be ultra-deep (0.5 uK-arcmin) and have unprecedented resolution (15 arcseconds at 150 GHz). Such a survey w…