activity
19982026
most citedA measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background

817 citations · 7.7k across the 125 of their papers we have counts for

collaborators

125 papers

astro-ph.CO2026

Solving the Cosmic Coincidence Problem: The Locally Pumped Dark Energy Model

Carlo R. Contaldi, Mauro Pieroni

We propose the Locally Pumped Dark Energy (LPDE) mechanism in which cosmic acceleration is triggered by the emergence of non-linear dark matter structure. In an effective-field-the…

astro-ph.IM2025★ 1 cited

The Simons Observatory: Science Goals and Forecasts for the Enhanced Large Aperture Telescope

The Simons Observatory Collaboration, M. Abitbol, I. Abril-Cabezas +419

We describe updated scientific goals for the wide-field, millimeter-wave survey that will be produced by the Simons Observatory (SO). Significant upgrades to the 6-meter SO Large A…

astro-ph.CO2024

Cosmic Shimmering: the Gravitational Wave Signal of Time-Resolved Cosmic Shear Observations

Giorgio Mentasti, Carlo R. Contaldi

We introduce a novel approach for detecting gravitational waves through their influence on the shape of resolved astronomical objects. This method, complementary to pulsar timing a…

astro-ph.IM2024★ 1 cited

In-Flight Performance of Spider's 280 GHz Receivers

Elle C. Shaw, P. A. R. Ade, S. Akers +84

SPIDER is a balloon-borne instrument designed to map the cosmic microwave background at degree-angular scales in the presence of Galactic foregrounds. SPIDER has mapped a large sky…

astro-ph.GA2024★ 9 cited

Analysis of Polarized Dust Emission Using Data from the First Flight of SPIDER

SPIDER Collaboration, P. A. R. Ade, M. Amiri +67

Using data from the first flight of SPIDER and from Planck HFI, we probe the properties of polarized emission from interstellar dust in the SPIDER observing region. Component separ…

gr-qc2023

Probing the galactic and extragalactic gravitational wave backgrounds with space-based interferometers

Giorgio Mentasti, Carlo R. Contaldi, Marco Peloso

We employ the formalism developed in \cite{Mentasti:2023gmg} and \cite{Bartolo_2022} to study the prospect of detecting an anisotropic Stochastic Gravitational Wave Background (SGW…