The Atacama Cosmology Telescope: a measurement of the Cosmic Microwave Background power spectra at 98 and 150 GHz
We present the temperature and polarization angular power spectra of the CMB measured
by the Atacama Cosmology Telescope (ACT) from 5400 deg 2 of the 2013–2016 survey …
by the Atacama Cosmology Telescope (ACT) from 5400 deg 2 of the 2013–2016 survey …
Planck 2018 results-VI. Cosmological parameters
We present cosmological parameter results from the final full-mission Planck measurements
of the cosmic microwave background (CMB) anisotropies, combining information from the …
of the cosmic microwave background (CMB) anisotropies, combining information from the …
Planck 2018 results-VIII. Gravitational lensing
We present measurements of the cosmic microwave background (CMB) lensing potential
using the final Planck 2018 temperature and polarization data. Using polarization maps …
using the final Planck 2018 temperature and polarization data. Using polarization maps …
Joint constraints on cosmology and the impact of baryon feedback: Combining KiDS-1000 lensing with the thermal Sunyaev–Zeldovich effect from Planck and ACT
We conduct a pseudo-C ℓ analysis of the tomographic cross-correlation between 1000 deg
2 of weak-lensing data from the Kilo-Degree Survey (KiDS-1000) and the thermal Sunyaev …
2 of weak-lensing data from the Kilo-Degree Survey (KiDS-1000) and the thermal Sunyaev …
[HTML][HTML] The Abell 3391/95 galaxy cluster system-A 15 Mpc intergalactic medium emission filament, a warm gas bridge, infalling matter clumps, and (re-) accelerated …
Context. Inferences about dark matter, dark energy, and the missing baryons all depend on
the accuracy of our model of large-scale structure evolution. In particular, with cosmological …
the accuracy of our model of large-scale structure evolution. In particular, with cosmological …
Projection effects on the observed angular spectrum of the astrophysical stochastic gravitational wave background
D Bertacca, A Ricciardone, N Bellomo, AC Jenkins… - Physical Review D, 2020 - APS
The detection and characterization of the stochastic gravitational wave background (SGWB)
is one of the main goals of gravitational wave (GW) experiments. The observed SGWB will …
is one of the main goals of gravitational wave (GW) experiments. The observed SGWB will …
Mapping the magnetic interstellar medium in three dimensions over the full sky with neutral hydrogen
SE Clark, BS Hensley - The Astrophysical Journal, 2019 - iopscience.iop.org
Recent analyses of 21 cm neutral hydrogen (H i) emission have demonstrated that H i gas is
organized into linear filamentary structures that are preferentially aligned with the local …
organized into linear filamentary structures that are preferentially aligned with the local …
Component-separated, CIB-cleaned thermal Sunyaev-Zel'dovich maps from Planck PR4 data with a flexible public needlet ILC pipeline
F McCarthy, JC Hill - Physical Review D, 2024 - APS
We use the full-mission Planck PR4 data to construct maps of the thermal Sunyaev–
Zel'dovich effect (Compton-y parameter) in our Universe. To do so, we implement a custom …
Zel'dovich effect (Compton-y parameter) in our Universe. To do so, we implement a custom …
Enhancing measurements of the CMB blackbody temperature power spectrum by removing cosmic infrared background and thermal Sunyaev-Zel'dovich …
A Kusiak, KM Surrao, JC Hill - Physical Review D, 2023 - APS
Extracting the cosmic microwave background (CMB) blackbody temperature power
spectrum—which is dominated by the primary CMB signal and the kinematic Sunyaev …
spectrum—which is dominated by the primary CMB signal and the kinematic Sunyaev …
The Websky extragalactic CMB simulations
We present a new pipeline for the efficient generation of synthetic observations of the
extragalactic microwave sky, tailored to large ground-based CMB experiments such as the …
extragalactic microwave sky, tailored to large ground-based CMB experiments such as the …