activity
20132026
most citedNeutrino Physics from the Cosmic Microwave Background and Large Scale Structure

282 citations · 819 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2026

The Collective Voice of Ly Emitters: Insights from JWST Stacked Spectroscopy

R. Tripodi, L. Napolitano, L. Pentericci +20

We present a spatially resolved stacked analysis of 287 LAEs at observed with JWST/NIRSpec prism spectroscopy. By constructing a two-dimensional stack from public surveys (CA…

astro-ph.GA2025

Extreme equivalent width-selected low-mass starbursts at : insights into their role in cosmic reionization

M. Llerena, L. Pentericci, R. Amorín +22

We investigate the properties of extreme emission line galaxies (EELGs) at and their role in reionization. Compact, low-mass galaxies with intense optical emission lines ar…

astro-ph.IM2025

CONCERTO: forward modeling of interferograms for calibration

A. Lundgren, A. Beelen, G. Lagache +36

The CarbON [CII] line in post-rEionisation and ReionisaTiOn epoch (CONCERTO) instrument is a low-resolution mapping Fourier-transform spectrometer, based on lumped-element kinetic…

astro-ph.HE2025

The origin of X-ray intra-day variability in HBL PKS 2155-304

W. Hu, J. L. Kang, J. X. Wang +2

The origin and physics of X-ray intra-day variability (IDV) in blazars, which is a long-standing issue, is studied by modelling the broad-band X-ray spectrum, the light curves (LCs…

astro-ph.GA2025★ 10 cited

Little impact of mergers and galaxy morphology on the production and escape of ionizing photons in the early Universe

S. Mascia, L. Pentericci, M. Llerena +28

Compact, star-forming galaxies with high star formation rate surface densities () are often efficient Lyman continuum (LyC) emitters at , likely as inten…

astro-ph.GA2024★ 1 cited

A resolved Lyman-Alpha profile with doubly peaked emission at z~7

C. Moya-Sierralta, J. González-López, L. Infante +7

The epoch of reionization is a landmark in structure formation and galaxy evolution. How it happened is still not clear, especially regarding which population of objects was respon…

astro-ph.IM2024★ 4 cited

CONCERTO at APEX -- On-sky performance in continuum

W. Hu, A. Beelen, G. Lagache +36

We present the data-processing algorithms and the performance of CONCERTO (CarbON CII line in post-rEionisation and ReionisaTiOn epoch) in continuum by analysing the data from the…

astro-ph.GA2024

CLASSY X: Highlighting Differences Between Partial Covering and Semi-Analytic Modeling in the Estimate of Galactic Outflow Properties

M. Huberty, C. Carr, C. Scarlata +17

Feedback driven massive outflows play a crucial role in galaxy evolution by regulating star formation and influencing the dynamics of surrounding media. Extracting outflow properti…

astro-ph.GA2024★ 49 cited

Peering into cosmic reionization: the Ly visibility evolution from galaxies at = 4.5-8.5 with JWST

L. Napolitano, L. Pentericci, P. Santini +28

The resonant scattering interaction between Ly photons and neutral hydrogen implies that a partially neutral IGM can significantly impact the detectability of Ly emission in…

astro-ph.GA2024★ 12 cited

A lack of LAEs within 5Mpc of a luminous quasar in an overdensity at z=6.9: potential evidence of quasar negative feedback at protocluster scales

Trystan S. Lambert, R. J. Assef, C. Mazzucchelli +13

High-redshift quasars are thought to live in the densest regions of space which should be made evident by an overdensity of galaxies around them. However, campaigns to identify the…

astro-ph.CO2023★ 11 cited

CONCERTO: Extracting the power spectrum of the [C II ] emission line

M. Van Cuyck, N. Ponthieu, G. Lagache +21

CONCERTO is the first experiment to perform a [CII] line intensity mapping survey to target . Measuring the [CII] power spectrum allows us to study the role of dusty star-fo…

astro-ph.CO2022

CONCERTO: Simulating the CO, [CII], and [CI] line emission of galaxies in a 117 field and the impact of field-to-field variance

A. Gkogkou, M. Béthermin, G. Lagache +29

In the submm regime, spectral line scans and line intensity mapping (LIM) are new promising probes for the cold gas content and star formation rate of galaxies across cosmic time.…

astro-ph.GA2022★ 56 cited

CONCERTO: High-fidelity simulation of millimeter line emissions of galaxies and [CII] intensity mapping

M. Bethermin, A. Gkogkou, M. Van Cuyck +27

The intensity mapping of the [CII] 158um line redshifted to the sub-mm window is a promising probe of the z>4 star formation and its spatial distribution into the large-scale struc…

astro-ph.IM2021★ 14 cited

CONCERTO at APEX: Installation and first phase of on-sky commissioning

A. Catalano, P. Ade, M. Aravena +40

CONCERTO (CarbON CII line in post-rEionisation and ReionisaTiOn) is a large field-of-view (FoV) spectro-imager that has been installed on the Cassegrain Cabin of Atacama Pathfinder…

astro-ph.IM2021★ 11 cited

CONCERTO at APEX: installation and technical commissioning

A. Monfardini, A. Beelen, A. Benoit +41

We describe the deployment and first tests on Sky of CONCERTO, a large field-of-view (18.6arc-min) spectral-imaging instrument. The instrument operates in the range 130-310GHz from…

astro-ph.IM2016★ 176 cited

eXTP -- enhanced X-ray Timing and Polarimetry Mission

S. N. Zhang, M. Feroci, A. Santangelo +181

eXTP is a science mission designed to study the state of matter under extreme conditions of density, gravity and magnetism. Primary targets include isolated and binary neutron star…

astro-ph.CO2013★ 282 cited

Neutrino Physics from the Cosmic Microwave Background and Large Scale Structure

K. N. Abazajian, K. Arnold, J. Austermann +74

This is a report on the status and prospects of the quantification of neutrino properties through the cosmological neutrino background for the Cosmic Frontier of the Division of Pa…

astro-ph.CO2013★ 193 cited

Inflation Physics from the Cosmic Microwave Background and Large Scale Structure

K. N. Abazajian, K. Arnold, J. Austermann +91

Fluctuations in the intensity and polarization of the cosmic microwave background (CMB) and the large-scale distribution of matter in the universe each contain clues about the natu…