output
19942026
most citedA Massive Pulsar in a Compact Relativistic Binary

3.9k citations

Showing 2024 · astro-ph.COShow all

8 papers · 2 filters

astro-ph.CO2024

Towards detecting Primordial non-Gaussianity in the CMB using Spherical Convolutional Neural Networks

Jorik Melsen, Thomas Flöss, P. Daniel Meerburg

This paper explores a novel application of spherical convolutional neural networks (CNNs) to detect primordial non-Gaussianity in the cosmic microwave background (CMB), a key probe…

astro-ph.CO2024★ 4 cited

Challenges to a sharp change in as a solution to the Hubble tension

Indranil Banik, Harry Desmond, Nick Samaras

It has been proposed that the gravitational constant abruptly decreased around 130 Myr ago, making Type Ia supernovae (SNe) in the Hubble flow intrinsically brighter than those…

astro-ph.CO2024★ 2 cited

Exploring the effect of different cosmologies on the Epoch of Reionization 21-cm signal with POLAR

Anshuman Acharya, Qing-bo Ma, Sambit K. Giri +8

A detection of the 21-cm signal power spectrum from the Epoch of Reionization is imminent, thanks to consistent advancements from telescopes such as LOFAR, MWA, and HERA, along wit…

astro-ph.CO2024★ 5 cited

Constraints on the Hubble and matter density parameters with and without modelling the CMB anisotropies

Indranil Banik, Nick Samaras

We consider constraints on the Hubble parameter and the matter density parameter from: (i) the age of the Universe based on old stars and stellar populations…

astro-ph.CO2024

Euclid preparation: 6x2 pt analysis of Euclid's spectroscopic and photometric data sets

Euclid Collaboration, L. Paganin, M. Bonici +252

We present cosmological parameter forecasts for the Euclid 6x2pt statistics, which include the galaxy clustering and weak lensing main probes together with previously neglected cro…

astro-ph.CO2024★ 6 cited

Euclid preparation: Determining the weak lensing mass accuracy and precision for galaxy clusters

Euclid Collaboration, L. Ingoglia, M. Sereno +279

We investigate the level of accuracy and precision of cluster weak-lensing (WL) masses measured with the \Euclid data processing pipeline. We use the DEMNUni-Cov -body simulatio…

astro-ph.CO2024★ 1 cited

Euclid preparation XLVI. The Near-IR Background Dipole Experiment with Euclid

Euclid Collaboration, A. Kashlinsky, R. G. Arendt +217

Verifying the fully kinematic nature of the cosmic microwave background (CMB) dipole is of fundamental importance in cosmology. In the standard cosmological model with the Friedman…

astro-ph.CO2024★ 5 cited

Improved Weak Lensing Photometric Redshift Calibration via StratLearn and Hierarchical Modeling

Maximilian Autenrieth, Angus H. Wright, Roberto Trotta +3

Discrepancies between cosmological parameter estimates from cosmic shear surveys and from recent Planck cosmic microwave background measurements challenge the ability of the highly…