output
20022026
most citedCosmological Constraints from the SDSS Luminous Red Galaxies

1.4k citations

Showing astro-ph.COShow all

95 papers · 1 filter

astro-ph.CO2026

Understanding constraints on primordial mass black holes made of dark matter using fast radio bursts

Surajit Kalita, Shruti Bhatporia, Amanda Weltman

In recent decades, a multitude of modified gravity theories have been proposed to address a variety of cosmological and astrophysical problems. While many of these theories remain…

astro-ph.CO2025

Prospects for measuring the Doppler magnification dipole with LSST and DESI

Isabelle Ye, Philip Bull, Caroline Guandalin +2

We forecast the detectability of the Doppler magnification dipole with a joint analysis of galaxy spectroscopic redshifts and size measurements. The Doppler magnification arises fr…

astro-ph.CO2025

Unbiased analysis of primordial non-Gaussianity: the multipoles of the full relativistic power spectrum

Chris Addis, Sêcloka L. Guedezounme, Jessie Hammond +5

A major goal of ongoing and future cosmological surveys of the large-scale structure is to measure local type primordial non-Gaussianity in the galaxy power spectrum through the sc…

astro-ph.CO2025

Visualising relativistic effects in redshift space distortions of large scale structure

Pritha Paul, Chris Clarkson

Observing large scale structure in redshift space gives rise to the well known redshift space distortions whereby a spherical distribution of galaxies is distorted into an ellipsoi…

astro-ph.CO2025★ 1 cited

Investigating the imprint of quintessence in cosmic magnification

Enas Mohamed, Didam Duniya, Hassan Abdalla +1

We study cosmic magnification beyond lensing in a late-time universe dominated by quintessence and cold dark matter. The cosmic magnification angular power spectrum, especially goi…

astro-ph.CO2025★ 1 cited

Angular correlation functions of bright Lyman-break galaxies at

Isabelle Ye, Philip Bull, Rebecca A. A. Bowler +3

We investigate the clustering of Lyman-break galaxies at redshifts of 3 5 within the COSMOS field by measuring the angular two-point correlation function. Our…