collaborators

5 papers

astro-ph.CO2026

Probing dark energy evolution with Quaia quasars through the integrated Sachs-Wolfe effect

M. Ghodsi Yengejeh, J. R. Bermejo-Climent, A. Kovács +2

The Integrated Sachs--Wolfe (ISW) effect probes the late-time evolution of gravitational potentials and provides a complementary test of the nature of dark energy. We investigate w…

astro-ph.CO2026

Euclid: Measuring the intrinsic alignment of galaxies around cosmic voids in the \Euclid Flagship simulation\

P. Vielzeuf, M. -C. Cousinou, A. Pisani +149

We present a methodology to measure the intrinsic alignment (IA) signal of galaxies in the vicinity of cosmic voids using the \Euclid-like Flagship cosmological simulation from the…

astro-ph.CO2026

Revisiting the angular size-redshift cosmological test with milliarcsecond radio structures in active galactic nuclei

Mina Ghodsi Yengejeh, Tatiana A. Koryukova, Leonid I. Gurvits +5

VLBI measurements of the sizes of compact extragalactic radio sources, jetted active galactic nuclei, provide data for probing the angular size--redshift relation, offering a compl…

astro-ph.CO2025

Integrated Sachs-Wolfe maps from the Gower Street CDM simulations

Mina Ghodsi Yengejeh, András Kovács, István Szapudi +1

The late-time linear Integrated Sachs-Wolfe (ISW) effect directly probes the dynamics of cosmic acceleration and the nature of dark energy. Detecting these weak, secondary temperat…

astro-ph.CO2025

A Multi-Probe ISW Study of Dark Energy Models with Negative Energy Density: Galaxy Correlations, Lensing Bispectrum, and Planck ISW-Lensing Likelihood

Payam Ghafari, Mahdi Najafi, Mina Ghodsi Yengejeh +3

We investigate the late-time imprints of three dark energy (DE) models, namely, the Chevallier-Polarski-Linder (CPL) parametrization, CDM, and an Omnipotent DE model, o…