collaborators

12 papers

astro-ph.CO2026

Does Early Dark Energy Absorb the DESI Late-Time Dynamics Signal? A Combined Analysis

Mohammad Malekjani, Saeed Pourojaghi

While the recent Baryon Acoustic Oscillation (BAO) measurements from the Dark Energy Spectroscopic Instrument (DESI) collaboration are largely consistent with a flat CDM cosmolo…

astro-ph.CO2026

Redshift Dependence of Dipole in Pantheon+ Supernovae

M. H. Jalali-Kanafi, E. Ó Colgáin, S. Pourojaghi +1

We examine the dipole structure in the local cosmic expansion rate using the Pantheon+ compilation of Type Ia supernovae. We reconstruct directional maps of across the…

astro-ph.CO2026

Crosschecking Cosmic Distances from DESI BAO and DES SNe

Mauricio Lopez-Hernandez, Eoin Ó Colgáin, Saeed Pourojaghi +1

We perform a consistency check of DESI DR2 BAO constraints ( by reconstructing the same quantities from DES supernovae (SNe) in bins with the same effective reds…

astro-ph.CO2026

How much has DESI dark energy evolved since DR1?

Eoin Ó Colgáin, Saeed Pourojaghi, M. M. Sheikh-Jabbari +1

DESI has reported a dynamical dark energy (DE) signal based on the CDM model that is in conflict with Hubble tension. Recalling that the combination of DESI DR1 BAO and DR…

astro-ph.CO2025

How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements

Mohammad Malekjani, Saeed Pourojaghi, Zahra Davari

The nature of dark energy is one of the big puzzling issues in cosmology. While CDM provides a good fit to the observational data, evolving dark energy scenarios, such as the C…

astro-ph.CO2025

On the Analysis Dependence of DESI Dynamical Dark Energy

Eoin Ó Colgáin, Saeed Pourojaghi, M. M. Sheikh-Jabbari

We continue scientific scrutiny of the DESI dynamical dark energy (DE) claim by explicitly demonstrating that the result depends on the analysis pipeline. Concretely, we define a l…