256 citations · 821 across the 15 of their papers we have counts for
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Reconstructing Star Formation Histories of High-Redshift Galaxies: A Comparison of Resolved Parametric and Non-Parametric Models
Moein Mosleh, Mohammad Riahi-Zamin, Sandro Tacchella
We investigate the optimal approach for recovering the star formation histories (SFHs) and spatial distribution of stellar mass in high-redshift galaxies (), focusing on…
Self-regulated growth of galaxy sizes along the star-forming main sequence
Shweta Jain, Sandro Tacchella, Moein Mosleh
We present a systematic analysis of the spatially resolved star formation histories (SFHs) using Hubble Space Telescope imaging data of , intermediate redshifts $0.5 \leq…
Self-Similar Buildup and Inside-Out Growth: Tracing the Evolution of Intermediate to High-Mass Star-Forming Galaxies Since
Maryam Hasheminia, Moein Mosleh, S. Zahra Hosseini-ShahiSavandi +1
We aim to discern scenarios of structural evolution of intermediate to high-mass star-forming galaxies (SFGs) since cosmic noon by comparing their stellar mass profiles with presen…
The motivation for flexible star-formation histories from spatially resolved scales within galaxies
Shweta Jain, Sandro Tacchella, Moein Mosleh
The estimation of galaxy stellar masses depends on the assumed prior of the star-formation history (SFH) and spatial scale of the analysis (spatially resolved versus integrated sca…
No Evolution in the Half-mass Radius of Milky Way-type Galaxies over the Last 10 Gyr
Maryam Hasheminia, Moein Mosleh, Sandro Tacchella +3
The Milky Way (MW) galaxy is in focus, thanks to new observational data. Here we shed new light on the MW's past by studying the structural evolution of MW progenitors, which we id…
Galaxy Sizes Since from the Perspective of Stellar Mass Distribution within Galaxies
Moein Mosleh, Shiva Hosseinnejad, S. Zahra Hosseini-ShahiSavandi +1
How stellar mass assembles within galaxies is still an open question. We present measurements of the stellar mass distribution on kpc-scale for galaxies with stellar mas…
Comparing IMF-sensitive indices of intermediate-mass quiescent galaxies in various environments
Elham Eftekhari, Moein Mosleh, Alexandre Vazdekis +1
Using samples drawn from the Sloan Digital Sky Survey, we study for the first time the relation between large-scale environments (Clusters, Groups and Voids) and the stellar Initia…
Stellar Mass Profiles of Quiescent Galaxies in Different Environments at
Moein Mosleh, Saeed Tavasoli, Sandro Tacchella
We present the stellar mass profiles of 147 isolated quiescent galaxies in very low-density environments (i.e., void regions) in the local Universe () from the Sloan D…
Connection Between Stellar Mass Distributions Within Galaxies and Quenching Since z =2
Moein Mosleh, Sandro Tacchella, Alvio Renzini +5
We study the history from to of the stellar mass assembly of quiescent and star-forming galaxies in a spatially resolved fashion. For this purpose we use multi-wa…