256 citations · 821 across the 15 of their papers we have counts for
15 papers
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…
Bayesian evidence and model selection approach for time-dependent dark energy
Mohsen Khorasani, Moein Mosleh, Ahmad Sheykhi
We use parameterized post-Friedmann (PPF) description for dark energy and apply ellipsoidal nested sampling to perform the Bayesian model selection method on different time-depende…
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…
On The Robustness of z=0-1 Galaxy Size Measurements Through Model and Non-Parametric Fits
Moein Mosleh, Rik J. Williams, Marijn Franx
We present the size-stellar mass relations of nearby (z=0.01-0.02) Sloan Digital Sky Survey galaxies, for samples selected by color, morphology, Sersic index n, and specific star f…
The Evolution of Mass-size Relation for Lyman Break Galaxies From z=1 to z=7
Moein Mosleh, Rik J. Williams, Marijn Franx +6
For the first time, we study the evolution of the stellar mass-size relation for star-forming galaxies from z ~ 4 to z ~ 7 from Hubble-WFC3/IR camera observations of the HUDF and E…
The evolution of the mass-size relation to z=3.5 for UV-bright galaxies and sub-mm galaxies in the GOODS-NORTH field
Moein Mosleh, Rik J. Williams, Marijn Franx +1
We study the evolution of the size - stellar mass relation for a large spectroscopic sample of galaxies in the GOODs North field up to . The sizes of the galaxies are m…
Galaxy Zoo: Dust in Spirals
Karen L. Masters, Robert C. Nichol, Steven Bamford +12
We investigate the effect of dust on spiral galaxies by measuring the inclination-dependence of optical colours for 24,276 well-resolved SDSS galaxies visually classified in Galaxy…
Galaxy Zoo: Passive Red Spirals
Karen L. Masters, Moein Mosleh, A. Kathy Romer +14
We study the spectroscopic properties and environments of red spiral galaxies found by the Galaxy Zoo project. By carefully selecting face-on, disk dominated spirals we construct a…