activity
20242026
collaborators

12 papers

astro-ph.GA2026

Global trends in morphology from massive to dwarf galaxies

Ilin Lazar, Sugata Kaviraj, Christopher J. Conselice +7

The morphological properties of dwarf galaxies (Mstar < 10^9.5 MSun) remain largely unexplored, particularly outside the local neighbourhood. We explore how morphology changes acro…

astro-ph.GA2026

Isophote shape analysis and the unfortunate subtlety of dwarf galaxy structure

A. E. Watkins, I. Lazar, T. Sedgwick +5

Dwarf galaxies (), being sensitive to key evolutionary drivers like baryonic feedback and tidal perturbation, are crucial for understanding galax…

astro-ph.GA2026

AGN in massive galaxies identified via optical broadband variability: lessons from VST-COSMOS for future LSST science

B. Bichang'a, D. De Cicco, S. Kaviraj +4

We study the properties of 56 massive (M > 10 M) galaxies at that host AGN, detected via their broadband optical variability in the VST-COSMOS…

astro-ph.GA2026

Downsizing does not extend to dwarf galaxies: identifying the stellar mass regimes shaped by supernova and AGN feedback

Ilin Lazar, Sugata Kaviraj, Garreth Martin +10

We explore how the fraction of red (quenched) galaxies varies in the dwarf galaxy regime (10^7 MSun < Mstar < 10^9.5 MSun), using a mass-complete sample of ~5900 dwarfs at z<0.15,…

astro-ph.GA2026

Multi-wavelength morphology and dust emission in low-redshift dwarf galaxies in COSMOS-Web with HST and JWST

D. Kakkad, I. Lazar, S. Harish +18

Low-mass or dwarf galaxies (M M) are abundant in the Universe, yet their formation and evolution remain poorly understood. Their enhanced sensitivity to fe…

astro-ph.GA2025

Variability-selected AGN in dwarf galaxies: the incidence of AGN in dwarf and massive galaxies is similar

S. Kaviraj, D. De Cicco, I. Lazar +4

We use the VST-COSMOS survey to identify, via their optical broadband variability, 30 AGN in nearby (z<0.4) dwarf (10^8 MSun < M < 10^10 MSun) galaxies. VST-COSMOS offers a 1 deg^2…