activity
20222025
most citedStar formation history and transition epoch of cluster galaxies based on the Horizon-AGN simulation

9 citations · 20 across the 4 of their papers we have counts for

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Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA20252 cited

Nearby dwarf galaxies with extreme star formation rates: a window into dwarf-galaxy evolution in the early Universe

S. Kaviraj, B. Bichang'a, I. Lazar +3

We study a sample of nearby (z~0.2) low-luminosity dwarf (10^7 MSun < M* < 10^8 MSun) galaxies which have extreme (0.1 - 3 MSun/yr) star formation rates (SFRs) for this mass regime…

astro-ph.GA2025

The quenching of star formation in dwarf galaxies: new perspectives from deep-wide surveys

S. Kaviraj, I. Lazar, A. E. Watkins +3

Dwarf galaxies dominate the galaxy number density, making them critical to our understanding of galaxy evolution. However, typical dwarfs are too faint to be visible outside the ve…

astro-ph.GA20249 cited

The structural properties of nearby dwarf galaxies in low density environments -- size, surface brightness and colour gradients

Ilin Lazar, Sugata Kaviraj, Aaron E. Watkins +3

We use a complete sample of 211 nearby (z<0.08) dwarf (10^8 MSun < Mstar < 10^9.5 Msun) galaxies in low-density environments, to study their structural properties: effective radii…

astro-ph.GA2024

The properties of AGN in dwarf galaxies identified via SED fitting

B. Bichang'a, S. Kaviraj, I. Lazar +5

Given their dominance of the galaxy number density, dwarf galaxies are central to our understanding of galaxy formation. While the incidence of AGN and their impact on galaxy evolu…

astro-ph.GA202424 cited

The morphological mix of dwarf galaxies in the nearby Universe

Ilin Lazar, Sugata Kaviraj, Aaron E. Watkins +3

We use a complete, unbiased sample of 257 dwarf (10^8 MSun < Mstar < 10^9.5 MSun) galaxies at z < 0.08, in the COSMOS field, to study the morphological mix of the dwarf population…

astro-ph.GA2023

The formation of cores in galaxies across cosmic time -- the existence of cores is not in tension with the LCDM paradigm

R. A. Jackson, S. Kaviraj, S. K. Yi +9

The `core-cusp' problem is considered a key challenge to the LCDM paradigm. Halos in dark matter only simulations exhibit `cuspy' profiles, where density continuously increases tow…