activity
20142026
most citedThe VIMOS Ultra-Deep Survey: ~10,000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2<z<~6

353 citations · 1.5k across the 26 of their papers we have counts for

collaborators

26 papers

astro-ph.GA2026

From DES to KiDS: Domain adaptation for cross-survey detection of low-surface-brightness galaxies

Hareesh Thuruthipilly, Krzysztof Lisiecki, Junais +19

Low-surface-brightness galaxies (LSBGs) are vital for understanding galaxy formation, but their diffuse nature makes them challenging to detect. Upcoming large-scale surveys are ex…

astro-ph.GA2025

Environmental dependence of galaxy properties in the southern GAMA regions

Koti Joy, Unnikrishnan Sureshkumar, Anand Narayanan +4

Using data from the Galaxy and Mass Assembly (GAMA) survey, we investigate how galaxy properties correlate with the local environment, focusing on the two southern regions of the s…

astro-ph.CO2024

Halo asymmetry in the modelling of galaxy clustering

Anna Durkalec, Agnieszka Pollo, Ummi Abbas

Conventional studies of galaxy clustering within the framework of halo models typically assume that the density profile of all dark matter haloes can be approximated by the Navarro…

astro-ph.GA2024★ 15 cited

Do galaxy mergers prefer under-dense environments?

U. Sureshkumar, A. Durkalec, A. Pollo +6

Galaxy mergers play a crucial role in galaxy evolution. However, the correlation between mergers and the local environment of galaxies is not fully understood. We aim to address th…

astro-ph.GA2023

A comparative study of the fundamental metallicity relation: the impact of methodology on its observed evolution

F. Pistis, A. Pollo, M. Figueira +10

We used 5487 star-forming galaxies at redshift z~0.63 extracted from the VIPERS and 143774 comparison galaxies in the local Universe from the GSWLC catalog. We employed two familie…

astro-ph.GA2022★ 12 cited

The fundamental metallicity relation from SDSS (z~0) to VIPERS (z~0.7) Data selection or evolution

F. Pistis, A. Pollo, M. Scodeggio +6

Aims. We focus on how to homogenize the comparison between galaxy samples having different characteristics. We check the projections of the fundamental metallicity relation (FMR) a…