collaborators

8 papers

astro-ph.GA2026

A systematic comparison of green valley selection criteria across multiparameter spaces using a homogeneous ultraviolet-optical dataset

Pius Privatus, Umananda Dev Goswami

We present a systematic comparison of commonly adopted green valley (GV) selection criteria by examining their distributions across multiple observational and physical parameter sp…

astro-ph.GA2026

What's Missing in AGN Feedback? Lessons learnt from Magneticum, IllustrisTNG and Simba

D. T. Mazengo, P. Popesso, I. Marini +20

Accurately balancing gas reservoirs, star formation, and feedback across cosmic time remains a central challenge for galaxy formation models in modern hydrodynamical simulations. W…

astro-ph.GA2025

Analysis of the Effect of Bars on Environmental Dependence of Disc Galaxies with MaNGA Survey Data

Pius Privatus, Umananda Dev Goswami

Bars are fundamental structures in disc galaxies, although their role in galaxy evolution is still not fully known. This study investigates the effect of the presence of bars on th…

astro-ph.GA2025

Galaxy Evolution in the Local Universe: Group Richness Effects on Mergers and Non-Mergers

Pius Privatus, Umananda Dev Goswami

In this study, we use the luminous volume-limited samples obtained from the twelfth release of Sloan Digital Sky Survey data and mergers from Galaxy Zoo Project to investigate the…

astro-ph.GA2025

Mapping Nearby Galaxies with Apache Point Observatory: Group and field galaxies' morphologies in the colour-magnitude plane

Pius Privatus, Umananda Dev Goswami

This study involves the use of integral field spectroscopy (IFS) data from Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) to investigate whether the morphology influen…

astro-ph.GA2025

Isolated and group environment dependence of stellar mass and different star formation rates

Pius Privatus, Umananda Dev Goswami

In this study, we explored the impact of isolated and group environments on stellar mass, star formation rate (SFR), and specific star formation rate (SSFR, i.e., the rate of star…