activity
20182022
most citedInvestigating the Effect of Galaxy Interactions on Star Formation at 0.5<z<3.0

37 citations · 67 across the 5 of their papers we have counts for

collaborators

9 papers

astro-ph.GA202237 cited

Investigating the Effect of Galaxy Interactions on Star Formation at 0.5<z<3.0

Ekta A. Shah, Jeyhan S. Kartaltepe, Christina T. Magagnoli +24

Observations and simulations of interacting galaxies and mergers in the local universe have shown that interactions can significantly enhance the star formation rates (SFR) and fue…

astro-ph.GA2022

Lack of influence of the environment in the earliest stages of massive galaxy formation

Marianna Annunziatella, PabloG. Pérez-González, Ángela García Argumánez +5

We investigate how the environment affects the assembly history of massive galaxies. For that purpose, we make use of SHARDS and HST spectro-photometric data, whose depth, spectral…

astro-ph.GA2022

From naked spheroids to disky galaxies: how do massive disk galaxies shape their morphology?

L. Costantin, P. G. Pérez-González, J. Méndez-Abreu +9

We investigate the assembly history of massive disk galaxies and describe how they shape their morphology through cosmic time. Using SHARDS and HST data, we modeled the surface bri…

astro-ph.GA20219 cited

Emission Line Galaxies in the SHARDS Frontier Fields I: Candidate Selection and the Discovery of Bursty Hα Emitters

Alex Griffiths, Christopher J. Conselice, Leonardo Ferreira +7

Emission line galaxies provide a crucial tool for the study of galaxy formation and evolution, providing a means to trace a galaxy's star formation history or metal enrichment, and…

astro-ph.GA2020

Investigating the Effect of Galaxy Interactions on AGN Enhancement at

Ekta A. Shah, Jeyhan S. Kartaltepe, Christina T. Magagnoli +30

Galaxy interactions and mergers are thought to play an important role in the evolution of galaxies. Studies in the nearby universe show a higher AGN fraction in interacting and mer…

astro-ph.GA202021 cited

Differences and similarities of stellar populations in LAEs and LBGs at 3.4 - 6.8

P. Arrabal Haro, J. M. Rodríguez Espinosa, C. Muñoz-Tuñón +6

The differences between the inherent stellar populations (SPs) of LAEs and LBGs are a key factor in understanding early galaxy formation and evolution. We have run a set of SP burs…