most citedSMARTY: The mileS Moderate resolution neAr-infRared sTellar librarY

1 citations · 2 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2024

Probing the major driver of stellar population properties over sub-galaxy scales with SDSS MaNGA IFU spectroscopy

Ignacio Ferreras, Marina Trevisan, Ofer Lahav +2

Thanks to Integral Field Unit survey data it is possible to explore in detail the link between the formation of the stellar content in galaxies and the drivers of evolution. Tradit…

astro-ph.GA2024

Determining star formation rates in AGN hosts from strong optical emission lines

Maitê S. Z. de Mellos, Rogemar A. Riffel, Jaderson S. Schimoia +11

The influence of Active Galactic Nuclei (AGN) on star formation within their host galaxies remains a topic of intense debate. One of the primary challenges in quantifying the star…

astro-ph.GA2024★ 1 cited

Digging deeper into NGC 6868 II: ionized gas and excitation mechanism

João P. V. Benedetti, Rogério Riffel, Tiago Ricci +9

We studied the ionized gas in the inner region ( pc) of the galaxy NGC 6868 using Gemini/GMOS integral field unit observations. Channel maps reveal complex ki…

astro-ph.GA2024

Massive Compact Quiescent Galaxies in the vs. Plane: Insights from stellar Population Properties

K. Slodkowski Clerici, A. Schnorr-Müller, M. Trevisan +1

We investigated the stellar population properties of a sample of 1858 massive compact galaxies (MCGs) extracted from the SDSS survey. Motivated by previous results showing that old…

astro-ph.GA2024

Observational constraints on the stellar recycled gas in active galactic nuclei feeding

Rogerio Riffel, Luis G. Dahmer-Hahn, Alexandre Vazdekis +15

Near-infrared long-slit spectroscopy has been used to study the stellar population (SP) of the low luminosity active galactic nuclei (AGN) and matched analogues (LLAMA) sample. To…

astro-ph.GA2024★ 1 cited

SMARTY: The mileS Moderate resolution neAr-infRared sTellar librarY

Michele Bertoldo-Coêlho, Rogério Riffel, Marina Trevisan +13

Most of the observed galaxies cannot be resolved into individual stars and are studied through their integrated spectrum using simple stellar populations (SSPs) models, with stella…