activity
20242026
collaborators

6 papers

astro-ph.GA2026

Probing IMF Variations in High-Redshift Early-Type Galaxies with SHARP

F. La Barbera, G. De Lucia, F. Ditrani +9

The stellar initial mass function (IMF), which describes the distribution of stellar masses at birth, is a fundamental ingredient in shaping galaxy evolution. Recent observations i…

astro-ph.GA2025

Caveats about measuring carbon abundances in stars using the CH band

Pablo Santos-Peral, Patricia Sánchez-Blázquez, Alejandro Vazdekis +4

Deriving accurate carbon abundance estimates for a wide variety of stars is still complex due to the difficulties in properly measuring it from atomic and molecular lines. The aim…

astro-ph.GA2025

Puzzling radial gradients of K-band absorption features in the giant elliptical galaxy M87

F. La Barbera, A. Vazdekis, A. Pasquali +8

We present new K-band spectroscopy for the giant elliptical galaxy M87 in the Virgo cluster, taken with the LUCI spectrograph at the Large Binocular Telescope (LBT). The new data a…

astro-ph.GA2025

Chemical abundance ratios for the bulge of M31

F. La Barbera, A. Vazdekis, A. Pasquali

We present abundance ratio estimates of individual elements, namely C, N, Na, and the so-called alpha elements, Mg, O, Si, Ca, and Ti, for the bulge of M31. The analysis is based o…

astro-ph.GA2024

Extragalactic globular cluster near-infrared spectroscopy: II. The stellar population synthesis model zero-point problem extends to the near-infrared

E. Eftekhari, A. Vazdekis, R. Riffel +5

Many recent studies have pointed out significant discrepancies between observations and models of stellar populations in the near-infrared (NIR). With current and future observing…

astro-ph.GA2024

Extragalactic globular cluster near-infrared spectroscopy: I. Integrated near-infrared spectra of Centaurus A/NGC 5128

L. G. Dahmer-Hahn, A. L. Chies-Santos, E. Eftekhari +6

One way to constrain the evolutionary histories of galaxies is to analyse their stellar populations. In the local Universe, our understanding of the stellar population properties o…