activity
20182026
most cited2D chemical evolution model: the impact of galactic disc asymmetries on azimuthal chemical abundance variations

60 citations · 76 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2026

The potential broader complex linked to the key Cepheid SV Vul

Daniel Majaess, Ignacio Negueruela, Leonid N. Berdnikov +10

A new distance was established to the Cepheid SV Vul () and its host cluster Alicante 13, and is tied in part to deeper UKIDSS-DR6 photometry and Gaia DR3 observatio…

astro-ph.SR2025★ 4 cited

Rare Find: Discovery and chemo-dynamical properties of two s-process enhanced RR Lyrae stars

Valentina D'Orazi, Giuliano Iorio, Borbála Cseh +15

We report the serendipitous discovery of two RR Lyrae stars exhibiting significant s-process element enrichment, a rare class previously represented solely by TY Gruis. Our goal is…

astro-ph.SR2025

The Gaia parallax discrepancy for the cluster Pismis 19, and separating Scutis from Cepheids

Daniel Majaess, Charles J. Bonatto, David G. Turner +10

Pre-Gaia distances for the open cluster Pismis 19 disagree with Gaia parallaxes. A 2MASS red clump distance was therefore established for Pismis 19 ( kpc), whic…

astro-ph.SR2024

Variable Star Light Curves in Koopman Space

Nicolas Mekhaël, Mario Pasquato, Gaia Carenini +4

We present the first application of data-driven techniques for dynamical system analysis based on Koopman theory to variable stars. We focus on light curves of RRLyrae type variabl…

astro-ph.IM2024★ 12 cited

The Wide-field Spectroscopic Telescope (WST) Science White Paper

Vincenzo Mainieri, Richard I. Anderson, Jarle Brinchmann +214

The Wide-field Spectroscopic Telescope (WST) is proposed as a new facility dedicated to the efficient delivery of spectroscopic surveys. This white paper summarises the initial con…

astro-ph.GA2018★ 60 cited

2D chemical evolution model: the impact of galactic disc asymmetries on azimuthal chemical abundance variations

E. Spitoni, G. Cescutti, I. Minchev +5

Galactic disc chemical evolution models generally ignore azimuthal surface density variation that can introduce chemical abundance azimuthal gradients. Recent observations, however…