collaborators

7 papers

astro-ph.SR2026

On the use of field RR Lyrae as Galactic probes:. IX. Radial velocities

K. Baeza-Villagra, V. F. Braga, M. Fabrizio +25

We present the largest and most homogeneous catalog of radial velocity (RV) measurements for field RR Lyrae (RRL) variables, based on both proprietary and publicly available spectr…

astro-ph.SR2026

Large Magellanic Cloud Globular Clusters in the Near-infrared. I. RR Lyrae in Reticulum

Anupam Bhardwaj, Susmita Das, Prashant Nishad +10

Reticulum is an old, metal-poor, and sparsely populated globular cluster in the outer regions of the Large Magellanic Cloud (LMC) and hosts a rich population of RR Lyrae stars. Bei…

astro-ph.GA2026

Star-Galaxy Classification in Deep LSST Data with Random Forest: A Pilot study on the Data Preview 1 Release

M. Gatto, V. Ripepi, M. Bellazzini +2

The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will produce unprecedentedly deep and wide photometric catalogs, enabling transformative studies of faint stell…

astro-ph.GA2026

On the Use of Field RR Lyrae as Galactic Probes -- VIII. Early Formation of the Galactic Spheroid

G. Bono, V. F. Braga, M. Fabrizio +54

We introduce a new photometric catalog of RR Lyrae variables (RRLs, 300,000) mainly based on data available in public datasets. We also present the largest and most homogeneo…

astro-ph.GA2026

Classical Cepheids in the Galactic thin disk I. Abundance gradients via non-local thermodynamic equilibrium spectral analysis

Antonino Nunnari, Valentina D'Orazi, Giuliana Fiorentino +23

Classical Cepheids (CCs) have long been considered excellent tracers of the chemical evolution of the Milky Way's young disk. We present a homogeneous, NLTE spectroscopic analysis…

astro-ph.HE2025

A long-period radio transient active for three decades

N. Hurley-Walker, N. Rea, S. J. McSweeney +22

Recently several long-period radio transients have been discovered, with strongly polarised coherent radio pulses appearing on timescales between tens to thousands of seconds [1,2]…