activity
20162026
most citedThe GIRAFFE Inner Bulge Survey (GIBS) III. Metallicity distributions and kinematics of 26 Galactic bulge fields

160 citations · 340 across the 14 of their papers we have counts for

collaborators

15 papers

cs.LG2026

Neural Dynamics as the Composition of Quantized Units

Jacopo Minniti, Aravinth Kulanthaivelu, Richard Sproat

Deep learning is commonly interpreted at two levels: the macroscopic, through aggregate trends in loss summarized by scaling laws, and the microscopic, through neurons, features, a…

astro-ph.GA2026

Classical Cepheids in the Nuclear Stellar Disk: membership via dynamical analysis

M. De Leo, M. Zoccali, R. Albarracin +2

(abridged) Four classical Cepheids have been associated to the Nuclear Stellar Disk (NSD), suggesting a burst of star formation 20 Myrs ago. In this work, we analyse all available…

cs.LG2026

Learned Relay Representations for Forward-Thinking Discrete Diffusion Models

Benjamin Rozonoyer, Jacopo Minniti, Dhruvesh Patel +4

When Masked Diffusion Models (MDMs) generate sequences through iterative refinement, the rich internal computation over masked positions is discarded, forcing every subsequent refi…

astro-ph.GA2025★ 4 cited

Converging on the Cepheid Metallicity Dependence: Implications of Non-Standard Gaia Parallax Recalibration on Distance Measures

Louise Breuval, Gagandeep S. Anand, Richard I. Anderson +20

By comparing Cepheid brightnesses with geometric distance measures including Gaia EDR3 parallaxes, most recent analyses conclude metal-rich Cepheids are brighter, quantified as $γ\…

astro-ph.GA2024★ 4 cited

Unveiling VVV/WISE Mira variables on the far side of the Galactic disk: Distances, kinematics and a new extinction law

Rogelio Albarracín, M. Zoccali, J. Olivares Carvajal +8

The structure and kinematics of the Milky Way disk are largely inferred from the solar vicinity. To gain a comprehensive understanding, it is essential to find reliable tracers in…

astro-ph.GA2024★ 8 cited

VVV catalog of ab-type RR Lyrae in the inner Galactic bulge

M. Zoccali, C. Quezada, R. Contreras Ramos +7

Context. Observational evidence has accumulated in the past years, showing that the Galactic bulge includes two populations, a metal poor and a metal rich one that, in addition to…

astro-ph.GA2024★ 38 cited

The VISTA Variables in the Vía Láctea eXtended (VVVX) ESO public survey: Completion of the observations and legacy

R. K. Saito, M. Hempel, J. Alonso-García +143

The ESO public survey VISTA Variables in the Vía Láctea (VVV) surveyed the inner Galactic bulge and the adjacent southern Galactic disk from . Upon its conclusion, the c…

astro-ph.SR2022★ 11 cited

Discovery of a binary-origin classical Cepheid in a binary system with a 59-day orbital period

Bogumił Pilecki, Ian B. Thompson, Felipe Espinoza-Arancibia +8

We report the discovery of a surprising binary configuration of the double-mode Cepheid OGLE-LMC-CEP-1347 pulsating in the first (P_1=0.690d) and second overtone (P_2=0.556d) modes…

astro-ph.GA2022★ 11 cited

A high resolution study of near-IR diffuse interstellar bands, search for small scale structure, time variability and stellar features

J. V. Smoker, A. Müller, A. Monreal Ibero +13

Diffuse interstellar bands comprise hundreds of absorption features in the ISM. Most DIBs are observed in the optical, but some are in the IR. We observed 76 early-type stars at R=…

astro-ph.GA2022

Spectroscopic analysis of VVV CL001 cluster with MUSE

Julio Olivares Carvajal, Manuela Zoccali, Alvaro Rojas-Arriagada +4

Like most spiral galaxies, the Milky Way contains a population of blue, metal-poor globular clusters and another of red, metal-rich ones. Most of the latter belong to the bulge, an…

astro-ph.GA2021★ 24 cited

Using classical Cepheids to study the far side of the Milky Way disk. II. The spiral structure in the first and fourth Galactic quadrants

J. H. Minniti, M. Zoccali, A. Rojas-Arriagada +9

In an effort to improve our understanding of the spiral arm structure of the Milky Way, we use Classical Cepheids (CCs) to increase the number of young tracers on the far side of t…

astro-ph.GA2020★ 33 cited

Using classical Cepheids to study the far side of the Milky Way disk: I. Spectroscopic classification and the metallicity gradient

J. H. Minniti, L. Sbordone, A. Rojas-Arriagada +9

The structure, kinematics, and chemical composition of the far side of the Milky Way disk, beyond the bulge, are still to be revealed. Classical Cepheids (CCs) are young and lumino…

astro-ph.SR2019★ 19 cited

New type II Cepheids from VVV data towards the Galactic center

V. F. Braga, R. Contreras Ramos, D. Minniti +5

The Galactic center (GC) is the densest region of the Milky Way. Variability surveys towards the GC potentially provide the largest number of variable stars per square degree withi…

astro-ph.GA2018★ 28 cited

Structure and kinematics of Type II Cepheids in the Galactic bulge based on near-infrared VVV data

V. F. Braga, A. Bhardwaj, R. Contreras Ramos +5

Type II Cepheids (T2Cs) are radially pulsating variables that trace old stellar populations and provide distance estimates through their period-luminosity (PL) relation. We trace t…

astro-ph.GA2016★ 160 cited

The GIRAFFE Inner Bulge Survey (GIBS) III. Metallicity distributions and kinematics of 26 Galactic bulge fields

M. Zoccali, S. Vasquez, O. A. Gonzalez +9

Several recent studies have demonstrated that the Galactic bulge hosts two components with different mean metallicities, and possibly different spatial distribution and kinematics.…