activity
20202026
most citedCepheid Metallicity in the Leavitt Law (C-MetaLL) survey: I. HARPS-N@TNG spectroscopy of 47 Classical Cepheid and 1 BL Her variables

43 citations · 202 across the 20 of their papers we have counts for

collaborators

21 papers

astro-ph.GA2026

Euclid: Data Release 1 (DR1) -- Fornax-7, an ultra-faint companion to the Fornax dwarf spheroidal galaxy? A remote star cluster or dwarf satellite of the Fornax dSph

T. Saifollahi, A. Lançon, A. M. N. Ferguson +165

We report the discovery of an ultra-faint stellar system in the vicinity of the Fornax dwarf spheroidal (dSph) galaxy in Euclid DR1. This system, which we designate Fornax-7, is lo…

astro-ph.SR2026

Determination of [Fe/H] in Fundamental mode Classical Cepheids from Gaia DR3 light curve Fourier parameters

Roberto Molinaro, Vincenzo Ripepi, Marcella Marconi +9

Estimating the iron abundance ([Fe/H]) of Classical Cepheids (CCs) is crucial both for validating the cosmic distance scale through the Period-Luminosity relation and for tracing t…

astro-ph.GA2026

STEP survey: III. STEPping stones between the clouds: the star formation history of the Magellanic Bridge

F. Ficara, V. Ripepi, M. Cignoni +8

The Magellanic Clouds (MCs) offer a unique laboratory for studying galaxy interaction and the evolution of dwarf galaxies. By investigating when and how stars formed, the star form…

astro-ph.SR2025★ 2 cited

The model fitting of Gaia DR3 Classical Cepheid light and radial velocity curves

R. Molinaro, M. Marconi, G. De Somma +6

Classical Cepheids are key astrophysical laboratories for studying stellar structure and evolution, and for calibrating the cosmic distance scale. Despite major progress, uncertain…

astro-ph.GA2024★ 3 cited

Ultra Long Period Cepheids as standard candles from Gaia to Rubin-LSST

I. Musella, S. Leccia, R. Molinaro +10

An analysis of the Ultra Long Period Cepheids (ULPs) properties could significantly contribute to understanding the Hubble constant tension, e.g. the current discrepancy between de…

astro-ph.GA2024★ 4 cited

The YMCA (Yes, Magellanic Clouds Again) survey: probing the outer regions of the Magellanic system with VST

Massimiliano Gatto, Vincenzo Ripepi, Michele Bellazzini +9

The Magellanic Clouds (MCs) are the Milky Way's most massive dwarf satellites. As they also represent the closest pair of galaxies in an ongoing tidal interaction, while simultaneo…

astro-ph.GA2024★ 16 cited

Cepheid Metallicity in the Leavitt Law (C- MetaLL) survey: VI: Radial abundance gradients of 29 chemical species in the Milky Way Disk

E. Trentin, G. Catanzaro, V. Ripepi +9

Classical Cepheids (DCEPs) are crucial for calibrating the extragalactic distance ladder, ultimately enabling the determination of the Hubble constant through the PL and PW relatio…

astro-ph.SR2023★ 3 cited

Cepheid Metallicity in the Leavitt Law (C- MetaLL) survey: IV. The metallicity dependence of Cepheid Period-Luminosity relations

E. Trentin, V. Ripepi, R. Molinaro +10

Classical Cepheids (DCEPs) play a fundamental role in the calibration of the extra-galactic distance ladder which eventually leads to the determination of the Hubble constant(…

astro-ph.GA2023★ 4 cited

The Dragon-II simulations -- I. Evolution of single and binary compact objects in star clusters with up to 1 million stars

Manuel Arca Sedda, Albrecht W. H. Kamlah, Rainer Spurzem +7

We present the first results of the \textsc{Dragon-II} simulations, a suite of 19 -body simulations of star clusters with up to stars, with up to of them initially…

astro-ph.GA2022★ 6 cited

KMHK 1762: Another star cluster in the Large Magellanic Cloud age gap

M. Gatto, V. Ripepi, M. Bellazzini +11

The star cluster (SC) age distribution of the Large Magellanic Cloud (LMC) exhibits a gap from 4 to 10 Gyr ago, with an almost total absence of SCs. Within this age gap, onl…

astro-ph.HE2022★ 5 cited

Properties of intra-cluster low-mass X-ray binaries in Fornax globular clusters

G. Riccio, M. Paolillo, M. Cantiello +9

We present a study of the intra-cluster population of low-mass X-ray binaries (LMXB) residing in globular clusters (GC) in the central 1 of the Fornax galaxy cluster. Diffe…

astro-ph.GA2022★ 6 cited

Deep VLT photometry of the faint stellar system in the Large Magellanic Cloud periphery YMCA-1

M. Gatto, V. Ripepi, M. Bellazzini +11

We present FORS2@VLT follow-up photometry of YMCA-1, a recently discovered stellar system located 13\degr~from the Large Magellanic Cloud (LMC) center. The deep color-magnitude dia…

astro-ph.GA2022★ 5 cited

Discovery of NES, an extended tidal structure in the North-East of the Large Magellanic Cloud

M. Gatto, V. Ripepi, M. Bellazzini +4

We report on the discovery of a new diffuse stellar sub-structure protruding for 5 degrees from the North-Eastern rim of the LMC disc. The structure, that we dub North-East Structu…

astro-ph.GA2021★ 12 cited

The Fornax Cluster VLT Spectroscopic Survey IV -- Cold kinematical substructures in the Fornax core from COSTA

N. R. Napolitano, M. Gatto, C. Spiniello +15

The COld STream finder Algorithm (COSTA) is a novel algorithm to find streams in the phase space of planetary nebulae (PNe) and globular cluster (GCs) populations. COSTA isolates g…

astro-ph.GA2021★ 25 cited

The Fornax Cluster VLT Spectroscopic Survey III -- Kinematical characterisation of globular clusters across the Fornax galaxy cluster

Avinash Chaturvedi, Michael Hilker, Michele Cantiello +7

The Fornax cluster provides an unparalleled opportunity to investigate in detail the formation and evolution of early-type galaxies in a dense environment. We aim at kinematically…

astro-ph.GA2021★ 43 cited

Cepheid Metallicity in the Leavitt Law (C-MetaLL) survey: I. HARPS-N@TNG spectroscopy of 47 Classical Cepheid and 1 BL Her variables

V. Ripepi, G. Catanzaro, R. Molinaro +11

Classical Cepheids (DCEPs) are the most important primary indicators of the extragalactic distance scale. Establishing the dependence on metallicity of their period--luminosity and…

astro-ph.GA2021★ 22 cited

STEP Survey II: Structural Analysis of 170 star clusters in the SMC

M. Gatto, V. Ripepi, M. Bellazzini +9

We derived surface brightness profiles in the \emph{g} band for 170 Small Magellanic Cloud (SMC) star clusters (SCs) mainly located in the central region of the galaxy. We provide…

astro-ph.GA2021★ 9 cited

YMCA-1: a new remote star cluster of the Milky Way?

M. Gatto, V. Ripepi, M. Bellazzini +11

We report the possible discovery of a new stellar system (YMCA-1), identified during a search for small scale overdensities in the photometric data of the YMCA survey. The object's…

astro-ph.SR2020★ 17 cited

A theoretical scenario for Galactic RR Lyrae in the Gaia database: constraints on the parallax offset

Marcella Marconi, Roberto Molinaro, Vincenzo Ripepi +5

On the basis of an extended set of nonlinear convective RR Lyrae pulsation models we derive the first theoretical light curves in the Gaia bands and the corresponding intensity-wei…

astro-ph.GA2020

COSTA: the COld STream finder Algorithm. Searching for kinematical substructures in the phase space of discrete tracers

M. Gatto, N. R. Napolitano, C. Spiniello +2

Context: We present COSTA (COld STream finder Algorithm), a novel algorithm to search for cold kinematical substructures in the phase space of planetary nebulae (PNe) and globular…

astro-ph.GA2020★ 20 cited

A search for star clusters in the outskirts of the Large Magellanic Cloud: indication of clusters in the age gap

M. Gatto, V. Ripepi, M. Bellazzini +7

The YMCA (Yes, Magellanic Clouds Again) and STEP ({The SMC in Time: Evolution of a Prototype interacting late-type dwarf galaxy) projects are deep g,i photometric surveys carried o…