activity
20072023
most citedX-ray flares on the UV Ceti-type star CC Eridani: a "peculiar" time-evolution of spectral parameters

16 citations · 16 across the 3 of their papers we have counts for

collaborators

6 papers

stat.ME2023

Maximum likelihood inference for a class of discrete-time Markov-switching time series models with multiple delays

José A. Martínez-Ordóñez, Javier López-Santiago, Joaquín Miguez

Autoregressive Markov switching (ARMS) time series models are used to represent real-world signals whose dynamics may change over time. They have found application in many areas of…

stat.CO2020

Adaptive quadrature schemes for Bayesian inference via active learning

F. Llorente, L. Martino, V. Elvira +2

Numerical integration and emulation are fundamental topics across scientific fields. We propose novel adaptive quadrature schemes based on an active learning procedure. We consider…

astro-ph.SR2018

The Gaia-ESO Survey: kinematical and dynamical study of four young open clusters

L. Bravi, E. Zari, G. G. Sacco +32

Context. The origin and dynamical evolution of star clusters is an important topic in stellar astrophysics. Several models have been proposed to understand the formation of bound a…

astro-ph.HE2016

Modeling non-thermal emission from stellar bow shocks

V. Pereira, J. López-Santiago, M. Miceli +2

Runaway O- and early B-type stars passing throughout the interstellar medium at supersonic velocities and characterized by strong stellar winds may produce bow shocks that can serv…

astro-ph.SR2010

A sparse population of young stars in Cepheus

A. Klutsch, D. Montes, P. Guillout +5

Once mixed in the ambient galactic plane stellar population, young stars are virtually indiscernible because neither their global photometric properties nor the presence of nearby…

astro-ph2007★ 16 cited

X-ray flares on the UV Ceti-type star CC Eridani: a "peculiar" time-evolution of spectral parameters

I. Crespo-Chacón, G. Micela, F. Reale +3

Context: Weak flares are supposed to be an important heating agent of the outer layers of stellar atmospheres. However, due to instrumental limitations, only large X-ray flares hav…