activity
20112026
most citedAutoRegressive Planet Search: Application to the Kepler Mission

34 citations · 122 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2026

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants

Lydia S. Cidale, Alejandra Christen, Aldana Alberici Adam +6

The properties of O-type supergiant stars remain largely unexplored. By analysing their light variations, we can unravel underlying physical phenomena, such as binarity, stellar pu…

astro-ph.SR2021

Analytical Solutions for Radiation-Driven Winds in Massive Stars II: The -slow Regime

I. Araya, A. Christen, M. Curé +7

Accurate mass-loss rates and terminal velocities from massive stars winds are essential to obtain synthetic spectra from radiative transfer calculations and to determine the evolut…

astro-ph.EP2019★ 34 cited

AutoRegressive Planet Search: Application to the Kepler Mission

Gabriel A. Caceres, Eric D. Feigelson, G. Jogesh Babu +5

The 4-year light curves of 156,717 stars observed with NASA's Kepler mission are analyzed using the AutoRegressive Planet Search (ARPS) methodology described by Caceres et al. (201…

astro-ph.SR2019★ 8 cited

A method to deconvolve stellar rotational velocities III. The probability distribution function via Maximum Likelihood utilizing Finite Distribution Mixtures

Rafael Orellana, Pedro Escarate, Michel Cure +3

The study of accurate methods to estimate the distribution of stellar rotational velocities is important for understanding many aspects of stellar evolution. From such observations…

astro-ph.EP2019★ 29 cited

AutoRegressive Planet Search: Methodology

Gabriel A. Caceres, Eric D. Feigelson, G. Jogesh Babu +5

The detection of periodic signals from transiting exoplanets is often impeded by extraneous aperiodic photometric variability, either intrinsic to the star or arising from the meas…

astro-ph.IM2016★ 6 cited

A method to deconvolve stellar rotational velocities II

A. Christen, P. Escarate, M. Cure +2

Knowing the distribution of stellar rotational velocities is essential for the understanding stellar evolution. Because we measure the projected rotational speed vsini, we need to…

math.PR2015★ 4 cited

Quantitative exponential bounds for the renewal theorem with spread-out distributions

J. -B Bardet, A Christen, J Fontbona

We establish explicit exponential convergence estimates for the renewal theorem, in terms of a uniform component of the inter arrival distribution, of its Laplace transform which i…

astro-ph.IM2014★ 6 cited

A method to deconvolve mass ratio distribution from binary stars

Michel Cure, Diego F. Rial, Alejandra Christen +2

To better understand the evolution of stars in binary systems as well as to constrain the formation of binary stars, it is important to know the binary mass-ratio distribution. How…

astro-ph.IM2014★ 33 cited

A method to deconvolve stellar rotational velocities

Michel Cure, Diego F. Rial, Alejandra Christen +1

Rotational speed is an important physical parameter of stars and knowing the distribution of stellar rotational velocities is essential for the understanding stellar evolution. How…

math.PR2011★ 2 cited

Total variation estimates for the TCP process

Jean-Baptiste Bardet, Alejandra Christen, Arnaud Guillin +2

The TCP window size process appears in the modeling of the famous Transmission Control Protocol used for data transmission over the Internet. This continuous time Markov process ta…