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JAVIER LOPEZ SANTIAGO

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Papers by JAVIER LOPEZ SANTIAGO

Research paper thumbnail of Marginal Likelihood Computation for Model Selection and Hypothesis Testing: An Extensive Review

Research paper thumbnail of VizieR Online Data Catalog: A high-resolution spectroscopic survey of late-type stars: chromospheric activity, rotation, kinematics, and age

Research paper thumbnail of On the computation of marginal likelihood via MCMC for model selection and hypothesis testing

2020 28th European Signal Processing Conference (EUSIPCO), 2021

Research paper thumbnail of UV image processing to detect diffuse clouds

Research paper thumbnail of Numerical simulations of jet- interstellar medium interactions

Research paper thumbnail of At the rescue of forgotten SNRs with XMM-Newton and Chandra

Research paper thumbnail of A Bayesian inference and model selection algorithm with an optimization scheme to infer the model noise power

Monthly Notices of the Royal Astronomical Society, 2021

Model fitting is possibly the most extended problem in science. Classical approaches include the ... more Model fitting is possibly the most extended problem in science. Classical approaches include the use of least-squares fitting procedures and maximum likelihood methods to estimate the value of the parameters in the model. However, in recent years, Bayesian inference tools have gained traction. Usually, Markov chain Monte Carlo (MCMC) methods are applied to inference problems, but they present some disadvantages, particularly when comparing different models fitted to the same data set. Other Bayesian methods can deal with this issue in a natural and effective way. We have implemented an importance sampling (IS) algorithm adapted to Bayesian inference problems in which the power of the noise in the observations is not known a priori. The main advantage of IS is that the model evidence can be derived directly from the so-called importance weights ā€“ while MCMC methods demand considerable postprocessing. The use of our adaptive target adaptive importance sampling (ATAIS) method is shown ...

Research paper thumbnail of Automatic Tempered Posterior Distributions for Bayesian Inversion Problems

Mathematics, 2021

We propose a novel adaptive importance sampling scheme for Bayesian inversion problems where the ... more We propose a novel adaptive importance sampling scheme for Bayesian inversion problems where the inference of the variables of interest and the power of the data noise are carried out using distinct (but interacting) methods. More specifically, we consider a Bayesian analysis for the variables of interest (i.e., the parameters of the model to invert), whereas we employ a maximum likelihood approach for the estimation of the noise power. The whole technique is implemented by means of an iterative procedure with alternating sampling and optimization steps. Moreover, the noise power is also used as a tempered parameter for the posterior distribution of the the variables of interest. Therefore, a sequence of tempered posterior densities is generated, where the tempered parameter is automatically selected according to the current estimate of the noise power. A complete Bayesian study over the model parameters and the scale parameter can also be performed. Numerical experiments show the b...

Research paper thumbnail of A Likely Magnetic Activity Cycle for the Exoplanet Host M Dwarf GJ 3512

The Astronomical Journal, 2020

Research paper thumbnail of The CARMENES Search for Exoplanets around M Dwarfs: A Low-mass Planet in the Temperate Zone of the Nearby K2-18

The Astronomical Journal, 2018

Research paper thumbnail of TheGaia-ESO Survey: Structural and dynamical properties of the young cluster Chamaeleon I

Astronomy & Astrophysics, 2017

Research paper thumbnail of Formation of X-ray emitting stationary shocks in magnetized protostellar jets

Astronomy & Astrophysics, 2016

Research paper thumbnail of Variation of the ultraviolet extinction law across the Taurus-Auriga star-forming complex. A GALEX based study

Monthly Notices of the Royal Astronomical Society, 2015

Research paper thumbnail of Study of the X-ray Emission of Stars with Hot Jupiters

Research paper thumbnail of VizieR Online Data Catalog: A catalogue of cross-matched radio/infrared/X-ray sources (Combi+, 2011)

Research paper thumbnail of TheGaia-ESO Survey: Extracting diffuse interstellar bands from cool star spectra

Astronomy & Astrophysics, 2014

Research paper thumbnail of Building galaxies, stars, planets and the ingredients for life between the stars. The science behind the European Ultraviolet-Visible Observatory

Astrophysics and Space Science, 2014

Research paper thumbnail of The most distant cluster of galaxies ever detected ?

Research paper thumbnail of Astronomy and astrophysics communication in the UCM Observatory

EAS Publications Series, 2005

Research paper thumbnail of Spectroscopic Monitoring with High Temporal Resolution of the Flare Star AD Leo

Highlights of Spanish Astrophysics III, 2003

... HIGH TEMPORAL RESOLUTION OF THE FLARE STAR AD Leo I. CRESPO-CHACON1, D. MONTES1, J. LOPEZ-SAN... more ... HIGH TEMPORAL RESOLUTION OF THE FLARE STAR AD Leo I. CRESPO-CHACON1, D. MONTES1, J. LOPEZ-SANTIAGO1 MJ FERNANDEZ-FIGUEROA1, D ... galaxies up to redshifts zā‰ˆ 2. 5 for subsequent optical and NIR spectroscopic studies with EMIR and OSIRIS on the ...

Research paper thumbnail of Marginal Likelihood Computation for Model Selection and Hypothesis Testing: An Extensive Review

Research paper thumbnail of VizieR Online Data Catalog: A high-resolution spectroscopic survey of late-type stars: chromospheric activity, rotation, kinematics, and age

Research paper thumbnail of On the computation of marginal likelihood via MCMC for model selection and hypothesis testing

2020 28th European Signal Processing Conference (EUSIPCO), 2021

Research paper thumbnail of UV image processing to detect diffuse clouds

Research paper thumbnail of Numerical simulations of jet- interstellar medium interactions

Research paper thumbnail of At the rescue of forgotten SNRs with XMM-Newton and Chandra

Research paper thumbnail of A Bayesian inference and model selection algorithm with an optimization scheme to infer the model noise power

Monthly Notices of the Royal Astronomical Society, 2021

Model fitting is possibly the most extended problem in science. Classical approaches include the ... more Model fitting is possibly the most extended problem in science. Classical approaches include the use of least-squares fitting procedures and maximum likelihood methods to estimate the value of the parameters in the model. However, in recent years, Bayesian inference tools have gained traction. Usually, Markov chain Monte Carlo (MCMC) methods are applied to inference problems, but they present some disadvantages, particularly when comparing different models fitted to the same data set. Other Bayesian methods can deal with this issue in a natural and effective way. We have implemented an importance sampling (IS) algorithm adapted to Bayesian inference problems in which the power of the noise in the observations is not known a priori. The main advantage of IS is that the model evidence can be derived directly from the so-called importance weights ā€“ while MCMC methods demand considerable postprocessing. The use of our adaptive target adaptive importance sampling (ATAIS) method is shown ...

Research paper thumbnail of Automatic Tempered Posterior Distributions for Bayesian Inversion Problems

Mathematics, 2021

We propose a novel adaptive importance sampling scheme for Bayesian inversion problems where the ... more We propose a novel adaptive importance sampling scheme for Bayesian inversion problems where the inference of the variables of interest and the power of the data noise are carried out using distinct (but interacting) methods. More specifically, we consider a Bayesian analysis for the variables of interest (i.e., the parameters of the model to invert), whereas we employ a maximum likelihood approach for the estimation of the noise power. The whole technique is implemented by means of an iterative procedure with alternating sampling and optimization steps. Moreover, the noise power is also used as a tempered parameter for the posterior distribution of the the variables of interest. Therefore, a sequence of tempered posterior densities is generated, where the tempered parameter is automatically selected according to the current estimate of the noise power. A complete Bayesian study over the model parameters and the scale parameter can also be performed. Numerical experiments show the b...

Research paper thumbnail of A Likely Magnetic Activity Cycle for the Exoplanet Host M Dwarf GJ 3512

The Astronomical Journal, 2020

Research paper thumbnail of The CARMENES Search for Exoplanets around M Dwarfs: A Low-mass Planet in the Temperate Zone of the Nearby K2-18

The Astronomical Journal, 2018

Research paper thumbnail of TheGaia-ESO Survey: Structural and dynamical properties of the young cluster Chamaeleon I

Astronomy & Astrophysics, 2017

Research paper thumbnail of Formation of X-ray emitting stationary shocks in magnetized protostellar jets

Astronomy & Astrophysics, 2016

Research paper thumbnail of Variation of the ultraviolet extinction law across the Taurus-Auriga star-forming complex. A GALEX based study

Monthly Notices of the Royal Astronomical Society, 2015

Research paper thumbnail of Study of the X-ray Emission of Stars with Hot Jupiters

Research paper thumbnail of VizieR Online Data Catalog: A catalogue of cross-matched radio/infrared/X-ray sources (Combi+, 2011)

Research paper thumbnail of TheGaia-ESO Survey: Extracting diffuse interstellar bands from cool star spectra

Astronomy & Astrophysics, 2014

Research paper thumbnail of Building galaxies, stars, planets and the ingredients for life between the stars. The science behind the European Ultraviolet-Visible Observatory

Astrophysics and Space Science, 2014

Research paper thumbnail of The most distant cluster of galaxies ever detected ?

Research paper thumbnail of Astronomy and astrophysics communication in the UCM Observatory

EAS Publications Series, 2005

Research paper thumbnail of Spectroscopic Monitoring with High Temporal Resolution of the Flare Star AD Leo

Highlights of Spanish Astrophysics III, 2003

... HIGH TEMPORAL RESOLUTION OF THE FLARE STAR AD Leo I. CRESPO-CHACON1, D. MONTES1, J. LOPEZ-SAN... more ... HIGH TEMPORAL RESOLUTION OF THE FLARE STAR AD Leo I. CRESPO-CHACON1, D. MONTES1, J. LOPEZ-SANTIAGO1 MJ FERNANDEZ-FIGUEROA1, D ... galaxies up to redshifts zā‰ˆ 2. 5 for subsequent optical and NIR spectroscopic studies with EMIR and OSIRIS on the ...

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