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R. Fernández

Publications and source records attributed to R. Fernández.

4 recordsLinked to original sources

Identification of Separable OTUs for Multinomial Classification in Compositional Data Analysis

High-throughput sequencing has transformed microbiome research, but it also produces inherently compositional data that challenge standard statistical and machine learning methods. In this work, we propose a multinomial classification framework for compositional microbiome data based on penalized log-ratio regression and pairwise separability screening. The method quantifies the discriminative ability of each OTU through the area under the receiver operating characteristic curve ($AUC$) for all pairwise log-ratios and aggregates these values into a global separability index $S_k$, yielding interpretable rankings of taxa together with confidence intervals. We illustrate the approach by reanalyzing the Baxter colorectal adenoma dataset and comparing our results with Greenacre's ordination-based analysis using Correspondence Analysis and Canonical Correspondence Analysis. Our models consistently recover a core subset of taxa previously identified as discriminant, thereby corroborating Greenacre's main findings, while also revealing additional OTUs that become important once demographic covariates are taken into account. In particular, adjustment for age, gender, and diabetes medication improves the precision of the separation index and highlights new, potentially relevant taxa, suggesting that part of the original signal may have been influenced by confounding. Overall, the integration of log-ratio modeling, covariate adjustment, and uncertainty estimation provides a robust and interpretable framework for OTU selection in compositional microbiome data. The proposed method complements existing ordination-based approaches by adding a probabilistic and inferential perspective, strengthening the identification of biologically meaningful microbial signatures.

stat.AP↗

Don't Buy it! Reassessing the Ad Understanding Abilities of Contrastive Multimodal Models

Image-based advertisements are complex multimodal stimuli that often contain unusual visual elements and figurative language. Previous research on automatic ad understanding has reported impressive zero-shot accuracy of contrastive vision-and-language models (VLMs) on an ad-explanation retrieval task. Here, we examine the original task setup and show that contrastive VLMs can solve it by exploiting grounding heuristics. To control for this confound, we introduce TRADE, a new evaluation test set with adversarial grounded explanations. While these explanations look implausible to humans, we show that they "fool" four different contrastive VLMs. Our findings highlight the need for an improved operationalisation of automatic ad understanding that truly evaluates VLMs' multimodal reasoning abilities. We make our code and TRADE available at https://github.com/dmg-illc/trade .

cs.CL↗

The Role of Magnetic Field Geometry in the Evolution of Neutron Star Merger Accretion Discs

Neutron star mergers are unique laboratories of accretion, ejection, and r-process nucleosynthesis. We used 3D general relativistic magnetohydrodynamic simulations to study the role of the post-merger magnetic geometry in the evolution of merger remnant discs around stationary Kerr black holes. Our simulations fully capture mass accretion, ejection, and jet production, owing to their exceptionally long duration exceeding $4$ s. Poloidal post-merger magnetic field configurations produce jets with energies $E_\mathrm{jet} \sim (4{-}30)\times10^{50}$ erg, isotropic equivalent energies $E_\mathrm{iso}\sim(4{-}20)\times10^{52}$ erg, opening angles $θ_\mathrm{jet}\sim6{-}13^\circ$, and durations $t_j\lesssim1$ s. Accompanying the production of jets is the ejection of $f_\mathrm{ej}\sim30{-}40\%$ of the post-merger disc mass, continuing out to times $> 1$ s. We discover that a more natural, purely toroidal post-merger magnetic field geometry generates large-scale poloidal magnetic flux of alternating polarity and striped jets. The first stripe, of $E_\mathrm{jet}\simeq2\times10^{48}\,\mathrm{erg}$, $E_\mathrm{iso}\sim10^{51}$ erg, $θ_\mathrm{jet}\sim3.5{-}5^\circ$, and $t_j\sim0.1$ s, is followed by $\gtrsim4$ s of striped jet activity with $f_\mathrm{ej}\simeq27\%$. The dissipation of such stripes could power the short gamma-ray burst (sGRB) prompt emission. Our simulated jet energies and durations span the range of sGRBs. We find that although the blue kilonova component is initially hidden from view by the red component, it expands faster, outruns the red component, and becomes visible to off-axis observers. In comparison to GW 170817/GRB 170817A, our simulations under-predict the mass of the blue relative to red component by a factor of few. Including the dynamical ejecta and neutrino absorption may reduce this tension.

astro-ph.HE↗

Possible loss and recovery of Gibbsianness during the stochastic evolution of Gibbs measures

We consider Ising-spin systems starting from an initial Gibbs measure $ν$ and evolving under a spin-flip dynamics towards a reversible Gibbs measure $μ\not=ν$. Both $ν$ and $μ$ are assumed to have a finite-range interaction. We study the Gibbsian character of the measure $νS(t)$ at time $t$ and show the following: (1) For all $ν$ and $μ$, $νS(t)$ is Gibbs for small $t$. (2) If both $ν$ and $μ$ have a high or infinite temperature, then $νS(t)$ is Gibbs for all $t>0$. (3) If $ν$ has a low non-zero temperature and a zero magnetic field and $μ$ has a high or infinite temperature, then $νS(t)$ is Gibbs for small $t$ and non-Gibbs for large $t$. (4) If $ν$ has a low non-zero temperature and a non-zero magnetic field and $μ$ has a high or infinite temperature, then $νS(t)$ is Gibbs for small $t$, non-Gibbs for intermediate $t$, and Gibbs for large $t$. The regime where $μ$ has a low or zero temperature and $t$ is not small remains open. This regime presumably allows for many different scenarios.

math-ph↗