Tootfinder

MultimodalHugs: Enabling Sign Language Processing in Hugging Face
Gerard Sant, Zifan Jiang, Carlos Escolano, Amit Moryossef, Mathias M\"uller, Rico Sennrich, Sarah Ebling
https://arxiv.org/abs/2509.09729

MultimodalHugs: Enabling Sign Language Processing in Hugging Face
In recent years, sign language processing (SLP) has gained importance in the general field of Natural Language Processing. However, compared to research on spoken languages, SLP research is hindered by complex ad-hoc code, inadvertently leading to low reproducibility and unfair comparisons. Existing tools that are built for fast and reproducible experimentation, such as Hugging Face, are not flexible enough to seamlessly integrate sign language experiments. This view is confirmed by a survey we…

Can NLP Tackle Hate Speech in the Real World? Stakeholder-Informed Feedback and Survey on Counterspeech
Tanvi Dinkar, Aiqi Jiang, Simona Frenda, Poppy Gerrard-Abbott, Nancie Gunson, Gavin Abercrombie, Ioannis Konstas
https://arxiv.org/abs/2508.04638

Can NLP Tackle Hate Speech in the Real World? Stakeholder-Informed Feedback and Survey on Counterspeech
Counterspeech, i.e. the practice of responding to online hate speech, has gained traction in NLP as a promising intervention. While early work emphasised collaboration with non-governmental organisation stakeholders, recent research trends have shifted toward automated pipelines that reuse a small set of legacy datasets, often without input from affected communities. This paper presents a systematic review of 74 NLP studies on counterspeech, analysing the extent to which stakeholder participati…

Lithium evolution in the Galactic thin disc from Main-Sequence and early Red-Giant-Branch stars
C. T. Nguyen, G. Cescutti, F. Matteucci, F. Rizzuti, A. Mucciarelli, D. Romano, L. Magrini, A. J. Korn, A. Bressan, L. Girardi
https://arxiv.org/abs/2508.14594

Lithium evolution in the Galactic thin disc from Main-Sequence and early Red-Giant-Branch stars
The role of novae as producers of galactic lithium has been suggested since the 1970s, and it has been reconsidered recently with the detection of $^7$Be in their outbursts. At the same time, stellar models are moving forward to comprehend the discrepancy between the primordial lithium abundance predicted by the standard Big Bang Nucleosynthesis theory and the measured value of old dwarf stars. In this work, we follow the evolution of $^7$Li in the galactic thin disc starting from a primordial …

Silicate clouds and a circumplanetary disk in the YSES-1 exoplanet system
Kielan K. W. Hoch, Melanie Rowland, Simon Petrus, Evert Nasedkin, Carl Ingebretsen, Jens Kammerer, Marshall Perrin, Valentina D'Orazi, William O. Balmer, Travis Barman, Mickael Bonnefoy, Gael Chauvin, Christine Chen, Rob J. De Rosa, Julien Girard, Eileen Gonzales, Matt Kenworthy, Quinn M. Konopacky, Bruce Macintosh, Sarah E. Moran, Caroline V. Morley, Paulina Palma-Bifani, Laurent Pueyo, Bin Ren, Emily Rickma…

Silicate clouds and a circumplanetary disk in the YSES-1 exoplanet system
Young exoplanets provide a critical link between understanding planet formation and atmospheric evolution. Direct imaging spectroscopy allows us to infer the properties of young, wide orbit, giant planets with high signal-to-noise. This allows us to compare this young population to exoplanets characterized with transmission spectroscopy, which has indirectly revealed the presence of clouds, photochemistry, and a diversity of atmospheric compositions. Direct detections have also been made for br…

The mid-infrared spectrum of $\beta$ Pictoris b. First VLTI/MATISSE interferometric observations of an exoplanet
M. Houll\'e, F. Millour, P. Berio, J. Scigliuto, S. Lacour, B. Lopez, F. Allouche, J. -C. Augereau, D. Blain, M. Bonnefoy, M. Carbillet, G. Chauvin, J. Leftley, A. Matter, J. Milli, P. Molli\`ere, E. Nasedkin, M. Nowak, P. Palma-Bifani, \'E. Pantin, P. Priolet, M. Ravet, J. Woillez, W. Balmer, P. Boley, V. G\'amez Rosas, J. H. Girard, X. Haubois, S. Hinkley, M. H…

The mid-infrared spectrum of $β$ Pictoris b. First VLTI/MATISSE interferometric observations of an exoplanet
Few spectra of directly-imaged exoplanets have been obtained in the mid-infrared (> 3 $μ$m). This region is particularly rich in molecular spectral signatures, whose measurements can help recover atmospheric parameters and provide a better understanding of giant planet formation and atmospheric dynamics. In the past years, exoplanet interferometry with the VLTI/GRAVITY instrument has provided medium-resolution spectra of a dozen substellar companions in the near infrared. The 100-meter interfe…