High-Dimensional Two-Sample Inference via Marginal Likelihood-Ratio Rank Statistics

Kavli Affiliate: Feng Long| Summary: We develop a rank-based framework for high-dimensional two-sample testing that detects marginal distributional differences beyond means and variances. Three marginal likelihood-ratio statistics generate SUM tests for widespread differences, MAX tests for concentrated departures, and Cauchy combinations for unknown signal sparsity. The procedures retain all pooled ranks and impose no moment […]


Continue.. High-Dimensional Two-Sample Inference via Marginal Likelihood-Ratio Rank Statistics

Supernova origin of galactic turbulence revealed by superbubbles

Kavli Affiliate: Lile Wang |Summary:Supernovae (SNe) are among the leading candidates for powering galactic-scale turbulence. SNe drive expanding shells of neutral atomic hydrogen (HI) known as superbubbles. Due to the lack of a sensitive, dynamically complete, galaxy-wide census, superbubbles have not been used to quantify the galactic-scale turbulent energy budget. Here we present a combined […]


Continue.. Supernova origin of galactic turbulence revealed by superbubbles

High Resolution Grid-based Simulations of the Warm-Hot Intergalactic Medium

Kavli Affiliate: Lile Wang |Summary:We present high-resolution cosmological hydrodynamic simulations of the Warm-Hot Intergalactic Medium (WHIM) using the GPU-optimized grid-based hydrodynamic code Kratos. Employing a uniform 4096^3 grid in a (100 h^-1 Mpc)^3 comoving volume, we achieve a spatial resolution of ~24.5 h^-1 kpc, sufficient to resolve the Jeans scale of gas at T ~ […]


Continue.. High Resolution Grid-based Simulations of the Warm-Hot Intergalactic Medium

Diagonalized Attention for Individualized Regression: Latent-Row Localization and Prediction

Kavli Affiliate: Feng Long| Summary: Modern text and image representations are often matrix-valued, with rows corresponding to tokens, patches, or other local feature vectors. Predictive information is often sparse but sample-specific, making classical sparse regression methods with a common support poorly suited to this heterogeneity. This paper formalizes an individualized sparse regression framework for matrix-valued […]


Continue.. Diagonalized Attention for Individualized Regression: Latent-Row Localization and Prediction

Free-Free Radio Emission from Little Red Dots as a Probe of Ionized Gas

Kavli Affiliate: Kohei Inayoshi | Summary:Recent studies have hypothesized that little red dots (LRDs) are rapidly accreting black holes surrounded by dense gaseous environments. Both neutral and ionized gas play a key role in explaining many of the puzzling spectral features of LRDs, including the emission line profiles in the optical-infrared bands, although the physical […]


Continue.. Free-Free Radio Emission from Little Red Dots as a Probe of Ionized Gas

Extremal Scalarization of Charged Black Holes: Miransky Scaling across Reissner-Nordström Extremality

Kavli Affiliate: Lijing Shao | Summary:We study spontaneous scalarization near and at extremality in Einstein-Maxwell-scalar theory. As Reissner-Nordström (RN) extremality is approached from below, the nonextremal scalarization existence curves collapse toward a common critical threshold $α_c=1/4$ given by the Breitenlohner-Freedman bound for the near-horizon throat (AdS$_2times S^2$) of its extremal black hole. For a polynomial […]


Continue.. Extremal Scalarization of Charged Black Holes: Miransky Scaling across Reissner-Nordström Extremality

The Contribution of Starspots to the Lithium Spread in NGC 2264

Kavli Affiliate: Gregory Herczeg | Summary:Star clusters with ages of a few Myr have a previously unexplained dispersion in the lithium equivalent widths. In this work, we show that much of the lithium spread of the young cluster NGC 2264 can be attributed to the observational presence of starspots. We demonstrate that the equivalent width […]


Continue.. The Contribution of Starspots to the Lithium Spread in NGC 2264

Pushing HST to the limit: Detection completeness and morphology robustness of faint galaxies in the EGS field

Kavli Affiliate: Luis Ho | Summary:Reliable catalogs at the faint limit are essential for statistical studies of galaxy evolution. However, detection and structural measurements of faint galaxies remain challenging. We evaluate detection completeness and structural parameter uncertainties of faint galaxies in the CANDELS/EGS field using mock images and observations from the HST and JWST. The […]


Continue.. Pushing HST to the limit: Detection completeness and morphology robustness of faint galaxies in the EGS field

Multi-wavelength Constraints on Dust Dynamics and Size Evolution in Protoplanetary Disk Rings. II. Observational Implications

Kavli Affiliate: Ruobing Dong | Summary:Spatially resolved dust rings in protoplanetary disks are widely used to infer disk and dust physics from multi-wavelength continuum observations. Their interpretation, however, often neglects grain growth and the evolution of the size distribution, limiting the connection between observed ring profiles and dust-evolution parameters. Building on a physical dust-ring model […]


Continue.. Multi-wavelength Constraints on Dust Dynamics and Size Evolution in Protoplanetary Disk Rings. II. Observational Implications

Forged in Quenching: Morphological Transformation across Star-forming and Quiescent Galaxies in EAGLE

Kavli Affiliate: Yingjie Peng | Summary:The connection between morphology and quenching in central galaxies is well established, but its physical origin remains widely debated. We address this by tracing the main progenitor branches of $z=0$ star-forming and quiescent central galaxies in the EAGLE cosmological simulation from $zgtrsim4$. Their disc-to-total ratio and triaxiality tracks are indistinguishable […]


Continue.. Forged in Quenching: Morphological Transformation across Star-forming and Quiescent Galaxies in EAGLE