Breaking the Blend: A multi-tracer kinematic decomposition method for IFS data applied to disentangling the AGN outflow and circumnuclear ring in NGC 5728 with JWST

Kavli Affiliate: Claudio Ricci | Summary:Integral field spectroscopy (IFS) of the central kiloparsecs of active galactic nuclei (AGN) reveals a mixture of spatially coincident emission from star-formation and AGN feedback exciting the interstellar medium. Disentangling these components remains a challenge, as most spectral tracers are affected by both processes, limiting robust interpretation of kinematics and […]


Continue.. Breaking the Blend: A multi-tracer kinematic decomposition method for IFS data applied to disentangling the AGN outflow and circumnuclear ring in NGC 5728 with JWST

Breaking the Blend: A multi-tracer kinematic decomposition method for IFS data applied to disentangling the AGN outflow and circumnuclear ring in NGC 5728 with JWST

Kavli Affiliate: Claudio Ricci | Summary:Integral field spectroscopy (IFS) of the central kiloparsecs of active galactic nuclei (AGN) reveals a mixture of spatially coincident emission from star-formation and AGN feedback exciting the interstellar medium. Disentangling these components remains a challenge, as most spectral tracers are affected by both processes, limiting robust interpretation of kinematics and […]


Continue.. Breaking the Blend: A multi-tracer kinematic decomposition method for IFS data applied to disentangling the AGN outflow and circumnuclear ring in NGC 5728 with JWST

A Helical Trajectory Interpretation of a Multi-wavelength Event in a Blazar S5 0716+714

Kavli Affiliate: Luis Ho | Summary:Relativistic jets in blazars exhibit strong variability across multiple timescales, but the connection between temporal variability and the evolution of jet structures remains poorly understood. In this work, we investigate the $γ$-ray variability of the BL Lac object S5 0716+714 from July 2014 to June 2015 and explore its possible […]


Continue.. A Helical Trajectory Interpretation of a Multi-wavelength Event in a Blazar S5 0716+714

Stellar Collisions from Self-consistent Stellar Dynamics Around Growing Supermassive black Holes

Kavli Affiliate: Pau Amaro Seoane | Summary:The centers of galaxies harbor the densest stellar environments, where a massive black hole (MBH) accelerates stars to such high velocities that direct collisions can result in high-energetic phenomena, such as gravitational wave sources, kilonovae, and supernova-like transients. These collisions can reshape the cluster’s density profile and release gas […]


Continue.. Stellar Collisions from Self-consistent Stellar Dynamics Around Growing Supermassive black Holes

A Tendon-Driven Robotic Jellyfish with Constrained Soft Actuation and Depth Control via Reinforcement Learning

Kavli Affiliate: Xian Chen| Summary: Jellyfish-inspired robots offer a compliant and efficient approach to underwater locomotion, but achieving large deformation together with repeatable actuation and closed-loop control remains challenging. In this work, we present a tendon-driven robotic jellyfish with constrained soft actuation. Each actuator combines a flexible substrate with discrete constraints, enabling bending up to […]


Continue.. A Tendon-Driven Robotic Jellyfish with Constrained Soft Actuation and Depth Control via Reinforcement Learning

Ubiquitous nuclear disks and bars embedded in massive galaxies in the cosmic morning

Kavli Affiliate: Luis Ho | Summary:The morphology of the central regions of high-redshift galaxies remains relatively unexplored, while recent case studies suggest that giant disks can emerge without first developing a prominent central spheroid. Here, we investigate the inner structures of a mass-complete sample of 45 massive galaxies at $z=3$ in the TNG50 simulation. Through […]


Continue.. Ubiquitous nuclear disks and bars embedded in massive galaxies in the cosmic morning

Mass Distribution of M31 from its Rotation Curve up to 167 kpc

Kavli Affiliate: Huawei Zhang | Summary:The mass distribution of the Andromeda galaxy (M31) is fundamental for understanding its dark matter content, assembly history, and dynamical role within the Local Group. However, estimates of M31’s total mass remain quite uncertain, partly because of limited dynamical constraints at large galactocentric radii. Moreover, M31’s recent merger history has […]


Continue.. Mass Distribution of M31 from its Rotation Curve up to 167 kpc

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

Hydrogen Line Emission in Accreting Low-Mass Objects I: Spectral Analysis of Shock-Origin Narrow Component

Kavli Affiliate: Gregory Herczeg | Summary:Hydrogen lines are widely used as tracers of stellar and planetary accretion. In classical T~Tauri stars, hydrogen lines are usually interpreted as arising from magnetospheric accretion columns, whereas in lower-mass counterparts (subsolar-mass objects including brown dwarfs and gas giant planets), the post-accretion-shock region can directly emit a substantial fraction of […]


Continue.. Hydrogen Line Emission in Accreting Low-Mass Objects I: Spectral Analysis of Shock-Origin Narrow Component

On the Detectability and Measurement of Galactic Bars as a Function of Redshift

Kavli Affiliate: Luis Ho | Summary:The cosmic evolution of galactic bars offers key insights into the dynamical history of disk galaxies. However, studies of high-redshift bars are severely hampered by observational effects such as resolution degradation and surface brightness dimming. To quantify these biases and establish a robust methodology of bar detection and measurement for […]


Continue.. On the Detectability and Measurement of Galactic Bars as a Function of Redshift