Deep Forcing: Training-Free Long Video Generation with Deep Sink and Participative Compression

Kavli Affiliate: Hsiao-Mei (Sherry) Cho| First 5 Authors: [#item_custom_name[1, [#item_custom_name[2, [#item_custom_name[3, [#item_custom_name[4, [#item_custom_name[5| Summary:Recent advances in autoregressive video diffusion have enabled real-time frame streaming, yet existing solutions still suffer from temporal repetition, drift, and motion deceleration. We find that naively applying StreamingLLM-style attention sinks to video diffusion leads to fidelity degradation and motion stagnation. To […]


Continue.. Deep Forcing: Training-Free Long Video Generation with Deep Sink and Participative Compression

Rethinking the Use of Vision Transformers for AI-Generated Image Detection

Kavli Affiliate: Hsiao-Mei (Sherry) Cho| First 5 Authors: [#item_custom_name[1, [#item_custom_name[2, [#item_custom_name[3, [#item_custom_name[4, [#item_custom_name[5| Summary:Rich feature representations derived from CLIP-ViT have been widely utilized in AI-generated image detection. While most existing methods primarily leverage features from the final layer, we systematically analyze the contributions of layer-wise features to this task. Our study reveals that earlier layers […]


Continue.. Rethinking the Use of Vision Transformers for AI-Generated Image Detection

Anomalous impurity-induced charge modulations in black phosphorus

Kavli Affiliate: Hsiao-Mei (Sherry) Cho| First 5 Authors: [#item_custom_name[1, [#item_custom_name[2, [#item_custom_name[3, [#item_custom_name[4, [#item_custom_name[5| Summary:We observe anomalous charge modulations induced by ionized indium impurities on the surface of the semiconductor black phosphorus by scanning tunneling microscopy (STM). When the im- purities are switched into a negatively charged state by the STM tip, periodic charge modulations emerge […]


Continue.. Anomalous impurity-induced charge modulations in black phosphorus

Characterizing the Low-Mass Pre-Main-Sequence Population in the Low-Metallicity Star-Forming Region Dolidze 25 Using VLT-MUSE

Kavli Affiliate: Gregory Herczeg | Summary:The metallicity of the star-forming environment is a fundamental parameter shaping the evolution of protoplanetary disks and the formation of planetary systems, yet its influence remains poorly constrained. We present a spectroscopic study of low-mass pre-main sequence (PMS) stars ($M < 1 , M_odot$) in the exceptionally metal-poor cluster Dolidze~25 […]


Continue.. Characterizing the Low-Mass Pre-Main-Sequence Population in the Low-Metallicity Star-Forming Region Dolidze 25 Using VLT-MUSE

Uncovering Students’ Inquiry Patterns in GenAI-Supported Clinical Practice: An Integration of Epistemic Network Analysis and Sequential Pattern Mining

Kavli Affiliate: Joel Moore | Summary:Assessment of medication history-taking has traditionally relied on human observation, limiting scalability and detailed performance data. While Generative AI (GenAI) platforms enable extensive data collection and learning analytics provide powerful methods for analyzing educational traces, these approaches remain largely underexplored in pharmacy clinical training. This study addresses this gap by […]


Continue.. Uncovering Students’ Inquiry Patterns in GenAI-Supported Clinical Practice: An Integration of Epistemic Network Analysis and Sequential Pattern Mining

Mini-supernovae from white dwarf-neutron star mergers: Viewing-angle-dependent spectra and lightcurves

Kavli Affiliate: Lijing Shao | Summary:Unstable mass transfer may occur during white dwarf-neutron star (WD-NS) mergers, in which the WD can be tidally disrupted and form an accretion disk around the NS. Such an accretion disk can produce unbound wind ejecta, with synthesized $^56mathrmNi$ mixed in. Numerical simulations reveal that this unbound ejecta should be […]


Continue.. Mini-supernovae from white dwarf-neutron star mergers: Viewing-angle-dependent spectra and lightcurves

Confronting cosmic shear astrophysical uncertainties: DES Year 3 revisited

Kavli Affiliate: George Efstathiou | Summary:Cosmology from weak gravitational lensing has been limited by astrophysical uncertainties in baryonic feedback and intrinsic alignments. By calibrating these effects using external data, we recover non-linear information, achieving a 2% constraint on the clustering amplitude, $S_8$, resulting in a factor of two improvement on the $Λ$CDM constraints relative to […]


Continue.. Confronting cosmic shear astrophysical uncertainties: DES Year 3 revisited

Neuronal calcium spikes enable vector inversion in the Drosophila brain

Kavli Affiliate: Keri Martinowich | Authors: Jason J Rehg, Daniel E Olivares, Ye Li, Keri Martinowich, Greg V Carr and Jorge Miranda-Barrientos | Summary: A typical neuron signals to downstream cells when it is depolarized and firing sodium spikes. Some neurons, however, also fire calcium spikes when hyperpolarized. The function of such bidirectional signaling remains […]


Continue.. Neuronal calcium spikes enable vector inversion in the Drosophila brain

Popcorn EMRIs: Transient Gravitational Wave Signals and Their Analysis in Schwartz Space

Kavli Affiliate: Pau Amaro Seoane | Summary:We investigate extreme-mass ratio inspirals (EMRIs) with orbital periods exceeding the observational timescale of mHz gravitational wave observatories. In their early, highly eccentric phases, these systems generate transient gravitational wave bursts during pericentre passages, separated by long quiescent intervals; we designate these signals “popcorn EMRIs.” We utilize a steady-state […]


Continue.. Popcorn EMRIs: Transient Gravitational Wave Signals and Their Analysis in Schwartz Space

Galactic bars are already mature at Cosmic Noon: bar strength and flatness at z ~ 1.5

Kavli Affiliate: John Silverman | Summary:In this work, we explore the nature of $z>1$ galactic bars. Once thought to be highly transient, our results demonstrate otherwise. Our sample consists of nine massive ($>10^10.5,rm M_odot$) star-forming barred-spiral galaxies at $z_rm spec sim 1.5$. Using rest-frame near-IR (F444W) JWST/NIRCam imaging, we apply ellipse fitting along with 1D […]


Continue.. Galactic bars are already mature at Cosmic Noon: bar strength and flatness at z ~ 1.5