Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution

Kavli Affiliate: Luis Ho | Summary:An intriguing puzzle in extragalactic astronomy is the scarcity of Little Red Dots (LRDs) at $z < 3$, compared to their higher abundance at earlier cosmic epochs. To investigate this, we measure the overdensity for 98 specpically confirmed LRDs at $3<z<7$, and find that these LRDs predominantly reside in under-dense […]


Continue.. Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution

Reduced incidence of little red dots at z < 3 based on number density and halo mass evolution

Kavli Affiliate: Luis Ho | Summary:An intriguing puzzle in extragalactic astronomy is the scarcity of Little Red Dots (LRDs) at $z < 3$, compared to their higher abundance at earlier cosmic epochs. To investigate this, we measure the overdensity for 98 specpically confirmed LRDs at $3<z<7$, and find that these LRDs predominantly reside in under-dense […]


Continue.. Reduced incidence of little red dots at z < 3 based on number density and halo mass evolution

An archival summary: 15 years of ALMA observations on disks and planet formation

Kavli Affiliate: Feng Long| Summary: The Atacama Large (sub-)millimeter Array (ALMA) has been in scientific operations for almost 15 years. We celebrate this achievement by providing a summary of the “Disks and planet formation” scientific category, with an emphasis on the disks located in the nearby star-forming regions. As of the beginning of February 2026, […]


Continue.. An archival summary: 15 years of ALMA observations on disks and planet formation

Transient Signatures of Star-Envelope Collisions in Little Red Dots

Kavli Affiliate: Kohei Inayoshi | Summary:Little red dots (LRDs) are compact high-redshift objects, newly discovered by the James Webb Space Telescope. Although LRDs exhibit broad Balmer emission lines suggestive of the presence of active galactic nuclei (AGN), their spectral features differ significantly from those of ordinary AGN. Recent studies suggest that their characteristics can be […]


Continue.. Transient Signatures of Star-Envelope Collisions in Little Red Dots

LoopFM: Learning frOm HistOrical RePresentations of Foundation Model for Recommendation

Kavli Affiliate: Xian Chen| Summary: Knowledge distillation (KD) transfers a single scalar prediction from a large foundation model (FM) to compact vertical models (VMs), suffering from diminishing transfer ratio — the fraction of FM improvement captured by the VM — as a single scalar cannot convey the rich intermediate knowledge that larger FMs learn. To […]


Continue.. LoopFM: Learning frOm HistOrical RePresentations of Foundation Model for Recommendation

LoopFM: Learning frOm HistOrical RePresentations of Foundation Model for Recommendation

Kavli Affiliate: Xian Chen| Summary: Knowledge distillation (KD) transfers a single scalar prediction from a large foundation model (FM) to compact vertical models (VMs), suffering from diminishing transfer ratio — the fraction of FM improvement captured by the VM — as a single scalar cannot convey the rich intermediate knowledge that larger FMs learn. To […]


Continue.. LoopFM: Learning frOm HistOrical RePresentations of Foundation Model for Recommendation

LoopFM: Learning frOm HistOrical RePresentations of Foundation Model for Recommendation

Kavli Affiliate: Xian Chen| Summary: Knowledge distillation (KD) transfers a single scalar prediction from a large foundation model (FM) to compact vertical models (VMs), suffering from diminishing transfer ratio — the fraction of FM improvement captured by the VM — as a single scalar cannot convey the rich intermediate knowledge that larger FMs learn. To […]


Continue.. LoopFM: Learning frOm HistOrical RePresentations of Foundation Model for Recommendation

Evidence for Systematically Larger Dust Grains in Upper Scorpius Relative to Taurus Disks

Kavli Affiliate: Feng Long| Summary: Infrared spectroscopy provides a powerful diagnostic for probing the mineralogical properties of dust grains in the terrestrial planet-forming regions of protoplanetary disks. The Upper Scorpius association offers an excellent laboratory for studying disk evolution because it represents an evolved stage (5-10 Myr) compared with younger star-forming regions such as the […]


Continue.. Evidence for Systematically Larger Dust Grains in Upper Scorpius Relative to Taurus Disks

Rank-Based Tests for Mutual Independence of High-Dimensional Random Vectors via $L_q$ Norm

Kavli Affiliate: Feng Long| Summary: We consider the problem of testing mutual independence among the components of a high-dimensional random vector. Building on the rank-based max-sum framework, we introduce fixed finite-$L_q$ power-sum statistics under three general classes of rank-based correlations: simple linear rank statistics, non-degenerate rank-based U-statistics and degenerate rank-based U-statistics. The proposed statistics interpolate […]


Continue.. Rank-Based Tests for Mutual Independence of High-Dimensional Random Vectors via $L_q$ Norm

Strong X-ray Variability of I Zwicky 1: Obscuration from Clumpy Accretion-Disk Winds

Kavli Affiliate: Luis Ho | Summary:Obscuration from clumpy accretion-disk winds has been invoked to explain the extreme X-ray weakness and X-ray variability observed in a substantial fraction of super-Eddington accreting quasars. We present a comprehensive study of the strong X-ray variability of the super-Eddington accreting active galactic nucleus (AGN) I Zwicky 1 (I Zw 1), […]


Continue.. Strong X-ray Variability of I Zwicky 1: Obscuration from Clumpy Accretion-Disk Winds