The JDISC Survey: Inner Disk Chemistry of Class I/FS Disks and Tentative Evidence for Early Pebble Drift

Kavli Affiliate: Feng Long| Summary: We present the first chemical survey of Class I and Flat-Spectrum (I/FS) disks using JWST MIRI/MRS, targeting sixteen sources in the Ophiuchus star-forming region. Through empirical line luminosity measurements and multi-component slab modeling, we characterize the molecular reservoir of these young systems and compare them to twelve Class II disks […]


Continue.. The JDISC Survey: Inner Disk Chemistry of Class I/FS Disks and Tentative Evidence for Early Pebble Drift

Elliptical Regularized Hotelling Tests for High-Dimensional Change-Point Detection

Kavli Affiliate: Feng Long| Summary: We propose an elliptical regularized Hotelling (ERHT) procedure for detecting location changes in high-dimensional sequences with heavy-tailed, cross-sectionally dependent observations. ERHT contrasts spatial medians on adjacent segments using a ridge-regularized inverse of the pooled centered spatial-sign covariance matrix, thereby combining robustness to radial variation with dependence-aware weighting. We establish Gaussian-process […]


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The Distinctive Evolution and Spectral Energy Distribution of Binary Massive Black Hole Accretion

Kavli Affiliate: Luis Ho | Summary:Binary (super-)massive black holes (BHs) are expected to reside in the center of some galaxies. In this work, we re-visit accretion onto binary massive BHs, incorporating recent advances in both accretion theory and the mass transfer rate between the two massive BHs. We focus on relatively bright systems with an […]


Continue.. The Distinctive Evolution and Spectral Energy Distribution of Binary Massive Black Hole Accretion

JWST/MIRI Reveals the Evolution from Molecular to Atomic Disk Winds

Kavli Affiliate: Gregory Herczeg | Summary:The evolution and dispersal of protoplanetary disks–governed by accretion, magnetically launched jets and winds, and photoevaporative winds–fundamentally shape planetary systems. Determining how these mass-loss processes co-evolve is crucial for constraining planet formation pathways. We analyze archival JWST/MIRI/IFU data of 72 inclined (i>40deg) mostly ClassII disks to identify and characterize spatially […]


Continue.. JWST/MIRI Reveals the Evolution from Molecular to Atomic Disk Winds

High-Dimensional Change Point Analysis for Temporally Dependent Data

Kavli Affiliate: Feng Long| Summary: This paper develops adaptive procedures for detecting and locating mean changes in high-dimensional time series. Quadratic CUSUM statistics target dense changes, whereas coordinatewise maximum statistics target sparse changes. Two weighting schemes are considered to accommodate both interior and boundary changes. Under general non-Gaussian vector dependence, we establish the limiting distributions, […]


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A dust-free hierarchically nested supermassive-star model for James Webb Space Telescope Little Red Dots

Kavli Affiliate: Pau Amaro Seoane | Summary:Observations by the James Webb Space Telescope reveal a population of high-redshift objects, the little red dots. These sources exhibit optical reddening alongside blue ultraviolet continua, host broad Balmer lines indicative of active black holes, and lack detectable x-ray emission. Their cosmic abundance at early epochs exceeds standard Eddington-limited […]


Continue.. A dust-free hierarchically nested supermassive-star model for James Webb Space Telescope Little Red Dots

Extreme Variability Reveals How the Eddington Ratio Regulates Coronal Power in Active Galactic Nuclei

Kavli Affiliate: Luis Ho | Summary:The bolometric luminosity ($L_rm bol$) of active galactic nuclei (AGNs) is a key tracer of accretion physics, but its direct determination is often hindered by limited spectral coverage and contamination of the host galaxy. Bolometric corrections ($κ_λ = L_rm bol/L_λ$) offer a practical means of estimating $L_rm bol$, with the […]


Continue.. Extreme Variability Reveals How the Eddington Ratio Regulates Coronal Power in Active Galactic Nuclei

Extreme Variability Reveals How the Eddington Ratio Regulates Coronal Power in Active Galactic Nuclei

Kavli Affiliate: Luis Ho | Summary:The bolometric luminosity ($L_rm bol$) of active galactic nuclei (AGNs) is a key tracer of accretion physics, but its direct determination is often hindered by limited spectral coverage and contamination of the host galaxy. Bolometric corrections ($κ_λ = L_rm bol/L_λ$) offer a practical means of estimating $L_rm bol$, with the […]


Continue.. Extreme Variability Reveals How the Eddington Ratio Regulates Coronal Power in Active Galactic Nuclei

Star formation powers optical line emission from the CGM

Kavli Affiliate: Luis Ho | Summary:Using integral field spectroscopy, we explore the disk-halo interface, or the inner circumgalactic medium (CGM), of individual galaxies by constructing and analyzing emission-line maps for a large sample (72) of normal, low-redshift galaxies spanning three orders of magnitude in stellar mass and four orders in star formation rate (SFR). We […]


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Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots

Kavli Affiliate: Luis Ho | Summary:Recent JWST observations have revealed a population of compact, optically red sources known as Little Red Dots (LRDs). A popular interpretation is that LRDs host massive black holes embedded in dense gaseous envelopes, yet the physical origin of such envelopes remains unclear. We propose that the optically thick outflow driven […]


Continue.. Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots