GATOS N: Extended circumnuclear dust emission in nearby Seyfert galaxies surveyed by JWST/MIRI

Kavli Affiliate: Claudio Ricci | Summary:The subarcsecond angular resolution and stable background of JWST has given us the first high-fidelity images of the arcsecond-scale environment around Active Galactic Nuclei (AGNs) in the nearby Universe. With mid-infrared (MIR) surface brightness sensitivities that are much deeper than the best ground-based instruments, the Mid-InfraRed Instrument imager (MIRIM) now […]


Continue.. GATOS N: Extended circumnuclear dust emission in nearby Seyfert galaxies surveyed by JWST/MIRI

GATOS XV: A JWST/MIRI survey of extended circumnuclear dust emission in nearby Seyfert galaxies

Kavli Affiliate: Claudio Ricci | Summary:The subarcsecond angular resolution and stable background of JWST has given us the first high-fidelity images of the arcsecond-scale environment around Active Galactic Nuclei (AGNs) in the nearby Universe. With mid-infrared (MIR) surface brightness sensitivities that are much deeper than the best ground-based instruments, the Mid-InfraRed Instrument imager (MIRIM) now […]


Continue.. GATOS XV: A JWST/MIRI survey of extended circumnuclear dust emission in nearby Seyfert galaxies

Cauchy Aggregation of Ridge-Regularized Hotelling Tests for High-Dimensional Change-Point Detection

Kavli Affiliate: Feng Long| Summary: Ridge-regularized Hotelling-type (RHT) change-point tests depend on a ridge parameter $λ$, but the power-optimal value is determined by the unknown covariance structure and the unknown mean shift. We avoid selecting a single ridge value by computing fixed-ridge p-values on a finite deterministic grid and aggregating them with the Cauchy combination […]


Continue.. Cauchy Aggregation of Ridge-Regularized Hotelling Tests for High-Dimensional Change-Point Detection

Ultraviolet Imaging of SR 12 c with HST/WFC3: Accretion and Variability of a Giant Planet at the End Stages of Growth

Kavli Affiliate: Gregory Herczeg | Summary:Many details of the gas accretion phase during giant planet formation remain untested. We present new 0.2$unicodex2013$0.7 $μ$m UV-through-red optical imaging of the young, wide-orbit planetary-mass companion SR 12 c from the Wide Field Camera 3 (WFC3) instrument on board the Hubble Space Telescope. SR 12 c exhibits strong accretion-related […]


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DESI as sparse Integral Field Spectrograph I: Spatially resolved chemical enrichment in star-forming galaxies at $zleq0.1$

Kavli Affiliate: Luis Ho | Summary:We present a spatially resolved chemical abundance analysis of 2291 star-forming galaxies at $z leq 0.1$, spanning nearly four orders of magnitude in stellar mass ($8 le rm log (M_star/M_odot) le 11.5$), by exploiting the multi-fibre spectra from the Dark Energy Spectroscopic Instrument (DESI) as a sparse integral field spectrograph. […]


Continue.. DESI as sparse Integral Field Spectrograph I: Spatially resolved chemical enrichment in star-forming galaxies at $zleq0.1$

Unification models of Active Galactic Nuclei

Kavli Affiliate: Claudio Ricci | Summary:This chapter presents an overview of the unification models for Active Galactic Nuclei (AGN), focusing on the physical structures, classification schemes, and evolutionary processes that characterize accreting supermassive black holes. We introduce the fundamental components of AGN, including the supermassive black hole, accretion disk, jets, outflows, broad-line and narrow-line regions, […]


Continue.. Unification models of Active Galactic Nuclei

Unification models of Active Galactic Nuclei

Kavli Affiliate: Claudio Ricci | Summary:This chapter presents an overview of the unification models for Active Galactic Nuclei (AGN), focusing on the physical structures, classification schemes, and evolutionary processes that characterize accreting supermassive black holes. We introduce the fundamental components of AGN, including the supermassive black hole, accretion disk, jets, outflows, broad-line and narrow-line regions, […]


Continue.. Unification models of Active Galactic Nuclei

Detection of a parsec-scale, compact, and fading ejecta from an accreting massive black hole

Kavli Affiliate: Luis Ho | Summary:Dwarf galaxies, characterized by their low luminosities and masses, are excellent candidates for searches for intermediate-mass black holes (IMBHs), particularly when they show strong accretion and ejection activity. The dwarf galaxy SDSS J101747.09+393207.7 has recently been found to display a very high X-ray luminosity and an X-shaped optical structure, possibly […]


Continue.. Detection of a parsec-scale, compact, and fading ejecta from an accreting massive black hole

Differentially Private Range Subgraph Counting

Kavli Affiliate: Xian Chen| Summary: Subgraph counting is a fundamental problem in graph analysis. Motivated by practical scenarios where graph analytics are performed on subgraphs induced by selected vertices — rather than on the entire graph — and by growing privacy concerns, we initiate the study of differentially private range subgraph counting (DPRSC). The goal […]


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Radiation Pressure Instability in the “turn-on” Changing-Look AGN SDSS J1430+2303

Kavli Affiliate: Claudio Ricci | Summary:We aim to investigate the multi-wavelength variability, spectral, and timing properties of the changing-look active galactic nucleus (CL AGN) SDSS J1430+2303, and to explore the physical origin of its peculiar variability pattern that has not been observed before in other CL AGN. We perform a multi-wavelength analysis using optical, ultraviolet, […]


Continue.. Radiation Pressure Instability in the “turn-on” Changing-Look AGN SDSS J1430+2303