SMA Observations Reveal Abundant HNC Chemistry in Transition Disks

Kavli Affiliate: Feng Long| Summary: The physical and chemical conditions of protoplanetary disks shape the properties of nascent planetary systems. The line ratios and relative abundances of the HCN-HNC isomer pair are well-suited for tracing these gas conditions, since isomer chemistry is linked to the underlying temperature, elemental abundances, and irradiation environment of the emitting […]


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Kratos-linerad: GPU-accelerated Monte Carlo radiative transfer of lines with efficient imaging

Kavli Affiliate: Lile Wang |Summary:Spectral lines encode the velocity, the temperature, and the chemical structure of astrophysical gas; interpreting them requires radiative transfer that is accurate at high optical depth, consistent with the local excitation, and efficient enough to synthesize velocity-resolved images. We present Kratos-linerad, a GPU-accelerated Monte Carlo radiative transfer code for spectral lines. […]


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Factor-Adjusted Location Tests for High-Dimensional Time Series

Kavli Affiliate: Feng Long| Summary: We study high-dimensional one-sample mean testing for time series with strong common serial dependence driven by latent dynamic factors. After estimating the dynamic factor loading space from lagged autocovariance, we project the data onto its orthogonal complement and construct three factor-adjusted tests: a max test for sparse alternatives, a quadratic […]


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Luminosity function of quasars at $1.0

Kavli Affiliate: Linhua Jiang | Summary:We present a study of the evolution of type 1 quasars at $1.0<z<3.5$, covering the peak epoch of quasar activity. The quasar evolution has been extensively explored by a variety of previous works and the derived quasar luminosity functions (QLFs) are not well consistent with each other, presumably due to […]


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SMA 200-400 GHz Survey for 10 faint Class II Disks in the Taurus Molecular Cloud

Kavli Affiliate: Feng Long| Summary: We have performed Submillimeter Array (SMA) observations of 198.0-407.5 GHz broadband spectra of 10 Class II protoplanetary disks in the Taurus-Auriga region. The 337 GHz flux densities ($F_rm 337 GHz$) of these objects are in the range of 8.2-34 mJy. The median and standard deviation of the 198-358 GHz spectral […]


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Inflow-driven galaxy evolution – I. Revealing the physics of the fundamental metallicity relation

Kavli Affiliate: Yingjie Peng | Summary:We present a unified physical framework for the fundamental metallicity relation (FMR), based on the mass-continuity equations. The FMR is not merely the anti-correlation between star formation rate (SFR) and gas metallicity ($Z_rm g$) at fixed stellar mass ($M_star$); it is a redshift-invariant surface in the $(M_star,rm SFR,Z_rm g)$ space. […]


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V557 Mon: Hot water vapour observed on an eruptive young star

Kavli Affiliate: Gregory Herczeg | Summary:In this paper, we present observations of an eruptive young star in the Rosette Nebula, identified by the Gaia Science Alerts system using Gaia time series data. We aim to investigate the evolution of the brightness and mass accretion rate of V557 Mon throughout its outburst and subsequent decline. In […]


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Hot water emission during an outburst on a classical T Tauri star

Kavli Affiliate: Gregory Herczeg | Summary:In this paper, we present observations of an eruptive young star in the Rosette Nebula, identified by the Gaia Science Alerts system using Gaia time series data. We aim to investigate the evolution of the brightness and mass accretion rate of V557 Mon throughout its outburst and subsequent decline. In […]


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XRISM Resolves the Circum-nuclear Environment of NGC 4945

Kavli Affiliate: Claudio Ricci | Summary:Compton-thick Active Galactic Nuclei (AGN) represent one of the most elusive phases of massive black hole growth, yet are expected to contribute substantially to the Cosmic X-ray Background and the integrated growth of massive black holes. NGC 4945 is the closest Compton-thick AGN and amongst the brightest AGN in the […]


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Changing-Look AGNs from DESI. VI. Host Galaxies

Kavli Affiliate: Linhua Jiang | Summary:Changing-look (CL) AGNs trace rapid changes in nuclear activity, but their connection to host galaxy properties remains unclear. We present a study of the host galaxies of 105 CL AGNs previously selected by comparing DESI and SDSS data. We apply a two-epoch spectrophotometric decomposition to the DESI and SDSS spectra […]


Continue.. Changing-Look AGNs from DESI. VI. Host Galaxies