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Covariant Energy Density Functionals for Modeling the Equation of State of Neutron Star Matter: Cross-comparison Analysis Using CompactObject. This study analyzes and contrasts different phenomenological methods used to model the nuclear equation of state (EOS) for neutron star matter based on covariant energy density ... | [
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A Pan-galaxy Study of Synthetic Giant Molecular Filaments: A Turbulence-dominated Life Cycle. Recent surveys of the Galactic plane have revealed dozens of giant molecular filaments (GMFs), with lengths ranging from tens to hundreds of parsecs, yet their origins and life cycles remain debated. In this work, we analyze o... | [
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Hunting Very High-energy-emitting (>100 GeV) High-synchrotron-peaked Blazars. Very high-energy (VHE; >100 GeV) γ-ray emission originates via some of the most extreme particle acceleration processes in the Universe. Considering beamed active galactic nuclei, i.e., blazars, only a small fraction, mainly high-synchr... | [
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Stray Light Correction for the Helioseismic and Magnetic Imager. We report a point-spread function (PSF) and deconvolution procedure to remove stray light from the Helioseismic and Magnetic Imager (HMI) data. Prelaunch calibration observations, postlaunch Venus transit, and lunar transit data were used to develop the P... | [
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JWST Exoplanetary Worlds and Elemental Survey (JEWELS). I. High-precision Chemical Abundances of 20 FGK Planet-hosting Stars from JWST Cycle 2. We present high-precision chemical abundances for 20 FGK stars hosting planets observed in JWST Cycle 2 GO programs. Using high-resolution, high-signal-to-noise ratio spectra f... | [
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QHSC: The Quasar Candidate Catalog for the Hyper Suprime-Cam Subaru Strategic Program. The Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) is a deep wide-field multiband imaging survey consisting of three layers (Wide, Deep, and UltraDeep), with the Wide layer covering ∼1470 deg2 to a depth of i ∼ 26 mag. We prese... | [
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Deep Andromeda JCMT SCUBA-2 Observations. The Submillimeter Maps and Giant Molecular Clouds. We have carried out unprecedentedly deep, nearly confusion-limited JCMT SCUBA-2 mapping observations on the nearest spiral galaxy, M31 (Andromeda). The 850 μm image with a ∼50 pc resolution yields a comprehensive catalog of 383... | [
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Vz-GAL: Probing Cold Molecular Gas in Dusty Star-forming Galaxies at z = 1─6. We present the first results of Vz-GAL, a high-redshift CO(J = 1─0) large survey with the Karl G. Jansky Very Large Array, targeting 92 Herschel-selected, infrared-luminous, dusty star-forming galaxies at redshifts 1─6. These sources are sele... | [
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A New Way to Discover Strong Gravitational Lenses: Pairwise Spectroscopic Search from DESI DR1. We present a new method to search for strong gravitational-lensing systems by pairing spectra that are close together on the sky in a spectroscopic survey. We visually inspect 26,621 spectra in the Dark Energy Spectroscopic ... | [
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Constraining the nHz Gravitational-wave Background with an X-Ray Pulsar-timing Array from NICER Observations. We present constraints on the nHz gravitational-wave background (GWB) using X-ray pulsar-timing data from the Neutron Star Interior Composition Explorer (NICER). By analyzing six millisecond pulsars over a 6 yr... | [
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A Comprehensive Model of the K-coronal Spectrum for the Inference of Electron Temperature and Bulk Flow Velocity in the Corona. The electron temperature of the corona is one of the key physical parameters which reflect the complexity of coronal-heating processes. L. E. Cram was the first to show that the K-coronal spec... | [
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Secondary Standards in the UKIRT Faint Standard Fields. We present precise J- and K-band photometric measurements for 128 near-infrared (NIR) secondary standard stars, located in the 19 United Kingdom Infrared Telescope/Maunakea Observatories (UKIRT/MKO) primary faint standard fields. The data were collected over more ... | [
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Toward a Comprehensive Grid of Cepheid Models with MESA. II. Impact of Physical and Numerical Assumptions on Elemental Abundances. Modern tools for modeling stellar evolution, such as the Modules for Experiments in Stellar Astrophysics, offer state-of-the-art implementations of stellar theories. However, this parametri... | [
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LSTM-MDNz: Estimating Quasar Photometric Redshifts with an LSTM-augmented Mixture Density Network. Quasar photometric redshifts are essential for studying cosmology and large-scale structures. However, their complex spectral energy distributions cause significant redshift─color degeneracy, limiting the accuracy of trad... | [
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Unveiling the Chemical Complexity and C/O Ratio of the HD 163296 Protoplanetary Disk: Constraints from Multiline ALMA Observations of Organics, Nitriles, and Sulfur-bearing and Deuterated Molecules. The physical and chemical conditions within a protoplanetary disk play a crucial role in determining its chemical composi... | [
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A Core-collapse Supernova Neutrino Parameterization with Enhanced Physical Interpretability. We introduce a novel parameterization of supernova neutrino energy spectra with a clear physical motivation. Its central parameter, τ(t), quantifies the characteristic thermal-diffusion area during the explosion. When applied t... | [
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Assessing the Effects of Composition and Surface Roughness on the Photopolarimetric Response of Planetary Regoliths. This study is part of an ongoing project in which we experimentally examine the effect of composition (refractive index) and surface roughness on the scattering matrix elements of a set of well-character... | [
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Comprehensive Analyses of Cumulative Frequency Distributions for Solar X-Ray Flares. We investigate the temporal evolution of cumulative flare frequency (CFF) distributions using solar X-ray data (0.5─4.0 Å) from Geostationary Operational Environmental Satellites between 1974 and 2020. Beyond the conventional power-law... | [
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Fast Deep Learning─based Imaging for Synthetic Aperture Array: Application to DART. DAocheng Radio Telescope (DART) is a radio synthetic aperture array consisting of 313 antennas, dedicated to monitoring solar activities and observing cosmic radio sources. To meet the real-time demands of interferometric brightness tem... | [
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A TimesNet-based Real-time Forecasting System for the F10.7 Index Using DRAO and Chinese Langfang Datasets. In this paper, we construct the DRAO univariate dataset, the DRAO multivariate dataset, and the Chinese Langfang dataset. We develop and compare five deep learning models (TimesNet, iTransformer, PatchTST, N-Beat... | [
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GMIMS-DRAGONS: A Faraday Depth Survey of the Northern Sky Covering 350─1030 MHz. Polarized synchrotron emission at meter to centimeter wavelengths provides an effective tracer of the Galactic magnetic field. Calculating Faraday depth, the most useful parameter for mapping the line-of-sight magnetic field, requires obse... | [
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NEXUS Early Data Release: NIRCam Imaging and WFSS Spectroscopy from the First (Partial) Wide Epoch. We present the early data release of the multicycle JWST-NEXUS treasury program (2024─2028), which includes NIRCam imaging and WFSS observations from the first (partial) NEXUS-Wide epoch covering the central 100 arcmin2 ... | [
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New Single-lined Spectroscopic Binaries Identified from the LAMOST Medium-resolution Spectroscopic Survey. A typical single-lined spectroscopic binary (SB1) consists of two stars with almost the same age but markedly different masses and physical properties. SB1s are essential for obtaining the statistical properties o... | [
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Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. XV. Reverberation Mapping of Mg II Emission Lines. As the 15th paper in a series reporting on a large reverberation mapping (RM) campaign of super-Eddington accreting massive black holes (SEAMBHs) in active galactic nuclei (AGNs), we present ... | [
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A Characterization of JWST MIRI Detector Persistence and Implications for High-contrast Imaging. The JWST MIRI detector exhibits a flux-deficit persistence, but its timescales and impacts remain largely uncharacterized, particularly at the longest imaging wavelengths. In this study, we analyze full-field MIRI imager ob... | [
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Simulations of Global Solar Convection with a Fully Compressible CHORUS++ Code. Fluid-dynamics simulations of global solar convection are a critically important tool for assessing the dynamics of the solar interior. However, simulation studies with a fully compressible hydrodynamics code are not yet common. The Compres... | [
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An Advanced Identification Method for Gamma-Ray Bursts with Data and Feature Enhancements. Gamma-ray bursts (GRBs) are challenging to identify due to their transient nature, complex temporal profiles, and limited observational datasets. We address this with a one-dimensional convolutional neural network integrated with... | [
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An 11 yr Catalog of Gamma-Ray Transients: A Comprehensive Search with Fermi Gamma-Ray Burst Monitor Data. The Gamma-ray Burst Monitor (GBM) on board the Fermi Gamma-ray Space Telescope has produced the largest database of all-sky observations in gamma rays with its continuous data with high time and energy resolutions.... | [
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ACCEPT 2.0: A Compilation of X-Ray Gas Properties for Clusters of Galaxies Observed by the Chandra X-Ray Observatory. Archive of Chandra Cluster Entropy Profile Tables (ACCEPT) 2.0 is an updated library of uniformly produced measurements of 532 galaxy clusters based on Chandra archival data. It contains radial density,... | [
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Dark Energy Survey Year 6 Results: Photometric Dataset for Cosmology. We describe the photometric dataset assembled from the full 6 yr of observations by the Dark Energy Survey (DES) in support of static-sky cosmology analyses. DES Y6 Gold is a curated dataset derived from DES Data Release 2 (DR2) that incorporates imp... | [
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A Morphokinematic Study of Galactic High-abundance Discrepancy Factor Planetary Nebulae Based on the VLT/UVES Deep Spectroscopy. We report detailed analyses of deep, high-resolution spectra of three Galactic planetary nebulae (PNe) with high abundance discrepancy factors (ADFs), Hf 2-2, M 1-42, and NGC 6153, obtained w... | [
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Magellanic Outflow and Chemistry Survey (MAGOS): Hot Cores in the LMC. The Large Magellanic Cloud (LMC) provides a key laboratory for exploring the diversity of star formation and interstellar chemistry under subsolar metallicity conditions. We present the results of a hot core survey toward 30 massive protostellar obj... | [
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The Milky Way Imaging Scroll Painting Survey: Data Release 1. We present the first data release (DR1) of the Milky Way Imaging Scroll Painting (MWISP) survey, a mapping in the J = 1 → 0 transition lines of 12CO, 13CO, and C18O toward the northern Galactic plane during 2011─2022. The MWISP survey was conducted using the... | [
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Finite Plasma β Three-dimensional Magnetic Field Extrapolation Based on the Magnetohydrodynamic Relaxation Method. The three-dimensional (3D) magnetic field in the solar atmosphere provides crucial information to help understand explosive phenomena such as solar flares and coronal mass ejections. Since it is still hard... | [
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Galactic Interstellar <SUP>32</SUP>S/<SUP>34</SUP>S Isotopic Ratio Traced by Sulfur Monoxide. To date, the Galactic interstellar radial 32S/34S gradient has only been studied with the CS isotopologues, which may be affected by uncertainties due to the use of a single tracer. As another abundant S-bearing molecules, SO ... | [
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BASS. L. Near-infrared Data Release 3: A Spectral Atlas and Characterization of Active Galactic Nuclei. We present an analysis of near-infrared (NIR) emission-line properties, active galactic nucleus (AGN) diagnostics, and circumnuclear gas dynamics for 453 hard X-ray selected (14─195 keV) AGNs from the BAT AGN Spectro... | [
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An Information-based Metric for Observing Strategy Optimization, Demonstrated in the Context of Photometric Redshifts for LSST. The observing strategy (OS) of an astronomical survey influences the degree to which its resulting data can be used to accomplish any science goal, necessitating upcoming programs, including t... | [
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A Chemically Peculiar Star Catalog from LAMOST DR12 Based on Deep Learning. Chemically peculiar (CP) stars offer a unique observational sample for exploring key processes in stellar evolution. Leveraging the massive amounts of data obtained from large-scale sky surveys, deep learning technology has significantly advanc... | [
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Uncovering Hidden Systematics in Extreme-precision Radial Velocity Measurements. We identify and correct for small but coherent instrumental drifts in 7 yr of radial velocity (RV) data from the EXtreme PREcision Spectrograph (EXPRES). The systematics are most notable for the six months before and after 2022 January, wh... | [
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The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Quasar Survey: Quasar Properties from Data Releases 10 to 12. We present the quasar catalog from Data Releases 10 to 12 of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Quasar Survey, comprising quasars observed between 2021... | [
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Spectuner-D1: Spectral Line Fitting of Interstellar Molecules Using Deep Reinforcement Learning. Spectral lines from interstellar molecules provide crucial insights into the physical and chemical conditions of the interstellar medium. Traditional spectral line analysis relies heavily on manual intervention, which becom... | [
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Millimeter-wave and Far-infrared Spectroscopic Characterization of Torsionally Excited Ethylene Glycol. Ethylene glycol has been detected in various astronomical sources, with rotational excitation temperatures ranging from ∼8 to 300 K. The higher end of this range approaches the energies of this molecule's lowest tors... | [
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Measuring the Coronal Magnetic Field with 2D Coronal Seismology: A Forward-modeling Validation. In recent years, a two-dimensional (2D) coronal seismology technique applied to spectral-imaging data from the Coronal Multi-channel Polarimeter (CoMP) and Upgraded Coronal Multi-channel Polarimeter (UCoMP) has enabled routi... | [
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Asteroseismically Inferred Ages of 132,000 Red Giants with TESS. NASA's Transiting Exoplanet Survey Satellite mission has identified at least 158,000 oscillating red giants, increasing the known sample by roughly an order of magnitude. After validating that these measurements are reliable to 5% for up to 90% of red gia... | [
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ExoClock Project. IV. A Homogeneous Catalog of 620 Updated Exoplanet Ephemerides. The ExoClock project is an open platform aiming to monitor exoplanets by integrating observations from space- and ground-based telescopes. This study presents an updated catalog of 620 exoplanet ephemerides, integrating 30,000 measurement... | [
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Overview of the JWST Advanced Deep Extragalactic Survey (JADES). We present an overview of the James Webb Space Telescope (JWST) Advanced Deep Extragalactic Survey (JADES), an ambitious program of infrared imaging and spectroscopy in the GOODS-S and GOODS-N deep fields, designed to study galaxy evolution from high reds... | [
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A Machine Learning Approach for Identifying Coronal Mass Ejection─associated Stellar Flares in TESS Observations. Coronal mass ejections (CMEs) are major drivers of stellar space weather and can strongly influence the habitability of exoplanets. However, compared to the frequent occurrence of white-light flares, confir... | [
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Gamma-Ray Millisecond Pulsars: Off-pulse Emission Characteristics, Phase-resolved Pseudoluminosity─Cutoff Energy Correlation, and High-energy Pulsed Emission. We investigate the γ-ray emission from 38 millisecond pulsars using 15 years of Fermi-LAT Pass 8 data in the 0.3─500 GeV range. Off-pulse intervals defined objec... | [
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HyperAIRI: A Plug-and-play Algorithm for Precise Hyperspectral Image Reconstruction in Radio Interferometry. The next-generation radio-interferometric (RI) telescopes require imaging algorithms capable of forming high-resolution, high-dynamic-range images from large data volumes spanning wide frequency bands. Recently,... | [
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Bayesian Model Comparison and Significance: Widespread Errors and How to Correct Them. Bayes factors have become a popular tool in exoplanet spectroscopy for testing atmosphere models against one another. We show that the commonly used method for converting these values into significance "sigmas" is invalid. The formul... | [
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A Catalog of 971 FR I Radio Galaxies from the FIRST Survey via Hybrid Deep Learning and Ridgeline Flux Density Distribution Analysis. We present a catalog of 971 FR I radio galaxies (FR Is) identified from the Very Large Array Faint Images of the Radio Sky at Twenty centimeters (FIRST) survey. The identifications were ... | [
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Searching for Solar-like Oscillations Using TESS 2 minute Cadence in the Southern Ecliptic Hemisphere. The TESS space mission has generated an extensive collection of light curves, providing a valuable opportunity to search for solar-like oscillations. Numerous studies have utilized TESS observations to search for sola... | [
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The LIRA─Ising Model: Estimating the Boundaries of Irregularly Shaped X-Ray Sources. Mapping the boundary of an extended source is a key step in the study of its morphology. The background contamination and statistical fluctuations of typical astronomical images make this a challenging statistical task, in particular f... | [
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Cold Dust Properties and Submillimeter Excess in 33 Nearby Spiral Galaxies. The origin of submillimeter excess in galaxies remains unclear. We analyze cold dust properties of 33 nearby spiral galaxies, identify a possible 850 μm excess, and explore its environments. Spectral energy distributions are fitted using a hier... | [
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Deep Learning─driven Atmospheric Parameter Prediction for Hot Subdwarf Stars with Synthetic and Observed Spectra. We design a convolutional neural network incorporating channel attention and spatial attention mechanisms to predict atmospheric parameters of hot subdwarfs. The experimental dataset comprises spectra at ni... | [
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The 2025 Evaluation of Experimental Thermonuclear Reaction Rates (ETR25). This work describes the formalism for estimating thermonuclear reaction rates for astrophysical applications, emphasizing modern statistical approaches such as Monte Carlo sampling and Bayesian models. We discuss related topics including the calc... | [
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A Novel Method of Estimating Gamma-Ray Burst Peak Energies beyond the Swift/BAT Limit. The Swift Burst Alert Telescope (BAT), operating in the 15─150 keV band, cannot directly measure the peak energy (Ep) for most gamma-ray bursts (GRBs), as typical Ep values of 200─300 keV lie beyond its upper energy limit. In this pa... | [
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Machine Learning─based Identification of the Solar Disk and Plages in Kodaikanal Solar Observatory Historical Suncharts. Kodaikanal Solar Observatory (KoSO) is one of the oldest solar observatories, possessing an archive of multiwavelength solar observations, including white light, Ca II K, and Hα images spanning over ... | [
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Diversity in Evolutionary Status and Magnetic Activity among Solar-type Twin Detached Eclipsing Binaries. We present a combined photometric and spectroscopic analysis of four detached eclipsing binaries (KIC 8957954, KIC 10593759, KIC 8302455, and TIC 207398432), all of which exhibit composite G-type spectra and nearly... | [
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SKYSURF. X. A Novel Method for Measuring Integrated Galaxy Light. We describe the drizzling pipeline and contents of the drizzled database for Hubble Space Telescope Cycle 27─29 Archival Legacy project "SKYSURF," the largest archival project ever approved for Hubble. SKYSURF aims to investigate the extragalactic backgr... | [
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A Catalog of 486 Barium Stars Identified in GALAH DR4. We present a catalog of 486 Ba stars identified in the GALAH DR4 survey using high-resolution spectra and precise abundance measurements. The sample was selected based on s-process enrichment criteria involving the abundances of Ba and La relative to Eu, and furthe... | [
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Magnetohydrodynamic Guiding Center Particle-in-cell Method for Multiscale Plasma Kinetic Simulations. We present the formulation, algorithm, and numerical tests of the magnetohydrodynamic particle-in-cell (MHD-PIC) method with particles treated under the guiding center approximation, which we term the MHD-gPIC method, ... | [
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Fundamental Properties of Novae in M31. The peak luminosities and rates of decline for a large sample of novae recently published by Clark et al. have been analyzed using the Yaron et al. nova models to estimate fundamental properties of the M31 nova population. The apparent white dwarf (WD) mass distribution is approx... | [
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The Hubble Arp Galaxy Survey. The typical galaxy in the local Universe is expected to be in a self-regulated quasi-equilibrium, displaying a settled morphology that falls within the Hubble sequence. The Arp and Arp─Madore catalogs are filled with striking examples of galaxies that defy these expectations, making them u... | [
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Active Galactic Nuclei and Star Formation in Nearby Galaxies (AGNSTRONG). II. Results for Jetted Type-I AGNs with Strong Ionized-gas Outflows. We investigate the correlation between ionized-gas outflows, jets, and star formation in a sample of 42 local type-I active galactic nuclei (AGNs) exhibiting significant [O III]... | [
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AthenaK: A Performance-portable Version of the Athena++ Adaptive Mesh Refinement Framework. We describe AthenaK: a new implementation of the Athena++ block-based adaptive mesh refinement framework using the Kokkos programming model. Finite volume methods for Newtonian, special relativistic, and general relativistic (GR... | [
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RM-Tools: Software for Analyzing Polarized Radio Spectra. Polarization observations using modern radio telescopes cover large numbers of frequency channels over broad bandwidths, and require advanced techniques to extract reliable scientific results. We present RM-Tools, analysis software for deriving polarization prop... | [
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Automated Detection of Coronal Mass Ejections with Few-shot Learning. Coronal mass ejections (CMEs) are a primary driver of severe space weather impacts, yet accurate delineation of CME structure in coronagraph images remains challenging. We present Segment Anything Model (SAM)─low-rank adaptation (LoRA), an efficient ... | [
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Large Language Model─driven Analysis of General Coordinates Network (GCN) Circulars. The General Coordinates Network (GCN) is NASA's time-domain and multimessenger alert system. GCN distributes two data products: automated "Notices" and human-generated "Circulars" that report the observations of high-energy and multime... | [
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Identification of Strongly Lensed Gravitational-wave Events Using Squeeze-and-excitation Multilayer Perceptron Data-efficient Image Transformer. With the advancement of third-generation gravitational-wave (GW) detectors, the identification of strongly lensed GW events is expected to play an increasingly vital role in c... | [
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Evolution of Stellar Activity and Habitable Zone. II. Ca II H and K Emissions of Late-type Dwarfs. Stellar chromospheric activity serves as a valuable proxy for estimating stellar ages, though its applicable range and accurate functional form are still debated. Utilizing LAMOST spectra, we have compiled a catalog of op... | [
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The Cyclic Variation of Magnetic Fields on the Quiet Sun Observed by SDO/HMI. Unraveling the origins of the quiet Sun's magnetic fields remains a key challenge. Using observations from Heliospheric Magnetic Imager on board Solar Dynamics Observatory, we identified over 86 million quiet region (QR) structures in daily f... | [
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The Second CHIME/FRB Catalog of Fast Radio Bursts. We present a catalog of 4539 fast radio bursts (FRBs) observed with the Canadian Hydrogen Intensity Mapping Experiment telescope between 2018 July 25 and 2023 September 15. These bursts originate from 3641 unique sources, including 981 bursts from 83 known repeating so... | [
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Through Thick and Thin: The Cosmic Evolution of Disk Scale Height. To investigate the formation and evolution of vertical structures in disk galaxies, we measure global sech2 scale heights, averaging thin and thick components when present, for 2631 edge-on disk galaxies with M* > 1010M⊙ at 0 < z < 3.5 from the... | [
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Spectral Reflectance Properties (0.3─2.5 μm) of LL Ordinary Chondrites. Spectral characterization of asteroids relies on meteorite spectral calibration to constrain their surface mineralogy. We have conducted a comprehensive spectroscopic study of LL chondrites to shed light on the factors that control their reflectanc... | [
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Cosmic-ray Magnetohydrodynamics: A New Two-moment Framework with Numerical Implementation. Cosmic rays (CRs) play a pivotal role in various astrophysical systems, delivering feedback over a broad range of scales. However, modeling CR transport remains challenging due to its inherently multiscale nature and complex micr... | [
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Unveiling Quasars in Gaia DR3: Multimodal Classification and Redshift Estimation of BP/RP Sources with Deep Learning. We present a multimodal deep learning framework that classifies stars, galaxies, and quasars and accurately estimates quasar redshifts using Gaia DR3's low-resolution BP/RP (XP) spectra, alongside astro... | [
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MARVEL Analysis of the Measured High-resolution Spectra of CO Isotopologues. Carbon monoxide is thought to be the second most abundant molecule in the Universe. This makes observation of both its parent isotopologue (12C16O) and its stable isotopologues, 13C16O, 12C18O, 12C17O, 13C18O, and 13C17O, important in variety ... | [
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MESA Isochrones and Stellar Tracks (MIST). III. The White Dwarf Cooling Sequence. We present a substantial update to the MESA Isochrones and Stellar Tracks (MIST) library, extending the MIST model grids and isochrones down the white dwarf (WD) cooling sequence with realistic physics for WD cooling timescales. This work... | [
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An Introduction to Single-antenna Radio Astronomical Polarimetry. This tutorial reviews the mathematical foundations of single-antenna radio polarimetry with the aim of fostering a conceptual understanding of the relationships between a physical description of signal propagation (gain, delay, reflection, down-conversio... | [
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Prospects for Measuring Black Hole Masses using TDEs with the Vera C. Rubin Observatory. Tidal Disruption Events (TDEs) provide an opportunity to study supermassive black holes that are otherwise quiescent. The Vera C. Rubin Legacy Survey of Space and Time will be capable of discovering thousands of TDEs each year, all... | [
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Mid-IR Luminosity Functions: Inferred Dusty Cosmic Star Formation and Black Hole Accretion Histories from the JWST SMILES. Mid-infrared (mid-IR) observations are crucial for understanding galaxy evolution, tracing star formation, and active galactic nuclei (AGN) activity via dust emission. This work presents mid-IR gal... | [
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Low-latency Forecasts of Kilonova Light Curves for Rubin and ZTF. The follow-up of gravitational-wave events by wide-field surveys is a crucial tool for the discovery of electromagnetic counterparts to gravitational wave sources, such as kilonovae. Machine learning tools can play an important role in aiding search effo... | [
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SHORES. II. Multi-frequency Characterization of the Sub-mJy Radio Population in FIR-selected Fields. We present a new deep multi-frequency radio survey of two extragalactic fields observed with the Australia Telescope Compact Array as part of the SHORES project (Serendipitous H-ATLAS-fields Observations of Radio Extrag... | [
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Classification of Double Neutron Stars Using the Extreme Deconvolution Method. The double neutron star (DNS) systems are pivotal compact binary systems for testing gravitational waves and general relativity—evidenced by radio telescope observations of their orbital decay and LIGO-Virgo-KAGRA detections of their coalesc... | [
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Four Giant Planets from 2024 KMTNet Microlensing Campaign. In this work, we present analyses of four newly discovered planetary microlensing events from the 2024 KMTNet survey season: KMT-2024-BLG-0176, KMT-2024-BLG-0349, KMT-2024-BLG-1870, and KMT-2024-BLG-2087. In each case, the planetary nature was revealed through ... | [
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Degassing of Comet Analogs: New Laboratory Measurements of Vapor Pressure between Sand─Ice Agglomerates. This work aims to investigate the rate of production of vapor from the nuclei of comets when they are composed of porous dust─ice agglomerates of different sizes. The reason for starting the research was the discrep... | [
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Rapid Brightening of 3I/ATLAS Ahead of Perihelion. Interstellar comet 3I/ATLAS has been approaching its 2025 October 29 perihelion while opposite the Sun from Earth, hindering ground-based optical observations over the preceding month. However, this geometry placed the comet within the fields of view of several space-b... | [
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A Simple, Flexible Method for Timing Cross-calibration of Space Missions. The timing (cross-)calibration of astronomical instruments is often done by comparing pulsar times-of-arrival (TOAs) to a reference timing model. In high-energy astronomy, the choice of solar system ephemerides and source positions used to baryce... | [
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SENPAI: Sidereal Enriched Rate-track Astrometry in Deep Imagery of Solar System Bodies. Rate-track imagery−in which a telescope tracks an object's proper motion instead of the stellar background−has long been used to enhance the signal-to-noise ratio of faint solar system bodies such as asteroids, comets, and artificia... | [
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Astrophysical or Terrestrial: Machine Learning Classification of Gravitational-wave Candidates Using Multiple-search Information. Low-latency gravitational-wave alerts provide the greater multi-messenger community with information about the candidate events detected by the International Gravitational-Wave Network. Prom... | [
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Design of a New Solar Radio Observing System Working in 3─6 GHz. Solar radio bursts from decimeter to centimeter wavelength originate from radiations from coherent to incoherent mechanism. This spectral domain hosts a rich variety of fine structures that encode critical information about energetic electron beams, coron... | [
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MSIHP-Net: A Multiscale Deep Learning Method for Identifying Green Pea Galaxies. Green Pea galaxies (GPs) are a rare class of compact, low metallicity star-forming galaxies characterized by strong [O III] λ5007 emission lines, and high specific star formation rates in surveys such as Sloan Digital Sky Survey (SDSS) and... | [
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KDP as A Thermal Blocking Filter—Deep Near IR Observations with A Warm Narrow Band Filter. Ground-based astronomy suffers from strong atmospheric line- and thermal continuum emission, at the near-infrared (NIR, 0.7─1.1 μm), and short-wave infrared (SWIR, 1.1─2.5 μm) wavelengths. The thermal continuum emission increases... | [
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