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On the Relationship between Nanoflare Energy and Delay in the Closed Solar Corona. Determining the relationship between nanoflare energies and their delays is the key for understanding the physical mechanism of the events and the plasma response. Nanoflares analyzed in this study were generated self-consistently via pr... | [
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Radio Studies of Supernovae 1979C, 1986J, and 2006X with LOFAR. We present LOw Frequency ARray (LOFAR) studies of supernovae SN 1979C, SN 1986J, and SN 2006X, focusing on new observations from the LOFAR Two-metre Sky Survey (LoTSS) and the International LOFAR Telescope (ILT). For Type Ia supernovae (SNe Ia) SN 2006X, w... | [
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Semianalytic Orbits: A Practical Implementation of Lynden-Bell's Planar Orbits and Extension to Vertical Oscillations. We present a practical implementation of the perturbation theory derived by Lynden-Bell for describing, to arbitrary precision, the orbit of a particle in an arbitrary spherically symmetric potential. ... | [
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Unifying the Circumstellar Environment in Broad-lined Type Ic Radio Supernovae toward Off-axis Gamma-Ray Burst Exploration. Decades have passed since the first confirmed association between a broad-lined Type Ic supernova (Type IcBL SN) and a long gamma-ray burst (GRB), and the number of known GRB-SN associations has s... | [
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SpecCLIP: Aligning and Translating Spectroscopic Measurements for Stars. In recent years, large language models (LLMs) have transformed natural language understanding through vast data sets and large-scale parameterization. Inspired by this success, we present SpecCLIP, a foundation model framework that extends LLM-ins... | [
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3D Numerical Simulations of Magnetar Crustquakes. Crustquakes are frequently invoked as a mechanism to trigger sudden transients in the magnetospheres of magnetars. In this picture, a mechanical failure of the crust excites seismic motions of the magnetar surface that launch force-free waves into the magnetosphere. We ... | [
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Bright [C II]158 μm Streamers as a Beacon for Giant Galaxy Formation in SPT2349-56 at z = 4.3. Observations of extreme starbursts, often located in the cores of protoclusters, challenge the classical bottom-up galaxy formation paradigm. Giant elliptical galaxies at z = 0 must have assembled rapidly, possibly within few... | [
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A Constrained Linear Model for Continuum Normalization of Stellar Spectra. Inferring stellar parameters and chemical abundances by forward modelling stellar spectra usually requires a spectral synthesis code, or an emulator constructed from a curated training set. In these situations continuum normalization is often im... | [
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Light Curves of Time-dependent Accretion Disks in Tidal Disruption Events. Tidal disruption events (TDEs) are believed to be an ideal laboratory for studying the evolution of accretion flow around a supermassive black hole (BH). In general, the mass feeding rate to the BH is suggested to be super-Eddington initially an... | [
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Evolution of an Alfvén Wave─driven Proton Beam in the Expanding Solar Wind. We investigate the self-consistent formation and long-term evolution of proton beams in the expanding solar wind using an ensemble of one-dimensional hybrid expanding box simulations. Initial conditions are chosen to represent a range of plasma... | [
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A Relativistic Formula for Radiation Intensity of Multiply Scattered Photons. We derive an analytical solution for the radiation intensity of scattered photons that is valid from the free-streaming phase immediately after photon emission to the diffusive phase after undergoing multiple scatterings. Assuming isotropic a... | [
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Long-term Radio Monitoring of PKS 1127─145: Detection and Physical Interpretation of Quasiperiodic Oscillations. We analyzed over four decades of UMRAO monitoring of PKS 1127─145 at 4.8, 8, and 14.5 GHz to search for quasiperiodic oscillations (QPOs) under red-noise variability. Lomb─Scargle and Weighted Wavelet Z-tran... | [
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Functionalization of Benzene Ices by Atomic Oxygen. Small aromatic molecules, including functionalized derivatives of benzene, are known to be present throughout the different stages of star and planet formation. In particular, oxygen-bearing monosubstituted aromatics, likely including phenol, have been identified in t... | [
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The Massive and Distant Clusters of WISE Survey 2: Detection of Splashback Radii in Galaxy Cluster Total Light Stacks. The splashback radius, the radius of the apocenter of the first orbit of infalling material, is a measurable quantity marking the boundary between a galaxy cluster and its infalling region. We report d... | [
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Delayed Radio Emission in Tidal Disruption Events from Collisions of Outflows Driven by Disk Instabilities. Delayed radio emission has been associated with a growing proportion of tidal disruption events (TDEs). For many events, the radio synchrotron emission is inferred to originate from the interaction of mildly rela... | [
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PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-Domain Field III. The James Webb Space Telescope North Ecliptic Pole (NEP) Time-Domain Field (TDF) has been monitored by Nuclear Spectroscopic Telescope Array (NuSTAR) and XMM-Newton with a regular cadence for 5 yr, starting in 2019... | [
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Exploring the Statistical Properties of Double Radio Relics in the TNG-cluster and TNG300 Simulations. Double radio relics, pairs of diffuse radio features located on opposite sides of merging galaxy clusters, are a rare subclass of radio relics that are believed to trace merger shocks and provide valuable constraints ... | [
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High-resolution Solar X-Ray Spectroscopy from Archived Solar Maximum Mission Data. Archived high-resolution X-ray spectra in the 13─22 Å range from the Flat Crystal Spectrometer (FCS), an instrument on the Solar Maximum Mission operating in the 1980s, are analyzed with reference to nonflaring active regions, and to the... | [
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Characterizing Dust Extinction and Spatially Resolved Paschen-α Emission within 97 Galaxies at 1 < z < 1.6 with JWST NIRCam Slitless Spectroscopy. We present results on the Paschen-α (Paα) emitting galaxies observed as part of the JWST FRESCO survey in the GOODS-North and GOODS-South fields. Utilizing the JWST NI... | [
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Unveiling the Dual Nature of V1180 Cas: UXor-like Dips and EXor-like Bursts across a Decade. We present a detailed analysis of the long-term photometric and spectroscopic evolution of V1180 Cas over a decade, aiming to identify the dominant mechanisms behind its variability. We combine multiband light curves from 1999 ... | [
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High-frequency Continuous Gravitational Wave Search in LIGO O3 Public Data with Einstein@Home. We search for nearly monochromatic gravitational-wave signals with frequencies 800.0 Hz ≤ f ≤ 1686.0 Hz and spin-down −2.7×10−9Hzs−1≤ḟ≤0.2×10−9Hzs−1 . We use LIGO O3 public data from the Hanford and Livingston detectors, an... | [
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HSTPROMO Internal Proper-motion Kinematics of Dwarf Spheroidal Galaxies. II. Velocity Anisotropy and Dark Matter Cusp Slope of Sculptor. We analyze three epochs of Hubble Space Telescope imaging over 20 yr for the Sculptor dwarf spheroidal galaxy, measuring precise proper motions for 119 stars and combining them with 1... | [
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Fundamental Understanding of Magnetic Reconnection via Spiral CT Scan. IV. Whistler Waves. For the first time, we reveal the distribution of whistler waves around a reconnection X-line by using the spiral CT scan technique, which is a novel technique analogous to that used in hospitals. This X-line was detected by the ... | [
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Young Planets around Young Accreting Stars. I. Migration and Inner Stalling Orbits. Planet migration in protoplanetary disks significantly influences exoplanet architectures. We investigate various migration mechanisms for young planets close to young stars. To quantify the stochastic migration driven by turbulent disk... | [
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A XRISM/Resolve View of the Dynamics in the Hot Gaseous Atmosphere of M87. The XRISM/Resolve microcalorimeter directly measured the gas velocities in the core of the Virgo Cluster, the closest example of active galactic nucleus (AGN) feedback in a cluster. This proximity allows us to resolve the kinematic impact of fee... | [
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Thermal Baroclinic Instabilities in Accretion Disks. II. Numerical Experiments for the Goldreich─Schubert─Fricke Instability and the Convective Overstability in Disks around Young Stars. The linear stability analysis of a stratified rotating fluid (see Paper I) showed that disks with a baroclinic stratification under t... | [
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Millimeter-wave Rotational Spectroscopy and Interstellar Search for 2-Mercaptoethanol (HSCH<SUB>2</SUB>CH<SUB>2</SUB>OH). Sulfur is one of the most abundant elements in the interstellar medium (ISM) and a key component for life, yet little is understood about its chemistry in the ISM. While increasingly larger molecule... | [
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Wind-fed Supermassive Black Hole Accretion in the Ultracompact Dwarf Galaxy M60-UCD1. Ultracompact dwarf galaxies (UCDs) are thought to be remnants of stripped galactic nuclei, among which a handful are known to host a central supermassive black hole (SMBH). As in stripped nuclear star clusters, the SMBHs in UCDs may b... | [
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Ring-gap Structures in the Class I Circumstellar Disk of CrA IRS 2 Associated with the Magnetic Flux-driven Bubble. Recent Atacama Large Millimeter/submillimeter Array (ALMA) observations with 0 .″ 1 resolution have revealed characteristic substructures in circumstellar disks around young Class I sources, providing clu... | [
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The Timescales of Embedded Star Formation as Observed in STARFORGE. Star formation occurs within dusty molecular clouds that are then disrupted by stellar feedback. However, the timing and physical mechanisms that govern the transition from deeply embedded to exposed stars remain uncertain. Using the STARFORGE simulati... | [
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A Comprehensive Photometric Study of the Eclipsing SU UMa-type Cataclysmic Variable OY Carinae. We present a comprehensive photometric study of the eclipsing dwarf nova OY Car based on ground-based observations and archival data from the Transiting Exoplanet Survey Satellite (TESS) and AAVSO. Eclipse timing analysis re... | [
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Beyond UV: Rest-frame B-band and Apparent Luminosity Functions of z = 5─9 Galaxies. We present new measurements of galaxy luminosity functions (LFs) from JWST/NIRCam imaging over the redshift range z = 4.5─9.7, using photometric catalogs from JADES and public extragalactic fields. Our analysis includes rest-frame UV an... | [
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Fluctuation Dynamos in Supersonic Turbulence at Pm ≳ 1. Fluctuation dynamos provide a robust mechanism for amplifying weak seed magnetic fields in turbulent astrophysical plasmas. However, their behaviour in the highly compressible regimes characteristic of the interstellar medium remains incompletely understood. Using... | [
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Cosmology with Supernova Encore in the Strong Lensing Cluster MACS J0138─2155: Time Delays and Hubble Constant Measurement. Multiply imaged supernovae (SNe) provide a novel means of constraining the Hubble constant (H0). Such measurements require a combination of precise models of the lensing mass distribution and an a... | [
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SNR 1987A: Spitzer Data from Days 6000 to 8000 Revisited. An excess emission has been observed by Spitzer in the 3─5 μm range of the SNR 1987A spectrum. It is generally argued that this excess could be due to the presence of warm amorphous carbon dust in the equatorial ring around the supernova, but the proposed models... | [
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A Fast, Parallelized, GPU-accelerated Photochemical Model, XODIAC, with Built-in Equilibrium Chemistry and Multiple Chemical Networks for Exoplanetary Atmospheres. The launch of the James Webb Space Telescope has delivered high-quality atmospheric observations and expanded the known chemical inventory of exoplanetary a... | [
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The Lyα and Continuum Origins Survey. III. Investigating the Link between Galaxy Morphology, Merger Properties, and LyC Escape. Characterizing the mechanisms and galaxy properties conducive to the escape of ionizing (LyC) emission is necessary to accurately model the Epoch of Reionization and identify the sources that ... | [
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Detectability of Atmospheric Biosignatures in Earth Analogs with Varying Surface Boundary Conditions: Prospects for Characterization in the UV, Visible, Near-infrared, and Mid-infrared Regions. The search for potentially habitable exoplanets centers on detecting biosignature molecules in Earth-like atmospheres, making ... | [
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Tails of Gravity: Persistence of Star Formation in the Central Molecular Zone. We characterize star-forming gas in six molecular clouds (Sgr B1-off, Sgr B2, Sgr C, the 20 and 50 km s−1 molecular clouds, and the Brick) in the Galactic central molecular zone (CMZ), and compare their star-forming activities with those in ... | [
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Axisymmetric Modeling of DSHARP Dusty Disks: Asymmetric Structures and Inner-disk Dispersal. High-resolution observations of Class II protoplanetary disks frequently reveal annular structures that may indicate the presence of embedded planets. In this study, we model brightness profiles and geometries for 16 dusty disk... | [
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Diffusive or Ballistic? Distributions and Spectra of PeV Cosmic Rays around Microquasars. In the standard Galactic cosmic-ray (CR) paradigm, protons are accelerated up to ∼1 PeV by Galactic sources. While supernova remnants have been traditionally considered as the primary accelerators, recent observations by LHAASO an... | [
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Broadband Variability Analysis of the Flat-spectrum Radio Quasar PKS 0402−362 with Indications of Quasi-periodic Modulation. We present a comprehensive temporal and spectral study of the flat-spectrum radio quasar (FSRQ) PKS 0402−362 using Fermi Large Area Telescope/Swift X-Ray Telescope/UVOT observations spanning from... | [
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Synchrotron Self-Compton Radiation in the ICMART Model: Spectral Simulations and Application to the Record-breaking GRB 221009A. This paper presents simulations of the synchrotron self-Compton (SSC) spectrum within the Internal-Collision-induced Magnetic Reconnection and Turbulence (ICMART) model. We investigate how ke... | [
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Difference between Half-mass Radius and Half-light Radius of Galaxies at 0.2 < z < 2.5 Revealed by JWST/NIRCam Data. Using JWST observations in CANDELS fields, we measure the half-light radius (re,light) and half-mass─radius (re,mass) for 14,333 galaxies with stellar masses M* > 109M⊙ at redshifts 0.2 < z &... | [
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New Hard X-Ray and Multiwavelength Study of the PeVatron Candidate Pulsar Wind Nebula G0.9+0.1 in the Galactic Center Region. We present a new X-ray study and multiwavelength spectral energy distribution (SED) modeling of the young pulsar wind nebula (PWN) powered by the energetic pulsar PSR J1747─2809, inside the comp... | [
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Advancing Solar Flare Forecasting with a Deep Learning Approach Using Multimodal Inputs. Solar flares are among the most energetic phenomena in the solar system, and their forecasting remains a major challenge in space weather research. In this study, we present a deep learning framework that predicts the occurrence of... | [
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Merger of Noncompact Binaries: Triggering Mechanisms and Merger Timescales of W UMa Contact Binaries. The merger of noncompact binaries can produce a variety of significant celestial objects, including blue stragglers, luminous red novae, and others. However, several key details of the merger of noncompact binaries rem... | [
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A Freefall-based Switching Criterion for P<SUP>3</SUP>T Hybrid N-body Methods in Collisional Stellar Systems. The P3T scheme is a hybrid method for simulating gravitational N-body systems. It combines a fast particle-tree (PT) algorithm for long-range forces with a high-accuracy particle─particle (PP; direct N-body) so... | [
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Extending the Micro-hertz Detection Horizons via Orbital Resonance Effect for Geocentric Gravitational Wave Antennas. The μHz gravitational wave (GW) band holds crucial insights into coalescing supermassive black hole binaries (SMBHBs) and stochastic backgrounds but remains inaccessible due to technical challenges. We ... | [
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Spectral Connection between Far UV and Soft X-Ray Emission from Active Galactic Nuclei Using AstroSat. We present the UV/X-ray joint spectral analyses of four Seyfert 1 galaxies (PG 0804+761, NGC 7469, SWIFT J1921.1-5842, and SWIFT J1835.0+3240) using the data acquired with the Ultraviolet Imaging Telescope and Soft X-... | [
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Novel Physics of Escaping Secondary Atmospheres May Shape the Cosmic Shoreline. Recent James Webb Space Telescope observations of cool, rocky exoplanets reveal a probable lack of thick atmospheres, suggesting the prevalent escape of the "secondary" atmospheres formed after losing primordial hydrogen. Yet, simulations i... | [
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Subtracting and Monitoring Tilt-to-length Noise under High Differential Wavefront Sensing Noise Using Convolutional Neural Networks and Time Delay Interferometry. Gravitational waves (GWs) provide a powerful tool to probe energetic astrophysical events and test fundamental physics, with space-based detectors enabling a... | [
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On the Significance of Covariance for Constraining Theoretical Models from Galaxy Observables. In this study, we investigate the impact of covariance within uncertainties on the inference of cosmological and astrophysical parameters, specifically focusing on galaxy stellar mass functions derived from the CAMELS simulat... | [
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JADES: Rest-frame UV-to-NIR Size Evolution of Massive Quiescent Galaxies from Redshift z = 5 to z = 0.5. We present the UV-to-near-IR (NIR) size evolution of a sample of 161 quiescent galaxies with M* > 1010 M⊙over 0.5 < z < 5. With deep multiband NIRCam images in GOODS-South from JADES, we measure the effecti... | [
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The Remarkable Late-time Flux Excess in Hubble Space Telescope Observations of the Type Iax Supernova 2012Z. Type Iax supernovae (SNe Iax) are thermonuclear explosions of white dwarfs (WDs), peculiar and underluminous compared to the normal Type Ia supernovae (SNe). Observations of SNe Iax provide insight into the phys... | [
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A Modified 3D Biconical Outflow Model: Spatial Constraints on Active Galactic Nuclei─Driven Outflows. We present a modified outflow model and its application to constrain ionized outflow properties of active galactic nuclei (AGNs). By adding a rotating disk component to the biconical outflow model of H.-J. Bae & J.... | [
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Escaping Ionizing Photons from Massive Spiral Galaxies at z ∼ 1. We report the detection of Lyman continuum (LyC) photons from three massive (M* > 1010 M⊙) spiral galaxies at a redshift of nearly 1 in the AstroSat UV Deep Field South. Notably, all three systems are viewed at low inclination (i.e., nearly face-on), p... | [
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Shocks, Winds, and a Torus: the Large Binocular Telescope Interferometer (LBTI) Resolves the Active Nucleus of NGC 4151. We present mid-infrared (MIR) observations of the Seyfert 1 galaxy NGC 4151 using the Large Binocular Telescope Interferometer (LBTI). We took open-loop Fizeau images with 66─104 mas (5.8─9.1 pc) res... | [
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Gravitational Wave Phase Shifts of Black Hole Mergers in AGN Disks. Ground-based gravitational wave (GW) detectors have discovered about 200 compact object mergers. The astrophysical origins of these events are highly debated, and it is possible that at least a fraction of them originate from dynamical environments. Am... | [
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Free-floating Planets Produced by Planet─Planet Scatterings: Ejection Velocity and Survival Rate of Their Moons. The discovery of numerous free-floating planets (FFPs) has intensified interest in their origins and dynamical histories. A leading formation mechanism is planet─planet scatterings in unstable multiplanetary... | [
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How Plasma Properties of the Fanaroff─Riley Jet Can Shape Its Morphology. Extragalactic jets are broadly classified into two categories based on radio observations: core-brightened jets, known as Fanaroff─Riley Type I (FR I), and edge-brightened jets, classified as Type II (FR II). This FR dichotomy may arise due to va... | [
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Supernovae Exploding within Dense Extended Material: Early Emission Regimes and Degeneracies in Parameter Inference from Observations. Early light curves of many core-collapse supernovae (SNe) are thought to be powered by the interaction of the shock wave with optically thick extended material, either a bound envelope ... | [
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CHILES. XI. Resolved H I Morphologies and the Evolution of the H<SUB>2</SUB>/H I Ratio over the Last Five Billion Years. We present the neutral gas morphology of four galaxies from z = 0.22 to 0.47 obtained with the COSMOS H I Large Extragalactic Survey (CHILES). The H I is resolved at the highest redshift with the 7 .... | [
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Methanol Formation via the Radical─Radical Reaction of OH and CH<SUB>3</SUB> Radicals Undergoing Transient Diffusion on Ice at 10 to 60 K. Methanol (CH3OH) is thought to form on interstellar ice dust via successive hydrogenation reactions. The reaction between CH3 and OH radicals could also conceivably generate methano... | [
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Height and Energy Evolution of X-Ray Double Sources in a Solar Flare. In the standard model, magnetic reconnection at a vertical current sheet above the flare arcade is key to explaining many aspects of solar eruptions. The supra-arcade region is where the vertical current sheet is supposedly located, and X-ray/extreme... | [
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The Impact of Cosmic Filaments on the Abundance of Satellite Galaxies. The impact of cosmic web environments on galaxy properties plays a critical role in understanding galaxy formation. Using the state-of-the-art cosmological simulation IllustrisTNG, we investigate how satellite galaxy abundance differs between filame... | [
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Exploring Selection Biases in Fast Radio Burst Dispersion─Galaxy Cross-correlations with Magnetohydrodynamical Simulations. The dispersion measures (DMs) of fast radio bursts (FRBs) can be used as powerful probes of the distribution of extragalactic plasma. With a large enough sample, the free-electron─galaxy power spe... | [
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Impact of Light-mass Nuclear Reactions on the r-process Nucleosynthesis, Revisited. Light-mass nuclear reactions can play a significant role in r-process nucleosynthesis in core-collapse supernovae (SNe) and collapsars. We investigate the sensitivity of both weak and main r-process nucleosyntheses, which are responsibl... | [
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Connection between Dwarf Galaxies and Globular Clusters: Insights from the Perseus Cluster Using Subaru Imaging and Keck Spectroscopy. We present a systematic study of 189 dwarf galaxies and their globular cluster (GC) systems in the Perseus Cluster, based on deep Subaru Hyper Suprime-Cam imaging and Keck spectroscopy,... | [
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Protoplanetary Disk Cavities with JWST-MIRI: A Dichotomy in Molecular Emission. The evolution of planet-forming regions in protoplanetary disks is of fundamental importance to understanding planet formation. Disks with a central deficit in dust emission, a "cavity," have long attracted interest as potential evidence fo... | [
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Irradiated Atmosphere. V. Effects of Vertical-mixing Induced Energy Transport on the Inhomogeneity. Atmospheric variations over time and space boost planetary cooling, as outgoing internal flux responds to stellar radiation and opacity. Vertical mixing regulates this cooling. Our study examines how gravity waves or lar... | [
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Taking a Break at Cosmic Noon: Continuum-selected Low-mass Galaxies Require Long Burst Cycles. While bursty star formation in low-mass galaxies has been observed in local populations and reproduced in simulations, the dormant phase of the burst cycle has not been well studied beyond the local Universe due to observatio... | [
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Leveraging Redshift Probabilities and Machine Learning Classification to Identify Catastrophic Outlier Photometric Redshift Estimates. We present results of using a basic binary classification neural network model to identify likely catastrophic outlier (CO) photometric redshift estimates of individual galaxies. The cl... | [
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A Method for Habitability Analysis of Planets with True Polar Wander. Finding unambiguous signs of extraterrestrial life is a central challenge in astrophysics and astrobiology. Habitability assessments typically focus on conditions such as the presence of liquid water. However, True Polar Wander (TPW)—the motion of th... | [
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The Major Solar Energetic Particle Event on 2024 May 20: Multispacecraft Observations of a Long-lasting Energetic Particle Reservoir. The fleet of spacecraft distributed across the inner heliosphere during 2024 May─June provided a unique opportunity to analyze, over a broad range of heliolongitudes, the effects produce... | [
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Kinematics of Circumgalactic O VI Gas and Disk Rotation of z ≍ 0.2 Star-forming Galaxies. Quasar sightline observations reveal that low ionization state gas corotates with the galaxy disk and often at subcentrifugal velocities, suggesting that the gas is spiraling toward the galaxy disk. However, while observations ubi... | [
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Bayesian Inference of Hybrid Star Properties from Future High-precision Measurements of Their Radii. Future high-precision X-ray and gravitational-wave observations of neutron stars (NSs) are expected to constrain NS radii with uncertainties as small as σ ≃ 0.1 km. Such unprecedented precision offers a unique opportuni... | [
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A Unified Photometric Redshift Calibration for Weak Lensing Surveys Using the Dark Energy Spectroscopic Instrument. The effective redshift distribution n(z) of galaxies is a critical component in the study of weak gravitational lensing. Here, we introduce a new method for determining n(z) for weak lensing surveys based... | [
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Joint Constraint on the Propagation Origin of the Cosmic-Ray Spectral Knee from Energy Spectrum and Anisotropy Observations. The origin mechanism of the cosmic-ray knee region remains an unresolved mystery, with acceleration, interaction, and propagation models drawing significant attention. The latest experimental obs... | [
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Thermal Effects of Acoustic-gravity Waves in Titan's Upper Atmosphere and Their Implications for Atmospheric Jeans Escape. Early observations from the Cassini spacecraft revealed the presence of acoustic-gravity waves in Titan's upper atmosphere. However, the impacts of wave modes with different temporal and spatial sc... | [
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Radio Emission from Broad Absorption Line Quasars. Broad Absorption Line Quasars (BALQs) generally exhibit significant outflows that may interact with the surrounding medium, resulting in radio emission. We selected a sample of 13 powerful radio-quiet (RQ) BALQs, where the UV outflow kinetic power is measurable, and de... | [
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Environment and Gas Fraction in Type 2 AGN versus Non-AGN Galaxies. We investigate the environmental parameters and gas fraction (fgas ) properties of type 2 active galactic nuclei (AGN) and non-AGN galaxies, utilizing a large sample of galaxies from the Sloan Digital Sky Survey DR7 with z ≤ 0.3. We find that the envir... | [
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Joint Analysis of Small-scale Galaxy Clustering and Galaxy─Galaxy Lensing from BOSS Galaxies. We present a joint analysis of galaxy clustering and galaxy─galaxy lensing measurements from BOSS galaxies using a simulation-based emulation method combined with a halo occupation distribution model. Our emulators are constru... | [
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Prediction of Multiwavelength Afterglows Associated with FRB 20200120E and FRB 20201124A. Fast radio bursts (FRBs) are mysterious radio transients with uncertain origins and environments. Recent studies suggest that some active FRBs may originate from compact objects in binary systems. In this work, we develop a unifie... | [
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An Improved Fit to the Density Fluctuations in Supersonic Isothermal Turbulence. The density distribution of supersonic isothermal turbulence plays a critical role in many astrophysical systems. It is commonly approximated by a log-normal distribution with a variance of σs,V2≍ln(1+b2MV2) , where s≡lnρ/ρ0, MV is the r... | [
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How Beaming Shapes the Demographics of Ultraluminous X-Ray Sources. Ultraluminous X-ray sources (ULXs) are off-nuclear compact objects with apparent luminosities above 1039 erg s−1, often exceeding the Eddington limit for stellar-mass black holes. Beaming is a commonly invoked mechanism to explain their extreme brightn... | [
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Characterizing Compact-object Binaries in the Lower Mass Gap with Gravitational Waves. The source binary of the gravitational-wave (GW) event GW230529, detected at the beginning of the fourth LIGO-Virgo-KAGRA observing run, was inferred to consist of a neutron star (NS) and a compact object in the lower mass gap, a pur... | [
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Danger Zone: Establishing Buffers for Enhanced Classification in BPT Diagrams. This study utilizes unsupervised machine learning, specifically the uniform manifold approximation and projection (UMAP) algorithm, to classify optical spectra originating from star-forming regions, Seyferts, and low-ionization (nuclear) emi... | [
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Testing the Physical Parameter Constraining Power of HCN and HNC with Neural Networks. We quantify the utility of HCN and HNC to characterize gas conditions in the nearby starburst galaxy NGC 253. We use measurements from the Atacama Large Millimeter/Submillimeter Array (ALMA) Large Program ALCHEMI: the ALMA Comprehens... | [
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Multimessenger Modeling of Low-luminosity γ-Ray Bursts. Low-luminosity γ-ray bursts (LL GRBs), a subclass of the most powerful transients in the Universe, remain promising sources of high-energy astrophysical neutrinos, despite strong IceCube constraints on typical long GRBs. In this work, a novel approach is introduce... | [
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Investigating FRB 20240114A with FAST: Morphological Classification and Drifting Rate Measurements in a Burst-cluster Framework. This study investigates the morphological classification and drifting rate measurement of the repeating fast radio burst (FRB) source FRB 20240114A using the Five-hundred-meter Aperture Spher... | [
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ALMA Observations of Cold Methanol Gas in the Large Magellanic Cloud: N79 South Giant Molecular Cloud. We report Atacama Large Millimeter/submillimeter Array continuum and molecular line observations at 0.1 pc resolution toward the super star cluster (SSC) candidate H72.97−69.39 in the N79 region of the LMC. The contin... | [
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SDSS-V LVM: Collisionless Shocks in the Supernova Remnant RCW86. The supernova remnant (SNR) RCW86 is among the few SNRs with Balmer-emission lines containing broad and narrow spectral components that trace fast, nonradiative shocks in partially ionized gas. These are invaluable laboratories for collisionless shock phy... | [
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The [Fe XIII] Infrared 10747 and 10798 Å Lines in Novae. The forbidden lines of [Fe XIII] at 10747 and 10798 Å are among the most prominent lines in the near-infrared spectrum of the solar corona. They have been used routinely, both outside and during eclipses, as sensitive probes of the electron density and polarizati... | [
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The Fate of Gaia's Wide Binaries: Interplay of White-dwarf Recoil and Tidal Interactions. White dwarfs (WDs) receive natal velocity boosts of ∼1 km s−1 due to recoil from asymmetric mass loss during the late asymptotic giant branch (AGB) stage. In a wide binary, the acceleration of a WD progenitor exerts a torque, modi... | [
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Effects of Numerical Resolution on Simulated Cloud─Wind Interactions. Mixing by hydrodynamical instabilities plays a key role in cloud─wind interactions, causing cloud destruction in the adiabatic limit and facilitating cloud survival with efficient radiative cooling. However, the rate of mixing in numerical simulation... | [
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The Structure and Kinematics of Three Class 0 Protostellar Jets from JWST. We present observations of jets within 2000 au of three deeply embedded protostars using 2.9─27 μm observations with JWST. These observations show the morphologies and kinematics of the collimated jets from three protostars, the low-mass Class 0... | [
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Primitive Crust Buried Below the Southern Highland of Mars. Geochemical studies of shergottites have predicted an enriched end member associated with the final residual liquid of the Martian magma ocean, which may result in the formation of a KREEP-like silica-rich primitive crust on early Mars. In this work, we invest... | [
"http://astrothesaurus.org/uat/1007",
"http://astrothesaurus.org/uat/1248",
"http://astrothesaurus.org/uat/1005"
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Coronal Hole Boundary Region: Multiple Facets and Connection to the Slow Solar Wind. It is commonly recognized that a coronal hole (CH) boundary region exists where the slow solar wind (SW) is formed by more than one physical process. The physical properties at the CH boundary region play an important role in dictating... | [
"http://astrothesaurus.org/uat/1873",
"http://astrothesaurus.org/uat/1504",
"http://astrothesaurus.org/uat/1493",
"http://astrothesaurus.org/uat/1534",
"http://astrothesaurus.org/uat/2038",
"http://astrothesaurus.org/uat/1483",
"http://astrothesaurus.org/uat/1503",
"http://astrothesaurus.org/uat/1484"... | [
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"Solar magnetic reconnection",
"Solar extreme ultraviolet emission",
"Solar wind",
"Solar coronal lines",
"Solar corona",
"Solar magnetic fields",
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"http://astrothesaurus.org/uat/1322",
"http://astrothesaurus.org/uat/1430",
"http://astrothesaurus.org/uat/1554"
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"Meridian",
"Quiet sun",
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JWST Reveals a Candidate Jellyfish Galaxy at z = 1.156. We report the discovery of COSMOS2020-635829 as a candidate jellyfish galaxy undergoing ram pressure stripping in a (proto)cluster at z > 1. High-resolution imaging from the James Webb Space Telescope reveals a symmetric stellar disk coupled to a unilateral tai... | [
"http://astrothesaurus.org/uat/584",
"http://astrothesaurus.org/uat/2007",
"http://astrothesaurus.org/uat/2126",
"http://astrothesaurus.org/uat/2125",
"http://astrothesaurus.org/uat/1569",
"http://astrothesaurus.org/uat/594",
"http://astrothesaurus.org/uat/597",
"http://astrothesaurus.org/uat/2171"
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"High-redshift galaxy clusters",
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"http://astrothesaurus.org/uat/1614",
"http://astrothesaurus.org/uat/1622",
"http://astrothesaurus.org/uat/2291"
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"Galaxy stellar disks",
"Stellar masses",
"Stellar populations",
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