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Pulsations Change the Structures of Massive Stars before Explosion: Interpreting SN 2023ixf and SN 2024ggi. Massive red supergiants (RSGs) are known to become hydrodynamically unstable before they explode. Still, the vast majority of supernova (SN) models assume RSG progenitors in hydrostatic equilibrium. Here we follo... | [
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Sound-horizon-agnostic Inference of the Hubble Constant and Neutrino Masses from Baryon Acoustic Oscillations, Cosmic Microwave Background Lensing, and Galaxy Weak Lensing and Clustering. We present a sound-horizon-agnostic determination of the Hubble constant, H0, by combining DESI Data Release 2 baryon acoustic oscil... | [
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A Multimessenger Search for the Supermassive Black Hole Binary in 3C 66B with the Parkes Pulsar Timing Array. A subparsec supermassive black hole binary (SMBHB) at the center of the galaxy 3C 66B is a promising candidate for continuous gravitational-wave searches with pulsar timing arrays (PTAs). In this work, we searc... | [
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Bayesian Inference of Gravity through Realistic 3D Modeling of Wide Binary Orbits: General Algorithm and a Pilot Study with HARPS Radial Velocities. When 3D relative displacement r and velocity v between the pair in a gravitationally bound system are precisely measured, the six measured quantities at one phase can allo... | [
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Joint Observation of SGR J1935+2154 with Insight-HXMT and KM40m during the Active Episode of 2022 October. SGR J1935+2154 is the so-far unique magnetar from which fast radio bursts (FRBs) have been detected. In 2022 October, it resumed its burst activity, and we implemented a dedicated target-of-opportunity observation... | [
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JWST/MIRI-MRS View of the Metal-poor Galaxy CGCG 007-025: The Spatial Location of Polycyclic Aromatic Hydrocarbons and Very Highly Ionized Gas. Polycyclic aromatic hydrocarbons (PAHs) are key diagnostics of the physical conditions in the interstellar medium and are widely used to trace star formation in the mid-infrare... | [
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First Detailed MeerKAT Imaging Spectroscopy of a Solar Flare. Radio observations provide powerful diagnostics of energy release, particle acceleration, and transport processes in solar flares. However, despite recent progress in radio interferometric imaging spectroscopy, current instruments still face limitations in i... | [
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The Role of Faraday Rotation in the Polarization of the X-Rays from Magnetically Powered Black Hole Coronas. Magnetic reconnection is one of the prime candidate mechanisms that may energize the plasma emitting the strongly polarized X-ray emission from black hole X-ray binaries (BHXRBs) in their hard states. The mechan... | [
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Gravitational Lenses in UNIONS and Euclid (GLUE). I. A Search for Strong Gravitational Lenses in UNIONS with Subaru, CFHT, and Pan-STARRS Data. We present the results of our pipeline for discovering strong gravitational lenses in the ongoing Ultraviolet Near-Infrared Optical Northern Survey (UNIONS). We successfully tr... | [
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Multiwavelength Variability and Jet Properties of Low-synchrotron-peaked BL Lacertae Objects. Low-synchrotron-peaked BL Lac objects (LBLs) are promising candidates for masquerading BL Lacs, and the mechanism responsible for their high-energy γ-ray emission still requires further investigation. In this paper, we conduct... | [
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Resonant Scattering of the He I 1.0833 μm Triplet in H II Regions: Emission Spectra. Resonant scattering of He I 1.0833 μm triplet photons by metastable He 2 3S1 is studied for optical depths characteristic of H II regions. Regions with large He 2 3S1 column densities are predicted to have unusually broad multipeaked 1... | [
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Multiband ALMA Polarization Observations of BHB 07-11 Reveal Aligned Dust Grains in Complex Spiral Arm Structures. Polarization-mode observations from the Atacama Large Millimeter/submillimeter Array (ALMA) are powerful tools for studying the dust grain populations in circumstellar disks. Many sources exhibit polarizat... | [
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A Comprehensive Interpretation of Fermi-LAT Pulsars: Fundamental-plane Death Border, Visibility Thresholds, and GeV─TeV Unification. We present a framework that links equatorial-current-sheet (ECS) physics to catalog-level, phase-averaged gamma-ray pulsar properties. Guided by analytic scalings and particle-in-cell (PI... | [
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The Solar Origin and Life Project: Detailed Characterization of Candidates for the Zero Age Main-sequence and Subgiant Stages. The context of the Sun in the Galactic neighborhood is not well understood, especially when we compare its physical properties to those of nearby stars. Thereby, we still cannot fully comprehen... | [
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A Simulation Study of an HFA-like Event at Mars. Hot flow anomalies (HFAs) are transient structures at planetary bow shocks characterized by hot, tenuous plasma. At Mars, where no global dipole field exists, such events interact with the induced magnetosphere in a unique and poorly understood way. This study employs a ... | [
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Direct Measurement of <SUP>59</SUP>Cu(p,α)<SUP>56</SUP>Ni Precludes a Strong NiCu Cycle in Type-I X-Ray Bursts. Model-observation comparisons of type-I X-ray bursts (XRBs) can reveal the properties of accreting neutron star systems, including the neutron star compactness. XRBs are powered by nuclear burning, and a hand... | [
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Unveiling SN 2022eyw: A Bright Member of the Type Iax Supernova Subclass. We present comprehensive photometric and spectroscopic observations of SN 2022eyw, a luminous member of the Type Iax supernova (SN Iax) subclass. SN 2022eyw reached a peak absolute magnitude of Mg = ─17.80 ± 0.15 mag and exhibited a rise time of ... | [
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Solar Wind Forecasting for Long-term Variations of the Global Heliosphere. The large-scale dynamics of the heliosphere is driven by solar activity and variable solar wind (SW) conditions. In situ SW observations inform time-dependent heliosphere modeling efforts but are only available up until the present day, thus res... | [
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Impact of Coronal Mass Ejection-driven Enhanced Magnetic Pressure on the Martian Northern Hemispheric Ionosphere during 2024 May 17─18. The Martian northern hemisphere (NH) is relatively devoid of ambient magnetic fields compared to the southern hemisphere (SH), which houses the strong crustal field regions. On 2024 Ma... | [
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Spectroscopic Signatures and Photochemical Stability of the ClSO<SUB>3</SUB> and ClOSO<SUB>2</SUB> Radicals: New Benchmarks for Atmospheric and Astrochemical Models. Chlorine─sulfur oxides represent potentially important yet largely uncharacterized intermediates in atmospheric and astrochemical environments, from explo... | [
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Dynamics of Slow Solar Wind Emerging from an Equatorial Coronal Hole. We present a three-dimensional reduced magnetohydrodynamics model to depict turbulence induced by Alfvén waves within the slow solar wind originating from an open magnetic field positioned in a coronal hole near the solar equator. The nonlinear inter... | [
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The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z = 1.5─4.4. I. A Diversity of Nebular Attenuation Curves and Evidence for Non-unity Dust Covering Fractions. We present the nebular attenuation curves and dust covering fractions for 24 z = 1.5─4.4 star-forming galaxi... | [
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Hot Springs and Dust Reservoirs: JWST Reveals the Dusty, Molecular Aftermath of Extragalactic Stellar Mergers. We present James Webb Space Telescope (JWST) observations of four luminous red novae (LRNe): dusty, extragalactic transients from stellar mergers following common-envelope evolution (CEE) in massive binary sta... | [
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The Effect of Tidal Heating and Volatile Budgets on the Outgassed Atmosphere of 55 Cancri e. 55 Cancri e (55 Cnc e) is an ∼8 Gyr rocky world (1.95 R⊕ and 8.8 M⊕) orbiting a K-type star. JWST observations suggest a carbon-dominated atmosphere (CO2 and CO) over a global magma ocean (>3000 K). We suggest that any CO2-d... | [
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Chaotic Motion of Ions in Finite-amplitude Low-frequency Alfvén Waves. Finite-amplitude low-frequency Alfvén waves (AWs) are ubiquitous in space plasmas, where they play a key role in the transport and dissipation of energy, particularly in the heating of ions in the solar corona and solar wind. In this study, we inves... | [
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HST Study of the Proper Motion of HST-1 in the Jet of M87. The radio galaxy M87 is well known for its jet, which features a series of bright knots observable from radio to X-ray wavelengths. The most famous of these, HST-1, exhibits superluminal motion, and our analysis of Chandra data reveals a correlation between the... | [
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Reconstructing the Assembly of Massive Galaxies. III. Quiescent Galaxies Lose Angular Momentum as They Evolve in a Mass-dependent Fashion. We study the evolution of stellar kinematics of a sample of 952 massive quiescent galaxies with M* > 1010.5 M⊙ at 0.6 < z < 1. Utilizing spatially integrated spectroscopy f... | [
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A Portrait of the Cosmic Reionization History in the Context of the Early Dark Energy Model. Recent JWST observations of Lyα emission at z ∼ 11─6 indicate a rapid reionization of the intergalactic medium within the first ∼700 Myr. The required Lyman continuum (LyC) photon budget may naturally arise from the unexpectedl... | [
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Upper Limits on Microhertz Gravitational Waves from Supermassive Black Hole Binaries Using PSR J1909─3744 Data from the Second IPTA Data Release. We present the results of a search for gravitational waves (GWs) from individual sources using high-cadence observations of PSR J1909−3744 obtained during an intensive observ... | [
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Coronal Mass Ejection Transit Time Prediction Based on Spatiotemporal Modeling Using 3D Convolutional Neural Networks. Coronal mass ejections (CMEs) are intense solar eruptions that, once reaching Earth, pose catastrophic risks to the near-Earth space environment. Thus, improving CME transit time forecast accuracy to m... | [
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Parallaxes, Proper Motions, and Near-infrared Photometry for 173 L and T Dwarfs from the US Naval Observatory Infrared Astrometry Program. We present near-infrared parallax and proper motion astrometry for 74 L dwarfs and 99 T dwarfs, as single objects or in binary systems, obtained with the ASTROCAM astrometric imager... | [
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Calibrating Mid-infrared Emission Features as Diagnostics of Star Formation in Infrared-luminous Galaxies via Radiative Transfer Modeling. Luminous infrared (IR) galaxies are key sites of obscured stellar mass assembly at z > 0.5. Their star formation rates (SFRs) are often estimated using the luminosities of the 6.... | [
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Simulations of Electron Beam Interactions in Brown Dwarf Atmospheres. Over two decades ago, the first detection of electron cyclotron maser instability radio emission from a brown dwarf confirmed the presence of aurorally precipitating electrons on these objects. This detection established that brown dwarfs can exhibit... | [
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Observational Evidence Linking Loop Length and Thermal─Nonthermal Peak Timing in Solar Flares. We investigate how the magnetic loop length of solar flares relates to the timing between their thermal and nonthermal emission signatures. Our study analyzes a sample of 96 C-, M-, and X-class flares observed between 2013 an... | [
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Correlations between Dust Extinction Features across All Wavelength Scales: From Diffuse Interstellar Bands to R(V). Understanding variations in the dust extinction curve is imperative for using dust as a tracer of local structure in the interstellar medium, understanding dust chemistry, and performing extinction corre... | [
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Looking at Infrared Background Radiation Anisotropies with Spitzer. II. Small Scale Anisotropies and their Implications for New and Upcoming Space Surveys. Spitzer-based source-subtracted cosmic infrared background (CIB) fluctuations at arcminute-to-degree scales indicate the presence of new populations, whereas subarc... | [
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A z ≃ 0.4 Galaxy Reflecting the High-redshift Little Red Dots: An Extended Starburst with an Overmassive Black Hole. One of the most remarkable discoveries of JWST is a population of compact, red sources at z > 4, commonly referred to as Little Red Dots (LRDs). Spectroscopic identifications reported that most LRDs a... | [
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NEXUS: A Spectroscopic Census of Broad-line AGNs and Little Red Dots at 3 ≲ z ≲ 6. We present a spectroscopic sample of 24 broad-line AGNs (BLAGNs) at 3 ≲ z ≲ 6 selected using F322W2+F444W NIRCam/WFSS grism spectroscopy of the central 100 arcmin2 area of the NEXUS survey. Among these BLAGNs, 15 are classified as Little... | [
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Constraining Properties of Dust Formed in Wolf─Rayet Binary WR 112 Using Mid-infrared and Millimeter Observations. Binaries that host a carbon-rich Wolf─Rayet (WC) star and an OB-type companion can be copious dust producers. Yet the properties of dust, particularly the grain size distribution, in these systems remain u... | [
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The Perpendicularity of Dust Lanes and Radio Jets in Early-type Galaxies: Implications for Active Galactic Nuclei Feedback. The orientation of radio jets relative to their host galaxies offers an interesting avenue for probing the connection between active galactic nuclei (AGN) and their surroundings. Several studies h... | [
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Ubiquitous High-frequency Waves and Disturbances in the Active Region Corona Observed with Cryo-NIRSP. The plasma of the solar corona harbors a multitude of coronal wave modes, some of which could be dissipated to provide the required energy and momentum to heat the corona and accelerate the solar wind. We present obse... | [
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Anomalous Narrow Line Seyfert I Galaxies from SDSS DR17. We present an analysis of 22,656 narrow-line Seyfert 1 galaxies (NLSy1s) from the Sloan Digital Sky Survey (SDSS) DR17 (0.1 ≤ z ≤ 0.9), identifying a sample of spectroscopically anomalous sources. These anomalies were detected via the Spectroscopic Quasar Anomaly... | [
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Atmospheric Circulation of High-obliquity Mini-Neptunes. With the operation of JWST, atmospheric characterization has now extended to low-mass exoplanets. In compact multiplanetary systems, secular spin-orbital resonance may preserve high obliquities and asynchronous rotation even for tidally despinning, low-mass plane... | [
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Instabilities, Wave Emission, and Energy Transport along Bursty Bulk Flows and Supra-arcade Downflows: Differences, Similarities, and Effects on the Surrounding Regions. We examine the stability conditions for two posteruptive phenomena in the solar─terrestrial environment, namely, bursty bulk flows (BBFs) in the Earth... | [
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The Role of Gas Stripping in the Quenching of Satellite Galaxies Using SHARK v2.0. Observational studies have made substantial progress in characterizing quenching as a function of galaxy stellar mass and environment, but they are often limited in their ability to constrain quenching timescales and to determine the dom... | [
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CW Cas: A Solar-type Contact Binary System with an Unseen Third Companion in a Hierarchical Quadruple System. We present a comprehensive multiband photometric and spectroscopic study of the G-type binary CW Cas. Analysis of its double-lined spectroscopic radial velocity curves yields a reliable mass ratio of q = 1.88(9... | [
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The Cosmic Owl: Twin Active Collisional Ring Galaxies with Starburst Merging Front at z = 1.14. Galaxy mergers play a critical role in driving galaxy evolution, especially by transforming galaxy morphology, redistributing gas around galaxies, triggering active galactic nuclei (AGN), and stimulating star formation. We p... | [
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Investigation of the Quasi-periodic Oscillation Phase Lag of RE J1034+396. We conduct an in-depth study of the quasi-periodic oscillation (QPO) properties of RE J1034+396 by constructing QPO phase-folded light curves from 10 XMM-Newton observations during 2020─2021. Our analysis reveals that the QPO in the source exhib... | [
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An Investigation of 5 yr Simultaneous X-Ray and Radio Light Curves of the Dwarf Seyfert Galaxy UGC 6728. We present serendipitous simultaneous radio and X-ray light curves of the dwarf Seyfert galaxy UGC 6728 spanning 5 yr. The X-ray light curve exhibits a flaring period, followed by a gradual rise and decline. Through... | [
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Saturation of the Large-scale Magnetic Field for Fast Rotating Solar-like Stars Driven by Inefficient Turbulent Angular Momentum Transport. Magnetic activity in solar-like stars shows a systematic dependence on stellar rotation rate, known as the "activity─rotation relationship." Recent observations further reveal that... | [
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BRITE Nanosat Photometry Reveals Bright Spots in the Single Wolf─Rayet Star EZ CMa That Can Drive Spectral-line-emitting Corotating Interaction Regions. We analyze an unprecedented 4.5 contiguous months of 2015─2016 BRITE nanosatellite precision optical photometry of the 7th mag Wolf─Rayet (WR) star EZ CMa = WR 6 = HD ... | [
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Energy Bounds from Relative Magnetic Helicity in Spherical Shells. Relative magnetic helicity is commonly used in solar physics to avoid the well-known gauge ambiguity of standard magnetic helicity in magnetically open domains. However, its physical interpretation is challenging, owing to the invocation of a reference ... | [
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The Extended Mapping Obscuration to Reionization with ALMA (Ex-MORA) Survey: 5σ Source Catalog and Redshift Distribution. One of the greatest challenges in galaxy evolution over the last decade has been constraining the prevalence of heavily dust-obscured galaxies in the early Universe. At z > 3, these galaxies are ... | [
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Far-infrared Emission Lines as Metallicity Diagnostic. The chemical abundance of the interstellar medium is a key tracer of galaxy evolution. Optical and ultraviolet emission lines are widely used to derive gas-phase metallicities, but suffer from uncertainties due to possible temperature fluctuations and extinction co... | [
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EIGER. VIII. First Stars Signatures in the Connection between O I Absorption and Galaxies in the Epoch of Reionization. We investigate the association between galaxies and neutral O I absorption systems at z ∼ 6, which trace metal-enriched gas during the epoch of reionization. We identify 40 galaxies across six quasar ... | [
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Wave Generation via Oscillatory Reconnection at a Three-dimensional Magnetic Null Point. This work conducts a three-dimensional (3D), nonlinear magnetohydrodynamic (MHD) simulation to investigate wave-generating, time-dependent reconnection around a magnetic null point. A nonperiodic perturbation (in the xz-plane) trig... | [
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Fastest or Significant: A Systematic Framework for Validating Global Minimum Variability Timescale Measurements of Gamma-Ray Bursts. The minimum variability timescale (MVT) is a key observable for probing the central engines of gamma-ray bursts, constraining both the emission region size and outflow Lorentz factor. How... | [
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The Phase Spiral's Origin and Evolution: Indications from Its Varying Properties across the Milky Way Disk. The phase spiral is a perturbation to the vertical phase-space distribution of stars in the Milky Way disk. We study the phase spiral's properties and how they vary with spatial position, in order to constrain it... | [
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Early Stages of Protostellar Disk Evolution: A Link to the Initial Cloud Core. We study the structure and evolution of the very early protostellar disk ("protodisk") just after protostar formation, where disk self-gravity dominates and the stellar contribution is dynamically minor. The disk redistributes angular moment... | [
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Shock Acceleration in the Intracluster Medium: Implications of Micromirror Confinement. Merging galaxy clusters exhibit strong observational evidence for efficient particle acceleration in the intracluster medium (ICM), particularly in the form of synchrotron-emitting radio relics and halos. Cosmic-ray (CR) electrons a... | [
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Planet Migration in Protoplanetary Disks with Rims. Complex structures, including sharp edges, rings, and gaps, have been commonly observed in protoplanetary disks with or without planetary candidates. Here we consider the possibility that they are the intrinsic consequences of angular momentum transfer mechanisms and ... | [
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Multiwavelength Signatures of Supernova Shock Breakout from Red Supergiants in Two Dimensions. We present new two-dimensional radiation hydrodynamic simulations of supernova shock breakout from red supergiants (RSGs) using the CASTRO code. Our progenitors are 20 and 25 M⊙ solar-metallicity stars evolved from the zero-a... | [
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Persistence of Solar Wind Velocity along Radial, Longitudinal, and Latitudinal Spacecraft Separation. Recent missions, including the Parker Solar Probe, Solar Orbiter, and the Mars Atmosphere and Volatile EvolutioN (MAVEN), have probed a wide range of heliocentric distances, enabling new investigations of solar wind ev... | [
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The Reliability of Local Correlation Tracking for Inferring Photospheric Intensity Vortices. Magnetoconvective simulations of the solar photosphere show ubiquitous formation of vortices in intergranular lanes, which are thought to contribute to the energy transfer between atmospheric layers. Observationally, these vort... | [
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Hydrogen-poor Superluminous Supernovae in the Nebular Phase: Spectral Diversity Due to Ejecta Ionization as a Probe of the Power Source. We present a large sample of 39 nebular-phase optical spectra of 25 hydrogen-poor superluminous supernovae (SLSNe-I) and jointly analyze them with previously published spectra of 12 e... | [
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The First Quantitative Study of Cometary Tail Regrowth following a Coronal Mass Ejection-driven Disconnection Event. Comet C/2023 P1 (Nishimura) was observed by the Solar Orbiter Heliospheric Imager (SoloHI), on board the Solar Orbiter spacecraft, from 2023 September 1 to 14. During this period, the ion tail of the com... | [
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Sigmoid Formation, Filament Destabilization, and Initiation of Weak Flare by Tether Cutting Reconnection. We have studied a B-class solar flare and an associated filament eruption through multiwavelength observations. The flare is triggered at 16:24 UT on 2017 June 7 from Active Region(AR) 12661, and it maximizes at 16... | [
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HOPS-288: A Laboratory for Complex Organics in Proto-binary/Proto-multiple Systems. Complex organic molecules (COMs) in young stellar objects have attracted significant attention in recent years due to their potential connection to prebiotic chemistry and their utility as tracers of warm or shocked gas components. Prot... | [
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Unipolarity of the Solar Magnetic Field in Equatorial Coronal Holes. A study of the unbalanced magnetic polarity distribution of 70 coronal holes was performed. Data from the Helioseismic and Magnetic Imager were used to examine the photospheric line-of-sight magnetic field (BLOS) beneath these coronal holes. The skewn... | [
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The Collision and Merger Products of Stars Do Not Look Alike: A Magnetohydrodynamics Comparison. A significant fraction of stars experience close interactions, including collisions resulting from gravitational encounters and mergers within close binary systems. These processes can produce more massive stars that may gi... | [
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A Single-pulse Study of Three CRAFTS Pulsars Discovered with FAST. We present a comprehensive single-pulse study of three pulsars, namely PSRs J1854─0036, J2159+0202, and J2112+0740, discovered by the Five-hundred-meter Aperture Spherical radio Telescope (FAST) in the Commensal Radio Astronomy FAST Survey (CRAFTS). We ... | [
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Herringbone Structures during an X-class Eruptive Flare. In this paper, we report quasiperiodic herringbone structures during the impulsive phase of an X-class flare, coinciding with the distinct acceleration phase of eruptive prominence ejection on 2023 December 31. The prominence propagates nonradially in the southea... | [
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Properties and Possible Physical Origins of γ-Ray Emission in Extreme Synchrotron Blazars. Extreme synchrotron blazars, characterized by a first peak in their broadband spectral energy distributions (SEDs) at frequencies exceeding 1017 Hz, often exhibit a second peak beyond 1 TeV. These sources serve as ideal laborator... | [
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JWST Discovery of High-velocity Mid-infrared Ionized Outflows in Ultraluminous Infrared Galaxies F11119+3257 and F05189-2524. Ultrafast outflows (UFOs) are thought to be a driving mechanism of large-scale winds driven by active galactic nuclei (AGN), which cause significant galactic feedback through quenching star form... | [
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HR-GO. II. Chemical Abundances of Low-E Retrograde Dynamically Tagged Groups: Revealing Thamnos as a Very Metal-poor Substructure. Milky Way halo substructures identified in dynamical space are known to suffer from contamination from the Milky Way in situ stars, which makes their accreted origins uncertain. We present ... | [
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The Dichotomy in the Nuclear and Host-galaxy Properties of High-redshift Quasars. The early growth of high-redshift quasars and their host galaxies raises critical questions about their cosmic evolution. We exploit the angular resolution and sensitivity of NIRCam to investigate the host galaxies of 31 quasars at 4 ≲ z ... | [
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The Lyα and Continuum Origins Survey. II. The Connection between the Escape of Ionizing Radiation and Lyα Halos in Star-forming Galaxies. One of the current challenges in galaxy evolution studies is to establish the mechanisms that govern the escape of ionizing radiation from galaxies. Here, we investigate the connecti... | [
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Solving Milky Way─sized Systems with HASKAP PIE: A Halo Finding Algorithm with Efficient Sampling, K-means Clustering, Tree-assembly, Particle Tracking, Python Modules, Intercode Applicability, and Energy Solving. We describe a new Python-based stand-alone halo finding algorithm, HASKAP PIE, that combines several metho... | [
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The Stripped-star Ultraviolet Magellanic Cloud Survey (SUMS): The Ultraviolet Photometric Catalog and Stripped-star Candidate Selection. Most massive stars (∼8─25M⊙) interact with a binary companion during their lifetimes. These interactions can remove the hydrogen-rich envelope, producing intermediate-mass (∼2─8M⊙) an... | [
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Stellar Populations in the Extreme Outer Halo of the Spiral Galaxy M96. We use deep Hubble Space Telescope imaging to study stellar populations in the outer halo of the spiral galaxy M96, located in the dynamically active Leo I galaxy group. Our imaging targets two fields at a projected distance of 50 kpc from the gala... | [
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Fast X-Ray Transients in NuSTAR Data. Fast X-ray transients (FXTs) are flashes of X-rays that last for a few hundreds of seconds to a few hours. An enigmatic population of these transients that did not have a clear origin has been known for several decades, mostly found serendipitously in soft X-ray imaging observation... | [
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A Multiwavelength ALMA View of Gas and Dust in Binary Protoplanetary System AS 205: Evidence of Dust Asymmetric Distribution. We present Atacama Large Millimeter/submillimeter Array observations of multiwavelength dust emissions at 3.1 and 1.3 mm, along with molecular line emissions of CO(2─1), CO(3─2), 13CO(3─2), and ... | [
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Universal Stochastic Process in Blazar Gamma-Ray Variability Revealed by Bayesian Kernel Comparison. Although Gaussian processes have been widely applied in modeling the high-energy light curves of blazars, a systematic comparison of the performances of different kernel functions within Gaussian processes has remained ... | [
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Effect of Flow-aligned External Magnetic Fields on Mushroom Instability. Mushroom instability (MI) is a shear instability considered to be related to generating and amplifying magnetic fields in relativistic jets. While astrophysical jets are usually magnetized, how MI acts in magnetized jets remains poorly understood.... | [
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Ion-neutral Drift Velocity as a Diagnostic of Dust Growth and Magnetic Fields in Star-forming Environments. Recent observations have revealed that the ion-neutral drift velocity in star-forming molecular clouds and dense cores is on the order of ∼100 m s−1. Theoretical studies have shown that, in ambipolar diffusion—th... | [
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Studies in Astronomical Time Series Analysis. VIII. The Double Lomb─Scargle Periodogram and Super Resolution. Multiple-frequency periodograms—based on time-series models consisting of two or more independent sinusoids—have long been discussed. What is new here is the presentation of a practical, simple-to-use computati... | [
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Long-term Timing Evolution of Four Anomalous X-Ray Pulsars. Anomalous X-ray pulsars (AXPs) and soft gamma-ray repeaters (SGRs) are believed to be manifestations of magnetars. Typically, AXPs exhibit higher X-ray luminosities, whereas SGRs are generally fainter and display significantly high signal-to-noise ratios only ... | [
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Investigating the Efficacy of Topologically Derived Time Series for Flare Forecasting. II. XGBoost Model. Solar flares are a primary driver of space weather, and forecasting their occurrence remains a significant challenge. This paper presents a novel flare prediction model based on topologically derived photospheric m... | [
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Investigating Possible Stellar Coronal Mass Ejections in M-type Dwarfs Using the CARMENES Data Release 1 Spectra. Stellar coronal mass ejections (CMEs) have significant impacts on surrounding exoplanets and stellar evolution. For M-type dwarf stars, hosting close-in habitable zones, frequent and intense stellar CMEs ma... | [
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