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SN 2023zcu: A Type IIP SN with Early Flash Features. We present a detailed photometric and spectroscopic analysis of the Type IIP supernova (SN) SN 2023zcu, which exploded in the galaxy NGC 2139 (redshift z = 0.006). SN 2023zcu exhibits a well-sampled light curve covering the rise, plateau, and nebular phases. It has a... | [
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"Type II supernovae",
"Astronomical techniques",
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"http://astrothesaurus.org/uat/1335",
"http://astrothesaurus.org/uat/1379"
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"Baade-Wesselink method",
"Ejecta",
"Light curves",
"Magnitude",
"Milky Way Galaxy",
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Revising the Milky Way Cepheid Calibration: Quantifying and Correcting for Previously Undetected Distance Modulus Errors in the Gaia-based Multiwavelength Period─Luminosity Relations. We examine the multiwavelength period─luminosity─color (PLC) relations for Cepheid variables in the Large and Small Magellanic Clouds an... | [
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REBELS─MOSFIRE: Weak C III] Emission Is Typical among Extremely UV-bright, Massive Galaxies at z ∼ 7. We present Keck/MOSFIRE H-band spectroscopic measurements covering the [C III] λ1907, C III] λ1909 doublet for a sample of eight z ∼ 7 spectroscopically confirmed star-forming galaxies drawn from the Reionization Era B... | [
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Complete Sampling of the uv Plane with Realistic Radio Arrays: Introducing the RULES Algorithm, with Application to 21 cm Foreground Wedge Removal. We introduce the Radio-array uv Layout Engineering Strategy (RULES), an algorithm for designing radio arrays that achieve complete coverage of the uv plane. Coverage is def... | [
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"Cosmology",
"Radio interferometers",
"H I line emission",
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Measuring the Central Dark Mass in NGC 4258 with JWST/NIRSpec Stellar Kinematics. We present a new stellar-dynamical measurement of the supermassive black hole (SMBH) mass in the nearby spiral galaxy NGC 4258 (M106), a critical benchmark for extragalactic mass measurements. We use archival James Webb Space Telescope (J... | [
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A Search for Millimeter-bright Blazars as Astrophysical Neutrino Sources. The powerful jets of blazars have been historically considered as likely sites of high-energy cosmic-ray acceleration. However, the particulars of the launched jet and the locations of leptonic and hadronic jet loading remain unclear. In the case... | [
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Bifractality and Crossover Behavior Observed in Solar Wind Intermittency by Parker Solar Probe: Rank-ordered Analysis and Partition Function Approach. Multifractal analysis of the intermittent solar wind magnetic energy fluctuations reveals new features of the young slow solar wind measured by Parker Solar Probe. The m... | [
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Orbital Classification in Rotating Bar Potentials Using an Empirical Proxy of the Second Integral of Motion. We present a novel method for classifying two-dimensional orbits in rotating bar potentials based on an empirical proxy for the second integral of motion, calibrated angular momentum (CAM), which is defined as t... | [
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Early Warning for Lensed Gravitational Wave Counterparts from Time Delays of Their Host Galaxies Observed in the Optical. Gravitational lensing of gravitational waves can be leveraged to provide early-warning times of O(hours) to O(days) before the merger of binary neutron stars (BNSs) and neutron star black holes ... | [
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Formation Channels of Magnetars. The formation channels of magnetars remain an open question. Although core-collapse supernovae of isolated massive stars are important, binary interactions—such as tidal interaction, common envelope evolution, and stellar mergers—may also play a significant role in making magnetars. Und... | [
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High-resolution Observations of "Dark" Neutral Hydrogen Clouds in the Virgo Cluster with the Very Large Array. We have observed six "dark" neutral hydrogen (H I) clouds discovered in the Virgo Cluster by the Arecibo Galaxy Environment Survey (AGES) with the Karl G. Jansky Very Large Array (VLA), giving higher angular a... | [
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The Radial Velocity Curve for He II Emission Cannot Be Used for Component Mass Determination in SS 433. More than 150 measurements of the He II 4686 Å emission line in spectra of SS 433 were obtained during 388 nights in 2020─2025 with the Transient Double-beam Spectrograph on the 2.5 m telescope of Caucasian Mountain ... | [
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Is the Milky Way Gravitationally Stable? A TNG50 View from the Cosmic Noon to the Present Day. We investigate the stability of Milky Way analogs (MWAs) in the TNG50 simulation against the growth of local axisymmetric instabilities, tracing their evolution from cosmic noon (z = 2.5) to the present day (z = 0). Using a t... | [
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Digging into the Interior of Hot Cores with ALMA (DIHCA). VII. Disk Candidates around High-mass Stars and Evidence of Anisotropic Infall. We study the kinematics of condensations in 30 fields forming high-mass stars with the Atacama Large Millimeter/submillimeter Array at a high resolution of ∼0.″08 on average (∼230 ... | [
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Low-metallicity Gas on the Outskirts of the Local Group: The Circumgalactic Medium of Sextans B. We present a UV absorption-line analysis of the circumgalactic medium (CGM) of Sextans B, a dwarf irregular galaxy at 1.3 Mpc distance on the outer frontier of the Local Group (LG). Using Hubble Space Telescope Cosmic Origi... | [
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The Milky Way Stellar Halo Is Twisted and Doubly Broken: Insights from DESI DR2 Milky Way Survey Observation. Using K giants from the second data release (DR2) of the Dark Energy Spectroscopic Instrument (DESI) Milky Way Survey, we measure the shape, orientation, radial profile, and density anisotropies of the Milky Wa... | [
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Critical Metallicity of Cool Supergiant Formation. II. Physical Origin. This study investigates the physical origin of the critical metallicity required for the formation of cool supergiants, as revealed by stellar evolution models. Using grids of stellar models, we show that the terminal-age main-sequence (TAMS) radiu... | [
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Growth of Metal-enriched Supermassive Stars by Accretion and Collisions. Supermassive stars (SMSs) are candidate progenitors of massive black hole seeds and may contribute to anomalous abundance patterns in high-redshift galaxies and globular clusters. Recent radiation-hydrodynamic simulations indicate that SMSs can fo... | [
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"http://astrothesaurus.org/uat/1289",
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Accretion Properties of the Young Brown Dwarf 2MASS J08440915-7833457. We present Hubble Space Telescope Cosmic Origins Spectrograph far-ultraviolet (FUV) and Space Telescope Imaging Spectrometer (STIS) optical observations toward the young accreting brown dwarf 2MASS J08440915-7833457 (J0844) from the UV Legacy Librar... | [
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The Self-limiting Nature of Jet-modulated Thermal Conduction in Cool Core Clusters. Conduction as a mechanism for explaining the disrupted cooling-flow in galaxy clusters has been mostly discounted, as the process is inefficient at transporting heat all the way from the cluster into the core. However, thermal conductio... | [
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Emergence of Photon Bose─Einstein Condensation from Down-scattering in Cold Electron Media. In this study, we investigate the kinematic enhancement of photon Bose─Einstein condensation (BEC) resulting from the interaction of high-energy photons with a cold electron gas. We employ a modified form of the Kompaneets equat... | [
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Modeling Solitonic Cores, Stabilization of Bar, and Suppression of Bar Dissolution in DDO 168 via GPP Formalism: A Detailed Analysis of Bose─Einstein Condensate/Fuzzy Dark Matter Halo Structure and Bar Dynamics in the Dwarf Galaxy DDO 168. The cusp─core problem remains a challenge to the ΛCDM model, since dwarf galaxie... | [
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Shapiro Delay Measurements from Fifteen Years of PSR J1231−1411 Radio Observations. We present 15 yr of Nançay and Green Bank radio telescope timing observations for PSR J1231−1411. This millisecond pulsar is a primary science target for the Neutron Star Interior Composition Explorer telescope (NICER, which discovered ... | [
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The Impact of Ram Pressure on the Radio Spectral Index and Magnetic Field of NGC 4522: A High-resolution VLA Continuum Study. We present high-resolution Very Large Array continuum observations at the S band (3 GHz, 560 pc scale) and X band (10 GHz, 200 pc scale) of the ram-pressure-stripped Virgo galaxy NGC 4522 to inv... | [
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Coherence of Supermassive Black Hole Binary Demographics with the nHz Stochastic Gravitational-wave Background. We present a refined estimation of the stochastic gravitational-wave background (SGWB) based on observed dual active galactic nuclei (AGNs) together with AGN X-ray luminosity functions, in light of recent Pul... | [
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A Census of Star-formation and Gas Mass Tracers in Two Lensed z ∼ 4 Dusty Star-forming Galaxies. We present new and archival Atacama Large Millimeter/submillimeter Array observations of two strongly lensed dusty star-forming galaxies (DSFGs) selected from the South Pole Telescope survey, SPT0418-47 (z = 4.225) and SPT2... | [
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Cloud─Cloud Collisions Induce Filament-mediated Super Star Cluster Formation in the Antennae Overlap Region: Evidence from ALMA and JWST. The formation of super star clusters (SSCs) in galaxies remains a fundamental yet unresolved problem. Among the proposed mechanisms, cloud─cloud collisions (CCCs) have been suggested... | [
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Ne and Fe Abundances in the Interstellar Medium: Archival Study of Fe-L and Ne-K Edges in Chandra and XMM-Newton. The abundance of elements in the interstellar medium is a key facet for many fields of astrophysical study. In the soft X-ray spectra, absorption by interstellar gas can result in deep absorption features t... | [
"http://astrothesaurus.org/uat/939",
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Equatorially Asymmetric Magnetic Fields and Their Impact on Black Hole Accretion Dynamics. We investigate the impact of equatorial asymmetry in the magnetic field geometry on accretion dynamics around a spinning black hole using axisymmetric general relativistic magnetohydrodynamic simulations. We consider a Fishbone─M... | [
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The Periastron Passage of T Tauri South B as Viewed by ALMA: Millimeter Flux Variations and Dust Heating Triggered by Orbital Motion. We present 225 and 350 GHz imaging of the iconic T Tauri system using the Atacama Large Millimeter submillimeter Array (ALMA). T Tauri is a hierarchical triple system, and the close bina... | [
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Envelope Inflation and Outflow Driven by Energy Deposition in Massive Stars. Evolved massive stars are known to undergo outflow with high-mass ejections, resulting in the loss of a substantial portion of their envelopes. One proposed mechanism driving these events is the release or deposition of energy within the stell... | [
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Rise of the Forsaken Relics: Connecting Present-day Stellar Streams and Phase-mixed Galaxies to the Epoch of Reionization. The "near─far" approach to studying reionization leverages the star formation histories of the Milky Way (MW) or Local Group (LG) galaxies, derived from resolved photometry, to infer the low-mass/f... | [
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First Resolution of a Main-sequence G star's Astrosphere Using Chandra. We report the resolution of a halo of X-ray line emission surrounding the zero-age main-sequence G8.5V star HD 61005 by Chandra/ACIS-S. Located only ∼36 pc distant, HD 61005 is young (100 ± 50 Myr) and X-ray bright (∼300 × solar), observed with a n... | [
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B-field Orion Protostellar Survey (BOPS). IV. The Relative Orientation between Magnetic Fields and Density Structures in Young Protostellar Envelopes. We investigate the relative alignment between density structures and magnetic fields in eight young protostars from the Atacama Large Millimeter/submillimeter Array B-fi... | [
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"http://astrothesaurus.org/uat/1565",
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"http://astrothesaurus.org/uat/1043",
"http://astrothesaurus.org/uat/1302",
"http://astrothesaurus.org/uat/1671"
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GW231123: Likely a Product of Successive Mergers from ∼10 Stellar-mass Black Holes. GW231123 is an exceptionally massive binary black hole (BBH) merger with unusually high component spins. Such extreme properties challenge conventional stellar evolution models, predicting a black hole (BH) mass gap due to pair-instabil... | [
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X-Ray Polarization of the Intrabinary Shock in Redback Pulsar J1723−2837. The intrabinary shocks (IBSs) in spider pulsars emit nonthermal synchrotron X-rays from accelerated electrons and positrons in the shocked pulsar wind, likely energized by magnetic reconnection. The double-peaked X-ray light curves from these sho... | [
"http://astrothesaurus.org/uat/1062",
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Dynamical Tide-modified Roche Limit in Eccentric, Asynchronous Binaries. The Roche limit, or the threshold separation within which a celestial object (the donor) M cannot remain in a stable configuration due to a companion's tidal field, has been well established when M is in hydrostatic equilibrium and has synchronous... | [
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"http://astrothesaurus.org/uat/497",
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"http://astrothesaurus.org/uat/498",
"http://astrothesaurus.org/uat/1184",
"http://astrothesaurus.org/uat/1207",
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Sulfur Enrichment in Close-in Exoplanet Atmospheres Induced by Pebble Drift across the Salt Line. Observations of JWST have revealed that several close-in exoplanets have sulfur-rich atmospheres through SO2 detections. Atmospheric sulfur is often thought to originate from solid accretion during planet formation, wherea... | [
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Evolution of Supermassive Black Hole Pairs on Inclined Orbits in Postmerger Galaxies. Theoretical models of the evolution of supermassive black hole (SMBH) pairs in postmerger remnant galaxies are necessary to motivate observational searches for dual active galactic nuclei (AGN) and gravitational-wave sources. Studies ... | [
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Inclination Bias in Techniques Used to Identify Be Star Candidates. Several methods for identifying Be star candidates are reviewed for observational bias with respect to system inclination, that is the angle between the stellar and disk rotation axis and the observer's line of sight, with focus on two photometric meth... | [
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Broadband Timing and Spectral Study of Accreting Millisecond X-Ray Pulsar SAX J1808.4─3658 during Its 2022 Outburst. We report on our investigation of the NuSTAR and AstroSat observations along with simultaneous NICER observations of the accreting millisecond X-ray pulsar SAX J1808.4─3658, obtained during its tenth out... | [
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Signatures of Large-scale Magnetic Field Disturbances and Switchbacks in Interplanetary Type III Radio Bursts. Type III solar radio bursts are driven by nonthermal electron beams travelling along heliospheric magnetic fields, with the radio emission frequency drift rate determined by the beam speed and the plasma densi... | [
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Unveiling the Hidden Radiation: The Persistent Emission of PSR B0823+26 in Its Quiescent State. In this study, we report on a detailed polarimetric single-pulse analysis of the radio emission from the pulsar B0823+26 (J0825+2637) during its quiescent state. Using the unprecedentedly high-sensitive observations carried ... | [
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Characterizing Density and Gravitational Potential Fluctuations of the Interstellar Medium. Substructure in the interstellar medium (ISM) is crucial for establishing the correlation between star formation and feedback and has the capacity to significantly perturb stellar orbits, thus playing a central role in galaxy dy... | [
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When Magnetic Field Lines Stretch, Snap, and Expand: A New Look at Solar Flares with L-maps. Understanding the three-dimensional evolution of coronal magnetic fields during solar flares remains challenging due to the lack of direct coronal field measurements. Here, we combine data-driven MHD simulations of NOAA AR 1115... | [
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Empirical Modeling of the Fast Solar Wind. In this work we derive empirical models of the fast solar wind by applying a Monte Carlo Markov Chain technique to in situ measurements of the wind charge state distributions to determine the wind's electron temperature, electron density, and bulk speed from the source region ... | [
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The SPHEREx Satellite Mission. Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer (SPHEREx), a NASA Explorer satellite launched on 2025 March 11, is carrying out the first all-sky near-infrared spectral survey. The satellite observes in 102 spectral bands from 0.75 to 5.0 μm wi... | [
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The Keck/DEIMOS Stellar Archive. I. Uniform Velocities and Metallicities for 78 Milky Way Dwarf Galaxies and Globular Clusters. We present a homogeneous spectroscopic dataset of 22,339 stars in 78 Milky Way dwarf galaxy satellites and globular clusters. All data were taken with the Keck II telescope and Deep Extragalac... | [
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Eccentricity Evolution of Warm Jupiters: The Role of Distant Perturbers and nearby Companions. Warm Jupiters (WJs)—giant exoplanets with orbital periods between 10 and 200 days—exhibit a broad range of eccentricities and are often accompanied by nearby low-mass planets. Understanding the origins of their orbital archit... | [
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Disentangling the Spectroscopic Signatures of Clumping and Corotating Interaction Regions in the Wolf─Rayet Star WR 6. Wolf─Rayet (WR) winds exhibit variability driven by small-scale clumping and large-scale corotating interaction regions (CIRs), but their interplay remains uncertain. Archival high-resolution ESPaDOnS ... | [
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2D Kelvin─Helmholtz Instability with Anisotropic Pressure. The Kelvin─Helmholtz (KH) instability occurs in multiple heliospheric (solar-wind stream interfaces, planetary magnetospheres, cometary tails, heliopause flanks) and interstellar (protoplanetary disks, relativistic jets, neutron star accretion disks) environmen... | [
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Older Ages for 23 Pre-main Sequence Stars in Upper Scorpius Using Dynamical-mass-constrained Stellar Evolutionary Models. We present revised stellar ages for 23 pre-main-sequence (PMS) K- and M-type stars in the Upper Scorpius (Upper Sco) star-forming region, derived using stellar dynamical masses to constrain isochron... | [
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White Dwarf Merger Remnants with Cooling Delays on the Q Branch Lack Strong Magnetism. A population of anomalous ultramassive white dwarfs discovered with Gaia, often referred to as the Q branch, show high (multi-Gyr) cooling delays produced by exotic physical mechanisms. They are believed to be the products of stellar... | [
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Investigation of Magnetic Topology and Triggering Mechanisms of a C-class Flare and Active Region Blowout Jet. Coronal jets are collimated plasma eruptions that are ubiquitous in the solar atmosphere. Believed to be triggered by magnetic reconnection, these jets can contribute to various phenomena, including coronal he... | [
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Elongation of a Solar Filament and its Three-dimensional Numerical Reconstruction for Magnetic Structures. Quiescent filaments are prominent features of the solar atmosphere, and their evolution reflects the coronal magnetic field's response to photospheric magnetic activity. Here, we report on a quiescent filament obs... | [
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Identifying Compact Chirping SMBHBs in LSST Using Bayesian Analysis. The Legacy Survey of Space and Time (LSST) is expected to observe up to ∼100 million quasars in the next decade. In this work, we show that it is possible to use such data to measure the characteristic frequency evolution of a "chirp" induced by gravi... | [
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Probing the Diversity of Type Ia Supernova Remnants in 3D Hydrodynamic Simulations with X-Ray Spectral Synthesis. Type Ia supernovae (SNe Ia), thermonuclear explosions of white dwarfs in binary systems, are widely used as standard candles owing to the empirical width─luminosity relation of their light curves. Recent th... | [
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New Insight from the James Webb Space Telescope on Variable Active Galactic Nuclei. Variability detected in galaxies is usually attributed to their active galactic nuclei (AGNs). While all AGNs are intrinsically variable, the AGN unification model predicts that Type 2 AGNs rarely vary because their engines are blocked ... | [
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Analytic Modeling of Tidally Locked Rocky Planet Atmospheres across Dynamical Regimes. We present a new first-principles analytic approach to interpreting eclipses and phase curves of rocky planets. Observations with JWST have reported nondetections of atmospheres around the majority of hot rocky planets orbiting M dwa... | [
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On the Active Sites of Mg-bearing Interstellar Dust Grains: An Experimental and Theoretical Model Study of CO<SUB>2</SUB> Activation. Magnesium silicates represent an important component of interstellar dust. While the formation of molecules in the interstellar region is typically thought to take place in icy mantles c... | [
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New Observations of an Extended Hall Interaction Region Downstream of Lunar Crustal Magnetic Fields. The lunar surface exhibits small-scale crustal magnetic fields that can give rise to various interactions when subjected to the incident solar wind plasma. These lunar crustal magnetic fields exhibit scale lengths that ... | [
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The NANOGrav 15 yr Dataset: Improved Timing Precision with Very Long Baseline Interferometry Astrometric Priors. Accurate pulsar astrometric estimates are essential to almost all high-precision pulsar timing experiments. Traditional pulsar timing techniques refine these estimates by including them as free parameters wh... | [
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Unification Model of Active Galactic Nuclei by Photoionization Equilibrium Calculation Based on Radiative Hydrodynamic Simulations. To investigate the origin of the dependence of the covering factor on the Eddington ratio suggested by X-ray observations, we examined the angular distribution of H I and H II based on two... | [
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The Shape-velocity Alignment of Satellites Forged by Tidal Locking and Dynamical Friction. Utilizing the TNG50 simulation, we study two types of alignments for satellites/subhalos: (1) the alignment of their major axes with the galactocentric radial directions (radial alignment), and (2) with the motion directions (orb... | [
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Eclipsed X-Ray Bursts from Magnetar SGR J1935+2154 and the Fireball Measurements. In theory, burst activity of the magnetar can lead to the formation of fireballs trapped by the magnetic field and corotating with the star. However, smoking-gun observational evidence of the fireball is elusive. We envisage that the fire... | [
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Galaxies Caught in Transition: The Role of Group Environment in Shaping the Mass─Size Relation in the Local Universe. The stellar mass─size relation is a sensitive probe of how environment shapes galaxy structure. We analyse this relation in the local Universe for galaxies in compact groups (CGs), low-mass groups (Mvir... | [
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Tilt Angles of Sunspot Groups in Different Latitude Bands and the Amplitude of the Next Solar Cycle. In the Babcock─Leighton and Parker dynamo models, the tilt angle of a sunspot group (SG) and the turbulence in the solar convection zone (one widely accepted generation mechanism responsible for the scatter of the tilt ... | [
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The Progenitor of the S147 Supernova Remnant. The supernova remnant (SNR) S147 contains the pulsar PSR J0538+2817 and a likely unbound binary companion, HD 37424. It is the only good Galactic candidate for a binary unbound by a core-collapse supernova. Using Gaia DR3 parallaxes and photometry, we select the stars local... | [
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Improving the Shock Propagation Model of SPM3 by Incorporating the Solar Energetic Particle Flux and the Principal Component Analysis Method. Coronal mass ejections (CMEs), as one of the most destructive solar activity phenomena, are the primary driver of extreme space weather events. Accurately predicting the probabil... | [
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Early Results from the Coma Legacy IFU Survey (CLIFS): Ram Pressure Induced Shocks and Ionization in Jellyfish Tails. Jellyfish galaxies, which exhibit tails of gas opposite to their direction of motion, are a galaxy population showcasing the most extreme effects of ram pressure stripping (RPS). We present the emission... | [
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Statistical Patterns in the Time Evolution of Interface Region Imaging Spectrograph Bright Points. Interface Region Imaging Spectrograph bright points (IBPs) are ubiquitous, small-scale energetic events with a multithermal nature, typically observed in the chromosphere or transition region and closely linked to photosp... | [
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Spectroscopy and Photochemistry of the Astrochemical Molecules SiCP and AlCP. Through characterization of the electronic excited-state topology, linear-SiCP is predicted to be photostable in the UV region, whereas linear-AlCP is predicted to undergo photodissociation to form Al+CP products after absorption of light in ... | [
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Searching for White Dwarf Candidates Formed Through Binary Evolution in Star Clusters. White dwarfs (WDs), the evolutionary endpoints of most stars, can form through both single-star and binary channels. While single-star evolutionary models enable reliable WD age estimates, binary evolution introduces interactions tha... | [
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Search for Ultra-high-energy Neutrons from Galactic Sources with the Pierre Auger Observatory. Deflections in the propagation of charged ultra-high-energy cosmic rays (UHECRs) caused by magnetic fields make the identification of their sources challenging. On the other hand, the arrival directions at Earth of neutrons p... | [
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Transverse Oscillations and Wave Propagation in the Magnetically Dominated M87 Jet. We present an in-depth analysis of the transverse oscillations in the M87 jet, as identified in our previous study, which reported oscillatory patterns with a characteristic period of ∼1 yr in the edge-brightened jet structure extending... | [
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Modeling the Time-variable Broadband Emission and Correlation Study of FSRQ S5 1044+71. We present a detailed temporal and spectral analysis of the blazar S5 1044+71 using multiwavelength data obtained from the Fermi-LAT and Swift-XRT/UVOT telescopes. Applying the Bayesian block algorithm to the 3-day binned γ-ray ligh... | [
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Deep-learning-based Identification of Solar Magnetic Tornadoes and Their Spatial Properties during Solar Minimum and Maximum. Solar magnetic tornadoes are dynamic, spiral-shaped plasma structures characterized by helical magnetic fields and rotating plasma flows in the solar atmosphere. They play a significant role in ... | [
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Numerical Exploration of a B-Class Flare Using the Synergy between XSM, GOES, AIA, and HMI. Solar flares are sudden, explosive events on the Sun in which magnetic energy, ranging from 1023 to 1032 erg, is released in the form of heat and acceleration of charged particles, along with a rearrangement of magnetic field li... | [
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In-depth Analysis of Bar Formation Mechanisms of Disk Galaxies in Halos of Different Concentrations. We use N-body simulations to investigate the distinct bar formation processes in disks residing in halos of various concentrations. In a highly concentrated halo, the bar development is limited by the dominant multiarm ... | [
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Encounters between M33 and Present-day M31 Satellites Hint at a Previous Group Accretion. This work investigates whether two known Andromeda (M31) satellites, Pisces (LGS 3) and Andromeda XVI (And XVI), have interacted with M33, M31's most massive satellite. ΛCDM predictions imply a handful of satellite galaxies around... | [
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Glimmers in the Cosmic Dawn. III. On the Photometrically Determined Black Hole Mass to Stellar Mass Relation across Cosmic Time. We present the results from performing spectral energy distribution (SED) fitting on 121 variable active galactic nuclei (AGN) candidates in the Hubble Ultra Deep Field using photometry from ... | [
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SN 2021aaev: A Hydrogen-rich Superluminous Supernova with Early Flash and Long-lived Circumstellar Interaction in an Unusual Host Environment. We present photometric and spectroscopic observations of SN 2021aaev, a hydrogen-rich, superluminous supernova with persistent (at least ∼100 days) narrow Balmer lines (SLSN-IIn... | [
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Lyα Intensity Mapping in HETDEX: Galaxy-Lyα Intensity Cross-power Spectrum. We present a measurement of the Lyα intensity mapping power spectrum from the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX). We measure the cross-power spectrum of the Lyα intensity and Lyα-emitting galaxies (LAEs) in a redshift range ... | [
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The Effects of Non-ideal Mixing in Planetary Magma Oceans and Atmospheres. Sub-Neptunes with hydrogen-rich envelopes are expected to sustain long-lived magma oceans that continuously exchange volatiles with their overlying atmospheres. Capturing these interactions is key to understanding the chemical evolution and pres... | [
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Dynamics of the Coronal Magnetic Field in the 2022 October 2 X-class Flare. Solar flares are driven by the release of free magnetic energy and are often associated with the restructurization of the magnetic field topology. Yet, observations of the evolving magnetic field in the flaring volume are limited to very few ca... | [
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ATOMS-QUARKS Survey: Inflow and Infall in Massive Protocluster G318.049+00.086— Evidence of Competitive Accretion. We present a gas kinematic study of the massive protocluster G318.049+00.086. The protocluster is reported to contain 12 prestellar core candidates and four protostellar cores. Filamentary structures are i... | [
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TTC: Transformer-based TDE Classifier for the Wide Field Survey Telescope (WFST). We propose the Transformer-based Tidal disruption events (TDE) Classifier (TTC), specifically designed to operate effectively with both real-time alert streams and archival data of the Wide Field Survey Telescope (WFST). It aims to minimi... | [
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First Detection of γ-Ray Emission from the Compact Symmetric Object JVAS J1311+1658. We report the first detection of γ-ray emission from the young radio galaxy JVAS J1311+1658, classified as a compact symmetric object (CSO). This detection is characterized by a recent GeV γ-ray flare identified in Fermi-Large Area Tel... | [
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A Black Hole Envelope Interpretation for Cosmological Demographics of Little Red Dots. Little Red Dots (LRDs) newly discovered with JWST are active galactic nuclei (AGNs) that may represent black hole (BH) growth at the earliest cosmic epochs. These sources show puzzling features unlike typical AGNs, including red opti... | [
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The Effect of Planetary Rotation Period on Clouds in a Global Climate Model with a Bin Microphysics Scheme. Clouds are the largest source of uncertainty in climate simulations. For exoplanets, cloud simulation is particularly challenging because of the lack of observational data to tune parameterized cloud models. Here... | [
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ALMA [C I] Image of the Circumnuclear Disk of the Milky Way: Inflowing Low-density Molecular Gas. We present Atacama Large Millimeter/submillimeter Array [C I] 3P1─3P0 imaging of the central 6.6 × 4.2 pc2 region of the Galaxy encompassing the circumnuclear disk (CND). The data reveal low-density ( nH2∼103 cm−3) molecul... | [
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TransFit-CSM: A Fast, Physically Consistent Framework for Interaction-powered Transients. We introduce TransFit-CSM, a fast and physically consistent framework for modeling interaction-powered transients. The method self-consistently couples the ejecta─circumstellar medium (CSM) shock dynamics to radiative diffusion fr... | [
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Constraining the Effects of Pre- and Post-accretionary Processes on Ryugu Insoluble Organic Matter. Asteroidal and cometary fragments have been indicated as possible sources of the building blocks of life for the early Earth. Samples returned from the asteroid Ryugu are uncontaminated and contain organic matter. Such s... | [
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The Radius Cliff is a Waterfall: Explaining Sub-Neptune Exoplanets with Steam Worlds. The demographics of Kepler planets provide a key testbed for models of planet formation and evolution, particularly for explaining the radius valley separating super-Earths and sub-Neptunes. A primordial interpretation based on differ... | [
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FEAST: Probing Hierarchical Star Formation with the Spatial Distributions of Young Star Clusters. We apply the angular two-point correlation function (TPCF) to the spatial distributions of young star clusters (YSCs) in four nearby star forming galaxies (NGC 628, NGC 4449, M51, and M83) in order to investigate their und... | [
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Beyond Two Parameters: Revisiting Dark Energy with the Latest Cosmic Probes. Dark energy (DE) models with many free parameters are often considered excessive, as constraining all parameters poses a significant challenge. While such models offer greater flexibility to probe the DE sector in more detail. With the rapid a... | [
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"http://astrothesaurus.org/uat/138",
"http://astrothesaurus.org/uat/322",
"http://astrothesaurus.org/uat/415",
"http://astrothesaurus.org/uat/1545",
"http://astrothesaurus.org/uat/1671",
"http://astrothesaurus.org/uat/1728"
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"Baryon acoustic oscillations",
"Cosmic microwave background radiation",
"Dwarf elliptical galaxies",
"Space probes",
"Surveys",
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Resonant Absorption and Fluctuations via Hybrid Simulations on Coronal Loops. II. Kinetic Description. The kinetic characteristics of resonant absorption of combined left- and right-hand polarized waves with finite amplitude are investigated. The plasma consists of a magnetized 2D slab with linearly inhomogeneous densi... | [
"http://astrothesaurus.org/uat/1477",
"http://astrothesaurus.org/uat/1476",
"http://astrothesaurus.org/uat/23",
"http://astrothesaurus.org/uat/2089"
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"http://astrothesaurus.org/uat/994",
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Radiative Transfer Modeling of Stripped-envelope Supernovae. I. A Grid for Ejecta Parameter Inference. We present 1800 multiwavelength Type Ib/c supernovae light-curve models obtained by running the radiation transport code Sedona and varying the mass distribution, velocity profile, and abundance ejecta profiles of hel... | [
"http://astrothesaurus.org/uat/1730",
"http://astrothesaurus.org/uat/1933",
"http://astrothesaurus.org/uat/1729",
"http://astrothesaurus.org/uat/918",
"http://astrothesaurus.org/uat/1967"
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"Neural networks",
"Type Ib supernovae",
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"http://astrothesaurus.org/uat/453",
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"http://astrothesaurus.org/uat/1335",
"http://astrothesaurus.org/uat/1599",
"http://astrothesaurus.org/uat/1634",
"http://astrothesaurus.org/uat/1668"
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"Ejecta",
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"Radiative transfer",
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Digging into the Chemical Complexity in the Outer Galaxy: A Hot Molecular Core in Sh 2-283. The outer Galaxy (Galactocentric distance ≳13.5 kpc) serves as an excellent laboratory for investigating the chemical complexity in low-metallicity environments. Here we present the chemical analyses for the outer Galactic hot c... | [
"http://astrothesaurus.org/uat/849",
"http://astrothesaurus.org/uat/1338",
"http://astrothesaurus.org/uat/844",
"http://astrothesaurus.org/uat/224",
"http://astrothesaurus.org/uat/75",
"http://astrothesaurus.org/uat/412",
"http://astrothesaurus.org/uat/1031",
"http://astrothesaurus.org/uat/2256"
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"Interstellar molecules",
"Radio astronomy",
"Interstellar line emission",
"Chemical abundances",
"Astrochemistry",
"Dust continuum emission",
"Metallicity",
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The Role of Gyrating Ions in Reformation of a Quasi-parallel Supercritical Shock. Collisionless shocks in space and astrophysical plasmas mediate energy exchange between charged particles and fields in two or more plasma flows. In this study we analyze the evolution of ion distributions around a reformation cycle of a ... | [
"http://astrothesaurus.org/uat/2086"
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"http://astrothesaurus.org/uat/994",
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