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On the Thermal and Magnetic Properties of an Active Region Jet. Jets, as an essential manifestation of the release of the free magnetic energy, are ubiquitous in the solar atmosphere. We present a comprehensive analysis of a multithermal blowout jet that occurred in active region AR 13102 on 2022 September 20, using ob... | [
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Cool-core Destruction in Merging Clusters with Active Galactic Nucleus Feedback and Radiative Cooling. The origin of the cool-core (CC) and non-cool-core (NCC) dichotomy of galaxy clusters remains uncertain. Previous simulations have found that cluster mergers are effective in destroying CCs but fail to prevent overcoo... | [
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The DESI Single Fiber Lens Search. I. Four Thousand Spectroscopically Selected Galaxy─Galaxy Gravitational Lens Candidates. We present 4110 strong gravitational lens candidates, 3887 of which are new discoveries, selected from a sample of 5,837,154 luminous red galaxies (LRGs) observed with the Dark Energy Spectroscopi... | [
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Insights into the Physical Nature of Polar-ring Galaxies from H I Observations. Polar-ring galaxies (PRGs) host an outer ring of gas and stars oriented nearly perpendicular to the main stellar body. They represent extreme examples of misaligned systems and provide valuable insights into galaxy interactions, gas accreti... | [
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COSMOS-Web: Comprehensive Data Reduction for Wide-area JWST NIRCam Imaging. We present the data reduction methodology used for the COSMOS-Web survey JWST NIRCam data. Covering 0.54 deg2 with four broadband filters (F115W, F150W, F277W, F444W) and a total exposure time of approximately 270 hr, COSMOS-Web represents the ... | [
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Small-scale Bright Point Characteristics at High-resolution with the Daniel K. Inouye Solar Telescope. Bright points (BPs) are small-scale, dynamic features that are ubiquitous across the solar disc and are often associated with the underlying magnetic field. Using broadband photospheric images obtained with the Visibl... | [
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Quantifying the Impact of Selection Effects on FRB DM─z Relation Cosmological Inference. Fast radio bursts (FRBs) have emerged as powerful probes of baryonic matter in the Universe, offering constraints on cosmological and feedback parameters through their extragalactic dispersion measure─redshift (DMexgal─z) relation.... | [
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Origin of the Lunar Inclination from Tidal Interaction of Multiple-Moon System. According to the giant impact theory, the Moon formed through accreting the debris disk produced by a collision between Theia and the proto-Earth, and the predicted lunar orbital inclination relative to the Earth's equatorial plane is about... | [
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First-principles Polar-cap Currents in Multipolar Pulsar Magnetospheres. X-ray pulse-profile modeling of millisecond pulsars offers a direct route to measuring neutron star masses and radii, thereby constraining the dense-matter equation of state. However, standard analyses typically rely on ad hoc hotspot parameteriza... | [
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XRISM Observation of the Supernova Remnant N103B: Velocity Structure and Thermal Properties. We present the first analysis of the X-ray Imaging and Spectroscopy Mission (XRISM) observation of the supernova remnant (SNR) N103B. We fit the X-ray spectrum taken with the Resolve microcalorimeter, which captured emission li... | [
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Comparative Analysis of Properties of Coronal Mass Ejections at High and Low Apparent Latitudes in 1996─2025. This study examines the statistical properties of coronal mass ejections (CMEs) over two and a half solar cycles (1996─2025) using coronal observations from the SOHO LASCO CDAW and CACTus catalogs, supplemented... | [
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Testing Magnetic Field Configurations in Spider Pulsar PSR J1723−2837 with IXPE. We present the first X-ray polarimetry observations of a redback millisecond pulsar binary, PSR J1723−2837, with the Imaging X-ray Polarimetry Explorer (IXPE). We conduct a spectropolarimetric analysis combining IXPE data with archival Cha... | [
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Proton Trapping in Ganymede's Magnetosphere: A Quantitative Test Particle Study. Ganymede, the largest moon in the solar system, possesses an intrinsic dipole magnetic field, creating a mini-magnetosphere within Jupiter's giant magnetosphere. Energetic protons from the upstream Jovian plasma can become temporarily conf... | [
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The 2024 July 23 Event: A Case Study of a Multispacecraft, Fe-rich Solar Energetic Particle Event. Occasionally, solar energetic particle (SEP) events associated with fast, wide coronal mass ejections (CMEs) driving interplanetary shocks exhibit Fe/O abundance ratios that are significantly higher than the nominal value... | [
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Exo─IPM Scattering as a Hidden Gatekeeper of Narrowband Technosignatures. Narrowband radio technosignatures can be significantly modulated by the host star's exoplanetary interplanetary medium (Exo-IPM), where turbulence in stellar winds and coronal mass ejections (CMEs) imprint spectral broadening. We present a novel ... | [
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Cosmological Prediction from the Joint Observation of MeerKAT and CSST at z = 0.4 ─ 1.2. Cross-correlating neutral hydrogen (H I) 21 cm intensity mapping with galaxy surveys provides an effective probe of astrophysical and cosmological information. This work presents a cross-correlation analysis between MeerKAT single-... | [
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Self-consistent Emission-line Diagnostics with Integrated Extinction Correction. We present a closed-form, self-consistent spectroscopic framework in which extinction correction is treated as an integral part of the inference rather than as a separate preprocessing step. From emission-line measurements alone, the metho... | [
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Ruling out Conventional Photoionization Models in the Closest LINER, M31, with CFHT/SITELLE Observations. The ionization mechanisms of low-ionization nuclear emission-line regions (LINERs), which are common in the local Universe, have been debated for decades. Our nearest large neighbor, M31, is classified as a LINER b... | [
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Helium Escape in Context: Comparative Signatures of Four Close-in Exoplanets. Observations of escaping atmospheres on close-in exoplanets show a wide range in the strength and morphology of He I 10830 Å and H I absorption. Scaling relations attempt to link the He I signal to X-ray and UV irradiation, mass loss, and bul... | [
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Determining the Spatial Origin of X-Ray and Optical Emission in the z = 3.1 Strongly Lensed Radio-quiet Quasar GraL J065904.1+162909 to Hundreds of Parsecs. We perform milliarcsecond X-ray astrometry of the quadruply lensed radio-quiet quasar GraL J065904.1+162909 (J0659). This zs = 3.083 quasar is lensed into four ima... | [
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From Common Envelope Evolution to Luminous Red Novae. I. A One-dimensional Radiation Hydrodynamic Model. The acceleration and unbinding of the common envelope during the plunge-in phase are governed by complex physical processes that often manifest observationally as luminous red novae. We investigate the dynamics of t... | [
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Orbital Motions of Binaries in Orion South. We present high-angular resolution ( ≃0.″06 ) Very Large Array and Atacama Large Millimeter/submillimeter Array observations of Orion South separated by 15.52 yr. The purpose of this study was to search for orbital motions in three close ( ≃0.″1 ) binary systems in the region... | [
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Inside-out Planet Formation. VIII. Onset of Planet Formation and the Transition Disk Phase. Inside-out planet formation (IOPF) is a theory of in situ formation via pebble accretion of close-in Earth to super-Earth mass planets at the pressure maximum associated with the dead zone inner boundary (DZIB), whose location i... | [
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Improving Precision in Kinematic Weak Lensing with MIRoRS: Model-independent Restoration of Reflection Symmetries. We present a novel, model-independent technique for fitting the cross-component of weak lensing shear, γ×, along a line of sight by combining kinematic and photometric measurements of a single lensed galax... | [
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Refinements to the Solar Polar Magnetic Flux: Implications from Inversion Methodologies. The magnetic fields in the solar polar region are important to our understanding of the internal dynamo process, the global coronal structure, and the origin of the solar wind. The inference of polar fields based on spectropolarime... | [
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Coevolution of Nuclear Star Clusters and Massive Black Holes: Extreme-mass-ratio Inspirals. We explore extreme-mass-ratio inspirals (EMRIs) in the coevolution of massive black holes (MBHs) and nuclear star clusters (NSCs), which host diverse stellar populations across a wide range of masses. The dynamics are simulated ... | [
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Solar Wind Heating near the Sun: A Radial Evolution Approach. Characterizing the plasma state in the near-Sun environment is essential to constrain the mechanisms that heat and accelerate the solar wind. In this study, we use Parker Solar Probe observations from Encounters 1 through 24 to investigate the radial evoluti... | [
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Graph-based Summary Statistics for Revealing the Stochastic Gravitational-wave Background in Pulsar Timing Arrays. In this work, we propose a graph-based method implemented on the pulsar timing residuals for stochastic gravitational-wave background (SGWB) detection within the nanohertz frequency regime and examining un... | [
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An Accretion-Modulated Internal Shock Model for Long GRBs. We introduce the accretion-modulated internal shock model as a possible framework for explaining the observational properties of long gamma-ray burst (GRB) prompt emission. In this scenario, the envelope of the prompt light curve follows the time-dependent mass... | [
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Diverse Origins of Broad Hα Lines in Heavily Obscured Active Galactic Nuclei Revealed by Multiepoch Spectroscopy. According to the classical active galactic nucleus (AGN) model, broad emission lines originate from the broad-line region (BLR) and are observable only when the attenuation by the dusty torus is small. Howe... | [
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"http://astrothesaurus.org/uat/16",
"http://astrothesaurus.org/uat/2109"
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"Supermassive black holes",
"Seyfert galaxies",
"Active galactic nuclei",
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"http://astrothesaurus.org/uat/1914",
"http://astrothesaurus.org/uat/2291"
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"Line of sight",
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Magnetic Flux Tubes Illuminated by Pulsar Winds. Observations of linear structure connecting pulsars to gamma-ray halos reveal injection of TeV electrons into the interstellar medium (ISM). In some cases, this could be attributed to nearly scattering-free electron transport along large-scale magnetic fields connected t... | [
"http://astrothesaurus.org/uat/1306",
"http://astrothesaurus.org/uat/847",
"http://astrothesaurus.org/uat/2215",
"http://astrothesaurus.org/uat/1346",
"http://astrothesaurus.org/uat/637"
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"Interstellar medium",
"Pulsar wind nebulae",
"Radio interferometry",
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"http://astrothesaurus.org/uat/994",
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Five-minute Periodicities in the Population of Solar Coronal Brightenings. The population of small-scale brightenings observed across broad regions of the quiet-Sun (QS) corona shows coherent strong periodicities of ≍5 minutes and amplitudes of 20% to 30% of the mean. The periodicity is in the total number of detected ... | [
"http://astrothesaurus.org/uat/1515",
"http://astrothesaurus.org/uat/1476",
"http://astrothesaurus.org/uat/1989",
"http://astrothesaurus.org/uat/312"
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Type Iax Supernovae as a Source of Iron-rich Silicate Dust. We model the formation of dust in the ejecta of Type Iax supernovae (SNe), which is a low-luminosity subclass of Type Ia SNe. A nonequilibrium chemical kinetic approach is adopted to trace the synthesis of molecules, molecular clusters, and dust grains in the ... | [
"http://astrothesaurus.org/uat/236",
"http://astrothesaurus.org/uat/75",
"http://astrothesaurus.org/uat/1728",
"http://astrothesaurus.org/uat/2269"
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"Astrochemistry",
"Type Ia supernovae",
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"http://astrothesaurus.org/uat/1012",
"http://astrothesaurus.org/uat/1668",
"http://astrothesaurus.org/uat/2233"
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Patterns of X-Ray and γ-Ray Flares: From Blazar to Magnetar and Sun. Using Gaussian process methods, we analyzed the light curves of three extreme solar X-ray flares observed by the RHESSI satellite. Their variability characteristics were then compared with those of HXMT-HE X-ray burst (XRB; in SGR 1935+2154) associate... | [
"http://astrothesaurus.org/uat/187",
"http://astrothesaurus.org/uat/1930",
"http://astrothesaurus.org/uat/1916",
"http://astrothesaurus.org/uat/1816"
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"http://astrothesaurus.org/uat/164",
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"http://astrothesaurus.org/uat/992",
"http://astrothesaurus.org/uat/1043",
"http://astrothesaurus.org/uat/1496",
"http://astrothesaurus.org/uat/1814",
"http://astrothesaurus.org/uat/2008"
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"Light curves",
"Magnetars",
"Astronomical methods",
"Solar flares",
"X-ray bursts",
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An Active Galaxy Cluster Merger at Cosmic Noon Revealed by JWST Weak Lensing and Multiwavelength Probes. The galaxy cluster XLSSC 122 is a rare system at z = 1.98, hosting surprisingly evolved member galaxies when the Universe was only one-third of its present age. Leveraging deep JWST/NIRCam imaging, we perform a weak... | [
"http://astrothesaurus.org/uat/1797",
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"http://astrothesaurus.org/uat/2291",
"http://astrothesaurus.org/uat/858",
"http://astrothesaurus.org/uat/353"
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"Weak gravitational lensing",
"High-redshift galaxy clusters",
"James Webb Space Telescope",
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"http://astrothesaurus.org/uat/1054",
"http://astrothesaurus.org/uat/1545",
"http://astrothesaurus.org/uat/1689"
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"Cosmology",
"Galaxies",
"Galaxy clusters",
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Unraveling the Emission Mechanism Powering Long Period Radio Transients from Interacting White Dwarf Binaries via Kinetic Plasma Simulations. Recent observations of long period radio transients, such as GLEAM-X J0704─37 and ILT J1101+5521, have revealed a previously unrecognized population of Galactic radio transient s... | [
"http://astrothesaurus.org/uat/982",
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"http://astrothesaurus.org/uat/739",
"http://astrothesaurus.org/uat/571",
"http://astrothesaurus.org/uat/1799",
"http://astrothesaurus.org/uat/801",
"http://astrothesaurus.org/uat/2008"
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"Magnetospheric radio emissions",
"High energy astrophysics",
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Discovery of Multiple Ultra-broad-velocity Molecular Features Associated with the W44 Molecular Cloud. We report the discovery of multiple compact molecular features exhibiting extremely broad velocity widths toward the W44 molecular cloud. Atacama Large Millimeter/submillimeter Array CO J = 3─2 data reveal eight "Peti... | [
"http://astrothesaurus.org/uat/849",
"http://astrothesaurus.org/uat/1667",
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Evidence of 5 minute Oscillations from Parker Solar Probe. The Sun's surface vibrates in characteristic 5 minute oscillations, known as p-modes, generated by sound waves trapped within the convection zone. Although these oscillations have long been hypothesized to reach into the solar wind, direct in situ evidence has ... | [
"http://astrothesaurus.org/uat/1872",
"http://astrothesaurus.org/uat/709",
"http://astrothesaurus.org/uat/830",
"http://astrothesaurus.org/uat/1534",
"http://astrothesaurus.org/uat/1483",
"http://astrothesaurus.org/uat/1484"
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"Helioseismology",
"Interplanetary turbulence",
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"http://astrothesaurus.org/uat/255",
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"http://astrothesaurus.org/uat/1515",
"http://astrothesaurus.org/uat/1545",
"http://astrothesaurus.org/uat/1693"
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Revealing the Unseen: The Discovery of Long-awaited Radiation from the Intermittent Pulsar PSR B1931+24. Pulsars are typically characterized by their stable, highly magnetized, and fast-rotating nature, which underpins their persistent radio emissions. However, the discovery of prolonged radio-quiet ("off") states in i... | [
"http://astrothesaurus.org/uat/1108",
"http://astrothesaurus.org/uat/1353"
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A Morphology Catalog of Galaxies in CEERS: Evolution in the Size and Color Gradients of Galaxies Since Cosmic Dawn. We present measurements of morphological parameters from fitting 53,885 galaxies detected to a magnitude limit of F356W < 28.5 in the CEERS NIRCam imaging with GALFIT in six broadband filters: F115W, F... | [
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JWST Observations of Starbursts: Polycyclic Aromatic Hydrocarbons Closely Trace the Cool Phase of M82's Galactic Wind. Stellar feedback drives multiphase gas outflows from starburst galaxies, but the interpretation of dust emission in these winds remains uncertain. To investigate this, we analyze new JWST mid-infrared ... | [
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No Observational Evidence for Dark Matter Nor a Large Metallicity Spread in the Extreme Milky Way Satellite Ursa Major III/UNIONS 1. The extremely low-luminosity, compact Milky Way satellite Ursa Major III/UNIONS 1 (UMaIII/U1; LV = 11 L⊙, a1/2 = 3 pc) was found to have a substantial velocity dispersion at the time of i... | [
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The Astrometric Resoeccentric Degeneracy: Eccentric Single Planets Mimic 2:1 Resonant Planet Pairs in Astrometry. Detections of long-period giant exoplanets will expand dramatically with Gaia Data Release 4, but interpreting these signals will require care. We derive the astrometric resoeccentric degeneracy: an astrome... | [
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Probing Binary Black Hole Formation Channels through Cosmic Large-scale Structure. The growing number of binary black hole mergers detected through gravitational waves offers unprecedented insight into their underlying population, yet their astrophysical formation channels remain unresolved. We present a new method to ... | [
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Probing Heavily Obscured Active Galactic Nuclei in Major Galaxy Mergers Using the Millimeter─X-Ray Correlation. The study of heavily obscured supermassive black hole (SMBH) growth in late-stage galaxy mergers is challenging: column densities NH > 1024 cm−2 can block most nuclear emission, leaving significant gaps in... | [
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Preperihelion Volatile Evolution of Interstellar Comet 3I/ATLAS Indicating Significant Contribution from an Extended Source in the Coma. Interstellar comets provide rare opportunities for probing the diversity of refractory and volatile inventory around other stars. As the second ever interstellar comet and the third i... | [
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The Cosmic-Ray Knee as a Local Signature of Nearby PeVatrons. A "knee" in the cosmic-ray spectrum, characterized by a sudden steepening of the spectral shape at ∼4 PeV, may be interpreted either as a global feature of Galactic cosmic rays or as a local signature. In the former scenario, cosmic-ray spectra throughout th... | [
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Upper Limit on HF(1─0) Absorption in a Dusty Star-forming Galaxy at z = 6: Constraints on Early Fluorine Enrichment. Wolf─Rayet (WR) stars have recently attracted attention as possible drivers of early chemical enrichment, including the production of fluorine, whose nucleosynthetic origin remains debated. To test the c... | [
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Superluminal Wave Activation at Relativistic Magnetized Shocks. Fast radio bursts (FRBs) are extremely energetic radio transients, where some are generated in magnetar magnetospheres and winds. Despite a growing number of observations, their emission mechanisms remain elusive. It has recently been proposed that Alfvéni... | [
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<SUP>56</SUP>Ni Production in Long-lived Binary Neutron Star Merger Remnants. We investigate the nucleosynthesis and kilonova emission based on numerical-relativity binary neutron star merger simulations that incorporate a two-moment neutrino-transport scheme. Unlike in previous works with simpler neutrino treatments, ... | [
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Discovery of a Gas-enshrouded Broad-line Active Galactic Nucleus at z ∼ 7. The Lyα absorption profile in star-forming galaxies serves as a powerful tracer of the extended, dense neutral hydrogen in their surroundings during the Epoch of Reionization (EoR). We report a unique galaxy, A2744-z7DLA, at z ≍ 6.87, gravitatio... | [
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New Approach to Superflare Energy Determination. We present a new method for estimating the total energy radiated by stellar flares in broadband continua, which assumes a constant emitting area but incorporates a time-dependent temperature evolution. This physically motivated approach offers an alternative to the commo... | [
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Cold Gas Infall onto a Brightest Group Galaxy via a Gas-rich Minor Merger. Dust and cold gas are not uncommon in nearby early-type galaxies (ETGs) and represent an important aspect of their evolution. However, their origin has been debated for decades. Potential sources include internal processes (e.g., mass loss from ... | [
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Bar-driven Shocks in NGC 1365 Revealed by the Most Luminous Extragalactic Class I Methanol Maser. We report the first detection of the 36.2 GHz (4−1 → 30 E) Class I methanol (CH3OH) maser in the central region of the barred spiral galaxy NGC 1365. This detection using the Australia Telescope Compact Array establishes N... | [
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Observations of Transition from Imbalanced to Balanced Kinetic Alfvénic Turbulence. We report observations of solar wind turbulence derived from measurements by the Parker Solar Probe. Our findings reveal the emergence of finite magnetic helicity within the transition range of the turbulence, aligning with signatures o... | [
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A Protoplanet Candidate in the PDS 66 Disk Indicated by Silicon Sulfide Isotopologues. Despite observational progress in planet formation, the stage in which planetesimals grow into planets remains poorly understood. During this phase, protoplanets may develop gaseous envelopes that are warmer than the surrounding disk... | [
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Nonlinear Mode Conversion from a Large-amplitude Propagating Kink Wave to Longitudinal Oscillations in a Quiescent Prominence. In this Letter, we present the direct observations of a mode conversion from a large-amplitude transverse propagating kink wave to antiphase large-amplitude longitudinal oscillations (LALOs) in... | [
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Emergence of a Lithium Dip in ∼35 Myr "Snake" Open Clusters. We report the discovery of a lithium dip (Li dip) in the stellar "Snake" (age = 35 ± 5 Myr), challenging the classical view that Li dips emerge only at ages ≳150 Myr. Using high-resolution spectra from GALAH Data Release 4 (R ∼ 28,000) for 211 member stars, w... | [
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Fading into Darkness: A Weak Mass Ejection and Low-efficiency Fallback Accompanying Black Hole Formation in M31-2014-DS1. Stellar-mass black holes (BHs) can form from the near-complete collapse of massive stars, causing them to abruptly disappear. The star M31-2014-DS1 in the Andromeda galaxy was reported to exhibit su... | [
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Evidence for a Peak at ∼0.3 in the Eccentricity Distribution of Typical Super-Jovian Exoplanets. In this study, we compute completeness-corrected occurrence rates of giant exoplanets as a function of mass, semimajor axis, and eccentricity, using the approximately uniform California Legacy Survey sample of radial veloci... | [
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Shock-like Magnetic Enhancements Generated by Kelvin─Helmholtz Instability above Weakly Magnetized Bodies. Shock-like magnetic field structures above weakly magnetized bodies such as the Moon have been reported for more than half a century and represent a key long-standing feature of their solar-wind interactions. Yet ... | [
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The Energy─Duration Relationship in Astrophysical Self-organized Criticality Systems. Scaling laws in astrophysical systems that involve energy, geometry, and spatiotemporal evolution provide the theoretical framework for physical models of energy dissipation processes. A leading model is the standard fractal-diffusive... | [
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The Maximum Offsets of Binary Neutron Star Mergers from Host Galaxies. We analytically derive, and illustrate with a population synthesis model, the maximum offset of binary neutron star mergers ejected from their host galaxies. This approximate maximum offset is 300 kpc ×(vesc/500kms−1)−7 , where vesc is the escape v... | [
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The Maximum Mass Ratio of Hierarchical Binary Black Hole Mergers May Cause the q─χ<SUB>eff</SUB> Correlation. Regardless of their initial spins, the merger of two roughly equal mass black holes (BHs) produces a remnant BH of dimensionless spin 0.69. Such remnants can merge with other BHs in dense stellar environments a... | [
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Indications of Rapid Dust Formation in the Inner Region of a Protoplanetary Disk. We report a significant increase in mid-infrared emission ≤10 μm in a transitional disk. The 2024 JWST/MIRI observation of the disk around CVSO 1942 reveals flux increase by a factor of 2 at λ ≤10 μm, compared to the near-photospheric flu... | [
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An Excited Dark Matter Solution to the MeV Galactic Center Excesses. Recent reanalyses of COMPTEL data reveal a ∼2 MeV continuum excess whose spatial distribution closely matches the 511 keV line observed by INTEGRAL/SPI (SPectrometer on INTEGRAL), pointing to a common population of low-energy Galactic positrons that i... | [
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IRS 9: The Case for a Dynamically Ejected Star from the Galactic Center. Measuring stellar motions at the Milky Way's Galactic center (GC) provides unique insight into the dynamical processes within galactic nuclei. We present proper-motion measurements for 23 SiO-maser-emitting stars within 45″ of SgrA*, including fou... | [
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Evidence for the Merger Hypothesis in V4332 Sgr: A Low <SUP>12</SUP>C/<SUP>13</SUP>C Ratio and Multiple Outbursts. Following the detections of the first extragalactic "luminous red nova" (LRN) M31RV in 1989, and its first Galactic counterpart V4332 Sgr in 1994, there have been many discoveries of similar, or closely re... | [
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The Origin of Energetic Solar Protons: Comparative Analysis of Ground-level Enhancement (GLE) Events and Non-GLE Solar Energetic Particle Events. This study explores the acceleration origins of solar energetic particles (SEPs) by analyzing the energy spectral characteristics of particles in ground-level enhancement (GL... | [
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FIELDMAPS Data Release: Far-infrared Polarization in the "Bones" of the Milky Way. Polarization observations of the Milky Way and many other spiral galaxies have found a close correspondence between the orientation of spiral arms and magnetic field lines on scales of hundreds of parsecs. This paper presents polarizatio... | [
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CANUCS/Technicolor Data Release 1: Imaging, Photometry, Slit Spectroscopy, and Stellar Population Parameters. We present the first data release of the Canadian NIRISS Unbiased Cluster Survey (CANUCS), a JWST Cycle 1 GTO program targeting five lensing clusters and flanking fields in parallel (A370, MACS0416, MACS0417, M... | [
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Multiscale Magnetic Reconnection in the Genesis of Young Slow Solar Wind. The genesis of solar wind remains elusive due to limited multi-instrument observations of its source regions. Here, we introduce a novel "see and touch" technique, integrating remote-sensing observations with in situ measurements from Parker Sola... | [
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Measurements of Cosmic Proton Flux through Neutron Monitors Using Deep Networks and Imputation Techniques in the AMS-02 Era. Accurate measurements of cosmic proton flux are essential for studying the modulation processes of cosmic rays during the solar activity cycle. A proton flux measurement method, based on ground-b... | [
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COSMOS Spectroscopic Redshift Compilation (First Data Release): 488,000 Redshifts Encompassing Two Decades of Spectroscopy. We present the COSMOS Spectroscopic Redshift Compilation encompassing ∼20 yr of spectroscopic redshifts within a 10 deg2 area centered on the 2 deg2 COSMOS legacy field. This compilation contains ... | [
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The NASA Ames PAH IR Spectroscopic Database: Computational Version 4.00, Software Tools, Website, and Documentation. Version 4.00 of the library of computed spectra of the NASA Ames PAH IR Spectroscopic Database (PAHdb) includes an expanded set of polycyclic aromatic hydrocarbon (PAH) spectra, totaling 10,749, calculat... | [
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Recalibration of the Landolt UBVRI Standard Stars and the Generation of 5.4 Million New UBVRI Standard Stars Using LAMOST and Gaia. We present an independent validation and recalibration of the Landolt 2013 (celestial equator and δ ∼ −50∘) and 2016 (δ ∼ −50∘) standard stars in the Johnson UBV and Kron─Cousins RI system... | [
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A Photometric Survey of over 200 V-type Asteroids and Their Phase-curve Analysis. V-type asteroids are considered to be crustal fragments of asteroid (4) Vesta and possibly of other differentiated parent bodies that once existed in the main asteroid belt. A dedicated photometric survey of 213 V-type asteroids and V-typ... | [
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200,000+ Deep Learning─inferred Periods of Stellar Variability from the All-Sky Automated Survey for Supernovae. Stars exhibit a range of variability periods that depend on their mass, age, and evolutionary stage. For space-based photometric data, convolutional neural networks (CNNs) have demonstrated success in recove... | [
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"http://astrothesaurus.org/uat/1668",
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The CAI Database: <SUP>26</SUP>Al─<SUP>26</SUP>Mg Isotope Systematics. We present a publicly available calcium─aluminum-rich inclusion (CAI) database that focuses on the initial 26Al/27Al0 ratio in CAIs, designed in a way that researchers in cosmochemistry and astrophysics may find useful. To date, the database contain... | [
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Planar Collisionless Shock Simulations with the Semi-implicit Particle-in-cell Model FLEKS. This study investigates the applicability of the semi-implicit particle-in-cell code FLexible Exascale Kinetic Simulator (FLEKS) to heliospheric shock simulations. We examine one- and two-dimensional local planar shock simulatio... | [
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A Systematic Search for Active Galactic Nucleus Flares in ZTF Data Release 23. Active galactic nuclei (AGNs) are known to exhibit stochastic variability across a wide range of timescales and wavelengths. AGN flares are extreme outbursts that deviate from this typical behavior and may trace a range of energetic physical... | [
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Highly Efficient Identification of Extreme Emission-line Galaxies in the Local Universe: >8000 New Green Pea Candidates at 0.12 < z < 0.36. The currently known compact extreme emission-line galaxies (the "Green Peas" (GPs)) in the Sloan Digital Sky Survey (SDSS) are rare and were mostly found among serendipito... | [
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A 6 cm Formaldehyde Line Survey toward WISE Point Sources. We conducted a 6 cm formaldehyde (H2CO) line survey across the northern sky, targeting 3149 high-mass star-forming region candidates selected from the all-sky Wide-field Infrared Survey Explorer (WISE) point-source catalog using the Shanghai TianMa 65 m Radio T... | [
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Dwarf Galaxy Integral-field Survey (DGIS): Survey Overview and the Results of a Global Mass─Metallicity Relation. Low-mass galaxies are the building blocks of massive galaxies in the framework of hierarchical structure formation. To enable detailed studies of galactic ecosystems in dwarf galaxies by spatially resolving... | [
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The Reason for the Occurrence of W-type Contact Binaries. For more than half a century, the puzzling W-type phenomenon in contact binaries has challenged astrophysicists. In these systems, the less massive component exhibits a higher surface temperature than its more massive companion, which is a reversal of the typica... | [
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The Green Bank Ammonia Survey: Data Release 2. We present an overview of the final data release (DR2) from the Green Bank Ammonia Survey (GAS). GAS is a large program at the Green Bank Telescope to map all Gould Belt star-forming regions with AV ≳ 7 mag visible from the Northern Hemisphere in emission from NH3 and othe... | [
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The ALPINE-CRISTAL-JWST Survey: JWST/IFU Optical Observations for 18 Main-sequence Galaxies at z = 4─6. To fully characterize the formation and evolution of galaxies, we need to observe their stars, gas, and dust on resolved spatial scales. We present the ALPINE-CRISTAL-JWST survey, which combines kiloparsec-resolved i... | [
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J-HERTz: J-PLUS Heritage Exploration of Radio Targets at z < 5. We introduce J-HERTZ (J-PLUS Heritage Exploration of Radio Targets at z < 5), a new multiwavelength catalog that combines optical narrowband photometry from J-PLUS, infrared observations from the Wide-field Infrared Survey Explorer, and deep low-freq... | [
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Milliarcsecond-resolution Radio-imaging Survey of Blazar Candidates at 4 < z < 5.4. We present a milliarcsecond-resolution radio survey of 17 high-redshift (4 ≤ z ≤ 5.4) blazar candidates observed with the European Very Long Baseline Interferometry (VLBI) Network at 5 GHz. The primary objective of this study was ... | [
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A Comprehensive Hadronic Code Comparison for Active Galactic Nuclei. We perform the first dedicated comparison of five hadronic codes (AM3, ATHEνA, B13, LeHa-Paris, and LeHaMoC) that have been extensively used in modeling the spectral energy distribution (SED) of jetted active galactic nuclei. The purpose of this compa... | [
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Searching for Dark Structures: A Comparison of Weak-lensing Convergence Maps and Lensing-weighted Galaxy Density Maps. We present the result of a comparison between the dark matter distribution inferred from weak gravitational lensing and the observed galaxy distribution to identify dark structures with a high dark-mat... | [
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Radial Gradients and Intrinsic Scatter in MaNGA Galaxies. We derive stellar population parameters and radial gradients within 0.65 Re for spatially resolved spectra of 2968 early-type galaxies from MaNGA, spanning stellar velocity dispersions (σ) of 50─340 km s−1. Light-weighted mean age, C, N, Na, Mg, and Fe abundance... | [
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Can AI Dream of Unseen Galaxies? Conditional Diffusion Model for Galaxy Morphology Augmentation. Observational astronomy relies on visual feature identification to detect critical astrophysical phenomena. While machine learning (ML) increasingly automates this process, models often struggle with generalization in large... | [
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Spectroscopic Identification and Population Properties of Cataclysmic Variables from DESI DR1. We present a systematic search for cataclysmic variables (CVs) using spectroscopic data from Data Release 1 of the Dark Energy Spectroscopic Instrument. Applying the Bagging-TopPush algorithm, we identified 433 CV candidates ... | [
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Fast Protoplanetary Disk Modeling with DUSTRAD: A Dust Evolution and Radiative Transfer Module for FARGO3D. We present DUSTRAD, a dust evolution and radiative transfer module for the FARGO3D hydrodynamic code, designed to efficiently simulate key aspects of long-term protoplanetary disk evolution. The dust evolution em... | [
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Changing-look Active Galactic Nuclei from the Dark Energy Spectroscopic Instrument. V. Dramatic Variability in High-ionization Broad Emission Lines. We present a systematic search for changing-look (CL) quasars at high redshift z > 0.9 by crossmatching the spectroscopic data sets from the Dark Energy Spectroscopic I... | [
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Magnetic Activity in M-type Stars Based on LAMOST DR11 and TESS Observations. We have used 898,351 M-type stellar spectra released by Large Sky Area Multi-Object Fiber Spectroscopic Telescope DR11 to calculate the equivalent width of the Ca II infrared triplet (IRT) lines, the residual chromospheric emission, and the p... | [
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