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Active Galactic Nuclei Do Not Exhibit Strictly Sinusoidal Brightness Variations. Periodic variability in active galactic nuclei (AGNs) light curves has been proposed as a signature of close supermassive black hole (SMBH) binaries. Recently, 181 candidate SMBH binaries were identified in Gaia DR3 based on apparently sta... | [
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Chemical Signatures of AGB Mass Transfer in Gaia White Dwarf Companions. We present a homogeneous abundance analysis of 160 main-sequence stars in astrometric white-dwarf + main-sequence (WD+MS) binaries with orbits from Gaia DR3. These systems have Astronomical unit-scale separations and are thought to have undergone ... | [
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Intermediate-mass Stripped Stars in the Magellanic Clouds: Forward Modeling the Observed Population Discovered Via UV Excess. Stripped stars are hot, helium-rich stars formed when binary interactions remove a star's hydrogen envelope. While low-mass (≲1 M⊙) and high-mass (≳8 M⊙) stripped stars are well studied as hot s... | [
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Hidden in Plain Sight II: Characterizing the Luminous Companion to κ Velorum with VLTI/GRAVITY. κ Vel (Markeb, HD 81188, 天社五) is one of the brightest stars in the Southern sky and has long been known to be a single-lined spectroscopic binary. The binary mass function is large, f(M) = 1.15 M⊙, suggesting that the bright... | [
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Low-luminosity Type IIP Supernovae from the Zwicky Transient Facility Census of the Local Universe. II. Lightcurve Analysis. The Zwicky Transient Facility Census of the Local Universe survey yielded a sample of 330 Type IIP supernovae (SNe) with well-constrained peak luminosities. In paper I, we measured their luminosi... | [
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Four Cold Super-Jupiters Revealed by Extended and Complex Microlensing Signals. We present the analysis of four microlensing events, KMT-2020-BLG-0202, KMT-2022-BLG-1551, KMT-2023-BLG-0466, and KMT-2025-BLG-0121, which exhibit extended and complex anomalies in their light curves. These events were identified through a ... | [
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Photometric Analysis of the Interstellar Comet 3I/ATLAS During its Pre-perihelion Period. We present a photometric study of the interstellar comet 3I/ATLAS based on observations obtained between 2025 July 3 and September 22 from two observatories in Spain (Z10 and Y71) using small-aperture telescopes. The comet was mon... | [
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Dynamical Interactions and Habitability in the TOI-700 Multi-planet System. The discovery of a second earth sized planet (TOI-700e) interior to the habitable candidate TOI-700d has prompted further research into this system, as the additional planet makes the TOI-700 system a tightly packed multi-planet system with mul... | [
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Imaging Venus-like Worlds: Spectral, Polarimetric, and UV Diagnostics for the Habitable Worlds Observatory. Understanding planetary habitability requires a comparative approach that explores the divergent evolutionary outcomes of Earth and Venus. The Habitable Worlds Observatory (HWO) will be uniquely positioned to con... | [
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Chasing the Tides: Searching for Orbital Decay Signatures in Transit Timing Data and Tidal Models for 20 Hot Jupiters. In this work, we present a transit timing variation analysis for 20 hot Jupiter systems, which we interpret with theoretical tidal dissipation models. For the majority of the sample, we conclude that a... | [
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Deep Synoptic Array Science: Searching for Long Duration Radio Transients with the DSA-110. We describe the design and commissioning tests for the DSA-110 Not-So-Fast Radio Burst (NSFRB) search pipeline, a 1.4 GHz image-plane single-pulse search sensitive to 134 ms−160.8 s radio bursts. Extending the pulse width range ... | [
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A High-frequency Geodetic VLBI Experiment for Optical Clock Comparison. An intercontinental metrological clock comparison between Italy and the Republic of Korea was performed by means of geodetic K-band VLBI observations. The comparison involved the hydrogen masers (H-masers) used at Medicina and Sejong radio telescop... | [
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An Efficient Framework for Automatic Carbon Star Detection Using Machine Learning Techniques on LAMOST DR9 and Gaia DR3. Carbon stars are characterized by carbon-rich atmospheres. They play a key role in stellar evolution, enrichment of the interstellar medium, and distance estimation. Therefore, assembling large sampl... | [
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CARTA—Cube Analysis and Rendering Tool for Astronomy: A Tool for Big Imaging Data. Data generated by modern telescopes continues to grow rapidly as a result of these instruments' advanced capabilities, including wide-field imaging with high angular and spectral resolution. The resulting image cubes are often too large ... | [
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Toward Millimagnitude Photometry at the Vera Rubin Observatory: Aerosol Monitoring with Quadband Dispersed Imaging. As the frontier of precision astronomical photometry continues to advance, correcting for time-variable atmospheric transmission becomes increasingly important. We describe an observational approach to mo... | [
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A New Astronomical Plate Digitizer at Shanghai Astronomical Observatory. The advancement of astronomy relies fundamentally on observational data. Between 1850 and 2000, astronomical observatories worldwide produced vast collections of photographic plates that remain invaluable for studying long-term celestial phenomena... | [
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Control Algorithms for Dual-wavefront Sensor Single-conjugate Adaptive Optics. High-contrast imaging systems using active control with adaptive optics (AO) are often limited by non-common path (NCP) aberrations that are seen only at the final science image. AO systems employing focal-plane wavefront sensors (FP-WFSs) a... | [
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The R2Pub Telescopes for Surveying: An Overview and Performance Evaluation of the System. The R2Pub, built by Beijing Planetarium, is a state-of-the-art 60 cm equatorial binocular telescope located at the Daocheng Site (with an altitude of 4700 m) of Yunnan Observatories in China. This paper provides an overview of the... | [
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Performance Study of an Intelligent Astronomical CMOS Camera. Mosaic sCMOS cameras are critical for wide-field astronomical surveys. However, the massive data volume generated by these high-resolution arrays imposes severe strains on traditional architectures, creating bottlenecks in data transmission bandwidth and sys... | [
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Detailed TESS-Based Light Curve Modeling and Fundamental Parameter Estimation of 27 W UMa-Type Contact Binaries. We performed a comprehensive analysis of 27 short period contact binary systems for which no light curve analysis had previously been reported. Photometric time-series data from the TESS mission were used in... | [
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KMT-2016-BLG-1337L: A Saturn-mass Planet Orbiting Within a Binary System of Low-mass Stars. We report the discovery and characterization of a planetary companion in the microlensing event KMT-2016-BLG-1337, which was produced by a binary system of low-mass stars. The light curve of the event exhibits a short-term anoma... | [
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Equatorial Waves Associated with Dust Storms as Simulated in a Mars General Circulation Model. Equatorial atmospheric waves provide a mechanism for variability on a wide range of timescales and for disturbances in one part of the tropics to influence other tropical locations around the globe. A Mars general circulation... | [
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Coupled 1D Chemical Kinetic Transport and 2D Hydrodynamic Modeling Supports a Modest 1─1.5× Supersolar Oxygen Abundance in Jupiter's Atmosphere. Understanding the deep atmospheric composition of Jupiter provides critical constraints on its formation and the chemical evolution of the solar nebula. In this study, we comb... | [
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On the Border: Searching for Cometary Activity near the Centaur─JFC Transition Line. Current wide-field surveys discover ∼15 Jupiter-family comets (JFCs) each year, typically identified via visual detection of a dust coma or tail. The same surveys also discover many asteroids that have distant JFC-like orbits, but with... | [
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3D Reconstruction of DART Ejecta at Dimorphos Reveals an Anisotropic, Filamentary Structure. We present a 3D reconstruction of the ejecta plume generated by the DART impact on Dimorphos based on LUKE images acquired by LICIACube. Using adaptive histogram equalization and geometric coregistration from multiple vantage p... | [
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Similar Topography and Crater Retention Record yet Divergent Space Weathering Extents across Reiner Gamma on the Moon. Electrostatic levitation and migration of charged dust may occur during the formation of lunar swirls. Due to interaction between crustal magnetic anomalies and solar wind, immature fine-grained partic... | [
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Interaction of Solar Wind Energy Helium Ions with Enstatite Surfaces Progressively Altered by Simulated Impact Melting. The interactions between micrometeoroid impacts and solar wind on the surface of the Moon remain a major area of investigation in the space weathering field. In this study, we first irradiated Fe-bear... | [
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Impact-induced Contamination of Ganymede's Deep Ice Shell. Juno flew by Ganymede in 2021 June and measured the microwave brightness temperatures of the ice shell at six frequencies from 0.6─22 GHz. Based on the increasing brightness temperature with wavelength, S. Brown et al. (2023) derived a geothermal temperature gr... | [
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Reliability of Assessing Lunar Crustal Density Structures Using the GRAIL Gravity Model. The spatial resolution of gravity data acquired by the Gravity Recovery and Interior Laboratory (GRAIL) mission is adequate to resolve relatively small-scale density structures larger than approximately tens of kilometers within th... | [
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From Dawn till Dusk: How Light Reduces Martian Granular Slope Angles. The maximum slope of a granular surface—beyond which particles start to move through avalanches—is determined by the balance of gravitational and interparticle forces and is independent of gravity when only frictional forces act between the particles... | [
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Revealing Callisto's Near-subsurface Thermophysical Properties with ALMA Calibration Data. Thermal images at different wavelengths probe varying subsurface depths of planetary bodies and therefore can inform us about their compositions, thermophysical properties, and impact histories. We identified six archival observa... | [
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Surface Modifications of a Space-weathered Ryugu Sample and the Reflectance Spectral Response. Reflectance spectra from the surface of asteroid Ryugu, measured by the Hayabusa2 spacecraft, exhibit a metal-OH absorption at ∼2.7 μm that is approximately half as deep as the returned samples measured in the laboratory and ... | [
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Inferring and Interpreting the Visual Geometric Albedo and Phase Function of Earth. Understanding reflectance-related quantities for worlds enables effective comparative planetology and strengthens mission planning and execution. Measurements of these properties for Earth, especially its geometric albedo and phase func... | [
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Dripping to Destruction: Exploring Salt-driven Viscous Surface Convergence in Europa's Icy Shell. The Europan ice shell is thought to be simultaneously a key contributor and a barrier to the underlying ocean's habitability. Life-supporting oxidants formed by surface radiolysis have the potential to be a significant com... | [
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Effect of a Surficial Porous Brittle Layer on the Dynamics and Equilibrium Thickness of Europa's Ice Shell. Tectonic and cryovolcanic features on Europa suggest a dynamically active ice shell with a highly deformable near-surface brittle layer. Shell thickness estimates based on geological interpretation and thermal mo... | [
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Spin Parameters and Shape Models of Near-Earth Asteroids (4660) Nereus, (21088) Chelyabinsk, (66146) 1998 TU3, and (297418) 2000 SP43. We present our shape and rotational characterization of four near-Earth asteroids observed as part of the Visible NEAs Observations Survey. This work includes 61 new light curves obtain... | [
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The Sesquinary Catastrophe on Deimos Can Reconcile Its Excited Past with Its Dynamically Cool Present. The origins of the Martian moons Phobos and Deimos are highly debated, and hypotheses include formation from an impact-generated circum-Martian disk and formation from capture of asteroids. With the impact scenario, D... | [
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Penetration Law in Loose Granular Medium for the Chang'E 5 and Chang'E 6 Footpad. This study investigates the penetration behavior of the footpads used in the Chang'e-5 (CE-5) and Chang'e-6 (CE-6) lunar probes when interacting with granular materials. Through a series of controlled impact experiments conducted using a ... | [
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Remote Compositional Analyses of Space-weathered Lunar Maria. Visible-to-shortwave infrared (VSWIR) reflectance spectroscopy has revolutionized our understanding of planetary surface compositions. However, space-weathering processes on airless bodies complicate quantitative compositional analyses. Here, we present a fr... | [
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The Prospects for Gravitational Seismology at Uranus with an Orbiting Spacecraft. We study the feasibility of conducting gravitational seismology at Uranus, that is, of detecting and characterizing Uranian normal-mode oscillations through their perturbations on the trajectory of an orbiting spacecraft. Characterizing s... | [
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Model for Determining the Origin of Lunar Volatiles Based on Their Composition: Application to NASA's VIPER and Other Landed Missions. Lunar volatiles provide a potentially pristine record of the history of the Earth─Moon system in terms of both geologic activity and delivery of volatiles from the outer solar system. E... | [
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Determination of Venus's Rotation State Using Radio-tracking Data from the Venus Express Spacecraft. Despite its similarities to Earth, our understanding of Venus remains limited, particularly regarding its long retrograde rotation period. This has been measured using both Earth-based and in-orbit methods. However, the... | [
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The Effect of Colored Noise on Doppler Measurements for Planetary Geodesy: Application to the VERITAS Gravity Science Experiment. Measurements of the Doppler shift of a carrier signal have always been the basis of radio science experiments, particularly for planetary gravity field recovery. Doppler observables are affe... | [
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Nucleus Ice Associations in Comets Derived from Spatially Resolved Properties of Volatile Gases in the Coma. Under favorable conditions, high-resolution long-slit infrared spectroscopic observations of comets can provide information on how ices are associated within the nucleus from spatially resolved properties of vol... | [
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An Integrated Framework for Global Detection and Quantification of Lunar Pyroclastic Deposits. Lunar pyroclastic deposits (LPDs) composed of Fe─Ti-bearing volcanic glasses are considered one of the best proxies to understand the primitive lunar mantle composition. These deposits are characterized by very low albedo and... | [
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Photochemistry in Jupiter's Ionosphere: Insights from Simultaneous <inline-formula> <mml:math><mml:msubsup><mml:mrow><mml:mi>H</mml:mi></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:msubsup></mml:math> </inline-formula> and Electron Density Observations during Juno Perijo... | [
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Spectral Evidence for Recent/Ongoing Activity in Mercury's Praxiteles Basin. Mercury's surface, as revealed by the MESSENGER probe, lacks distinctive absorption features in the visible─near-infrared spectral range, except for hollows that display a 630 nm feature ascribed to sulfides. The general absence of spectral fe... | [
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Modeling the Meteoroid Environment Far from the Ecliptic Plane. We describe a new version (numbered 3.1) of NASA's Meteoroid Engineering Model, in which we extend the model to handle locations that lie more than a few degrees in latitude off the ecliptic plane. We provide our algorithms for computing the spatial densit... | [
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Mass-wasting Features on Galilean Icy Moons: Morphological Analysis and Implications. This study investigates mass-wasting features on the icy Galilean satellites Europa, Ganymede, and Callisto. Through comparative morphological analysis, we identified and classified slides, slumps, and flow-like deposits as mass-wasti... | [
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Toward Reliable Interpretations of Small-exoplanet Compositions: Comparisons and Considerations of Equations of State and Materials Used in Common Rocky Planet Models. The bulk compositions of small planets (Rp < 2 R⊕) are directly linked to their formation histories, making reliable compositional constraints impera... | [
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Covertly Active Comet (139359) 2001 ME1. On 2018 November 18, coronagraphs onboard the Solar and Heliospheric Observatory (SOHO) captured an unrecognized comet crossing its fields of view. We identified this comet to be the minor planet (139359) 2001 ME1, whose previously unnoticed dust activity near perihelion became ... | [
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A One-dimensional Microphysical Model of the Venus Cloud System between 40 and 80 km Including Photochemistry and Radiative-dynamic Feedback. We present results from 1D simulations using PlanetCARMA for Venus in which, for the first time, a sophisticated 1D cloud microphysics model has simultaneously incorporated simpl... | [
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Modeling the Effects of Anthropogenic Activities on the Lunar Environment with a Systems-theoretic Approach. An increasing number of missions to the Moon are planned for the future. However, their long-term, cumulative impacts on the lunar environment are unknown. Research indicates that some important scientific disco... | [
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Dawn─Dusk Asymmetry of the Io Plasma Torus Derived from Io's Auroral Footprints Observed by Juno-UVS. The Io plasma torus (IPT) is a dense plasma cloud that corotates around Jupiter near Io's orbit. A dawn-to-dusk electric field shifts the IPT dawnward. The shift orientation has been previously measured, but the observ... | [
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Evolution of the Mercurian Crust as Recorded in Carbon. Mercury and other silicate bodies are essential for understanding planetary formation and evolution. The surface of Mercury is unique and enigmatic, yet this innermost planet remains the least explored. The crust exhibits relatively low reflectance, possibly due t... | [
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The Surface Mineralogy of the Spinel-rich Asteroids from Mid-infrared Spectroscopy with JWST. The "Barbarian" L-type asteroids are purported to contain a high abundance of calcium─aluminum inclusions (CAIs), the oldest solar system solids, based on the dominance of the mineral spinel in their near-infrared spectra. We ... | [
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A Mars Microbial Survival Model: Calculating Bioburden Reductions for Past Mars Spacecraft to Estimate Forward Contamination on Mars. Minimizing the forward contamination of Mars from terrestrial microorganisms is a key objective of planetary protection. To model the survivability of terrestrial spacecraft microorganis... | [
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The Relative Cold-trapping Likelihood of Water on Airless Rocky Bodies. Many planetoids are airless, but despite the lack of a collisional atmosphere, these bodies can experience volatile migration toward the polar regions via the exosphere. However, there is a lack of parametrical studies that focus on cold-trapping a... | [
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Dating Young, Low-K Martian Meteorites with an In Situ K─Ar Isochron Technique for Mars Missions. Accurate age determination is fundamental to advancing our understanding of planetary evolution. While sample-return missions provide the most accurate age measurements, in situ methods via one-way missions offer a signifi... | [
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Formation Age of Ernutet Crater, Ceres, and Implications for Origin of the Organics. Ceres is the largest body in the Main Asteroid Belt and has a unique composition characterized by products of aqueous alteration such as carbonates, ammoniated phyllosilicates, and organic materials in concentrated regions. A large org... | [
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Formation and Survival of Complex Organic Molecules in the Jovian Circumplanetary Disk. Europa, Ganymede, and Callisto are key targets in the search for habitability due to the potential presence of subsurface oceans. Detecting complex organic molecules (COMs), essential for prebiotic chemistry, is crucial to assessing... | [
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Thermal Stability of Ice at Shackleton Crater: Implications for Water Ice Detection for the Chang'E-7 Mission. The candidate landing region for China's Chang'E-7 (CE-7) lunar exploration mission is near Shackleton crater at the lunar south pole, and the CE-7 mission will perform in situ detection of water ice. We model... | [
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Near-infrared Hapke Photometric Analysis of the Moon's Regolith with Passive Radiometry from the Lunar Orbiter Laser Altimeter (LOLA). Measurements of the Moon's surface reflectance across a broad range of wavelengths and geometries can provide vital clues about the processes acting on its regolith. In the near-infrare... | [
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Formation of Water-rich Giant Planet Satellites at Decretion Disk Ice Lines. The volatile budgets of giant planet satellites are critical to unraveling the origin of their building blocks within the circumplanetary disks that hosted them. The Galilean moons Ganymede and Callisto, as well as the Saturnian moon Titan, ar... | [
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Inferring Exoplanet Parameters from Transit Timing Variations Using LSTM Networks. Transit timing variation (TTV) analysis provides a valuable complement to traditional transit and radial-velocity techniques, particularly in compact, near-resonant planetary systems where dynamical interactions amplify timing signals an... | [
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Surface Properties, Orbital Dynamics, and Thermophysical Modeling of the Primitive Asteroid (269) Justitia. The Emirates Mission to the Asteroid Belt (EMA) will study the ultrared asteroid (269) Justitia. In this work, we present the first detailed investigation of Justitia's surface dynamics using the newly developed ... | [
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Thermophysical Modeling of Asteroid (15) Eunomia from Spatially Resolved ALMA and VLA Data. Asteroid (15) Eunomia is the largest S-type asteroid in the main belt and the largest member of the Eunomia asteroid family. Previous visible-to-mid-infrared data suggested that Eunomia's hemispheres have different olivine-to-py... | [
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UV─Vis─NIR Reflectance Spectra of Ilmenite Mixtures: Implications for Estimation of TiO<SUB>2</SUB> Content in Lunar Mare Regions. We performed spectral measurements on mixtures of ilmenite powder (<48 μm) and clinopyroxene or gabbro powder (<155 μm) to investigate the effect of ilmenite content on the spectral c... | [
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The Flux of Large Impacts on the Moon Enhanced near the Beginning of the Copernican Period. The size─frequency distribution (SFD) of lunar impactors was believed to be time independent for the last 3.5 billion years (Gyr). Here, I use linear and nonlinear topographic diffusion models to determine the degradation states... | [
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Distribution of Buried Volcanic Deposits in the Schiller─Schickard Region of the Moon. Cryptomaria are ancient volcanic units on the Moon that are key to understanding early lunar thermal history but are difficult to study because they have been buried and obscured from direct view by later impact ejecta. The Schiller─... | [
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A Comprehensive Spectroscopic Reference of the Solar System and Its Application to Exoplanet Direct Imaging. We present a calibrated database of reflectance spectra for the solar system planets (i.e., Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune) and for Titan, spanning from the ultraviolet to the near... | [
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Origin of Hyperion and Saturn's Rings in a Two-stage Saturnian System Instability. The age of the rings and some of the moons of Saturn is an open question, and multiple lines of evidence point to a recent (few hundred Myr ago) cataclysm involving the disruption of past moons. The main driver of the evolution of the Sa... | [
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Impact-driven Deposition of Metallic Titanium on the Moon. Impact-induced high temperatures are a key driver of titanium (Ti) redistribution in Ti-bearing phases, which is crucial for understanding element cycling on the Moon. However, direct mineralogical evidence for the redistribution pathways of Ti during extreme i... | [
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Haze, Methane, and Carbon Monoxide in Titan's North Polar Atmosphere from a Cassini/VIMS Specular Transmission Spectrum on the T104 Flyby. We analyze a specular reflection of the Sun off of Titan's largest sea, Kraken Mare, observed by the Cassini Visual and Infrared Mapping Spectrometer on the T104 flyby (2014 August ... | [
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Hydration Features on Near-Earth Objects: Integrating New Data with Prior Results. Near-Earth objects (NEOs) are excellent laboratories for testing processes that affect airless bodies, as well as informing us about solar system history. Though most NEOs are nominally anhydrous because they formed inside the solar syst... | [
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The Fate of Frozen Carbonated Water at Europa-like Conditions. We present the results of experiments probing the retention of CO2 in crystalline water ice, frozen sodium chloride (NaCl) brines, and flash-frozen carbonated water using diffuse reflectance infrared spectroscopy. Characteristic absorptions alluding to the ... | [
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Early Observations of New Active Asteroid 2025 VZ<SUB>8</SUB>. We report observations of main-belt asteroid 2025 VZ8 using multiple telescopes from UT 2025 November 24 to UT 2025 December 23 that confirm the presence of visible comet-like activity. These observations were motivated by online reports that an abrupt brig... | [
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Infrared Spectroscopy of the Nova V5115 Sagittarii during Its Fe II Phase. V5115 Sagittarii was a very fast nova (t2 = 7 days) from a massive white dwarf (1.2 M⊙). Our 0.8─5.0 μm spectrum from 19 days after discovery shows numerous Fe II lines and weak, just emerging He I emission and falls clearly within the Fe II-typ... | [
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First Separation of Iron Lines in the Cataclysmic Variable IGR J14536-5522 with Suzaku/XIS. We present new analysis of the cataclysmic variable IGR J14536-5522 observed with the X-ray Imaging Spectrometer onboard the Suzaku satellite. Based on the light curve, we did not confirm the periodicity (3756 s) reported in the... | [
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Spatially Resolved Analysis of Ionization Mechanisms in SGAS1723+34. Understanding the ionizing sources inside galaxies has been a decades-long goal for astronomers. Using spatially resolved JWST/NIRSpec data, we explore the emission line diagnostics [O III]/Hβ versus [N II]/Hα and [S II]/Hα in SGAS1723+34, a galaxy at... | [
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A Long Tidal Feature Extending from a Low-redshift Galaxy Revealed in Rubin Data Preview 1 Imaging. Using the Vera C. Rubin Observatory Data Preview 1, we present the detection and photometric analysis of a stellar stream extending along the minor axis of a massive disk-galaxy, LEDA 751050, at a redshift of z = 0.1 in ... | [
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A Précis of the MOA-II Observations. The Microlensing Observations in Astrophysics (MOA) collaboration is an international research project that uses gravitational microlensing for the discovery of exoplanets. MOA was initiated in the late 1990s and primarily involves institutions from Japan and New Zealand. The collab... | [
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Discovery of Microsecond Duration Radio Flashes with Small Radio Telescopes. We present the discovery of floods of short duration transient radio events detected simultaneously by at least 3 of 7 small horn radio telescopes, when continuously observing the sky at 1421.5 ± 3.0 MHz. The goal of these observations is to d... | [
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Modeling of Circumstellar Alumina and Silicate Dust around Evolved Stars. Spectra of some asymptotic giant branch (AGB) and red supergiant (RSG) stars show emission features at mid-infrared wavelengths, such as at 13 μm, that have previously been inconclusively identified. We present models of dust emission seen in spe... | [
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Automatic Dust Detection, Isolation, and Mass Measurement Pipeline. Dust in elliptical galaxy cores provides insights into the interstellar medium and galactic evolution. I present an automated pipeline analyzing archived Hubble Space Telescope WFPC2 and ACS images to detect and measure dust masses in early-type galaxi... | [
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Monsters in the Dark: Revealing Hidden Bars in Submillimeter Galaxies. Using JWST NIRCam F444W imaging from the SCUBADive project, we identify five sub-millimeter galaxies that host stellar bars. These include AzTECC91_0 at z = 1.91 ± 0.11, which has the most extended bar known at z > 1 (8.42 ± 0.05 kpc), and AzTECC... | [
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Ionization Stratification and Stellar Feedback in the Galactic H II Region Sh2-124 from Deep Narrowband Imaging. I present deep narrowband imaging of the Galactic H II region Sh2-124 obtained with a total integration time of 79 hr using 2.5 nm S II, Hα, and O III filters. The observations reveal a well-defined shell mo... | [
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The Size of 3I/ATLAS from Non-gravitational Acceleration. The third macroscopic interstellar object detected in the solar system recently passed through perihelion, with the best-fitting models of its trajectory now featuring non-gravitational accelerations (NGAs). We assess how much mass loss is required to produce pl... | [
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A Terrestrial-sized Planet Candidate Orbiting the Nearby M-dwarf TIC 22760643.01. The identification and multi-sector validation of a terrestrial-sized planet candidate orbiting the nearby M-dwarf TIC 22760643 (L 326-21, d ≍ 15.8 pc) are reported. Using TESS photometry from Sectors 10, 37, and 64, a periodic transit si... | [
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A Simple One-free-parameter Model of the Solar Chromosphere Explains Solar Chromospheric Line Variations Measured by NEID at WIYN during the 2023 October Solar Eclipse. We have modeled Hα equivalent width and Ca II H & K S index measurements of disk-integrated sunlight during the 2023 October solar eclipse as measu... | [
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First Tabulation of the Sunspot-cycle Start in the Seventeen Cycles Since the Cycle's Discovery: Consequences for the Solar Dynamo?. In the seventeen Cycles 8─24 the first new-cycle sunspot group is tabulated for the first time in each solar hemisphere (thirty-four groups). This allows the determination of the central-... | [
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Gravity-darkening Coefficients for the Space Mission JWST, Based on PHOENIX Spherical Models at High Resolution: NIRCam, NIRISS, and NIRSpec Passbands. Space-based photometry has revealed the subtle effects of gravity darkening on the light curves of transiting exoplanets, allowing valuable new information on these obj... | [
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Rare Near-opposition Alignment of 3I/ATLAS on 2026 January 22. We point out that on 2026 January 22, the interstellar object 3I/ATLAS will align to within an exceptionally small angle, α=0.°69 , with the Earth─Sun axis. This rare alignment provides unique circumstances for measuring the opposition surge and polarimetr... | [
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Hidden Companions to Intermediate-mass Stars. XXXIV. Discovery of the Companions in Five "Boring" Accelerating A-type Stars. Better constraints on the multiplicity properties of A-type stars are relevant to understand the formation of intermediate-mass multiple systems as well as to constrain the multiplicity propertie... | [
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Effect of Different Non-gravitational Accelerations on the Trajectory of Interstellar Comet 3I/ATLAS. Comet C/2025 N1 or 3I/ATLAS is the third confirmed interstellar object. It has passed perihelion on 2025 October 29, and is currently on a path to leave the solar system. During its outbound journey, it will pass close... | [
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Determination of the Abundance of Mercury from the Hg II Line at 5677.10 Å in Late B-type Stars. XXVII. HD 1909 (AV Scl). The weak line of Hg II located at 5677.10 Å is used to measure the mercury abundance in the most massive component of the SB 2 HgMn star HD 1909 (AV Scl). This line, which absorbs about 5% of the ad... | [
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"http://astrothesaurus.org/uat/128",
"http://astrothesaurus.org/uat/1024",
"http://astrothesaurus.org/uat/1192",
"http://astrothesaurus.org/uat/1634",
"http://astrothesaurus.org/uat/1761"
] | [
"B stars",
"Mercury (planet)",
"Overabundances",
"Stellar types",
"Variable stars"
] | [
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