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The Tantalizing Case of the Quasar J0950+5128. I. Presentation of the Data and Detailed Exploration of the Binary Supermassive Black Hole Scenario. Spectroscopic observations of the quasar J0950+5128 spanning 22 yr reveal monotonic radial velocity variations in its broad Hβ emission line. Moreover, the line profile bec... | [
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Multiwavelength Study of a Superflare on RS CVn─Type Star HD 22468 Triggered at Hard X-Ray by SVOM. Detection of stellar flares at hard X-ray is still rare at the current stage. A transient was recently detected by the hard X-ray camera ECLAIRs on board the SVOM mission at 11:39:01.2 UT on 2025 January 09. Simultaneous... | [
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A Multiwavelength Study of the 2025 Low State of the Intermediate Polar BG CMi. We present multiwavelength observations of the first recorded low state of the intermediate polar BG CMi. Optical monitoring of the source by members of the American Association of Variable Star Observers reveals a decrease of ∼0.5 mag that... | [
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Detection of a Millisecond Periodicity in BATSE Short Gamma-Ray Bursts. Coherent oscillations at kilohertz frequencies have recently been detected in a small number of gamma-ray bursts (GRBs), suggesting quasiperiodic dynamics in their central engines. A prominent example is GRB 230307A, which exhibited a brief, highly... | [
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Investigating Polarization Signatures from GRB Models. There is still much debate around the inner workings of the gamma-ray-burst (GRB) prompt emission phase, with many questions still left unanswered. Polarization signatures offer a promising new avenue for discriminating between the various GRB prompt emission model... | [
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Dependence of Halo Properties on Central-satellite Magnitude Gaps through Weak Lensing Measurements. The magnitude gap between the central and satellite galaxies encodes information about the mass accretion history of a dark matter halo and serves as a useful observational probe for the mass distribution in a halo. In ... | [
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A Highly Magnetic Ultramassive White Dwarf with a 23 minute Rotation Period. We present a physical characterization of Tsinghua University-Ma Huateng Telescope for Survey (TMTS) J00063798+3104160 (J0006), a rapidly rotating, ultramassive white dwarf (WD) identified in high-cadence light curves from the TMTS. A coherent... | [
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Unveiling Obscured Accretion in the Local Universe. Heavily obscured active galactic nuclei (AGNs), especially Compton-thick sources with line-of-sight column density (NH,los) > 1024 cm−2, are critical to understanding supermassive black hole growth and the origin of the cosmic X-ray background. However, their obser... | [
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Lensing, Not Luck! Detection Prospects of Strongly Lensed Gravitational Waves. A small fraction of gravitational-wave (GW) signals detected by ground-based observatories will be strongly lensed by intervening galaxies or clusters. This may produce multiple copies of the signals (i.e., lensed images) arriving at differe... | [
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Turbulent Properties of Interplanetary Coronal Mass Ejections Observed by Solar Orbiter in the Inner Heliosphere. We investigate the turbulent properties of 12 interplanetary coronal mass ejections (ICMEs) observed by Solar Orbiter between 0.29 and 1.0 au. We analyze fluctuation power, spectral indices, break scales, a... | [
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Ruling Out Compact Jets as the Dominant Source of Radio Emission in Radio-quiet, High-Eddington-ratio Active Galactic Nuclei. The origin of core radio emission in radio-quiet active galactic nuclei (AGNs) is still actively debated. General-relativistic magnetohydrodynamics simulations often predict the launching of mod... | [
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XFit: Global Optimization and Degeneracy Mapping in X-Ray Spectral Modeling. The standard approach to modeling X-ray spectral data relies on local optimization methods, such as the Levenberg─Marquardt algorithm. While effective for simple models and speedy spectral fitting, these local optimizers are prone to becoming ... | [
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Statistical Analysis of Multiband Plateaus in Gamma-Ray Burst Afterglows. Plateau features are frequently observed in the afterglows of gamma-ray bursts (GRBs), yet their physical origins remain under debate. In this work, we compile a sample of 124 GRBs with known redshifts and simultaneous X-ray and optical afterglow... | [
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Probing Dust Composition in Distant Galaxies with JWST Mid-IR Spectroscopy of Quasars with Foreground 2175 Å Absorbers. I. Methodology. Interstellar dust plays a crucial role in gas cooling and molecule formation, influencing galaxy evolution. However, the composition and structure of dust in distant galaxies are still... | [
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The Mass Distribution of Clumpy Accretion onto the Nearby Young Star TW Hya. The proliferation of high time resolution and decades-long monitoring of classical T Tauri stars provides a vast opportunity to test the variability of star─disk connections. However, most monitoring surveys use single broadband filters, which... | [
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A Comprehensive Study of the Relations between the Properties of Planetary Systems and the Chemical Compositions of Their Host Stars. The giant planet─metallicity correlation revealed that planetary formation depends on the stellar properties. There is growing evidence that it is also valid for smaller hot planets, but... | [
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ALMAGAL. VII. Cataloging Hierarchical Continuum Structure from Cores to Clumps across the Galactic Disk. Investigating the multiscale fragmentation of dense clumps into compact cores is essential for understanding the processes that govern the initial distribution of mass in stellar clusters and how high-mass stars (&g... | [
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The Impact of Orbital Anisotropy Assumptions in Lensing-dynamics Modeling. We investigate potential systematic biases introduced by assumptions regarding stellar orbital anisotropy in joint lensing-dynamics modeling. Using massive early-type galaxies from the TNG100 simulation at redshifts z = 0.2, 0.5, and 0.7, we gen... | [
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Simulating Image Coaddition with the Nancy Grace Roman Space Telescope. IV. Hyperparameter Optimization and Experimental Features. For weak gravitational lensing cosmology with the forthcoming Nancy Grace Roman Space Telescope, image coaddition (or construction of oversampled images from undersampled ones) is a critica... | [
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Next-generation Improvements in Giant-exoplanet Evolutionary and Structural Models. Many evolutionary models of giant exoplanets still rely on simplifying assumptions that are no longer adequate, given detailed constraints from Jupiter, Saturn, and modern exoplanet observations. Here, we identify the key physical impro... | [
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A JWST Paα Calibration of the Radio Luminosity─Star Formation Rate Relation at z ∼ 1.3. As radio emission from normal galaxies is a dust-free tracer of star formation, tracing the star formation history of the Universe is a key goal of the Square Kilometre Array and the Next-Generation Very Large Array. In order to inv... | [
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An Enhanced Sample of Galactic Red Supergiants Reveals Spiral Structures. Red supergiants (RSGs), representing a kind of massive young stellar population, have rarely been used to probe the structure of the Milky Way, mainly due to the long-standing scarcity of Galactic RSG samples. The Gaia BP/RP spectra (hereafter XP... | [
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Tracing Pebble Drift History in Two Protoplanetary Disks with CO Enhancement. Pebble drift is an important mechanism for supplying the materials needed to build planets in the inner region of protoplanetary disks. Thus, constraining pebble drift's timescales and mass flux is essential to understanding planet formation ... | [
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A Physics Informed Neural Network for Deriving MHD State Vectors from Global Active Regions Observations. Solar active regions (ARs) do not appear randomly but cluster along longitudinally warped toroidal bands ("toroids") that encode information about magnetic structures in the tachocline, where global-scale organizat... | [
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Discovery of a 21 cm Absorption System at z = 2.327 with CHIME. We report the detection of a new 21 cm absorption system associated with the radio source NVSS J164725 + 375218 at a redshift of z = 2.327, identified through a pilot survey conducted by the Canadian Hydrogen Intensity Mapping Experiment (CHIME). This is t... | [
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The Most Luminous Hβ Reverberation Mapping of E1821+643 Indicates the Lower Boundary of the Radius─Luminosity Relation. The radius─luminosity (RBLR─L5100) relation is fundamental to active galactic nucleus (AGN) studies, enabling supermassive black hole (SMBH) mass estimates and AGN-based cosmology applications. Howeve... | [
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Radio Near-infrared Imaging of Dual Active Galactic Nuclei Candidates. We report the results of a pilot study that searched for dual active galactic nuclei (AGN) in local (z < 0.25) galaxies hosting double-peaked narrow emission lines in their optical spectra. We present high-resolution L-band (1.5 GHz or 18 cm) con... | [
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Single-pulse Correlations in PSR B0329+54: Implications for Radio Emission Zones. Individual radio pulses from a pulsar are directly linked to the underlying emission processes and the associated magnetic field geometry within its magnetosphere. Thus, single-pulse studies across frequencies can provide crucial insights... | [
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The Impact of Diffusion and Turbulent Mixing on Chemical Abundance Variations in the Open Cluster NGC 2420. The mixing of material in stellar envelopes critically determines surface elemental abundances. A well-established tension remains between theoretical models and observational data for stars near the main-sequenc... | [
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NuSTAR and TESS Discovery of an Intermediate Polar IGR J19173+0747. IGR J19173+0747 was discovered as an X-ray source by the INTEGRAL satellite and was initially classified as either a high-mass X-ray binary (HMXB) or a magnetic cataclysmic variable. Here, we report the detection of a coherent X-ray pulsation with a pe... | [
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The Spectral Features of Single-band Type III-like Radio Bursts Observed by PSP during Its First Nine Orbital Encounters. The spectral features of 1122 single-band type III-like radio bursts were analyzed statistically using data from the Parker Solar Probe (PSP) during the first nine orbital encounters. After excludin... | [
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Variability Study and Searching for Quasiperiodic Oscillations with Day-like Periods in the Blazar S5 0716+714 with TESS. Using an unprecedented cadence of 30 minutes provided by the Transiting Exoplanet Survey Satellite, we have examined the optical light curves (LCs) of the blazar S5 0716+714 obtained from its Sector... | [
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Taming the Tarantula: How Stellar Wind Feedback Shapes Gas and Dust in 30 Doradus. Observations of massive star-forming regions show that classical stellar wind models overpredict the luminosity of the X-ray-emitting gas, indicating a significant fraction of wind energy is lost. In this paper, we present a multiwavelen... | [
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Spin-down Changes in PSR B0540-69 Induced by a Drift of the Magnetic Axis. The dynamics of the solid crust + magnetic field lines of pulsars is a much debated issue and remains unsettled after 50 yr. Some pieces of evidence have emerged to complete and confirm theoretical calculations and expectations. We discuss in th... | [
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Exploring Cosmological Constraints of the Void-lensing Cross Correlation in the CSST Photometric Survey. We investigate the cosmological constraints from the void-lensing cross correlation assuming the wCDM model for the Chinese Space Station Survey Telescope (CSST) photometric survey. Using Jiutian simulations, we con... | [
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When IIb Ceases To Be: Bridging the Gap between IIb and Short-plateau Supernovae. Hydrogen-rich supernovae (SNe) span a range of hydrogen envelope masses at core collapse, producing diverse light curves from extended plateaus in Type IIP SNe to double-peaked Type IIb SNe (SNe IIb). Recent simulations predict a continuo... | [
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Long-term (250 yr) Hydrodynamical Simulation of the Supermassive Black Hole Binary OJ 287. With upcoming facilities capable of detecting photometric and gravitational wave signals from supermassive black hole (SMBH) binaries, studying their long-term accretion-driven variability is timely. OJ 287 is a bright, nearby (z... | [
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Evidence of Gas Depletion in Quasars with Moderate Radio Emission. The energy released by active galactic nuclei (AGNs) is considered to have a profound impact on the cold gas properties of their host galaxies, potentially heating or removing the gas and further suppressing star formation. To understand the feedback fr... | [
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Secular Excitation of Polar Neptune Orbits in Pure Disk─Planet Systems. The stellar spin─orbit angles of Neptune-sized planets present a primordial yet puzzling view of the planetary formation epoch. The striking dichotomy of aligned and perpendicular orbital configurations are suggestive of obliquity excitation throug... | [
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Void Galaxies and Active Galactic Nucleus Activity in ZOBOV-identified TNG300 Voids from z = 3 to z = 0. We study void galaxies in the TNG300 simulation between redshifts z = 3 and z = 0. Cosmic void catalogs were constructed using a watershed-based void-finding algorithm, and we define four populations of field galaxi... | [
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Limiting Eccentricity in Restricted Hierarchical Three-body Systems with Short-range Forces. A hierarchical three-body model can be widely applied to diverse astrophysical settings, from satellite─planet─star systems to binaries around supermassive black holes. The octupole-order perturbation on the inner binary from t... | [
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A Low-mass Model of the Milky Way: The Disk Warp Resulting from a Galaxy Merger. Previous studies have shown that disk warps can result from galaxy mergers. Recent research indicates a noticeable decline in the rotation curve (RC) of the Milky Way, suggesting the need for a new low-mass model to describe its dynamical ... | [
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Multiband Gravitational-wave Observations of Eccentric Escaping Binary Black Holes from Globular Clusters. Stellar-mass binary black holes (sBBHs) formed in globular clusters (GCs) are promising sources for multiband gravitational-wave (GW) observations, particularly with low- and middle-frequency detectors. These sBBH... | [
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How to Evaluate the Sufficiency and Complementarity of Summary Statistics for Cosmic Fields: An Information-theoretic Perspective. The advent of increasingly advanced surveys and cosmic tracers has motivated the development of new inference techniques and novel approaches to extracting information from cosmic fields. A... | [
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ALMA Polarization Study of the Magnetic Fields in Two Massive Clumps in the 20 km s<SUP>−1</SUP> Cloud of the Central Molecular Zone. We present the Atacama Large Millimeter/submillimeter Array observations of linearly polarized 870 μm continuum emission at ∼0 .″ 2 (2000 au) resolutions toward the two massive clumps, C... | [
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Convolutional Neural Networks for Classifying Galaxy Mergers: Can Faint Tidal Features Aid in Classifying Mergers?. Identifying mergers from observational data has long been a crucial aspect of studying galaxy evolution and formation. Tidal features, typically fainter than 26 magarcsec−2 , exhibit a diverse range of a... | [
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The Orbital Parameters of Gamma-Ray Binary PSR J2032+4127. PSR J2032+4127 is the only gamma-ray binary that exhibits pulsations in gamma rays. Previous research has indicated that the pulsar and the Be star MT91 213 orbit each other in a highly eccentric orbit with an extremely long period, with the pulsar reaching its... | [
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νGAN: A Deep Learning Emulator for Cosmic Web Simulations with Massive Neutrinos. Understanding the impact of neutrino masses on the evolution of the Universe is a central goal of modern cosmology. Due to their large free-streaming lengths, neutrinos significantly affect structure formation at nonlinear scales, requiri... | [
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Inferring Photospheric Horizontal Flows from Multiple Observations with SUVEL Models. Photospheric horizontal velocity fields play essential roles in the formation and evolution of numerous solar activities. Various methods for estimating the horizontal velocity field have been proposed in the past. Aiming at the highe... | [
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On the Estimation of Sulfuric Acid Vapor Concentrations below the Venus Cloud Deck Using the Akatsuki Radio Science Experiment. We report new constraints on the vertical distribution of sulfuric acid vapor in the Venusian atmosphere, derived from a refined analysis of radio occultation (RO) data. The method estimates t... | [
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The Observation of Ground-level Enhancement GLE 77 by the Neutron Detectors of the Experimental Complex NEVOD. A ground-level enhancement (GLE) event was observed by neutron detectors designed for the registration of extensive air showers (EASs) at the Experimental Complex (EC) NEVOD. The potential for that was unlocke... | [
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Analyzing Polycyclic Aromatic Hydrocarbons as a Tracer of Anomalous Microwave Emission near the Galactic Plane Using the COSMOGLOBE DIRBE Reduction. The physical mechanism producing anomalous microwave emission (AME) has been an unresolved puzzle for close to 30 yr. One candidate mechanism is rotational emission from p... | [
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Spin Frequency of Neutron Star in the Bright Atoll Source 4U 1705-44 Using NICER Observation. We conducted a systematic study of two thermonuclear type I X-ray bursts (B1 and B2) and the spectral properties of the bright atoll type neutron star low-mass X-ray binary 4U 1705−44 using NICER observation. In our analysis, ... | [
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A Practical Framework for Estimating the Repetition Likelihood of Fast Radio Bursts from Spectral Morphology. The repeating behavior of fast radio bursts (FRBs) is regarded as a key clue to understanding their physical origin, yet reliably distinguishing repeaters from apparent nonrepeaters with current observations re... | [
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Predicting Associations between Solar Flares and Coronal Mass Ejections Using SDO/HMI Magnetograms and a Hybrid Neural Network. Solar eruptions, including flares and coronal mass ejections (CMEs), have a significant impact on Earth. Some flares are associated with CMEs, and some flares are not. The association between ... | [
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A Compact Object with a K-type Star Companion in the Solar Neighborhood: A Wide Postcommon Envelope Binary with a White Dwarf Candidate. Post-common envelope binaries (PCEBs) consisting of a white dwarf (WD) plus a main-sequence star can constrain current prescriptions of common envelope evolution (CEE) and calibrate t... | [
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Metal Pipe: A Broadly Applicable Stellar Abundance Pipeline Using Isochronal Parameters. Characterizing exoplanet host stars at the population level requires a method of homogeneously characterizing stellar properties across all spectral types. To this end, we have developed Metal Pipe, a new code for determining stell... | [
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Constraining Nuclear Molecular Gas Content with High-resolution CO Imaging of GOALS Galaxies. We present measurements of the cool molecular gas mass around the nuclei of two gas-rich mergers, III Zw 035 and IRAS F01364−1042, whose enclosed masses (Menc) within the central 40─80 pc would be overmassive if attributed ent... | [
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A Tale of Two Dust Disks in Our Milky Way. Cosmic dust plays a vital role in stellar and galactic formation and evolution, but its three-dimensional structure in the Milky Way has remained unclear due to insufficiently precise reddening and distance measurements. Although early studies typically adopted a single-disk m... | [
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ODIN: A New Lyα Blob Selection Method, Sample, and Statistical Analysis at z ∼ 3.1. Lyα blobs (LABs) are large, spatially extended Lyα-emitting objects whose nature remains unclear. Their statistical properties, such as number densities and luminosity functions, are still uncertain because of small sample sizes and lar... | [
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A Comoving Framework for Planet Migration. The migration of planets within their nascent protoplanetary disks is a fundamental process that shapes the final architecture of planetary systems. However, studying this phenomenon through direct hydrodynamical simulations is computationally demanding, with traditional metho... | [
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An Accretion Flare Interpretation for the Ultra-high-energy Neutrino Event KM3-230213A. We study the origin of the ultra−high-energy (UHE) neutrino event KM3-230213A detected by KM3NeT, focusing on MRC 0614−083, which has been pinpointed as the closest blazar to the neutrino localization exhibiting variable multiwavele... | [
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Fraction of Energy Carried by Coherent Structures in the Turbulent Cascade in the Solar Wind. Turbulence is prevalent in astrophysical plasma flows. Both wave─wave interactions and coherent structures offer mechanisms to mediate turbulent cascades. Solar Orbiter in situ satellite observations of plasma turbulence in th... | [
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SN 2024afav: A Superluminous Supernova with Multiple Light-curve Bumps and Spectroscopic Signatures of Circumstellar Interaction. We present a comprehensive optical and near-infrared (NIR) spectroscopic study of SN 2024afav, a hydrogen-poor superluminous supernova (SLSN-I) that peaks at ≍−20.7 mag and exhibits an unusu... | [
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Evolutionary Tracks and Spectral Properties of Quasi-stars and Their Correlation with Little Red Dots. JWST has revealed a population of red, compact, high-redshift (z ∼ 3─10) objects referred to as "Little Red Dots" (LRDs). These objects exhibit unusual spectral features reminiscent of stellar spectra with blackbody-l... | [
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Intruder Alert: Breaking Resonant Chains with Planetesimal Flybys. The orbital architectures of compact "Kepler-multi" (KM) exoplanet systems record their complicated dynamical histories. The "breaking-the-chains" hypothesis proposes that compact systems typically form in chains of mean-motion resonances and subsequent... | [
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Discovery of a Dwarf Planet Candidate in an Extremely Wide Orbit: 2017 OF201. We report the discovery of a dwarf planet candidate, 2017 OF201, currently located at a distance of 90 au. Its orbit is extremely wide and extends to the inner Oort cloud, with a semimajor axis of 830 au and a perihelion of 45 au, precisely d... | [
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Molecular Hydrogen Controls the Temperatures of Flares on TRAPPIST-1. Early JWST observations of TRAPPIST-1 have revealed an unexpected puzzle: energetic white-light flares (E > 1030 erg) reach temperatures of only ∼3500─4000 K, nearly 3 times cooler than typical solar flares, which peak around 9000─10,000 K. Here w... | [
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Ancient Relic Moderately Metal-rich Bulge Cluster Tonantzintla 2. The assembly history of the Galactic bulge is intimately tied to the formation of the proto─Milky Way, yet reconstructing this early phase is difficult because mergers and secular evolution have erased most of its original structure. Among present-day st... | [
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The Effect of a Nonuniversal Extinction Curve on the Wesenheit Function and Cepheid Distances. The Wesenheit function is widely used to reduce the effects of interstellar reddening in distance measurements. Its construction, however, relies on the assumption of a universal extinction curve and on fixed values of the to... | [
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Type IIb Supernova Progenitors in 3D: Variability and Episodic Mass Loss Revealed by Radiation Hydrodynamics Simulations. We present the first 3D radiation hydrodynamics simulations of partially stripped ( Mcore∼10M⊙ , Menv ∼ 0.1─1M⊙) yellow supergiant (L ∼ 105L⊙, Teff ≍ 5000─8000 K) envelopes, constructed with Athena+... | [
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The NANOGrav 15 yr Dataset: Targeted Searches for Supermassive Black Hole Binaries. We present the first targeted searches for continuous gravitational waves (CWs) from 114 active galactic nuclei that may host supermassive black hole binaries, using the NANOGrav 15 yr dataset. By incorporating electromagnetic priors on... | [
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The Maximum Particle Energy Gain during Magnetic Reconnection. The factors that control the maximum energy attained by protons and electrons during magnetic reconnection are investigated analytically and using large-scale simulations with the kglobal model. Previous work revealed that a strong ambient guide field stron... | [
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A Global View of Jupiter's Upper Atmosphere Through H<inline-formula> <mml:math><mml:msubsup><mml:mrow></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>. Planetary upper atmospheres couple the deep atmosphere to the space environment. Th... | [
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Surprisingly Similar: The Mass Function of Gaia Neutron Stars and Firstborn Double Neutron Stars. The mass distribution of neutron stars (NSs) encodes information about their formation and binary evolution. We compare the masses of two distinct populations: (I) the recently identified Gaia NSs in wide orbits with solar... | [
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Secular Evolution of PSR J2021+4026: Long-term γ-Ray Flux and Spin-down Variability beyond State Transitions. PSR J2021+4026 is a remarkable γ-ray pulsar exhibiting repeated transitions between high γ-ray flux (HGF) and low γ-ray flux (LGF) states. With 17 yr Fermi Large Area Telescope monitoring, we reveal persistent ... | [
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A 2 au Resolution View by ALMA of the Planet-hosting WISPIT 2 Disk. We present deep, high-spatial-resolution interferometric observations of 0.88 mm continuum emission from the TYC 5709-354-1 system, hereafter WISPIT 2, obtained with the goal of detecting circumplanetary emission in the vicinity of the newly discovered... | [
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Water Production of Interstellar Comet 3I/ATLAS from SOHO/SWAN Observations after Perihelion. The Solar Wind Anisotropies all-sky hydrogen Lyman-alpha camera on the Solar and Heliosphere Observatory observed the hydrogen coma of interstellar comet 3I/ATLAS, also called C/2025 N1 (ATLAS), beginning on 2025 November 6, 9... | [
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Bridging Scales: How Much Do Supermassive Black Holes Grow in the Suppressed Bondi Regime?. The coevolution of supermassive black holes (SMBHs) and their host galaxies remains one of the central open questions in cosmology, rooted in the coupling between accretion, feedback, and the multiscale physics that links the ev... | [
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On Schur Decomposition of Magnetic and Velocity Gradient Tensors in Space Plasma Turbulence. The study of the statistics of gradient tensors' invariants is useful to characterize the morphological/topological features of magnetic flux and plasma velocity flow lines in turbulent space plasmas. In the recent past, some s... | [
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Reexamining Evidence of a Pair-instability Mass Gap in the Binary Black Hole Population. The fourth Gravitational-Wave Transient Catalog (GWTC-4) has enabled empirical probes of the theorized pair-instability gap in the higher end of the binary black hole (BBH) mass spectrum. In this Letter, using flexibly parameterize... | [
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Brightest Gamma-Ray-burst Flare Observed in GRB 221009A: Bridging the Last Gap between the Prompt Emission and Flare in Gamma-Ray Bursts. Flares are usually observed during the afterglow phases of Gamma-ray bursts (GRBs) in the soft-X-ray, optical, and radio bands—but rarely in the gamma-ray band. Despite its extraordi... | [
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Perihelion Asymmetry in the Water Production Rate of the Interstellar Object 3I/ATLAS. 3I/ATLAS is an interstellar object whose activity provides critical insights into its composition and origin. However, due to its orbital geometry, the object is too close to the Sun near perihelion to be observed from the ground, an... | [
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Molecular Gas Morphological Analogs for the Milky Way. Complete catalogs of molecular clouds in the Milky Way allow analysis of the molecular medium and the star formation properties of the Milky Way that closely follows the method used for nearby galaxies. We explore whether the big dip in the radial distribution of m... | [
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"http://astrothesaurus.org/uat/622",
"http://astrothesaurus.org/uat/834"
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"http://astrothesaurus.org/uat/1569",
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A Possible "Too-many-satellites" Problem in the Isolated Dwarf Galaxy DDO 161. The abundance of satellite galaxies provides a direct test of ΛCDM and galaxy formation physics on small scales. While satellites of Milky Way-mass galaxies are well studied, those of dwarf galaxies remain largely unexplored. We present a sy... | [
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"http://astrothesaurus.org/uat/416",
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An Unexpected Population of Quenched Galaxies Harboring Undermassive SMBHs Revealed by Tidal Disruption Events. Restricted by event horizon suppression, tidal disruption events (TDEs) provide a unique window into otherwise hidden supermassive black holes (SMBHs) at the lower end of the mass spectrum, allowing the conne... | [
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"http://astrothesaurus.org/uat/1851",
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"http://astrothesaurus.org/uat/1696",
"http://astrothesaurus.org/uat/2016",
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WHALES. The Weighing Halos Accurately, Locally, and Efficiently with Supernovae Survey: Overview and Initial Data Release. We present an overview of the Weighing Halos Accurately, Locally, and Efficiently with Supernovae (WHALES) survey, the first to discover and measure Type Ia supernovae (SNe Ia) in and around galaxy... | [
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"http://astrothesaurus.org/uat/1657",
"http://astrothesaurus.org/uat/1668",
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JWST Confirmation of a Runaway Supermassive Black Hole via Its Supersonic Bow Shock. We present JWST/NIRSpec integral field unit observations of a candidate runaway supermassive black hole (SMBH) at the tip of a 62 kpc long linear feature at z = 0.96. The JWST data show a sharp kinematic discontinuity at the tip, with ... | [
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Stereoscopic Observations of Solar X-Ray Sources Explained by a Data-constrained Magnetohydrodynamic Simulation. We investigated the three-dimensional (3D) magnetic structures and dynamics responsible for particle acceleration in an X7.1-class flare that occurred on 2024 October 1, in NOAA active region 13842. We combi... | [
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Testing the Association of Supermassive Black Hole Infrared Flares and High-energy Neutrinos. The physical origin of the observed cosmic neutrinos remains an open question and the subject of active research. While matter accretion onto supermassive black holes is long thought to accelerate particles to high energies, i... | [
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Preperihelion CN Production Rate of Interstellar Comet 3I/ATLAS. We present spectroscopic observations of the third interstellar comet 3I/ATLAS obtained with the DOLORES instrument on the 3.58 m Telescopio Nazionale Galileo on 2025 August 16 (rh = 2.98 au). The spectrum revealed a red slope of 12.68% ± 0.05%/1000 Å acr... | [
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Hubble's Multiyear Search for Exospheres in the TRAPPIST-1 System Reveals Frequent Microflares. Lyα observations provide a powerful probe of stellar activity and atmospheric escape in exoplanetary systems. We present here an analysis of 109 Hubble Space Telescope (HST)/Space Telescope Imaging Spectrograph (STIS) orbits... | [
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Evidence of Feedback Effects in Low-luminosity Active Galactic Nuclei Revealed by JWST Spectroscopy. This Letter presents an analysis of the infrared (∼3─28 μm) spectra extracted from the nuclear (r < 150 pc) regions of four low-luminosity active galactic nuclei (AGN), observed by JWST NIRSpec/integral field unit an... | [
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Variations in the Milky Way's Stellar Mass Function at [Fe/H] < −1. We present the first determination of the Galactic stellar mass function (MF) for low-mass stars (0.2─0.5 M⊙) at metallicities [Fe/H] ≲ −1. A sample of ∼53,000 stars was selected as metal-poor on the basis of both their halolike orbits and their spe... | [
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Meteorite Radioisotope Ages Reveal Late Dynamical Chaos in the Solar System. The orbital elements of the solar system's ancient asteroid families are highly dispersed, recording the last dynamical chaos in its history. However, dynamics alone cannot precisely date this when this terminal chaos occurred. Instead, we can... | [
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Lack of Detailed Balance at Sub-ion Scales in Turbulent Solar Wind. A notable feature of turbulence in solar wind is the presence of an additional power-law spectral domain at scales below the ion inertial length. This spectral domain has been attributed to a distinct turbulent regime involving alternative wave modes. ... | [
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ALMA and JWST Identification of Faint Dusty Star-forming Galaxies up to z ∼ 8 and Their Connection with Other Galaxy Populations. We exploit a new sample of around 400 bright dusty galaxies from the Atacama Large Millimeter/submillimeter Array (ALMA) CHAMPS Large Program, together with the rich JWST multiband data prod... | [
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"http://astrothesaurus.org/uat/1671",
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The Strong Fe K Line and Spin of the Black Hole X-Ray Binary MAXI J1631─479. We study the transient black hole binary MAXI J1631─479 observed simultaneously by NICER and NuSTAR in its soft spectral state. Its puzzling feature is the presence of a strong and broad Fe K line, while the continuum includes a prominent disk... | [
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A Super-Eddington, Lensing-magnified Quasar at z = 5.07 Observed with JWST. We present JWST/NIRCam F070W and F480M imaging for a quasar at z = 5.07, J0025─0145, which is magnified by a foreground lensing galaxy. Existing Hubble Space Telescope (HST) imaging does not have sufficient spatial resolution to determine wheth... | [
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"http://astrothesaurus.org/uat/2129",
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Reanalysis of the Eclipses of LHS 1140 c: No Evidence of an Atmosphere and Implications for the Internal Structure of the Planet. We present a reanalysis of three 15 μm JWST/MIRI secondary eclipses of LHS 1140 c, a warm super-Earth (Rp = 1.272 R⊕) in a 3.78 day orbit around an M4.5 dwarf. We present a novel method for ... | [
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"http://astrothesaurus.org/uat/1858",
"http://astrothesaurus.org/uat/486",
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"http://astrothesaurus.org/uat/1577",
"http://astrothesaurus.org/uat/1655",
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