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Photo: Moon and Jupiter over the small dome
Moon and Jupiter over the small dome
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 News from astronomynow.com
› Binoculars to boost your night-sky viewing
› Lyra’s stunning smoke ring – M57
› Is the Hubble Tension Resolved?
› Universe’s end – sooner rather than later
› Caught in the current of the wonderful Whirlpool
› A faint star will reveal itself as it throws a hissy-fit
› Saturn’s Rings to “Disappear”
› The Lithium Problem
› Discover the many fascinating moons of our Solar System
› A bigger and better helicopter to Mars
RSS  Latest preprints on astro-ph:
› Exploring the parameter space of hierarchical triple black hole systems
› Are Helium Atmospheres Hiding as Volatile-rich in Current Exoplanet Analysis Frameworks?
› A systematic search for dormant galaxies at z~5-7 from the JWST NIRSpec archive
› Bahamas: BAyesian inference with HAmiltonian Montecarlo for Astrophysical Stochastic background
› Simulation-based population inference of LISA's Galactic binaries: Bypassing the global fit
› MOSDEF-3D: Keck/OSIRIS Maps of the Ionized ISM in $z \sim 2$ Galaxies
› Multimessenger Emission from Very-High-Energy Black Hole-Jet Systems in the Milky Way
› Implications for dark energy of cosmic transparency in light of DESI data
› On beam characterization of ground-based CMB radio telescopes using UAV-mounted sources: application to the QUIJOTE TFGI and plans for LSPE-Strip
› Ultrahigh Energy Cosmic Ray Production in Binary Neutron Star Mergers
› Kilonova constraints for the LIGO/Virgo/KAGRA neutron star merger candidate S250206dm: GW-MMADS observations
› The model fitting of Gaia DR3 Classical Cepheid light and radial velocity curves
› DeepDive: A deep dive into the physics of the first massive quiescent galaxies in the Universe
› Blending effects on shear measurement synergy between Euclid-like and LSST-like surveys
› Double Compact Binary Merger Rate Density in Open Star Clusters: Black Holes, Neutron Stars, and White Dwarfs
› First results from the UTMOST-NS pulsar timing programme
› The diffuse supernova neutrino background: a modern approach
› Exploring the signature of assembly bias and modified gravity using small-scale clusterings of galaxies
› Polar alignment of a circumbinary disc around a brown dwarf binary
› A dynamical coherency gate for state recovery: Statistical requiem for the long arc of cislunar orbital mis-prediction
› Meridional Movements of Individual Sunspots and Pores
› Timing results of 22 years for PSR J0922+0638
› Bayesian constraints on quark and neutron stars from multi-messenger observations
› Observed Anti-parallel Correlation Between Spiral Galaxy and Cosmic Filament Spins
› Examining statistical isotropy of CMB low multipoles from Planck PR4 data
› Probing foreground residuals in cleaned CMB temperature maps from Planck
› Probing Binary Neutron Star Merger Ejecta and Remnants with Gravitational Wave and Radio Observations
› Characterizing the Dynamics and Chemistry of Transiting Exoplanets with the Habitable World Observatory
› The effectively optically thin accretion flow and its implication in supermassive black holes
› A Comprehensive Statistical Study of Gamma-Ray Bursts and Supernovae Association
› Braking index of the frequently glitching PSR J0537$-$6910
› Reconstructing dark energy with model independent methods after DESI DR2 BAO
› XRISM View of the Newly Detected Galactic Source MAXI J1744-294
› Resolving the negative neutrino mass with cosmic birefringence
› Effects of Large Optical Depth on CD HI 21-cm Non-Gaussian Signal
› ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter
› The most massive star clusters in molecular clouds: Insights from the integrated cloud-wide initial mass function (ICIMF) theory
› How Do Ionizing Photons Escape from Star-Forming Galaxies?
› Correlation between H$\alpha$ emitters and their cosmic web environment at $z \sim 1$
› Unveiling the Nature and Fate of the Almost-Dark Cloud AGC 226178 through HI Mapping
› Deep survey of millimeter RRLs towards the planetary nebulae IC 418 and NGC 7027
› A systematic bias in template-based RV extraction algorithms
› BASIL: Fast broadband line-rich spectral-cube fitting and image visualization via Bayesian quadrature
› On the origin of short-lived cocoon in 3C84: powered by tidal disruption events ?
› On inertial forces (indirect terms) in problems with a central body
› Ultra High Energy Neutrino Event KM3-230213A as a Signal of Electroweak Vacuum Turbulence in Merging Black Hole Binaries
› An investigation into correlations between FRB and host galaxy properties
› Uncover 3D Dark Matter Distribution of the Milky Way by an Empirical Triaxial Orbit-Superposition Model: Method Validation
› Probing the detectability of electromagnetic signatures from Galactic isolated black holes
› Search for Higher Harmonic Signals from Close White Dwarf Binaries in the mHz Band
› Thermal Inertia Controls on Titan's Surface Temperature and Planetary Boundary Layer Structure
› What Prevents Resolving the Hubble Tension through Late-Time Expansion Modifications?
› Acceleration and Transport of the Unstable Cosmic-ray Isotope $^{60}$Fe in Supernova-Enriched Environments
› On the validity of separate-universe approach in transient ultra-slow-roll inflation
› Evolutionary Map of the Universe: Detection and Analysis of the Shell Surrounding the Runaway Wolf-Rayet Star WR16
› The hydrodynamic thermal continuum, with applications to stratified atmospheres and 1D coronal loop models
› Unveiling supermassive black hole binaries with FUV-to-NIR spectropolarimetry
› Multiscale Turbulence Synthesis: Validation in 2D Hydrodynamics
› Even Redder than we Knew: Color and $A_{\mathrm{V}}$ Evolution up to $z=2.5$ from JWST/NIRCam Photometry
› Multi-Model Framework for Reconstructing Gamma-Ray Burst Light Curves
› Is convective turbulence the only exciting mechanism of global p modes in the Sun?
› Measuring the Suns radial velocity variability due to supergranulation over a magnetic cycle
› Studying the multi-phase interstellar medium in the Large Magellanic Cloud with SRG/eROSITA -- I. Analysis of diffuse X-ray emission
› The NEID Earth Twin Survey. III. Survey Performance After Three Years on Sky
› Macroscopic states in Bose-Einstein condensate dark matter model with axionlike interaction
› Simulation of images of protoplanetary disks after collision with free-floating planets
› Scalar-induced gravitational waves from coherent initial states
› Enhanced Thermodynamic Framework for Third-Order Galaxy Correlation Functions: From Theory to Observations
› Constraining the Origin of FRB 20121102A's Persistent Radio Source with Long-Term Radio Observations
› Spectropolarimetric synthesis of forbidden lines in MHD models of coronal bright points
› Modeling blazar broadband emission with convolutional neural networks -- III. proton synchrotron and hybrid models
› Avalanching together: A model for sympathetic flaring
› Three-dimensional Transport-induced Chemistry on Temperate sub-Neptune K2-18b, Part I: the Effects of Atmospheric Dynamics
› Continuum optical-UV and X-ray variability of AGN: current results and future challenges
› Exploring the Wolf Approach to Constraining NIR Extinction Laws in the Corona Australis Molecular Cloud
› A possible two-fold scenario for the disc-corona of the luminous AGN 1H 0419--577: a high-density disc or a warm corona
› Sagittarius A* near-infrared flares polarization as a probe of space-time I: Non-rotating exotic compact objects
› Variability-finding in Rubin Data Preview 1 with LSDB
› High-precision polarization measurements with Lumped Element Kinetic Inductance Detectors
› Line-of-sight acceleration as a test of the Galactic Yukawa potential
› A planet-host ratio relation to synthesize microlensing and transiting exoplanet demography from Roman
› Anchoring Stellar Age Indicators: A Cross-Calibration of [C/N] and Gyrochronology Ages via the Age-Velocity-Dispersion Relation
› Listening Across the Cosmic Time: Standard Sirens from Ground- and Space-Based Missions in the Next Decade
› EMPRESS. XV. A New Determination of the Primordial Helium Abundance Suggesting a Moderately Low $Y_\mathrm{P}$ Value
› Recurring region for neutron-star observables
› The distribution of metals in simulated Milky Way-mass galaxies
› Tidal Inflation is Stronger for Misaligned Neptune-Sized Planets Than Aligned Ones
› Constraining self-interacting ultrahigh-energy neutrinos by cosmic microwave background spectral distortion
› Beneath the Surface: >85% of z>5.9 QSOs in Massive Host Galaxies are UV-Faint
› Studying Protoplanets and Protoplanetary Disks with the Habitable Worlds Observatory
› Constraining Cubic Curvature Corrections to General Relativity with Quasi-Periodic Oscillations
› Assisted Fibre Inflation in Perturbative LVS
› Dark Matter Induced Neutron Production Search Limits
› Projective Transformations for Regularized Central Force Dynamics: Hamiltonian Formulation
› Optical appearance of Schwarzschild black holes with optically thin and thick accretion disks at various inclination angles
› A unified origin for dark energy and resonant dark matter from strongly-coupled gauge theory
› Generating Moving Field Initial Conditions with Spatially Varying Boost
› Satellite telescope of electrons and protons STEP-F of the space scientific project "CORONAS-Photon"
› Running scalar spectral index in warm natural inflation
› From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data
› Searching for quasinormal modes from Binary Black Hole mergers
› Significance of soft-scale breaking on primordial black hole production in Coleman-Weinberg type supercooling-phase transition
› Superconducting Ring Resonators: Modelling, Simulation, and Experimental Characterisation
› The Lifespan of our Universe
› Cosmic Axions Revealed via Amplified Modulation of Ellipticity of Laser (CARAMEL)
› (SHERRY) JCMT-SCUBA2 High Redshift Bright Quasar Survey -- II: the environment of z~6 quasars in sub-millimeter band
› Spatially Resolved Properties of Extraplanar Diffuse Ionized Gas in NGC$\,$3511 and NGC$\,$3513
› Dark Matter Fraction in Disk-Like Galaxies Over the Past 10 Gyr
› Initial Results From the First Field Expedition of UAPx to Study Unidentified Anomalous Phenomena
› On the Physical Nature of Ly$\alpha$ Transmission Spikes in High Redshift Quasar Spectra
› Chronicling the reionization history at $6\lesssim z \lesssim 7$ with emergent quasar damping wings
› Fractal dimension of star clusters
› A hierarchical Bayesian approach to point source analysis in high-energy neutrino telescopes
› Two-Component gamma-ray Emission Spectrum and X-Ray Polarization of the Radio Galaxy Pictor A
› Characterisation of local halo building blocks: Thamnos and Sequoia
› Stellar reddening map from DESI imaging and spectroscopy
› The JWST Emission Line Survey (JELS): Extending rest-optical narrow-band emission line selection into the Epoch of Reionization
› The JWST Emission Line Survey (JELS): An untargeted search for H$\alpha$ emission line galaxies at $z > 6$ and their physical properties
› Investigating the Origin of CMB Large-Scale Features Using LiteBIRD and CMB-S4
› Machine Learning Approach for Estimating Magnetic Field Strength in Galaxy Clusters from Synchrotron Emission
› Velocity evolution of broad-lined type-Ic supernovae with and without gamma-ray bursts
› A Hybrid Scheme for Fuzzy Dark Matter Simulations Combining the Schr\"odinger and Hamilton-Jacobi-Madelung Equations
› Exploring the anisotropic gravitational wave background from all-sky mock gravitational wave event catalogues
› Using t-SNE for characterizing glitches in LIGO detectors
› Protostellar disc structure and dynamics during star formation from cloud-scale initial conditions
› Impact of particle production during inflation on the CMB detection
› Revealing the $\chi_{\rm eff}$-$q$ correlation among Coalescing Binary Black Holes and { Tentative} Evidence for AGN-driven Hierarchical Mergers
› Tuning the cosmic instrument: robust cosmology through combined probes
› Accounting for motion of supernova host galaxy in statistical inference from SNIa data
› Spectroastrometry and Reverberation Mapping of Active Galactic Nuclei. II. Measuring Geometric Distances and Black Hole Masses of Four Nearby Quasars
› MaNGA AGN dwarf galaxies (MAD). III. The role of mergers and environment in active galactic nucleus activity in dwarf galaxies
› Computing Anharmonic Infrared Spectra of Polycyclic Aromatic Hydrocarbons Using Machine-Learning Molecular Dynamics
› Comparison of Bar Formation Mechanisms. II. Does a Tidally Induced Bar Grow Faster Than an Internally Developed Bar?
› Consistencies and inconsistencies in redshift-independent distances
› DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest
› Neutrino emission and corona heating induced by high-energy proton interactions in Seyfert galaxies
› Effects of Environment on the Size Evolution of Quiescent Galaxies: Comparing Galaxies in Clusters and in the Field at Two Rest-frame Wavelengths
› Group Accretion in Milky Way-like Stellar Haloes
› Evidence for Large-Scale Cold Gas Outflows Associated with Nuclear Winds in Reionization-Era Quasars
› CAMPOS II. The onset of protostellar disk substructures and planet formation
› Improving CMB constraints on early Universe physics with LSS: A multi-probe forecast including cross-covariance
› Mock Observations: Morphological Analysis of Galaxies in TNG100 Simulations
› An interferometric study of B star multiplicity
› Revealing the nature of ultra-long period objects with space-based gravitational-wave interferometers
› NuSTAR Detection of an Absorption Feature in ESP 39607: Evidence for an Ultra-Fast Inflow?
› Distribution of Dark Matter in Galaxies
› Influence of Dark Matter on the Formation of Biogenic Elements in Early Universe Stars
› Understanding gas mixing in the circumgalactic medium
› The Intracluster Light of Abell 3667: Unveiling an Optical Bridge in LSST Precursor Data
› Impact of convective overshooting on the single-degenerate model of Type Ia supernovae
› Accurately simulating core-collapse self-interacting dark matter halos
› To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation
› Properties of $\mathrm{H_2O}$ masers and their associated sources in Sagittarius B2
› X-ray investigation of the remarkable galaxy group Nest200047
› What new physics can we extract from inflation using the ACT DR6 and DESI DR2 Observations?
› Detailed Chemical Abundance Analysis of Metal-Poor Turn-Off Stars: One with [Fe/H] < -4 and Three with [Fe/H] < -3
› Birthplaces of X-ray emission lines in Cygnus X-3
› Probing Solar Polar Regions
› Stable dark matter from Pauli blocking in the degenerate fermion background with Quantum Field Theory
› Quasilocal Newtonian limit of general relativity and galactic dynamics
› Stable massless scalar polarization of f(R) gravity
› Quasinormal mode frequencies and gravitational perturbations of spinning black holes in modified gravity through METRICS: The dynamical Chern-Simons gravity case
› How Much NEC Breaking Can the Universe Endure?
› Quasinormal modes and absorption cross-section of a Bardeen black hole surrounded by perfect fluid dark matter in four dimensions
› Jupiter's ultraviolet auroral bridge: the influence of the solar wind on polar auroral morphology
› On the Dark-Energy Enigma

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