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 News from astronomynow.com

› Astronomy Now under new ownership
› 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
RSS  Latest preprints on astro-ph:

› On the Image Profiles of Transients in the Palomar Sky Survey
› A Generative Model for Disentangling Galaxy Photometric Parameters
› Physical parameter regression from black hole images via a multiscale adaptive neural network
› The VISCACHA Survey: XIII. The extended main-sequence turn-off in intermediate-age low-mass clusters
› oLIMpus: An Effective Model for Line Intensity Mapping Auto- and Cross- Power Spectra in Cosmic Dawn and Reionization
› Hidden binaries in star-forming regions
› A Late-time Radio Search for Highly Off-axis Jets from PTF Broad-lined Ic Supernovae in GRB-like Host Galaxy Environments
› Orbital and Physical Properties of the Pleiades Binary 27 Tau (Atlas)
› Converging on the Cepheid Metallicity Dependence: Implications of Non-Standard Gaia Parallax Recalibration on Distance Measures
› GRB 241105A: A test case for GRB classification and rapid r-process nucleosynthesis channels
› The HETDEX Survey: Probing neutral hydrogen in the circumgalactic medium of ~88,000 Lyman Alpha Emitters
› Measuring and modelling the Splash with APOGEE/Gaia and ARTEMIS
› Carbon burning cannot explain puffy hypervelocity white dwarfs
› A Semi-Empirical Estimate of Solar EUV Evolution from 10 Myr to 10 Gyr
› Stellar evolution through the Red Supergiant phase
› The Red and Yellow Hypergiants
› Host galaxy identification of LOFAR sources in the Euclid Deep Field North
› Red Supergiants in the Milky Way and Nearby Galaxies
› Red Supergiants -- The Other Side of the H-R Diagram
› Betelgeuse, the Prototypical Red Supergiant
› Resolving Black Hole Family Issues Among the Massive Ancestors of Very High-Spin Gravitational-Wave Events Like GW231123
› Molecules and Chemistry in Red Supergiants
› Red Supergiant Mass Loss and Mass-Loss Rates
› Red Supergiants as Supernova Progenitors
› Relativistic X-ray reflection and thermonuclear burst from accreting millisecond X-ray pulsar SRGA J144459.2-604207
› Double-offset Cassegrain telescopes for the Ultraviolet Type Ia (UVIa) mission concept
› Prospects for GeV Neutrino Transient Searches with the IceCube Upgrade
› Interplanetary magnetic correlation and low-frequency spectrum over many solar rotations
› Building Earth with pebbles made of chondritic components
› Applying multimodal learning to Classify transient Detections Early (AppleCiDEr) I: Data set, methods, and infrastructure
› The project of a ground-based wide-angle EAS Cherenkov light imaging detector for PCR mass composition study in the 1-1000 PeV energy range
› Testing gravitational physics by combining DESI DR1 and weak lensing datasets using the E_G estimator
› Extensive Air Shower Registration at Two Depths with SPHERE-3 Detector
› The results of the development of the SPHERE-3 detector for studying the PCR mass composition in the 1-1000 PeV energy range. The status of 2025
› Dissecting Reionisation with the Cosmic Star Formation and AGN Luminosity History
› Simba Simulation: The Effect of Feedback Physics on Matter Distribution in the Cosmic Web
› Waiting Time Distribution of Supra-Arcade Downflows
› A Comprehensive Analysis of Rovibrational CO in the Era of JWST
› Central Concentration and Escape of Ionizing Photons in Galaxies at the Epoch of Reionization
› The VISCACHA survey XIV. Chemical evolution history of the SMC: The Southern Bridge Clusters
› Observational constraints on phenomenological emergent dark energy and barotropic dark matter characterized by a constant equation of state parameter
› Ionized gas in NGC 4258: Exploring the AGN -- Star formation connection
› An AI super-resolution field emulator for cosmological hydrodynamics: the Lyman-{\alpha} forest
› Can GRB Empirical Correlations Be Used for Population Studies?
› TOI-880 is an Aligned, Coplanar, Multi-planet System
› Galaxy Evolution in the Local Universe: Group Richness Effects on Mergers and Non-Mergers
› Early-type Galaxies on the Star Formation Main Sequence: Internal Star Formation Geometry Revealed with MaNGA and Their Environmental Origin
› The mass of TOI-654 b: A short-period sub-Neptune transiting a mid-M dwarf
› Ly$\alpha$ Emission from [OIII] Emitters Near Reionization: The role of environment in galaxy Ly$\alpha$ detection
› Observations of microwave emission from solar jets and comparison with MHD simulations
› The THESAN project: environmental drivers of Local Group reionization
› Understanding the magnetic field and plasma-$\beta$ along umbral fan loops traced using 3-min slow waves
› Challan: Solar Full-disk Imaging-Spectroscopic Telescope using the Drift-Scanning Technique
› ANTIHEROES-PRODIGE: Quantifying the connection from envelope to disk with the IRAM 30m telescope and NOEMA I. Attack of the streamers: L1448N's fight for order in the chaos
› Investigating Interacting Dark Energy Models Using Fast Radio Burst Observations
› Lunar Orbital VLBI Experiment: motivation, scientific purposes and status
› Deep Chandra X-ray observation of the isolated black hole OGLE-2011-BLG-0462
› A Unified Volumetric Rate-Energy Relation from Magnetar Radio Bursts to Fast Radio Bursts
› The Large Magellanic Cloud as a source of the highest energy cosmic rays
› Recent advances on multimessenger astrophysics: Centaurus A, GW 170817, and KM3-230213A
› Observation of VER J2019+368 with the SST-1M stereoscopic system
› Sometimes they come back: pulsations in A 0538-66 at 69 ms rediscovered with NICER
› Modelling gyrosynchrotron emission from coronal energetic electrons in a CME flux rope
› The effect of stellar magnetic activity on measurements of morning and evening asymmetry of planetary terminator
› Fast magneto-acoustic waves in the solar chromosphere: Comparison of single-fluid and two-fluid approximations
› Intra-night optical variability and radio characteristics of extremely radio-loud narrow-line Seyfert 1 galaxies
› The SST-1M stereoscopic system
› Very-high-energy observations of the Seyfert galaxy NGC 4151 with MAGIC -- Indication of another gamma-ray obscured candidate neutrino source
› A $6.37\,{\rm Hz}$ quasi-periodic oscillating photospheric emission in GRB~240825A
› Exploring the properties of newborn pulsars with high-energy neutrinos
› Low D/H ratio for benzonitrile in TMC-1: Implication for the origin of polycyclic aromatic hydrocarbons in cold dark clouds
› Cosmological Preference for a Positive Neutrino Mass at 2.7$\sigma$: A Joint Analysis of DESI DR2, DESY5, and DESY1 Data
› Inference of matter power spectrum at z=0 using DESI DR1 Full-Shape data
› The Event Rate and Luminosity Function of Fermi/GBM Gamma-Ray Bursts
› Forecast constraints on null tests of the $\Lambda$CDM model with SPHEREx
› The gravitational potential of spiral perturbations. I the 2D (razor-thin) case
› Stereo performance of SST-1M at different altitudes
› Assessing robustness and bias in 1D retrievals of 3D Global Circulation Models at high spectral resolution: a WASP-76 b simulation case study in emission
› The GHOSDT Simulations: II. Missing Molecules in Simulations of a Self-Regulated Interstellar Medium
› Simulating realistic Lyman-$\alpha$ emitting galaxies including the effect of radiative transfer
› Planck constraints on the scale dependence of isotropic cosmic birefringence
› Hybrid concept of detection for a wide-field gamma-ray observatory using Cherenkov telescopes
› Weinberg's theorem, phantom crossing and screening
› Considering contact forces during the formation of planetesimals by gravitational collapse: mutual orbits, spin states, and shapes
› Artifacts in Halo Shapes: Imprints of the Initial Condition
› A double-degenerate scenario with a merger to explosion delay time to explain type Ia supernova SN 2020aeuh
› Discovery of SiC and Iron Dust Around AGB Stars in the very Metal-Poor Sextans A Dwarf Galaxy with JWST: Implications for Dust Production at High Redshift
› The SOFIA Massive (SOMA) Radio Survey. II. Radio Emission from High-Luminosity Protostars
› Silicate mineralogy and bulk composition of exoplanetary material in polluted white dwarfs
› Primordial black holes with anisotropic hair
› Stellar Mass-Dispersion Measure Correlations Constrain Baryonic Feedback in Fast Radio Burst Host Galaxies
› Mixture-of-Expert Variational Autoencoders for Cross-Modality Embedding of Type Ia Supernova Data
› Weyl-invariant Einstein-Cartan gravity with a heavy ALP: Higgs Inflation and $\alpha$-attractors
› Probing displaced (dark)photons from low reheating freeze-in at the LHC
› Wino and Real Minimal Dark Matter Excluded by Fermi Gamma-Ray Observations
› Testing Real WIMPs with CTAO
› Distinguishing Neutron Star vs. Low-Mass Black Hole Binaries with Postmerger Gravitational Waves $-$ Sensitivity to Transmuted Black Holes and Non-Annihilating Dark Matter
› Sub-GeV Dark Matter Under Pressure from Direct Detection
› dot-PE: Sampler-free gravitational wave inference using matrix multiplication
› ARTEMIS observations of electrostatic shocks inside the lunar wake
› Probing Double-Peaked Gamma-Ray Spectra from Primordial Black Holes with Next-Generation Gamma-Ray Experiments
› Split supersymmetry and hybrid inflation in light of Atacama Cosmology Telescope DR6 data
› Towards a theory of coupled sociopolitical events-planetary boundaries, crises, policrisis and Earth System syndromes
› Impact of cavities on the detection of quadratically coupled ultra-light dark matter
› Dark matter explanations for the neutrino emission from the Seyfert galaxy NGC 1068
› Multiple ALPs and enhanced echoes
› Gravitational Wave Scattering on Magnetic Fields
› Alpha clustering in warm and dense nuclear matter from heavy-ion collisions
› Cosmology with a Non-minimally Coupled Dark Matter Fluid I. Background Evolution
› Multi-field TDiff theories: the mixed regime case
› Evidence for Extended Hydrogen-Poor CSM in the Three-Peaked Light Curve of Stripped Envelope Ib Supernova
› JWST/MIRI reveals the true number density of massive galaxies in the early Universe
› Multi-Zone Modeling of Black Hole Accretion and Feedback in 3D GRMHD: Bridging Vast Spatial and Temporal Scales
› LIGO Detector Characterization in the first half of the fourth Observing run
› Kinetic simulations of the cosmic ray pressure anisotropy instability: cosmic ray scattering rate in the saturated state
› Impact of Low ell's on Large Scale Structure Anomalies
› Exploring the interaction between the MW and LMC with a large sample of blue horizontal branch stars from the DESI survey
› Reconciling PTA and JWST and preparing for LISA with POMPOCO: a Parametrisation Of the Massive black hole POpulation for Comparison to Observations
› A Novel Bispectrum Estimator of the Kinematic Sunyaev-Zel'dovich Effect using Projected Fields
› Can decaying vacuum solve the H_0 Tension?
› Euclid: Early Release Observations of diffuse stellar structures and globular clusters as probes of the mass assembly of galaxies in the Dorado group
› The Local Galactic Transient Survey Applied to an Optical Search for Directed Intelligence
› The Type Ia Supernova and AGB-Regulated Interstellar Medium of Massive Galaxies
› Nuclear Neural Networks: Emulating Late Burning Stages in Core Collapse Supernova Progenitors
› The effects of projection on measuring the splashback feature
› What's the matter with $\Sigma m_{\nu}$?
› The rise of the galactic empire: luminosity functions at $z\sim17$ and $z\sim25$ estimated with the MIDIS$+$NGDEEP ultra-deep JWST/NIRCam dataset
› Enhancement of primordial curvature perturbations in $R^3$-corrected Starobinsky-Higgs inflation
› Characterizing 3D Magnetic Fields and Turbulence in H I Clouds
› Learning novel representations of variable sources from multi-modal $\textit{Gaia}$ data via autoencoders
› The Kick Velocity Distribution of Isolated Neutron Stars
› Is Ozone a Reliable Proxy for Molecular Oxygen? II. The impact of N$_2$O on the O$_2$-O$_3$ relationship for Earth-like atmospheres
› Neutrino pair annihilation driven jets from black-hole torus systems
› IIb or not IIb: A Catalog of ZTF Kilonova Imposters
› Detection of positron in-flight annihilation from the Galaxy
› Cosmic structure from the path integral of classical mechanics and its comparison to standard perturbation theory
› Model-independent observational constraints with fast radio bursts
› X-SHOOTER Spectrum of Comet 3I/ATLAS: Insights into a Distant Interstellar Visitor
› Roles of SN and AGN Feedback in Shaping the Baryonic Content in a Wide Range of Dark Matter Halo Mass
› Supermassive Stars Match the Spectral Signatures of JWST's Little Red Dots
› Multi-wavelength study of the high Galactic latitude supernova remnant candidate G118.4+37.0 associated with the Calvera pulsar
› AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing
› Identifying the Quadrupolar Nature of Gravitational Wave Background through Space-based Missions
› Dirac Leptogenesis in Left-Right Symmetric Models
› On Formation of Primordial Naked Singularities
› Pre-thermalized Gravitational Waves
› Rotating Einstein-Maxwell-Dilaton Black Hole as a Particle Accelerator
› Detectability of gravitational atoms in black hole binaries with the Einstein Telescope
› Scale separation, rolling solutions and entropy bounds
› Soft Oscillons
› Evolution of a black hole cluster in full general relativity
› Universal Cosmologies
› Galactic double neutron stars as dual-line gravitational-wave sources: Prospects with LISA and Cosmic Explorer
› Time as a test-field: the no-boundary universe in motion and a smooth radiation bounce

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