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 News from astronomynow.com

› Astronomy Now relaunches digital platform
› Potentially habitable planet TRAPPIST-1e displays tentative evidence for an atmosphere
› Ten-Year Lease Extension Confirmed at Herstmonceux Observatory
› Venus and Jupiter’s bright morning conjunction
› It’s time again for Perseid meteors!
› Lonely giant planets may form their own planetary systems
› Congratulations Professor Michele Dougherty – our new Astronomer Royal
› Astronomy Now under new ownership
› Binoculars to boost your night-sky viewing
› Lyra’s stunning smoke ring – M57
RSS  Latest preprints on astro-ph:

› CWT-LSTM Autoencoder: A Novel Approach for Gravitational Wave Detection in Synthetic Data
› Gravitational Recoil and Suppression of Super Massive Black Hole Seeds in the Early Universe
› A Systematic Review of Lagrange Points Applications in the Solar System
› Active galactic nuclei do not exhibit stably periodic brightness variations
› CMB component-separated power spectrum estimation by Spectral Internal Linear Combination (SpILC)
› Bias in the tensor-to-scalar ratio from self-interacting dark radiation
› The HST Ultraviolet Spectrum of V723 Mon: Additional Evidence of a Stellar Companion
› Assembling GW231123 in star clusters through the combination of stellar binary evolution and hierarchical mergers
› The Photochemical Plausibility of Warm Exo-Titans Orbiting M-Dwarf Stars
› GLACE survey: OSIRIS/GTC multi-object spectroscopy of the rich galaxy cluster ZwCl 0024.0+1652 at z~0.4. III. The mass-SFR relation and the quenching of cluster galaxies
› An Introduction to Dust Evolution and Vertical Transport in Protoplanetary Disks
› The Discovery of a Large Active Wind from the Milky Way's Central Black Hole
› LEO-Vetter: Fully Automated Flux- and Pixel-Level Vetting of TESS Planet Candidates to Support Occurrence Rates
› Central-star extinctions towards planetary nebulae
› Radiation GRMHD Models of Accretion onto Stellar-Mass Black Holes: II. Super-Eddington Accretion
› A candidate to the long sought optical counterpart to the Rapid Burster in the bulge fossil fragment Liller 1
› Characterizing the interplay between Galactic star formation and ionization feedback with PRIMA
› SDSS-V Local Volume Mapper (LVM): Revealing the Structure of the Rosette Nebula
› Formation of Cosmic Noon Protogalaxies via Quasar-Induced Fragmentation of a Cosmic Filament
› Using white dwarf lensing to resolve accretion flows
› Statistical Analysis of Magnetic Patches in Solar Active Regions Using the Complex Network Method
› Orbit-based structural decomposition and stellar population recovery for edge-on barred galaxies
› Measuring neutrino masses with joint JWST and DESI DR2 data
› Primordial Black Holes (PBHs) and The Signatures of Cosmic Non-Gaussianity
› Evidence of Galactic Center Expansion from Gaia DR3 Stars along the South North Axis: Implications for the JWST Early Galaxy Problem
› Space Astrometry with Gaia: Advances in Understanding our Galaxy
› Mitigating Random-Phase Sampling Noise in the Cepheid Period-Luminosity Relation: A Cross-Filter Consistency Approach
› New constraint on Europa's ice shell: magnetic signature from the ocean
› Hydrocarbon Hazes on Temperate sub-Neptune K2-18b supported by data from the James Webb Space Telescope
› Joint Bayesian calibration and map-making for intensity mapping experiments
› The M- and X-class White-light Flares in Super Active Region NOAA 13664/13697 Observed by ASO-S/LST/WST
› Consistent Modeling of Non-equilibrium Dust Sublimation and the Interactions with Dust Evolution in the Inner Regions of Protoplanetary Disks
› JWST/NIRCam imaging of the Bipolar Planetary Nebula NGC 6537: the (Infra)red Spider, Revealed
› The Signature of Sub-galactic Dark Matter Clumping in the Global 21-cm Signal of Hydrogen
› Dust Attenuation of Lyman-Werner Feedback: Reassessing Early Super Massive Black Holes Seed Formation
› A Dark Matter Model with Quadratic Equation of State: Background Evolution and Structure Formation
› Probing small-scale dark matter clumping with the large-scale 21-cm power spectrum
› Decomposing wave activity in the solar atmosphere: Shocks, jets and swirls in the quiet Sun
› Simulations of Tidal Disruption of Supernova in Galaxy Nuclear Region: A Novel Model for Ambiguous Nuclear Transients
› Origin of the lunar farside highlands from Earthshine-induced global circulation in lunar magma ocean
› Investigating Phosphorus Abundances in a Sample of APOGEE-2 Bulge Globular Clusters
› Neural networks in the search for fast radio bursts with RATAN-600
› Probing Hernquist dark matter with black hole shadows: A comprehensive study of various accretions
› Analytic Model for Scattered Ly$\boldsymbol{\alpha}$ Emission in the Post-reionization Intergalactic Medium
› Tracing correlations between galaxy properties across the Cosmic Web: An IllustrisTNG-based study
› The Orbits of Isolated Dwarfs in the Local Group from New 3D Kinematics: Constraints on First Infall, Backsplash, and Quenching Mechanisms
› The SRG/eROSITA All-Sky Survey $J$-Band Follow-Up Observations for Selected High-Redshift Galaxy Cluster Candidates
› Solar Eruption Onset and Particle Acceleration in Nested-Null Topologies
› Demystifying Strange O VI Line Widths with Hydrodynamic Simulations
› Role of magnetic shear distribution on the formation of eruptive flux ropes
› Dense Molecular Ring-like structure in gaseous CO depletion region G34.74-0.12
› Three binary-source binary-lens microlensing events from the 2024 microlensing campaign
› Scaling relations at the central regions of nearby galaxies
› The Polar Orbit of TOI-2374 b, a Planet in the Neptunian Ridge
› Equilibrium Points and Surface Dynamics About Comet 67P/Churyumov-Gerasimenko
› Compression, Impact and Hot Rebound Flows from Coronal Rain Downflows
› Hurst Index of Gamma-Ray Burst Light Curves and Its Statistical Study
› Molecular Jets from an Evolved Protostar: Insights from JWST-ALMA Synergy
› The Curious Case of V CVn
› Quantifying the Impact of Lunar and Planetary Occultation on Experimental Global 21 cm Cosmology
› Angle-dependent hardening of the reprocessed spectra in ULXs powered by accretion onto neutron stars
› Magnetic reconnection sustains the mass budget of the solar wind
› Disentangling disc and atmospheric signatures of young brown dwarfs with JWST/NIRSpec
› Self-lensing binaries as probes of Supernova physics
› Investigating the correlations of bulk properties of hyperon star with dark matter
› Dense gas properties and star formation in M 82
› JWST's first view of the most vigorously star-forming cloud in the Galactic center -- Sagittarius B2
› The averaged broadband spectral energy distribution study of Fermi bright BL Lac objects
› A comprehensive view of PKS 2155-304 from 2008 to 2023 through a multi-epoch modeling of its spectral energy distributions
› Understanding variations of galactic energetic particles in the heliosphere: modelling and radiation hazard assessment
› Precise Measurement of the Absolute Sky Brightness at 60 to 350 MHz
› Education and Outreach Across Seventeen Countries of the Pierre Auger Collaboration
› Astrophysics: a Modern Discipline with a Newtonian origin
› The impact of external gas accretion on the distribution of HI gas in galaxies
› Bayesian recalibration of flux scale factors in diffuse radio maps using low-resolution absolute radiometers
› Testing CCC+TL Cosmology with Galaxy Rotation Curves
› Testing $n_s=1$ in light of the latest ACT and SPT data
› Dust trapping in protoplanetary discs after stellar flybys
› Chemical Abundances of M and G Dwarfs in the Hyades and Coma Berenices Open Clusters from APOGEE Spectra
› Frequency evolution of pulsar emission: Further evidence for fan beam model
› Atacama Cosmology Telescope: Constraints on the Millimetre Flux of the Crab Pulsar
› Radio Galaxy Zoo: Morphological classification by Fanaroff-Riley designation using self-supervised pre-training
› STRAWBERRY: Finding haloes in the gravitational potential
› Discovery of femto Gauss intergalactic magnetic fields towards Mkn 501
› Periodic Variations in Visible Light Brightness as Tracers of Fine Coronal Structures
› Revealing Event Rate of Repeating Fast Radio Bursts
› The dependence of the Type Ia Supernova colour-luminosity relation on their host galaxy properties
› Gravitational Signatures of Axion Dark Matter via Parity-Violating Interactions
› A Study of Spectral Variability between flaring and non-flaring state in M74 X-1
› Characterization of Two Cool Galaxy Outflow Candidates Using Mid-Infrared Emission from Polycyclic Aromatic Hydrocarbons
› Observational Evidence of Dust Evolution in Supernova Remnants: Size Redistribution Toward Larger Grains in Early Sedov Phase
› YOLO-CIANNA: Galaxy detection with deep learning in radio data: II. Winning the SKA SDC2 using a generalized 3D-YOLO network
› High-energy interstellar isomers: cis-N-methylformamide in the G+0.693-0.027 molecular cloud
› Spectral Energy Distribution Analysis of the Supersoft X-ray Source CAL 87: Multiwavelength Constraints
› White Dwarfs with Infrared Excess in the HET Dark Energy Experiment
› Evidence for a gap in the envelope mass fraction of sub-Saturns
› A Short Introduction to Cosmology and its Current Status
› Pressure Regulated Formation of Molecular Clouds and Stars: The case of the Milky Way
› Hydrodynamical models of the $\beta$ Lyr A circumstellar disc
› Combining PIC and MHD to model particle acceleration in astrophysical shocks
› Negative gas-phase metallicity gradients in the narrow line region and galactic disc of local AGN-host galaxies
› Chandra Large Project Observations of the Supernova Remnant N132D: Measuring the Expansion of the Forward Shock
› A New Population of Point-like, Narrow-line Objects Revealed by the James Webb Space Telescope
› Deriving accurate galaxy cluster masses using X-ray thermodynamic profiles and graph neural networks
› Breaking Dark: Hunting Heavy Decaying Dark Matter with Tibet AS$_\gamma$ and LHAASO-KM2A
› Exploring Multi-view Symbolic Regression methods in physical sciences
› Theoretical Signatures of QCD Phase Transitions in Compact Astrophysical Systems
› Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency
› Black Hole Superradiance of Interacting Multi-Field
› Sign-Flipping Axion Potentials via Kapitza-Type Modulation by Heavy Axions
› Gravitational Waves from $\textit{Type-I}$ Strings in a Neutrino Mass Model
› Inflationary trispectrum of gauge fields from scalar and tensor exchanges
› Analytical Perturbative Construction of Initial Data for Binary Black Holes up to Third Order in Spin and Momentum
› An interstellar mission to the closest black hole?
› Solving the Trans-Planckian Censorship Problem with a Power-law Tail in $R^2$ Inflation: A Dynamical System Approach
› Charged particle dynamics in magnetosphere generated by current loop around Schwarzschild black hole
› A study of the pulsar EXO 1745-248 in $f(Q)$ gravity with pseudo-spheroidal geometry
› High-Precision Measurement of D($\gamma$, $n$)$p$ Photodisintegration Reaction and Implications for Big-Bang Nucleosynthesis
› Can LIGO Detect Daylight Savings Time?
› Letter of Intent: 100m Atom Interferometer Experiment at CERN
› Anomalous electron heating in laboratory magnetized quasi-perpendicular collisionless shocks
› An Optomechanical Accelerometer Search for Ultralight Dark Matter
› New constraints on $Z^\prime$ from captured dark matter annihilation in astrophysical objects
› Solar fusion III: New data and theory for hydrogen-burning stars
› Neutron-quark stars: Discerning viable alternatives for the higher-density part of the equation of state of compact stars
› Discover high-z BL Lacs by Swift and SARA observations with the dropout technique
› Gravitational wave energy spectral density properties from BPASS Galactic binary population in the Milky Way galaxy
› Stellar Obliquity Excitation via Disk Dispersal-Driven Resonances in Binaries
› Globally Stable Dark Energy in $F(R)$ Gravity
› Interpreting the LHAASO Galactic diffuse emission data
› So long Kolmogorov: the forward and backward turbulence cascades in a supernovae-driven, multiphase interstellar medium
› Incorporating Magnetic Field Characteristics into EUV-Based Automated Segmentation of Coronal Holes
› Galaxy mergers classification using CNNs trained on S\'ersic models, residuals and raw images
› The Effect of Massive Trans-Neptunian Objects in the Long-term Evolution and Leaking Rates of Neptune's 3:2 and 2:1 Mean Motion Resonances
› Systematic bias in dark siren statistical methods and its impact on Hubble constant measurement
› Using the antenna impedance to estimate soil electrical parameters for the MIST global 21-cm experiment
› Spatiotemporal Low FIP Abundance: A Catalyst for Coronal Condensation
› Luminis Stellarum et Machina: Applications of Machine Learning in Light Curve Analysis
› Dynamical Measurement of Supermassive Black Hole Masses: QPE Timing Method
› Starlight from JWST: Implications for star formation and dark matter models
› Addressing the too-big-to-fail problem and the void phenomenon through a modified initial power spectrum
› The vertical structure of debris discs and the role of disc gravity: A primer using a simplified model
› Interaction of a spatially uniform electron beam with a rotational magnetic hole in a form of a Harris current sheet
› The Star Formation and Chemical Evolution Histories of Ursa Minor Dwarf Spheroidal Galaxy
› Radiation GRMHD Models of Accretion onto Stellar-Mass Black Holes: I. Survey of Eddington Ratios
› Multi-band Emission from Star-Disk Collision and Implications for Quasi-Periodic Eruptions
› Calibrating baryonic effects in cosmic shear with external data in the LSST era
› High Dimensional Beam Inference II: Inference of a Perturbed HERA Beam from Simulated Visibility Data
› Timing and spectral studies of SRGA J144459.2$-$604207 with NICER, Einstein Probe, IXPE, NuSTAR, Insight-HXMT and INTEGRAL during its 2024 outburst
› The star HIP 41378 potentially misaligned with its cohort of long-period planets
› A Simulation Framework for the LiteBIRD Instruments
› The long-term stability of the Vast Polar Structure and its connection to a possible previous passage of the LMC
› The IACOB project XV. Updated calibrations of fundamental parameters of Galactic O-type stars
› Bayesian Inference of Gravity through Realistic 3D Modeling of Wide Binary Orbits: General Algorithm and a Pilot Study with HARPS Radial Velocities
› Self-Consistent Heating of the Magnetically Closed Solar Corona: Generation of Nanoflares, Thermodynamic Response of the Plasma and Observational Signatures
› On the Encounter Rate of Open Star Clusters
› A two-phase model of galaxy formation: IV. Seeding and growing supermassive black holes in dark matter halos
› A fast machine learning tool to predict the composition of astronomical ices from infrared absorption spectra
› Nuclear Stellar Discs
› Solar System Experiments in the Search for Dark Energy and Dark Matter
› The Optical and Mechanical Design of POEMMA Balloon with Radio
› Detection of a septuple stellar system in formation via disk fragmentation
› Suppression of pair beam instabilities in a laboratory analogue of blazar pair cascades
› The large-scale kinematics of young stars in the Milky Way disc: first results from SDSS-V
› Euclid: Early Release Observations -- The star cluster systems of the Local Group dwarf galaxies IC 10 and NGC 6822
› Which is which? Identification of the two compact objects in gravitational-wave binaries
› Comparing strange and non-strange quark stars within resummed QCD at NLO
› Sub-GeV dark matter and nano-Hertz gravitational waves from a classically conformal dark sector
› Signatures of Einstein-Maxwell dilaton-axion gravity from the observed quasi-periodic oscillations in black holes
› Generalized relativistic second-order dissipative hydrodynamics: coupling different rank tensors
› What KM3-230213A events may tell us about the neutrino mass and dark matter
› Multiscale Cosmic Curvature: from Local Structures to Cosmology
› t-channel dark matter at the LHC -- a whitepaper
› QSHS: An Axion Dark Matter Resonant Search Apparatus
› Primordial black holes and magnetic fields in conformal neutrino mass models
› Modelling Cosmic-Ray Transport: Magnetized versus Unmagnetized Motion in Astrophysical Magnetic Turbulence
› A pipeline for searching and fitting instrumental glitches in LISA data
› Inflationary power spectrum from the Lanczos algorithm
› Vortices without inflow: bound spectra in horizonless rotational analogs
› External Attention Transformer: A Robust AI Model for Identifying Initial Eccentricity Signatures in Binary Black Hole Events in Simulated Advanced LIGO Data
› Quasi-Normal Modes and Nonlinear Electrodynamics in Black Hole Phase Transitions
› Directed searches for gravitational waves from ultralight vector boson clouds around merger remnant and galactic black holes during the first part of the fourth LIGO-Virgo-KAGRA observing run

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