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 News from astronomynow.com

› See Titan’s shadow transit Saturn – next chance 2038!
› Nova outburst in Centaurus
› 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
RSS  Latest preprints on astro-ph:

› MUSEQuBES: Physical conditions, origins, and multi-element abundances of the circumgalactic medium of an isolated, star-forming dwarf galaxy at z=0.57
› Modeling gravitational wave sources in the MillenniumTNG simulations
› New ultralight scalar particles and the mass-radius relation of white dwarfs -- the important role of Sirius B
› Beyond the stars: Linking H$\alpha$ sizes, kinematics, and star formation in galaxies at $z\approx 4-6$ with JWST grism surveys and $\texttt{geko}$
› A Deep Look into the Intermediate-Age Open Cluster NGC 2506: What Binary Systems Reveal About Cluster Distance and Age
› Comparing XRISM cluster velocity dispersions with predictions from cosmological simulations: are feedback models too ejective?
› Preferential Accretion onto the Secondary Black Hole Strengthens Gravitational Wave Signals
› Asymmetries in stellar streams induced by a galactic merger
› Phase-resolved optical spectroscopy of the rapidly varying white dwarf ZTF 1851+1714
› A Walk on the Retrograde Side (WRS) project. II. Chemistry to disentangle in situ and accreted components in Thamnos
› MEGATRON: Disentangling Physical Processes and Observational Bias in the Multi-Phase ISM of High-Redshift Galaxies
› Are all Binary Black Holes Detected from LIGO-Virgo-KAGRA Follow the Universal Time-Delay Distributions? Likely Not
› Evidence of violation of Case B recombination in Little Red Dots
› JWST occultation reveals unforeseen complexity in Chariklo's ring system
› The rise and fall of Little Red Dots could be driven by the environment
› The first proper motion measurement of the acceleration regions in the large-scale jets of SS 433 powering the W50 nebula
› Radiation magnetohydrodynamics modeling of an impulsively driven chromospheric jet in the solar atmosphere
› CCAT: Readout of over 10,000 280 GHz KIDs in Mod-Cam using RFSoC Electronics
› Ensemble seismic study of the properties of the core of Red Clump stars
› Primordial Black Holes and their Mass Spectra: The Effects of Mergers and Accretion within Stasis Cosmologies
› RFSoC receiver calibration system for 21-cm global spectrum experiments from space: The CosmoCube case
› Revisiting the Orbital Dynamics of the Hot Jupiter WASP-12b with New Transit Times
› Dual perspectives on GX 17+2: a simultaneous NICER and NuSTAR study
› A chemodynamical study of $r$-process-enhanced stars
› Ionized gas components in low surface brightness galaxy AGC 111629
› Formation of A Nuclear Star Cluster Through A Merger Event In The Low Surface Brightness Galaxy AGC 223218
› The Star-forming Main Sequence and Bursty Star-formation Histories at $z>1.4$ in JADES and AURORA
› Spectropolarimetry of NGC 1275 reveals a narrow-line radio galaxy with polarization parallel to its radio jet axis
› 3D B-fieLds in the InterStellar medium and Star-forming regions (3D-BLISS): I. Using Starlight Polarization in Massive IRDC Filament G11.11-0.12
› Benchmarking AI-evolved cosmological structure formation
› Diagnosing the Properties and Evolutionary Fates of Black Hole and Wolf-Rayet X-ray Binaries as Potential Gravitational Wave Sources for the LIGO-Virgo-KAGRA Network
› Identifying the secondary jet in the RadioAstron image of OJ~287
› Warm absorber outflows in radio-loud active galactic nucleus 3C~59
› A Sample of HeII {\lambda}4686 "Changing-Look" Quasars
› Low-noise Fourier Transform Spectroscopy Enabled by Superconducting On-Chip Filterbank Spectrometers
› A Giant Peanut-shaped Ultra-High-Energy Gamma-Ray Emitter Off the Galactic Plane
› Hard X-ray view of two $\gamma$-ray detected low-luminosity active galactic nuclei: NGC 315 and NGC 4261
› JWST observations of photodissociation regions: II. Warm molecular Hydrogen spectroscopy in the Horsehead nebula
› MEGATRON: The environments of Population III stars at Cosmic Dawn and their connection to present day galaxies
› Unlocking AGN Variability with Custom ZTF Photometry for High-Fidelity Light Curves and Robust Selection
› The radial acceleration relation at the EDGE of galaxy formation: testing its universality in low-mass dwarf galaxies
› Recasting the nature of INTEGRAL hard X-ray transients previously classified as active galactic nuclei
› Textual interpretation of transient image classifications from large language models
› Is the high-energy environment of K2-18b special?
› Simulations of Globular Cluster Evolution with Multiple Stellar Populations
› 1FLAT: a Firmamento-based catalog of AGN in Fermi-LAT high Galactic latitude {\gamma}-ray sources
› In-flight performance of the IXPE telescopes
› Understanding an origin of palladium in metal-poor stars based on the non-LTE analysis of Pd~I lines
› Protoplanetary disc population synthesis I. Constraining disc parameters to reproduce disc observations
› Revealing the Temporally Stable Bimodal Energy Distribution of FRB 20121102A with a Tripled Burst Set from AI Detections
› Modeling the formation of N2 and CH4 frost on Pluto's slopes
› Machine Learning Techniques to Distinguish Giant Stars from Dwarf Stars Using Only Photometry -- Pushing Redwards
› The formation of Gaia BH3
› Prolonged fallback and late-time rebrightening episodes in stellar tidal disruptions as imprints of a galactic environment
› Machine Learning for Radial Velocity Analysis I: Vision Transformers as a Robust Alternative for Detecting Planetary Candidates
› Polka-dotted Stars II: Starspots and obliquities of Kepler-17 and Kepler-63
› CURLING -- II. Improvement on the $H_{0}$ Inference from Pixelized Cluster Strong Lens Modeling
› Disk fraction among free-floating planetary-mass objects in Upper Scorpius
› Archival Inference for Eccentric Stellar-Mass Binary Black Holes in Space-Based Gravitational Wave Observations
› Fomalhaut's debris disc is not dominated by primordial Plutos
› Probing the cosmological 21~cm global signal from the Antarctic ice sheet
› AppleCiDEr II: SpectraNet -- A Deep Learning Network for Spectroscopic Data
› High-energy variability of the gravitationally lensed blazar PKS 1830-211
› Testing new-physics scenarios with the combined LHAASO and Carpet-3 fluence spectrum of GRB 221009A: axion-like particles and Lorentz-invariance violation
› JWST-TST High Contrast: Medium-resolution spectroscopy reveals a carbon-rich circumplanetary disk around the young accreting exoplanet Delorme 1 AB b
› Beyond diagnostic-diagrams: A critical exploration on the classification of ionization processes
› The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; varying hydrodynamic models, dust, and wide-field, narrow-band imaging detection
› A Comoving Framework for Planet Migration
› Confirming Near- to Mid-IR Photometrically-Identified Obscured AGNs in the JWST era
› Probing evolution of Long GRB properties through their cosmic formation history aided by Machine Learning predicted redshifts
› Diffuse continuum emission and large extended sources at MeV energies
› Rolling with modular symmetry: quintessence and de Sitter in heterotic orbifolds
› Magnetic Helicity, Magnetic Monopoles, and Higgs Winding
› Vision Transformer for Transient Noise Classification
› A comprehensive look into the accuracy of SpEC binary black hole waveforms
› Classification of $g$-modes for neutron stars with a strong transition: Novel universal relation including slow stable twin stars
› Influence of Solar Sails on Magnetic Field Measurements in Space Plasmas
› A Review of 10 Years of ProtoSpace: Spacecraft CAD Visualization in Collaborative Augmented Reality
› Measurement of the $^{35}Cl(n, p)^{35}S$ cross-section at the CERN n\_TOF facility from subthermal energy to 120 keV
› When vacuum breaks: a self-consistency test for astrophysical environments in extreme mass ratio inspirals
› Unified Dark Matter and Dark Energy in a model of Non-Canonical Scalar-Tensor Theory
› GW231123: extreme spins or microglitches?
› On Inflation and Reheating Features in the Higgs-$R^2$ Model
› Tracing satellite planes in the Sculptor group: II. Discovery of five faint dwarf galaxies in the DESI Legacy Survey
› Distribution of Europium in The Milky Way Disk; Its Connection to Planetary Habitability and The Source of The R-Process
› A Semi-analytic Framework of Population III and Subsequent Galaxy Formation on Cosmological N-body Simulations
› The Southern Photometrical Local Universe Survey (S-PLUS): searching for metal-poor dwarf galaxies
› AGN ruled out as the dominant source of cosmic reionization
› Foreground Removal in Ground-Based CMB Observations Using a Transformer Model
› Cosmology with One Galaxy: Auto-Encoding the Galaxy Properties Manifold
› Dark sirens and the impact of redshift precision
› Investigating dusty Red Supergiant outflows in Westerlund 1 with 3D Hydrodynamic simulations
› Forming the local starburst galaxy Haro 11 through hydrodynamical merger simulations
› Determining the 3D Dynamics of Solar Flare Magnetic Reconnection
› Gravitational Wave Memory of Primordial Black Hole Mergers
› Prospects for disentangling dark matter with weak lensing
› Cosmic Ray Perpendicular Superdiffusion and Parallel Mirror Diffusion in a Partially Ionized and Turbulent Medium
› Are magnetic fields in cosmic voids primordial?
› The hot circumgalactic medium in stacked X-rays: observations vs simulations
› Direct reconstruction of the Reionization history from 21cm 2D Power Spectra
› Requirements on bandpass resolution and measurement precision for LiteBIRD
› Type Ibn supernovae from ultra-stripped supernova progenitors
› Thick Disks around White Dwarfs viewed 'Edge-off': Effects on Transit Properties and Infrared Excess
› Synthesizer: a Software Package for Synthetic Astronomical Observables
› Magnetars in Binaries as the Engine of Actively Repeating Fast Radio Bursts
› Hyper Suprime-Cam Y3 results: photo-$z$ bias calibration with lensing shear ratios and cosmological constraints from cosmic shear
› Spectral characterization and performance of SPT-SLIM on-chip filterbank spectrometers
› The source of the cosmic-ray excess in the Centaurus region -- constraints on possible candidates, mass composition and cosmic magnetic fields
› Matter power spectrum reconstruction with KiDS-Legacy: Improved internal $\Lambda$CDM consistency and preference for strong baryonic feedback
› Supergranulation and poleward migration of the magnetic field at high latitudes of the Sun
› Evaluating Solar Wind Forecast Using Magnetic Maps That Include Helioseismic Far-Side Information
› Expectations for the first supermassive black-hole binary resolved by PTAs II: Milestones for binary characterization
› Expectations for the first supermassive black-hole binary resolved by PTAs I: Model efficacy
› Abundance of strontium in the Galactic globular cluster 47 Tuc
› A Link Between Rocky Planet Density and Host Star Chemistry
› M5 -- Mars Magnetospheric Multipoint Measurement Mission: A multi-spacecraft plasma physics mission to Mars
› Sharpening the dark matter signature in gravitational waveforms I: Accretion and eccentricity evolution
› Background-dependent and classical correspondences between $f(Q)$ and $f(T)$ gravity
› Prospects of future MeV telescopes in probing weak-scale Dark Matter
› Unveiling a New $\beta$-Scaling of the Tearing Instability in Weakly Collisional Plasmas
› The Dark Matter Diffused Supernova Neutrino Background
› Framework for phase transitions between the Maxwell and Gibbs constructions at finite temperature
› Modeling Gravitational Wave Modes from the Inspiral of Binaries with Arbitrary Eccentricity
› Universality of gravitational radiation from magnetar magnetospheres
› Flavour interferometry in Reissner-Nordstrom background
› The impact of Alfvenic shear flow on magnetic reconnection and turbulence
› High-Quality Axion Dark Matter at Gravitational Wave Interferometers
› Regression of Suspension Violin Modes in KAGRA O3GK Data with Kalman Filters
› Extra Radiation Cosmologies: Implications of the Hubble Tension for eV-scale Neutrinos
› WISPFI Experiment: Prototype Development

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