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view from south-west
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 News from astronomynow.com

› 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
› Is the Hubble Tension Resolved?
› Universe’s end – sooner rather than later
RSS  Latest preprints on astro-ph:

› Tera-Hertz Counterparts to Fast Radio Bursts from Coherent Cherenkov Radiation by Tilted Bunches
› The End of the Road for Far-infrared Reddening Maps? Evidence for Reddening Errors Driven by Changes in PAH Abundance
› A Panchromatic View of Late-time Shock Power in the Type II Supernova 2023ixf
› Hot, cold, and multi-component accretion flows around supermassive black hole binaries
› The Wrath of KAN: Enabling Fast, Accurate, and Transparent Emulation of the Global 21 cm Cosmology Signal
› Theory of Exozodi Sources and Dust Evolution
› Late-time Hubble Space Telescope Ultraviolet Spectra of SN 2023ixf and SN 2024ggi Show Ongoing Interaction with Circumstellar Material
› Semi-analytic studies of accretion disk and magnetic field geometry in M87*
› MINDS. Strong oxygen depletion in the inner regions of a very low-mass star disk?
› Characterizing, correcting, and repairing the effects of radiation damage in the COSI germanium cross-strip detectors
› Comparative Analysis of Two Astrometric Measuring Methods on Five Known Binaries
› Where does non-Universality in Assembly Bias come from?
› Frequentist Cosmological Constraints from Full-Shape Clustering Measurements in DESI DR1
› Serendipitous discovery of a young cluster of galaxies at $z \sim 0.5$ projected next to the nearby tadpole galaxy KUG 1138 + 327
› Blue supergiants in the Pinwheel Galaxy M101: comparison with H II region chemical abundances, spectroscopic distance and an independent determination of the Hubble constant
› The Design and Performance Characteristics of the NRL4 ASIC Developed for the COSI Small Explorer Gamma-ray Satellite
› The BSN Application-I: Photometric Light Curve Solutions of Contact Binary Systems
› Dark Matter and the Early Formation of Supermassive Black Holes
› Limitations in constraining neutron star radii and nuclear properties from inspiral gravitational wave detections
› BSN-II: The First Light Curve Study of Eight Total Eclipsing Contact Binary Stars with Shallow Fillout Factors
› Evidence for ultra-water-rich ammonia hydrates stabilized in icy exoplanetary mantles
› Mapping feedback signatures in 3C 297: A quasar-host merger at Cosmic Noon
› Rings around giant planets and smaller bodies
› Machine learning-based classification of variable stars using phase-folded light curves
› Bayesian Inference of Gravity through Realistic 3D Modeling of Wide Binary Orbits: General Algorithm and a Pilot Study with HARPS Radial Velocities
› The origin of extreme N-emitters in star-forming galaxies at z$
› Mitigating point-source contamination in CMB polarization: a Generalized Point Spread Function fitting approach
› Cosmology-informed Neural Networks to infer dark energy equation-of-state
› Long term variability of Cygnus X-1. IX. A spectral-timing comparison of Cygnus X-1 and MAXI J1820+070 in the hard state
› Examining AGN UV/Optical Variability Beyond the Simple Damped Random Walk. II. Insights from 22 Years Observations of SDSS, PS1 and ZTF
› Scalable and robust wide-field facet calibration with LOFAR's longest baselines
› Magnetars in Binaries as the Engine of Actively Repeating Fast Radio Bursts
› Origin of High Dark Remnant Fractions in Milky Way Globular Clusters: The Crucial Role of Initial Black Hole Retention
› Investigating the Kinematics of Molecular Gas in Cometary Globule L1616
› How the cosmic voids contribute to stalling and quenching the giant galaxies on their surfaces
› Detection of young massive white dwarfs in core-collapsed globular cluster NGC 362
› Linking Stochastic Self-Propagating Star Formation and Spatio-Temporal Point Processes
› Destruction of "Peas in a Pod?" A Candidate Multi-planet System Around the Nearby, Bright Star, HD208487
› Activity-Cycle Variations of Convection Scales in Subsurface Layers of the Sun
› Type IIb Supernova Progenitors in 3D: Variability and Episodic Mass Loss revealed by Radiation-Hydrodynamics Simulations
› The JWST Rocky Worlds DDT Program reveals GJ 3929b to likely be a bare rock
› Mass Loss and Subsequent Thermal Evolution of Surviving Helium White Dwarfs Shocked by Thermonuclear Supernovae
› Group Therapy for Halos: Advancing Halo Mass Estimation for Galaxy Groups
› Three-Dimensional Numerical Simulations of Magnetar Crust Quakes
› The highest mass Kepler red giants -- II. Spectroscopic parameters, the amplitude-activity relation, and unexpected halo orbits
› SMILES Data Release II: Probing Galaxy Evolution during Cosmic Noon and Beyond with NIRSpec Medium-Resolution Spectra
› The Fraction of Distilled White Dwarfs with Long-Lived Habitable Zones
› A Tale of Two Sightlines: Comparison of Hydrocarbon Dust Absorption Bands toward Cygnus OB2-12 and the Galactic Center
› Spatially and Dynamically Extended Molecular Gas in Stephan's Quintet Revealed by ALMA CO(1-0) Total Power Mapping
› Image Profile (IMPRO) Fitting of Massive Protostars. I. Method Development and Test Cases of Cepheus A and G35.20-0.74N
› The Demographics of Binary Companions to Stripped-Envelope Supernovae: Confronting Observations with Population Synthesis
› On constraining initial orbital eccentricity of purely inspiral events
› Runaway stars and the Galactic supernova remnant landscape: non-thermal emission and observational evidence
› Observational Analysis of Multi-thermal Counter-streaming Flows in a Forming Filament and Their Relationship with Local Heating at Filament Footpoints
› How many stars form in compact clusters in the local Milky Way?
› Photospheric radius expansion thermonuclear burst and X-ray reflection from the neutron star X-ray binary 4U 1702-429
› Energy relaxation in superthermal collisions of carbon with oxygen: the influence of isotopic substitution
› PEARLS: Globular Clusters and Ultra-Compact Dwarfs in the El Gordo Galaxies at z=0.87
› An empirical determination of the Cosmic Shoreline
› A bird's eye view of stellar evolution through populations of variable stars in Galactic open clusters
› Adaptive Uniform Weighting: Pre-conditioning to Improve Image Fidelity
› TIRAMISU: Non-LTE radiative transfer for molecules in exoplanet atmospheres
› Planetary Nebulae in the eROSITA eRASS1 catalog
› Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors
› Self-Consistent Heating of the Magnetically Closed Solar Corona: Generation of Nanoflares, Thermodynamic Response of the Plasma and Observational Signatures
› Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars
› Energy Conversion and Electron Acceleration and Transport in 3D Simulations of Solar Flares
› Comparing X-ray Emission Line Fluxes of NGC 5548 to NGC 1068
› Size Distributions of Arcsecond-Scale Properties of Solar Flare Ribbons
› A test of Ca ii H & K photometry for isolating massive globular clusters below the metallicity floor
› EP250207b is not a collapsar fast X-ray transient. Is it due to a compact object merger?
› A 15 Mpc rotating galaxy filament at redshift z = 0.032
› Double-Peaked Optical Afterglows with X-ray Shallow Decay Inferring a Magnetized Thick Shell Ejecta
› Molecular Hydrogen in High-redshift Damped Lyman-{\alpha} Absorbers
› Activity in White Dwarf Debris Disks I: Spitzer Legacy Reveals Variability Incompatible with the Canonical Model
› The ALPINE-CRISTAL-JWST survey: spatially resolved star formation relations at $z\sim5$
› Aligned Stellar Obliquities for Two Hot Jupiter-hosting M Dwarfs Revealed by MAROON-X: Implications for Hot Jupiter Formation
› Impact of Non-Thermal Leptogenesis from Early Matter Domination on Gravitational Wave from FOPT
› A New Paradigm for Testing Gravity: Theory-Independent Constraints Using Data From All Astrophysical and Cosmological Scales
› Spacetime Perspective of Gravitational Lensing in Perturbed Cosmologies
› High-Energy Neutrinos from Cosmic-Ray Scatterings with Supernova Neutrinos
› Energy extraction from the accelerating Kerr black hole via magnetic reconnection in the plunging region and circular orbit region
› Wavelets for power spectral density estimation of gravitational wave data
› GW200105: A detailed study of eccentricity in the neutron star-black hole binary
› Scalarized neutron stars with a highly relativistic core in scalar-tensor gravity
› A Neural-Network Framework for Tracking and Identification of Cosmic-Ray Nuclei in the RadMap Telescope
› Completing Axion Double Level Crossings
› Morphological classification of eclipsing binary stars using computer vision methods
› Current sheet formation under radiative cooling
› Stellar metallicity is a key parameter for the search of Life in the Universe
› Partial tidal disruptions of spinning eccentric white dwarfs by spinning intermediate mass black holes
› Dust attenuation evolution in $z \sim 2$-$12$ JWST galaxies
› In-Flight Performance of Spider's 280 GHz Receivers
› A reassessment of LVE method and hemispherical power asymmetry in CMB temperature data from Planck PR4
› Estimating the gravitational wave background anisotropy: a Bayesian approach boosted by cross-correlation angular power spectrum
› NutMaat: A Python package for stellar spectral classification on the MK system
› High-cadence observations of galactic nuclei by the future two-band UV-photometry mission QUVIK
› Exploring lensing signatures through spectrotemporal correlations: implications for black hole parameter estimation
› The cosmological Mass Varying Neutrino model in the late universe
› Cosmic Strings-induced CMB anisotropies in light of Weighted Morphology
› Primordial black holes and scalar induced gravitational waves from sound speed resonance in non-minimal derivative coupling inflation model
› Massive Double White Dwarf Binary Mergers from the Moon: Extending the Reach of Multi-messenger Astrophysics
› XL-Calibur measurements of polarised hard X-ray emission from the Crab
› Evolution of Shock Structures and QPOs After Halting BHL Accretion onto Kerr Black Hole
› A non-uniform metal distribution in the ram-pressure stripped circumgalactic medium of M86
› JWST/NIRSpec Observations of High Ionization Emission Lines in Galaxies at High Redshift
› Bayesian pulsar timing and noise analysis with Vela.jl: the wideband paradigm
› Exploring the Interior Structure and Mode of Tidal Heating in Enceladus
› Wavelet Flow For Extragalactic Foreground Simulations
› Mass-feeding of jet-launching white dwarfs in grazing and common envelope evolution
› Direct High-Resolution Imaging of Earth-Like Exoplanets
› Head-on collisions of fuzzy/cold dark matter subhalos
› Differentiation, the exception not the rule -- Evidence for full miscibility in sub-Neptune interiors
› First release of LiteBIRD simulations from an end-to-end pipeline
› The z=1.03 Merging Cluster SPT-CL J0356-5337: New Strong Lensing Analysis with HST and MUSE
› The impact of natal kicks on black hole binaries
› Quasi-periodic variation during a fast X-ray outburst of a high-mass X-ray binary MAXI J0709-159 / LY CMa observed by NICER
› The $z=7.08$ quasar ULAS J1120+0641 May Never Reach a "Normal" Black Hole to Stellar Mass Ratio
› Tightening constraints on primordial oscillations with latest ACT and SPT data
› Hubble Space Telescope Observations of the Interstellar Interloper 3I/ATLAS
› The role of migration traps in the formation of binary black holes in AGN disks
› Meridional circulation molecular-weighted
› Evidence For Turbulent Concentration In Particle-Laden Midplane Layers of Planet-Forming Disks
› The Compilation and Validation of the Spectroscopic Redshift Catalogs for the DESI-COSMOS and DESI-XMMLSS Fields
› Starobinsky in Stereo: SKA-CMB Synergy in SBI
› Evidence for Evolving Dark Energy from LRG1 and Low-$z$ SNe Ia Data
› New black hole mergers in the LIGO-Virgo O3 data from a gravitational wave search including higher-order harmonics
› No-hair and almost-no-hair results for static axisymmetric black holes and ultracompact objects in astrophysical environments
› Self-consistent microscopic calculations for electron captures on nuclei in core-collapse supernovae
› Generalizing the Bogoliubov vs Boltzmann approaches in gravitational production
› A Distribution-Free Approach to Testing Models for Angular Power Spectra
› The Discriminant Power of Bubble Wall Velocities: Gravitational Waves and Electroweak Baryogenesis
› Cosmic strings in the complex symmetron model
› Extreme mass ratio inspirals in rotating dark matter spikes
› Self-Tracking Solutions for Asymptotic Scalar Fields
› SPLENDOR: a novel detector platform to search for light dark matter with narrow-gap semiconductors

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