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Photo: The Mt. Suhora 60cm telescope
The Mt. Suhora 60cm telescope
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 News from astronomynow.com
› Astronomy Now relaunches digital platform
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› Congratulations Professor Michele Dougherty – our new Astronomer Royal
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RSS  Latest preprints on astro-ph:
› GW231109_235456: A Sub-threshold Binary Neutron Star Merger in the LIGO-Virgo-KAGRA O4a Observing Run?
› Precise Constraints on the Energy Budget of WASP-121 b from its JWST NIRISS/SOSS Phase Curve
› Double Trouble: Two spectroscopically confirmed low-mass quiescent galaxies at z>5 in overdensities
› The New Generation Planetary Population Synthesis (NGPPS). VII. Statistical comparison with the HARPS/Coralie survey
› Witnessing downsizing in the making: quiescent and breathing galaxies at the dawn of the Universe
› Spatially Offset Active Galactic Nuclei in the Very Large Array Sky Survey: Tracers of Galaxy Mergers and Wandering Massive Black Holes
› Early Stages of Dusty Tori: The First Infrared Spectra from a Highly Multiscale Quasar Simulation
› Commissioning and Testing of IceAct Telescopes at the IceCube Neutrino Observatory
› Progress toward a demonstration of high contrast imaging at ultraviolet wavelengths
› The Last Stand Before Rubin: a consolidated sample of strong lensing systems in wide-field surveys
› The invariance of group occupation across the cosmic web
› An Improved Fit to the Density Distribution in Supersonic Isothermal Turbulence
› Sensitivity of spectral lines to granulation: The Sun
› Discovery and Analysis of Afterglows from Poorly Localised GRBs with the Gravitational-wave Optical Transient Observer (GOTO) All-sky Survey
› Dynamically New Comet C/2025 D1 (Groeller) with Record Perihelion Distance
› Optimized HDBSCAN clustering for reconstructing the merger history of the Milky Way: applications and limitations
› Initial conditions for tidal synchronisation of a planet by its moon
› Propeller effect in action: unveiling quenched accretion in the transient X-ray pulsar 4U 0115+63
› Trends in the Population of Binary Black Holes Following the Fourth Gravitational-Wave Transient Catalog: a Data-Driven Analysis
› Stellar halo subtraction alternative for accreting companions' characterization with integral field spectroscopy: Analytical and on-sky demonstration on the PDS70, HTLup, and YSES1 systems
› PeV particle acceleration and non-thermal emission in the `minimalist' model of the extended jets in W50/SS433
› Kinematics of the lens host S0 galaxy NGC 1553: role of secular processes
› Laplace-Fourier linear stability analysis of non-relativistic magnetized rotational jets: mode identification by Hamiltonian analysis and the occurrence of mode transitions
› Supra-arcade downflows in an extensive fan associated with a giant quiescent solar filament eruption
› Encyclopedia of Astrophysics: The Expanding Universe
› Which Solar Latitude Follows the Sunspot Cycle Exactly?
› The Hubble constant from the improved lens modeling of cluster-lensed supernova Refsdal with new spectroscopic redshifts and the Jackknife method
› Unified $g$-mode and $r$-mode Analysis of Accreting White Dwarf Stars
› Effects of harmonic magnetic field boundary conditions in mean-field solar dynamo
› A star-by-star correspondence between X-ray activity and rotation in the young open cluster NGC 2516 with eROSITA
› High Power Accretion in Massive Binary Systems and the Impact of Metallicity
› Rotating twisted magnetosphere of magnetars: approximate analytical solutions
› Multi-GeV Fermi-LAT Detection of PSR B1259-63
› A massive primordial atmosphere on early Mars
› ALMA reveals diverse dust-to-gas mass ratios and quenching modes in old quiescent galaxies
› An intense geomagnetic storm originated from stealth Coronal Mass Ejection: remote and $in situ$ observations by near radially aligned spacecraft
› An ultraviolet burst oscillation candidate from the low-mass X-ray binary EXO 0748-676
› Impact of stochastic star-formation histories and dust on selecting quiescent galaxies with JWST photometry
› Reionization in HESTIA: Studying reionization in the LG through zoom simulations
› A four-planet system orbiting the old thick disk star TOI-1203
› Cluster Ages to Reconstruct the Milky Way Assembly (CARMA) IV. Chrono-dynamics of seven old star clusters in the Large Magellanic Cloud and the peculiar origin of NGC 1841
› Calculating Occultation Light Curves using Wavelets: Exponential Atmospheres and the Constraints of Static Stability
› Magnetic effects on fundamental modes in rotating neutron stars with a purely toroidal magnetic field
› Towards Precision Cosmology With Improved PNLF Distances Using VLT-MUSE. III. Impact of Stellar Populations in Early-Type Galaxy
› Interaction between disk and extended corona in general relativistic framework. I. Static slab corona in global energy balance with the underlying disk
› Ionospheric Electron Heat Flow Modulates Planetary Ambipolar Electric Fields
› Further evidence for natal kick segregation by spectral type in high-mass X-ray binaries
› Signatures of dynamical activity in the hot gas profiles of groups and clusters in the FLAMINGO simulations
› The 21-cm signature of X-ray heated halos around galaxies during cosmic dawn
› UV-irradiated outflows from low-mass protostars in Ophiuchus with JWST/MIRI
› Astroclimes -- measuring the abundance of CO$_2$ and CH$_4$ in the Earth's atmosphere using astronomical observations
› Stellar populations of quasar host galaxies with MFICA decomposition
› A Differentiable Surrogate Model for the Generation of Radio Pulses from In-Ice Neutrino Interactions
› A MeerKAT view of the parsec-scale jets in the black-hole X-ray binary GRS 1758-258
› Is cosmic dust porous?
› The merger of spinning, accreting supermassive black hole binaries
› The electron temperature distribution and the high ionization just behind the shock in the Cygnus Loop
› Can a gamma-ray dim radio blazar produce a 200-PeV neutrino? The case of PMN J0606$-$0724 and KM3-230213A
› CMB Constraints on Quantized Spatial Curvature $\Omega_K$ in globally CPT-symmetric universes
› The large-scale kinematics of young stars in the Milky Way disc: first results from SDSS-V
› Testing the nature of compact objects in the lower mass gap using gravitational wave observations
› Primordial Black Hole Formation in a Scalar Field Dominated Universe: Investigation of the Critical nature of the Collapse
› Statistic of stars with poor astrometric solutions of Gaia DR3 in open star clusters
› Euclid: Early Release Observations -- The star cluster systems of the Local Group dwarf galaxies IC 10 and NGC 6822
› The CHARA Array Polarization Model and Prospects for Spectropolarimetry
› Joint X-ray, kinetic Sunyaev-Zeldovich, and weak lensing measurements: toward a consensus picture of efficient gas expulsion from groups and clusters
› Extending the Dynamical Systems Toolkit: Coupled Fields in Multiscalar Dark Energy
› Probing Light Primordial Black Holes through Non-cold Dark Matter
› Extraction of neutron-capture cross sections on $^{92}$Zr using the charge-exchange Oslo method
› What do the fundamental constants of physics tell us about life?
› Next generation direct RF sampling LLRF control and monitoring system for linear accelerators
› FLARE-SSM: Deep State Space Models with Influence-Balanced Loss for 72-Hour Solar Flare Prediction
› The Doppler boosted LISA response to gravitational waves
› Nuclear chiral density wave in neutron stars?
› Effective Mass in Quantum Hadrodynamics-I and its Impact on the Equation of State of Neutron Matter
› Bertrand's Representation of the Optimal Detector
› Ten years of gravitational-wave astronomy
› Gravitational Wave Signature and the Nature of Neutrino Masses: Majorana, Dirac, or Pseudo-Dirac?
› Gravitational wave signatures from the phase-transition-induced collapse of a magnetized neutron star
› Bridging the micro-Hz gravitational wave gap via Doppler tracking with the Uranus Orbiter and Probe Mission: Massive black hole binaries, early universe signals and ultra-light dark matter
› Removal of interloper contamination to line-intensity maps using correlations with ancillary tracers of the large-scale structure
› Decoding Dark Matter Admixed Neutron Stars: From Static Structure to Rotational Deformation
› Development of a Compton Imager Setup
› Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data?
› ImageMM: Joint multi-frame image restoration and super-resolution
› Influence of the Galactic Halo on the UHECR Multipoles
› Different physical and numerical sources of scatter in the $M_{\star}$-$M_{\mathrm{BH}}$ relation and their connection to galaxy evolution
› Study of mass outflows from magnetized accretion disks around rotating black holes with thermal conduction
› The Power of the Cosmic Web
› Rapid Construction of Joint Pulsar Timing Array Datasets: The Lite Method
› MARTA: Temperature-temperature relationships and strong-line metallicity calibrations from multiple auroral-line detections at cosmic noon
› A universal natal spin in stellar-mass black holes
› Machine Learning-Based Analytical Expressions for Gray-Body Factors and Application to Primordial Black Holes
› Variability of X-ray polarization of Cyg X-1
› The Moon as a possible source for Earth's co-orbital bodies
› Mitigation of the Flexing-Filtering Effect in Time-Delay Interferometry
› Separating Angular and Radial Modes with Spherical-Fourier Bessel Power Spectrum on All Scales and Implications for Systematics Mitigation
› General-relativistic magnetar magnetospheres in 3D with physics-informed neural networks
› Pushing the limits of eccentricity in planet-disc interactions
› The NEID Earth Twin Survey. III. Survey Performance After Three Years on Sky
› Quantifying the intrinsic variability due to randomness of the Auriga galaxy formation model
› A double-degenerate scenario with a merger to explosion delay time to explain type Ia supernova SN 2020aeuh
› Atomic hydrogen reservoirs in quiescent galaxies at z = 0.4
› Machine learning classification of black holes in the mass--spin diagram
› The frequency-independent radio luminosity -- orbital/rotational period relation of RS CVn stars
› The Impact of Spectroscopic Redshift Errors on Cosmological Measurements
› Machine Learning Classification of COSMOS2020 Galaxies: Quiescent vs. Star-Forming
› Detection of a septuple stellar system in formation via disk fragmentation
› Auriga Streams III: the mass-metallicity relation does not rule out tidal mass loss in Local Group satellites
› Searching for GEMS: The Occurrence of Giant Planets orbiting M-dwarfs within 100 pc
› Reconstruction of the depth of the shower maximum of air showers with the SD-750 surface detector of the Pierre Auger Observatory using neural networks
› LMC+: Large-scale mapping of [CII] and [OIII] in the LMC molecular ridge, I. Dataset and line ratio analyses
› Lepton collider as a window to reheating via freezing in dark matter detection. Part I
› A Universal Bound on QCD Axions from Supernovae
› Inner crust of neutron stars: Polymorphism and superconductivity in the liquid drop model
› A Distribution-Free Approach to Testing Models for Angular Power Spectra
› Bulk Viscosity of Two-Flavor Color Superconducting Quark Matter in Neutron Star Mergers
› Ultralight Boson Ionization from Comparable-Mass Binary Black Holes

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