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Astronomia w Krakowie
Photo: Halo, moon dogs and parhelic circle around the Moon
Halo, moon dogs and parhelic circle around the Moon
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 News from astronomynow.com
› Happy New Year, Mars! The Red Planet is turning 39
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› Europe’s Mars rover may land in the remains of a vast ancient water system
› Moon dust preserves record of life’s building blocks
RSS  Latest preprints on astro-ph:
› Diffusion Models for Polarimetric Reconstruction of Circumstellar Environments in Correlated Speckle Noise
› Multi Kernel Gaussian Process Guiding: Predictive Correction for Mounts with Several Gear Stages
› The orbital dynamics of the LMC and SMC about the Milky Way
› Not So Heavy Metal I: Low Metallicity Enhances the Rate of high-redshift Superluminous Supernovae
› Nearby Supernova Science in the Era of High Cadence, Deep Time Domain Surveys
› Close Pulsar Pairs See Dark Matter Substructure through the Gravitational-Wave Background
› Testing Offsets Between Cluster-Scale Halos and BCGs in Strong Lensing Models Using the Jackknife Method
› Gestalt: a meta-foundation model for astronomy
› An Infant Sub-Saturn in Scorpius-Centaurus
› Surveying for Close Binaries among Lithium-rich Giants
› An X-ray Extremely wide-field Spectroscopic Surveyor (XESS, or "chess")
› Revealing the accretion disc structure in Changing State AGN: NGC1566
› Learning Gaia: A Generative Model Trained on the Gaia Data Release 3 Source Catalog
› Cosmic-neighbor-associated distances to VHE and candidate VHE BL Lacs via SDSS photometric redshifts
› HESS J1507-622: A Plausible Young Galactic Kilonova Remnant
› VLBI Astrometric Procedure and Performance with CHIME/FRB Outriggers
› A New Hope for AGN SED Fitting: X-Ray Spectral Analysis of 12MGS AGN with the C2PO-Torus Model
› NEXUS: Discovery of a Luminous Young Transient at $z=5$
› PTED: A multi-dimensional two-sample test for scientific inference and generative machine learning
› Fisher and DALI posterior approximations for testing gravity with gravitational waves
› AdS - de Sitter transition in interacting dark energy models
› Cosmic Collisions I: Optical Morphologies for MIRI-selected galaxies from the PRIMER survey
› Space Journey Beyond Earth: Exploring the properties of exoplanets and multi-planetary systems
› Toward Detecting the Moving Lens Effect with Optical Spectroscopy
› Migration and Evolution of giant ExoPlanets (MEEP). III. Twenty-Nine Giant Planets from the TESS Mission
› Relativistic Spherical Accretion in Nonrotating Black Hole Spacetimes: Astrophysical Implications
› Modeling of the Yarkovsky effect. I. Thermal dependence
› A triple-induced merger in T Ori C, solves the proplyd lifetime problem and the curiously young shell of M42
› Nonthermal hotspot orbiting the supermassive black hole Sgr A*
› aRieL - Reinforcement Learning for the Ariel Space Telescope Scheduling
› Angular structure of finite-field vacuum birefringence in magnetars
› Sunrise III/SUSI reveals extended and spectrally structured Ca II K emission above the solar limb
› Chandra X-ray Spectral Evidence of the Dual AGN Nature of the Gravitational lens MG B2016+112 at z=3.273 with 175 pc separation
› A Probabilistic Trajectory and Dispersion Study of Martian Tumbleweed Rover Swarms in Global Dust Storm Conditions
› New Constraints on $r$-process Nucleosynthesis in Neutron Star Mergers from GW170817 Late-Phase Spectra
› HLX-1 as a Repeating Partial Tidal Disruption Event around an Intermediate-Mass Black Hole
› Magnetic field diagnostics of a solar active region filament
› Pulsar glitches triggered by quakes when stress reaches a threshold
› MATCH: Performance Characterization and Scientific Observations of the Wuhan University 1-m Optical Telescope
› Planetesimal Formation under Realistic Gas Dynamics: Dust Concentration in Turbulent and Windy Protoplanetary Disks
› The impact of the turbulent Mach number on star formation and the initial mass function
› The "Fork" Geometry in the DESI Main Survey DR1: Implications of Target Selection for Galaxy Evolution Studies
› Metastable Dark Energy on the Phantom Brane
› Stacked strong and weak lensing united: Improved measurement of the stellar and dark matter distributions in massive early-type galaxies at $z\sim 0.5$
› Improved Population and EOS Joint Inference for Binary Neutron Star Systems
› The Simons Observatory: Design and Initial Performance of the Detector Readout System for the Large-Aperture Telescope
› AGC 322753: a Dark Galaxy Candidate detected by ALFALFA and FASHI
› Probing Helical Primordial Magnetic Fields via Chiral Gravitational Waves in the LISA-TAIJI Network
› Electromagnetic Counterparts of Stellar-mass Binary Black Hole Mergers in AGN Accretion Disks: Theoretical Models and Observational Status
› The Astronomical Hub: A Unified Ecosystem for Modern Astronomical Research
› The impact of primordial magnetic fields on the formation of galaxies
› Correlating Surface Magnetic Field Decay with Internal Field Depth of Isolated Neutron Stars
› Exploring the Primordial Power Spectrum with Dark-Age 21 cm fluctuations
› The AI crisis for teaching: "Train your own neural network!"
› Early Planet Formation in Embedded Disks (eDisk). XXV. Inclination-Induced Minor-Axis Brightness Asymmetries Reveal Limited Dust Settling in Embedded Protostellar Disks
› FAIR-Compliant Architecture for Heterogeneous Astronomical Data: KazVO Framework
› ArxSP: A Python-Based Modular Application for the Reduction of Digitized Archival Spectra
› An LSST-DESC Precursor Project: Hyper Suprime-Cam Year 1 $3\times2$pt in Harmonic Space
› Internal Structure, Not Environment, Shapes Metallicity Gradients in Low-Mass Galaxies from MaNGA
› Deep radio characterization of the supernova remnant G343.1-00.7
› High velocity dust grains produced by a supernova explosion
› Effects of a central dark matter core on time-delay cosmography with galaxy clusters
› An improved standardization framework for Type II-P supernovae using a hierarchical Bayesian approach
› XRISM Resolve Spectroscopy of GX 5-1: Constraints on Iron Spectral Features in a Luminous Neutron-Star Binary
› The Cosmological Correlation Dimension Beyond the Linear Regime: Analytical Approximation and Parameter Sensitivity
› Towards breaking the degeneracy between stellar ages and unresolved multiplicity
› Raising the Optical Depth to Reionization with Dark Matter Decay
› High-Priority Compact-Object Candidates in Young Clusters from the \textit{Gaia} DR3 Non-Single-Star Catalog
› The role of velocity dispersion in the Kennicutt-Schmidt relation
› A New Sample of Closely Separated Dual and Binary AGN Candidates Revealed with the Radio Fundamental Catalog
› Toward the Italian Astronomical Community's Contribution to HWO: Science, Technology, and Instrument Concepts
› Project CERES: Nuclear Thermal Transportation and In-Situ Propellant Production A Foundational Architecture for Solar System Logistics
› Tracing star formation across the Rosette nebula using deep Spitzer imaging
› MAGiDiff: Sampling the Photospheric Vector Field from UV/EUV Filtergrams
› When Streams Curve Away: a Test of Dark Matter from Extragalactic Stellar Stream Populations
› Flow dynamics of cryolava or impact melt on Titan's surface
› A machine learning-based method for populating dark matter halos in N-body simulations with substructure
› Improved Constraints on Cosmic Microwave Background Circular Polarization with CLASS
› The assembly history of NGC 1365 through chemical archaeology
› A new method for inspiral-to-ringdown waveforms of compact binaries: Helmholtz orbits and spherical-Bessel flux
› Is DESI Seeing Dynamical Dark Energy, or a Cosmic Glitch in Gravity?
› Sub-kiloparsec Test of the Kennicutt-Schmidt Relation in a Strongly Lensed Dusty Star-Forming Galaxy at z~2.78
› Two bits about lossy compression: On the limits of compression in cosmology
› Probing the Reionization History and Bubble Sizes with JWST Lyman-$\alpha$ Fraction Measurements
› Slowly rotating Black Holes in DHOST Theories
› A Strong Cosmologically Coupled Mass Growth Solution in Linearized General Relativity
› Searching for BSM Experimental Signatures with Large Lagrangian Models
› How collective modes terminate in the dispersion relation of neutrino plasmas
› Constraints on Complex Electroweak WIMPs from Solar Capture
› Kilopixel Performance of the Kinetic Inductance Detectors for the Terahertz Intensity Mapper
› Primordial Tensor Signatures and Gravitational Wave Constraints in Lorentz Violating Inflation with Non-Canonical Kinetics
› Heavy Dark Baryons at Large $N$: Self-Interactions across All Scales
› Heavy Dark Baryons as Self-Interacting Dark Matter: A GeV-Scale Coincidence
› MADGRAV: a multilevel anomaly-detection pipeline for gravitational-wave searches applied to LIGO data
› Enhancing Constraints on Ultralight Axion Dark Matter from Gravitational Capture
› Interpreting the High-Recoil LUX-ZEPLIN Event with Bino-/Singlino-like and Higgsino Dark Matter
› Clash of the Titans: ultra-high energy KM3NeT event versus IceCube data
› Euclid preparation CIX. Baryon acoustic oscillation analysis of photometric galaxy clustering in configuration space
› Spatio-Temporal Log-Gaussian Cox-Hawkes Processes with Inhibition and Excitation for Stochastic Star Formation
› The Einstein Gap: an unrecognised strong lensing feature in weak lensing mass density profiles
› Effects of primordial magnetic fields on 21 cm multifrequency angular power spectra
› Relativistic jets from millisecond proto-magnetars
› Factorized neural posterior estimation for rapid and reliable inference of parameterized post-Einsteinian deviation parameters in gravitational waves
› Heavy-particle production during inflation and its gravitational-wave signal
› Reconstruction of cosmic-ray direction and energy in radio arrays using deep ensemble graph neural networks
› Starbursts hiding in the main sequence: a pathway toward quenching?
› Proto-NUX: A prototype telescope for ground-based near-ultraviolet observations
› CMB constraints on dark matter-proton scattering: investigating prior-volume effects using profile likelihoods
› Non-LTE Ionization Modeling for Helium and Strontium in Neutron Star Merger Ejecta
› Galactic tides and the outer density profile of the Sculptor and Ursa Minor dwarf spheroidals
› Bayesian power spectrum estimation with modelling of systematic effects in delay-fringe rate space
› Galaxy luminosity functions from far-UV to submillimetre at $z=0$ in the COLIBRE simulations
› Exploring the Transitional Parameter Space of Blazars using Gamma-ray and X-ray Population Diagnostics
› Cosmic web stripping and starvation of low-mass filament galaxies in TNG50
› Observations of stable pickup He$^+$ tori in a magnetic flux rope at 0.85 au
› Hybrid neural denoising for resource-efficient near- and sub-threshold radio triggering of extensive air showers
› A Consistent Implementation of Cluster Strong Lensing in Cosmological Simulation Light Cones
› Gas-induced gravitational-wave dephasing and accretion periodicities of live post-Newtonian massive black hole binaries: warm disk
› DANTE: A Reference-Guided Unsupervised Pipeline for Extended-Transient Anomaly Characterization in LIGO O4a
› Characterization of the RF Board for microwave SQUID multiplexing readout electronics
› Modeling Uncertainties in Modified Gravity Predictions for the Stochastic Gravitational-Wave Background
› Radiation-hydrodynamics of star-disc collisions: From system parameters to outflows and lightcurves
› Circumstellar Disc and X-ray Variability in the Be/X-ray Binary SXP 5.05 During its 2024 Outburst
› Propagation Diagnostics of Supernova Remnant Environments around Young Repeating Fast Radio Bursts. I. Hydrodynamic Evolution of the Source-local Dispersion Measure
› SPT-3G D1: Foreground-Robust Lensing Templates for Primordial Gravitational Wave Searches
› On the Acceleration of Pulsar Timing computations using Normalising Flows and Parallelisation
› JW-FD: A 15-Year Multimodal Dataset for Solar Flare Forecasting
› Do DESI-DR2 BAO data imply a coupling of dark matter and dark energy?
› Connecting Dynamo Theory with DNS Data: A Computational Analysis of $\alpha$ and $\beta$ effects
› Forecasting Coupled Dark Energy Parameters with the One-Loop Galaxy Power Spectrum
› Inelastic scattering effects on polarization predictions for cold and warm atmospheres in the X-rays
› K-dwarf starspot hunters: how to directly characterize spot and faculae properties with UV-IR panchromatic transit spectra
› Slow-roll inflation in $f\left(R, T, R_{ab}T^{ab}\right)$ gravity
› Primordial black hole formation in matter domination
› Bounds on massive graviton-like particles from searches for axion-like particles coupling to photons
› Development of Neutron Transmutation Doped Germanium (NTD-Ge) for Cryogenic Applications
› Infrared Screening of the Cosmological Constant

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