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Astronomia w Krakowie
Photo: Międzynarodowa Stacja Kosmiczna i Księżyc z halo
Międzynarodowa Stacja Kosmiczna i Księżyc z halo
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RSS  Latest preprints on astro-ph:
› Bridging scales: How much do supermassive black holes grow in the suppressed Bondi regime?
› JWST/NIRSpec Reveals a Small Population of Dominant Dust-Obscured Ionizing Sources in Galaxies at 1 < z < 3
› An almost NIRCam-dark dusty star-forming galaxy at z=6.63
› Where Giants Dwell: Probing the Environments of Early Massive Quiescent Galaxies
› The binary landscape of massive stars at low $Z$: Insights from the BLOeM Campaign
› Evidence for in-situ acceleration of relativistic particles in the wings of X-shaped radio galaxies
› Highly Efficient Identification of Extreme Emission Line Galaxies in the Local Universe: >8000 New Green Pea Candidates at 0.12 < z < 0.36
› Bridging scales: Modeling suppressed Bondi accretion on black holes and its impact on galaxy growth
› Radiation-mediated shocks in gamma-ray bursts: spectral evolution
› Kinematic scaling relations of disc galaxies from ionised gas at $z\sim~1$ and their connection with dark matter halos
› No TiO detected in the hot Neptune-desert planet LTT-9779 b in reflected light at high spectral resolution
› Gravity-Selected Galaxy Clusters: a Tight Mass-Richness relation and an unclear Compton $Y$-richness trend
› Isolating the gravitational influence of Uranus's winds requires close passages inward of the rings
› Identification of Candidate Halos Hosting Massive Black Hole Seeds in the \textit{Renaissance} Simulations with Support Vector Machines
› Conservation laws in non-inertial frames and non-conservation of energy of relative motion in two-body problem
› How to evaluate the sufficiency and complementarity of summary statistics for cosmic fields: an information-theoretic perspective
› 3D MHD simulations of coronal loops heated via magnetic braiding I. Continuous driving
› 3D MHD simulations of coronal loops heated via magnetic braiding II. Automatic detection of reconnection outflows and statistical analysis of their properties
› WATSON-Net: Vetting, Validation, and Analysis of Transits from Space Observations with Neural Networks
› Symbolic Regression Is All You Need: From Simulations to Scaling Laws in Binary Neutron Star Mergers
› Probing the Molecular Hearts of Extreme Bipolar Planetary Nebulae with ALMA
› Model of super-Alfv\'enic MHD turbulence and structure functions of polarization
› Kinetic Theory and the Mechanics of Isothermal Gas Spheres: Derivation of the Classical Emden--Chandrasekhar Equation via the Vlasov--Poisson Formalism
› JWST Reveals Carbon-rich Chemistry in a Transitional Disk
› Analytical Description of Baryonic Matter Fluctuations Using Jeans Filtering Functions in Second-Order Cosmological Perturbation Theory
› An axisymmetric shock breakout indicated by prompt polarized emission from the type II supernova 2024ggi
› Stellar Populations with MaNGA: Iron Kink and Nitrogen Fuzz
› Detection Prospects for AGNs with the Cherenkov Telescope Array
› Gas excitation of post-starburst galaxies at 0.6 < z < 1.3
› Modelling Millisecond Pulsar Populations in Globular Clusters with NBODY6++GPU
› CoronaGraph Instrument Reference stars for Exoplanets (CorGI-REx) I. Preliminary Vetting and Implications for the Roman Coronagraph and Habitable Worlds Observatory
› Mock Observations for the CSST Mission: CPI-C -- Instrument Simulation
› Measuring the magnetic fields in the chromospheres of low-mass stars
› Probing Intrinsic Ellipticity in Neutron Star Binaries
› Low-Frequency Noise Performance of Microstrip-Coupled Lumped-Element Aluminum KIDs using Hydrogenated Amorphous Silicon Parallel-Plate Capacitors for NEW-MUSIC
› Continuum variability in multi-epoch quasar spectra from the Sloan Digital Sky Survey
› Improved Modeling of Quasi-Static Thermal and Optical Response of Lumped-Element Aluminum Manganese KIDs
› Search for host galaxies of unlocalized Fast Radio Bursts in the SDSS IV catalog
› The Dawn of Gravitational Wave Astronomy at Light-year Wavelengths: Insights from Pulsar Timing Arrays
› JW-Flare: Accurate Solar Flare Forecasting Method Based on Multimodal Large Language Models
› Design of a Six-band, 2.4-Octave (80--420 GHz) Hierarchically Summed Phased-Array Slot-Dipole Antenna Array for NEW-MUSIC
› Evolution of the radio source position uncertainties in radio astrometric catalogs over the past three decades
› Models of long-period variables of the globular cluster 47 Tuc
› Mock Observations for the CSST Mission: HSTDM--Synthetic Data Generation
› J-PAS: A Neural Network Approach to Single Stellar Population Characterization
› Multiwavelength spectral and temporal analysis of VHE Blazar 1ES 1959+650: Tracing emission mechanisms across flux states
› Detection of Lensed Gravitational Waves from dark matter halos with deep learning
› Superhot (> 30 MK) flare observations with STIX: Joint spectral fitting
› Not all roads lead to merger: AGN disc properties influence the interactions of highly unequal mass black holes
› Emission-Line and Continuum Reverberation Mapping of the NLS1 Galaxy WPVS 48
› Numerical Simulation of Impact Cratering and Induced Seismic Waves in Sand Targets
› Interstellar medium phases and abundances in the central parsec: A JWST MIRI/MRS view of the Galactic center
› Little red dots as embryos of active galactic nuclei
› Radio Burst from a Stellar Coronal Mass Ejection
› Occurrence rate of stellar Type II radio bursts from a 100 star-year search for coronal mass ejections
› Variability of optical spectral index to support a central sub-parsec binary black hole system in quasar SDSS J001224-102226.51
› A magnetic field study of two fast-rotating, radio bright M dwarfs. StKM 1-1262 and V374 Peg
› Recombination Clumping Factor of Physically Defined Intergalactic Medium at the Epoch of Reionization
› Ray-trax: Fast, Time-Dependent, and Differentiable Ray Tracing for On-the-fly Radiative Transfer in Turbulent Astrophysical Flows
› Rapid-response characterization of near-Earth asteroid 2024 YR4 during a Torino Scale 3 alert
› Bright Cosmic-Ray Source as a Solution to Auger-TA Tensions
› Compelling Evidence for a Harmonic in the Light Curve of the Supermassive Black Hole Binary Candidate PKS J1309+1154
› POLAR-2 - Latest Developments of the Next Generation GRB Polarimeter
› Ultra extreme high-frequency-peaked BL Lacs: a potential population of MeV synchrotron blazars?
› Comprehensive Study of the Lunar Energetic Particle Environment with LunPAN
› Development of a planar cable-driven parallel robot for submillimeter and terahertz beam mapping measurements
› Unbiased analysis of primordial non-Gaussianity: the multipoles of the full relativistic power spectrum
› Revisiting the Hubble tension problem in the framework of holographic dark energy
› TIME Commissioning Observations: I. Mapping Dust and Molecular Gas in the Sgr A Molecular Cloud Complex at the Galactic Center
› Adsorption and condensation of molecules on astrophysical dust grain surfaces: Ab-initio calculalations and kinetic Monte Carlo simulations
› From M100 to NGC 7331: A Multiband Study and Physical Parameters in Nearby Galaxies
› Global Distribution of the Key Species on the Surface of Europa
› Collisions in a system of conical jet/counterjet outflows
› A ring-shaped starburst as a galactic wind-generating mechanism: Morphology, emission, and mass ejection
› Probing Time-Dependent Physics with Phase-Folding CMB Maps
› Warped Disk Galaxies: Statistical Properties from DESI Legacy Imaging Surveys DR8
› Mitigating Nonlinear Systematics in Weak Lensing Surveys II: Stability and Diagnostics with Intrinsic Alignment
› Abiogenesis on Different Star Types; a Dissipative Photochemical Perspective
› Massive Inflationary Amplitudes: New Representations and Degenerate Limits
› Excitation factors for horizonless compact objects: long-lived modes, echoes, and greybody factors
› Did our Universe Tunnel out of the Wrong Higgs Vacuum?
› Progress on the ALETHEIA project and new approaches to events overlap mitigation
› Emergent Dark Matter
› Impact of reactor antineutrinos on the neutrino floor in low-mass WIMP-like dark matter searches
› A Unified Dark-Matter--Driven Relativistic Bondi Route to Black-Hole Growth from Stellar to Supermassive Scales
› Imaging and polarization patterns of various thick disks around Kerr-MOG black holes
› Conservation of magnetic-helicity fluctuations due to spatial decorrelation of fluxes in decaying MHD turbulence
› Phase transition during inflation and the gravitational wave signal at pulsar timing arrays
› Approximate reconstruction of inflationary potential with ACT observations
› Nature-inspired optimization, the Philippine Eagle, and cosmological parameter estimation
› Genetic algorithm demystified for cosmological parameter estimation
› The Atacama Cosmology Telescope: DR6 Power Spectrum Foreground Model and Validation
› Dynamic Diffusion Schr\"odinger Bridge in Astrophysical Observational Inversions
› On the prospects of thermalization of axion-SU(2) inflation
› The fine structure of the mean magnetic field in M31
› Consistent Initial Conditions for Early Modified Gravity in Effective Field Theory
› Three-dimensional equation of state extension of quark matter in Fermi-liquid theory
› UNIONS Optical Identifications for VLASS Radio Sources in the Euclid Sky (UNVEIL) I. A Catalog of ~146,000 Radio Galaxies up to z~5
› Interpreting Hubble tension with a cascade decaying dark matter sector
› Exploring Spatially-Resolved Metallicities, Dynamics and Outflows in Low-Mass Galaxies at $z \sim 7.6$
› Inflation from a generalized exponential plateau: towards extra suppressed tensor-to-scalar ratios
› Beyond Extreme Burstiness: Evolving Star Formation Efficiency as the Key to Early Galaxy Abundance
› Machine learning analysis of Photometric data from the Dark Energy Survey
› Cepheid Metallicity in the Leavitt Law (C--MetaLL) survey: VII. Metallicity dependence of Period-Wesenheit relations based on a homogeneous spectroscopic sample
› Lensing amplitude anomaly and varying electron mass alleviate the Hubble and $S_8$ tensions
› On the optical emission in the mini-outburst of the black hole X-ray binary MAXI J1348-630
› Probing the H0 Tension with Holographic Dark Energy in Unimodular Gravity: Insights from DESI DR2
› Radio Astronomy in the Era of Vision-Language Models: Prompt Sensitivity and Adaptation
› Second Generation Planet Formation in Post-AGB Discs: Testing the Role of Gravitational Instability
› Disentangling Milky Way halo populations at low metallicities using [Al/Fe]
› Reionization optical depth and CMB-BAO tension in punctuated inflation
› Witnessing downsizing in the making: quiescent and breathing galaxies at the dawn of the Universe
› Quintessential inflation studied through Semiclassical Methods
› Both Stellar Mass and Gravitational Potential Shape the Gas-Phase Metallicity
› A Photometric Classifier for Tidal Disruption Events in Rubin LSST
› Ionization Sources of the Local Interstellar Clouds: Two B-stars, Three White Dwarfs, and the Local Hot Bubble
› FlowLensing: Simulating Gravitational Lensing with Flow Matching
› Using simultaneous mass accretion and external photoevaporation rates for d203-504 to constrain disc evolution processes
› The richest clusters in the Coma and Leo superclusters: Properties and evolution
› Re-envisioning Euclid Galaxy Morphology: Identifying and Interpreting Features with Sparse Autoencoders
› The chemical DNA of the Magellanic Clouds IV. Unveiling extreme element production: the Eu abundance in the Small Magellanic Cloud
› Discovery of Seven Cold and Distant Brown Dwarfs with JWST RUBIES
› JWST provides a new view of cosmic dawn: latest developments in studies of early galaxies
› JWST Lensed Quasar Dark Matter Survey III: Dark Matter Sensitive Flux Ratios and Warm Dark Matter Constraint from the Full Sample
› In-Orbit GRB Identification Using LLM-based model for the CXPD CubeSat
› Towards direct imaging and orbital parameter estimation of supermassive black hole binaries with spaceborne VLBI
› Euclid preparation. Non-Gaussianity of 2-point statistics likelihood: Precise analysis of the matter power spectrum distribution
› On the problem of initial conditions for inflation
› Bayesian network 3D event reconstruction in the Cygno optical TPC for dark matter direct detection
› Discrete Chi-Square Method beats Discrete Fourier Transform and other similar parametric time series analysis methods

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