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Astronomia w Krakowie
Photo: View over the dome at night
View over the dome at night
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Temperature
16.3 °C

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 80%

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12.9 km/h

Pressure
1008.4 hPa

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Moon

 News from astronomynow.com
› How to observe the 12 August 2026 solar eclipse
› Falcon 9 lunar impact: More than a new crater
› Euclid opens a new window on the first billion years of cosmic history
› Caught in the act: the wind that could kill a galaxy
› Europe’s Mars rover may land in the remains of a vast ancient water system
› Moon dust preserves record of life’s building blocks
› Dark matter may come in multiple forms, new model suggests
› Witness to history: Artemis II, lunar exploration and hope
› Artificial Intelligence uncovers more than 100 new worlds in NASA data
› XRISM solves gamma-Cas’s 50-year X-ray mystery
RSS  Latest preprints on astro-ph:
› Controlling artificial surface heating in neutron star simulations: Application to hybrid equations of state
› TomoSphero: Fast Differentiable Projector for Planetary and Solar Tomography on Spherical Grids
› A Critical Eddington Ratio for X-Shaped Radio Galaxies
› A JWST/MIRI Study of Dust in a Sample of Normal Type IIP Core Collapse Supernovae
› Probing the $\gamma$-ray emission region and the connection to jet ejections in NRAO 150 with VLBI
› Resolving Nearby Supermassive Black Holes with the Black Hole Explorer
› General relativistic hydrodynamics of stellar tidal disruptions in Kerr spacetime: methods, validation, and first applications
› Merging Galaxy Clusters and the Search for New Physics of Dark Matter: A Review
› Causes of Hot Jupiter Inflation from Causal Discovery
› A comprehensive cluster census of Orion. An application of the Significance Mode Analysis (SigMA) algorithm
› GEMS JWST: Hold on to your HATS(-6 b), a sub-solar metallicity giant planet with water, methane and ammonia in its atmosphere
› The Gamma-ray Burst Jet Energy Distribution Suggests A Quasi-universal, Weakly Magnetized Jet Evolving Over Cosmic Time
› Interacting stellar winds feeding Sgr A*: from the system of mass-losing stars to the binary IRS 16SW
› Diverse ionized gas conditions in a dynamically hot, interacting galaxy at $z = 9.31$ revealed by JWST/NIRSpec IFU
› Broadband emission of microquasar remnants
› Sr and Ba yields of the First Generation(s) of stars: Constraints from metal-poor stars
› Spectral Fingerprints Beyond Degeneracies in Primordial Gravitational-Wave Sources
› Extreme-Mass-Ratio Inspirals in Gaseous Disks
› A Statistical Mechanics Model for Stable Rings Outside the Roche Limit
› SCExAO/CHARIS High-Contrast Pre-Launch Vetting of Roman Coronagraph Technology Demonstration PSF Reference Stars
› A novel technique for reflection coefficient measurement in precision cosmology
› The VariableTNG project: Unveiling the physical drivers of galaxy quenching
› Measuring Simulated Circumgalactic Medium Turbulence with Emission-Weighted Projected Velocity Structure Functions in FOGGIE
› Understanding the Energy Input Required for Methane Emission on CWISEP J193518.59-154620.3: A Comprehensive Analysis
› Tracking nonlinear solar-wind dynamics over three solar cycles using Wind observations
› The X-Ray Continuum Emission Region in the Lensed Quasar SDSS J133907.23+131038.6 is Much Smaller than the Accretion Disk
› The Roman Coronagraph Community Participation Program: data reduction pipeline design and implementation
› pynucastro 3: A community library for nuclear astrophysics
› The Roman Coronagraph Community Participation Program: pre-launch reference star list and impact of reference star properties on post-processing performance
› The Roman Coronagraph Community Participation Program: trials and triumphs of designing an observing program for a technology demonstration instrument
› Intrinsic Alignments in Redshift Space I: Symmetries
› Simulating Zernike-based CWFS with HCIPy
› Confirmation of the Finch Flatter-Fainter Relation for the Quadruple Images of Lensed Point Sources
› The Roman Coronagraph Community Participation Program: Observation planning and data reduction for polarimetric mode
› The Roman Coronagraph Community Participation Program: target database and tools
› On-sky demonstration of dual-field interferometry at the CHARA Array
› Atmospheric Reconnaissance of TRAPPIST-1 f with JWST NIRISS SOSS: No Evidence for the Transit Light Source Effect
› Dark Energy in the $w-c_s^2$ Plane
› Investigating The Effects of Early Dark Energy on Large-scale Structure Within the EDENS Suite
› JWST-MIRI's multi-dimensional view of mass loss in the irradiated disks of NGC 1977
› Surface gravity wave on a neutron star ocean trapped around a magnetic pole
› AT 2020afjz (TSS2020a): The First Fast Extragalactic Transient Discovered by TESS
› The Roman Coronagraph Community Participation Program: corgisim - a simulation suite for the Nancy Grace Roman Space Telescope Coronagraph Instrument
› The VariableTNG project: how baryonic mechanisms shape galaxy properties
› Sudden emergence of a low-frequency hard X-ray lag in the Seyfert 1 galaxy Mrk 1044
› The Roman Coronagraph Community Participation Program: early calibration plan and pilot observation of a companion
› The Roman Coronagraph Community Participation Program: calibration strategy for the Mueller matrix using on-sky sources
› Diffuse Dwarf Galaxies in Galaxy Clusters: I. Stellar Populations and Radial Gradients
› Candidates for the most [$O_{III}$] $\lambda5007$-luminous planetary nebula in the Milky Way. I. Integrated light properties of NGC 6572, NGC 6884, and M 1-71
› Discovery of an Eccentric Hot Super-Jupiter Leaving the Transiting Geometry of the Early-A-type star TOI-1355
› Density-induced dark-baryon conversion in $\Delta-$admixed hypernuclear neutron stars
› Formation of heavy double neutron stars II: the role of heavy first-born neutron stars and low metallicity
› EON-SII: Design of a transportable picosecond stellar intensity interferometer for compact-star astrophysics
› Ejecta clumps revealed by study of reverse-shocked ejecta through MUSE integral field spectroscopy of SNR 0509-67.5
› Impact of Upstream Clumpiness on Supernova Remnant Forward Shock Evolution in Molecular Cloud Environments
› Modelling s-process chemical clocks: insights from high-precision Kepler data
› Modelling mountains on accreting magnetized neutron stars
› From Variability to SED Modeling: A Multiwavelength Study of the Neutrino Blazar TXS 0506+056
› NMMA-Astro-COLIBRI: An Automated Light-Curve Supernovae Classification Service in the Multi-Survey Era
› Dianoga simulations of galaxy clusters and groups: Properties of the baryonic components
› The PANSY Meteor Head-echo Orbit Catalogue: Continuous Antarctic Radar Observations of Southern Meteoroid Streams
› Complex morphology and kinematics at the heart of the very low luminosity object IRAM 04191+1522
› SST-1M: Recent results and prospects for observation of the Galactic Center region
› Revisiting neutrino event epochs for the blazar PKS 0735+178 with TESS
› A stochastic forward model for the intergalactic dispersion-measure distribution of Fast Radio Bursts
› A Semi-Analytical Theory for Improved Orbit Design of the GARAT\'EA-L
› Infrared Lines from Sterile-Neutrino Transition Magnetic Moments at JWST
› $R_{\rm e}$, or not $R_{\rm e}$: Developing $R_5\equiv R_{-2}$ as a scale radius for galaxy sizes, masses, and mass-to-light ratios
› Radar observations of Europa in 2011-2024: New insights into radar scattering properties
› Large eROSITA X-ray sources as 2MRS galaxy groups
› A Catalog of Homogeneously Derived Stellar Parameters for Spectroscopic Survey Stars
› eROSITA cosmology with galaxy groups: hot gas budget out to the virial radius
› The initial evolution of SN 2011dh: The importance of inhomogeneities
› The Roman Coronagraph Community Participation Program: Using the Zernike wavefront sensor for a full characterisation of the Roman Space Telescope and the Coronagraph Instrument
› The high entropy of the UHECR arrival direction distribution favors a light composition
› Simulation tools for realistic high-order wavefront correction with the Roman Coronagraph
› Accurately simulating gain and clock-induced charge production in the EMCCD gain register
› Triggered Fragmentation in Self-Gravitating Protoplanetary discs: Cooling, Mass Movement and Instability
› 3D simulations of magnetospheric accretion in T Tauri stars: I. Disk truncation, stellar torques, and application to observations
› The Stellar Population of NGC 346 in the Small Magellanic Cloud with JWST
› Concerns regarding recurrent fluorescence's impact on smaller diffuse ISM aromatics
› The segmented spiral structure of the Solar neighbourhood traced by young clustered populations
› Hydrodynamics modeling of the water snow line in young protoplanetary disks with dust-size-dependent opacities
› Vera C. Rubin LSST Synthetic Magnitudes derived from Gaia XP Spectra
› Observations of Disrupted CME Material Falling Back Into the Low Corona
› Evidence of self-organized criticality in the prompt emission of a bright gamma-ray burst
› The Spin Angular Momentum and Black Hole Mass Components of Sagittarius A*
› The Roman Coronagraph Community Participation Program: data reduction pipeline astrometric calibration
› Imprints of Mass Accretion History on Galaxy Cluster Morphology
› The instantaneous mass accretion rate of novae in quiescence: - an archival ultraviolet optical spectral analysis
› Generalized Non-linear Bayesian Pulsar Timing with Enterprise
› Variable Star Polarimetry with PICSARR-2
› The Effects of Binary Reference Stars on JWST NIRCam Coronagraphy
› Fundamental Cosmic Anisotropy and its Ramifications II: Perturbations in Bianchi spacetimes, and fixed in the Newtonian gauge
› Detecting Lorentz-violation induced by a tensor field with S-star's motion around Sgr A*
› Validating direct solvers for Newton's gravitational N-body problem, and the systematic comparison between IEEE floating point and Posits
› Exact black hole solutions with semi-symmetric vectorial torsion
› The FLARE Facility
› Seeding baryonic dark matter
› Generative artificial intelligence for reconstructing neutron-star matter
› An axion constraint from the diffuse supernova neutrino background indicated by Super-Kamiokande
› VERaiPHY -- Validation & Evaluation for Robust AI in PHYsics
› Astrobiology and the Transformation of Scientific Epistemology
› Revised $^{45}$V($p,\gamma$)$^{46}$Cr reaction rate and its impact on the production of $^{44}$Ti in core-collapse supernovae
› A compact analytic formula for the one-loop triangle cosmological correlator
› Confining density functional approach to the QCD phase diagram at low temperatures and thermal twin stars
› Particle Acceleration Time due to Turbulence-Induced Magnetic Reconnection
› The Cooling of Old White Dwarfs in 47 Tucanae
› Vacuum birefringence and the polarized X-ray emission from a radio magnetar
› Formation of Substructure in Luminous Submillimeter Galaxies (FOSSILS): Initial sample and the discovery of a dusty spiral at cosmic noon
› Formation of Substructure in Luminous Submillimeter Galaxies (FOSSILS): Evidence of Multiple Pathways to Trigger Starbursts in Luminous Submillimeter Galaxies
› Baryonic Masses and Properties of Gaseous Satellite Galaxies
› Radial dust distributions and obscuring geometry in AGN from JWST/MIRI spectroscopy
› Sensitivity of the Hongmeng 21cm experiment to scattering dark matter
› OutLines: Modeling Spectral Lines from Winds, Bubbles, and Outflows
› Prospecting MeerKAT Continuum Data for Enigmatic Radio Sources with Unsupervised Vector-Quantised Variational Autoencoders
› Orbital stability of compact three-planet systems III. The role of three-body resonances
› 3D Rotation of the Open Cluster NGC 2516
› Comprehensive neutrino light curves and spectra: from pre-supernova evolution to early supernova phase
› The Steep-spectrum Radio-loud AGN Luminosity Function and Its Implications for Black Hole Growth and Star Formation
› Microscopic primordial black holes as macroscopic dark matter from large extra dimensions
› White dwarf + M dwarf Detached Binaries in Long Period Radio Transients: Observed Binary Parameters, Evolution, and Population Constraints
› Shortest period for outer orbit in compact hierarchical triple? Discovery of SB1 around V0885 Per
› No model-independent evidence for a peak in binary black hole spin (mis)alignments
› Neutrino Flavor Conversion Shapes the Rate of Failed Core-collapse Supernovae
› Flavor Conversion Enhances or Suppresses Supernova Explodability Independent of the Progenitor Mass
› Changing-look Active Galactic Nuclei from SDSS, LAMOST and DESI Surveys
› X-ray Polarization Signatures from Comptonization by Magnetic Reconnection Plasmoids
› GRB 260310A / SN 2026fgk: A Multi-Wavelength Study of a Nearby Underluminous Long GRB and SN with a Complex Afterglow
› Can finite-density QCD matter support a regular black hole core?
› X-Shooter survey of disk accretion in Upper Scorpius II. A lack of correlation between accretion rates and disk properties
› Are Cosmological Data Excluding Sterile Neutrinos or Only the Fully Thermalized Limit?
› Micron-Scale Technosignatures: How a Cubic Metre of Lunar Regolith May Begin to Constrain the Number of Past Technological Civilisations in the Galaxy
› Tidal origin of dark-matter free dwarf galaxies in the NGC 1052 group
› Refined reduction and standardisation of 53 years of UBV photometry at Hvar
› Detection of Quasiperiodic Oscillations in the Blazar PKS 0735+178 with TESS
› Predicting the final states of binary-single scattering with machine learning
› Exploring cosmic magnetism with gamma-ray burst afterglow emission
› Three-Dimensional Expansion of Iron Ejecta in Cassiopeia A with Chandra and XRISM
› Full-Covariance Bayesian Inference of Stochastic Gravitational Wave Backgrounds with Time-Domain Simulations for Taiji-like Missions
› $\texttt{Aether.jl}$ : A High-Performance 3D MHD and Multifluid Dust Code Written in a Dynamic Language with an Interactive Human-AI Development Framework
› The Galactic Centre G+0.633-0.0604 Molecular Cloud: A New Gold Mine for Astrochemistry
› Stress-Testing DANTE under Detector Domain Shift: a Representation-Coherent Reanalysis of LIGO O4a
› Halo Mass of ULIRGs at Cosmic Noon
› A Cross-Band (X-ray $\times$ Optical) Periodicity Search for Supermassive Black Hole Binaries: A Null Result and the First Completeness-Corrected Constraint
› Gravitational Waves and Cosmological Observables from First-Order Phase Transitions: Thermal Corrections at Low Temperature
› Testing a cosmological teleparallel modified f(T) model with parametric H(z)
› New constraints on axion with gamma-ray observations of the Crab Nebula
› Addressing the Hubble tension with Sterile Neutrino Dark Matter
› Ruling Out Spiky WIMP Dark Matter using Indirect Searches
› A Deep Learning Framework for Amplitude Generation of Generic EMRIs
› Nonperturbative suppression of beyond-General-Relativity effects in quadratic gravity
› Multi-field oscillons/I-balls in the Friedberg-Lee-Sirlin model

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