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Astronomia w Krakowie
Photo: The Mt. Suhora 60cm telescope
The Mt. Suhora 60cm telescope
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Allsky

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Temperature
5.7 °C

Humidity
 82%

Wind
1.6 km/h

Pressure
1025.4 hPa

Moon

Moon

 News from astronomynow.com
› Happy New Year, Mars! The Red Planet is turning 39
› 3I/ATLAS was born in the deep freeze
› Roman Space Telescope launches on mission to survey the Universe
› JWST’s ‘impossible’ early galaxies may be even more massive than we thought
› 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
RSS  Latest preprints on astro-ph:
› Resolving the heart of the Wolf-Rayet binary Apep with ALMA
› Discovery of eclipses in the cataclysmic variable MASTER OT J232100.42+494614.0
› Resolving the AGN Feeding and Feedback Cycle with ALMA2040
› Pathfinder results for populations of planet-forming discs with SKA
› The environments forming stellar and planetary systems
› Observational Signatures of Kerr Black Hole Lensing
› Hidden Disruption in Milky Way-like Satellite Galaxy Populations
› The bar-driven central complex of NGC 6946: A panchromatic and spatially resolved view of its star formation history and interstellar medium
› Four Which I Knew Not: The Hexadecapole Nearly Cancels the Octupole in Librating Kozai-Lidov Cycles
› Contrasting geometries of kiloparsec-scale stellar flows associated with giant Galactic cavities
› Let Sleeping Stars Li: Mapping Turnoff Lithium, the Lithium Dip, & Testing Standard Model Predictions in GALAH DR4 Subgiants
› An ALMA view on molecular complexity: water, methanol, and methyl formate in the HD 100546 and IRS 48 disks
› Combining Rubin and Roman photometry and its implications for photometric redshift estimation
› Searching for Dwarf Novae in 47 Tucanae
› The Magnetized Universe: From planet-forming disks to the high-redshift universe
› The LSST Science Pipelines Software: Optical Survey Pipeline Reduction and Analysis Environment
› The Occurrence of Circumbinary Planets Around TESS M-dwarf Eclipsing Binaries
› Primordial Power Spectrum from the Lensed CMB Temperature Spectrum using Iterative Delensing and Fourier Denoising
› Sparking Dynamic, Relativistic Magnetic Reconnection in a Twisted Flux Tube
› The transformative power of ALMA2040 for mm-VLBI
› Double Trouble: How Unresolved Spectroscopic Binary Stars Skew GALAH DR4 Stellar Parameters
› A New AI/ML Based Image Reconstruction Technique for Hard X-ray Coded Aperture Imagers
› Multi-modal transmission forecasting for the Vera C. Rubin Observatory
› Functional Analysis of Widefield Radio Interferometry
› Dust in Galaxies at $z=10-15$: Attenuation and Re-emission Predictions from the FirstLight Simulations
› A Multiwavelength View of SPLUS J102139.31-282247.5: an X-ray Luminous and Eclipsing Dwarf Nova
› Gaia in Technicolor. I. A Simple Variability-Encoded Color-Magnitude Diagram
› A Unified Solution to the Low-Mass X-ray Binary Diversity Puzzle: Saturated Magnetic Braking Coupled with Irradiation-Driven Winds
› Analytic and numerical study of dark matter halos in the Horndeski theory
› MIDSSAR: MId Dispersion Spectrograph for Stellar Activity Research
› $\texttt{GASTRO-BH}$: Effects of a Central Black Hole in GSE-like Dwarf-galaxy Mergers Around Milky Way-like Hosts
› On the foundations of anthropic reasoning: Implications for life across the universe
› The START mission: Probing the 2029 Apophis Flyby via a Low-Cost Geocentric SmallSat
› $N$-body simulations of the open cluster M67 -- I: global cluster properties
› How bright can a galaxy be? Extreme value predictions for high-redshift survey observables
› Gamma-ray calorimetry of Seyfert winds
› What can a uniform reflection pipeline establish about supermassive black hole spin? An audit and a corrected analysis of 57 AGN with XMM and NuSTAR
› Maximal efficiency of geometric beaming and polarization of highly super-Eddington X-ray sources
› Seeing Through the RFI Mask: DT-FISTA Inpainting of Pulsar Dynamic Spectra via Fourier Sparsity
› Extended J-band spectroscopy of red supergiants: parameter identifiability and metallicity robustness
› Ranking Prompt--Plateau Correlations in Gamma-Ray Bursts with Symbolic Regression
› Numerical study of multiple scattering intensities obtained from dust grains of different sizes and compositions in an impact-induced ejecta curtain
› A new submillimeter Class I methanol maser at 345.903 GHz near the massive protostar S255IR NIRS3
› Relations between optical spectral parameters and the (far-)infrared continuum in Type~1 active galactic nuclei
› Understanding sub-arcsecond scale radio sources and space weather with the SKA-Low using interplanetary scintillation
› The coordinated radio and infrared survey for high-mass star formation - VI. Higher-resolution follow-up of point-like northern ultra-compact H II regions
› The GAGE survey. I. Deep multi-band stellar variability characterization and automated classification toward Baade's window
› Milky Way Near Twins (MWNeTs). II. Applications of a Hierarchical Framework to NGC 3521, NGC 2903, UGC 11487, and CGCG 047-026
› Foreground Groups and Host-Galaxy Geometry in the Dispersion-Measure Scatter of Fast Radio Bursts
› The Dancing Bonfire: An Unusual Persistent X-ray Source in M81 Exhibiting Recurrent Luminous Flares
› Inferring the delay time distribution of type Ia supernovae with CAALAM I: SED modelling choices and their effect on the delay time distribution
› Comparing Infrared & X-ray-selected Active Galactic Nuclei host galaxy star formation rates to the galaxy main sequence
› A blazar is a blazar is a blazar ... Comparing long-term varaibility properties of PKS 1510-089 and PKS 2155-304
› Broad Line Regions behind a Haze II: A Three-dimensional Electron-scattering Model of the Broad Br$\gamma$ Line in NGC 3783
› Three-dimensional spatial modelling of nuclear de-excitation lines
› Prospects for Simultaneously Detecting Long and Short Duration Gravitational Waves from Pulsar Glitches with Current and Future Detectors
› Exploring Cosmic Rays from Gravity-Limited Acceleration at Supermassive Black Holes
› Impact of neutron captures on the r-process: I. Propagation of statistical model uncertainties
› Topological Defects in Cosmic Shear
› A Neural Network - Based Tool for Rapid Orbital Solution of Contact Binary Systems
› SN 2025wiu: A Type Ib Supernova with Post-Peak Optical Rebrightening
› ExHaLe-jet: Modeling blazar jets with an extended hadro-leptonic radiation code
› Isomer-resolved ion-molecule reaction kinetics of HCO+ and HOC+
› Can coupled thawing quintessence reproduce DESI DR2? A test with two potentials
› The Atmospheric Chemistry and Surface Interactions on Mars (ACSIOM) Workshop 2025
› Possible detection of Baryon Acoustic Oscillations imprinted in the HI sources from the FASHI catalog
› Galaxy bias of radio AGN and star-forming galaxies from MIGHTEE and CMB lensing
› A Hectospec Spectroscopic Census of Kinematic Members in the Orion Nebula Cluster
› Survey of Orion Disks with ALMA (SODA) IV: Millimeter variability of protoplanetary disks
› Does the inverse distance ladder rule out late-time solutions to the Hubble tension? A model-independent test using DES-Dovekie supernovae and DESI DR2 BAO
› BRISK: An accelerated wide-field imager for radio astronomy
› Characterizing the Martin Luther King Event: Sun to Earth Evolution of the January 19, 2026 Geomagnetic Storm
› Foreground dependence of the 20 GeV Galactic halo gamma-ray excess and its proposed connection to the LUX-ZEPLIN event
› A precessing AGN with S-shaped morphology discovered in MALS
› Clustering of JWST LRDs. Implications for PBHs and other early-forming seeds
› Gravitational Waves as a Probe of Multi-Fluid Cosmologies: General Formalism and the Case of Cosmological Stasis
› Revisiting the Mass and Scale Dependence of the "Lensing is Low" Effect with DECADE
› Detecting Exoplanetary Rings with Roman CGI Reflected Light Phase Curve Observations
› Entering the Era of Circumplanetary Ring Detection with Direct Imaging
› Flashing with colours: Photometric indicators of an early interaction in type II supernovae
› Geometrical and Optical Design of the GUEST Laser-Ranged Test Masses for the Detection of Gravitational Waves in the $\mu$Hz range
› Beyond Mergers: the Role of Metallicity in Forming a Reservoir of Massive and Detached Binary Black Hole Systems
› Long-Lived Charge Trap Characterization for Rare-Event Searches with Skipper-CCDs
› Star Light, Star Bright: Can Multimodal Models Parse an Astronomy Visual Question Answering Dataset Right?
› Modeling extreme mass-ratio inspirals in astrophysical and dark-matter environments
› No cosmic horizons from a strengthened higher-dimensional strong energy condition
› Constraints on Decaying Dark Matter with $B=1$ from Fermi-LAT
› Trapping of nanofabricated SiO$_2$ high-aspect-ratio discs in an optical lattice
› Pair-exchange dynamics of magnetohydrodynamic turbulence
› Native Geometry vs. Linear Recoverability: How Alignment Changes Platonic Scaling
› Laboratory Characterization of a Ge-CCD Prototype for Future Near-Infrared Astronomical Instrumentation
› Simulating dust collapse: the impact of gauge choices on primordial black hole formation
› The metric-affine $\mathring{R}^2$ scalaron: parameter-free inflation
› Andreev Beta Conversion and Bulk Viscosity in Superfluid Neutron-Star Matter
› Principle of no paradoxical Universe
› Hidden Sector Relic Abundances from an Effective Planck Mass
› Learning without relearning physical symmetry: an SO(3)-equivariant convolutional network (CNN) on the sphere
› ENFR: Evidence Networks with Flow-Matched References for Amortized Simulation-Based Model Inference
› New catalog of distances to planetary nebulae based on Gaia parallaxes and statistical distances
› Galaxy Luminosity Function of the Coma Cluster from Deep $u'-g'-r'$ Wendelstein Imaging Data
› Hydrodynamic instabilities in long-term three-dimensional simulations of neutrino-driven supernovae of 13 red supergiant progenitors
› Clustering effects on the Dark Siren determination of $H_0$: A simulation study
› Self-resonance preheating in deformed attractor models: oscillon formation and evolution
› A unified harmonic framework for dark siren cosmology
› Revisiting Constraints on Primordial Curvature Power Spectrum from PBH Abundances
› The Effect of Mass Loss and Convective Overshooting on the Pre-Collapse Structure, Composition, and Neutrino Emission of Red Supergiants
› Charged-current neutrino opacity within the relativistic Hartree-Fock framework for astrophysical simulations of core-collapse supernovae and binary neutron star mergers
› Can current models predict the local black hole merger rate?
› Constraints with CMB lensing on dark matter decays to massive decay products
› Cosmological constraints from the DESI DR1 Bispectrum Full-Shape and DR2 BAO
› Differentiable design of the PIAA-ZWFS: a flexible wavefront sensor that approaches the fundamental limit
› Transition from Diffusion to Drift-Dominated Cosmic Ray Transport and the Origin of the Knee
› FRANZ: Framework for analytical one-zone blastwave dynamics
› Gas Motions in Hydra-A: XRISM Constraints on ICM Kinematics Across Jet-Inflated Cavities
› A Deep Look at the Ultra-Faint Milky Way Satellite Virgo III with Rubin Observatory Data Preview 2
› An ALMA study of hub-filament systems II.Quiescent filaments converging towards highly dynamic hubs
› An "inside-out" approach to modeling supermassive black hole binary inspiral
› Bifrost spectral inversions: Fast non-LTE solar chromospheric diagnostics from 3D simulations
› HURACAN: A comparison of stellar and interstellar proper motions inside L1688
› Constraints from big bang nucleosynthesis and cosmological observations on varying Higgs vacuum expectation value
› IXPE observation of the new magnetar source EP J223759.5+531421
› Resistive alignment of a black-hole magnetosphere
› The origin of the high heavy-element content of warm Jupiters
› EMU detection of mysterious multiple component radio-continuum emission from nearby spiral Seyfert I type galaxy 'Sand-timer' (NGC 7213)
› Constrain the Size of Broad Line Region in NGC 1068 Using Sub-millimeter Excess
› Missed Detections and False Alarms in a CNN Technosignature Detector on Breakthrough Listen Data
› Dark Matter in the Galaxy: Insights from the Dynamics of Stellar Streams
› Chemical Demographics of Star-forming Regions
› NeuralDMD: Interpretable Neural Representation of Dynamics from Sparse and Noisy Measurements
› Scattered light noise due to dust particles contamination in the vacuum pipes of the Einstein Telescope
› Chaotic Imprints in Gravitational Waves from Extreme-Mass-Ratio-Inspirals Embedded in Dark Matter Halo
› Dark Photon mediated Inelastic Dark Matter in Cosmology, Astrophysics and Colliders
› Thermodynamic Gravity with Non-Extensive Horizon Entropy and Topological Calibration
› Cracking Gravitational Wave Multiple Ringdown Modes in Space
› Path-Degenerate Quantum Interferometry for Loss Resilience in Gravitational-Wave Detectors

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