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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
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Humidity
 94%

Wind
1.6 km/h

Pressure
1017.1 hPa

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 News from astronomynow.com
› 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
› Dark matter may come in multiple forms, new model suggests
RSS  Latest preprints on astro-ph:
› On modelling the 2017 galactic cosmic ray depression
› Dark Matter-Baryon Separability Predicts the Dynamics of an Almost-Dark Galaxy
› Small-Body Science with the Nautilus Space Observatory: From Cislunar Space Resilience to Mapping the Kuiper-Belt-to-Oort-Cloud Transition
› More than half of recent astronomy papers are written with language-model assistance
› Aletheia: Emulating the halo mass function with evolution mapping
› The relevance of the cosmic microwave background for cosmology
› A data processing pipeline for the WINTER near-infrared surveyor using the $\texttt{mirar}$ framework
› Emulator-Assisted Calibration of a Semi-Analytic Galaxy Formation Model for the Roman Galaxy Redshift Survey
› The CHIME/FRB Outriggers: Commissioning the Hat Creek Outrigger and an Updated Calibration Scheme for Mitigating RFI
› Energy deposition in planetary and exoplanetary atmospheres induced by cosmic rays
› Strong Black Hole Natal Kicks in Magnetized Accretion-Powered Explosions
› Sorting a mess I: Addressing velocity-axis correlation of cross-correlation functions. A census of atomic and ionised species in KELT-9b's atmosphere
› PBH runaway during reheating
› Detection of hard X-ray pulsations in non-ULX X-ray pulsar 3X J0042 in M31
› Probing dynamics of extreme galaxies I. Dark matter content in ultra-diffuse galaxies
› Predictions for astrometric microlensing in Gaia
› BIND (Baryonic INpainting with Deep learning): A Field-level Emulator for Galaxy Groups and Clusters
› BINDing the lightcone: A suite of astrophysical ray-traced weak lensing and SZ maps
› WASP-43b TESS Phase Curve Mapping: Evidence for a Hot Interior
› Teglon: A Pixel-Level Pipeline for Galaxy-Informed Gravitational-Wave Follow-up Planning and Efficiency Analysis
› Hbeta Spicules, Small-scale Jets, and Hbeta Microflashes: Sub-arcsecond Dynamic Events and their Magnetic Origins in the Lower Solar Chromosphere Observed by DKIST
› Solar Flare Prediction Using a Hybrid Convolutional Neural Network and Transformer Model
› A Novel Approach to 3D Dust Mapping of the Central Molecular Zone
› Low-Mass Magnetic Monopoles in the Galaxy: Simulations and Comparison with Ultra-High-Energy Cosmic-Ray Data
› UX Men: Detached Eclipsing Binary as a Benchmark Candidate
› $w_0w_a$ or $bc$: DESI constraints on relative baryon-CDM perturbations
› The THRILS Factor: Investigating the properties of Little Red Dots (LRDs) at 3
› Instrument-Level Validation of Upper Sideband Syntonization Concept
› Fast and Furious: Long-term orbit integrations with collocation integrator Lobbie
› Magnetising the quokka code with fast, second-order accurate, error-correcting schemes for magnetohydrodynamics on GPUs
› Frozen-composition effects on rotational failure of neutron-star crusts
› XRISM observations of the Perseus cluster along two arms: Chaotic ICM motions probed by resonant scattering
› Constraining Tidal Migration with the Hot Jupiter Population
› Studying Outflows with Synthetic Absorption Line Spectra from High Resolution Simulations
› Impact of LSST systematics on stellar-stream density fluctuations for dark matter
› Towards High-Throughput Visible Photonic Lanterns for the EMARCOT Project
› IceCube neutrino point-source searches in the direction of the KM3NeT ultra-high-energy event
› Fast Dynamical Modelling of Milky Way Globular Clusters -- II. Impacts of Black Hole Prescriptions
› Eclipse Properties and Superhump Evolution in the SU UMa-Type Dwarf Nova Z Cha
› Constraining spinning primordial black holes with interstellar dust heating
› Classical Nova V1405 Cas Had $M_{\rm ejecta}$$>$$M_{\rm accreted}$ and so is Unlikely to be a Type Ia Supernova Progenitor
› Two-parameter continuous deformation of Starobinsky inflation as a bridge between Planck and ACT DESI data with $N_\star\in(50,60)$
› Science operation, data handling, and ground support system of the SOLAR-C mission
› A prolonged plateau-to-tail transition in the Type II supernova SN2025abyc
› Uncovering the Origin of Slow Rotators among Intermediate-Mass Stars in the Star-Forming Cluster Trumpler 14
› A Tale of Two Gauges: Effective Field Theory for Relativistic Behavior of Cosmological Axions
› (Re)constructing Accurate Axion Oscillations
› Evidence for the binary nature of the long-period radio transient ASKAP/DART J1832-0911
› SPURS: An Ultra-deep View Inside the Compact, Nitrogen-Enriched Nuclei of Little Red Dots
› Nitrogen-Loud Quasars from the Dark Energy Spectroscopic Instrument. I. Sample Selection and Basic Properties
› Statistical evidence for linear combination frequencies in {\gamma} Doradus stars being nonlinear resonant modes
› The EDD Radio Astronomy Backend Framework
› SMART : Spherical Mass ApeRture Toolkit
› Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster
› Non-axisymmetric Transport of Magnetic Flux Tubes: A Mechanism for Joy's Law and Poloidal Field Generation via Meridional Flows
› Nonbirefringent model of orthogonal polarization modes in radio pulsars - New view on S swing and mode structure in pulsar beam
› Initial clustering of primordial black holes: A general formulation for arbitrary local non-Gaussianity
› No Detectable One-halo Galactic Conformity Signal with Halo-mass Estimates Consistent with Weak-lensing Constraints
› Constraints on the fuzzy dark matter mass using globular clusters in dwarf galaxies from Euclid ERO data
› Lava Tube Exploration with LunarLeaper
› The properties of central stellar knots embedded in galactic bulges of CIELO simulations
› Spin-down of the accreting magnetar candidate 4U 0114+65: possible first evidence for a strong coupling regime
› Tracing Warm Gas through C IV Radiative Transfer
› Resonantly Scattered CIV Emission in Local Star-forming Galaxies: Radiative Transfer Constraints on High-ionization Gas in Reionization Analogs
› Generating the wide sequence of Diffuse Galaxies with de Broglie waves of Dark Matter
› Cosmological Evolution of Primordial Black Holes: UV/IR Decoupling and the KM3NeT 220 PeV Neutrino Anomaly
› Evidence for plasmoid formation related to a hot UV burst in the solar atmosphere
› Evidence for CME--CME Interaction in a Magnetic-Cloud-Like Ejecta: Insights from Multipoint Observations and Polytropic Analysis
› Testing Chemical Tagging with LAMOST: Intrinsic Abundance Dispersion of Subgiant Stars in the Galactic Disk
› The MICADO first light imager for the ELT: the PSF Reconstruction Software
› Towards First Light for MICADO: Validation of the PSF-R service with real data
› An RFSoC-based Backend and Timing System for the Balloon-borne Very Long Baseline Interferometry Experiment
› Probing the details of relativistic electrons with multifrequency observations of M87 black hole
› One Precessing Jet Pair, Diverse Core-Collapse Supernova Remnant Morphologies
› TDCOSMO XXXI: New techniques in line-of-sight studies of time delay lenses
› The atomic multiphase interstellar medium of galaxies in the COLIBRE simulations
› The Balloon-borne VLBI Experiment (BVEX) Radio Telescope and Position Tracking System
› Bayesian Superiority in On/Off analysis
› Relativistic Magnetohydrodynamics from Myers-Pospelov Lorentz-Violating Electrodynamics
› Spectral evolution of NS binary system GX 349+2 using AstroSat observations
› Planetary Accretion Is Less Frequent in Wide Binaries: Evidence from Metal-Enriched White Dwarfs in DESI DR1
› The Dyn-Atmo Survey: High-contrast Imaging Spectroscopy of the Substellar Companion HD 13724 B with the JWST NIRSpec IFU
› The Dyn-Atmo Survey: JWST/NIRSpec spectroscopy of dynamical benchmark GJ 758 B
› A Homogenized Catalogue of Variable Stars in the Globular Cluster M22: Membership, Physical Parameters, and Distance
› Learning JWST. I. A Foundation Model for New Population Discoveries and Morphology-Aware Photometric Redshift Measurements in the JADES Survey
› Hierarchical Population Inference with Normalizing Flows for Binary Black Holes
› Reconstructing Early Primordial Black Hole Domination from Gravitational-Wave Backgrounds
› A Multi-Axion Ladder Across Cosmic History: From Inflation, BBN, and Early Dark Energy to Late-Time Accelerated Expansion
› Teleparallel torsion and white dwarf structure in \(f(T)=T+\Xi T^2\) gravity
› The Mysterious Inspiral of WASP-12b: Why Obliquity Tides Cannot Drive Orbital Decay
› Perturbations of Charged Black Holes with Higher-Order Interactions
› Post-fabrication trimming of a 1024-pixel, single-photon counting, Microwave Kinetic Inductance Detector array with a pixel pitch of 150 micron
› Beyond the BLUE I: the advantage ceiling - how much can any estimator beat the matched filter in mm/submm survey data?
› For Whom Does Bell Hold?
› Einstein and the Solar Eclipses - Why Albert Einstein joined the Astronomische Gesellschaft in Potsdam 1921
› The Crab Nebula progenitor: recovering the 1054 AD supernova event as galactic Gamma-ray burst
› Implications of Inelastic Dark Matter for Primordial Dark-Star Evolution: Kinematic Thresholds and Nonthermal Capture
› Ultralight Axial Dark Matter
› On the Numerical Integration of One-Loop Cosmological Collider Signals
› Re-examining the sensitivity of JWST to decaying axion dark matter
› Wave optical imaging of an oscillating electric dipole orbiting a black hole
› EFT Approaches to Sommerfeld Enhancement and Bound States in Singular Potentials
› Binary-black hole spin population results may be driven by prior degeneracies
› New Method for Path-length Equalization of Long Single-mode Fibers for Interferometry
› Higgsino dark matter in the Starobinsky supergravity with the MSSM in light of the LUX-ZEPLIN event
› Nuclear-physics-guided Gaussian Processes
› Might the radiation era extend back to the Big Bang? On dark matter production and the relic graviton background in quadratic gravity
› Solar Neutrino Constraints on Inelastic Dark Matter Scattering in Light of Recent LUX-ZEPLIN Observations
› Theoretical Aspects of Direct Waves in Kerr Black Holes: Pole-Splitting Method for Ringdown Analysis
› Properties of molecular clumps and cores in colliding magnetized flows
› Robust Joint Estimation of Galaxy Redshift and Spectral Templates using Online Dictionary Learning
› Precision spectral estimation at sub-Hz frequencies: Closed-form posteriors and Bayesian noise projection
› Hot New Early Dark Energy: Dark Radiation Matter Decoupling
› Model-Dependent Galactic Environment Effects on Multi-Transonic Accretion and Emergent Acoustic Gravity around Kerr Black Holes
› Height-dependent thermal properties of extreme-ultraviolet campfires in the quiet Sun
› Optimizing Photometric Redshift Training Sets I: Efficient Compression of the Galaxy Color-Redshift Relation with UMAP
› Dark Acoustic Oscillations as an Early-Universe Explanation of the DESI Anomaly
› Hidden Vela Supercluster Revealed by First Hybrid Redshift & Peculiar Velocity Reconstruction
› Cosmological Constraints from Gravitational Wave-Fast Radio Burst Associations without Redshift Measurements for LIGO-Virgo and Cosmic Explorer
› Deciphering the IceCube Diffuse Neutrino Observations via AGN Variability
› Precision Kinematic Sunyaev--Zel'dovich Measurements Across Halo Mass and Redshift with DESI DR2 and ACT DR6: Part I. Luminous Red Galaxies
› Statistical evidence for massive black hole recoils in active galactic nuclei
› Inflaton accretion onto primordial black holes during reheating
› Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations - II. The role of AGN feedback and environment on their emergence
› Investigating the young stellar populations and hierarchies in nearby galaxies with the UVIT. II. Presenting the properties of ~25,000 UV-detected star-forming clumps
› Galaxy clusters in the VIDEO fields: detection and characterisation in the context of MOONRISE
› A Population of Little Red Dot-like Quasars in SDSS
› Mass-Ratio Reversal as an Alternative to Hierarchical Mergers for GW241011
› Effect of Ice Charging on the Astrochemistry of Interstellar Sulfur Bearing Species on Amorphous Solid Water
› Resolving dense photodissociation regions: the structure of photochemical fronts in three-dimensional gas distributions
› Beyond $w_0-w_a$ and Phantom Crossing: Testing Models of Coupled Dark Sector
› The Venus Benchmark: Resolving Degeneracies in Terrestrial Exoplanet Spectra with DAVINCI
› Two extremely irradiated volatile-rich sub-Neptunes with companions in the TOI-426 and TOI-1839 systems: Insights into arrival and survival near the lower edge of the Neptunian desert
› Unresolved triple systems in the aged open cluster Trumpler 19: Discovery, confirmation, and implications
› Interstellar Complex Organic Molecules and Molecular Outflows in NGC 1333 IRAS 4B and 4B' Observed Using NOEMA
› TEMPUS: Relativistic coordinate time scales for any solar-system body from arbitrary ephemerides
› Open Clusters as Laboratories for Cool Star Evolution: Highlights from the Cool Stars 23 Splinter Session
› Characterization of Orbits in Bars in Disc Galaxies Using Fourier Frequencies
› Dark matter interpretation of GRB 221009A: a singlet scalar explains LHAASO data
› Post-Reheating Inflaton Production as a Probe of Reheating Dynamics
› Laboratory measurements of energy partitioning and anomalous electron heating in magnetized, perpendicular collisionless shocks
› Properties of neutron stars with hyperons within a generalized relativistic approach
› Effective dissipative cosmology with $\Lambda$ from the first law of thermodynamics
› Systematic Biases in Gravitational-Wave Parameter Estimation from Neglecting Orbital Eccentricity in Space-Based Detectors
› Electro-Weak Phase Transitions and Collider Signals in the Aligned 2-Higgs Doublet Model
› Inflaton Regeneration via Scalar Couplings: Generic Models and the Higgs Portal
› Constraining dark matter self-interaction from kinetic heating in neutron stars
› Data-Driven Acceleration of Eccentricity Reduction for Binary Black Hole Simulations
› Baryoid Dark Matter from $\mathbb{Z}_N$ Domain Walls: The $(N-1):1$ origin of the dark matter-baryon coincidence
› Molecular clouds constraints on sub-GeV DM and asteroid-mass PBHs
› Breakdown of the Plane-Wave Trojan Horse Analysis of the $^{12}\mathrm{C}+{}^{12}\mathrm{C}$ Fusion Reaction: Critical Role of Coulomb Distortions
› Project Setu: 3D Multi-Physics Design and Scaled Structural Analysis for a Relativistic Lightsail Architecture
› Solar Capture Tests of Inelastic Dark Matter after the LZ High-Recoil Event

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