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Astronomia w Krakowie
Photo: Dome at sunrise
Dome at sunrise
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Temperature
9.6 °C

Humidity
 70%

Wind
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Pressure
1024.7 hPa

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 News from astronomynow.com
› 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
› Witness to history: Artemis II, lunar exploration and hope
RSS  Latest preprints on astro-ph:
› TNFlow: Amortized Posterior Inference for Trans-Neptunian Object Surface Composition
› Nebular Spectra of the Extremely Metal-Poor SN II 2023ufx Over a Year After Explosion: A Massive Progenitor and Unique Circumstellar Environment
› Supernova microlensing as a probe of ultracompact minihalos and primordial cosmology
› A Swift X-ray view of the SMS4 sample - III: Deeper insight into previously undetected sources
› Development of quantum technologies for optical/infrared interferometry
› ALPACA I: Controlling source and PSF systematics in JWST time-delay cosmography with differentiable lens modeling
› It's All About the Environment: Local $f_{\rm NL}$ from a Dark Matter Conditioned Multitracer Analysis
› The DESI Data Release 1 white dwarf catalogue
› JWST/NIRSpec Reveals Diverse Nuclear Environments in Dwarf Galaxies Hosting AGN
› A Kinematic Measurement of the Effective Viscosity of the Intracluster Medium: The Cold Front of A3667 Seen by XRISM
› Super-Eddington Accretion and Early-Stage Feedback in Ton S180
› Composition gradients in sub-Neptunes: K2-18 b and TOI-270 d as case studies
› Resolved Dust-Gas-Metallicity relations in nearby spiral galaxies
› AGN-DB: A Unified Multi-Wavelength Database of Active Galactic Nuclei
› Improvements to Asteroseismic Fitting of White Dwarfs in the Gaia Era
› Recovering Ionizing Photon Escape and Galaxy Scaling Relations in the LzLCS via Si II and C II Absorption Lines and Mock Spectra from a Radiation-Hydrodynamic Simulation
› Widespread Inflows Reveal Baryonic Cycling in Star-forming and Quiescent Galaxies
› Model Predictive Scoring Shows Specific BAO Observations (not SNIa) Drives $w_0w_a$ Tension
› H I Absorbers as Beacons of Hidden Structure at $z \sim 3$: Multi-Component, Metal-Rich Absorption System near a Protocluster
› Extending the Stellar-to-Halo Mass Relation to Dwarf Galaxies with DESI DR1
› Hint of bimodal Mg-Al anticorrelation in the metal-poor Globular Cluster NGC 4372
› Linking orbital history to the quenching of isolated dwarf galaxies
› KKR 18: A Late Arrival Galaxy?
› Circumbinary planets in coplanar triple-star systems: I. Minimum eccentricity variation region
› Identifying Casual SETI Transmissions and Ultra-Faint RFI with Cumulant Imaging
› The Super-Sample Covariance of Line-Intensity Mapping Power Spectrum
› Preferential accretion onto eccentric and unequal binary black holes
› Implementation of frequency-correlated noise in CMB component separation: Method, Validation, and Early Applications
› Star Formation Evolution in Galaxy Pairs: Constraints from Morphological Disturbances and Recent Star Formation Histories
› A Cross-Laboratory Comparison Study of Titan Haze Analogs: Surface Energy II
› Retrieving Ocean Glint Reflectance Signatures from Directly Imaged Earth-like Exoplanets
› A Differentiable Neural Surrogate for Photon Propagation in Neutrino Telescopes
› Validating the SCALES DRP: A Performance Study of the Medium-Resolution IFS Mode
› Evidence of Orbital Evolution of Gigahertz-Peaked Spectra in Binary Millisecond Pulsar
› Studies on the dark sector interaction from joint analysis of cosmological probes
› Through a glass, darkly: a combined framework for estimating fast radio burst host galaxy and population properties in an era of uncertain host identification
› The angular structure of the GW170817 jet from prompt emission alone
› Signatures of rocky debris accretion in AF-Type planet hosts
› A guide to choosing data compression methods for cosmological inference
› Membership Determination of 45 Open Clusters Beyond 3 kpc
› Habitable-zone Earths at the detection frontier: Measured completeness and false-alarm rate of a transit pipeline for the PLATO M-dwarf sample
› Quantifying collision-driven mass loss in supermassive star formation: the role of stellar structure and accretion
› Disk dispersal freezes overstable resonant librations
› Multi-Wavelength Post-Perihelion Polarimetry of Interstellar Comet 3I/ATLAS
› The metallicity of giant exoplanets around low-mass stars and how Ariel can help
› Mapping the WISPIT2 Planet-Hosting Cavity at Sub-Hill-Radius scales
› Rubin J122659.4+090236: An Extremely Low Surface Brightness Galaxy Candidate Discovered in the Rubin LSST Early Data Preview 2
› Updated in-flight calibration of the Hayabusa2/NIRS3 spectrometer: new global near-infrared photometric properties of asteroid (162173) Ryugu
› Late-Time Emergence of Dark Energy and Its Interaction with Dark Matter
› Expanding the scope of dark siren cosmology: Inferring the population properties of gravitational wave-hosting galaxies
› The October 2022 flare in OJ 287 and the mass of its primary black hole
› Corona Australis 151: an extremely young protostar
› Nonstationary Stochastic Timing Signatures in the Prompt Gamma-Ray Light Curve of GRB 170817A
› Supernovae Unite: Combining Pantheon+ and DES-SN5YR
› Gravitational instability in planet-forming discs
› Modelling Palomar Transients: Constraints from Reflection Geometry and Orbital Altitude
› Can isolated binaries form unequal-mass binary black-hole mergers with a high-spin primary black hole?
› Stability of circumbinary planets: the role of binary properties and migration scenarios
› Euclid. A two-point correlation approach to diagnosing star-related systematics in the Euclid spectroscopic survey
› PPN--spin degeneracies in mock S62-like stellar-orbit inference
› The dispersal law of young star clusters: free expansion -- A Gaia/eROSITA census of Orion and Sco--Cen
› Laboratory characterization of Hierarchical Fringe Tracking
› Active focal plane phase mask coronagraphy with a discrete pixelated device: I. Study of the theoretical performance trade space
› Exploring the connection between Fast Radio Bursts and binary neutron star mergers
› Stellar Population and Dynamical Modeling of Galaxies with Kinematically Misaligned Components: Age and Metallicity of Structural Components
› Planetary gas gaps and kinematic signatures in the planet forming disk around WISPIT 2
› What is new in NuRadioMC: Multilayer Analytic Raytracer
› A Homogeneous Survey of JWST MIRI Transmission Spectra of 10 Exoplanets
› Enabling Metallicity Measurements of Microlensing Lenses through Multi-band Lens Photometry
› Energy Partitioning at the Termination Shock
› ROCKETS I: Investigating the Impact of the Rocket Effect on Two Nearby Young Open Clusters Encased in Infrared Bubbles
› Rapid quenching and early gas depletion in the core of a galaxy protocluster at z=2.2
› JWST Excludes Exomoons Down to 0.1 Earth Radii Around a Rocky, Temperate Exoplanet
› Evidence for LP 890-9d via Transit Timing Variations
› Supernovae Unite: Host-Galaxy Mass Measurements of Type Ia Supernovae and Their Impact on Cosmology
› Contrasting C/O ratios in Uranus and Neptune from disequilibrium chemistry: A clue to distinct evolutionary pathways?
› Electromagnetic alignment and jet precession around supermassive black holes: Quasi-periodic oscillations in tidal disruption events
› Dust Substructures and Line Perturbations driven by a Forming Planet in J16120
› Ion abundances in the plasma tail of 3I/ATLAS show that it is N2-rich
› Metallicity dependence of Wolf-Rayet binaries using detailed binary models: An absence of long-period systems at low metallicity
› Early against Late: A contrast on dark energy in the light of DESI DR2
› Tracing the Cosmic Origins: Machine Learning Reconstruction of the Primordial Density Field from EoR Observations
› 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
› Waveform models for the gravitational-wave memory effect: III. Phenomenological frequency-domain model for nonspinning binaries
› Stability of Collective Neutrino Oscillations -- A Distributional Approach
› Breakdown of the Plane-Wave Trojan Horse Analysis of the $^{12}\mathrm{C}+{}^{12}\mathrm{C}$ Fusion Reaction: Critical Role of Coulomb Distortions
› Probing Dark Matter with Strongly Lensed Binary Black Hole Mergers: Prospects in the Near Future
› Probing Neutron Star Equation of State Universality with Gravitational Waves
› Fast Bayesian Inference for Long-Duration Gravitational-Wave Signals in 3G detectors
› Interpreting the Hubble tension with a cascade decaying dark matter sector
› A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
› Mass dependence of halo baryon fractions from the kinetic Sunyaev-Zeldovich effect
› Not all cores are equal: Phase-space origins of dynamical friction, stalling and buoyancy
› Design and Performance of the Upgraded Prototype Schwarzschild-Couder Telescope Camera Module
› The Third Option: Color Phase Curves to Characterize the Atmospheres of Temperate Rocky Exoplanets
› GAME: Genetic Algorithms with Marginalised Ensembles for model-independent reconstruction of cosmological quantities
› Radiation GRMHD Models of Accretion onto Stellar-Mass Black Holes: III. Near-Eddington Accretion
› ODIN: Confirmation and 3D Reconstruction of Six Massive Protoclusters at Cosmic Noon
› High efficiency superconducting filterbank with impedance-defined resolution for millimeter-wave spectroscopy
› A generic $\omega_b$ tension in early-time solutions to the Hubble tension
› Dark ages bounds on nonaccreting massive compact halo objects
› The Low-$\alpha$ Splash Population in the Milky Way
› Puzzling Ultra-Diffuse Galaxy Evolution (PUDGE). II. A transformation pathway from ultra-diffuse galaxies to compact dwarfs in galaxy clusters
› VROOM-SBI: A Fast Simulation-Based Bayesian Inference Methodology for Stokes QU-Fitting in Radio Interferometry
› Collisional excitation of H$_2$CO by He: Experimental validation of state-of-the-art scattering calculations
› Rogue Ones: Orbital census of Galactic Cepheids and their Anomalies
› Effects of Rotation on the Gravitational Momentum Transfer in Neutron-Star Kicks and Implications for Spin-Kick Alignment
› Ice Giants Revisited: Uranus and Neptune as Magma Ocean Worlds
› Stellar proper motions compared with the plane-of-sky magnetic field
› Dependences of radio pulsar parameters on the kick velocity
› UV artefacts in ultra-slow-roll models of inflation
› Periodic Radio Technosignature Search toward 3I/ATLAS with FAST
› Hubble tension: the shape wall
› The Non-Principal-Axis Rotation and Convex Shape Model of Earth Quasi-Satellite and the Target of China's Tianwen-2 Mission (469219) Kamo`oalewa
› Exploration of Exoplanet Atmospheres with the James Webb Space Telescope
› Concerns regarding recurrent fluorescence's impact on smaller diffuse ISM aromatics
› Demonstration of a multimode-to-multimode photonic lantern for astronomy
› Revisiting the Hubble tension with an inverse power-law early dark energy
› Dissecting ultra-diffuse galaxies in the field
› Reconciling Galactic rotation curve constraints with stellar stream modeling
› Complex Lags from Simple Physics
› Energy deposited by black holes in the hot X-ray gas of elliptical galaxies, groups and clusters
› 3.5-meter Segmented-Mirror Robotic Space Telescope Mission White Paper I. Overall Architecture and Scientific Mission
› Topological dark energy from spacetime foam: A challenge for $\Lambda$CDM
› Study of neutrino spin oscillations in a gravitational field with a differential equations method
› Naturally small Dirac neutrino mass and $B-L$ dark matter
› Leveling of MHD turbulence imbalance in shear flows
› Mapping Dark-Matter Clusters via Physics-Guided Diffusion Models
› Experimental evidence for coronal mass ejection suppression in strong stellar magnetic fields
› Three-dimensional recoil-electron reconstruction using combined optical imaging and waveform readout for electron-tracking Compton cameras
› Neutron Portal and Dark Matter-Baryon Coincidence: from UV Completion to Phenomenology
› Strong Constraints on Line Signals from Dark Matter Annihilation in a Nearby Subhalo

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