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Astronomia w Krakowie
Photo: Dome at sunrise
Dome at sunrise
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Temperature
2.6 °C

Humidity
 94%

Wind
0.0 km/h

Pressure
1014.7 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:

› Alignment-driven binary evolution in warped circumbinary discs: 3D moving-mesh hydrodynamics of eccentric and inclined binaries
› Newtonian I-Love-Q relations: An enthalpy-based approach
› A Study of the 30 May 2026 Meteor Event Employing Data from Raspberry Boom Infrasound Sensors in the Boston Area
› Non-Axisymmetric Pillar Structures due to Embedded Stars in AGN Accretion Discs
› An Extra-nuclear Water Maser in NGC 1106 Likely Driven By An AGN Shock: Implications for Maser-based Black Hole Mass Measurements
› Image Morphology of Misaligned Magnetically Arrested Disks
› From Inspiral to Outburst: Modeling a Potential Luminous Red Nova from Betelgeuse
› Collapsars Are Not Heavy $r$-Process Factories
› Prospects of Detecting Cosmological Domain Walls in the Cosmic Microwave Background
› FastSpec: Fast and versatile stellar spectrum synthesis code
› The Galactic Center Reference Frame: A 30-Year Solution
› AMICO galaxy clusters in KiDS-1000: Cosmological constraints from the two-point correlation function
› The Impact of Orbital Data Centers on the NSF-DOE Vera C. Rubin Observatory
› Demographics of Close-In TESS Exoplanets Orbiting FGK Main-sequence Stars II. Spectral-Type Dependence and the Neptunian Landscape
› Cluster connectivity in DES Y3 data: impact on galaxy properties
› Physics-Informed Neural Networks vs U-Net: Application to thermal dust emission recovery in the microwave
› Best Bulk Bennu (B3): Elemental compositions of aggregate samples from asteroid Bennu
› Listening to the Standard Candles: A Survey-Scale Search for Phase-Coded Beacons in Cepheids, RR~Lyrae and $\beta$~Cephei Stars
› Semi-Analytic Predictions for Strong-Lensing Perturbers in Cold and Self-Interacting Dark Matter
› Discovery of activity on Main Belt Asteroid 6993 (1995 BJ4)
› The SDSS-V Local Volume Mapper (LVM): Technical Overview
› Tilt, warp, and dissipation flare in hydrodynamic disks around kicked compact objects
› The Impact of Inclination, Redshift, and Mass Ratio Selection on Cosmological Constraints from Bright Sirens Beyond Conventional Fisher Approximations
› OGLE-2015-BLG-1395Lb: A Cold Sub-Saturn Mass Planet Orbiting an M Dwarf
› A Unified Model for Radioactive Signatures and Source Identifiability in Neutron Star Mergers
› FacilityAudit-Agent: Beyond Mention-as-Usage for Fine-Grained Facility Contribution Attribution in Astrophysics Publications
› SMMAN Studies of AGN Variability. I. Long-term Spectral Evolution and a Candidate $\sim1000$-day Quasi-periodic Modulation in 4C+72.28
› Galaxy Luminosity Functions at z~7-10 from Four Years of JWST Observations
› Radio Galaxies as UHECR Sources in Light of Recent Microquasar Results
› A Framework for Analysing Nebular-Phase JWST Supernova Spectra with Application to Type Ic SN 2024aecx
› Differential and integral scaling laws of the mass density of molecular clouds
› Probing Red Giant Interiors with g-Dominated Mixed Modes II: The Cases of KIC 6117517, KIC 9475697, KIC 10123207 and KIC 10200377
› Estimation Of The Mass And The Spin Of The Neutron Star 4U 1728-34 Using Triples Of X-Ray Quasi-Periodic Oscillations
› Introducing the GION Lightcone Simulation Suite for Multi-Wavelength Large-Scale Structure Cosmology
› A comprehensive reanalysis of HD 99458. Not a magnetic Ap star but an oscillating Algol with ongoing mass transfer
› Binary Dynamics and Mergers in a Stellar Disk and the Formation of Dusty Objects in the Galactic Center
› Local Analogs of Little Red Dots: Clues to the X-ray Weakness
› Luminosity-weighted galaxy and gravitational wave cross-correlations
› Star clusters at cosmic dawn I: the emergence of the initial cluster mass function
› Comparison of observed and theoretically calculated amplitudes of Forbush effects for events associated with the arrival of a shock wave
› The MIRI/MRS Library. III. Detector-based optimal spectral extraction and high-contrast imaging applications
› The Galactic rotation curve from the ALS III catalogue of OB Stars
› Accuracy of electric current inference assuming three-dimensional hydrostatic equilibrium
› Forward model of the Gaia DR3 selection function
› Polarization Observations of NGC 315 with FAST
› Spatial distribution of star formation in dwarf galaxies: Merger-driven and secular starburst
› Magnetic Reconnection Modifies Cosmic-Ray Transport in the Interstellar Medium
› Tracking the Evolution of Supermassive Black Hole Binaries with Pulsar Terms
› Systematic Slopes in NIRSpec BOTS Observations
› ARENA: Active Region attENtion Aggregation for interpretable solar flare prediction
› Probing the star-forming environment of GRB across cosmic ages with high-resolution X-ray spectroscopy: From \textit{{XMM-Newton}}/RGS and \textit{XRISM}/Resolve to \textit{NewAthena}/X-IFU
› Joint Angular-Power Distributions of Interfering Nanohertz Gravitational Waves
› The GAPS Programme at TNG LXXXI. The puzzle of the HeI absorption signal in the atmosphere of V1298 Tau b with GIARPS@TNG
› Research of signs of star formation in three S0 galaxies - members of isolated pairs
› Diversity of planetary origins and compositions traced by stellar abundance differences of co-natal star systems
› The Physics of the Cold and Warm Interstellar Medium Through Radio Recombination Lines
› Modelling kNN-CDFs of biased tracers in redshift space using hybrid Lagrangian bias expansion
› Physics Informed Neural Network for Multi-dimensional Turbulent Self-gravitating Flows
› The Galactic Center Gamma-Ray Excess and the Look-Elsewhere Effect
› GRB 260924A: Extreme Energetics, Bright GeV Emission, and Exceptional X-ray and Optical Luminosity
› The ALMA Survey of Gas Evolution of PROtoplanetary disks (AGE-PRO): Evolution of dust properties from multi-wavelength observations
› Complete Multi-Band Structural Characterization for 10 Million Galaxies in the Hyper Suprime-Cam Wide Survey using Deep Learning
› A Population Synthesis Model for Odd Radio Circles Produced by Shock-Bubble Interactions
› One-Million-Year-Old Nascent Eclipsing Binaries in the LMC
› Three subpopulations of binary black holes in mass, spin magnitudes and tilts following GWTC-5
› ExoVetter and a TESS Exoplanet Transit Search of Kepler Stars as Ground Truth
› A probabilistic approach to separate mergers and jellyfish galaxies: Application of morphological non-parametric indexes to the DESI Legacy Survey
› Comprehensive Visible and Near-infrared Keck and Gemini Monitoring and Characterization of Interstellar Comet 3I/ATLAS during its Encounter with the Solar System
› Exceptional points and hysteresis in Kerr-Newman quasi-normal modes
› Gravitational waves from inclined orbits around Kerr black holes
› Non-Markovian Cosmology with Causal Memory Kernels
› Finite-distance effects and scalar suppression in massive gravity
› Magnetic field effect on neutral color superconductivity as a mechanism to boost the inner magnetic field of magnetars
› Stochastic dynamics of cosmological inflation in general relativity
› Gauge-field energy density in inflationary kinetic-coupling models: QFT regularization versus horizon cutoffs
› Natural Inflation with Exponentially Small Tensor-To-Scalar Ratio
› Euclid: Quick Data Release (Q1) -- Ultracool dwarfs in the Euclid Deep Fields
› Resilience of Primordial Black Hole Formation from Inflation with a Light Spectator Field
› Tracing the evolution of eccentric precessing binary black holes: a hybrid approach
› Testing the Correlations between X-ray Spectral Properties and Polarization for High Synchrotron Peaked Blazars
› Primordial Black Holes from Inflation with a Spectator Field
› OmniSpectra: A Unified Foundation Model for Universal Spectra Representation Learning
› Cosmological Equivalence of Scalar-Tensor-Vector Modified Gravity and Cold Dark Matter
› Kinematic cosmic dipole from a large sample of strong lenses
› Quantitative modelling of type Ia supernovae spectral time series II: Exploring the diversity of thermonuclear explosion scenarios
› Toward Bayesian photometric cosmic chronometers: Application to VIPERS
› Stellar Population Spectra Incorporating Detailed Binary Evolution using POSYDON
› UCLCHEM 4.0: An open source gas-grain astrochemistry simulation framework
› The Best Guess: Testing new and old formalisms for the common envelope against observations
› What visibility-graph curvature measures in Forbush decreases: a calibration on the two largest events of solar cycle 25
› Even central galaxies feel their environment: cosmic siphoning of cool gas accretion
› Effective reheating in Gauss--Bonnet inflation with $\mu(\phi,X)$ coupling
› Astrophysical Constraints on Hadron--Quark Crossover in Hybrid Neutron Stars
› Decoupling candidate dual AGN from chance superpositions in the GOTHIC survey via a deep-learning framework
› AXIS Could Have Accessed Dark Matter Decays
› Tracing the Cosmic Origins: Machine Learning Reconstruction of the Primordial Density Field from EoR Observations
› The Loud Tail of the Supermassive Black Hole Binary Population: Multimessenger Candidates and Prospects for SKAO
› Machine Learning $\beta$-decay Half-lives and Their Application to $r$-Process Observables
› Separating the Optical to Near-Infrared Light of AGN and Their Host Galaxies
› Radio Continuum Study of One of the Brightest Large Magellanic Cloud Supernova Remnants N 132D
› CosmoAgent: AI Agent for Theoretical Cosmology
› LHAASO Constraints on New-Source Cosmic Rays:Abundance Scenarios and Injection Spectral Indices
› The DARWIN Project: Cosmological Simulations of Galaxy Formation down to Dwarf Scales in Diverse Environments
› The ALMA REBELS Survey: The [C II] Luminosity Function of UV-Selected Galaxies at $z\sim7$
› Detection and Statistics of large-scale Sector Boundary Crossings in the Solar Wind: The SBCross Catalog
› A neural-network model to find correlations in astrochemical space
› Dark Matter, Baryon Number, and Cosmic-Ray Antinuclei
› Extra-dimensional Origins of Chemical Potentials at the Cosmological Collider
› The iSTORM Instrument for Airborne Measurements of Gamma-Ray Emissions from Thunderstorms
› Direct detection of right-handed fermionic dark matter: electron-recoil measurements in Xe atoms
› Adding slow magnetoacoustic mode to the HLL-type multi-state approximate Riemann solution
› Effects of Alfv\'enicity on the Compressible Energy Cascade in Magnetohydrodynamic Solar Wind Turbulence: Evidence from Parker Solar Probe, Solar Orbiter, and WIND observations

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