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Astronomia w Krakowie
Photo: view from south-east
view from south-east
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Cloud

Rain conditions

Rainfall

Allsky

S Sky

Temperature
6.0 °C

Humidity
 73%

Wind
11.3 km/h

Pressure
1013.2 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:

› Interpretation of Nanohertz Gravitational Waves via Cosmic Strings in Post-BBN Matter and Kination Domination
› Kinematic and Dynamical Properties of Solar Neighborhood White Dwarfs from SDSS DR19 and Gaia DR3
› Global and Local Infall in the ASHES Sample (GLASHES). III. Physical Parameters of Contracting Motion onto Dense Cores in 70 $\mu$m Dark Massive Clumps
› Primordial black holes as a natural consequence of scale-invariance
› Exemplary Merging Clusters II: XMM-Newton and Chandra X-ray Observations of MACS J1752.0+4440 and ZwCl 1856.8+6616
› Wind-Fed Magnetic Flux and the Emergence of X-ray Coronae in Active Galactic Nuclei
› A Multi-dimensional Analysis of the Open Clusters NGC 2423 and NGC 2482 with Gaia DR3
› Neutrino flavor conversion alters the lepton-emission self-sustained asymmetry in core-collapse supernovae
› Cosmic Duets II. Growth and accretion in Gaia Multi-Peak dual AGN at Cosmic Noon
› Discovery of a Nearby Ultra-fast Magnetic White Dwarf Propeller: Common Pathways to Magnetic Cataclysmic Variables
› Accreting Neutron Stars in Low-Mass X-ray Binaries
› The Origin of the Fermi Halo-like Emission: A New Model of the Fermi Bubbles
› A "universal" supernova efficiency to drive the HI turbulence in nearby star-forming galaxies
› Atypical White Dwarfs in Open Clusters
› EK Cha b: multi-tracer detection of a protoplanet candidate in a gas-rich environment
› Prevalence of radio Active Galactic Nuclei in galaxy groups since z=3.5 in the COSMOS-Web field
› NGC 4936: abundant multi-phase medium in the central weak X-ray cool core and optically dark H I clouds in the group
› First uGMRT Constraints on Rotation Measure in the Radio-Quiet Seyfert Galaxy NGC 4235
› Descalarization bursts from Galactic supramassive neutron stars: a kHz continuous-wave target
› Population II Post-AGB Stars. I. Methodology, Initial Results, and the First Luminosity Function
› Feedback-Conditional 3D Reconstruction of Cosmic Baryons with Flow Matching
› Primordial black holes
› Pushing Variability Searches to Extreme Dwarf Galaxies with the Vera C. Rubin Observatory Data Preview 2
› Microwave Loss in Low-Temperature ICPCVD Silicon Nitride: Dependence on Precursor Ratio and RF Substrate Bias
› Debiasing Local Cluster Infall Reveals $\boldsymbol{H_0}$: Application to the Virgo Cluster
› The progenitor galaxies of the intracluster light
› Shortening the Baseline: Characterising Type Ia Supernovae Using $\Delta m_{10}(X)$
› Systematic non-compliance of satellite megaconstellations with IAU brightness limits
› Mass Proxy Quality of Halo Properties in IllustrisTNG and FLAMINGO Simulations: II. Galaxies, Stars, and Black Holes
› Understanding how Coronal Heating and Magnetic Field Scaling Affect Global Properties of the Low and Middle Corona
› Stochastic Snowball States in Planetary Climate
› The conditional colour-magnitude distribution: III. A study of galaxy colour- and luminosity-dependent counts-in-cells statistics
› Central stellar depletion in the Draco dwarf from Subaru photometry
› Flux Dependence of the 1\,keV Soft X-ray Feature in SAX J1808.4-3658 with \textit{NICER}
› DeepDISC on LSST Data Preview 1: Scene-Level Detection, Deblending, and Star/Galaxy Classification in the ECDFS and EDFS Fields
› NGC 6426: Colour-Magnitude diagram and variable star population as indicators of metallicity, distance, and age
› Galaxy Clustering Can Reveal Host-Galaxy Properties of Binary Black Hole Mergers
› The Binary Fraction of Milky Way Field Stars in DESI: Dependence on Chemical Abundance
› Improved analysis of time delays between radio wavelengths and X-ray of Sgr A* flares in the shock oscillation model
› Direct Numerical Comparison of Data Driving Strategies for Solar Flux Emergence in Magnetohydrodynamics: B-driving vs E-driving
› Pinpointing the cosmic web between massive galaxy clusters I. The incidence of HI and OVI as WHIM tracers
› Oxygen isotopic ratio in open cluster RGB stars: A new method for accurate mass and age estimations
› radio-astro-tools: linking radio astronomical data to the astronomical Python ecosystem
› Neutron star cooling with $\Delta$ dUrca processes
› Pseudo Closed-Loop Bootstrapping for Reinforcement Learning Based AO Control
› Gaseous SiO and Silicate Clouds in Three Benchmark Early-L Dwarfs
› Isotopic ratios as probes of star formation and the origin of molecular gas in the Central Molecular Zone
› Measuring radial flows in disc galaxies
› Radio Continuum Study of One of the Brightest Large Magellanic Cloud Supernova Remnants N 132D
› Gravitational Microlensing
› A Coherent Harmonic Summing Pulsar Search Code
› Probing Massive Star Formation with Intrinsic Multiplicity Constraints from TESS Eclipsing Binaries
› Metallicity does not reorder line-to-line sensitivity to granulation in solar-like stars
› What powers the most energetic flares in the Kepler field? Revisiting the superflaring star KIC 2852961
› The Hand of God Revisited: Revealing the Shell Structure and Jet-Supernova Remnant Interaction in MSH 15-52
› Investigating the nature of magnetic turbulence in Tycho's SNR using X-ray observation
› From GeV to PeV: Orbital Modulation and Wind-Regulated Ultrahigh-energy Emission in Cygnus~X-3
› Magnetic flux cancellation in a 3D magnetohydrodynamic simulation of an emerging flux tube with a non-uniform twist
› Size, Shape, and Geometric Albedo of Dwarf Planet Quaoar's Largest Satellite Weywot
› Volume Dependence of Helicity-based Eruption Diagnostics in Recurrent Coronal Jets
› On-chip filled array hyperspectral kinetic inductance detectors (FHYKID) for line intensity mapping
› Binding Energies of Astrophysically Relevant Molecules on CO$_2$ Clusters: Benchmarking and the Donor-Acceptor Origin of Surface-Dependent Binding
› A New Era for Supernova Science with the James Webb Space Telescope
› An updated model of neutrino emission from proto-neutron stars
› EWOCS-XI: Anisotropic expansion and shear in the cluster Westerlund 1. A 2D kinematic analysis with Gaia DR3
› Too many or too bright? Status and perspectives in the study of the UV Luminosity Function at z>10
› Discovery of the Slowest Radio Pulsar in the Small Magellanic Cloud
› HI intensity mapping with MeerKAT: A measurement of the 21-cm auto-spectrum on cosmological scales
› Modeling CO Line Luminosity Using FIRE Simulations: I. Methodology and Validation of Molecular Gas and CO Abundance
› Autocorrelation in black hole flare movies: Departures from Kerr
› Evidence for orbital eccentricity supports a hierarchical origin for GW231123
› An analytical model for non-local stochastic field-level galaxy bias on the sphere
› Gen-EBM: an energy balance model for terrestrial planets. Climate multistability from snowball to post-runaway greenhouse climates
› Longitudinal distribution of Io's dayside atmospheric density
› Opening the Black Box: What Neural Networks Learn from Pulsar Timing Array Data
› Data Representation Matters: Optimizing Machine Learning for X-ray Source Classification by Leveraging Spatio-Spectral Information
› JWST CAPERS: Spectroscopic evaluation of very high redshift galaxy candidates
› Rotation period of the O giant xi Persei: Coexistence of cyclic and periodic variability. A weakly magnetic candidate star
› A morphological search for stable year-scale modulation in gamma-ray blazars
› Funnel Leakage of the Wien Fireball in the Early Nebula after a Binary Neutron Star Merger
› Inflow-driven galaxy evolution - II: A hierarchy in the scaling relations of star-forming galaxies
› ACORN I. Massive Black Hole Seeding and Tidal Disruption Events from Star Clusters in Cosmological Simulations
› Cosmic topology. Part IId. Eigenmodes and correlation matrices of lens spaces
› Discovery of Hidden Extragalactic Pulsars in the Parkes Archival Data
› Disk Structure May Determine AGN Variability and Explain the Accretion Disk Size Problem: No Broad Line Region Required
› The neutrino magnetic moment and supernovae with strong magnetic fields
› A weakly modelled view of the joint compact-binary mass plane: population structure and spectral-siren cosmology
› Impact of site-dependent noise configurations on Einstein Telescope science at low frequency
› Matter-Antimatter Asymmetry from Dirac-Majorana Flip-Flop
› Observational Signatures of Dyonic Black Holes in Non-Linear Electrodynamics
› Massive de Sitter Correlators as Finite Mellin-Barnes Integrals
› Accounting for detector calibration uncertainty in black-hole ringdown analysis
› Systematic Uncertainties in Ultralight Boson Constraints from Superradiance
› Production Memory of the $^{225}\mathrm{Ra}$-$^{225}\mathrm{Ac}$ Clock in Neutron-Star Merger Ejecta
› Analysis of p-Wave Sommerfeld Resonance Behavior in Finite-Size Dark Matter
› Implications of tachyonic phase transition in classically scale invariant general $U(1)_{X}$ models
› Reference-Filter-Driven Transition Probabilities for IMM-Based Satellite Maneuver Detection
› Holographic dark energy from generalized entropies and extended infrared cut-offs
› Nonreciprocal black holes with primary hair in beyond Horndeski gravity: Exact solutions and stability
› Testing Extra-Dimensional Gravitational-Wave Polarizations with Compact-Binary Observations
› Testing General Relativity with Binary Lens Microlensing Events
› Gas-phase chemistry of $\mathrm{C}_3\mathrm{H}_3^+$: a key building block for carbon mass growth in space
› Cavity Characterization for the Princeton Axion Search
› Quantum Co-Design of Inhomogeneous Many-Body Neutrino Fast Flavor Transformation
› A Pairwise Surrogate for Gravitational-Wave Spectra from Highly Relativistic Vacuum Bubble Collisions
› Listening to the Horizon: Probing Near-Horizon Reflectivity with GW250114
› A scalar-extended ${\rm U(1)_{L_{\mu}-L_{\tau}}}$ explanation of the LUX-ZEPLIN 248 keV excess
› Revising the Spin and Kick Connection in Isolated Binary Black Holes
› DESI results and Dark Energy from QCD topological sectors
› Rapid bulge assembly in young galaxy disks at Cosmic Dawn
› New Signs Pointing Toward a Correlation Between Astrophysical Neutrinos and Radio Flares
› Stable mass transfer in massive binaries leading to merging black holes
› High-resolution Very Large Array Radio Observations of the Boomerang Pulsar Wind Nebula
› Collisionless Accretion of Finite-Angular-Momentum Plasma onto a Spinning Black Hole
› Superposition model for energy reconstruction and mass identification in cosmic ray spectra
› Velocity dispersion of Solar Energetic Particles in turbulent heliosphere
› Learning to See Sharper: A Physics-Informed Artificial Intelligence Framework for Super-Resolving Galaxy Spectra
› Point-like Off-pulse GeV Emission from the Millisecond Pulsar PSR J0437-4715
› Shape of the direct-method mass-metallicity relation with JWST: Fast-Track Nitrogen and Helium Enrichment
› From protogalaxy through thick and thin: Why did the Milky Way evolve in three kinematic phases?
› Phase-space averaging for stellar convection II. Maximum-entropy closures for mixed radiative-convective envelopes
› The age of the Universe from a large sample of the oldest Galactic stars
› Long-Baseline VLF Observations of Solar Flares from Antarctica
› Will a Supernova explode in CD-30{\deg}11223?
› Cosmological constraining power of the redshifts, heights, and angular clustering of weak gravitational lensing peaks
› Spectroscopic follow-up of compact object binary candidates from Gaia DR3: White dwarfs, neutron stars, black holes, and the parallax zeropoint
› Collisionless Shock Driven by a Supersonic Velocity Shear
› Multi-Height Spectropolarimetric Signatures of Magnetoacoustic Waves in Solar Plage
› Examining Temporal Characteristics of GCRs in the AMS-02 era
› Characterizing the hierarchical structure of filaments I. On the origin of the length-mass (L-M) scaling relation
› Why most neutron star low-mass X-ray binaries accrete transiently: an evolutionary study of transient and persistent phases
› Gravitational-Susceptibility Dip Behind DESI's results: Addressing the Phantom Crossing by Local limit of Nonlocal Gravity
› N/O-enhanced chemical enrichment by massive stars: the interplay of optically-thick winds and rotation
› Discovery of thermal radio recombination line emission toward the high-mass protostar IRAS18162$-$2048
› Relaxation of a Vlasov gas to an inhomogeneous state due to phase space mixing in an axisymmetric potential: A Newtonian analogy of the Kerr orbital motion
› High-Angular-Resolution Survey of Stars within 18 pc of the Sun: Part I
› Mitigating prior-volume effects in galaxy clustering by adopting Mpc over Mpc/h units
› PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-Domain Field V: Unraveling X-ray Spectral Variability
› Two Low-Mass-Ratio Microlensing Planets from High-Magnification Events: KMT-2021-BLG-0247 and MOA-2023-BLG-169
› Widespread steep X-ray spectra of luminous $z\simeq5.85-7.5$ quasars and their implications for future X-ray surveys
› Effect of ultralight dark matter on compact binary mergers
› Optimized numerical evolution of perturbations across sharp background trajectory turns in multifield inflation
› Probing soft signals of gravitational-wave memory with space-based interferometers
› Reviving primordial black hole formation in slow first-order phase transitions
› Exploring neutrino loss with diffuse astrophysical neutrino fluxes
› Matter Flavor Conversion Mediated by Pseudo-Sterile States as the Possible Origin of Neutrino Oscillation Anomalies
› Production of Leptophilic Bosons in Ultradegenerate Relativistic Matter
› Neutron Star Bounds on Muonic Fifth Forces from Picometer to Meter Scales
› Inflation with vector fields revisited: non-Gaussianities
› Stochastic gravitational-wave background from self-interacting superradiant clouds
› Heavy Higgsino Dark Matter With Low Reheating in View of the LZ High-Recoil Event
› Kilopixel Performance of the Kinetic Inductance Detectors for the Terahertz Intensity Mapper
› Convergence of Roberts flow dynamos in Eulerian and Lagrangian codes

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