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Astronomia w Krakowie
Photo: Międzynarodowa Stacja Kosmiczna i Księżyc z halo
Międzynarodowa Stacja Kosmiczna i Księżyc z halo
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Temperature
14.9 °C

Humidity
 94%

Wind
1.6 km/h

Pressure
1015.0 hPa

Moon

Moon

 News from astronomynow.com
› 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
› Artificial Intelligence uncovers more than 100 new worlds in NASA data
› XRISM solves gamma-Cas’s 50-year X-ray mystery
RSS  Latest preprints on astro-ph:
› Equivalence of mapping gravitational wave background anisotropy across bases at equal information content
› Inventories of Rich Carbon-Chain Chemistry in Prestellar and Starless Cores in the Perseus Molecular Cloud
› Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$
› A Galactic intermediate-mass stripped star with a Wolf-Rayet-like wind
› On the Origin of the Ly$\alpha$ Damping Wing in Galaxies at $8\le z \le 10$: Explorations using the NINJA Simulations
› Emission line formation in scattering dominated media: implications for LRDs
› Variations in the 3.3 ${\mu}$m Polycyclic Aromatic Hydrocarbon Feature Across Nearby Galaxies Driven by Metallicity and Radiation Field Spectrum
› Size Constraints for the Pre-atmospheric Parent Bodies of Ordinary Chondrites
› Summary statistic for pulsar timing arrays
› 3-form dark energy and cosmic birefringence
› Expanding stellar associations as Galactic accelerometers
› AT2025agpz in Rubin commissioning data: distinguishing a luminous interacting supernova from nuclear transients in compact galaxies
› Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud
› White Dwarf Stellar Structure from Effective Polymer Geometry in Loop Quantum Gravity
› Comparative analysis of fiber Bragg grating filter losses inscribed by continuous wave UV and femtosecond-IR lasers for astrophotonics
› Revisiting BV & BW Draconis: Detailed Study of Intriguing Multiple System
› Comparing the contrast performance of two IFU technologies for exoplanet direct imaging with ELT-PCS
› Information Geometry meets Functional ANOVA: An Exact Fisher-Information Decomposition, with an Application to Radio Luminosity Functions
› Graph reconstruction from random-walk co-visitation: Geometric, empirical, and controlled networks
› Proof of concept of the COSMOCal project at the IRAM 30m telescope
› Development of next-generation event-driven x-ray hybrid CMOS detectors
› The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars
› SMA 200-400 GHz Survey for 10 faint Class II Disks in the Taurus Molecular Cloud
› The Zero-Age Massive Stellar Population of W49A from VLA Observations
› Reconstructing Core-Collapse Supernova Gravitational-Wave Signals with Transdimensional Bayesian Inference
› The forced orbital planes of the Plutinos and other resonant KBOs
› The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars
› A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis
› Beyond Point Masses. VI. Spin-Orbit Evolution of the Centaur Binary Typhon-Echidna
› Hot molecular cores in the W49A molecular cloud complex
› photo-3x2-pt: Cosmology from cosmic shear and galaxy clustering with a single photometric galaxy catalog
› A Roadmap for Transient Hunters: Mapping Stellar Mass and Star Formation Rate Anisotropies in the Local Universe
› No evidence for a supermassive black hole binary in GSN 069
› MARS: A Lightweight Morphology-Aware RFI Segmentation Network for Mask-Guided Mitigation in Radio Astronomy
› Distribution of magnetic helicity and energy with height in solar atmosphere
› Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects
› New Statistical Topology Theory Predicts Turbulent Magnetic Emergence from the Sun's Interior
› Reconnection Jets Detected during the Footpoint Drift of a CME Flux Rope: New Signatures of Ongoing 3D Arcade-Flux Rope Reconnection
› An ALMA study of hub-filament systems II.Quiescent filaments converging towards highly dynamic hubs
› Dust transport in envelopes of disk-embedded planets: I. Convectively stable envelopes
› Dust transport in envelopes of disk-embedded planets: II. Fully convective envelopes
› Identification of a superbright nova in our Galaxy: revisiting the light curve analyses of the candidate novae CP Lac, CP Pup, V838 Her, V597 Pup, V5583 Sgr, and V5589 Sgr
› Kinematically Resolving the Fe K Complex in Her X-1: The Accretion Disk and Ionized Wind Across X-ray Eclipses
› GRAVITY+: reducing non-common-path aberrations for sub-10 {\mu}as astrometric accuracy
› GeV {\gamma}-ray emission in the star-forming region S140
› Photometric Distances for Metal-poor Giants and a Search for Hypervelocity Stars with LAMOST DR13 and Gaia DR3
› Ruffled Feathers: Merger-driven galaxy size growth and structural transformation in EAGLE
› Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories
› A broadband outburst of the compact steep-spectrum quasar 3C 138 in 2024-2026
› Investigating radio source population $\&$ spatial characteristics of diffuse Galactic synchrotron emission in the GAMA-23 field with uGMRT Band-3
› Cosmological Distance Measurements of High Redshift Blazars: OJ 248 (z=0.939) and 4C +38.41 (z=1.814)
› NestyNet. I. Physics Functions Are Hard to Fit with Neural Networks: A Framework for Accurate Surrogates and Analytic Derivatives
› Exploration of Exoplanet Atmospheres with the James Webb Space Telescope
› Phase-resolved QPO Analysis of GX 339-4: Improved Technique and Consistent Behaviors between QPOs and Broadband Noise
› Optical Counterparts of MeerKLASS L-band and UHF-band surveys
› Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry
› The SPACE Program II: No discernible spectral features in the transmission spectrum of the sub-Neptune HD 191939 b observed with HST/WFC3
› Chromospheric Dynamics of an Umbral Flare Kernel - Based on Coordinated SUNRISE III SCIP and Domeless Solar Telescope Observations
› Thermal Non-equilibrium Cycles in a Non-eruptive Pseudo-Streamer
› Luminosity function of quasars at $1.0
› Kilogauss magnetic fields from simulations of small-scale dynamo action in the convective envelope of a white dwarf
› The impact of nuclear equations of state on the dynamics and multi-messenger emission of magnetorotational stellar explosions
› A space of inference spaces in the space sciences - Parametric Bayesian inference in astronomy, cosmology and particle physics
› The Lunar Polar Icy Regolith and Possible Moonflows
› Search for an all-sky and a Galactic Ridge diffuse neutrino emission with the first 2 years of KM3NeT/ARCA data
› Mira variable stars in the galactic bulge and halo
› They Won't Be Giants: Missing Metal-Rich RGB Stars in Gaia Data Indicate Truncated Stellar Evolution
› Veiled in Starlight: Impacts of Stellar Contamination on Retrievals of TRAPPIST-1f's Atmospheric Composition
› HI envelope around the carbon star V420 Vul
› Reanalyzing Megamasers: a low value of $H_0$ from a local probe changes our view of the Hubble Tension
› A Streamer Driving Misalignment in the Circumtriple Disk of GW Ori
› An "inside-out" approach to modeling supermassive black hole binary inspiral
› NestyNet. II. Coherent Function-Space Posteriors from Scientific Neural Surrogates (or How to Avoid Expensive MCMC)
› The plunging region of thin accretion discs across the black hole spin range
› On the degeneracy of solutions from stellar spectropolarimetric data
› Strong Zeeman effects in the Fe I 5434.5 {\AA} line observed in a sunspot on August 17, 2024
› Decomposition of Solar Wind Velocity Distribution Functions with Orthogonal Polynomials
› A unified modeling of X-ray and gamma-ray spectro-polarimetric data: the case of Cygnus X-1
› SPT-3G D1: Foreground-Robust Lensing Templates for Primordial Gravitational Wave Searches
› Clump Migration in Disk Galaxies: Revisiting Chandrasekhar's Dynamical Friction
› The two faces of tides: gravitational instability during galaxy mergers
› The glow of eternal black holes
› Axion-driven spontaneous leptogenesis, precisely
› Novel Signatures of Matter-Induced Dark Matter Decay in Large-Volume Neutrino Telescopes
› X-ray Driven Trihydrogen Formation on Silica Nanosurfaces
› A Novel Kerr-like Black Hole in a General Double Power Law Dark Matter Environment: Geometry, Spectroscopy, and Energy Extraction
› Coherent End-to-End Search for Generic Extreme-Mass-Ratio Inspirals
› Integrable models of inflation beyond slow-roll
› Magnetic Dynamo Driven by Inertial Waves
› The Local Sky as an Introductory Solar System Astronomy Laboratory Using Smart-Telescopes
› A Neutron Star Hidden Inside a Black Hole
› The Quantum Mechanics of Rare Events: From Quantum Walks to Stochastic Inflation
› Large Gravitational Wave Phase Shifts from Strong 3-body Interactions in Dense Stellar Clusters
› Impact of Interacting Dark Energy on the Growth of Matter Density Perturbations: Observational Constraints from DESI and Multi-Probe Data
› Vacuum birefringence and the polarized X-ray emission from a radio magnetar
› Can the Efron-Petrosian Method Recover the Inverse-Square Distance Law for Simulated Radio Pulsar Fluxes?
› The Origins of the Bulk flow
› Radio-Interferometric Image Reconstruction with Denoising Diffusion Restoration Models
› Improved frequency hierarchy treatment for anisotropic spectral distortions
› Compression-Driven Kinetic Instabilities in Magnetically Arrested Disks
› A numerical framework for Newtonian-noise estimation at the Einstein Telescope: 2-D simulations beyond the plane-wave approximation
› Near-Infrared and Optical Observations of SN 2024rbc: The First Early Detection of CO and Dust in a Type Ib Supernova
› Diagnostic Consistency Tests of the Concordance Cosmology
› Ghosts of eruptions past: Searching for historical Galactic supernovae using variable thermal dust echoes and machine learning
› Constraints on Coupled Dark Energy in the DESI Era
› BEACON: JWST NIRCam Pure-parallel Imaging Survey. III. Constraints on the UV LF and the Clustering of z~7-14 Galaxies
› TDCOSMO XXVI: Uniform lens modeling of eight doubly imaged quasars
› Charge diffusion and modulation transfer function in a Nancy Grace Roman Space Telescope detector
› Non-uniform particle injection into black hole jets by radiative magnetic reconnection
› Characterizing the bolometric-photoevaporative transition in young sub-Neptunes with radiation-hydrodynamic simulations
› Primordial black hole contribution to the stochastic background of gravitational waves
› Analytical method for computing the covariance matrix of cosmic shear two-point correlation function
› Suppressed diffusion and gamma-ray emission from the Cygnus bubble
› Measuring radii of merging neutron stars with interface-mode asteroseismology informed by nuclear theory and experiment
› Global Multi-ion Solar Wind Model. I. Ion Temperatures
› Prediction for IMAP: Revealing the Role of the Solar Magnetic Field in the Heliotail
› Two inner dust clumps in PDS 70. A third protoplanet traced by trojan material or a substructured inner disk?
› The MAGPI survey: Stellar population radial trends and mass assembly in star-forming galaxies at z~0.3
› Constraints on the VHE counterpart of two binary black hole mergers observed by the MAGIC and CTAO LST-1 telescopes
› SMDET-1: a Nearby Y Dwarf Candidate
› The Dynamics of Planetary Ejection
› Pollux: high-resolution precision spectroscopy and polarimetry for the Habitable Worlds Observatory
› The Research Impact of the Jodrell Bank Observatory and Other Facilities affected by the UK Science Funding Cuts in 2025
› The Constant Evolution of the Neil Gehrels Swift Observatory: Two Decades of Operational Innovation for Time-Domain and Multi-Messenger Astrophysics
› Fundamental Limits of Quantum Sensors for Gravitational Wave Detection
› Relativistic frequency shifts in gravitational waves from axion clouds
› Three-flavor supernova neutrino simulation using a hybrid quantum-classical algorithm with qutrits
› Unified dark sector and Hubble-tension alleviation in scalar-vector-tensor gravity

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