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Podchorazych 2, 30-084 Krakow, Poland. tel.: (+48 12) 662 6301; fax: (+48 12) 637 2243; Obs. tel.: (+48) 502 113714
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Astronomia w Krakowie
Photo: Dome at sunrise
Dome at sunrise
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Temperature
19.9 °C

Humidity
 51%

Wind
4.8 km/h

Pressure
1020.3 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:

› Magnus mountains on spinning neutron stars
› Synchrotron and Inverse-Compton Signatures of Black to White Hole Explosions: Weibel-Mediated External Shocks in the Interstellar Medium
› Microscopic Interaction versus Purely Gravitational Coupling in Strange Quark Stars Admixed with Dark Matter: A One-Fluid and Two-Fluid Comparison
› Climates of Gl 514 b
› The \^G Infrared Search for Extraterrestrial Civilizations with Large Energy Supplies. V. When Galaxies Glow with Industry
› Recycled Gas Dominates the Metal-rich Fuel of Supermassive Black Holes
› Interacting Supernovae: a Radio and X-ray Strategy to Constrain the Structure of the Circumstellar Medium
› Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics
› Don't Cut Corners: How Training Outside the Prior Makes Simulation-Based Inference More Robust
› FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables
› Trace the Self-Gravitating Gas Using CO Isotopologues
› Astronomical Cardiology II: A Search For Heartbeat Stars Using APOGEE and TESS
› CLASSY. XV. Kinematics and Spatial Distributions of Outflows in Local Highly Star-Forming Galaxies
› Ripples in the OCEANS: Broad Line Variability of Little Red Dots
› 3D Radiative Transfer of Lyman-series Lines with SKIRT
› Large-Scale Dynamos Driven by Shear-Flow-Induced Jets
› Observing Co-Located Neutral and Ionized Gas-Phase Iron Depletion in the Magellanic Clouds
› Laser-micromachined silicon-platelet feedhorns for large-scale submillimeter and millimeter-wave focal planes
› The Wave-Regulated Precursor of a Near-Parallel Interplanetary Shock Observed by Parker Solar Probe
› Gaia parallax bias via spherical harmonics: A Python tool and discussion of possible causes
› How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition
› Titanium Oxide Absorption as a Proxy to Detect Long term Variation and Activity Cycle in Proxima Centauri
› An Evolving Leptonic Jet Model for Delayed Radio Flares in Neutrino Blazars
› SPURS: Massive Stars, Dense Gas, and Ly$\alpha$ Escape in GN-z11 at $z = 10.6$
› ALMA observations of pre-JWST z ~ 10 galaxy candidates: A CO(J = 9-8) line from a ULIRG at z = 2.54 and revisit of the photometric redshifts with JWST photometry
› Are Near Resonant Multiple-planet Systems from Kepler Young?
› Are Hot Jupiters Tidally Disrupted During Stellar Main Sequence?
› Photospheric Kelvin--Helmholtz Vortices as Possible Drivers of Coronal Heating: Implications of the DKIST Observations
› Waterfall-modulated $\alpha$-attractors
› Tropospheric Ducting Prediction based on GFS Model Data at Inyarrimanha Ilgari Bundara, the CSIRO Murchison Radio-astronomy Observatory
› X-ray signals converted from high-frequency gravitational waves emitted by spinning light primordial black hole dark matter
› Elemental Composition Evolution during the 2024 September 30 Solar Eruption: A Comparison of Hot and Cool Plasma Components with Solar Orbiter/SPICE, Hinode/EIS, and Chandrayaan-2/XSM
› Chondrule formation in the outer disk from the primary three-dimensional chemical composition of CM chondrules
› Gal3D: Superellipsoid Modeling of Radial 3D Galaxy Structure in IllustrisTNG and EAGLE Simulations
› Cross-spectral Analysis of the Type-C Quasi-periodic Oscillation Shoulder Component in GX 339-4
› SNIFFLES I: Intended Emission, Unwanted Emission, and Unintended Radiation from Low-Earth Orbiting Satellites Impacting Radio Astronomy from 1-26 GHz
› AT 2024qfm: a luminous fast blue optical transient at a redshift of z = 0.2267 identified by Lasair-ZTF
› TIC 433545934: The first 2+2 type doubly eclipsing binary with extra, mutual eclipses
› Revisiting gravitational instability in protostellar discs with improved radiative cooling models
› Complex Energy-Dependent Behaviour of Quasi-Periodic Oscillation Observed in GRS 1915+105
› Cosmic Structures in CDM and SIDM
› Forecast for the detectability of patchy hydrogen reionization in WEAVE-QSO measurements of the Lyman-$\alpha$ forest power spectrum at redshift $z \geq 4$
› The atmospheric vertical structure of Uranus and Neptune from thermochemical models: the impact of model assumptions
› A Radon-Transform Perspective on Exoplanet Transits
› Cosmography with DESI-DR1 Cosmic Chronometers: Direct H(z) measurements from Luminous Red Galaxy ages
› FOSSIL's preliminary thermal architecture
› Optical development of the BISOU breadboard
› Assessing Planetary Stability and Long-Term Habitability in Nearby Stellar Binaries: 70 Oph, 36 Oph, $\gamma$ Leo
› Optical concept model of the future cosmology project BISOU
› The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs
› Stellar tidal systematics in apsidal-motion searches for circumbinary planets: CH Ind and SW CMa
› X-ray Flaring and Variability in NGC 1275, the Heart of the Perseus Cluster
› Radio Properties of Narrow-Line and Broad-Line Seyfert 1 Galaxies
› Differential Reddening and Extinction Law Analyses of Galactic Open Clusters
› JWST Detects a Dusty AGB-like Source Before the Type Ia-CSM Supernova 2026sqf
› Radio Monitoring of Classical Novae using the ASKAP Variable and Slow Transients Survey
› Automatic detection of fast oscillations of dark matter scalar field and updated cosmological constraints on QCDM
› The Most Probable Outer Density Profile from Excursion Set Theory
› Widefield Arecibo Virgo Extragalactic Survey: II. Characterizing the HI properties and environment of the WAVES South region
› The Production of Electron-Capture Elements in Thermonuclear Supernovae: Theory vs. Observations
› JWST MIRI Medium Resolution Spectrometer Point Fixed Pattern Corrections: Cleaner and Higher Signal-to-Noise Spectra of Point Sources
› Strict Limits on Helium Absorption from LHS 1140 b from Four JWST NIRISS Transits
› No Helium Detected in LHS 1140 b from Four JWST NIRISS/SOSS Transits
› Higher-Order Analytical Expansion of Thawing Dark Energy with an Exponential Potential
› Numerical Model Simulation of the Carruthers GCI Images
› The sensitivity of TESS to transiting planets in TOIs with close-in stellar companions
› Production of Primordial Black Holes in the Double D3-Brane - anti-D3-Brane Inflation Model
› Gas Flows and Mass Accretion Rates in Eight Dippers: HD 142666, HD 143006, HD 145718, V935 Sco, DoAr 25, EPIC 204638512, EPIC 205151387, and EPIC 203850058
› Learned proposals in trans-dimensional inference are optimal at equilibrium, not during assembly
› Effects of Quantum Spin-Connection Foam in the Solar System, Galaxies, and the Universe
› Thermal false vacuum decay near black holes is aspherical
› Singlet-Doublet fermion origin of dark matter, neutrino mass and inverse first-order electroweak phase transition
› Spontaneous Scoto-leptogenesis
› Massive cold hybrid stars in a modified Polyakov-Nambu-Jona-Lasinio model
› Scalar induced gravitational waves as probes of dark QCD
› Temperature effects on white dwarfs in modified gravity
› Long-term 3+1 simulations of primordial black hole formation during radiation domination
› Vector Perturbations in Ghost-Free Quasidilaton Massive Gravity
› Development of an Embedded Receiver for Space Exploration Missions
› Deep Investigation of Neutral Gas Origins (DINGO): Options for the Processing and Storage of Radio Astronomy Data for robust Deep Spectral Line Imaging in the SKA-Era using uv-Grids
› The origin of the galaxy size-stellar metallicity relation: A semi-analytical perspective
› StarEmbed: Benchmarking Time Series Foundation Models on Astronomical Observations of Variable Stars
› Dark Matter profiles of "in silico" galaxies: deep learning inference
› Gravitational potential drives the concentration dependence of the stellar mass-halo mass relation
› Discovery of Isolated, Quenched Candidate Backsplash Dwarf Galaxies near M101
› Cosmic Chance Superpositions: Largest Catalog of Quasar-Galaxy Pairs at a Projected Separation of $D \lesssim 20$ kpc
› Probing Dark Matter Halos of High-redshift Quasars via Wide-Field Clustering
› McFACTS. IV. Electromagnetic Counterparts to AGN-disk-embedded Binary Black Hole Mergers
› Filling The Pockets: The Spherical Nature of 3D Deflagration in Thermonuclear Supernovae
› Sound Speed Resonance in the Gravitational Wave Background as a probe for non-standard early universe cosmologies
› Nonminimally coupled quintessence with sign-switching interaction
› Measurement of the minimum cold dark matter halo mass with strong gravitational lensing
› Theoretical Constraints on Neutron Star Superfluidity from Her X-1 Precession
› A Unified [CII] Morpho-Kinematic Corpus for 31 Star-Forming Galaxies at z = 4.26-5.68: The High-z Kinematic Corpus Z1
› The EPS Research Astro-RAG Platform: A Unified Open-Science Infrastructure for Cross-Epoch Astrophysical Kinematic Analysis, LLM-Assisted Research Workflows, and Educational Outreach
› The Delta Resonance in the Neutrino Sky
› Probing Baryonic Feedback Effect with CSST Weak Lensing and Future FRB Measurements
› Pulsed Infrared Emission from Magnetar 4U 0142+61 Detected by JWST
› A Model Context Protocol Server for Astrophysical RAG: Unified Access to HI, Dwarf, Globular Cluster, IntZ, and ALPINE Kinematic Corpora with FAISS Semantic Search
› The emergence of X-ray emission lines during relativistic radio-jet formation in the changing-look active galactic nucleus 1ES 1927+654
› MOA-2020-BLG-108Lb: A Giant Planet Beyond the Snow Line of a Low-Mass Lens Near the Lower Boundary of the Mass-Ratio Desert
› Planet-moon ejections in close stellar encounters
› Quantifying the Information Gain from Future High-Precision Radius Measurements for Identifying Twin Neutron Stars
› Environmental Noise Challenges for the Einstein Telescope - A Review
› Lunar Reflective Interferometry
› Gauge-Invariant Bubble Nucleation and Gravitational Waves from First-Order Electroweak Phase Transitions
› Towards Accurate Gravitational Wave Predictions: Gauge-Invariant Nucleation in the Electroweak Phase Transition
› Sub-Leading Logarithms for Scalar Potential Models on de Sitter
› Forbidden dark matter assisted by first-order phase transition and associated gravitational waves
› Not So Minimal Warm Inflation
› Can Primordial Black Holes Be Seeds for Early Galaxies in Models Satisfying the Covariant Entropy Bound?

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