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Astronomia w Krakowie
Photo: view from north-east
view from north-east
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Temperature
13.9 °C

Humidity
 70%

Wind
1.6 km/h

Pressure
1023.8 hPa

Moon

Moon

 News from astronomynow.com

› 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
› Dark matter may come in multiple forms, new model suggests
RSS  Latest preprints on astro-ph:

› FPCA-Enhanced Simulation-Based Inference for Robust Type Ia Supernova Cosmology
› Tails and Trails: Comets and NEOs Survive Co-addition in Rubin Early Data Preview 2
› A Self-Consistent Jeans Analysis of the Milky Way Rotation Curve
› Non-linear dynamo waves in magnetized shear flows: a candidate mechanism for the solar cycle
› Hidden in the Halo: New Diffuse Star Clusters in the M82 Starburst with JWST
› TRICEPS. I. Tracing cold gas, dust, and stars at sub-kpc scales in massive star-forming galaxies at z = 4-5
› Saturation Mechanism of Cosmic Ray Streaming Instabilities with a Shell Distribution
› Mass and spin properties of black-hole mergers reveal formation in triples
› Selective state space model for photon energy estimation in microwave kinetic inductance detectors
› Revealing Optically Hidden Companions to Intermediate-Mass Stripped Stars with Radial Velocities
› Analyzing $\mu$ Parameter Range and the Duration of Reheating in the Polynomial $\alpha$-attractor Models using CMB Observations
› Interaction of stellar dipole and disk magnetic fields in accretion-ejection systems
› Machine Learning $\beta$-decay Half-lives and Their Application to $r$-Process Observables
› SN Helios: A Multiply Imaged Type II Supernova Opening Time-Delay Cosmography beyond redshift of 3
› A tidal disruption event in a quasar at redshift 7.19
› Infrared Cavity Surrounding T Pyxidis: Evidence of a Nova Super-remnant?
› Spectral and Polarization Properties of Coherent Radio Emission from Relativistic Magnetized Pair Plasma Shocks
› Collisional excitation of E- and Z-ethanimine to model cold molecular clouds
› The 91T/99aa-like Type Ia Supernova 2019vrq, Part II: 3D, Non-LTE, Low-Amplitude, Pulsating Delayed-Detonation Models of a Promising Standard Candle
› FOTO: Figure-Level Semantic Search for Astronomy
› Breaking the AGB Color Degeneracy with Variability and H$_2$O: A Consistent Picture of AGB Chemistry, Dust, and the J-Region Across Environments
› Hot Rocks Survey VI: An anomalously hot dayside for the rocky planet GJ 357 b
› The JWST Proto-PAH project. Computational modeling of the emission carriers
› The JWST Proto-PAH project: Aromatic backbones with extensive aliphatic substitution account for both the aromatic and aliphatic emission
› Evidence for the Typhon Stellar Stream as the Remnant of a Recently-disrupted Dwarf Galaxy
› Tracing the Host-Galaxy Environments of FRBs with a New Sample of Localized Sources Detected with the DSA-110
› Deciphering the VHE gamma-rays spectra of Extreme High-Frequency peaked BL Lac Objects through a Photohadronic Model
› A VLA Study of the Disturbed Massive Cluster PLCK G165.7 + 67.0 and Its Two Narrow Angle Tail Galaxies
› A Cyanopolyyne-rich but COM-poor Massive Protostar: The First Hot Carbon Chain Chemistry Source G28.28-0.36
› A Comprehensive Study of the Long-Period Cataclysmic Variable V630 Cassiopeiae
› A Sample of Long-Period Binaries with Dormant Compact-Object Candidates from LAMOST DR13 MRS and Gaia DR3
› Pulsed Accretion onto Eccentric Binaries in Highly Misaligned Circumbinary Disks
› BS Cassiopeiae: A Contact Binary with Starspot-Driven Variability and Evidence for Additional Components
› Long-term X-ray variability of the NLS1 Ark 564
› On the Compositions of Interstellar Objects
› KBSS-InCLOSE II: First Detailed Insights on the Inner CGM of Low-Mass $z\sim2.3$ Galaxies
› Near-infrared spectra of chemically peculiar stars and applications to kilonova spectra
› Beating and coupling in pulsating stars: a unified Fourier description and observational diagnostics
› TS23/McDonald and FIES/NOT strike again. Two new warm Jupiter systems and outer companions in a third
› Convolutional non-parametric Gamma-Ray Signal and Background Separation
› AKARI near-infrared spectroscopy of circumstellar hydrocarbon dust associated with young stellar objects
› Simulating tidal disruption events in nuclear star clusters
› Probing the cosmic web with fast radio bursts: II. Scintillation
› The NEMESIS general YSO catalogue - I. Supervised classification with deep learning methods
› Observational constraints on scalar-vector-tensor dark energy with phantom-divide crossing
› JWST detection of methane emission from a young brown dwarf
› ATLASGAL: The HCN-IR Star Formation Relation for the Milky Way
› N-Body Dynamics as a Mechanism for Mean Motion Resonance Formation in the Post-Gas Era
› MATISSE-py: a high-level Python interface for efficient, automated VLTI/MATISSE data reduction
› H2 emission in the Orion Bar, NGC7023 and the Horsehead Nebula observed with the James Webb Space Telescope
› A solution to the paradox of youth in the Galactic centre
› SQuIGG$\vec{L}$E: Spatially resolved NIRSpec Pa$\alpha$ reveals that the most CO-luminous, $z\sim0.7$ post-starburst galaxies exhibit falling---but still active---star formation behind optically thick dust
› SQuIGG$\vec{L}$E: Ubiquitous Cool Gas Outflows with Large Mass-Loading Factors in $z\sim0.7$ Post-starburst Galaxies
› A statistical hardness classification of ultraluminous X-ray sources using long-term Swift/XRT monitoring
› The Molecular Circumstellar Environments of Red Supergiants in Galactic Open Clusters
› Kruglov-entropy cosmology from apparent-horizon thermodynamics: background dynamics and observational constraints
› 4FHL: The Fourth Catalog of Hard Fermi-LAT Sources
› Neutron Economy and Freeze-out Dynamics in the Late-Time Cold r-Process
› Physics-induced impact on the properties of Kepler/K2 solar analogs in the light of PLATO's requirements
› The 91T/99aa-like Type Ia Supernova 2019vrq, Part I: Photometry, Spectroscopy, and Spectropolarimetry of a Nearly Standard Candle
› Cosmic Heterogeneity Shapes the Evolution of Dark Energy and Time
› A Comprehensive Study of the Magnetic White Dwarfs in DESI DR1
› Inclination of Miranda as a Constraint on the Tidal Dissipation of Uranus
› A Multidimensional General-Relativistic Boltzmann Solver for Neutrino Transport: Implementation, Discretization and Optimization
› MAGGIE: A Magnetic Gravitational Wave Induction Experiment
› Metastable Neutron Stars as Transient-Rate Detectors of Heavy Dark Matter
› Hybrid Partial Dressing: Correct Effective Potentials at All Temperatures
› Tracing out massive fields in cosmology
› Rotating Weyssenhoff fluids in linearized Einstein-Cartan theory
› Propagation delays and regional intensity changes in lensed hotspot images
› A Bonded-Particle Discrete-Element Model with Self-Gravity for the Collision and Reaccumulation of Rubble-Pile Asteroids: Formulation and Numerical Protocol
› Sub-Horizon and Quasi-Static Approximations in Interacting Dark Sector Models Involving Scalar Field Dark Energy
› Bayesian inference of non-Maxwellian distribution functions from collective Thomson scattering spectra
› Set Transformer inference of the neutron star equation of state from stellar observations
› Architecture Acceleration of Machine Learning Gravitational Waveform Surrogate Models
› From Image Morphology to Multiphysics Earth Posteriors
› Natural Saturation Of The Sterile Neutrino Dark Matter Resonant Production By a High Lepton Flavor Asymmetry In Primordial Plasma
› Mind the second gap: The impact of gaps on noise and signal parameter inference
› Dark Bondi Accretion Aided by Baryons and the Origin of JWST Little Red Dots
› MEGATRON: the impact of non-equilibrium effects and local radiation fields on the circumgalactic medium at cosmic noon
› MAGNUS I: A MUSE-DEEP Sample of Early-type Galaxies at Intermediate Redshift
› MAGNUS II: Rotational support of massive early-type galaxies decreased over the past 7 billion years
› VELOCE III. Reconstructing Radial Velocity Curves of Classical Cepheids
› DESI-Like Hubble Expansion From Staged Symmetry Breaking: Constraints on Renormalizable Models
› The Clustering of Little Red Dots from Ultra-Strongly Self-Interacting Dark Matter
› Interpreting the diversity of afterglow emission from radio-detected tidal disruption events with instantaneous and delayed outflows
› Partial Relief of the Hubble Tension and a Natural Self-Interacting Dark Matter Candidate From Staged Symmetry Breaking
› Exploring Beyond {\Lambda}CDM with the Weak Lensing Power Spectrum and Bispectrum
› Does supernova feedback regulate the star formation rate in dwarf galaxies?
› Euclid preparation. XCV. Cosmology Likelihood for Observables in Euclid (CLOE). 2. Code implementation
› Introducing SAGUARO -- Simulating IGM Evolution and Environments At High Resolution: Setup and First Results
› Investigating the $H_0$ Tension and Expansion-History Mismatch with Diverse Dark Energy Parametrization Frameworks
› TDCOSMO XXVI: Uniform lens modeling of eight doubly imaged quasars
› Identifying the host of compact binary mergers
› Vision-Language Model Ensembles Achieve Human-Expert Accuracy for Galaxy Merger Classification
› Isochrones in primordial magnetic field evolution
› SIDM and CDM interpretations of the million-solar-mass lensing perturber JVAS B1938+666-$\mathcal{V}$
› MOSAIC at ELT: Design and First Prototyping of Novel Robotic Optical-Relay Positioners
› Signatures of photospheric convection throughout the solar atmosphere: the EVE Sun-as-a-star mHz continuum
› Primordial Black Hole mass growth from neutrinos during the radiation era
› Turbulent Transport of Galactic Magnetic Fields into Cosmic Voids: Insights from IllustrisTNG
› Falsifiable anthropic model from the string landscape
› Structural quasi-universality in highly magnetized differentially rotating neutron stars
› J0011+3443: a GPS compact symmetric object, gravitational lens, or dual AGN?
› On the formation of subdwarf B stars via engulfment of substellar companions I. Conditions for and occurrence of envelope ejection events
› Volatile depletion in rocky planets as a chemical fingerprint of hybrid accretion
› Early against Late: A contrast on dark energy in the light of DESI DR2
› A Spectral Framework for Testing the Quasi-Star Hypothesis in Little Red Dots I: Weighing LRDs by Their Super-Eddington Luminosity Ratios---No Signs of Overmassive Black Holes
› First results on the search for the Galactic Center Excess in the sub-GeV band with the emulsion telescope in GRAINE 2023
› High Resolution Grid-based Simulations of the Warm-Hot Intergalactic Medium
› Silencing the stellar glare with kernel-nulling and active phase control on photonic chips
› Pushing high angular resolution and high contrast observations on the VLTI from Y to L band with the Asgard instrumental suite: integration status and plans
› Formation of adducts of C$_6$H with Na$^+$, Mg$^+$ and Al$^+$ metal cations by radiative association
› Gravitational and kinematic redshifts of black holes in nonlinear electrodynamics
› Black hole binaries in shift-symmetric Einstein-scalar-Gauss-Bonnet gravity experience a slower merger phase
› Addressing leakage and mode suppression in angular power spectrum estimation for gravitational-wave backgrounds using pulsar timing arrays
› ThousandWorlds: A benchmark for climate emulation of potentially habitable exoplanets
› Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures
› Isochrone fitting of Galactic globular clusters - IX. Tip of the red-giant branch for 27 clusters and constraints on new particle physics
› Promoting Green Computing in High Energy Physics and Astrophysics
› Higgsino Dark Matter Interpretation of the LUX-ZEPLIN 248 keV Nuclear-Recoil Event
› Sub-TeV Singlino Dark Matter in light from Sagittarius A$^\ast$ and LUX-ZEPLIN Nuclear-Recoil Event

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