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Astronomia w Krakowie
Photo: In the dome
In the dome
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Allsky

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Temperature
15.0 °C

Humidity
 66%

Wind
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Pressure
1028.9 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:

› Asteroseismic Detection of a Massive Unseen Companion to the $\delta$ Scuti Star TIC 160582982
› Extreme Kerr Newman Black Holes: Differential Geometry, Symmetry, and the Golden Ratio
› Water enhances the formation of refractory sulfur in interstellar ices
› Gaia neutron stars: demographics, birth rates, and connections to other neutron star populations
› Three New Likely Spider Millisecond Pulsar Binaries and Optical Kinematic Tracers of Intrabinary Shocks
› Which Milky Way Streams Make the Best Dark Matter Detectors?
› XClass: An Automated Multiwavelength Machine-Learning Pipeline for Classification of Extragalactic X-ray Sources. I. Pipeline Description
› How eccentric is the debris disk of epsilon Eridani? ALMA reveals a near-circular belt
› LIGHTS. Limitations of Far-Infrared Tracers for Galactic Cirrus Mitigation in the Era of Ultra-Deep Imaging
› Inferring radio beams from sparse sampling patterns: a case study with the Murchison Widefield Array
› Eppur binaria non \`e esclusa: Pulsations in CZ Tuc appear to be tidally excited by its veiled companion
› NASA ASTRA White Paper : A Chandra Successor in the 2030s
› The impact of relativistic AGN jets on realistic galaxy cluster environments
› The star formation history of Orion is structured and episodic
› Constraining Primordial Magnetic Fields with Weak Lensing
› A Multi-Wavelength Picture of the Surprisingly Short 2024/25 Outburst from EXO 0748-676
› Automated multi-stressor optical fiber focal ratio degradation and throughput characterization system for future massive multiplex spectroscopic survey
› X-ray Through Radio Observations and Modeling of the Soft X-ray Flash GRB 250419A
› Prototyping the Next-Generation Spectrograph for Space Exploration: Digital Micromirror Device-based Multi-Object Spectrograph (DMD-MOS) Calibration and Performance Assessment
› Star Formation Mitosis: The Effects of Particle Splitting on the Star Formation Outcome
› Measuring the linear gain performance for the OrcaQuest CMOS imaging sensor
› The Impact of Simulation Resolution on Dwarf Galaxy Stellar Stream Populations in FIRE
› Theoretical RR Lyrae Instability Strip from MESA-RSP Pulsation models and updated BaSTI Evolutionary Tracks
› The X-ray and optical emission of the intermediate polar Swift J0614.0+1709
› AT2018hyz: Predictions for a Sky Projection from a Delayed Off-Axis Jet
› Unresolved triples in the open cluster NGC 2437 (M 46) confirmed by the KMOS VVVX-GalCen Spectroscopic Survey
› ROBIN-PIP: Robust Bayesian Field-Level Inference with Physics-Informed Priors
› Emulation of the Halo Mass Function with Neural Networks
› Early Emergence of SSS emission in RS Oph
› Near-Noiseless Single-Photon Detection in the Infrared with a Megapixel Semiconductor Array for Low-Background Astronomy
› Correlations between the Carbon-to-Oxygen Ratio and the Orbital and Physical Properties of Exoplanets
› Optimal Pulsar Timing Array Strategies with the Deep Synoptic Array
› Towards Retrieval Augmented Generation in High-Energy and Astroparticle Physics
› LeoNet: A Machine Learning Method for Binary Pulsar Classification
› High-energy neutrinos from shocked circumnuclear material around optically-bright and infrared-only tidal disruption events
› Effects of Poisson Isocurvature Perturbations on Induced Gravitational Waves
› Weak-Lensing Shear Response for Photometric Redshift-Based Tomographic Binning
› 1RXS J174320.1-042953: another polar with a red-shifted absorption component in emission line wings
› Comparing Optimized Systematic Error Correction Methods on Selected TESS Light Curves
› Planetary eccentricity enhances inward comet transport but suppresses gentle impacts
› Eight Gamma-Ray Bursts Observed with the Fermi Gamma-ray Burst Monitor: Significant Quasi-Thermal Components and Conditional Jet Constraints
› Superorbital Phase Evolution and Identification of New Anomalous Low State Candidates for Her X-1
› Do Submillimeter Galaxies Trace Megaparsec Large-scale Structures? -- An Overdensity Analysis of 449 Submillimeter Galaxies in COSMOS
› Chemical complexity in feedback from supernova remnants: first detection of PO+ in IC443 and W44
› 25 Years of Mrk 421 with XMM-Newton: Unveiling Structured Jets and Energy-Dependent Escape
› Probing Accretion and Outflow in V1180 Cas through High-Resolution Optical Spectroscopy
› Structure of Convective-Reactive Zone in a Supernova Progenitor
› Towards solar many-line inversions
› Solarprop 2.0: Modern charge-sign dependent solar modulation for everyone
› Resolving the physics of Quasar Ly$\alpha$ Nebulae (RePhyNe): II. The dense and clumpy CGM of Quasars at $z \sim$ 3.5
› Detection of kilosecond hard lags in the new pulsating ULX candidate NGC 7456 ULX-1
› Constraining the density distribution of the cold Circumgalactic Medium of quasars at z>2 through Lya, HeII and Ha emission
› Disk-Like Matter Outflow from a Kerr-Type Wormhole: Possible Observational Manifestations and Magnetic Effects
› Constraining Particle Stiffness in Asteroid Regolith from Early-Time High-Speed Penetrator Dynamics under Local Granular Variability
› Weighing Galaxies Inside-Out: Small-Scale Lensing and the Stellar Mass Problem
› Delayed, Line-dependent Reorganization of Pore Oscillations Following a Compact C8.2 Flare Observed by Sunrise III/SUSI
› Ensemble pulsational characteristics of eclipsing binaries containing $\beta$ Cep stars observed by the TESS mission
› Galaxy Protoclusters as Drivers of Cosmic Reionization: II. Te-Based Metallicities of Lyman-{\alpha} Emitters
› Diverse Protoclusters at $z\sim3$ Disclosed by Systematic Spectroscopy
› Cosmological inference from a joint DESI DR1 full-shape power spectrum and bispectrum analysis
› Slingshot on compact binaries in the nuclear region of galaxies as the origin of large offset gamma-ray bursts
› hyprfine: simulating the 21-cm signal from the Dark Ages through to the Epoch of Reionization on a GPU
› Recycling serendipitous observations of XRISM for dark matter searches
› Radio Interferometric Calibration with the Exponential Map
› Stationarity and angular momentum conservation in pulsar spin noise
› LACHESIS: Robust stellar parameters through Bayesian model averaging of isochrone grids
› Wolf-Rayet formation through L/M-dependent superwinds
› Intrinsic versus observation induced spin nonstationarity in pulsar timing
› The Impact of a Clumpy Ambient Medium on the Dynamics and Synchrotron Emission of AGN Jets
› Interpreting effective homogeneous rheologies through a local differential map with application to the Moon
› Spurious sources in high-resolution VLA surveys
› Bayesian Image Reconstruction with Spatially Variant PSFs in X-ray Astronomy
› A comprehensive simulation framework for multi-modal kilonova observations from all-sky surveys
› Non-Gaussian Parameter Bias: Formalism and Validation
› Strongly mixed cosmological collider at unequal sound speeds
› A New Framework for Modeling Solar Flares from MHD to Kinetic Processes
› Normalizing Flow Emulator for Gravitational Wave Detection Probability in the LIGO/Virgo/KAGRA O4 Observing Run
› From the Old to the New Starobinsky Inflation
› Primordial Black Hole and Gravitational Wave by Peaked Cosmic Perturbations from Axion Curvaton
› QCD axion misalignment during reheating
› Best practices in software citation
› Coexistence of strange quark stars and neutron stars: metastability and nucleation in proto-neutron stars
› State of the Art in Direct Dark Matter Detectors: Technologies, Performance, and Future Directions
› Graceful Exit to Radiation Domination in the Starobinsky Model: A Dynamical Realization
› Trace-anomaly decomposition and universal dark matter scaling in compact stars
› Markov Chain Monte Carlo for Bayesian Parametric Galaxy Modeling in LSST
› Analytical weak-lensing shear response of galaxy model fitting
› Clustering of Primordial Black Holes in Excursion Set Theory
› Evidence for inefficient dust production in a massive, metal-rich galaxy at $z=7.13$ uncovered by JWST and ALMA
› JWST View of the Supernebula in NGC 5253. II. Nebular Lines
› Eight New Ultramassive Black Hole Masses confirm Best Correlation with Galaxy Core Sizes
› Recovering Subtle Cosmological Information with the Zel'dovich-inspired Transform
› Unveiling Multimessenger Emission from Hidden Cores of Microquasars
› Starbursts hiding in the main sequence: a pathway toward quenching?
› Two-stage disruption of resonant chains
› A Census of Na D-traced neutral ISM and outflows at $0.6
› Search for Anisotropic Pair Halos Associated with Blazar Jets
› Testing $\Lambda$CDM with ANN-Reconstructed Expansion History from Cosmic Chronometers
› Reionization, UV Luminosity and 21$\,$cm Sensitivity to Primordial Magnetic Fields: Impact of Energy Losses
› Secondary Dependence of Baryonic Effects on the Density Profile of Dark Matter Halos
› Lyman-alpha Radiation Pressure in Dense Star Clusters: Implications for Star Formation and Winds at Cosmic Dawn
› Gravitational wave detectability range informed by external messengers
› Ring Position Angles and Spin in M87* and Sgr A*
› Cosmology with Intensity Mapping via Statistics Beyond the Power Spectrum in the SKAO Era
› Fractional-Dimension Gravity and the Milky Way Galaxy
› Disentangling modified gravity and galaxy bias with field-level inference
› Revisiting 2D and 3D Dainotti Correlations for GRBs Using Bayesian Neural Networks
› Black hole astrometric binaries in the Roman Galactic Bulge Time Domain Survey
› Relativistic outflows power a quasi-periodic eruption: constraints on energetics, mass loss, and emission mechanisms
› The Role of Big Bang Nucleosynthesis in Joint Cosmological Analyses
› Probing submillimeter number counts below the confusion limit: extreme-value statistics of the P(D) distribution and its modulation by gravitational lensing
› Limits on Primordial Black Hole Evaporation from LUX-ZEPLIN
› Selective state space model for photon energy estimation in microwave kinetic inductance detectors
› Testing Offsets Between Cluster-Scale Halos and BCGs in Strong Lensing Models Using the Jackknife Method
› Early Planet Formation in Embedded Disks (eDisk). XXV. Inclination-Induced Minor-Axis Brightness Asymmetries Reveal Limited Dust Settling in Embedded Protostellar Disks
› ArxSP: A Python-Based Modular Application for the Reduction of Digitized Archival Spectra
› U-spin symmetry energy and hyperon puzzle in $\Lambda$-admixed neutron stars
› Testing the wormhole echo hypothesis for GW231123
› Hadronic description of nuclear matter and neutron star properties
› Twin-peaked gravitational wave signals from a $\mathcal{Z}_2$ phase transition
› Diffuse Supernova Neutrinos with Secret Neutrino Interactions
› Cosmology with a Non-minimally Coupled Dark Matter Fluid II. Cosmological Perturbations
› Analytic backreaction of a scalar wig on a Schwarzschild black hole
› Seeding baryonic dark matter

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