Obserwatorium Astronomiczne na Suhorze Strona główna
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ul. Podchorążych 2, 30-084 Kraków. tel.: (+48 12) 662 6301; fax: (+48 12) 637 2243; Obs. tel.: (+48) 502 113714
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Obserwatorium Astronomiczne na Suhorze

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Astronomia w Krakowie
Zdjecie: Halo, księżyce poboczne i krąg parheliczny wokół Księżyca
Halo, księżyce poboczne i krąg parheliczny wokół Księżyca
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 Wiadomości z astronet.pl

› Warsztaty AstroNETu 2025
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RSS  Najnowsze prace na astro-ph:

› The power of polarimetry for characterising exoplanet atmospheres, clouds, and surfaces with NASA's Habitable Worlds Observatory
› Teareduce: a Python package with utilities for teaching reduction techniques in Astronomy
› Projection effects in star-forming regions: I. Nearest-neighbour statistics and observational biases
› Little Red Dot $-$ Host Galaxy $=$ Black Hole Star: A Gas-Enshrouded Heart at the Center of Every Little Red Dot
› It's More Complicated Than You Think: A Forward Model to Infer the Recent Star Formation History, Bursty or Not, of Galaxy Populations
› How supermassive black holes shape central entropies in galaxy clusters
› Constraining high-energy neutrinos from tidal disruption events with IceCube high-energy starting events
› What drives bar rotation? The effect of internal properties and galaxy interactions on bar pattern speeds
› Radiation hydrodynamic simulation of the Haro 11 galaxy: the escape of LyC and Ly$\alpha$ in a dwarf galaxy merger
› Euclid: Early Release Observations -- The star-formation history of massive early-type galaxies in the Perseus cluster
› Turbulent Dynamo Action in Binary Neutron Star Mergers
› Anomalous narrow line Seyfert I galaxies from SDSS DR17
› First constraints on causal sources of primordial gravitational waves from BICEP/Keck, SPTpol, SPT-3G, Planck and WMAP $B$-mode data
› Early results in the search for extreme coronal line emitters with the Dark Energy Spectroscopic Instrument
› Proposal to Search for the CP Violating Electromagnetic Vacuum Angle at the Event Horizon Telescope
› The Third Option: Color Phase Curves to Characterize the Atmospheres of Temperate Rocky Exoplanets
› A Universal CMB $B$-Mode Spectrum from Early Causal Tensor Sources
› The Lambert $W$ equation of state in light of DESI BAO
› Tidal features as tracers of galaxy merger histories: the colours of tidal features in HSC-SSP
› Properties of Polarized Radio Sources in the Wide Chandra Deep Field South from 2 to 4GHz
› Radio-Near Infrared Imaging of Dual Active Galactic Nuclei Candidates
› The Initial Mass Function as the Equilibrium State of a Variational Process: why the IMF cannot be sampled stochastically
› 27 years of Spaceborne IR Astronomy: An ISO, Spitzer, WISE and NEOWISE Survey for Large-Amplitude Variability in Young Stellar Objects
› Balancing Variety and Sample Size: Optimal Parameter Sampling for Ariel Target Selection
› The LEGARE Project. I. Chemical evolution model of the Nuclear Stellar Disc in a Bayesian framework
› Towards precision astrometry of scattered images of compact radio sources: scintillometry theory and prospects
› A rotation-based census of blue lurker candidates in open clusters
› Thermal emission spectra of the ultra-hot Jupiter WASP-33 b
› NOCTURNE. I. The radio spectrum of narrow-line Seyfert 1 galaxies
› Disk Wind Feedback from High-mass Protostars. V. Application of Multi-Modal Machine Learning to Characterize Outflow Properties
› The First Quantitative Study of Tail Regrowth of CME-Driven Disconnection in Comet C/2023 P1 Nishimura
› Euclid preparation. Decomposing components of the extragalactic background light using multi-band intensity mapping cross-correlations
› Discovery of a compact hierarchical triple main-sequence star system while searching for binary stars with compact objects
› The Pre-He White Dwarfs in Eclipsing Binaries. V. TIC 399725538
› Strontium-84 Enrichments in Presolar Grains Provide First Evidence of p-process Nucleosynthesis in Core-collapse Supernovae
› A Comprehensive Network for the Discovery and Characterization of Interstellar Objects
› Proposal of a Novel Physical Parameter Characterizing Solar Wind Speed in a Wave-Driven Model
› Data-Driven Generation of Neutron Star Equations of State Using Variational Autoencoders
› Realizing the phantom-divide crossing with vector and scalar fields
› Evaluating Classifications of Extremely Metal-poor Candidates Selected from Gaia XP Spectra
› A redshift survey of the nearby galaxy cluster Abell 2199 : No upturn of the faint-end slope of galaxy luminosity function
› Cross-correlating galaxies and cosmic dispersion measures: Constraints on the gas-to-halo mass relation from 2MASS galaxies and 133 localized fast radio bursts
› Coupled thermal-chemical evolution models of sub-Neptunes reveal atmospheric signatures of their formation location
› TeV Gamma-Rays from the Low-Luminosity Active Galactic Nucleus NGC 4278: Implications for the Diffuse Neutrino Background
› Cosmological analysis of the DESI DR1 Lyman alpha 1D power spectrum
› MgAl burning chain in M 54: the globular cluster-like properties of a nuclear star cluster
› Wave generation via oscillatory reconnection at a three-dimensional magnetic null point
› How large spectroscopic surveys are shaping our understanding of massive stars
› Compton hump reverberation lag in the bright Seyfert 1 galaxy IC 4329A with NuSTAR
› The dynamically hazardous asteroid 2025 TV$_{10}$. A new co-orbital asteroid of Venus
› Nucleus and Postperihelion Activity of Interstellar Object 3I/ATLAS Observed by Hubble Space Telescope
› DESHIMA 2.0: A 200-400 GHz Ultra-wideband Integrated Superconducting Spectrometer
› Galaxy-Galaxy Blending in SPHEREx Survey Data
› A Low-mass Model of The Milky Way: The Disk Warp Resulting from A Galaxy Merger
› Eta-Virginids: another asteroidal meteoroid stream
› Little Red Dots and Supermassive Black Hole Seed Formation in Ultralight Dark Matter Halos
› PERTURB-c: Correlation Aware Perturbation Explainability for Regression Techniques to Understand Retrieval Black-boxes
› Investigating the emission signatures of pulsar halo candidate HESS J1813-126
› Mixing-induced thermal instabilities and coronal condensations
› Pulse-resolved Classification and Characteristics of Long-duration GRBs with \emph{Swift}-BAT Data.I. Precursors versus Main Bursts
› Detection of hot subdwarf binaries and sdB stars using machine learning methods and a large sample of Gaia XP spectra
› Detection of Gravitational Anomaly at Low Acceleration from a Highest-quality Sample of 36 Wide Binaries with Accurate 3D Velocities
› Asymptotic power spectra and visibilities of damped mixed modes
› AGN Variability with Rubin Observatory in the 2030s
› Hidden Gems in TESS: sherlock finds two new rocky planets around nearby M dwarfs
› Progress towards a 3D Monte Carlo radiative transfer code for outflow wind modelling: II. 3-D applications
› Composition and Space Weathering Characteristics of Tianwen-2 Mission's First Target Near-Earth Asteroid (469219) Kamo`oalewa
› EWOCS-V: Is Wd1-72 a recent post-interaction WR+O binary?
› Forecasting Constraints on Cosmology and Modified Gravitational-wave Propagation by Strongly Lensed Gravitational Waves Associating with Galaxy Surveys
› Late-time X-ray afterglows of GRBs: Implications for particle acceleration at relativistic shocks
› A UV-Luminous Galaxy at z=11 with Surprisingly Weak Star Formation Activity
› Extreme-Value Distribution Analysis of the Second CHIME/FRB Catalog: Assessing the Rarity of the One-off FRB 20250316A
› Orbital decomposition of the nuclear regions in the early-type galaxy FCC 47: Unveiling the nuclear cluster origin
› Critical Evaluation of Studies Alleging Evidence for Technosignatures in the POSS1-E Photographic Plates
› Spectroscopic Variability of the Broad H$\beta$ Emission Line in Sloan Digital Sky Survey Quasars
› Stellar Populations in the Extreme Outer Halo of the Spiral Galaxy M96
› Constraining Black Hole Parameters from Shadow and Inner-Shadow Morphology Considering Effects from Thick Disk Accretion Flows
› Inclination Bias in Techniques Used to Identify Be Star Candidates
› The Volatile Inventory of 3I/ATLAS as seen with JWST/MIRI
› A null test of the Hubble tension
› Mapping the Extended Lyman-Alpha Emission within the Circumgalactic Medium of Quasars Hosted by Dusty Starbursts with CubeCarve
› BE Lyncis is not a Black Hole Binary: Lessons From Gaia and Hipparcos Astrometry
› Probing the Sound Speed of Dark Energy with a Lunar Laser Interferometer
› Densities of small planets around the M dwarfs TOI-4336 A and TOI-4342 with ESPRESSO: Three sub-Neptunes, one super-Earth, and a Neptune-mass candidate
› Rethinking Resonance Detectability during Binary Neutron Star Inspiral: Accurate Mismatch Computations for Low-lying Dynamical Tides
› Exact analytic rotating black-hole solutions with primary hair
› Is Phantom Divide Crossing in General Relativity Completely Impossible? Shortcomings and Possible Solutions
› $\mathcal{R}^2$-corrected Tachyon Scalar Field Inflation, the ACT Data, and Phantom Transition
› High-Pressure Torsion-Induced Transformation of Adenosine Monophosphate: Insights into Prebiotic Chemistry of RNA by Astronomical Impacts
› Primordial black holes and Scalar-Induced Gravitational Waves formed by inflation potential with non-trivial characteristics
› Leveraging rapid parameter estimates for efficient gravitational-wave Bayesian inference via posterior repartitioning
› Perturbative analysis of singularity-free cosmological solutions in unimodular Kaluza-Klein theory
› The reason peculiar velocities grow faster in general relativity than in Newtonian gravity
› Compact Stars Sourced by Perfect Fluid Dark Matter Halos
› Numerical simulations of primordial black hole formation via delayed first-order phase transitions
› $f$-Mode oscillations and the gravitational response of compact stars with analytic equations of state
› Optimal cross-correlation technique to search for strongly lensed gravitational waves
› Mapping the narrow-line Seyfert 1 galaxy 1H 0323+342
› Untangling PBH overproduction in $w$-SIGWs generated by Pulsar Timing Arrays for MST-EFT of single field inflation
› A neutrino flare candidate potentially associated with X-ray emission from tidal disruption event ATLAS17jrp
› Convective stability analysis of massive neutron stars formed in binary mergers
› Press-Schechter Formalism and The PBH Mass Distributions
› On Validating Angular Power Spectral Models for the Stochastic Gravitational-Wave Background Without Distributional Assumptions
› A Cosmic Miracle: A Remarkably Luminous Galaxy at $z_{\rm{spec}}=14.44$ Confirmed with JWST
› Cosmic filaments confirm unexplained cooling of CMB photons in two independent redshift ranges
› SKYSURF IX -- The Cosmic Optical and Infrared Background from Integrated Galaxy Light Measurements
› Modeling Non-Gaussianities in Pulsar Timing Array data analysis using Gaussian Mixture Models
› RUBIES spectroscopically confirms the high number density of quiescent galaxies from $\mathbf{2
› Large $n$-point Functions in Resonant Inflation
› Nonradial oscillations of stratified neutron stars with solid crusts: Mode characterization and tidal resonances in coalescing binaries
› Uncertainties in high-$z$ galaxy properties inferred from SED fitting using JWST NIRCam photometry
› GMIMS-DRAGONS: A Faraday Depth Survey of the Northern Sky Covering 350-1030 MHz
› Evidence for the dynamical dark energy with evolving Hubble constant
› Atmospheric collapse and re-inflation through impacts for terrestrial planets around M dwarfs
› String-induced vacuum decay and its gravitational wave signatures
› Adding electromagnetic birefringence to pulsar timing and astrometry to detect gravitational waves
› Binarity at LOw Metallicity (BLOeM): Projected rotational velocities
› Simulations of facular magnetic fields on cool stars I: Main sequence stars with solar metallicity
› SPHEREx Re-Observation of Interstellar Object 3I/ATLAS in December 2025: Detection of Increased Post-Perihelion Activity, Refractory Coma Dust, and New Coma Gas Species
› Deep Search for Joint Sources of Gravitational Waves and High-Energy Neutrinos with IceCube During the Third Observing Run of LIGO and Virgo
› A persistent bow shock in a diskless magnetised accreting white dwarf
› Dark Energy Survey Year 6 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
› Spatial distribution of organics in the Horsehead nebula: signposts of chemistry driven by atomic carbon
› Mathematical Anatomy of Neutrino Decoherence in Red Turbulence: A Fractional Calculus Approach
› Climates of Terrestrial Exoplanets and Biosignatures
› Probing baryogenesis with gravitational waves
› Neutrino Oscillations as a Probe of Macrorealism
› Linear analysis of I-C-Love universal relations for neutron stars
› Vector Horndeski black holes in nonlinear electrodynamics
› Updating GUT-Scale Pole Higgs Inflation After ACT DR6
› Primordial magnetogenesis in loop quantum cosmology
› GWTC-4.0: Searches for Gravitational-Wave Lensing Signatures

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