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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 Wiadomości z astronet.pl

› Kosmiczna inicjatywa państw Trójmorza
› Spotkaj eksperta. Efekty misji IGNIS: mózg w kosmosie – komunikacja bez użycia mięśni
› Nowe dowody dotyczące atmosfer w układzie TRAPPIST-1
› Start Sojuza-5 Irtysz: czy Rosja wraca w kosmos?
› Fotografujemy zorzę polarną…
› Kosmiczny przegląd miesiąca AstroNETu – kwiecień 2026 roku
› Niebo w maju 2026 roku
› SpaceShield Hack 2026 – Stalowa Wola centrum innowacji w sektorze space & defence
› Kwantowy debiut na warszawskiej giełdzie – Creotech Quantum już na GPW
› Blue Origin po raz pierwszy ponownie wykorzystał booster – misja New Glenn NG-3
RSS  Najnowsze prace na astro-ph:

› A PINK update: Improvements to the CELEBI fast radio burst data reduction and analysis pipeline
› Complex organic molecules and cosmic ray ionisation rate towards the massive protostar Cepheus A HW2
› Origins of Extreme Emission-Line Ratios in z > 3 Galaxies: Insights from the Lumen Model
› A Glimpse of the Low-Mass End of the Direct Mass-Metallicity Relation at $z\sim6-8$
› An HST Wide Field Survey of the Galactic Bulge: Overview, Strategy, and First Results
› Radial redistribution of stellar orbits in FIRE simulations of Milky-Way-mass galaxies
› The galaxy ultraviolet luminosity function from $z=7$ to $15$ in the COLIBRE simulations
› Dark siren cross-correlations and the sensitivity of $H_0$ to methodological choices
› Machine Learning Techniques for Astrophysics and Cosmology: Photometric Redshifts
› Hidden Monsters with SPHEREx I: A goldmine for heavily reddened quasars at cosmic noon
› The study of the circumnuclear environment of accreting supermassive black holes with realistic X-ray spectral models
› On the origin of the environmental step: A BayeSN view of the ZTF SN Ia DR2
› Radio Continuum and Water Maser Monitoring of the Outburst in HOPS 373: Free-Free Emission Does Not Respond to the Outburst
› The impact of envelope binding energies on the merger rate density of binary compact objects
› The Hubble Advanced Spectral Product (HASP) Program
› Taxonomy of 14042 asteroids from Gaia DR3 reflectance spectra
› Spectrally and spatially resolved (sub)millimeter HCN-to-HCO$^{+}$ flux ratios in nearby ultraluminous infrared galaxies
› On the origin of the rotation of massive stars
› $V/\sigma$ Trends with Mass for Dwarf Galaxies from the Marvelous Massive Dwarfs Suite
› $Ab$ $initio$ modeling of Galactic dust polarized CMB foreground
› Diverse dust vertical height and settling strength conditions in protoplanetary discs
› You Only Stack Once (YOSO): A Motion-Filtered, Deep-Learning Framework for Detecting Faint Moving Sources
› X-ray spectroscopy mass constraints on V1674 Her: the fastest nova does not have a near-Chandrasekhar white dwarf
› Scylla VI: Parsec-Scale Dust Extinction Maps in the SMC and LMC
› Exploring TRAPPIST-1 Climate States with an Energy Balance Model
› Characterizing the Extended Molecular Hydrogen Winds in Protoplanetary Disks from the JWST Disk Infrared Spectroscopic Chemistry Survey
› Nuclear Constraints on $^{12}$C$(\alpha,\gamma)^{16}$O and Their Impact on Black-Hole Mass Predictions
› First Interstellar Detection of Methyl Carbamate: A New Observational Anchor for Glycine Chemistry
› Anisotropic Thermal Conduction as a Driver of Jet Collimation and Magnetic Field Amplification on Cold Fronts
› Resonant Inverse Compton Scattering and Hard X-ray Emission in Magnetar Magnetospheres
› Mass Production of 2023 KMTNet Microlensing Planets. III: Three Planets from the Subprime Field
› Diffuse gamma-ray emissions around the stellar cluster Berkeley 59
› Dynamical evolution of Milky Way globular clusters on the cosmological timescale II. Terzan 2, 4, and 5 mass loss and collision tracking
› KM3-230213A and potential astrophysical sources
› Origin and evolution of NiI and FeI in the coma of the interstellar comet 3I/ATLAS throughout its trajectory
› Advance warning of $\gamma$-ray blazar flares from \textit{Fermi}-LAT light curves: a strictly causal machine-learning backtest
› The diverse morphologies and evolution of low-luminosity edge-brightened radio galaxies
› Young Massive Star Clusters as TeV Emitters: Constraints from H.E.S.S. and LHAASO
› Potamides: Mapping Dark Matter Halo Shapes from Stellar Stream Tracks in the Local Universe
› Detection of persistent helium absorption in the 91bg-like type Ia Supernova 2022an
› A New Global Chemical Equilibrium Code: Refractory Element Signatures in Super-Earths and Sub-Neptunes
› HAT-P-70b through the Eyes of MAROON-X: Constraining Elemental Abundances of Metals and Insights on Atmosphere Dynamics
› Investigating Pre-flare Signatures in Spectroscopic Observations of an X9-class Solar Flare
› Constraining the Galactic bar using the M92 stellar stream
› Systematic Comparison between Constrained Transport and Mixed Divergence Cleaning Methods for Astrophysical Magnetohydrodynamic Simulations
› A Changing-Look Seyfert Discovered by eROSITA Reveals a Two-Component Broad-Line Region
› Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff
› Space as a spectroscopic laboratory: High-resolution spectroscopy of the [$^{13}$C II] hyperfine structure with SOFIA/upGREAT
› The Spitzer Spectroscopic Data Fusion -- Merged Spectroscopic Redshift Catalogs in Spitzer Fields
› Inferring Asteroseismic Parameters from Short Observations Using Deep Learning: Application to TESS and K2 Red Giants
› Magnetar field dynamics driven by chiral anomalies without magnetic helicity
› CMB Limits on the Absorption of Light Vector and Axial-Vector Dark Matter
› Neutrino-Antineutrino Conversion from Ultralight Vector Dark Matter
› The structure of multi-axion solutions to the strong CP problem
› Plasma heating during the chiral plasma instability
› Decaying spin-3/2 dark matter from baryon number violation
› Formulation of testing gravitational redshift based on Laser Time link between China Space Station and a ground station
› Probing the Inert Doublet Dark Matter with Stellar-Mass Black Hole Mini-Spikes
› TopoFisher: Learning Topological Summary Statistics by Maximizing Fisher Information
› Kinetic Sunyaev Zel'dovich velocity reconstruction from Planck and unWISE
› Are all models wrong? Falsifying binary formation models in gravitational-wave astronomy
› Multi-Model Framework for Reconstructing Gamma-Ray Burst Light Curves
› 4MOST Cosmology Redshift Survey (CRS): Clustering Properties of CRS Bright Galaxy and Luminous Red Galaxy Target Catalogues
› The Eddington Ratio Distribution of Narrow Line Active Galactic Nuclei
› High-energy radiation from the pulsar Equatorial Current Sheet
› On the Diversity of Pulsar's Frequency-Dependent Circular Polarization
› Light-tight skipper-CCDs for X-ray detection in space
› Diffuse neutrino flux from relativistic reconnection in AGN coronae
› Triaxial Magnetars as Sources of Fast Radio Bursts
› Still Accelerating: Type Ia supernova cosmology is robust to host galaxy age evolution
› Simulated LSST Observations of Real Metre-scale Imminent Impactors
› A General Formulation of the Kinematic Dipole as a Functional of Selection and Source Properties: Beyond the Ellis--Baldwin Approximation
› Molecular Gas Excitation in z ~ 0.7 Gas-Rich Post-starburst Galaxies from SQuIGGLE
› NEXUS: Quick Release Notes
› A jet formation model for astrophysical objects
› Fast X-ray Transients produced by Off-axis Jet-Cocoons from Long Gamma-Ray Bursts
› Coma Physics of an Interstellar Object: JWST Spatial-Spectral Mapping of 3I/ATLAS
› Return to the Great Attractor: Strong Evidence for a Steradian-sized Flow Converging at $\sim$70 Mpc within the GA Supercluster and Aligned with the CMB Dipole
› First Lunar Farside SETI Observations for Periodic Signals with the Low-frequency Radio Spectrometer of Chang'E-4 Mission
› JWST Observations of Starbursts: Dust Processing in the M82 Superwind
› Investigating the Circumgalactic Medium through Mg II absorption coincidence
› TTV-Not-So-Fast: Uniqueness and Degeneracy in Perturbing Planet Parameters
› Stellar flare-driven evolution of primordial early exo-Earth atmospheres: Insights from a Young M Dwarf Flare model
› Long-term study of the gamma-ray emission of Cygnus X-3 with MAGIC and Fermi-LAT
› Alleviating the Hubble Tension Using $\Lambda$sCDM Model: A Coupled Dark Energy - Dark Matter Interaction
› Wave interference as the origin of the cyclic magnetorotational dynamo in accretion disks: insights from weakly nonlinear theory and local shearing box simulations
› A Gaussian process framework for testing general relativity with gravitational waves
› Ultralight dark matter detection with trapped-ion interferometry
› Generalized Perturbed Kepler Problem: Gravitational Wave Imprints from Eccentric Compact Binaries
› Ab initio calculations of beta-decay half-lives for $N=50$ neutron-rich nuclei
› From Weibel seeds to collisionless dynamos beyond pair-plasmas
› Gravitational scalar production with a generic reheating scenario
› Scattering from compact objects: Debye series and Regge-Debye poles
› Revisiting the sphaleron and axion production rates in QCD at high temperatures
› Emergent gravity from nonlinear perturbation of spherical accretion with variable adiabatic index

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