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

› Katalog Caldwella: C19
› Misje kosmiczne XX wieku: Program Landsat
› Katalog Caldwella: C88
› Katalog Caldwella: C28
› Katalog Caldwella: C102
› Liczba czarnych dziur we wszechświecie może być mniejsza niż wcześniej zakładaliśmy
› Sterowanie lotem za pomocą balonów – projekt DracoSat
› Katalog Caldwella: C13
› Misje Kosmiczne XX wieku: Endeavour
› Katalog Caldwella: C103
RSS  Najnowsze prace na astro-ph:

› Quenching pathways in the green valley at low redshift: confronting SDSS AGN hosts with IllustrisTNG and EAGLE
› Multi-Messenger Predictions for T Coronae Borealis: Probing Particle Acceleration in Novae
› On the origin of sinusoidal brightness variations in F to O-type stars through radial velocities
› Water Production of Interstellar Comet 3I/ATLAS from SOHO/SWAN Observations after Perihelion
› Clustering Confuses Spectro-photometry: An Investigation of 2D and 3D Forced Profile Matching for Stacking Line-intensity Mapping Data on Source Catalogues
› Interstellar Interloper 3I/ATLAS: Nucleus Size, Photometry in RGB, Af(rho) and Antitail Structure Analysis
› Formation of the Moon and Binary Asteroids
› Simulations of facular magnetic fields on cool stars I: Main sequence stars with solar metallicity
› Space AI: Leveraging Artificial Intelligence for Space to Improve Life on Earth
› On the origin and nature of double-double radio galaxies
› Chain Reactions in Space: Analyzing the Impact of Satellite Collisions and Debris Accumulation
› Starkindler: An Uncertainty Aware Objective for Photometric Redshift Estimation
› Evidence for a Stratified Accretion Disk Wind in AGN
› Kinematical and Photometric Deconstruction of the UGC 694-IC 412 System: Evidence for a Line-of-Sight Projection
› A Generative Reconstruction of Low-$\ell$ CMB B-Mode Signal using Reverse Diffusion in Deep Learning
› Lithium abundance and stellar rotation in the Galactic halo and thick disc: Contribution from low-mass giant field stars
› Cloud Properties and Star Formation in M31
› Heavy dark matter in rapidly evolving massive stars
› Rotation and stability of the circumnuclear gas disk in the Galactic Center potential by the ALMA CMZ Exploration Survey (ACES)
› Hierarchical Test of Lorentz Invariance with Gamma-Ray Burst Spectral-Lag Measurements
› Primordial black holes within Higgs hybrid metric-Palatini approach
› Impacts of the $^{16}$O($^{16}$O, n)$^{31}$S reaction rate on the evolution and nucleosynthesis in Pop III massive stars
› A new path to constrain the expansion history of the Universe in future spectroscopic galaxy surveys
› Pulsed, Polarized X-ray Emission from Neutron Star Surfaces: the Effects of Vacuum Birefringence in the Magnetosphere
› An Empirical Law to Reproduce the Galaxy Rotation Curves
› Dark matter direct detection: status, results and future plans
› A Linearized Approach to Radial-Velocity Extraction. II: Shot-Noise-Limited Precision via Spectral Factorization
› Finding Quasars behind the Galactic Plane. IV. Candidate Selection from Chandra with Random Forest
› Two birds with one stone: simultaneous realization of both Lunar Coordinate Time and lunar geoid time by a single orbital clock
› Why Machine Learning Models Systematically Underestimate Extreme Values II: How to Fix It with LatentNN
› The GLASS-JWST Early Release Science Program. V. H$\alpha$ luminosity functions at $z\sim1.3$ and $z\sim2.0$
› MAMMOTH-LyC: Investigating the Role of Galaxy Mergers in a Strong Lyman Continuum Leaker at $z=2.39$
› Unveiling Multimessenger Emission from Hidden Cores of Microquasars
› Interpreting the diversity of afterglow emission from radio-detected tidal disruption events with instantaneous and delayed outflows
› SN 2022acko: a low-luminosity SNe IIP with signs of early circumstellar interaction
› New Constraints on Cosmic-ray boosted Sub-GeV Dark Matter via Light Mediators
› The Dependence of the Extinction Coefficient on Reddening for Galactic Cepheids
› Kilonova and progenitor properties of merger-driven gamma-ray bursts
› Predicting the detection yields of giant planets and brown dwarfs with CSST astrometry
› SiO emission in the filamentary Infrared Dark Cloud G035.39-00.33: An ALMA view
› Revisiting the Reported Period of FRB 20201124A Using MCMC Methods
› Possibility of Month-scale Quasi-periodic Oscillations in the Gamma-ray Light Curve of OP 313
› Three channel dissipative warm Higgs inflation with global inference via genetic algorithms
› Unveiling SN 2022eyw: A Bright Member of the Type Iax Supernova Subclass
› On Systematic Errors in Cross-Identification of Binary Stars in Gaia
› Detections of Compact Radio Continuum toward Methanol Maser Rings Using the VLA
› Observations of the Fermi bubbles and the Galactic center excess with the DArk Matter Particle Explorer
› Lossless compression of simulated radio interferometric visibilities
› Sidelobe Modification for an Offset Gregorian Reflector System using a Reconfigurable Intelligent Surface-Equipped Subreflector
› Not Just Gas: How Solid-Driven Torques Shaped the Migration of the Galilean Moons
› Limits on dark matter existence in neutron stars from recent astrophysical observations and mass correlation analysis
› The 24 Aqr triple system: A closer look at its unique high-eccentricity hierarchical architecture
› Precise Physical Parameters, Habitability, and Orbital Stability of Sun-like SB2 Systems: HD 130669, HD 184467, HD 191854, and HD 214222
› Classification and Characteristics of Double-trigger Gamma-ray Bursts
› Galaxy Zoo Evo: 1 million human-annotated images of galaxies
› Matter environments around black holes: geodesics, light rings and ultracompact configurations
› Gravitational waves from seesaw assisted collapsing domain walls
› Cosmological long-wavelength solutions in non-adiabatic multi-fluid systems
› Double to tenfold M-shell photoionization of singly charged lanthanum ions
› Exploring Interplays Between $^3\text{P}_2$ Neutron Superfluid Vortices and $^1\text{S}_0$ Proton Fluxtubes in the Outer Core of Neutron Stars
› Schwinger-Keldysh Cosmological Cutting Rules
› Toward the Effective Light and Heavy QCD Axion Scenarios
› Multi-messenger detectability of continuous gravitational waves from the near future to next generation detectors
› Colloquium: Multimessenger astronomy with continuous gravitational waves and future detectors
› Gravitational Noether-Ward identities for scalar field
› Mini-review on the production of Primordial Black Holes from First-Order Phase Transitions in the Early Universe
› Reconstructing Relativistic Magnetohydrodynamics with Physics-Informed Neural Networks
› Search for Annual Modulation in Combined ANAIS 112 and COSINE 100 Data using Bayesian Model Comparison
› Neutron Star Equation of State with Nucleon Short-Range Correlations: A Concise Review and Open Issues
› Compact star and compact star matter properties from a baryonic extended linear sigma model with explicit chiral symmetry breaking
› Frozen Neutron Stars in Four-Dimensional Non-polynomial Gravities
› Defect Formation in NaI Crystals: A Novel Pathway to Dark Matter Detection
› The new generation lunar gravitational wave detectors: sky map resolution and joint analysis
› Predicting large scale cosmological structure evolution with generative adversarial network-based autoencoders
› First Use of GPS Satellites for Beam Calibration of Radio Dish Telescopes
› Vortex driven Schwingrer pair creation in the magnetosphere of SgrA*
› Probing the Cosmic Reionization History with JWST: Gunn-Peterson and Ly$\alpha$ Damping Wing Absorption at $4.5 < z < 13$
› Non-Stationary Discs and Instabilities
› Impact of general relativistic accretion on primordial black holes
› Nonminimal infrared gravitational reheating in light of ACT observation
› A joint JWST and HST view of Omega Centauri: Multiple stellar populations and their kinematics
› Investigating FRB 20240114A with FAST: Morphological Classification and Drifting Rate Measurements in a Burst-Cluster Framework
› A Generative Model for Disentangling Galaxy Photometric Parameters
› The Lyman-$\alpha$ Forest from LBGs: First 3D Correlation Measurement with DESI and Prospects for Cosmology
› Cooling of dark neutron stars
› Alpha effect and dynamo in density-stratified turbulence with large-scale shear: applications to protoplanetary discs and astrophysical clouds
› VLA FRAMEx. III. Circumnuclear Radio Emission Mechanisms in Hard X-ray Selected Active Galactic Nuclei
› Search for a photon peak from keV-scale dark matter annihilation with NuSTAR: Constraints on $\langle \sigma v \rangle$ after 11 years of observations
› Extended mass distribution of PBHs during QCD phase transition: SGWB and mini-EMRIs
› The Formation of Electron-capture Supernovae: A Review
› Optically thick winds of very massive stars suppress intermediate-mass black hole formation
› The ALPINE-CRISTAL-JWST Survey: JWST/IFU Optical Observations for 18 Main-Sequence Galaxies at z=4-6
› A Unified Photometric Redshift Calibration for Weak Lensing Surveys using the Dark Energy Spectroscopic Instrument
› Radiation-dominated polar emitting region of an accreting X-ray pulsar -- I. Polarization- and spectrum-dependent structure, and the emergent continuum
› Study the nature of dynamical dark energy by measuring the CMB polarization rotation angle
› Starobinsky Inflation and the Latest CMB Data: A Subtle Tension?
› A Dynamical Scalar Field Model for Dark Energy: Addressing the Hubble Tension and Cosmic Evolution
› Doppler imaging combined with high-cadence photometry. I. Revisiting the surface of a pre-main-sequence flare star
› Connecting clustering and the cosmic web:Observational constraints on secondary halo bias
› The Evolving Baryonic Tully Fisher Relation: A Universal Law from Galaxies to Galactic Clusters
› A Search for Hard X-ray/Soft $\gamma$-ray Emission from SPT-CL J2012-5649 (Abell 3667) Using INTEGRAL/ISGRI
› The Serendipitous Axiodilaton: A Self-Consistent Recombination-Era Solution to the Hubble Tension
› Cygnus X-3: A variable petaelectronvolt gamma-ray source
› Towards an agnostic algorithm for sampling empirical structure models: The case of Uranus and Neptune
› A Correlation Between Black Hole Mass and Dark Matter Halo Concentration in Cosmological Simulations
› Robust and scalable simulation-based inference for gravitational wave signals with gaps
› $\mathbf{\Omega_1\Omega_2}$-$\mathbf{\Lambda}$CDM: A promising phenomenological extension of the standard model of cosmology
› A systematic study on the aromatic and aliphatic hydrocarbon emission features of nearby galaxies using AKARI near-IR spectra
› Theory-agnostic searches for non-gravitational modes in black hole ringdown
› Modified Models for Neutrino Masses and Mixings
› Dynamical de Sitter conjecture and quintessence model
› Unveiling the Velocity-Space Signature of Ion Cyclotron Damping Using Liouville Mapping
› Electron Inertia and Magnetic Reconnection
› Light thermal dark matter models in the light of DAMIC-M 2025 constraints
› Some Properties of Multi-Component Axion Dark Matter
› Higher Curvature Inflation and the Species Scale
› Nearly forgotten results in development of physical cosmology
› Streamlined Supergravity
› Can the 3 neutrino masses really be found using SN 1987A data?
› A mini-review on combinatorial solutions to the Marcus-Lushnikov irreversible aggregation
› Modified light-cylinder and centrifugal acceleration in Schwarzschild geometry

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