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

› Wada zwierciadła Kosmicznego Teleskopu Hubble’a
› Drugi w historii lot komercyjnej rakiety z lądowaniem boostera!
› Misje Kosmiczne XX wieku: Atlantis
› Recenzja książki „Księżyc. Jak zmienił naszą planetę, przewodził ewolucji i stworzył nas takimi, jakimi jesteśmy”
› Insekty przyszłością diety astronautów?
› W Układzie Słonecznym: Obłok Oorta
› Misje kosmiczne XX wieku: Challenger
› Galaktyczny kartograf – Teleskop Nancy Grace Roman
› Niebo w listopadzie 2025 roku
› Misje kosmiczne XX wieku: Discovery
RSS  Najnowsze prace na astro-ph:

› Further correction to the STARFORGE methods paper: Planck-mean dust opacities
› A Unified Analytic Framework for Microlensing Caustics: Geode Solutions and Hyper--Catalan Signatures
› Iron Nuclei in Ultra-High Energy Cosmic Rays Near the Earth
› Trading oxygen for iron II. Oxygen- versus iron-dependent cosmic star formation history
› Fossil group origins XIV: The radial orbits of A267
› Efficiency of Hydrodynamic Atmospheric Escape in Hot Jupiters and Super Earths
› Decoding the Radio Sky: Bayesian Ensemble Learning and SVD-Based Feature Extraction for Automated Radio Galaxy Classification
› Do z>6 quasars reside in protoclusters?
› Electron densities from [S II] lines significantly overestimate the impact of ionised AGN outflows
› A first look at a complete view of spatially resolved star formation at 1
› How Bright in Gravitational Waves are Millisecond Pulsars for the Galactic Center GeV Gamma-Ray Excess? A Systematic Study
› The MeerKAT Fornax Survey VI. The collapse of the galaxy HI Mass Function in Fornax
› Universal depletion of metal-poor globular clusters in inner galaxy regions: Fossil record of black hole retention
› The Noisy Universe
› The abundance and properties of the lowest luminosity dwarf galaxies around the Milky Way: Insights from Semi-Analytic Models
› Unveiling Chemical Enrichment in the Abell 2029 Core with XRISM, XMM-Newton, and Chandra
› Revised optical classification of a sample of gamma-ray emitting AGN with GTC and VLT
› Numerical Determination of the Gravitational Cross Sections of an Accreting Binary
› The SPHEREx Image and Spectrophotometry Processing Pipeline
› Observational constraints on the product of dark energy chemical potential and number density in out-of-equilibrium models
› Methane on the temperate exo-Saturn TOI-199b
› DESI-Like Hubble Expansion From Staged Symmetry Breaking
› Mean Mass Density near the Sun from the Divergence Theorem and Pulsar Accelerations
› CLASSY XIII. Cutting through the Clouds - Comparing Indirect Tracers of Ionizing Photon Escape
› Helium Depletion in Escaping Atmospheres of Sub-Neptunes: A Signature of Primary-to-Secondary Transition
› Post-Supernova Accretion of Light Elements onto a New-Born Neutron Star and NS 1987A
› Effects of New Forces on Scalar Dark Matter Solitons
› SN 2019vxm: A Shocking Coincidence between Fermi and TESS
› Solar Filament Physiognomy: Inferring Magnetic Quantities from Imaging Observations
› Formation of Extremely Low-Mass White Dwarfs in Wide Orbits
› JWST observations of cosmic-ray-excited H$_2$ in Barnard 68: spatial variations and constraints on cosmic-ray attenuation
› Cosmological Constraints on the Phenomenological Interacting Dark Energy Model with Fermi Gamma-Ray Bursts and DESI DR2
› The PAU Survey: The $i$-band galaxy luminosity function from the present-day to $z = 2$
› Analytical Solutions for Planet-Scattering Small Bodies
› Optimization design and analysis for the mechanical test platform of scientific probe module of the Cool Planet Imaging Coronagraph
› Large gas inflow driven by a matured galactic bar in the early Universe
› Too Quiet for Comfort: Local Little Red Dots Lack Variability over Decades
› Forecasting the Constraint on the Hu-Sawicki $f(R)$ Modified Gravity in the CSST $3\times2$pt Photometric Survey
› Type II Cepheids: Period-Luminosity-Metallicity relations for the Population II distance scale
› Chemical evolution of bulges of active galactic nuclei in the early Universe: roles of accreting stars
› Creation of Viscous Dark Energy by the Hubble Flow: Comparison with SNe Ia Master Sample Binned Data
› Coupled atmospHere Interior modeL Intercomparison (CHILI) Protocol Version 1.0: A CUISINES Intercomparison Project of Magma Ocean Models
› MAMMOTH-Grism: Revisiting the Mass-Metallicity Relation in Protocluster Environments at Cosmic Noon
› Two Epochs of VLBI Observations of 8 KISSR Seyfert & LINER Galaxies: Suggestions of Fast and Filamentary Outflows
› A pilot VLBI study of the SQUAB quasar sample featuring multiple Gaia detections
› The Fluorescence Camera for the PBR mission
› Hidden Metallic Iron in Amorphous Silicate Dust? Insights from Condensation Experiments and Mid-Infrared Spectroscopy
› Asteroid phase curve modeling with empirical correction for shape and viewing geometry
› Constraining interacting dark energy models with black hole superradiance
› Constraining the Corona Geometry of Cyg X-1 with Broad Band Spectrum and Polarimetric Analysis Based on Observations in May 2022
› Dynamical simulation of the Interstellar Comet 3I/ATLAS
› Accelerating Reionization Constraints: An ANN-Emulator Framework for the SCRIPT Semi-numerical Model
› Absorption effects in the expanding Universe: spectral transmittance functions of intergalactic medium for distant sources
› Thermal equilibrium curves of accretion disks driven by magnetorotational instability
› Can Wolf-Rayet stars be the missing ingredient to explain high-z He II ionizing radiation?
› Environmental Invariance of the Galaxy Size-Mass Relation
› An observationally based wind model contemporaneous with the radio detections in $\tau$ Bo\"otis
› WFC3/UVIS EPER CTE 2009-2025
› WFC3/IR Geometric Distortion - Time Evolution of Linear Terms w.r.t. Gaia DR3
› Grain growth in protoplanetary disks in the Upper Scorpius revealed by millimeter-wave spectral indices
› How Single-Star Guiding affects HST's Pointing Stability
› Denoising weak lensing mass maps with diffusion model and generative adversarial network
› Aql X-1 from dawn 'til dusk: the early rise, fast state transition and decay of its 2024 outburst
› Tracing Early Cosmic Chemical Enrichment: A Uniform XMM-Newton Survey of Metallicity in Galaxy Groups and Clusters
› Collision frequency between dark matter subhaloes within Milky Way-like galaxies
› Searching for primitive, dark, spectrally red asteroid families in the main belt with Gaia
› A homogeneous TTV investigation of all TESS systems with a confirmed single transiting planet
› A Butterfly's Eye Camera for Intensity Interferometry with Cherenkov Telescopes
› Two-beam Multiparticle Many-body simulations of Inhomogeneous FFI
› Neutron star heating vs. HST observations
› Disc fragmentation. I. Ejection of Jupiter-mass Free Floating Planets from growing binary systems
› Fundamental effective temperature measurements for eclipsing binary stars - VII. The solar twin in LL Aquarii
› Dark Matter-Dark Radiation Interactions and the Hubble Tension
› Bayesian polarization calibration and imaging in very long baseline interferometry
› FQ Circini: An Ordinary Nova with a High-mass B1 V(n)(e) Companion Whose Decretion Disk Transfers Mass to the White Dwarf via Roche-Lobe Overflow
› Dark energy after pre-recombination early dark energy in light of DESI DR2 and the latest ACT and SPT data
› Searching for close-in planets around TWA 7 with SPIRou
› The ensemble broad-frequency power spectrum of Stripe-82 quasars from multiple surveys
› Excitation of Inertial Modes in 3D Simulations of Rotating Convection in Planets and Stars
› A Core-Collapse Supernova Neutrino Parameterization with Enhanced Physical Interpretability
› Lucky Strikes: On the Origins of GW190814 Through Isolated Binary Evolution
› Connecting the Dots: A Machine Learning Ready Dataset for Ionospheric Forecasting Models
› Holographic Constraints on the String Landscape
› How light can ALP dark matter be?
› Teukolsky by Design: A Hybrid Spectral-PINN solver for Kerr Quasinormal Modes
› A scattering perspective on gravitational lensing
› Structure Formation with Dark Magnetohydrodynamics
› Streamlined Supergravity
› Neuromorphic Astronomy: An End-to-End SNN Pipeline for RFI Detection Hardware
› Temperature definitions and phase transitions within non-minimal large and small inflationary potentials
› Development and Testing of a Modular Large-Area Cosmic Ray Telescope Using Scintillator-Fiber Hybrid Design for Millimeter-Level Muon Tracking
› Herglotz-type $f(R,T)$ gravity
› High-frequency Gravitational Waves from Superstring Phases in the Early Universe
› Development & Characterization of Electrodes for large-scale Xenon Time Projection Chambers
› WIMP Freeze-out dynamics under Tsallis statistics
› Deep Learning Framework for Enhanced Neutrino Reconstruction of Single-line Events in the ANTARES Telescope
› k-inflation: Non-separable case meets ACT measurements
› Domain walls in the scaling regime: Equal Time Correlator and Gravitational Waves
› Prospects for Neutrino Observation and Mass Measurement from Binary Neutron Star Mergers
› An Introduction to Single-Antenna Radio Astronomical Polarimetry
› Mirage Sources and Large TeV Halo-Pulsar Offsets: Exploring the Parameter Space
› Cross-correlating the EMU Pilot Survey 1 with CMB lensing: Constraints on cosmology and galaxy bias with harmonic-space power spectra
› Compact Size, High $\Sigma$SFR: Defining Morphological Features of Ly$\alpha$-Emitters
› Constraining the Hubble Constant with a Simulated Full Covariance Matrix Using Neural Networks
› Aeos: The Impact of Population III Initial Mass Function and Star-by-Star Models in Galaxy Simulations
› Analytic calculation of dynamical friction for Plummer sphere in ultralight dark matter
› Did DESI DR2 truly reveal dynamical dark energy?
› $f$-mode oscillations in hot Neutron Stars: Effect of hyperons and neutrino trapping
› Planetary dynamos driven by semiconvection in stably stratified layers
› Optimizing Gaussian Process Kernels Using Nested Sampling and ABC Rejection for H(z) Reconstruction
› On the interpretation of XRISM X-ray measurements of turbulence in the intracluster medium: a comparison with cosmological simulations
› Stochastic star formation activity of galaxies within the first billion years probed by JWST
› Converging on the Cepheid Metallicity Dependence: Implications of Non-Standard Gaia Parallax Recalibration on Distance Measures
› JWST spectroscopic confirmation of the Cosmic Gems arc at z=9.625 -- Insights into the small scale structure of a post-burst system
› Cosmological observational tests in the JWST Era. I: angular size - redshift
› Differential rotation of solar {\alpha} sunspots and implications for stellar light curves
› The Cosmic Dance: Observational Detection of Coherent Spin in Galaxy Clusters
› A generalized study of linear electromagnetic cascades in astrophysical sources
› Quasar Radiative Feedback May Suppress Galaxy Growth on Intergalactic Scales at $z = 6.3$
› Characterizing Vortex-Driven Dynamics in the Solar Atmosphere Using Information Theory
› Unlocking 21cm Cosmology with SBI: A Beginner friendly NRE for Inference of Astrophysical Parameters
› Signatures of dynamical activity in the hot gas profiles of groups and clusters in the FLAMINGO simulations
› Spectral survey of the diffuse gas toward BL Lac in the Q band
› Asymmetries in stellar streams induced by a galactic merger
› Black-hole X-ray binary Swift J1727.8$-$1613 shows simultaneous Type-B and Type-C quasi-periodic oscillations across the hard-intermediate and soft-intermediate states
› Galaxy Protoclusters as Drivers of Cosmic Reionization: I. Bubble Overlap at Redshift z ~ 7 in LAGER-z7OD1
› Assessing the star formation history of all-sky and part-sky 100pc white dwarf samples
› Morphology of Inflationary Gravitational Wave Spectra imprinted by a Sequence of Post-Inflationary Epochs $via$ ${\rm GWInSpect}$
› DiffstarPop: A generative physical model of galaxy star formation history
› JWST lensed quasar dark matter survey IV: Stringent warm dark matter constraints from the joint reconstruction of extended lensed arcs and quasar flux ratios
› Dust Recycling and Icy Volatile Enhancement (DRIVE): A Novel Method of Volatile Enrichment in Cold Giant Planets
› JWST Lensed Quasar Dark Matter Survey III: Dark Matter Sensitive Flux Ratios and Warm Dark Matter Constraint from the Full Sample
› POLAR-2 -- Latest Developments of the Next Generation GRB Polarimeter
› TIME Commissioning Observations: I. Mapping Dust and Molecular Gas in the Sgr A Molecular Cloud Complex at the Galactic Center
› The Atacama Cosmology Telescope: A demonstration of CMB lensing measurement from daytime data
› Indirect forces in disc-planet interaction
› Shaping the Mantle: The Role of Superheated Cores After Giant Impacts
› The ALMA-QUARKS survey: Evidence of a candidate high-mass prestellar core aside a bright-rimmed cloud IRAS 18290-0924
› Type Iax supernovae as a source of iron-rich silicate dust
› Prospects for detecting asteroid-mass primordial black holes in extreme mass-ratio inspirals with continuous gravitational waves
› Partial tidal disruption of White Dwarfs in off-equatorial orbits around Kerr black holes
› Energy transfer by feebly interacting particles in supernovae: the trapping regime
› Leading bounds on micro- to picometer fifth forces from neutron star cooling
› Neutrino-Mass-Driven Instabilities as the Earliest Flavor Conversion in Supernovae
› Creating a Universe from Nothing as an Alternative to the Cosmological Principle
› Heat propagation in rotating relativistic bodies
› Gravitational collapse with torsion and universe in a black hole
› Hybrid Active-Passive Galactic Cosmic Ray Simulator: experimental implementation and microdosimetric characterization

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