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
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1018.2 hPa

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 Wiadomości z astronet.pl

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RSS  Najnowsze prace na astro-ph:

› First detection of the moving lens effect with ACT and DESI LS
› The Lumina Project: CMB Optical Depth Fluctuations from Patchy Reionization
› The pre-infall bias of subhalos
› Bulgeless Evolution And the Rise of Discs (BEARD) II. The role of mergers in shaping the Milky Way analogues in TNG50
› Mars as an Exoplanet: Lessons from a Planet at the Edge of Habitability
› Planetary formation tracks on the Hertzsprung-Russell diagram: Visualising the processes of giant planet growth
› Mapping 3-D Explosive Nucleosynthesis with Type II Supernova Infrared Emission Lines
› Astrometric exoplanet detection survives solar-like stellar contamination
› Automating the detection of polarization angle rotations in blazars. Re-analysis of RoboPol data reveals 27 new rotations
› Directly tracking the re-brightening of a supermassive black hole accretion disk
› Hyrax: An Extensible Framework for Rapid ML Experimentation and Unsupervised Discovery in the Era of Rubin, Roman, and Euclid
› Low-Luminosity Type IIP Supernovae from the Zwicky Transient Facility Census of the Local Universe. III: Hunting for electron-capture supernovae using nebular spectroscopy
› Environmental Sculpting of Galaxy Structure at Fixed Stellar Mass: A Multi-Scale Analysis Across Cosmic Time using 3 Million HSC Galaxies
› Flavor Conversion Enhances or Suppresses Supernova Explodability Independent of the Progenitor Mass
› GRB 260310A/SN 2026fgk: Photometric and Spectroscopic Evolution of a Nearby GRB-Supernova and an Exceptionally Bright Afterglow at z=0.153
› Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues
› Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies
› How High-Specific-Energy Winds Regulate the Circumgalactic Medium of Dwarf Galaxies
› High-resolution X-ray spectroscopy with XRISM/Resolve reveals super-Solar abundance ratios in Virgo/M87
› Summary of Discussion Sessions from "The Dusty Universe 2025: The Fifth Pandust Conference"
› Blue Straggler Stars in Old Open Clusters and the Kraft Break
› Exoplanets in ancient stellar populations: occurrence constraints and hot-Jupiter candidates in the Galactic halo
› Detection of propadiene (CH$_2$CCH$_2$), propene (C$_3$H$_6$) and non-detection of propane (C$_3$H$_8$) in Jupiter's northern polar stratosphere
› Optimal mitigation of random telegraph noise for improved photometry at high frame rates
› IceCube Second Track Data Release IceTracks-DR2: Data from 2008-2022 for Neutrino Source Searches
› Magnetohydrodynamics Simulations
› VarWISE: Infrared Variability via NEOWISE Single Exposure Photometry
› JWST Observations of Starbursts: Molecular Hydrogen Excitation and Disequilibrium in M82
› Dependence on the Equation of State in SPH Simulations of Proto-Uranian Disk Formation from a Giant Impact
› Radiative PIC simulations of relativistic pair plasma: multiple interacting current sheets and turbulent evolution
› A Cloud-Based Tool for Meteorite Recovery Using Drones and Machine Learning
› Lossless Compression of Cosmological Information from Type Ia Supernova Distance Measurements
› Temporal evolution of the circumstellar disk orientation in the transient X-ray pulsar GRO J1008-57
› Taking Inventory of the Most Promising Lensed Radio Sources for Constraining Fundamental Properties of Dark Matter
› Faraday Complexity and Depolarization in LOFAR Two-metre Sky Survey (LoTSS-DR2) Polarized Radio Sources
› Peculiar velocities at low Galactic latitude
› Active Galactic Nucleus Tori: Potential Birthplace to Millions of Planets
› Correlation between baryonic process and galaxy assembly bias
› Constraints on the Crystallinity of Water Ice in Planet-forming Disks from Infrared Scattered-Light Spectra
› AMPM I. A Targeted Search for Asteroid Mass Primordial Black Hole Microlenses
› A Systematic NLTE Study of Very Metal-Poor Stars with Metallicity Down to $-4.3$ dex. II. Lithium Abundance and New Insight to the Lithium Plateau
› Recombination Thickness as an Uncertainty in Inflationary Observables
› AMPM II. A Lunar-Mass Primordial Black Hole Microlensing Candidate in the Milky Way Halo
› Gaia21bja: pre-main sequence star with quasi-periodic bursts
› Dwarf and Intermediate-Mass Galaxies in MaNGA: Evidence for Different Evolutionary Trends
› Formation of a nuclear star cluster through the inspiral of globular clusters: A case study of the dwarf elliptical galaxy UGC 7346
› Spectro Capture: A Software System for Automated Small-Observatory Spectroscopy
› Memory burden effect of regular primordial black holes
› Chromospheric resonator model for sunspot revealed by multi-height observation of umbral wave
› Radio-X-ray Time Lags in GX 339-4: Probing Magnetic Field Transport in Black Hole Accretion
› Prospect of Measuring the Cosmic Dipole by Strongly Lensed Gravitational Waves Associated with Galaxy Surveys
› Methodological Synergies between Technosignature and UHE Neutrino Searches
› The Astro2Geo Project I. Radio astrometric offsets correlated with Gamma-ray brightness
› A Value-added Physical Properties Catalog for Low-redshift Galaxies from DESI Legacy Imaging Surveys DR10
› Towards inertial-mode helioseismology: Direct sensing of solar rotation at 75 deg latitude and 0.8 Rsun
› Recent Findings from the Telescope Array Experiment
› From mass-loss histories to lightcurves: a generalised framework for interaction-powered transients
› Reassessing the Statistical Necessity of Stellar Velocity Anisotropy in Strong-Lensing Cosmology with Lens-by-Lens Photometric Constraints
› Mare versus highland lunar impact flash light curve dichotomy
› Evidence for Intermediate-Mass Black Holes From Microlensing Signatures in CHIME/FRB catalog 2
› The PARADIGM Project II: Characterising Nuclear and Diffuse Radio Components in Local U/LIRGs
› COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0
› Solar Atmospheric Abundances in Space & Time
› The Small Phased Array DEmonstrator (SPADE) -- Description and first results
› A Parameterized YSO Accretion Disk Model with Increasing Accretion Rate: Predicted Outburst Lightcurves
› Magnetized neutron stars: perturbative versus fully-numerical approaches
› CMB lensing imprints of cosmic voids in DESI Legacy Survey DR9 LRGs with photometric redshift calibration
› Inflaton Accretion onto Primordial Black Holes During Reheating
› Domain-wall Quintessence
› How long can you trust a Starlink TLE? An empirical comparison of SGP4 and high-fidelity propagation against operator-updated truth across a megaconstellation
› Facing the phase: Gravity-mode offset and buoyancy glitches in red--giant branch stars
› Latitudinal variations in Neptune's temperature profile observed with ALMA
› The first IXPE view of the eclipsing ADC source 4U 1822-37
› Arm morphology in off-centre barred galaxies
› New NanoSIMS Multielement Isotope Data Reveal CO Novae As Key Sources Of 13C-rich Presolar Silicon Carbide Grains
› Probing String-Theory-Inspired Topologies of the Early Universe through CMB Temperature and Polarization Anisotropies
› Simulating the Convective Urca Process with Multiple Urca Pairs in a Simmering White Dwarf
› ComPACT: Mass-Redshift Properties of the galaxy cluster catalogue
› Interacting Dark Sector field theory with phantom crossing
› TIC 295741342: A Triply-Eclipsing Triple Star System with a Giant Tertiary
› Gravitational-wave constraints on $H_0$ are robust to (putative) redshift evolution in the binary black hole mass spectrum at current sensitivity
› The potential of diffuse Galactic Ridge neutrino measurements to constrain dark matter
› Galaxy Proximate Damped Lyman-Alpha Systems and HI Reionization Topology in TECHNICOLOR DAWN
› Spectral classification of brown dwarfs using machine learning
› The exceptional 2017 gamma-ray flare of the radio galaxy NGC 1275: VERITAS and Multiwavelength Observations
› Exceptional Points and Resonance in Black Hole Ringdown
› Structure of the $^8$B and $^8$Li nuclei and the astrophysical $S_{17}(0)$-factor of the $^7$Be($p,\gamma$)$^8$B direct capture process within a three-body model
› The Majoron Cosmological Window: Dark Matter and Thermal Leptogenesis
› Magnetic Prandtl number dependence of plasmoid-mediated reconnection
› Quasinormal modes of Proca and Maxwell fields in $d$-dimensional Schwarzschild-AdS black holes
› Affine ANEC selects the closed FRW branch for geodesically complete cosmology
› GstLAL O4 Online Results Paper
› Elemental Stoichiometry as an Ecological Biosignature with Applications to Life Detection
› Locality in effective field theory for inflationary soft modes
› The stability of color-flavor-locked quark matter and massive CFL quark stars
› Neutron stars more compact than black holes in quasi-topological gravity: Equilibrium configurations and radial stability
› A new analysis of the "hep" S-factor and the "hen" cross section
› A novel pre-inflationary model in view of the lack of angular correlation of CMB
› Dark Matter Interpretation of the Super-Kamiokande Antineutrino Excess and Predictions for JUNO
› WIMP-like Dark Matter Without Thermalization At Freeze-Out
› Direct T_e-based Metallicities of z=2-9 Galaxies with JWST/NIRSpec: Empirical Metallicity Calibrations Applicable from Reionization to Cosmic Noon
› The AURORA Survey: The Nebular Attenuation Curve of a Galaxy at z=4.41 from Ultraviolet to Near-Infrared Wavelengths
› Sulfur on Venus: Atmospheric, Surface, and Interior Processes
› Particle Acceleration Time due to Turbulent-Induced Magnetic Reconnection
› Cosmic Ray Ionization of Low-Excitation Lines in Active Galactic Nuclei and Starburst Galaxies
› Low-Luminosity Type IIP Supernovae from the Zwicky Transient Facility Census of the Local Universe. I: Luminosity Function, Volumetric Rate
› DEMNUni: the Sunyaev-Zel'dovich effect in the presence of massive neutrinos and dynamical dark energy
› Low-Luminosity Type IIP Supernovae from the Zwicky Transient Facility Census of the Local Universe. II: Lightcurve Analysis
› A Census of Variable Radio Sources at $3\,$GHz
› The AURORA Survey: High-Redshift Empirical Metallicity Calibrations from Electron Temperature Measurements at z=2-10
› $f$-mode Oscillations for Hyperons and H-dibaryons in Neutron Stars
› Primordial black holes versus their impersonators at gravitational wave observatories
› Cosmic-ray impact on optical and mid-infrared emission line diagnostics in NGC 5728
› Constraining gamma-ray burst parameters with the first ultra-high energy neutrino event KM3-230213A
› Effects of primordial magnetic fields on 21 cm multifrequency angular power spectra
› Under Pressure: Decoding the Effect of High Densities on Derived Nebular Properties
› Addressing prior dependence in hierarchical Bayesian modeling for PTA data analysis II: Noise and SGWB inference through parameter decorrelation
› Disk warping and black hole X-ray binaries I. Tentative unification of low-frequency quasi-periodic oscillations
› High-Precision Amplitude-Modulated Continuous-Wave Lunar Laser Ranging
› The impact of strong feedback on galaxy group scaling relations
› Kennicutt-Schmidt relation of galaxies over 13 billion years in the COLIBRE hydrodynamical simulations
› A radially broad collisional cascade in the debris disk of $\gamma$ Ophiuchi observed by JWST
› Propulsion Trades for a 2035-2040 Solar Gravitational Lens Mission
› Detection horizon for the neutrino burst from the stellar helium flash
› Constraining Neutrino Mass with the Void Weak Lensing Effect
› Reconstructing the Type Ia Supernova Absolute Magnitude with Two-Probe Physics-Informed Neural Networks
› Orbital Debris in Earth Orbit: Operations, Stability, Control, and Market Formation
› Oxygen and nitrogen isotopologues on cold COCONUTS-2b observed with MIRI/MRS
› Stardust Galaxies at z>9: A Dust-Origin Transition Behind the Excess of UV-Bright Galaxies
› Energy Evolution from the Chromosphere to the Heliosphere in the 2021 October 28 Solar Eruption
› From inter-filamentary gas to filaments and hubs: gas flows in the Mon R2 hub-filament system
› Higher-order statistics of the stochastic gravitational wave background from supermassive black hole binaries
› Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties
› On binary pulsars and the force of gravity
› Classical and Semiclassical Stability of Emergent Universes in Jordan-Brans-Dicke Theory
› Reviving WIMP dark matter with temperature-dependent couplings
› The Muonic Portal to Vector Dark Matter:connecting precision muon physics, cosmology, and colliders
› Data-driven exploration of the neutron $^3\text{P}_2$ pairing gap using Cassiopeia A neutron star observational data: Direct $\chi^2$ minimization
› Minimal Freeze-in Dark Matter: Reviving electroweak doublet dark matter with Boltzmann suppressed freeze-in
› GR from RG: Gravity Is Induced From Renormalization Group Flow In The Infrared
› Modifications of CMB Temperature and Polarization Quadrupole Signals in Thurston Spacetimes

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