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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RSS  Najnowsze prace na astro-ph:

› Multi-wavelength morphology and dust emission in low-redshift dwarf galaxies in COSMOS-Web with HST and JWST
› All the Massive Galaxy Overdensities during Reionization: JWST Rest-Frame Optical Selection Reveals Young, Chemically Evolved Galaxies Embedded in Dense, Neutral Gas at z > 5
› Downsizing does not extend to dwarf galaxies: identifying the stellar mass regimes shaped by supernova and AGN feedback
› A Faint Progenitor System for the Faint Supernova 2024vjm
› Polarization Signatures of Inspiraling Hotspots around Kerr Black Holes
› Black Hole Feedback, Galaxy Quenching and Outflows at Cosmic Dawn: Analysis of the SEEDZ Simulations
› Continuous Gravitational Waves from Supersoft X-ray Sources: Promising Targets for deci-Hz Detectors
› An Interactive Metrics Dashboard for the Keck Observatory Archive
› Limits on the Post-eclipse Emission Spectrum of HD 80606 b From High-Resolution Spectroscop
› Spectral response of SPHEREx
› NIAC project report: Solar system-scale VLBI to dramatically improve cosmological distance measurements
› The Y Dwarf Population with HST: unlocking the secrets of our coolest neighbours -- III. Near-Infrared Photometry
› Unraveling the mysteries of Jets in peculiar NLSy1 galaxies through multi-wavelength variability
› A Comparative Study of the Supernova Remnant Cassiopeia A from 2013--2020 Deep [Fe II]+[Si I] Images
› Probing Dust Composition in Distant Galaxies with JWST Mid-IR Spectroscopy of Quasars with Foreground 2175 A Absorbers I: Methodology
› Unipolarity of the solar magnetic field in equatorial coronal holes
› A Gravitational Wave Background from Intermediate Mass Black Holes in AGN Disks
› astromorph: Self-supervised machine learning pipeline for astronomical morphology analysis
› Characterisation of starspot structure and differential rotation of Kepler-411
› Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology
› Transient Relativistic Iron Emission Line from an X-ray Flaring Supermassive Black Hole
› Towards a general field equation for galaxies and galaxy clusters
› ALMA [CI] Image of the Circumnuclear Disk of the Milky Way: Inflowing Low-density Molecular Gas
› Are carbon deflagration supernovae triggered by dark matter ?
› Origin of Hyperion and Saturn's Rings in A Two-Stage Saturnian System Instability
› Selecting Post-Starburst Galaxies Based on Star Formation History
› Orbital Period Changes of Recurrent Nova T Pyxidis Demonstrate that M_ejecta >> 11.3xM_accreted and Is Not a Type Ia Supernova Progenitor
› Spectroscopic He I 1083 nm prominence eruption observations in the middle corona with MLSO/UCoMP
› Mass-Radius Constraints for 2S 0918-549 from an RXTE Superexpansion Burst: A Direct Cooling-Tail Analysis
› A Monopolar Jet from Protostar HOPS 10: Evidence for Asymmetric Magnetized Launching
› The compositions of the HR 8799 planets reflect accretion of both solids and metal-enriched gas
› A deep MeerKAT view of associated HI absorption in radio AGNs at intermediate redshift: Role of absorber geometry and conditions of the gas
› A new strategy for achieving multiple continuous cooling stages in an adiabatic demagnetization refrigerator
› Systematic Study of the Simultaneous Events Detected by GECAM
› A Narrowband Technosignature Search Toward the Hycean Candidate K2-18b Using the VLA and MeerKAT
› Microlensing events and primordial black holes in the axionlike curvaton model
› Herschel/HIFI Observations of Molecular Lines Toward G10.47+0.03
› X-ray Timing and Spectral studies of bare AGN Mrk 110
› Highly suppressed tensor-to-scalar ratio from a modified Lennard-Jones inflationary potential
› Comet 73P/Schwassmann-Wachmann 3's Dust Trail as a Source of Pickup Ions
› Organic Acid Chemistry in ISM: Detection of Formic Acid and its Prebiotic Chemistry in Hot Core G358.93$-$0.03 MM1
› EMU Radio Observations of Barred Spiral Galaxy NGC 5938 (Araish)
› Global statistical entropy and its implications for the main sequences of stars and galaxies
› Talking with the Latents -- how to convert your LLM into an astronomer
› Two-dimensional metallicity distribution of the ionized gas in NGC 628 and NGC 6946
› A Deep Precursor-Dip-Main Superoutburst Sequence in VW Hydri Observed with TESS: High-Cadence Constraints on the Thermal-Tidal Instability Model
› Stellar-mass black holes in young massive and open stellar clusters -- VII. Comparisons with gravitational-wave events until LVK-O4a and Gaia compact binaries
› Non-minimally Coupled Running Curvaton: A Unified Approach to Early-Universe Inflation and Phantom Dark Energy
› Massive disk galaxies with high surface brightness plus low surface brightness stellar disks, hosted by massive dark matter halo -- a TNG50 simulation study
› Characterisation of an EXor outburst SPICY 97589
› Analysis of Galactic cirrus filaments in HSC-SSP high-resolution deep images using artificial neural networks
› Estimating Electron Densities in the Middle Solar Corona using White-light and Radio Observations
› The Pollux European instrument concept for HWO: a high-resolution spectrograph and spectropolarimeter from the far-UV to the near-IR
› Searching for rotational X-ray modulation on TIC 277539431
› Investigating the Nested Structure of the Outflow from the Low Luminosity Protostar IRAS 16253-2429 using JWST and ALMA
› A comparison of G-band brightness as a proxy-magnetometer in various magnetic configurations
› Resolved Dust Emission and CO Isotopologues in Giant Molecular Clouds of the Andromeda Galaxy
› In-flight calibration of the INTEGRAL/IBIS Compton mode: Application to the Crab Nebula polarization
› Reference File Updates Following the Application of New Geometric Distortion and Walk Corrections I: Overview
› A Detailed Study of the Physical and Orbital Characteristics, and Eclipse Timing Variations of the Post Common Envelope Binary DD CrB
› Chromospheric Flashes in a Solar Pore: Insights from Multi-line Spectropolarimetric Diagnostics
› Physical properties of circumnuclear ionising clusters. IV. NGC 1097
› The supernova remnant J0450.4-7050 possesses a jets-shaped point-symmetric morphology
› Operational Mass Measurement for Flyby Reconnaissance Missions of Potentially Hazardous Asteroid
› Dark Energy Survey Year 6 Results: Cosmological Constraints from Cosmic Shear
› Gaia white dwarfs with infrared excess I. The 100 pc catalogue
› SDSS-V Local Volume Mapper (LVM): Helix Nebula public data, Data Analysis Pipeline data products
› Constraining long-lived dark sector particles with CMB and Lyman-$\alpha$
› Effects of Numerical Resolution on Simulated Cloud-Wind Interactions
› Narrow absorption lines from intervening material in supernovae. IV. Type Ia supernovae: Na I D line strength relating to external material and intrinsic properties
› Measurement of the Full Shape of the Thermal Sunyaev-Zeldovich Power Spectrum from South Pole Telescope and {\it Herschel}-SPIRE Observations
› The canonical energy-momentum currents in cosmology
› Systematic biases in parameter estimation on LISA binaries. II. The effect of excluding higher harmonics for spin-aligned, high-mass binaries
› Tuning the violins: dark sector phase transition models for the PTA signal
› Optical Signatures of a Schwarzschild Black Hole in a Dehnen-Type Dark Matter Halo
› A Small Patch Hypothesis in Cosmology
› Three-Body Barrier Dynamics of Double-Alpha Decay in Heavy Nuclei
› Minimal Freeze-in Dark Matter: Reviving electroweak doublet dark matter with Boltzmann suppressed freeze-in
› Inflation with the Chern-Simons term in the Palatini formulation
› Dark Energy Survey Year 6 Results: Cell-based Coadds and Metadetection Weak Lensing Shape Catalogue
› GEMS JWST: Transmission spectroscopy of TOI-5205b reveals significant stellar contamination and a metal-poor atmosphere
› The temperature and metallicity distributions of the ICM: insights with TNG-Cluster for XRISM-like observations
› Circumgalactic medium of quasar host galaxies at 0.4
› Retrieving the hot circumgalactic medium physics from the X-ray radial profile from eROSITA with an IlustrisTNG-based forward model
› Probing Dark Matter Substructures with Free-Form Modelling: A Case Study of the `Jackpot' Strong Lens
› Kiloparsec-scale turbulence driven by reionization may grow intergalactic magnetic fields
› Time-Dependence of Subsurface Solar Convection Using the Time-Distance Deep-Focus Method
› $\texttt{SwiftC}_\ell$: fast differentiable angular power spectra beyond Limber
› The Multi-Wavelength Context of Delayed Radio Emission in TDEs: Evidence for Accretion-Driven Outflows
› Cosmic structure from the path integral of classical mechanics and its comparison to standard perturbation theory
› Probing small-scale primordial power spectra with induced gravitational waves
› If quasars form from primordial black holes
› Interpreting nebular emission lines in the high-redshift Universe
› Evolution of a Long-Lived Deep-Seated Main-Sequence Magnetic Field During White Dwarf Cooling
› The Atacama Cosmology Telescope: Release of A databaSe of millimeTeR ObservatioNs of Asteroids Using acT (ASTRONAUT)
› Precise Measurement of the Absolute Sky Brightness at 60 to 350 MHz
› YOLO-CIANNA: Galaxy detection with deep learning in radio data: II. Winning the SKA SDC2 using a generalized 3D-YOLO network
› ExoIris: fast exoplanet transmission spectroscopy in Python
› Non-explosive pre-supernova feedback in the COLIBRE model of galaxy formation
› Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters
› Detecting gravitational lensing by matter currents
› 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
› Witten-O'Raifeartaigh potential revisited in the context of Warm Inflation
› Hidden in Plain Sight II: Characterizing the luminous companion to Kappa Velorum with VLTI/GRAVITY
› The Binary Fraction of Stars in the Dwarf Galaxy Ursa Minor via Dark Energy Spectroscopic Instrument
› 2D or not 2D? Exploring 3D relativistic magnetic reconnection dynamics with highly accurate numerical simulations
› Magnetic field spreading from stellar and galactic dynamos into the exterior
› Space AI: Leveraging Artificial Intelligence for Space to Improve Life on Earth
› Towards an optimal extraction of cosmological parameters from galaxy cluster surveys using convolutional neural networks
› Long Period Transients (LPTs): a comprehensive review
› A multiwavelength ALMA view of gas and dust in binary protoplanetary system AS 205: Evidence of dust asymmetric distribution
› The Tarantula massive binary monitoring VII. The nature of the eccentric O+BH binary candidate VFTS 812
› Weak Lensing Low Multipoles
› Cosmographic parameters from current and next-generation gravitational wave detectors
› NovaMoon: A Strategic Lunar Reference Station for Positioning, Timing, and Largely Enhanced Science in the Earth-Moon System
› RedDots: Multiplanet system around M dwarf GJ 887 in the solar neighborhood
› Direct Detection of Dark Photon Dark Matter with the James Webb Space Telescope
› A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments
› The NHIM bifurcation scenario of a particle in an asymmetric binary system of dwarf galaxies
› Black Hole Ringdown Amplitudescopy
› Phantom cosmology with arbitrary potential: New accelerating scaling attractors
› Galactic magnetic fields seeded by ultralight dark photons

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