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Obserwatorium Astronomiczne na Suhorze

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Najnowsze prace na astro-ph:
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Searching for Life-As-We-Don't-Know-It: Mission-relevant Application of Assembly Theory for Exoplanet Life Detection ›
SpectralUnmix: A Torch-Based Regularized Non-negative Matrix Factorization ›
The ocean worlds science case for the Pollux spectropolarimeter ›
Martian concretion sizes predicted from two independently constrained inputs: atmospheric dust grain size and obliquity-forced wetting duration ›
Masses of Potentially Habitable Planets Characterized by the Habitable Worlds Observatory ›
AREPAS: A Resource for Exploring Protostellar Accretion Systems - Data Release I ›
Kinematic cosmic dipole from a large sample of strong lenses ›
Solar twins in Gaia DR3 GSP-Spec II. Age distribution and its implications for the Sun's migration ›
GSE vs. LMC: reshaping of radially biased stellar haloes by satellites ›
The TRGB-SBF Project. IV. A Color Calibration of the TRGB in the JWST F090W+F150W Filters ›
FlowSN: Normalising Flows for Simulation-Based Inference under Realistic Selection Effects applied to Supernova Cosmology ›
Isophote shape analysis and the unfortunate subtlety of dwarf galaxy structure ›
Gravitational Wave Measurement of the Mbh-Mbulge Intrinsic Scatter at High Redshift ›
Large-scale environments of star-forming active galactic nuclei: How black hole mass, accretion rate, and luminosity connect to dark matter halos ›
Long GRB 250916A: an Off-axis Powerlaw Jet with Thermal Cocoon ›
The Kinematically Hot, Extremely Metal-Poor C-19 Stellar Stream in DESI DR2 ›
Spontaneous Baryogenesis and Primordial Black Hole Dark Matter from Ultra-Slow-Roll Inflation ›
A systematic study of AGN feedback in a disk galaxy I: global overview ›
AGN obscuration in optical and X-rays: Host properties and the interplay of nuclear and galactic gas and dust in a combined SDSS-XMM sample ›
Imprints of Reheating Dynamics on Gravitational Waves from Phase Transitions ›
Not Where You Left Them: Displaced $\gamma$-Rays and X-Rays Reveal the Cosmic Ray Scattering Rate ›
Thermal Evolution of the Central Star in Pa 30 ›
Upgrading Alpha Crucis to a seven star system. Discovery of Bb and orbital misalignment ›
Cold giant discoveries from a joint radial-velocity and astrometry framework ›
Unveiling Massive Main-Sequence Stars in Sextans A through Panchromatic Photometry ›
Very long-term relaxation of harmonic 1D self-gravitating systems ›
Neutrino Spectral Pinching in 3D Core-Collapse Supernovae: Late-Time Convergence, Failed-Explosion Signatures, and Viewing-Angle Dispersion ›
Two Point Correlation Function Estimation with Contaminated Data ›
Post-processing Probabilistic Forecasts of the Solar Wind by Data Mining Similar Scenarios ›
PACHA: Probing AGN Coronae with High-redshift AGN ›
New Observations of the Strongly Magnetic O-star NGC 1624-2 Reveal Its Magnetic South Pole ›
Strong Prevalence of Hammerhead Velocity Distributions Close to the Heliospheric Current Sheet ›
Proto-NUX: A prototype telescope for ground-based near-ultraviolet observations ›
Balmer Decrements and Nebular-Stellar Reddening in JADES Galaxies at $2.7 ›
Galactic Stellar Halo Luminosity Function ›
An Orbit for a Massive Wolf-Rayet Binary in the LMC: An Example of Binary Evolution ›
Imploding Remnants: detection bias against AGNs in massive clusters ›
Gravitational Lensing Effects by Galaxy Clusters on Ionised Bubble Size Distribution during the Epoch of Reionisation ›
BLUEPRINT: Blue-dominant Lyman-alpha (Ly$\alpha$) emission as an evidence of gas inflow in ultra-low-mass galaxies at z = 3 ›
Marginally stable nuclear burning triggered at different depths of the neutron star surface in Low-mass X-ray binary 4U 1608-52 ›
Numerical Simulations of the Circularized Accretion Flow in Population III Star Tidal Disruption Events. II. Radiative Properties ›
Three-dimensional Global Relativistic Radiation Magnetohydrodynamics of Magnetically Arrested Disk Accretion Flows in AGNs ›
50-250 MHz Pulsar Census with an SKA-Low prototype station: Spectra and Polarization ›
Atmospheric Escape Rates from Mars - If it Orbited an Old M-Dwarf Star ›
JWST's PEARLS: A clumpy ring galaxy at $z = 4.0148$ ›
Warm Inflation Beyond the Markovian Limit ›
SN 2023axu: A Type IIP Supernova Interacted with a Low-Density Stellar Wind1 ›
Exploring the Viability of Fisher Discriminants in Galaxy Morphology Classification ›
Constraints on Axion-Photon Mixing from Fast Radio Burst Dispersion Measures ›
pyKurucz: A Pure Python Reimplementation of Kurucz SYNTHE for Stellar Spectrum Synthesis ›
A unified scalar-field resolution of the $H_0$, $S_8$ and evolving Dark Energy tensions ›
Revisiting early afterglows of gamma-ray bursts with finite-thickness ejecta: Implications from XRF 080330 and GRB 080710 ›
The Inner and Outer Shock Layers of Bow Shocks in Cataclysmic Variables ›
Merger-driven buildup of the $M_{\rm BH}$ - $M_*$ relation bridging high-$z$ overmassive black holes with the local relation ›
Reconstruction of Cepheid Radial Velocity Curves from the shape of the V-band Light Curves ›
Self-consistent-field method for triaxial differentiated bodies in hydrostatic equilibrium ›
Photometric and Spectral Evolution of the Symbiotic Nova HM Sagittae since 2003 ›
Origin of open clusters revealed by the evolution of the m_max$-$M_ecl relation ›
Equilibrium figure of Haumea and possible detection by stellar occultation ›
Continuum Reverberation in Bright Quasars Using NASA/ATLAS ›
Binary disruption during the early phase of open clusters ›
Chemo-dynamical reconstruction of Milky Way globular cluster progenitors: age--metallicity relations and the universality of multiple stellar populations ›
The impact of baryons on weak lensing statistics as a function of halo mass and radius ›
Energy dependence of the X-ray power spectrum in NGC4051 and NGC4395 ›
Cosmological gravity on all scales V: MCMC forecasts combining large scale structure and CMB lensing for binned phenomenological modified gravity ›
\HI 21-cm Line Properties of the Nearby LIRG IRAS 04296+2923 ›
Unveiling the biconical geometry of the outflow in the ultraluminous X-ray source NGC 5204 X-1 ›
AS-Bridge: A Bidirectional Generative Framework Bridging Next-Generation Astronomical Surveys ›
Identifying highly magnetized white dwarfs: A dimensionality reduction framework for estimating magnetic fields ›
The Cold Debris Disk Surveys I. Host Star Properties ›
The twin-jet system in the FRII radio galaxy 3C 452: A sub-parsec scale VLBI study ›
Sensitivity to Axion-like Particle dark matter with very-high-energy gamma-ray observations of Active Galactic Nuclei located behind Galaxy Clusters ›
A Cloudy Fit to the Atmosphere of WASP-107 b ›
Detection of a weak magnetic field in the Balmer emission line white dwarf WDJ1653-1001 ›
Chemical radial gradients for the bulge-bar stellar populations from the APOGEE survey ›
The shocking features in the closest rich galaxy cluster Norma ›
Comparison of Bar Formation Mechanisms. IIIA. The role of classical bulges in spontaneous bar formation ›
Rediscussion of eclipsing binaries. Paper XXIX. The F-type twin system BS Draconis ›
The Targeted Standard Siren Cosmology with Pulsar Timing Arrays ›
AstroSat-UVIT observations of a possibly interacting pair of galaxies in HCG 77 ›
Small-Scale and Transient EUV Kernels in Solar Flare Ribbons ›
GATOS N: The first direct kinematic evidence of dusty outflows from AGN via PAH kinematics of local Seyfert galaxies with JWST ›
X-ray evidence from NuSTAR for a Mach 3 shock in Merging Galaxy Cluster ZWCL 1856.8 ›
Comparing the $M_{gas}-N_{yso}$ Relation inside a Giant Molecular Cloud ›
Magnetoacoustic Shocks and Spectropolarimetric Signals in He I 10830 {\AA} ›
Scale-Dependent Loop Corrections to the Inflationary Power Spectrum ›
An Updated \synthpop Model for Microlensing Simulations I: Model Description, Evaluation, and Microlensing Event Rates Near the Galactic Center ›
Intrinsic Nonlocality of Spin- and Polarization-Resolved Probabilities in Strong-Field Quantum Electrodynamics ›
Rayleigh-Taylor Unstable Flames: Thin and Thick ›
Plasma effects on gravitational lensing and shadow observables of a Kerr-like black hole in a dark matter halo ›
Analytic Singular Slow-roll Inflation ›
Phase Retrieval using Nonlinear Curvature Sensing within Convergent Beams ›
Overdamping of Neutron-Mirror-Neutron Transitions in Neutron Stars ›
Assessing the robustness of amortized simulation-based inference to transient noise in gravitational-wave ringdowns ›
Shifted-geodesic approximation for spinning-body gravitational wave fluxes ›
Hawking Radiation from Tunneling in Black Hole Quantum Mechanics ›
Strong Evidence Against a Statistically Isotropic Universe ›
A search for super-imposed oscillations to the primordial power spectrum in Planck and SPT-3G 2018 data ›
Tidal deformability of black holes surrounded by thin accretion disks ›
Novel density profile for isothermal cores of dark matter halos ›
Quintessential Implications of the presence of AdS in the Dark Energy sector ›
Redshift Assessment Infrastructure Layers (RAIL): Rubin-era photometric redshift stress-testing and at-scale production ›
Curvaton in light of the ACT results ›
Stellar initial mass function in the 100-pc solar neighbourhood ›
Constraining the contribution of Seyfert galaxies to the diffuse neutrino flux in light of point source observations ›
Cosmic baryon census with fast radio bursts and gravitational waves ›
Finding strangelets in cosmic rays from HESS J1731-347, a possible strange quark star using the Cherenkov Telescope Array Observatory ›
Atmospheric Characterisation with the Twinkle Space Telescope Following Advances from JWST Observations ›
Constraints on Dark Matter Models from Supermassive Black Hole Evolution ›
Islands of Electromagnetic Tranquility in Our Galactic core and Little Red Dots that Shelter Molecules and Prebiotic Chemistry ›
Introducing SESHAT: A Tool for Object Classification from JWST Catalogs ›
Ultra-Faint Milky Way Satellites Discovered in Carina, Phoenix, and Telescopium with DELVE Data Release 3 ›
A constant upper luminosity limit of cool supergiant stars down to the extremely low metallicity of I Zw 18 ›
SN 2019vxm: A Shocking Coincidence between Fermi and TESS ›
A Smooth Transition from Giant Planets to Brown Dwarfs from the Radial Occurrence Distribution ›
Stellar Cores Live Long and Prosper in Cuspy Dark Matter Halos ›
The polar IL Leo in a low accretion state ›
High-energy Emission from Turbulent Electron-ion Coronae of Accreting Black Holes ›
Scalar-induced gravitational waves and primordial black holes from a localized bump or dip feature in a single-field inflationary potential ›
Time-variable Scattered Light in Herbig Disks Observed with Subaru/SCExAO ›
The Dawes Review 14: A Decade of Ultra-Diffuse Galaxies ›
The rotational and magnetic properties of Polaris from long-term spectropolarimetric monitoring ›
A candidate proton cyclotron feature in the ultraluminous X-ray source NGC 4656 ULX-1 ›
Spectral Decomposition Reveals Surface Processes on Europa ›
Translating current ALP photon coupling strength bounds to the Randall-Sundrum model ›
Freeze-In Dark Matter and Leptogenesis: a $\psi'$SM route ›
Dark Matter Clumps as Sources of Gravitational-Wave Glitches in LIGO/Virgo/KAGRA data ›
Multi-field TDiff theories: the mixed regime case ›
Testing Seesaw and Leptogenesis via Gravitational Waves: Majorana versus Dirac ›
Natural inflation in Palatini $F(R)$ ›
Superluminal constraints from ultra-high-energy neutrino events ›
Resonances in binary extreme mass ratio inspirals ›
The reason peculiar velocities grow faster in general relativity than in Newtonian gravity ›
Schwarzian Theory and Cosmological Constant Problem ›
Scaling Laws for Template-Free Detection of Environmental Phase Modulation in Gravitational-Wave Signals ›
Orbital Dynamics and Gravitational Wave Signatures of Extreme Mass Ratio Inspirals in Galactic Dark Matter Halos ›
On the Value of Tokeniser Pretraining in Physics Foundation Models ↓↑