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Obserwatorium Astronomiczne na Suhorze

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Najnowsze prace na astro-ph:
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Astronomical Advantages of a Boost Mission to Facilitate HST Science into the 2030s: Imaging the Circumgalactic Medium of Galaxies ›
Eigenvalue formulation of Stochastic Inflation and application to large perturbation generating inflationary features ›
Magnesium Silicate Clouds in the Atmosphere of HD 209458b from a Rule-Based Tree-Structured Data Reduction ›
Ultraviolet diversity of Little Red Dots as a probe for direct-collapse black hole ages ›
JWST Reveals Large Reservoirs of Dust and Ongoing Circumstellar Interaction in SN Ibn/Icn 2023xgo over a Year Post-Explosion ›
On the Faint Early-time Radio and X-ray Emissions in TDE2025aarm ›
Subarcsecond Multi-line Observations of NH$_3$ with VLA toward the Class 0 Source IRAS 16293-2422 ›
Far-infrared synchrotron properties of the inner lobes of the radio galaxy Centaurus A revealed with the Herschel observatory ›
Hubble Science in the 2030s White Paper: High-Contrast Optical and UV Spectroscopy with HST/STIS ›
Prospects of resolving and localising individual supermassive black hole binaries with pulsar timing arrays: the host ranking challenge ›
21cmEMUv3: a hybrid diffusion-LSTM emulator of 21cmFAST summary observables ›
It's Not Just Star Formation: A trend of low dark matter densities in the Andromeda dwarf galaxy system ›
Comparative properties of X-Ray Flashes and Gamma-Ray Bursts from BeppoSAX observations of Fast X-ray Transients ›
BBH-Genesis: Disentangling Binary Black Hole Formation Channels with GWTC-4 ›
The Delta Resonance in the Neutrino Sky ›
OCEANS of Absorption: High-resolution NIRSpec Spectroscopy Reveals Diverse Balmer-line Absorption in Little Red Dots ›
Constraining Extragalactic Proper Motion with Gaia Astrometry ›
Halo stars harbour few wide ultracool companions ›
Building a Global Astrotourism Community of Practice Through Astronomy for Development ›
Hard X-ray Sources in Fermi UFOs ›
Spectroscopic characterization of Young Stellar Populations and their Feedback in NGC 5253 ›
The sound of dynamical dark energy and modified gravity ›
Vision-Language Model Ensembles Achieve Human-Expert Accuracy for Galaxy Merger Classification ›
Narrowing the solar surface flux transport parameter space through nonlinear feedbacks ›
Jets and Superrotation in Deep and Shallow Planetary Atmospheres ›
Some Thoughts on the Future of Technosignature Searches: Constraining the Fermi Paradox ›
Non-linear Dynamical Stability of Magnetic Polytropes ›
Suppression of boosted relic neutrinos by photon backgrounds during ultra-high-energy cosmic ray propagation ›
Decaying Dark Matter as a Possible Solution for Cosmological Tensions ›
Interacting dark energy constraints from Fermi GRBs and Pantheon+ SNe Ia with full GRB covariance ›
Testing the cosmological principle with quasars ›
Calibrating Self-Weighted Shear Estimation via Field Distortion ›
Non-detection of HC(S)SH: Estimating Upper Limits and Constraining Chemistry ›
Prospects for Astrobiology and Technosignature Searches with the Vera C. Rubin Observatory Legacy Survey of Space and Time ›
The Mass, Orbit and Location of Planet Nine Derived from Classical Astrophysics ›
Ca-bearing cyanopolyynes in IRC+10216 ›
The Radio--X-ray Correlation of High-Redshift AGN: A Numerical Study of Inverse-Compton Scattering of the CMB Photons in Relativistic Jets ›
Bayesian estimation of spectral parameters of the 6.7-GHz methanol maser G339.884-1.259 from GRAO observations ›
The Pan-Pacific Planet Search -- IX. A menagerie of companions orbiting evolved stars ›
TeV gamma-ray spectral spikes produced by magnetic reconnection in blazar jets: the case of the 2014 high state of Markarian 501 ›
Generative Diffusion Priors for 3D Mapping of the Dark Universe ›
High-Synchrotron-Peaked BL Lacs as Multi-Messenger Sources: Connecting Ultra-High-Energy Cosmic Rays and Neutrinos ›
The cosmic ray ionization rate from H3+ observations can be overestimated due to neglect of time-dependent chemistry ›
Photochemical CS$_2$ Gas Detected on a 20-Myr-old Exoplanet ›
Understanding the Broad-line Region of Active Galactic Nuclei with Photoionization. II. Slim disks, Self-shadowing, and BLR sizes ›
Enhancing the Angular Resolution of Large Array of imaging atmospheric Cherenkov Telescope (LACT) at Ultra-High Energies ›
Hunting for Compact Object Binaries from eRASS1 Optical Counterparts through ZTF Time-domain Photometry and Multi-wavelength Census ›
Photon Escape from Slab Thomson Media: A Scattering-order-resolved Recursive Formalism for Comptonization Applications ›
The First Glimpse of Water Ice Absorption Map in the Milky Way ›
Deep Optical Follow-up Observations to IceCube Cosmic Neutrinos: a case for IC230724A with Subaru/HSC and prospects with Rubin/LSST ›
Is the Dark Comet 1998 KY$_{26}$ the Spacecraft Phobos 1? ›
PSF-like Alpha-Particle Events in LSST Images ›
Inside-Out vs. Outside-In Quenching of MaNGA Galaxies: Dependence on Stellar Mass and Environment ›
A short review on Quintom dark energy theory ›
Assessment of the Mass Loss and Radius Change of 3I/ATLAS Based on Observed Production Rates ›
Multiwavelength study of the Carina--Sagittarius Arm. I.Astrometric and photometric search for new open clusters in the 320$^ \circ $ $\le$ l $\le$ 325$^ \circ $ region ›
The Information Content of Quasar Variability Light Curves: How Well Can we Infer Stochastic Model Parameters? ›
Optimal Transport Reconstruction of Biased Tracers in Primordial Non-Gaussian Fields ›
JAXtronomy: A JAX port of lenstronomy ›
Morphology of Optical Changing-Look AGN-host Galaxies: Evidence for an Important Role of Mergers ›
Primordial black holes spin from cosmological first-order phase transitions ›
Study of Massive OBA Stars with X-ray Emission ›
Signatures of Accreting Black Holes in Line Intensity Mapping ›
Rapid quasi-periodic reconfiguration of the accretion column in pulsar 1A 0535+262 ›
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised ›
Magneto-Gravitational Regulated Streamer Accretion onto a Class 0 Protostellar System ›
Large ephemeral regions and their tilt angles ›
Design and development of Fabry-Perot based wavelength calibration system for PARAS-2 spectrograph ›
Reconnection-Driven Injection and Stochastic Reacceleration during Cosmological Magnetogenesis ›
A new Chandra look at the globular cluster NGC 6540 and its peculiar X-ray flaring source ›
A 0.03 Hz Radio Quasi-periodic Oscillation During the 2025 Flare of GRS 1915+105 ›
Possible High-Energy Neutrino Emission from Dark Matter Annihilation in the Disrupting Dwarf Galaxy Bo\"{o}tes~III ›
Fast radio bursts, magnetars and earthquakes: their "family feud"? ›
LAMOST J010103.13+275449.6: A New Binary with a Gradually Halving Photometric Variability Period ›
Mass and Spin Growth of Very Massive Stars in Star Clusters Potentially Associated with Little Red Dots ›
Distribution and Evolution of the Debris Cloud from the Fragmentation of Intelsat 33E ›
Visualizing the Magnetic Structure in Interplanetary Coronal Mass Ejections with ATHARV ›
CSST large-scale structure analysis pipeline: IV. Cosmic Voids Identified from Galaxy Group Samples as Probes of the Large-scale Structure ›
Accurate inner stellar density slopes from projected surface densities in galaxies ›
Radio Continuum Emission from Evolving Star-Forming Galaxies -- I. Correlations Involving the Total Synchrotron Luminosity ›
Polarized lines of the second solar spectrum (SrI, SrII, CaI, BaII) observed at the Pic du Midi Turret Dome spectropolarimeter with the slit orthogonal to the limb ›
Locating the Production Sites of High-Energy Neutrinos in Blazar Jets ›
A study of the Physical Properties and Star Formation Activity of a Large Sample of Molecular Clouds: I Distances ›
Revealing the high redshift host galaxy of the short GRB 061201 with JWST ›
Hierarchical assembly in action: a galaxy tail from a disrupting group in the Virgo cluster outskirts ›
Escape of Water- and Metal-enriched Atmospheres from compact Hot mini-Neptunes with CHAIN ›
Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference ›
AstroSkyFlow: an astronomical sky image flow simulator for time domain survey validation and machine learning ›
The magnetic field of the Milky Way: an observational perspective ›
Statistical properties of type-II bursts in Rapid Burster observed with Insight-HXMT ›
The light curve of T Cephei: humps, long-term changes and recent phenomena ›
The First Detection of Sub-Populations in the Delay-Time Distribution of Binary Black Holes in GWTC-4 of LIGO-Virgo-KAGRA ›
Solar vortex detection methods in MHD simulations: impact of magnetic field and spatial resolution ›
Revisiting ram pressure stripping in Wolf-Lundmark-Melotte: No evidence for stripped HI with LGLBS ›
Modeling the Thermal Low-Frequency Radio Sun with Ray Tracing ›
Regression on Regression: Mapping Data-Driven Binary Black Hole Merger Rate Fits to Progenitor Histories ›
Size limits on tidal debris around white dwarfs: the km-size barrier ›
Orbit Refinement of WASP-18 b and Evidence Against the Existence of WASP-18 c ›
Evaluating Cepheid Metallicity Effect Determinations via IC1613 and Gaia-independent Parallaxes ›
On the Relationship between Solar Spicules and Propagating Coronal Disturbances: The Role of Shocks ›
JWST's Little Red Dots as collapsed Supermassive Dark Stars ›
Mergers Matter: Gravothermal Collapse in Dwarf Halos with Self-Interacting Dark Matter ›
Searching for a waveform-agnostic gravitational wave signal in pulsar timing arrays ›
Linear causality and stability constraints on relativistic second-order magnetohydrodynamics ›
Coupled nuclear and leptonic longitudinal collective modes in neutron star matter : a covariant Vlasov approach ›
A quarkyonic matter model ›
Self-gravitating quantum stars with a globally relevant Bohm potential ›
The Heuristic Approach to General Relativity in the Laplace-Beltrami Formalism ›
Improving the resolution of double white dwarf systems with spaceborne gravitational wave observatories using a robust astrophysical prior ›
He-CF4-CH4 ternary mixtures as target gas for the CYGNO directional dark matter experiment ›
Gravitational-wave astronomy with a space-based optical clock network ›
Pitching Cosmic Curveballs: Environmental Effects on Extreme-Mass-Ratio Inspirals with Spinning Secondaries ›
Ellis-Bronnikov Wormhole Shadows with Spherically Symmetric Accretion Flow ›
Tachyonic particle production: quantum 2PI formalism with momentum exchanging collisions ›
COSMOS: A numerical relativity code specialized for PBH formation ›
Counterintuitive Magnetic Connectivity and Energetic Particle Flux Differences among Nearby Spacecraft During the 2023 February 24 Solar Energetic Particle Event ›
Dyonic Quark Stars in Quasi-Topological Electromagnetism ›
On the Role of Chapman's Hydrostatic Solar Wind Mechanism in Parker's Hydrodynamic Solar Wind Model ›
Cosmology with the angular cross-correlation of gravitational-wave and galaxy catalogs: forecasts for next-generation interferometers and the Euclid survey ›
Low-Metallicity Star Formation Survey in Sh2-284 (LZ-STAR). II. The inital mass function ›
From Voids to Clusters: Mergers and Evolutionary Pathways of Star-Forming and Quenched Low-Mass Galaxies ›
Testing Cosmic Distance Duality Relation and Transparency with DESI DR2 ›
Reconstructing Barrow Holographic Dark Energy in $f(Q,T)$ Gravity and Cosmic Constraint ›
Analytical transit light curves for arbitrary power-law limb darkening: a unified framework ›
Modelling $\delta$ Scuti pulsations: A new grid of p, g, and f modes across pre-main-sequence to post-main-sequence evolution ›
Exploring Cosmic Dawn with PANORAMIC I: The Bright End of the UVLF at $z\sim9 -17$ ›
The Atacama Cosmology Telescope: Release of A databaSe of millimeTeR ObservatioNs of Asteroids Using acT (ASTRONAUT) ›
The Nature of Post-Starburst Galaxies: Real Deal or Masquerading Impostors? ›
Holographic dark energy in a coasting cosmology ›
BlackTHUNDER: Evidence of three massive black holes in a z~5 galaxy ›
halox: Dark matter halo properties and large-scale structure calculations using JAX ›
3D B-fieLds in the InterStellar medium and Star-forming regions (3D-BLISS): I. Using Starlight Polarization in the Massive IRDC Filament G11.11-0.12 ›
Confirming the uniformity of the Hubble flow with Pantheon+ Supernovae ›
Accelerated inference of microlensed gravitational waves with machine learning ›
The role of the galaxy stellar mass function in determining the cosmological distribution of astrophysical transients with applications to fast radio bursts and merging binary black holes ›
Self-lensing of moving gravitational-wave sources can break the microlensing crossing timescale degeneracy ›
Resolving the (Debate About) Nozzle Shocks in Tidal Disruption Events ›
Observational constraints on 3-forms dark energy ›
Inference of Neutron Star Mass Distributions and the Dense Matter Equation of State from Multi-messenger Observations ›
Reconnection-Driven Turbulent Fluctuations in the Magnetically Dominated Collisionless Regime ›
Are Primordial Black Holes Truly Fine-Tuned? ›
The Progenitor of the Type II-Plateau SN 2025pht in NGC 1637: The Dustiest, Most Luminous Red Supergiant So Far? ›
Semi-analytical approach to Ly$\alpha$ multiple-scattering in 21-cm signal simulations ›
Realizing the phantom-divide crossing with vector and scalar fields ›
Gamma-Ray Bursts: Evidence for a Common Origin of X-ray Plateaus with Diverse Temporal Decay Index ›
Radiation-hydrodynamics of star-disc collisions for quasi-periodic eruptions ›
Tidal triggers and the predictability of solar activity ›
New Dynamical Measurements from a Lensed Quasar Sample: Joint Analysis Constrains the Mass Profile Evolution of Lens Galaxies ›
The impact of the formation channel on gravitational-wave-galaxy cross-correlations ›
Transient X-ray Sources as Extremely Eccentric Mass-Transfer Binaries with Compact Companions ›
Probing inflationary features with galaxy ultraviolet luminosity function observables ›
LCEz4-M1: A Lyman Continuum Emitter Candidate at z = 4.444 in the MUSE Hubble Ultra Deep Field ›
Radiation GRMHD Models of Accretion onto Stellar-Mass Black Holes: III. Near-Eddington Accretion ›
New black hole mass calibrations and the fundamental plane of the broad-line region size, luminosity, and velocity ›
Worlds Next Door. IV. Mapping the Late Stages of Giant Planet Evolution with a Precise Dynamical Mass and Luminosity for $\epsilon$ Ind Ab ›
Spectroscopic galaxy redshifts in the Peanut cluster - a massive nearly head-on cluster merger shortly after pericenter passage ›
A Panchromatic JWST Spectrum of a Giant Starspot on the Fully Convective M-dwarf TOI-3884 ›
The Sunrise Chromospheric Infrared Spectro-Polarimeter SCIP: an instrument for SUNRISE III ›
Resizing the giants: How modelling adiabatic interiors impacts predicted planetary radii ›
Revisiting Marked Galaxy Clustering from a Joint Point Process Perspective ›
Shortest period for outer orbit in compact hierarchical triple? Discovery of SB1 around V0885 Per ›
Radial evolution of Alfv\'en wave Parametric Decay Instability in the near-Sun solar wind: Effects of Temperature Anisotropy ›
The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk ›
Measurement of the Weyl Potential Evolution and $E_G$ Statistic from KiDS-1000, BOSS and 2dFLenS ›
uGMRT and MeerKAT observation of RXCJ0232-4420: a quiet cluster with a giant radio halo ›
Mean tropical year length at arbitrary ecliptic longitude ›
The jet-shaped pipe morphology in planetary nebulae and core-collapse supernova remnants ›
Observational Signatures and Constraints on the Intermediate Neutron-Capture Process. The Case of the CEMP star TYC 6044-714-1 (RAVE J094921.8-161722) ›
UNIONS-3500 Weak Lensing: IV. 2D cosmological constraints in harmonic space ›
Beyond AI as Assistants: Toward Autonomous Discovery in Cosmology ›
Photometric classification of quasars from DES and photo-$z$ estimation with Machine Learning ›
Blue-tilted Runnings and the JWST Early Galaxy Tension ›
Gravitational Waves from Post-Inflationary Magnetism: Direct and Scalar-Induced Contributions ›
Cosmic Ray Feedback in Galactic Disks: Star Formation, Cosmic Ray Transport, and Multiphase Outflows in TIGRESS++ Simulations ›
Probabilistic Data-Driven Modelling of Astrophysical Transients: The Neural Process Family for Ultrafast and Class-Agnostic Light Curve Reconstruction with NightLANP ›
Ejected Surface Regolith as a Potential Source Material for Centaur Rings ›
Harmonics as a Hidden Window into the Turbulent Convective Envelope of non-Blazhko RRab Stars ›
Updated Constraints on Omnipotent Dark Energy: A Comprehensive Analysis with CMB and BAO Data ›
Gravitational Bound State Perturbations Inside Black Holes and Isospectrality ›
An Enhanced "Flux-Corrected Transport"-Based Plasmasphere Refilling Model ›
Loop-Level Lepton Flavor Violation and Diphoton Signals in the Minimal Left-Right Symmetric Model ›
Non-minimally coupled loop quantum inflation with inverse-volume corrections ›
Non-local gravity effects in cosmological dynamics probed by IceCube/KM3NeT signals and dark matter relic abundance ›
Massive hybrid stars within the extended three-flavor quark-meson diquark model ↓↑