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Obserwatorium Astronomiczne na Suhorze

Widok nad kopułą w nocy

Kamerka S

Kamerka N

Niebo
Temperatura
18.7 °C
Wilgotność
63%
Wiatr
1.6 km/h
Ciśnienie
1014.8 hPa

Księżyc
Najnowsze prace na astro-ph:
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Mars, a Post-Habitable Planet? ›
The role of the Hubble Space Telescope in advancing our understanding of atmospheric escape in exoplanets ›
From Hubble to HWO: Bridging the Frontier of White Dwarf Exoplanet Science ›
Exploring Space Weather From Young Solar-like Stars as Windows to Exoplanetary Habitability ›
White dwarf planetary systems in the ultraviolet ›
Bimodality in Rotational Modulation of Planet-Hosting Stars ›
A framework for modelling Population III stars in cosmological simulations ›
How galaxies acquire their stellar mass at high redshift: High star formation efficiencies and the relative roles of dust and initial mass function ›
Field-level multi-tracers simulation-based inference of cosmological parameters from 3D maps ›
NISER-IUCAA New Simulations of JWST GAlaxies and Quasars(NINJA): Properties of galaxies at $5 \leq z \leq 10$ ›
The Persistent Missing Mass Problem in Planet Formation ›
Dynamical Stability and Habitability in the HD 20794 System ›
Strong Constraints on Millisecond Pulsar Injection Spectra from Fermi-LAT Observations of the Galactic Center ›
Limited imprint of high-mass IMF variations on sodium abundances in main-sequence galaxies ›
Bar-halo interaction: the role of orbital anisotropy ›
Constraining Scattering Medium Geometry with Cyclic Spectroscopy ›
Cosmic Ray Feedback in Galactic Disks: Star Formation, Cosmic Ray Transport, and Multiphase Outflows in \tigresspp\ Simulations ›
NuSTAR as an Axion Helioscope: probing axion-nucleon and axion-electron couplings ›
Nuclear Physics of Binary Neutron Star Mergers ›
A distributed resource-adaptive implementation of the widefield radio-interferometric measurement model for scalable image formation ›
The Role of Whistler and Ion Cyclotron Waves in Particle Escape from Mirror Modes in the Intracluster Medium ›
Inversion of CHASE H$\alpha$ Spectral Line during Solar Flares Based on RADYN Dataset via Deep Learning ›
An SMA Molecular Inventory of the Edge-on Protoplanetary Disk Gomez's Hamburger ›
Unveiling the dark matter nature with reionization relics ›
Constraining the Supernova Remnant Environment of FRB 190520B with Dispersion Measure and Scattering Timescale ›
A Modified Multi-Level Tracking Scheme for the Detection of Sunspot Umbral Dots ›
The DECam MAGIC Survey $-$ Mapping the Ancient Galaxy in CaHK: Overview and Summary of Early Science ›
OH/IR stars in the inner Galactic bulge: I. Colour, CO line, and stellar light curve characteristics ›
Spectra and Ionization Efficiencies of Charged Decay Particles in Kilonova Ejecta ›
Detection of the distant quasar OP 313 with the first Large-Sized Telescope of CTAO ›
From supernovae to neutron stars: crust formation time ›
Interior-Atmosphere Coupling on TRAPPIST-1 f, g, and h: Cryovolcanic Water Exospheres and Infrared Detectability ›
Invariant manifolds in barred galaxy simulations. II. Quantitative evidence of manifold-trapping in spiral arm formation ›
Evidence for Systematically Larger Dust Grains in Upper Scorpius Relative to Taurus Disks ›
Granulation signatures as seen by Kepler short-cadence data. II. A hierarchical route to inferring stellar radii from granulation ›
Constraining Early Dark Energy cosmological models with Big Bang Nucleosynthesis ›
From streamers to stars: overcoming mass loss in protoplanetary disks ›
The spectral energy distribution of YSES 1 b and its circumplanetary disc ›
Magnetic field Topology and Star Formation in the Cepheus B Filamentary cloud under External Feedback ›
Survival of very small carbonaceous dust grains in the inner-CGM of NGC 891 from JWST/MIRI MRS ›
Future Detections of the Warm-Hot Intergalactic Medium using Bright Power Law Sources with NewAthena ›
The Baryonic Faber-Jackson Relation and Fundamental Plane of Galaxy Groups, Elliptical Galaxies, and Dwarf Galaxies ›
Veiling of Photosphere Lines in the Spectra of UX ORI Stars at Deep Light Minima. I. The Star RR Tau ›
The small transiting planet population revealed by ESPRESSO with extreme precision radial velocities ›
The Physical Nature of Regolith on Icy Moons ›
The Simons Observatory: Rotation Performance of Cryogenic Half-Wave Plate Polarization Modulators ›
Analysis of Short-term Solar Activity Variability and Estimating the Timings of the Next Enhanced Bursts ›
Destructuring the disk of AB Aurigae: Dynamics and accretion ›
Cosmological Constraints from Bias-Robust Wavelet Scattering Statistics for Stage-IV Galaxy Surveys ›
Observations of stable pickup He$^+$ tori in a magnetic flux rope at 0.85 au ›
Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra-I cluster. VI. A star-forming UDG in Hydra I: a rare UDG or a transition phase? ›
Nearby galaxies in the LOFAR Two-metre Sky Survey IV. A fundamental plane of the radio-SFR relation ›
The pollution from massive AGB stars favoured by strong hot bottom burning ›
Regular black hole solutions and the quark chemical potential at the QCD phase transition ›
Digging into the Massive Protostar S255IR NIRS3: A Study of Nitrogen-Bearing Molecules and Their Prebiotic Chemistry ›
For modified gravity, it's the LITTLE THINGS that matter ›
Constraints on Dynamical Dark Energy from Multiple Probes in the Full Dark Energy Survey ›
GWTC-5.0: Population Properties of Merging Compact Binaries ›
GWTC-5.0: Constraints on the Cosmic Expansion Rate and Modified Gravitational-wave Propagation ›
$w_0$-probe: A new diagnostic of dark energy based on $Om$ ›
A Fast Method to Compute Scalar Induced Gravitational Waves on a Lattice with Primordial Non-Gaussianities ›
The SPHERE infrared survey for exoplanets (SHINE) V. Full sample characterization ›
Temperature-resolved sensitivities of $^{56}{\rm Ni}$ production to helium-burning reactions in pair-instability supernovae ›
Heavy element enrichment of gas in surface-accretion disks: A possible origin of the mass-metallicity anti-correlation in exoplanets ›
The Neptunian ridge planet WASP-156 b does not have a polar orbit ›
Effective Phantom Dark Energy: What Cosmological Reconstruction Does and Does Not Imply ›
Supermassive Black Holes: modelling strongly and weakly magnetised misaligned accretion disks ›
Impact of Clouds on the Atmosphere-Mantle Interface of Sub-Neptunes ›
Gaussian Process Reconstruction of Cosmological Parameters with Gravitational Wave Sirens using Machine Learning ›
Hot Jupiters' Isolation Is Not Unique to High-Eccentricity Tidal Migration ›
The first near-infrared high-resolution \'echelle spectroscopy of the outflow in NGC 4151. A study of the clouds covering the Eye of Sauron ›
A Minute-Cadence Deep Bulge Survey: First Data Release of DREAMS ›
First Light and Reionization Epoch Simulations (FLARES) XXII: UV-dust spatial offsets at the Epoch of Reionisation ›
Inflatable devices for planetary aerocapture and aerobraking manoeuvres ›
Electromagnetic Signatures From Primordial Black Holes in the Solar System ›
Charging Across the Phantom Divide with Modified Gravity ›
Energy extraction from NED-deformed rotating black holes via the Comisso-Asenjo reconnection process ›
Improved Big Bang Nucleosynthesis constraints on decaying massive relics ›
Looking for Condensed Gluons: A Cross-Scale Journey from the Deep Structure of Protons to High-Energy Cosmic Rays -- A Mini-Review ›
Open Data from LIGO, Virgo, and KAGRA through the Second Part of the Fourth Observing Run ›
Hybrid Expansion Cosmology in f(T) Gravity: Late-Time Evolution and Observational Bounds ›
GWTC-5.0: An Introduction to Version 5.0 of the Gravitational-Wave Transient Catalog ›
GWTC-5.0: Methods for Identifying and Characterizing Gravitational-wave Transients ›
GWTC-5.0: Observations from the Second Part of the Fourth LIGO-Virgo-KAGRA Observing Run and Updates to the Gravitational-Wave Transient Catalog ›
Strong-lensing degeneracies of black holes embedded in self-interacting scalar field dark matter halos ›
HAMSTER: Hyperspectral Albedo Maps dataset with high Spatial and TEmporal Resolution ›
Exploring Galactic open clusters with Gaia. II Dynamical Evolution and Stellar Population Properties in Fifteen Nearby Open Clusters ›
Exploring effects of IMF sampling and SN feedback injection on star formation and metallicity in ultra-faint dwarf galaxies ›
Co-evolution of cosmic ray energy spectra, composition, and anisotropies ›
Relativistic accretion and burdened primordial black holes ›
Echoes in Different Tempo: Long-Term Monitoring of Crab Echoes with CHIME ›
A Melody in the Noise: Modeling Echoes of the Crab Nebula ›
X-ray polarization of reflected thermal emission ›
Properties of cluster red-sequence spiral galaxies ›
Deciphering the explosion mechanism of Type Ia SNe using their remnants II: a deep dive into double detonations with SNR 0509-67.5 ›
TOI-2155 b: A Massive Brown Dwarf or a Very Low-Mass Star? ›
ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution ›
On the consistency of jet feedback modelling across different astrophysics hydrodynamical codes ›
Multi Messenger Study of GRB 221009A with VHE Gamma-ray and Neutrino Afterglow from a Gaussian Structured Jet ›
Simulation Study of Binary Mergers of Galaxy Clusters I: Properties of Merger Shocks and Radio Emission ›
Episodic planetesimal disruptions triggered by dissipation of gas disk ›
ODIN: Clustering Properties of Ly$\alpha$ Blobs at $z$ $\sim$ 2.4 and 3.1 ›
Democratic heliocentric coordinates underestimate the rate of instabilities in long-term integrations of the Solar System ›
The Role of Inner Halo Angular Momentum (Spin) in Shaping Dark Matter Bars in Milky Way Analogs ›
LISA and the LISA Science Team ›
On the rotation of M-type asteroids: statistical evidence for higher rotation rates ›
Direct simulations of H-He mixtures at planetary interior conditions: demixing, insulator-metal transition and miscibility boundaries ›
Implications of the nanoHertz Gravitational-Wave Background for Galactic Feedback and Massive Black Hole Growth ›
IGR J12580+0134: A Possible Repeated Partial Tidal Disruption Event Inferred from Late-Time Radio Re-brightenin ›
You can't see me: Super-Eddington growth hindering X-ray detection in high-z broad-line active galactic nuclei ›
Multimessenger Characterization of High-Energy Neutrino Emission from the Brightest Neutrino-Active Galactic Nuclei ›
Inflation with the Gauss-Bonnet term in the Palatini formulation ›
Smoothed Particle Hydrodynamics in pkdgrav3 for Shock Physics Simulations. II. Shear Strength ›
Dynamical Systems in Cosmology: Reviewing An Alternative Approach ›
Exploring the interplay of late-time dynamical dark energy and new physics before recombination ›
The velocity dispersion function of red galaxies in four Hubble Frontier Fields galaxy clusters ›
Emergence of Complex Web Structures ›
Breaking Free from the Swampland of Impossible Universes through the DESI Portal ›
Velocity-resolved [O I] 63,145 um, [C II] 158 um, and OH mapping along the Orion BN/KL explosive outflow and irradiated shocks ›
Spectra as Language: Large Language Models for Scalable Stellar Parameter and Abundance Inference ›
Rotation-curve residuals reveal a suppressed acceleration branch in dwarf galaxies ›
Performance analysis of extragalactic classifications in Gaia Data Release 4 ›
Nature of HD 251108: an RS CVn binary with a long-term evolving spot ›
HiFAST: An HI data calibration and imaging pipeline for the FAST IV: The stray-radiation correction ›
The Evolution of Cataclysmic Variables Under Various Magnetic Braking Prescriptions ›
Reassessing high-energy emission correlations in gamma-ray bursts using a large, homogeneous sample of X-ray afterglows ›
Core-collapse supernovae and supernova neutrinos ›
Comparing a Compact-Binary Mass-Shell Model with Select Observed Gravitational Waves ›
Examining the influence of anisotropy on the fundamental mode of nonradial oscillation in neutron stars on a complete general relativistic scheme ›
Ultralight Dark Matter from the Edge of Field Space ›
Semi-convection in rotating spherical shells: flows, layers and dynamos ›
Universal relation between dipole polarizability of finite nuclei and neutron-star compactness ›
AI-based separation of turbulence from coherent background flows in decaying hydrodynamic turbulence ›
Numerical simulations of primordial black hole formation via delayed first-order phase transitions ›
High-power Test and System Integration of Direct RF Sampling Based LLRF Control and Monitoring System for S-Band Accelerating Structures ›
Dynamics of Binary System around a Supermassive Black Hole :Binary Scattering and Eccentric vZLK Oscillations ›
Quantification of atmospheric carbon dioxide from the Geostationary Operational Environmental Satellite (GOES East) ›
Aurora Hunter: A Two-Stage Framework for Probabilistic Visibility Forecasting ↓↑