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Obserwatorium Astronomiczne na Suhorze

Teleskop

Kamerka S

Kamerka N

Niebo
Temperatura
5.4 °C
Wilgotność
57%
Wiatr
0.0 km/h
Ciśnienie
1016.3 hPa

Księżyc
Najnowsze prace na astro-ph:
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Bypassed Core Formation in Milky Way-Mass SIDM Halos: Implications for the Local Group Past-Pericenter Scenario ›
High-dimensional inference for the $\gamma$-ray sky with differentiable programming ›
Primordial Neutron Stars ›
Temperature asymmetry in the Milky Way's hot circumgalactic medium induced by the Magellanic Clouds ›
Choice of optical transformation for photonic circuit wavefront sensors ›
The Hubble sequence in JWST CEERS from unbiased galaxy morphologies ›
Ghosts of eruptions past: Searching for historical Galactic supernovae using variable thermal dust echoes and machine learning ›
GLIMPSED: Direct evidence for a fast AGN-driven outflow from a z=6.64 Little Red Dot host galaxy ›
Positive YORP effect induced by lateral heat conduction in a crater ›
Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing Strategies ›
EPISODE IV: Ice Inventory in the Envelope of EC 53 ›
Colloquium: Radio astronomy with the Arecibo 305-m telescope: In contemporaneous context ›
Development of the New Optical Sensor for IceCube-Gen2 ›
The Fate of Frozen Carbonated Water at Europa-like Conditions ›
A practical re-weighting scheme of data fitting: application to asteroids orbit determination with Gaia ›
Overview of Hayabusa2 extended mission's flyby of Near-Earth Asteroid (98943) Torifune ›
Validating a Non-conventional Method for Expansion of Coronal Mass Ejections (CMEs) and Investigating the Evolution of a CME Substructures Using Solar Orbiter and Wind Observations ›
cTreeBalls: a fast 3-point correlation function code for clustering measurements ›
FolpsD: combining EFT and phenomenological approaches for joint power spectrum and bispectrum analyses ›
What Heats the Dense Gas in the Galactic Center? ›
A Convolutional Neural Network-Derived Catalog of Solar Flares from Soft X-Ray Observations ›
Polarimetry in Planetary Sciences and Astronomy ›
Spectral signatures from the habitable zone ›
Recent advances in modelling of global-scale collisions using smoothed particle hydrodynamics ›
Photoionization modelling of circumstellar nebulae using irregular grains ›
The formation of planetary systems: physics, populations, and architectures ›
Recent development in high-precision high-fidelity spectrographs for exoplanet research and characterization ›
Giant Planet Formation by Disk Instability ›
Beyond Mass and Multiscale Environments: What Shapes Low Surface Brightness Galaxies? Evidence from MaNGA ›
The Northern High Time Resolution Universe pulsar survey: III. Single-pulse search continuation, follow-up observations, and initial results ›
Optical identification of the FASHI sources: toward the extended Local Volume ›
Radio Monitoring Campaign of Active Repeater FRB 20220912A with CHIME ›
Dust Processing in Protoplanetary Discs From Infall to Dispersal: the Origin of Solar System Isotopic Heterogeneities ›
A New Measurement of the Extragalactic Background Light using 15\,yr of {\it Fermi}-Large Area Telescope Data ›
Bounding axion dark energy ›
The Cosmic Web and Its Filaments: Neutrino Mass from Topology and Persistent Homology ›
Machine Learning as a Transformative Tool for (Exo-)Planetary Science ›
Joining forces: 30 years optical monitoring of the Einstein Cross ›
The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$ ›
Fast and Scalable Production of Stacked Prism X-ray Lenses for Astrophysics Using Two-Photon Polymerization ›
Terrestrial planet formation in the era of GPU computing ›
Tracing the s-Process: Spectroscopic Insights into Chemical Abundances in O- and C-rich Evolved Stars ›
An automated method for planetary nebula detection with SIGNALS: first applications to NGC 4214 and NGC 4449 ›
The evolution of the mid-infrared spectrum of SN 1987A observed with the JWST/MIRI-MRS ›
Methanimine as a sink in the HCN and HNC solid state hydrogenation network ›
Unseen Astronomy ›
Long-period transiting exoplanets: advances in detection and characterization ›
The Illusory Precision of TTV Masses: Hidden Solutions Behind Kepler-9's Tight Mass Ratio ›
Detecting nitrogen-carriers in the inner regions of protoplanetary disks ›
A first [CII] view of high-z quiescent galaxies ›
Constraining the Molecular Kennicutt-Schmidt Relation with Multi-Transition CO Observations of Nearby Galaxies ›
Nii-body: Bayesian Inference of Multiplanet Dynamics via N-body Simulations ›
NCCR PlanetS: Observational and computational characterization of exoplanet atmospheres ›
A TeV-based Determination of the Local Extragalactic Background Light and its Consistency with Galaxy Counts and Direct Measurements ›
Paschen Jumps in Little Red Dots: Evidence for Nebular Continua ›
Enhancing event reconstruction for $\gamma$-ray particle detector arrays using transformers ›
Analytic compression of the effective field theory of the Lyman-alpha forest ›
Large or bright satellite constellations: Effects on observations, including on the background sky brightness ›
Blueshifted lines from the inner accretion disc's rotation can explain quasar absorption "forests'' ›
Finding Circumbinary Planets: A Semi-Automated Transit Search of TESS Eclipsing Binaries ›
IFS spectrograph designs for the Wide-field Spectroscopic Telescope: Architecture and performance gains from curved sensors ›
The k-MENDEL sample of local analogs to reionization galaxies. Spectral identification of EELGs and properties of green peas in DESI ›
Gardening on the Moon: An Advection-Diffusion Model to Guide the Search for Supernova Debris in the Lunar Regolith ›
High-Contrast Imaging of Forming Protoplanets: VLTs, JWST, and the Promise of ELT ›
The missing ultra-faint satellites of the Milky Way ›
Inverse Energy Cascade in Turbulent Taylor-Couette Flows ›
Resolving satellite-in situ mismatches in Net Primary Production using high-frequency in situ bio-optical observations in the subpolar Northwest Atlantic ›
Love numbers of black holes and compact objects ›
Minimum mass, maximum charge and hyperbolicity in scalar Gauss-Bonnet gravity ›
Tidal Response of Compact Objects ›
Evaluating Deep Learning Models for Multiclass Classification of LIGO Gravitational-Wave Glitches ›
labrador: A domain-optimized machine-learning tool for gravitational wave inference ›
Genericness of quantum damping of cosmological shear in modified loop quantum cosmology ›
Probing the Kinematic Dipole with LISA: an analytical treatment ›
Relative Magnification Factor of Point Sources on Accretion Disks ›
Covariant scalar-tensor theories beyond second derivatives ›
Short-Time Plasma Evolution: Flow Generation and Magnetogenesis ›
Probing Solar Symmetrons with Direct Detection ›
CMB signatures of gravity-mediated dark radiation in $\mathbf{\Delta N_{\rm eff}}$ ›
Classification of Symmetric Four-Body Dziobek Central Configurations and Application to the Earth--Moon System ›
BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$ ›
Revealing Flare Energetics and Dynamics with SDO EVE Solar Extreme Ultraviolet Spectral Irradiance Observations ›
Build-up and survival of the disc: From numerical models of galaxy formation to the Milky Way ›
Beyond Spherical geometry: Unraveling complex features of objects orbiting around stars from its transit light curve using deep learning ›
Leveraging Photometry for Deconfusion of Directly Imaged Multi-Planet Systems ›
BayeSN-TD: Time Delay and $H_0$ Estimation for Lensed SN H0pe ›
Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM ›
Dark winds on the horizon: Prospects for detecting neutrino and hot dark matter wakes in large-scale structure ›
statmorph-lsst: Quantifying and correcting morphological biases in galaxy surveys ›
Aql X-1 from dawn 'til dusk: the early rise, fast state transition and decay of its 2024 outburst ›
A window for water-hydrogen demixing on warm metal-rich sub-Neptunes ›
Non-thermal Synchrotron Emission and Polarization Signatures during Black Hole Flux Eruptions ›
High-energy Neutrino Predictions for T Coronae Borealis: Probing Particle Acceleration in Novae ›
Validation of Satellite Lifetime Predictions at Leonid Space ›
The Volatile Inventory of 3I/ATLAS as seen with JWST/MIRI ›
Little Red Dots on FIRE: The Ability of Bursty Galaxies to Host an Abundant Population of High-Redshift AGN ›
Sunrise III: The Wavefront Correction System ›
A method to derive self-consistent NLTE astrophysical parameters for 4 million high-resolution 4MOST stellar spectra in half a day with invertible neural networks ›
The Baryon Budget of Galaxies across the First Billion Years ›
SPACE-Timers -- A Stack-Based Hierarchical Timing System for C++ ›
Formation of mega-parsec giant radio sources from hosts residing in dark matter halos with normal hot baryonic gas fractions ›
An Updated SynthPop Model for Microlensing Simulations I: Model Description & Evaluation ›
Magnetic Connectivity in the Time-Dependent Corona and Heliosphere ›
The role of inner disk edges in shaping ultra-short-period planet systems around late M dwarfs ›
Euclid preparation. Galaxy power spectrum and bispectrum modelling ›
What Are Pulsar Companions Made of? Using Gravitational Tides to Probe Their Compositions ›
Spectroscopic Redshifts for 461 Euclid Q1 Strong Gravitational Lenses from NISP Slitless Spectroscopy ›
Numerical simulations of density perturbation and gravitational wave production from cosmological first-order phase transition ›
PRECESSION 2.1: black-hole binary spin precession on eccentric orbits ›
Inflation in theories with broken diffeomorphisms ›
Characterization of compressible fluctuations in solar wind streams dominated by balanced and imbalanced turbulence: Parker Solar Probe, Solar Orbiter and Wind observations ↓↑