ul. Podchorążych 2, 30-084 Kraków.
tel.: (+48 12) 662 6301;
fax: (+48 12) 637 2243;
Obs. tel.: (+48) 502 113714
Obserwatorium Astronomiczne na Suhorze

Zachód Słońca

Chmury

Opady

Niebo
Temperatura
-2.3 °C
Wilgotność
93%
Wiatr
0.0 km/h
Ciśnienie
1014.4 hPa

Księżyc
Najnowsze prace na astro-ph:
›
Global detector network to search for high-frequency gravitational waves (GravNet): conceptual design ›
Neutrino and electromagnetic signatures from Superluminous Supernovae: a case study for SN 2017egm ›
BLAZ4R and the eROSITA view of z>4 blazars ›
Clouds with a silicate lining: Using JWST spectra to probe atmospheric diversity in young AB Dor L dwarfs ›
Disentangling auroral, cloud and magnetic spot driven variability in three early L-dwarfs with HST/WFC3 ›
A Probabilistic Autoencoder for Galaxy SED Reconstruction and Redshift Estimation: Application to Mock SPHEREx Spectrophotometry ›
Systematic Monitoring of Extreme X-ray Variability from Weak-line Quasars ›
A Fast, Hot Wind from a Nuclear Starburst ›
Beyond the Largest Lyapunov Exponent: Entropy-Based Diagnostics of Chaos in Henon-Heiles and N-Body Dynamics ›
The background gas humming and multi-messenger transients of stalled supermassive black hole binaries ›
GJ 523b is a Massive, 170 Myr-old Mega-Earth, Likely on a Polar Orbit ›
The rise of the black hole X-ray binary AT2019wey observed with TESS ›
A New Method to Simulate Dark Matter-Baryon Interactions and Application to an Isolated Disk Galaxy ›
The mmax-Mecl relation in the LEGUS clusters ›
A PANORAMIC of UV-optical morphologies of "Little Red Dots": Two groups of LRDs distinguished by UV half-light radius ›
From dust to planets -- II. Effects of wide binary companions and external photoevaporation on planetesimal and embryo formation ›
A scalable Bayesian framework for galaxy emission line detection and redshift estimation ›
Photon Ring Astrometry I: A Simple Spin Measurement Technique for High-Resolution Images of M87* ›
A striking excess of red quasars with steep radio spectral slopes: a dusty blow-out phase revealed through AGN-driven shocks? ›
The Coldest Known Y Dwarfs: Estimates of their Effective Temperatures ›
The Diffuse Gamma-ray Sky of a Milky Way Analogue: Local Diversity and Global Constraints ›
Production of heavy $\alpha$-elements and $^{44}$Ti in Cas A: comparison to abundances from 1D core-collapse supernova models and evidence for Carbon-Oxygen shell mergers ›
Distance estimate to NGC 6951 from supernova siblings Type IIP SN 2020dpw and Type Ib SN 2021sjt ›
Deep radiative zones affect the planetary cooling and internal structure: implications for exoplanet characterisation ›
Resizing the giants: How modelling adiabatic interiors impacts predicted planetary radii ›
Signatures of coronal mass ejections in differential emission measure analysis of the Sun as a star ›
SaNDi-SHoP: Searching for Satellites'N'Disks with a Star-Hopping Program I. Analysis of the close surroundings of DI companions ›
Understanding Balmer Decrements in T Tauri stars in terms of Multiflow Magnetospheric Accretion ›
On the importance of laboratory experiments for interpreting exoplanet observations ›
ALMAGAL VIII. Early phases of triggered star formation in source AG286.0716$-$1.8229 ›
Large-scale weak lensing convergence in nonlinear general relativity ›
Large Scale Spectrophotometric Relative Flux Calibration for the Roman High Latitude Wide Area Survey ›
Interstellar stereoisomerism ›
From Origins to Observables: Distinguishing Dark Compact Objects with Population-Level Microlensing Signatures ›
Propagating Kink Waves in Chromospheric Jet-like Structures and Coronal Plumelets ›
Revisiting the Claim for a Direct-Collapse Black Hole in UHZ1 at $z=10.05$ ›
Dynamics and stability of magnetized AGN-blown bubbles in clusters of galaxies ›
Flare-driven habitability: Expanding life's potential around low-mass stars ›
Investigation on the X-ray emission of NGC 4051 during its 2009 optical/UV-X-ray dissociation phase ›
Bar Properties and Star-by-Star Bar Membership via Action Conservation ›
Constraints on the Physical Association between ICECAT1 Neutrinos and Fast Radio Bursts Using the Second CHIME/FRB Catalogue ›
A post-perihelion constraint on the CO$_{2}$/H$_{2}$O ratio of interstellar comet 3I/ATLAS from [O I] forbidden lines ›
Probing Dust Composition in Distant Galaxies with JWST Mid-IR Spectroscopy of Quasars with Foreground 2175 {\AA} Absorbers II. Measurements of Grain Composition and Extinction Properties ›
X-ray spectral and temporal evolution of atoll source 4U 1820-30 with AstroSat: detection of high frequency quasi-periodic oscillation ›
The 'Forgotten' Neutrons: Implications for the Propagation of High-Energy Cosmic Rays in Magnetized Astrophysical and Cosmological Structures ›
Fitting the light curves of tidal disruption events with non-parabolic model ›
Development of a one-dimensional position sensitive detector for Compton X-ray polarimeters ›
Binary neutron star mergers with a subsolar mass star ›
Bulge Fossil Fragments as a new population of factories of gravitational wave sources in the Galaxy ›
Verification of the Polarimetric Capability of the East Asia VLBI Network ›
Core and mantle thermal evolution constraints on the onset of plate tectonics and a long-lived geodynamo ›
Star-Galaxy Classification in Deep LSST Data with Random Forest: A Pilot study on the Data Preview 1 Release ›
Development of ProtoPol: a medium resolution echelle spectro-polarimeter for PRL telescopes, Mt Abu, India -- Part I : the design, development and laboratory characterization ›
Interaction between vegetation and Snowball phases in the late Proterozoic Earth ›
Calibration of key parameters during the in-orbit phase for the Taiji-2 gravitational reference sensor ›
Jet Power Estimates of FSRQs PKS 1441+25 and Ton 599 from Broadband SED Modeling ›
Cluster gravitational redshifts: uncertainties and survey requirements ›
Development of ProtoPol: a medium resolution echelle spectro-polarimeter for PRL telescopes, Mt Abu, India -- Part II : the data-reduction pipeline, on-sky characterization $\&$ performance verification and first science results ›
Tracing neutral hydrogen in UGCA 320: A MHONGOOSE perspective on an edge-on dwarf galaxy in a group environment ›
Eclipsing binary classification with machine learning techniques ›
Probing the Solar Corona and the Solar Wind Using Angular Broadening Observations with the SKA ›
The Effect of Expansion and Instabilities in the Thermodynamic Regulation of the Young Solar Wind Plasma ›
Implementation of a Near-Realtime Recording and Reporting System of Solar Radio Bursts ›
Advancing weak lensing mass mapping with a mask-aware HEALPix transformer ›
The Circumbinary Disc of HD 34700A II. Analysis of a strong dust asymmetry ›
Bayes-SCF: A Bayesian filter to mitigate foreground leakage in the 21-cm power spectrum ›
The Impact of Fuzzy Dark Matter Dynamics on the Accumulation and Fragmentation of Primordial Gas ›
Particle Physics and Gravitational Waves as complementary windows on the Universe ›
POP-CORN: Validation of a new coronal hole detection tool based on neural networks ›
Structural Analysis of a Scalar-Tensor Realization of Interacting Dark Energy ›
Inferring the mass of the circumgalactic medium using X-ray resonant scattering ›
Ice chemistry that can be unveiled with the JWST: SynthIceSpec, a synthetic spectrum generator to test spectral limits. Solid CO_2 as a dust thermometer and solid CH_3CN detectability in cold cores ›
Painting a full radio sky -- Empirical mock catalogues with multiple source populations for future radio surveys ›
Double-Adiabatic Equations of State for Relativistic Plasmas ›
Interpretation of 21 cm Auto Power Spectrum Measurement at $z\sim 1$ by the Canadian Hydrogen Intensity Mapping Experiment ›
Nonlinear Information from DESI Luminous Red Galaxies: An Emulator-Based Analysis of Pre- and Post-Reconstruction Power Spectra ›
Identifying Surface Degeneracies in Single-Visit Reflected Light Observations of Modern Earth using the Habitable Worlds Observatory ›
Bayesian analysis of $\alpha$-Starobinsky model with Planck, ACT and DESI data ›
CMB constraints on dark matter-proton scattering: investigating prior-volume effects using profile likelihoods ›
Parameterizing Dark Energy at the density level: A two-parameter alternative to CPL ›
Testing Dark Energy with Black Hole Ringdown ›
Cosmological coupled black holes immersed in dark sector ›
Cosmological correlators from the Inflation end to CMB sky via reheating ›
Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge ›
ACT-Planck data and phase transitions from a viable no-scale Standard Model completion ›
The Universe Originating from an Empty Planck-Size Torus ›
UV-complete and stable Quintom Dark Energy models in the light of DESI DR2 ›
Cogenesis of visible and dark matter in type-I Dirac seesaw ›
Primordial black hole formation from transient $f(T)$ cosmology ›
Critical Behavior of Photon Rings in Kerr-Bertotti-Robinson Spacetime ›
A Telescope System for Charge and Position Measurement of High Energy Nuclei ›
Non parametric constraints of gravitational-electromagnetic luminosity distance ratio ›
Bayesian analysis of proton-proton fusion in chiral effective field theory ›
QED cross sections in strong magnetic fields ›
On the double-adiabatic equations in the relativistic regime ›
Halo Spin Depends on The Distance to Cosmic Filament ›
Bloodhound Unleashed: Particle-based Substructure Tracking for Cosmological Simulations ›
Semi-Supervised Learning for Lensed Quasar Detection ›
The Search for Stable Nickel: Investigating the Origins of Type Ia Supernovae with Late-time NIR Spectroscopy from the Carnegie Supernova Project-II ›
Differentiable Fuzzy Cosmic-Web for Field Level Inference ›
Evidence for Phenylium Reactivity under Interstellar Relevant Conditions ›
Cosmological constraints from galaxy clustering and galaxy-galaxy lensing with extended SubHalo Abundance Matching ›
Deciphering Baryonic Feedback from ACT tSZ Galaxy Clusters ›
Breaking the Mass-sheet Degeneracy in Time-delay Cosmology with Lensed and Unlensed Type Ia Supernovae ›
Orientation of orbital planes of planetary systems detected in microlensing campaigns ›
Simulation based inference of the ionization history from the 2D 21 cm power spectrum ›
Optimization procedure of the baffle of the GroundBIRD Telescope to mitigate stray light ›
Cloudy solutions for the clear skies of WASP-80b: 3D cloud feedback on the atmosphere and spectra of a warm Jupiter ›
Catalog of Mock Stellar Streams in Milky Way-Like Galaxies ›
Spatial Variations of Polarized Synchrotron Emission in the QUIJOTE MFI Data using Neural Networks ›
Readdressing the contribution of photonuclear reactions to the muon content of extensive air showers: a heuristic approach ›
Abundance Stratification in Type Iax SN 2020rea with TARDIS ›
Distinct Rotational Evolution of Giant Planets and Brown Dwarf Companions ›
HST view of NGC 5044: Constraints on Filament Widths, Magnetic Support, Multiphase Structure, and Comparison with Cluster Environments ›
A fast method for deriving relative small-scale magnetic field variations from high-resolution spectroscopy ›
Searching for Unparticles with the Cosmic Microwave Background ›
Graph Path Likelihood for Galaxy Formation on Layered Halo Graphs ›
What Shape is the Inflationary Bispectrum? ›
Stellar characterization with photometric colors from J-PLUS and 2MASS surveys ›
Improved dark matter measurements with flexible modeling of resolved strongly-lensed quasar narrow-line emission ›
Impact of Antenna Structure and Orientation on Forward-Modelled Global 21 cm Signal Recovery ›
Unlocking HST's Stellar Treasure Trove: Stellar Activity Minima for HAT-P-11 Offer Prime Windows for Transmission Spectroscopy ›
Notes on Gravitational Physics ›
Wideband Search for Axionlike Dark Matter Using Octupolar Nuclei in a Crystal ›
pylevin: Efficient numerical integration of integrals containing up to three Bessel functions ›
The Cosmic Horizon of Neutrinos ›
Dark Matter and Electroweak Baryogenesis with Spontaneous $CP$ Violation in the Early Universe ›
Designing trajectories in the Earth-Moon system: a Levenberg-Marquardt approach ›
Light scalars in light of UV/IR mixing: classicalization via synergy between Vainshtein and chameleon screenings ›
Fifty shades of grayness: parametrizations of spectral distortions and applications in cosmology ›
Conformal symmetry in force-free electrodynamics ›
A Unified Interpretation of Supernova, GRB, and QSO Time Dilation Signals in a Generalized Cosmological Time Framework ›
A dual description of quarks and baryons: Quarkyonic matter within a relativistic quark model ›
Breaking the degeneracy among regular black holes with gravitational lensing ↓↑