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

Widok nad kopułą w nocy

Kamerka S

Kamerka N

Niebo
Temperatura
-- °C
Wilgotność
--%
Wiatr
-- km/h
Ciśnienie
-- hPa

Księżyc
Najnowsze prace na astro-ph:
›
\texttt{py5vec}: a modular Python package for the 5-vector method to search for continuous gravitational waves ›
Formation and relaxation of halos in the context of wave DM particles evolving on a background of neutrino condensate ›
AGILE: an end-to-end Rubin-LSST simulation of AGNs, galaxies, and stars I. Software description and first data release ›
Field-Level Inference from Galaxies: BAO Reconstruction ›
Inferring the mass and size of 3I/ATLAS from its non-gravitational acceleration ›
Halo assembly bias in the early Universe: a clustering probe of the origin of the Little Red Dots ›
Multi-phase AGN-driven outflow in the NLSy1 IRAS 17020+4544. Unveiling dual-feedback and an energy-conserving ionized outflow with MEGARA/GTC integral field spectroscopy ›
Hankel low-rank matrix approximation for gravitational-wave data analysis ›
Shocks from Exploding Primordial Black Holes in the Early Universe ›
A 5kHz modulator for pyramid wavefront sensors ›
BL Lac host galaxies: how to systematically characterise them in optical-NIR spectroscopy ›
Magnetar counterparts, kinematics and birth sites with HST and JWST ›
BASS. LI. Cool gas supply of HI-massive local Seyfert galaxies ›
Single-source-class interpretation of the diffuse astrophysical neutrino flux ›
Out of oxygen: Extremely metal-poor galaxy candidates identified at $2.5 < z < 6.5$ with deep JADES medium-band imaging ›
Optimizing the Roman Space Telescope High-Latitude Wide Area Survey for mitigating chromatic PSF effects on shear measurement ›
Self-Consistent Nonlinear Classical Cepheid Pulsations During Stellar Evolution with MESA ›
NEATH V: the relationship between line emission from dense gas tracers and the star formation rate ›
Confidently Wrong: Why Ignoring Binaries Biases IMF Inference at Large Sample Sizes ›
Late-Onset Energy Injection in Type Ic SNe and W-Shaped O II Absorption in SLSNe-I ›
Revisiting observational constraints on coupled exponential quintessence with energy and momentum transfers: degeneracy with massive neutrinos ›
Experimental evidence for granular shear-flow instability in the Epstein regime ›
First detailed optical spectroscopic observations of the supernova remnants G107.7-5.1 and G150.3+4.5 ›
ODIN: Searching for LyC emission from Lyman-$\alpha$ emitters at $z=4.5$ in the E-COSMOS and XMM-LSS fields ›
Exploring memory-burdened primordial black holes with ultra-high-energy cosmic-rays ›
Spectral Hierarchy of the Cosmic Web ›
Gravitational-Wave Propagation Through the Axiverse ›
EGS-z11-R0: a red, dust-rich galaxy at Cosmic Dawn ›
A Third Galaxy Missing Dark Matter along a Trail of Galaxies in the NGC 1052 Field ›
Dark Energy with Constant Inertial Mass Density: Updated Constraints and Curvature-Induced Sign Transitions in $\rho_{\rm DE}$ and $\rho_{\rm DE}+p_{\rm DE}$ ›
Analysis of spatially resolved stellar populations and emission line properties in nearby galaxies with J-PLUS data. II-Results for the M51 group and first comparison with the M101 group ›
NEO Colors from The Mission Accessible Near-Earth Object Survey (MANOS) ›
SN 2025adpq: A Type Ia supernova in a collisional ring formed during a major galaxy merger ›
Measurements on the kinetic origin of streamer dynamics ›
A chemical perspective on planet formation in reduced systems ›
Cosmological prospects for multiband detection of intermediate-mass binary black holes with Taiji and ground-based detectors ›
Emulation of SPHEREx Galaxy Power Spectra I: Neural Network Details and Optimization ›
A Candidate Open Cluster Pulsar: Timing Analysis of PSR J1922+3745 in NGC 6791 ›
HESS J1832$-$085: evidence for a new gamma-ray binary candidate ›
Evolution of fractality in centrally concentrated young clusters ›
Cosmological hydrodynamical simulations of clustering dark energy with Nefertiti ›
Resonant scattering at the center of the galaxy cluster PKS 0745-191 with XRISM ›
Time-Lag properties associated with LFQPO in X-ray variability classes of GRS 1915+105: Findings from AstroSat ›
Optimising the FRB Search Pipeline for the Northern Cross Radio Telescope ›
Explainable machine learning workflows for radio astronomical data processing ›
High-Precision Photometry with a scientific CMOS Camera: II On-Sky Testing of the Marana camera at the NGTS facility ›
Detectability of Nearby Binary Neutron Stars with Future sub-mHz Gravitational Wave Missions ›
The role of ambipolar heating in the energy balance of solar prominences ›
Correlations Between kHz QPOs and Spectral Parameters from Time-Resolved Spectro-Temporal Analysis of 4U 1728-34 ›
Perturbative Effects of Dark Matter Environments on Black Hole Shadows ›
Unveiling an Hourglass-Shaped Magnetic Field toward IRDC G351.77-0.53 ›
LenghuSky-8: An 8-Year All-Sky Cloud Dataset with Star-Aware Masks and Alt-Az Calibration for Segmentation and Nowcasting ›
GEMS JWST: A sub-Solar metallicity atmosphere for giant planet TOI-5293Ab orbiting a rapidly changing M-dwarf ›
Diversity of Type Ia supernova optical light curves among different spectroscopic subclasses ›
Color and Size Distributions of Small Jupiter Trojans ›
Geometric Search for Hawking Radiation from Nearby Primordial Black Holes ›
Stellar Wind of Components of Detached Binary Systems ›
Singular Templates of Imaging Cherenkov Shower distribution (STOICS): A background estimation method for Very-High-Energy $\gamma$-ray observations ›
Laplace-Legendre expansion of the planar planetary Hamiltonian ›
Testing the Coexistence of Dark Energy and Dark Matter with Late-time Observational Data ›
Observational Constraints on WIMP Mini-Spikes Around Stellar-Mass Primordial Black Holes with 17 Years of Fermi-LAT Data ›
A Search for the Lost Comet P/2010 H2 (Vales) ›
The sensitivity and behaviour of the curvature in the \'echelle diagram of red-giant stars ›
Particle acceleration at recollimation shocks in sub-relativistic jets A model for jets in Seyfert Galaxies, Microquasars and Protostellar Systems ›
Stars with Plumbing Issues: The Formation of Collimated Outflows on Common-Envelope Simulations and Comparison to Water Fountains Observations ›
The shape and spin state of (275677) 2000 RS11 from ground-based radar and optical observations ›
Novel insights on the Coma Cluster kinematics with DESI. I. Linking mass profile, orbital anisotropy and galaxy populations ›
The long-term accretion luminosity of V4641 Sgr through binary evolution simulations: implications for its ultrahigh-energy gamma-ray emission ›
Cosmic Dipole as a Symmetry Response: From the Ellis--Baldwin Formula to Correlation Function Dipoles ›
A Unified Origin of Faraday Rotation toward 3C 84: The Circumnuclear Ambient Medium within the Parsec-Scale Bondi Radius of the Host Galaxy NGC 1275 ›
Type Ia supernovae interacting with a close circumstellar material (SNe Ia-CSM) are SNe Ia inside planetary nebulae (SNIPs) ›
Beyond $\Lambda$CDM with a Logistic RG-like Flow of the Low Redshift Cosmic Evolution ›
Optical Magnus effect on gravitational lensing ›
Cosmological Collider Searches beyond the Hubble Scale with Planck Data ›
Crowdsourcing Gravitational Waves from Superradiant Axions ›
Observing Micro Black Hole Dark Matter ›
Quasi-pole quintessential inflation in metric-affine gravity ›
Probing keV mass QCD axions with the SACLA X-ray free electron laser ›
Twin-peaked gravitational wave signal from a dark sector phase transition ›
Sensitivity of neutron star observables to microscopic nuclear parameters of realistic equations of state ›
Nuclear pasta in hot neutron-star matter and proto-neutron stars ›
Energy Conditions in Gauss-Bonnet Gravity ›
Advances in the Fabrication of On-chip Superconducting Integral Field Units for CMB and Line-Intensity Astronomy ›
On the survival of strong nuggets in the early Universe ›
New benchmarks for direct detection of freeze-in dark matter in vector portal models ›
Probing hadronic gamma-ray and high-energy neutrino emission from Gaia DR2 star clusters ›
Orbital eccentricity in a neutron star - black hole merger ›
Can a Breakdown of Hawking Evaporation Open a New Mass Window for Primordial Black Holes as Dark Matter? ›
X-ray Emission Signatures of Neutron Star Mergers ›
Gravitational waves from strong first order phase transitions ›
Primordial black holes save $R^2$ inflation ›
Dayside Clouds and an Elevated C/O Ratio in the Atmosphere of the Ultra-hot Jupiter WASP-19b ›
Unveiling the dark Universe with HI and EMBER-2 ›
Rotational Effects on Neutrino Emission in Core-collapse Supernovae ›
Quantifying the Effects of Parameters in Widespread SEP Events with EPREM ›
Directly Probing Neutrino Interactions through CMB Phase Shift Measurements ›
Weakly model-independent determination of total expansion during inflation ›
The Spatially Resolved Hot Gas Properties of NGC 1266's AGN-Driven Outflow ›
Vision-Based CNN Prediction of Sunspot Numbers from SDO/HMI Images ›
Ly{\alpha} Intensity Mapping in HETDEX: Galaxy-Ly{\alpha} Intensity Cross-Power Spectrum ›
The Nephele ecosystem: stars, globular clusters, and stellar streams associated with the progenitor galaxy of $\omega$ Centauri ›
Twinkle Twinkle Little Star, Roman Sees Where You Are: Predicting Exoplanet Transit Yields in the Rosette Nebula with the Nancy Grace Roman Space Telescope ›
A TESS View of Post-Eruption Variability in the Novae V1405 Cas,V1716 Sco, and V1674 Her ›
APOGEE chemical abundances of stars in the MW satellites Fornax, Sextans, Draco and Carina ›
Self-bound quark stars with a first-order two-to-three flavor phase transition ›
Evaluating the Prospects of Cyclic Deconvolution across 312 Pulsars ›
Multicolour Validation of Two Temperate Mini-Neptunes Around M-dwarf Habitable Zones ›
Towards Unveiling the Origins of the Milky Way Bulge through Multi-band-Messenger Sky Surveys ›
On the gravitational stratification of multi-fluid-multi-species plasma ›
Weak lensing of bright standard sirens: prospects for $\sigma_8$ ›
The early r-process nucleosynthesis scenarios ›
Magneto-Archeology of White Dwarfs. Revisiting the fossil field scenario with observational constraints during the red giant branch ›
Spectral response of SPHEREx ›
Most Strong Lensing Deflectors in the AGEL Survey Are in Group and Cluster Environments ›
Toward Black Hole Stars: supermassive black hole growth in nuclear clusters via stellar-object and gas accretion ›
First Dark Photon Search Results from the Dandelion Experiment ›
A steadily declining dispersion measure for the repeating fast radio burst FRB 20220529A: Evidence for an FRB engine embedded in an expanding supernova remnant ›
PICASO 4.0: Clouds and Photochemistry in Climate Models of Brown Dwarfs and Exoplanets ›
The Baryon Budget of Galaxies across the First Billion Years -- Theoretical Predictions for Gas Phases, Depletion Times, and Stellar Return Fractions ›
Evidence for a Delayed UV Counterpart to X-ray Quasi-periodic Eruptions in Ansky ›
Merger-driven buildup of the $M_{\rm BH}$ - $M_*$ relation bridging high-$z$ overmassive black holes with the local relation ›
Robustness of Neural Networks for CMB Polarization Foreground Removal ›
Signatures of Reconnection and a Split Heliospheric Tail in High-Energy Energetic Neutral Atoms ›
Mass Production of 2023 KMTNet Microlensing Planets. II: Two Planets and A Brown Dwarf ›
Spectral Variations of $\gamma$-rays in Mrk 421 ›
The Chandrasekhar's Conditions as Equilibrium and Stability of Stars in a Universal Three-Parameter Non-Maxwell Distribution ›
Freeze-in gravitational waves and dark matter in warm inflation ›
Observational bounds on Dark Matter Admixed Neutron Stars from Gravitational Wave Data ›
Fermionic Love of Black Holes in General Relativity ›
Dark matter: red or blue? ›
Dark matter silences Cepheids in the Galactic Center ›
Bubble Nucleation from Boson Star Collapse ›
ANNA: a toolbox for Newtonian Noise Analysis ↓↑