Podchorazych 2, 30-084 Krakow, Poland.
tel.: (+48 12) 662 6301;
fax: (+48 12) 637 2243;
Obs. tel.: (+48) 502 113714
Mount Suhora Astronomical Observatory

Before observations ...

Cloud

Rainfall

S Sky
Temperature
3.7 °C
Humidity
93%
Wind
0.0 km/h
Pressure
1023.3 hPa

Moon
Latest preprints on astro-ph:
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Early massive galaxy formation in the core of a galaxy protocluster 650 million years after the Big Bang ›
MESA-QUEST: Tracing the formation of direct collapse black hole seeds via quasi-stars ›
The Blue Jay Survey: Deep JWST Spectroscopy for a Representative Sample of Galaxies at Cosmic Noon ›
The PHANGS-MUSE/HST-Halpha Nebulae Catalogue ›
Spatial Profiles of 3I/ATLAS CN and Ni Outgassing from Keck/KCWI Integral Field Spectroscopy ›
Cross-correlation of Luminous Red Galaxies with ML-selected AGN in HSC-SSP III: HOD Parameters for Type I and Type II Quasars ›
Violent mergers revisited: The origin of the fastest stars in the Galaxy ›
Spin and Obliquity Distributions of Low-mass Planets Shaped by Dynamical Instability ›
Connecting Cores and Black Hole Dynamics Across Scales: From Globular Clusters to Massive Ellipticals ›
ELPIS: Accelerated metal and dust enrichment in a proto-cluster core at $z\approx8$ ›
Searching for GEMS: TOI-5916 b & TOI-6158 b are two Saturn-density planets orbiting M2 dwarfs ›
Eruptive mass loss less than a year before the explosion of superluminous supernovae. II. A systematic search for pre-explosion eruptions with VLT/X-shooter ›
Dwarf diversity in $\Lambda$CDM with baryons ›
Delayed phase mixing in the self-gravitating Galactic disc ›
Wind and nearby stellar environment of the quiescent luminous blue variable Var 2 in the Galaxy M33 ›
Preferential accretion of binary stars ›
Hubble reveals complex multi-scale structure in the edge-on protoplanetary disk IRAS 23077+6707 ›
Evolutionary Links: From Gaia Neutron Star Binaries to Pulsar White Dwarf Endpoints ›
The resilience of the sailboat stable region ›
A (very) simple proof of the gravitational energy formula of polytropic spheres ›
Magnetic Decay Index Profile and Coronal Mass Ejection Speed ›
A Systematic North-South asymmetry in the Steady-state Climate of rapidly-rotating Oblique Water Worlds ›
Ultraviolet radiation and neutrinos: two messengers from CCSNe in the CSM scenario ›
Abundances of Rarely Detected s-process Elements Derived from the Ultraviolet Spectrum of the s-process-enhanced Metal-poor Star HD 196944 ›
Near the Runaway: The Climate and Habitability of Teegarden's Star b ›
PLATOSpec: a precise spectrograph in support of space missions ›
GALACTICNUCLEUS: A high angular resolution JHKs imaging survey of the Galactic centre ›
Rotation of Polarization Angle in Gamma-Ray Burst Prompt Phase. III. The Influence of the Magnetic Field Orientation ›
Impact of Cosmic Ray Acceleration on the Early Evolution of Bow Shocks around Massive Runaway Stars ›
Deep JWST spectroscopy of galaxies in a candidate ionized bubble at $z = 8.7$: probing reionization at pMpc scales with Ly$\alpha$ emission ›
The Two-Zone Temperature Distribution Model: Inferences on the Structure and Composition of Dusty Protoplanetary Disks ›
Short-Lived Radioisotopic enrichment from AGB interlopers in low-mass star-forming regions ›
Very-Long Baseline Interferometry Imaging with Closure Invariants using Conditional Image Diffusion ›
Using gravitational lensing to probe for bright quintessential galaxies in the Epoch of Reionization ›
A Possible Shutting-Down Event of Mass Accretion in An Active Galactic Nucleus at z~1.8 ›
Eternal inflation bubble collision signature on CMB remote dipole and quadrupole fields ›
Polar Filaments Capture High Latitude Solar Poloidal Field Interactions and can Foretell the Future Sunspot Cycle Amplitude before Polar Field Precursors ›
CCAT: Optical Responsivity, Noise, and Readout Optimization of KIDs for Prime-Cam ›
Beyond the Brightest: A Deep Learning Approach to Identifying Major and Minor Galaxy Mergers in CANDELS at $z \sim 1$ ›
The AURORA Survey: Ionizing Photon Production Efficiency with Minimal Nebular Dust Attenuation Systematics ›
Violent mergers can explain the inflated state of some of the fastest stars in the Galaxy ›
Computational advances and challenges in simulations of turbulence and star formation ›
YSO Variability in the W51 Star-Forming Region ›
Encapsulating Textual Contents into a MOC data Structure for Advanced Applications ›
A census of quiescent galaxies across $0.5 < z < 8$ with JWST/MIRI: Mass-dependent number density evolution of quiescent galaxies in the early Universe ›
Is Milky Way stable all the way ? A TNG50 view from cosmic noon to the present day ›
Experimental tests of the calibration of high precision differential astrometry for HWO ›
Spatio-Temporal Evolution of the March 2022 ICME Revealed by Multi-Point Observations of Forbush Decreases ›
Fe XVIII-XXIV K beta Inner-shell Absorption Lines in the X-ray Spectra of Neutron Star and Black Hole Binaries with XRISM ›
Hidden Figures of Globular Clusters: Integrated Stellar Populations Impacted by Hot Subdwarfs ›
Discovery of new magnetic {\delta} Scuti stars and impact of magnetism on pulsation excitation ›
The rings of (2060) Chiron: Evidence of an evolving system ›
Association of cold gas, massive galaxies, and AGNs in a filamentary protocluster traced by triple narrow-band imaging ›
Infrared spectral signatures of light r-process elements in kilonovae ›
Extremely UV-bright starbursts at the end of cosmic reionization ›
Lanthanide Impact on the Infra-Red Spectra of Nebular Phase Kilonovae ›
Catalog and Characterization of Science Orbit Configurations for an Enceladus Orbiter ›
Optically thick winds of very massive stars suppress intermediate-mass black hole formation ›
Enhanced Localization of Dark Lensed Gravitational Wave Events Enables Host Galaxy Identification and Precise Cosmological Inference ›
Asteroseismic calibration of the Rossby number and its connection to the stellar dynamo and fundamental properties ›
Jets in Low-Mass Protostars ›
Faint galaxies in the Zone of Avoidance revealed by JWST/NIRCam ›
A Catalog of Filaments in the Central Molecular Zone ›
Limits of Standard Tidal Models at Quaoar: Matching Weywot's Orbit, Missing the Spin ›
Polarization from Rapidly Rotating Massive Stars ›
DIPLODOCUS II: Implementation of transport equations and test cases relevant to micro-scale physics of jetted astrophysical sources ›
The double neutron star PSR J1946+2052 I. Masses and tests of general relativity ›
Gamma-rays from Wolf-Rayet stellar winds ›
Spectroscopic Reverberation Mapping for SARM: The Case of Mrk 1048 and Mrk 618 ›
Widespread Hot Molecular Gas Heated by Shear-induced Turbulence in the Galactic Center ›
A 50-min coronal kink oscillation and its possible photospheric counterpart ›
Using simultaneous mass accretion and external photoevaporation rates for d203-504 to constrain disc evolution processes ›
Non-linear structure formation with elastic interactions in the dark sector ›
Mass dependence of halo baryon fractions from the kinetic Sunyaev-Zeldovich effect ›
Modeling gamma-ray signatures of particle acceleration in stellar clusters from GeV to PeV ›
JWST and Keck Observations of the Off-Nuclear TDE AT 2024tvd: A Massive Nuclear Star Cluster and Minor-Merger Origin for its Black Hole ›
A constant upper luminosity limit of cool supergiant stars down to the extremely low metallicity of I Zw 18 ›
The MIRI Excesses around Degenerates (MEAD) Survey I: A candidate cold brown dwarf in orbit around the nearby white dwarf 2MASS J09424023-4637176 ›
Formation of protostars and the launching of stellar core outflows with moving-mesh radiation non-ideal magnetohydrodynamics ›
Cloudy with a chance of starshine: Possible photometric signatures of nebular-dominated emission in $1.5 < z < 8.5$ JADES galaxies ›
Alleviating the $H_0$ tension through new interacting dark energy model in light of DESI DR2 ›
GEFF: The Gradient Expansion Formalism Factory - A tool for inflationary gauge-field production ›
Searching for Stellar-Feedback-Driven Outflow Signatures: A Deep Dive into NGC 3741 ›
Energy calibration of LHAASO-KM2A using the cosmic ray Moon shadow ›
The Influence of the Accretion Disc Structure on X-ray Spectral States in Symbiotic Binaries ›
Enigmatic centi-SFU and mSFU nonthermal radio transients detected in the middle corona ›
Tycho supernova exploded inside a planetary nebula (SNIP) ›
The diverse shapes of binary asteroid satellites born from sub-escape-velocity moonlet mergers ›
Hierarchical summaries for primordial non-Gaussianities ›
Interacting galaxies in the IllustrisTNG simulations - IX: Mini mergers trigger AGN in cosmological simulations ›
Mapping the Perseus Galaxy Cluster with XRISM: Gas Kinematic Features and their Implications for Turbulence ›
An Ultra-Short Period Super-Earth and Sub-Neptune Spanning the Radius Valley Orbiting the Kinematic Thick Disk Star TOI-2345 ›
Visual morphological classification of the full MaNGA DR17 sample: a general characterization ›
Born Dry or Born Wet? A Palette of Water Growth Histories in TRAPPIST-1 Analogs and Compact Planetary Systems ›
The Gravitational Wave Memory from Binary Neutron Star Mergers ›
Black Hole Ringdown Amplitudescopy ›
Quasinormal modes from numerical relativity with Bayesian inference ›
False Alarm Rates in Detecting Gravitational Wave Lensing from Astrophysical Coincidences: Insights with Model-Independent Technique GLANCE ›
On the Speed-up of Wave-like Dark Matter Searches with Entangled Qubits ›
Dynamically generated tilt of isocurvature fluctuations ›
New Tests of Low-Scale Quantum Gravity with Cosmic-Ray Collisions ›
Gravitational Wave Signatures from Lepton Number Breaking Phase Transitions with Flat Potentials ›
Phase space analysis of an exponential model in $f(Q)$ gravity including linear dark-sector interactions ›
Model of deep zonal flows in giant planets ›
The importance of being non-minimally coupled: scalar Hawking radiation from regular black holes ›
The probe limit in MHD and its implications for magnetic transport ›
Observational Constraints on Chaplygin Gas Models in Non-Minimally Coupled Power Law $f(Q)$ Gravity with Quasars ›
High-energy photons from Gamma-Ray Bursts, but no neutrinos ›
Hunting Primordial Black Hole Dark Matter in Lyman-$\alpha$ Forest ›
Reconstruction of the swampland conjectures with DESI DR1 BAO data ›
Value Added Catalog of physical properties of more than 1.3 million galaxies from the DESI Survey ›
Measuring Star Formation Histories from Asymptotic Giant Branch Stars I: A Demonstration in M31 ›
How Many Bursts Does it Take to Form a Core at the Center of a Galaxy? ›
The $z \gtrsim 9$ galaxy UV luminosity function from the JWST Advanced Deep Extragalactic Survey: insights into early galaxy evolution and reionization ›
Enhancing the reliability of machine learning for gravitational wave parameter estimation with attention-based models ›
Unveiling the trends between dust attenuation and galaxy properties at z ~ 2 - 12 with the James Webb Space Telescope ›
A Time-Dependent Solution for GSN 069 Disk Evolution and the Nature of Long-Lived Tidal Disruption Events ›
The Giant Arc -- Filament or Figment? ›
Clustering analysis of BOSS-CMASS galaxies with semi-analytical model for galaxy formation and halo occupation distribution ›
HeII emitters at cosmic noon and beyond. Characterising the HeII {\lambda}1640 emission with MUSE and JWST/NIRSpec ›
Prospects for probing dark matter particles and primordial black holes with the Square Kilometre Array using the 21 cm power spectrum at cosmic dawn ›
Ultra-long MeV transient from a relativistic jet: a tidal disruption event candidate ›
Tidal heating in detached double white dwarf binaries ›
In-Situ Formation of the Cold Classical Kuiper Belt ›
DIPLODOCUS I: Framework for the evaluation of relativistic transport equations with continuous forcing and discrete particle interactions ›
The redshift distribution of Einstein Probe transients supports their relation to gamma-ray bursts ›
Investigating aerosols as a way to reconcile K2-18 b JWST MIRI and NIRISS/NIRSpec observations ›
Dwarf galaxy halo masses from spectroscopic and photometric lensing in DESI and DES ›
Extended mass distribution of PBHs during QCD phase transition: SGWB and mini-EMRIs ›
1FLAT: a Firmamento-based catalog of AGN in Fermi-LAT high Galactic latitude {\gamma}-ray sources ›
JWST Spectroscopy of SN Ia 2022aaiq and 2024gy: Evidence for Enhanced Central Stable Ni Abundance and a Deflagration-to-Detonation Transition ›
Resolving stellar populations, star formation, and ISM conditions with JWST in a large spiral galaxy at z $\sim$ 2 ›
The Relation Between AGN and Host Galaxy Properties in the JWST Era: II. The merger-driven evolution of Seyferts at Cosmic Noon ›
Resonant W and Z Boson Production in FSRQ Jets: Implications for Diffuse Neutrino Fluxes ›
The Sunburst Arc with JWST. IV. The importance of interaction, turbulence, and feedback for Lyman-continuum escape ›
Emergent Cosmological Expansion in Scalar-Tensor Theories of Gravity ›
Anatomy of singlet-doublet dark matter relic: annihilation, co-annihilation, co-scattering, and freeze-in ›
Verifiable type-III seesaw and dark matter in a gauged $\boldsymbol{U(1)_{\rm B-L}}$ symmetric model ›
Characterized behaviors of black hole thermodynamics in the supercritical region ›
Electroluminescence and charge multiplication in liquid xenon with a VCC-like Microstrip Plate ›
Accelerated inference of binary black-hole populations from the stochastic gravitational-wave background ›
Radio emission from airplanes as observed with RNO-G ›
Projective Transformations for Regularized Central-Force Dynamics: Hamiltonian Formulation ›
Space-based cm/kg-scale Laser Interferometer for Quantum Gravity ›
Small Progenitors, Large Couplings: Type Ic Supernova Constraints on Radiatively Decaying Particles ›
Splitting the Gravitational Atom: Instabilities of Black Holes with Synchronized/Resonant Hair ›
GW250114 reveals black hole horizon signatures ↓↑