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

In the dark

S Webcam

N Webcam

S Sky
Temperature
9.0 °C
Humidity
83%
Wind
4.8 km/h
Pressure
1023.6 hPa

Moon
Latest preprints on astro-ph:
›
Stable 3-dimensional Vortex Families Consistent with Jovian Observations Including the Great Red Spot. (arXiv:2310.01435v1 [physics.flu-dyn]) ›
Quantum Scales of Galaxies from Ultralight Dark Matter. (arXiv:2310.01442v1 [astro-ph.GA]) ›
Measuring stellar rotation and activity with PLATO. (arXiv:2310.01465v1 [astro-ph.IM]) ›
A modern view of galaxies and their stellar populations. (arXiv:2310.01473v1 [astro-ph.GA]) ›
Pavo: Discovery of a star-forming dwarf galaxy just outside the Local Group. (arXiv:2310.01478v1 [astro-ph.GA]) ›
The Origin of the Consistent Planetary Nebula Luminosity Function Bright-end Cutoff. (arXiv:2310.01479v1 [astro-ph.SR]) ›
Vector Space Integration for Dark Matter Scattering. (arXiv:2310.01480v1 [hep-ph]) ›
Nonlinear acoustics and shock dynamics in isentropic atmospheres. (arXiv:2310.01481v1 [physics.flu-dyn]) ›
HI discs of L$_{\ast}$ galaxies as probes of the baryonic physics of galaxy evolution. (arXiv:2310.01482v1 [astro-ph.GA]) ›
Wavelet-Harmonic Integration Methods. (arXiv:2310.01483v1 [hep-ph]) ›
Stellar Escape from Globular Clusters. II. Clusters May Eat Their Own Tails. (arXiv:2310.01485v1 [astro-ph.GA]) ›
Sandwiched planet formation: restricting the mass of a middle planet. (arXiv:2310.01488v1 [astro-ph.EP]) ›
First constraints on Non-minimally coupled Natural and Coleman-Weinberg inflation in the light of massive neutrino self-interactions and Planck+BICEP/Keck. (arXiv:2310.01491v1 [astro-ph.CO]) ›
Cluster Ages to Reconstruct the Milky Way Assembly (CARMA) I. The final word on the origin of NGC6388 and NGC6441. (arXiv:2310.01495v1 [astro-ph.GA]) ›
The Cosmic Baryon Partition between the IGM and CGM in the SIMBA Simulations. (arXiv:2310.01496v1 [astro-ph.GA]) ›
AGN STORM 2. VI. Mapping Temperature Fluctuations in the Accretion Disk of Mrk 817. (arXiv:2310.01497v1 [astro-ph.HE]) ›
Considering the Single and Binary Origins of the Type IIP SN 2017eaw. (arXiv:2310.01498v1 [astro-ph.HE]) ›
Extended Main-Sequence Turnoff and Red Clump in intermediate-age star clusters: A study of NGC 419. (arXiv:2310.01499v1 [astro-ph.GA]) ›
SpectAcLE: An Improved Method for Modeling Light Echo Spectra. (arXiv:2310.01501v1 [astro-ph.IM]) ›
Distinguishing AGN Feedback Models with the Thermal Sunyaev-Zel'dovich Effect. (arXiv:2310.01502v1 [astro-ph.GA]) ›
Observational evidence for neutrino natal kicks from black-hole binary VFTS 243. (arXiv:2310.01509v1 [astro-ph.HE]) ›
X-ray and Radio Monitoring of the Neutron Star Low Mass X-ray Binary 1A 1744-361: Quasi Periodic Oscillations, Transient Ejections, and a Disk Atmosphere. (arXiv:2310.01511v1 [astro-ph.HE]) ›
The search for failed supernovae with the Large BinocularTelescope: The Mid-IR Counterpart to N6946-BH1. (arXiv:2310.01514v1 [astro-ph.HE]) ›
The birth and early evolution of a low mass protostar. (arXiv:2310.01516v1 [astro-ph.SR]) ›
Reading Between the Lines: Investigating the Ability of JWST to Identify Discerning Features in exoEarth and exoVenus Transmission Spectra. (arXiv:2310.01527v1 [astro-ph.EP]) ›
A comprehensive hydrodynamical study of SB DEM L50: understanding off-centre SNe and soft X-ray luminosity. (arXiv:2310.01531v1 [astro-ph.HE]) ›
GW190521: tracing imprints of spin-precession on the most massive black hole binary. (arXiv:2310.01544v1 [astro-ph.HE]) ›
Superradiant scattering of electromagnetic fields from ringing black holes. (arXiv:2310.01548v1 [gr-qc]) ›
Hot Jupiters Have Giant Companions: Evidence for Coplanar High-Eccentricity Migration. (arXiv:2310.01567v1 [astro-ph.EP]) ›
Ultracool Spectroscopic Outliers in Gaia DR3. (arXiv:2310.01576v1 [astro-ph.SR]) ›
Angular Correlations of Cosmic Microwave Background Spectrum Distortions from Photon Diffusion. (arXiv:2310.01578v1 [astro-ph.CO]) ›
Uncovering the MIR emission of quiescent galaxies with $JWST$. (arXiv:2310.01601v1 [astro-ph.GA]) ›
The GBT Diffuse Ionized Gas Survey (GDIGS): Discrete Sources. (arXiv:2310.01607v1 [astro-ph.GA]) ›
Indication of Sharp and Strong Phase-Transitions from NICER Observations. (arXiv:2310.01619v1 [astro-ph.HE]) ›
A Review of Infrasound and Seismic Observations of Sample Return Capsules since the End of the Apollo Era in Anticipation of the OSIRIS-REx Arrival. (arXiv:2310.01629v1 [astro-ph.EP]) ›
X-ray Polarization of the BL Lac Type Blazar 1ES 0229+200. (arXiv:2310.01635v1 [astro-ph.HE]) ›
The SOFIA FEEDBACK Legacy Survey: Rapid molecular cloud dispersal in RCW 79. (arXiv:2310.01657v1 [astro-ph.GA]) ›
Synthesis of infrared Stokes spectra in an evolving solar chromospheric jet. (arXiv:2310.01692v1 [astro-ph.SR]) ›
Spatially-Resolved Temperature and Density Structures of Nearby HII regions. (arXiv:2310.01703v1 [astro-ph.GA]) ›
A Strategy for Identifying Periodic Sources Contributing to the Galactic Center Excess. (arXiv:2310.01724v1 [astro-ph.HE]) ›
Super-Earth LHS3844b is tidally locked. (arXiv:2310.01725v1 [astro-ph.EP]) ›
Ultra-High-Energy Gamma-Ray Astronomy. (arXiv:2310.01744v1 [astro-ph.HE]) ›
Distinguishing the impact and signature of black holes from different origins in early cosmic history. (arXiv:2310.01763v1 [astro-ph.CO]) ›
J0107a: A Barred Spiral Dusty Star-forming Galaxy at $z=2.467$. (arXiv:2310.01782v1 [astro-ph.GA]) ›
On the influence of shock-cloud interactions on the nonthermal X-ray emission from the supernova remnant RCW 86. (arXiv:2310.01797v1 [astro-ph.HE]) ›
Semi-analytic calculations for extended mid-Infrared emission associated with FU Ori-type objects. (arXiv:2310.01813v1 [astro-ph.SR]) ›
Quantum algorithm for the Vlasov simulation of the large-scale structure formation with massive neutrinos. (arXiv:2310.01832v1 [quant-ph]) ›
Dark Matter Search with Cherenkov Telescope Array. (arXiv:2310.01847v1 [astro-ph.HE]) ›
End-To-End Optimization of the Layout of a Gamma Ray Observatory. (arXiv:2310.01857v1 [astro-ph.IM]) ›
Chemical Evolution in Galactic Nuclear Discs. (arXiv:2310.01899v1 [astro-ph.GA]) ›
The AstroSat UV Deep Field North: Direct determination of the UV Luminosity Function and its evolution from z $\sim$ 0.8-0.4. (arXiv:2310.01903v1 [astro-ph.GA]) ›
Spot-Based Measurement of the Brighter-Fatter Effect on a Roman Space Telescope H4RG Detector and Comparison with Flat-Field Data. (arXiv:2310.01920v1 [astro-ph.IM]) ›
Performance of the joint LST-1 and MAGIC observations evaluated with Crab Nebula data. (arXiv:2310.01954v1 [astro-ph.IM]) ›
Hall-magnetohydrodynamic simulations of X-ray photoevaporative protoplanetary disc winds. (arXiv:2310.01985v1 [astro-ph.EP]) ›
Updated bounds on Axion-Like Particle Dark Matter with the optical MUSE-Faint survey. (arXiv:2310.01996v1 [astro-ph.CO]) ›
DAGnabbit! Ensuring Consistency between Noise and Detection in Hierarchical Bayesian Inference. (arXiv:2310.02017v1 [gr-qc]) ›
Assessment of the CRD approximation for the observer's frame RIII redistribution matrix. (arXiv:2310.02021v1 [astro-ph.SR]) ›
Outgassing Composition of the Murchison Meteorite: Implications for Volatile Depletion of Planetesimals and Interior-atmosphere Connections for Terrestrial Exoplanets. (arXiv:2310.02028v1 [astro-ph.EP]) ›
A plausible link between dynamically unsettled molecular gas and the radio jet in NGC 6328. (arXiv:2310.02033v1 [astro-ph.GA]) ›
Multi-point study of the energy release and transport in the 28 March 2022, M4-flare using STIX, EUI, and AIA during the first Solar Orbiter nominal mission perihelion. (arXiv:2310.02038v1 [astro-ph.SR]) ›
Cold atomic gas identified by HI self-absorption. Cold atomic clouds toward giant molecular filaments. (arXiv:2310.02077v1 [astro-ph.GA]) ›
Impact of blending on weak lensing measurements with the Vera C. Rubin Observatory. (arXiv:2310.02079v1 [astro-ph.CO]) ›
Simulations of two-temperature jets in galaxy clusters: II. X-ray property of forward shock. (arXiv:2310.02105v1 [astro-ph.HE]) ›
Simulations of two-temperature jets in galaxy clusters: I. Effect of jet magnetization on dynamics and electron heating. (arXiv:2310.02109v1 [astro-ph.HE]) ›
Main sequence companions to white dwarfs II: the age-activity-rotation relation from a sample of Gaia common proper motion pairs. (arXiv:2310.02125v1 [astro-ph.SR]) ›
Light QCD Axion Dark Matter from Double Level Crossings. (arXiv:2310.02126v1 [hep-ph]) ›
Status of the Medium-Sized Telescopes for the Cherenkov Telescope Array Observatory. (arXiv:2310.02127v1 [astro-ph.IM]) ›
The deconfinement phase transition in $Sp(2N)$ gauge theories and the density of states method. (arXiv:2310.02145v1 [hep-lat]) ›
Enhanced Bayesian RFI Mitigation and Transient Flagging Using Likelihood Reweighting. (arXiv:2310.02146v1 [astro-ph.IM]) ›
Performances of an upgraded front-end-board for the NectarCAM camera. (arXiv:2310.02155v1 [astro-ph.IM]) ›
CNN photometric redshifts in the SDSS at $r\leq 20$. (arXiv:2310.02173v1 [astro-ph.CO]) ›
Atmospheric dynamics and shock waves in RR Lyr. (arXiv:2310.02180v1 [astro-ph.SR]) ›
Multimodality for improved CNN photometric redshifts. (arXiv:2310.02185v1 [astro-ph.CO]) ›
H I content of selected mid-infrared bright, starburst blue compact dwarf galaxies. (arXiv:2310.02202v1 [astro-ph.GA]) ›
Neutrino Emissions of TXS 0506+056 caused by a Supermassive Binary Black Hole Inspiral?. (arXiv:2310.02212v1 [astro-ph.HE]) ›
Turbulent Structure In Supernova Remnants G46.8-0.3 And G39.2-0.3 From THOR Polarimetry. (arXiv:2310.02213v1 [astro-ph.GA]) ›
The orbital period of the nova V1674 Her as observed with TESS. (arXiv:2310.02220v1 [astro-ph.SR]) ›
Spectro-polarimetry of 4U 1957+115 with IXPE: Effects of spin and returning radiation on polarised emission of black hole in thermal state. (arXiv:2310.02222v1 [astro-ph.HE]) ›
Mapping the Intracluster Medium in the Era of High-resolution X-ray Spectroscopy. (arXiv:2310.02225v1 [astro-ph.HE]) ›
High Angular Resolution Imaging of the V892 Tau Binary System: A New Circumprimary Disk Detection and Updated Orbital Constraints. (arXiv:2310.02241v1 [astro-ph.SR]) ›
Detecting New Visual Binaries in Gaia DR3 with Gaia and 2MASS Photometry I. New Candidate Binaries Within 200 pc of the Sun. (arXiv:2310.02256v1 [astro-ph.SR]) ›
Unifying supervised learning and VAEs -- coverage, systematics and goodness-of-fit in normalizing-flow based neural network models for astro-particle reconstructions. (arXiv:2008.05825v4 [cs.LG] UPDATED) ›
Dark matter halo mass functions and density profiles from mass and energy cascade. (arXiv:2210.01200v3 [astro-ph.CO] UPDATED) ›
Probing the low-mass end of core-collapse supernovae using a sample of strongly-stripped Calcium-rich Type IIb Supernovae from the Zwicky Transient Facility. (arXiv:2210.05729v2 [astro-ph.HE] UPDATED) ›
Nozzle Shocks, Disk Tearing and Streamers Drive Rapid Accretion in 3D GRMHD Simulations of Warped Thin Disks. (arXiv:2210.10053v2 [astro-ph.HE] UPDATED) ›
Pre-solar grains from novae and "Born-again giants". (arXiv:2211.12410v2 [astro-ph.EP] UPDATED) ›
Collisional flavor instability in dense neutrino gases. (arXiv:2212.03750v2 [hep-ph] UPDATED) ›
Nonperturbative collapse models for collisionless self-gravitating flows. (arXiv:2301.09154v2 [astro-ph.CO] UPDATED) ›
Primordial-tensor-induced stochastic gravitational waves. (arXiv:2302.14080v2 [gr-qc] UPDATED) ›
Reconstructing Galactic magnetic fields from local measurements for backtracking ultra-high-energy cosmic rays. (arXiv:2303.10099v2 [astro-ph.HE] UPDATED) ›
$\kappa$monty: a Monte Carlo Compton Scattering code including non-thermal electrons. (arXiv:2303.15522v2 [astro-ph.HE] UPDATED) ›
Proposed host galaxies of repeating fast radio burst sources detected by CHIME/FRB. (arXiv:2304.02638v2 [astro-ph.HE] UPDATED) ›
Signatures of Cosmic Ray Heating in 21-cm Observables. (arXiv:2304.07201v2 [astro-ph.CO] UPDATED) ›
Extreme-mass-ratio inspirals into rotating boson stars: nonintegrability, chaos, and transient resonances. (arXiv:2305.05691v2 [gr-qc] UPDATED) ›
Two-body problem in theories with kinetic screening. (arXiv:2305.07725v2 [gr-qc] UPDATED) ›
Rescaling strange-cluster stars and its implications on gravitational-wave echoes. (arXiv:2305.13323v2 [astro-ph.HE] UPDATED) ›
Lagrange top: integrability according to Liouville and examples of analytic solutions. (arXiv:2306.02394v4 [physics.class-ph] UPDATED) ›
Optimal Estimation of the Binned Mask-Free Power Spectrum, Bispectrum, and Trispectrum on the Full Sky: Tensor Edition. (arXiv:2306.03915v2 [astro-ph.CO] UPDATED) ›
Thomson scattering: One rate to rule them all. (arXiv:2306.06165v3 [astro-ph.CO] UPDATED) ›
Rapidly Rotating Massive Pop III stars: A Solution for High Carbon Enrichment in CEMP-no Stars. (arXiv:2306.06433v3 [astro-ph.SR] UPDATED) ›
Dissecting a 30 kpc galactic outflow at $z \sim$ 1.7. (arXiv:2306.07328v2 [astro-ph.GA] UPDATED) ›
Caract\'erisation et int\'egration de composants d'optique int\'egr\'ee sur l'interf\'erom\`etre fibr\'e FIRST au t\'elescope Subaru pour l'\'etude des protoplan\`etes en accr\'etion. (arXiv:2306.08989v2 [astro-ph.IM] UPDATED) ›
A Hunt for Magnetic Signatures of Hidden-Photon and Axion Dark Matter in the Wilderness. (arXiv:2306.11575v2 [hep-ph] UPDATED) ›
A metallicity dependence on the occurrence of core-collapse supernovae. (arXiv:2306.11962v2 [astro-ph.SR] UPDATED) ›
CMB Spectral Distortions from an Axion-Dark Photon-Photon Interaction. (arXiv:2306.13135v2 [hep-ph] UPDATED) ›
Influence of Dark Matter on the Magnetized Neutron Star. (arXiv:2306.17510v2 [astro-ph.HE] UPDATED) ›
AT2023fhn (the Finch): a Luminous Fast Blue Optical Transient at a large offset from its host galaxy. (arXiv:2307.01771v2 [astro-ph.HE] UPDATED) ›
Gauge fixing in cosmological perturbations of Unimodular Gravity. (arXiv:2307.04873v3 [gr-qc] UPDATED) ›
Quasinormal modes of black holes encircled by a gravitating thin disk. (arXiv:2307.07360v2 [gr-qc] UPDATED) ›
Analysis of Unified Galaxy Power Spectrum Multipole Measurements. (arXiv:2307.07475v3 [astro-ph.CO] UPDATED) ›
Cluster profiles from beyond-the-QE CMB lensing mass maps. (arXiv:2307.11711v2 [astro-ph.CO] UPDATED) ›
Simulations of Weakly Magnetized Turbulent Mixing Layers. (arXiv:2307.12355v2 [astro-ph.GA] UPDATED) ›
Extra-tensor-induced origin for the PTA signal: No primordial black hole production. (arXiv:2307.13109v2 [astro-ph.CO] UPDATED) ›
Intergenerational gauged $B-L$ model and its implication to muon $g-2$ anomaly and thermal dark matter. (arXiv:2307.14053v2 [hep-ph] UPDATED) ›
Supernova Simulations Confront SN 1987A Neutrinos. (arXiv:2308.01403v2 [astro-ph.HE] UPDATED) ›
Double black hole mergers in nuclear star clusters: eccentricities, spins, masses, and the growth of massive seeds. (arXiv:2308.10884v2 [astro-ph.HE] UPDATED) ›
Objects in JWST's mirrors are closer than they appear. (arXiv:2308.13347v2 [astro-ph.GA] UPDATED) ›
Teukolsky-like equations in a non-vacuum axisymmetric type D spacetime. (arXiv:2309.06237v2 [gr-qc] UPDATED) ›
Modelling the interaction of Alfv\'enic fluctuations with coronal mass ejections in the low solar corona. (arXiv:2309.06266v2 [astro-ph.SR] UPDATED) ›
Science Opportunities for IMAP-Lo Observations of Interstellar Neutral Helium, Neon and Oxygen During a Maximum of Solar Activity. (arXiv:2309.06931v2 [astro-ph.GA] UPDATED) ›
Assessment of Brightness Mitigation Practices for Starlink Satellites. (arXiv:2309.14152v3 [astro-ph.IM] UPDATED) ›
Black Hole Growth, Baryon Lifting, Star Formation, and IllustrisTNG. (arXiv:2309.14818v2 [astro-ph.GA] UPDATED) ›
Inverse-problem versus principal component analysis methods for angular differential imaging of circumstellar disks. The mustard algorithm. (arXiv:2309.14827v2 [astro-ph.IM] UPDATED) ›
Large numbers in the Universe and the origin of the Cosmic magnetic field. (arXiv:2309.14930v2 [astro-ph.CO] UPDATED) ›
Inferring coupling strengths of mixed-mode oscillations in red-giant stars using deep learning. (arXiv:2309.17372v2 [astro-ph.SR] UPDATED) ›
Bayesian inference methodology to characterize the dust emissivity at far-infrared and submillimeter frequencies. (arXiv:2310.01062v2 [astro-ph.GA] UPDATED) ›
Dissecting Cosmological Filaments at High Redshifts: Emergence of Spaghetti-type Flow Inside DM Haloes. (arXiv:2310.01369v2 [astro-ph.GA] UPDATED) ›
Jet Lorentz factor constraint for GRB 221009A based on the optical depth of the TeV photons. (arXiv:2310.00631v1 [hep-ph] CROSS LISTED) ↓↑