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

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RSS  Najnowsze prace na astro-ph:

› The LISA Astrophysics MBHcatalogues Project: A comparison of predictions of simulated massive black hole binaries
› A New Robust Constraint on the Self-interaction Cross-section of Dark Matter with Double Radio Relic Clusters
› The dark and featureless surface of rocky exoplanet LHS 3844 b from JWST mid-infrared spectroscopy
› Self-consistent numerical simulations for the formation and dynamics of solar prominences
› Deep Learning galaxy cluster's structural parameters from Weak Lensing observations
› Towards a measurement of the primordial helium isotope ratio
› Radiation Total Dose for PRIMA: Cold Exposure with Alpha Particles
› Confirmation of Fe I on MASCARA-5 b's Dayside Observed With EXPRES
› EMBER: Machine-Learning Detection of Modulated Ion Acoustic Waves and Associated Core-Electron Heating in the Solar Wind with Parker Solar Probe
› Smaller Than Earth Habitability Model (STEHM): The Lower Size Limit for Atmosphere Retention in the Habitable Zone
› A Detailed View of the Large-Scale Sloshing Cold Front in RXJ2014.8-2430
› Correspondence between a decaying dark matter sector scenario and scalar field model
› Extinction law and stellar mass in the Nuclear Bulge from kinematically-selected red clump stars
› Ultra-deep imaging of nearby dwarf irregular galaxies: stellar haloes and disk structure
› ExoplaNeT accRetion mOnitoring sPectroscopic surveY (ENTROPY) III. Optical He I line profiles of the accreting super Jupiter Delorme 1 (AB)b
› Exploring RR Lyrae Variable Stars in the Vera C. Rubin Observatory Data Preview 1
› A Universal Dance of Galactic Disks: Ubiquitous Precession and Its Implications
› Random Polarization Position Angle Behaviors across Bursts of Repeating Fast Radio Bursts
› Training a neural network to rapidly identify candidate gravitational-wave events in the lower mass gap
› Maximal mass of neutron stars constrained by neutron star observations
› Measuring $f\sigma_8$ and BAO scale in the Local Universe: a joint real and redshift space analysis from CosmicFlows-4++
› A consistent formulation of stochastic inflation I: Non-Markovian effects and issues beyond linear perturbations
› XMAGNET -- Stir before serving: a Lagrangian perspective on mixing-driven condensation in the intracluster medium
› Multi-messenger Constraints on a Primordial Black Hole Origin of the KM3-230213A Event
› Red Quasars: Selecting Candidates in SDSS DR16 and Estimating Their Physical Parameters
› The NIKA2 Cosmological Legacy Survey in COSMOS: Final 1.2mm and 2mm source catalogs and redshift distribution of dusty star-forming galaxies
› Kinematic properties of the TW Hya association
› The Rocky Planet Picture Show: Implementation of Surface Reflection and Emission in $\texttt{POSEIDON}$ with Application to and Interpretation of JWST Data
› Beyond Bragg-Mirrors for Gravitational Wave Telescopes: A Fabrication Tolerant Hybrid Metasurface-Bragg Mirror Design
› A bright wideband radio burst from the isolated neutron star 2XMM J104608.7$-$594306
› DESI and Gravitational Wave Constraints Challenge Quintessential {\alpha}-Attractor Inflation
› Life After the Quasar: Overmassive Black Holes and Remnant Ionised Bubbles in and Around Two z~6.6 Galaxies
› Magnetic loops in the solar transition region
› Upstream neutrino production and delayed jet emission in the blazar GB6 J1542+6129
› A Global 7% Systemic Sensitivity Floor in Gaia DR3: Multi-Wavelength Validation using 2MASS, Pan-STARRS and the 0.75-Magnitude Offset
› $4\times3$ Point Correlation Functions in Galaxy Surveys: Impact of Baryonic Feedback
› Optimization of Weak Lensing Lightcone Simulations for Higher-Order Statistics in the LSST era
› PEARLS: Two Distinct Populations of AGN Hosts Moving Between Star Formation and Quiescence
› Gravitational particle production, the cosmological tensions and fast radio bursts
› Study of cosmic ray impacts on cryogenic high sensitivity detectors
› Novel Chemical Pathways for the Formation of Nucleobase Precursors via Benzene {\pi}-Bond Addition to HCN
› Quantum Noise Fraction and the Thermal Frontier in High-Frequency Gravitational Wave Detection
› Pre-inflationary QCD axion stars after moduli domination
› Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries
› Radial Dependency of ICME-associated Particle Acceleration Processes: Statistical Multipoint Observations from 2016-2023
› High-resolution ro-vibrational and rotational spectroscopy of the open-shell, linear CCH$^+$ ion ($^3\Pi$)
› Anisotropy of Cosmic Background Photons from Annihilating/Decaying Dark Matter
› IceCube Results and Perspective for Neutrinos from LHAASO Sources
› Hyperactive Magnetar Eruptions: Giant Flares, Baryon Ejections, and Fast Radio Bursts
› Cosmic dipole tensions: confronting the cosmic microwave background with infrared and radio populations of cosmological sources
› Generalized Distributions of Host Dispersion Measures in the Fast Radio Burst Cosmology
› Ripples in the baryon to dark matter ratio in $\Lambda$CDM: implications for galaxy formation
› Solar Cycle Variation of Sustained Gamma Ray Emission from the Sun
› An effective $\boldsymbol{\Lambda}$-Szekeres modelling of the local Universe with Cosmicflows-4
› KL Dra as a Benchmark Laboratory for Accretion-Disk Physics: Constraints from TESS and Ground-Based Surveys
› Searching for Isolated Black Hole Candidates within 15 pc of the Solar System in Gaia DR3
› Maximum Energy of Particles Accelerated in GRB Afterglow Shocks
› An essential building block for cosmological zoom-in perturbation theory
› Cosmological analysis of the DESI DR1 Lyman alpha 1D power spectrum
› A Unified Framework for 10 TeV to EeV Diffuse Neutrino Sky and KM3-230213A
› Deeper detection limits in astronomical imaging using self-supervised spatiotemporal denoising
› The hydrodynamics of stratified ultra-relativistic outflows and the origin of GRB X-ray plateaus
› The TESS All-Sky Rotation Survey: Periods for 1,046,317 Stars Within 500 pc
› Interstellar Dust Transport Through the Heliosphere Including the Sector Region
› A systematic study of AGN feedback in a disk galaxy using MACER II: predictions of X-ray surface brightness profiles and comparison with eROSITA observations
› Weighing the mass of LHS 3844 b
› The RRATalog: a Galactic census of rotating radio transients
› Scale-dependent surface and volume density properties of filaments in molecular clouds
› Impact of Baseline, Cadence, and Host Contamination on AGN Variability Metrics: A Systematic Study with ZTF
› Benchmarking Two Chemical Networks used in General Circulation Models of Hot Jupiters
› Calibration-Induced Systematics in SALT3 Training and Their Impact on Dark Energy Constraints from Stage IV Supernova Surveys
› The Deep Newtonian Regime in Late-Time Blast Waves: Inevitable Transition and Distinct Flux Signatures
› SWIM: Stochastic Warm Inflation Module to generate and analyse Warm Inflationary power spectrum
› Waveform Modelling for the Laser Interferometer Space Antenna
› Weaving Life into Regolith: Engineered Autotrophic-Heterotrophic Consortia for Autonomous Biofabrication from Granular Feedstocks
› Parameter Estimation with Targeted Eccentric Numerical-Relativity Simulations for GW200208_22 and GW190620
› Stochastic Inflation in Numerical Relativity
› High Frequency Spectrum of Primordial Gravitational Waves
› Shadow signatures and energy accumulation in Lorentzian-Euclidean black holes
› Primordial black holes as cosmic accelerators of light dark matter: Novel direct detection constraints
› Gravitational Sommerfeld Effects: Formalism, Renormalization, and Perturbation to $O(G^{10})$

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