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Obserwatorium Astronomiczne na Suhorze

gwiazdy nad kopułą

Kamerka S

Kamerka N

Niebo
Temperatura
7.3 °C
Wilgotność
55%
Wiatr
11.3 km/h
Ciśnienie
1010.4 hPa

Księżyc
Najnowsze prace na astro-ph:
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A simulation-based inference of the Milky Way merger history ›
Phenomenology of an Open Effective Field Theory of Dark Energy ›
Simulating AGN wind feedback with variable feedback efficiencies in idealised disc galaxies ›
A Hot DOG Forged in FIRE: Nuclear and Starburst Spectral Decomposition of a Luminous Infrared Galaxy Simulation with a Resolved Dust Torus ›
Fast Fourier Transform evaluation of the Fresnel integral for gravitational-wave lensing ›
Probing Cosmology through Higher-Order CMB Lensing Statistics ›
Microquasar remnants as reservoirs of PeV cosmic rays ›
Reheating with Axion-SU(2) and Gravitational Chern-Simons Couplings ›
Confirmation of the hot super-Neptune TOI-672 b with NIRPS and HARPS and Insights into the Neptunian desert around M dwarfs ›
Robustness of Neural Networks for CMB Polarization Foreground Removal ›
The SMUGGLE-Ring project: Bar and bulge effects on nuclear disk and ring formation ›
HaloFlow II: Robust Galaxy Halo Mass Inference with Domain Adaptation ›
Gravitational self-lensing of Fast Radio Bursts in neutron star magnetospheres: II. Applications to strong repeaters and the CHIME population ›
SPHEREx Wide-Field Infrared Spectral Mapping of Interstellar Ices and Polycyclic Aromatic Hydrocarbons ›
Long-term monitoring of WASP-19 b: Signs of apsidal precession and molecular signatures ›
Refinements to the Solar Polar Magnetic Flux: Implications from Inversion Methodologies ›
Integral Field Spectroscopy of Collisional Ring Galaxies I: Stellar Populations Analysis ›
Standard Perturbation Theory for Interacting Dark Sector cosmologies I: Breakdown of Einstein de Sitter kernels ›
Relativistic astrospheres of gamma-ray binaries: modeling of non-thermal processes ›
Bridging the Gap: Using Brown Dwarfs to Examine Silicate Clouds in Giant Exoplanet Atmospheres ›
Exploring Beyond {\Lambda}CDM with the Weak Lensing Power Spectrum and Bispectrum ›
Spatial and spectral constraints on resolved mass-loss of the massive Post-RSG star IRAS 17163-3907 and its Fried Egg Nebula ›
Hot Jupiter - Cold Jupiter: A complex sibling relation ›
Sound Speed Resonance in the Gravitational Wave Background as a probe for non-standard early universe cosmologies ›
Galaxy fly-bys sustain bar-halo friction and bar slowdown in disk galaxies ›
Spectral Dataset of Stripped-Envelope Supernovae from the Tsinghua Supernova Group ›
Slowly Rotating Two-Fluid Neutron Stars: Coupled Frame-Dragging, Inertia Splitting, and Universal Relations ›
Mock Observations of Multiple Stellar Populations in Tidal Streams of Palomar 5 for the Chinese Space Station Survey Telescope ›
Beyond the Merger-Quasar-Quench Paradigm I: Mergers are neither necessary nor sufficient to quench central galaxies in IllustrisTNG ›
The influence of plasma lensing magnification to the luminosity function of fast radio bursts ›
Bolometric corrections of stellar oscillation mode amplitudes as observed by the PLATO mission. I. Planck-spectrum estimates ›
Chemical Properties and Sagittarius-induced Dynamical Perturbations of the GD-1 Stream ›
Spectroscopical Confirmation and Lens Modeling of a Complex Strong Lensing System Produced by a Close Galaxy Pair at $z_d=0.79$ ›
Halo abundance and clustering in cosmologies with massive and asymmetric neutrinos ›
A Census of Active Galactic Nuclei Identified by the Mid-infrared [Ne v] Line at $\boldsymbol{z \leq 0.025}$ ›
Gaia GraL X.: The GraL catalogue of gravitationally lensed quasars Matched with \textit{Gaia} data, redshifts, and time delays ›
Does supernova feedback regulate the star formation rate in dwarf galaxies? ›
Scrutinizing the 2020 multiwavelength outburst of PKS 0903-57 through observations with H.E.S.S ›
exoALMA XXI: The Morphology and Dynamics of Vertical Flows ›
Hub Formation and Filament-Filament Collision: An Analytical Model ›
ZTF J021804.16+071152.93: a dead cataclysmic variable and potential solution to the missing period bouncers ›
WISDOM Project -- XXVIII. Molecular gas measurement of the supermassive black hole mass of the galaxy NGC 1387 ›
MAXI J1820+070: A rapidly spinning black hole with mild disk truncation in the soft state and a warm corona ›
A low mass and radius neutron star candidate in XTE J1810-189? ›
Tied-array beam flatfielding ›
A near field guide to Roman's wide-area surveys ›
Detection of a molecular hydrogen envelope around nova GK Persei ›
Are supernovae driving turbulence in the solar neighborhood? ›
Calibrating Galaxy Infall Times in Groups and Clusters with IllustrisTNG Simulations ›
Simulation-based inference from the Lyman-alpha forest 1D power spectrum with CAMELS ›
exoALMA XXII: A Two-dimensional Atlas of Deviations from Keplerian Disks ›
Towards the Two-Loop EFTofLSS in Galaxy Lensing Surveys ›
A unified harmonic framework for dark siren cosmology ›
Impact of stellar spots on the high-resolution transmission spectra of a giant planet around a Sun-like star ›
IceCube Search for MeV Neutrinos from Mergers using Gravitational Wave Catalogs ›
Three-band dark-siren cosmology with intermediate-mass black hole binaries: synergy of Taiji, LGWA, and Einstein Telescope ›
exoALMA. XXIV. Formaldehyde Emission in Protoplanetary Disks of exoALMA Compared with Their Properties and Dynamical State ›
Signatures of Reconnection and a Split Heliospheric Tail in High-Energy Energetic Neutral Atoms ›
Modelling the expulsion of baryons from haloes from first principles: the role of feedback and of the cosmological constant ›
Ridged Lagrangian Perturbation Theory (RLPT) ›
The elusive cyclotron line in 4U 1901+03: hidden, yet present ›
When Dark Energy Turns On: Constraints on a Critical Emergence Model ›
Structural Parameters of the Globular Cluster M 15 ›
Euclid preparation. Simulated galaxy catalogues for non-standard cosmological models ›
exoALMA XXIII. Estimating Disk and Planet Properties from Dust Morphologies with DBNets2.0 ›
exoALMA XX: Tomographic Detection of Embedded Planets in Protoplanetary Disks ›
Connecting JWST Silicate Cloud Observations to Exoplanet Cloud Microphysics with Nimbus ›
Ortho-Para Chemistry of H2CO in the Protoplanetary Disk TW Hya ›
Clustering Astronomical Orbital Synthetic Data Using Advanced Feature Extraction and Dimensionality Reduction Techniques ›
Euclid preparation. Far-infrared predictions for Euclid galaxy catalogues: cluster, protocluster, and field ›
Optimising Foreground Modelling for Global 21cm Cosmology with GPU-Accelerated Nested Sampling ›
A Commensal Radio-Only Cosmic Ray Detector at the Owens Valley Radio Observatory Long Wavelength Array ›
Negative Masses and Spatial Curvature: Alleviating Neutrino Mass Tensions in LambdaCDM and Extended Cosmologies ›
Comparison of Cross-Correlation Methods for Line Intensity Mapping ›
A 2% determination of $N_{\rm eff}$ from primordial element abundance, cosmic microwave background, and baryon acoustic oscillation measurements ›
Looking for non-gaussianity in Pulsar Timing Arrays through the four point correlator ›
Dark Matter, Baryon Number, and Cosmic-Ray Antinuclei ›
All-electron dark matter-electron scattering with random-phase approximation dielectric screening and local field effects ›
Traversable Wormholes induced by Thomas-Fermi energy density ›
Weibel Instability in Collisionless Plasmas Across Astrophysical and Laboratory Shocks ›
Not So Minimal Warm Inflation ›
Design of a Dichroic Transmissive Huygens' Metasurface Unit-Cell Presenting Refraction Angle Duality ›
A basic model for high energy cosmic ray interactions ›
The Migdal effect in Semiconductors for the Effective Field Theory of Dark Matter Direct Detection ›
Axion search with telescope for radio astronomy (ASTRA): forecast for observations between 0.5 and 4~GHz ›
Challenging the Weak Cosmic Censorship with Phantom Fields ›
Disentangling the anisotropic radio sky: Fisher forecasts for 21cm arrays ›
BICEP/Keck XIX: Extremely Thin Composite Polymer Vacuum Windows for BICEP and Other High Throughput Millimeter Wave Telescopes ›
Toward a Distributed Radio Telescope Using Global IoT Networks: Calibration Methods and Feasibility Analysis ›
Continuous Design and Reprogramming of Totimorphic Structures for Space Applications ›
Estimating the Lensing Probability for Binary Black Hole Mergers in AGN disk by Using Mismatch Threshold ›
Implementation of CR Energy SPectrum (CRESP) algorithm in PIERNIK MHD code. II. Propagation of Primary and Secondary nuclei in a magneto-hydrodynamical environment ›
Exploring future synergies for large-scale structure between gravitational waves and radio sources ›
Turbulence in Simulated Local Cluster Analogs: One-to-one comparisons between SLOW and XRISM/Hitomi ›
Revealing tensions in neutron star observations with pressure anisotropy ›
Mitigating point-source contamination in CMB polarization: a Generalized Point Spread Function fitting approach ›
Diversity and Evolution of Dust Attenuation Curves from Redshift z ~ 1 to 9 ›
Optimized HDBSCAN clustering for reconstructing the merger history of the Milky Way: applications and limitations ›
DELVE Milky Way Satellite Galaxy Census I: Satellite Population and Survey Selection Function in DES, DELVE, and Pan-STARRS ›
Two-phase formation of galaxies: the coevolution between galaxies and dark matter halos ›
The causal structure of galactic astrophysics ›
Elusive Plunges and Heavy Intermediate-mass-ratio Inspirals from Single and Binary Supermassive Black Holes ›
Saving Doomed Planets: Mass Loss and Angular Momentum Return Boost Hot Jupiter Survival Rates ›
Solving the cooling flow problem with combined jet-wind AGN feedback ›
Finding the boundary: Using galaxy membership to inform galaxy cluster extent through machine learning ›
Gas excitation of post-starburst galaxies at 0.6 < z < 1.3 ›
Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension ›
Optical and cm follow-ups of the Changing-Look event in Mkn 590 ›
Enhancing evidence estimation through informed probability density approximation ›
Dynamical disequilibrium in dwarf galaxies: rethinking gas dynamics, rotation curves, and dark matter inference ›
Primordial Black Holes as Seeds for Extremely Overmassive AGN Observed by JWST ›
An effective $\boldsymbol{\Lambda}$-Szekeres modelling of the local Universe with Cosmicflows-4 ›
Born in the Dark: The Catastrophic Collapse of Fuzzy Dark Matter Solitons as the Origin of Little Red Dots ›
Unveiling the spectral morphological division of fast radio bursts with CHIME/FRB Catalog 2 ›
A positive period derivative in the quasi-periodic eruptions of ZTF19acnskyy ›
A Catalogue of Orbital Periods of Cataclysmic Variables and Candidates from TESS Observations ›
Euclid: A blue galaxy population and a brightest cluster galaxy in the making in a $z\sim1.74$ MaDCoWS2 galaxy cluster candidate ›
Martian concretion sizes predicted from two independently constrained inputs: atmospheric dust grain size and obliquity-forced wetting duration ›
FlowSN: Neural Simulation-Based Inference under Realistic Selection Effects applied to Supernova Cosmology ›
Neutrino Spectral Pinching in 3D Core-Collapse Supernovae: Late-Time Convergence, Failed-Explosion Signatures, and Viewing-Angle Dispersion ›
SN 2023axu: A Type IIP Supernova Interacted with a Low-Density Stellar Wind ›
Solar neutrino physics ›
A Traveling-Wave Parametric Amplifier and Converter ›
Multifield theories invariant under transverse diffeomorphisms: The mixed regime case ›
Cosmic Axion Background Detection Using Resonant Cavity Arrays ›
A dynamical systems perspective on the thermodynamics of late-time cosmology ›
Efficient Reconstruction of Matched-Filter Signal-to-Noise Ratio Time Series from Nearby Templates for Compact Binary Coalescences Searches ›
Natural inflation in Palatini $F(R)$ ›
Small-scale turbulent dynamo for low-Prandtl number fluid: comparison of the theory with results of numerical simulations ›
Simulating first-order phase transition during inflation ›
Accelerating Black Hole Image Generation via Latent Space Diffusion Models ›
Detectability Scaling Laws for Environmental Phase Modulation in Gravitational-Wave Signals ↓↑