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Obserwatorium Astronomiczne na Suhorze

Suhora w nocy

Chmury

Opady

Niebo
Temperatura
5.2 °C
Wilgotność
73%
Wiatr
6.4 km/h
Ciśnienie
1005.6 hPa

Księżyc
Najnowsze prace na astro-ph:
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A practical guide to implementing zero-order-hold interplanetary trajectory legs ›
Clustering constraints on super-early galaxy formation scenarios ›
Spectroscopic Bolometric Corrections and Empirical Zero-point Constants of \textit{Gaia} Magnitudes, $G$, $G_{\rm BP}$, and $G_{\rm RP}$, from \textit{Gaia} XP Spectra ›
A correlation predicting galaxies without dark matter ›
Observational Signatures and Constraints on the Intermediate Neutron-Capture Process. The Case of the CEMP star TYC 6044-714-1 (RAVE J094921.8-161722) ›
A Uniform Determination of the Bulk Metallicities and Alpha Enrichments of Confirmed Exoplanet Systems with TRES ›
The Impact of Cosmic Variance and Satellites on JWST Clustering Measurements at Redshift around 6 ›
New Isocurvature Constraints from JWST UV Luminosity Function ›
FLAMINGO: The thermal history of the Universe from tSZ effect cross-correlations and its dependencies on cosmology and baryon physics ›
A Quantum Gravitational Mechanism for Isotropization of de Sitter Cosmologies ›
The $R$-Process Alliance: The $R$-Process Enhancement of Stars from Chemodynamically Tagged Groups in the Milky Way Halo ›
Seasonal Insolation Variability on Early Venus: Implications for Energy Budget ›
The Quadruply Lensed Supernova SN 2025wny: Implications for LSST ›
Chemical signatures of planetary systems in their host stars. Near-infrared spectroscopy of four planet-hosting wide binaries ›
Survey Footprint Explorer: A Browser-Based Interactive Tool for Visualizing and Cross-Matching Astronomical Survey Footprints ›
Tracing Radio AGN-Driven Quenching in Post-Starburst Galaxies at Cosmic Noon ›
A Cyclic Burst Rate Behavior of a Persistent X-ray Burster: Recent XMM-Newton and NuSTAR Observations of 4U 1323-62 ›
Detection and Characterization of the Temperate Super-Earth Ross 318 b ›
An Outer Giant Planet or Brown Dwarf in the 51 Pegasi System? ›
Quantifying the Reconstructability of Astrophysical Methods with Large Language Models and Information Theory: A Case Study in Spectral Reconstruction ›
From raw data to neutrino candidates: a neural-network pipeline for Baikal-GVD ›
The Extended Plane of the Local Supercluster ›
Prospects for multi-messenger discovery of the gravitational-wave background anisotropies via cross-correlation with galaxies ›
The applicability of the JAGB method for measuring the distance of galaxies subject to different metal enrichment rates ›
Variable stars in the field of the Galactic globular cluster M71 ›
Black Hole Binary Detection Landscape for the Laser Interferometer Lunar Antenna (LILA): Signal-to-Noise Calculations & Science Cases ›
Optical Design of OPTICAM-ARG: A Three-Channel High-Time-Resolution Camera for the Jorge Sahade Telescope ›
Continuous mass ablation of planets engulfed in stellar envelopes ›
Transonic accretion and the analogue gravity in multi-component elliptical galaxies hosting pseudo-Schwarzschild black holes ›
The Internal Nebular Attenuation Curve of Three-Dimensional Turbulent HII regions ›
An investigation of magnetic energy and helicity thresholds at the onset of solar eruptions based on numerical simulations ›
Exploring the stellar streams and satellites around the giant low surface brightness galaxy Malin 1 ›
Evolution of Crab Pulsar: Magnetic Inclination Angle and Spin ›
Revisiting GW170817 at milliarcsecond scale: high-precision constraints on jet geometry and $H_0$ ›
A Nearly Constant Compton y-parameter for Mildly Relativistic Slab Coronae in AGN ›
Secondary-Mass Features improve Spectral-Siren $H_0$ Constraints ›
A Hybrid Origin for the Multiple Ring-Gap Structures in the Large Protoplanetary Disk V1094 Sco: A Low-Mass Planet and Secular Gravitational Instability ›
Black Hole Ringdown Seen in Photon Polarization Swings ›
Are Single-Zone Emission models Sufficient to Explain GRB 220426A and GRB 230812B? ›
A hierarchical Bayesian pipeline for soliton-plus-NFW inference on SPARC rotation curves: diagnostics and prior-boundary behaviour ›
Interacting Binary Stars as Progenitors for Interacting Supernovae ›
Metal Enrichment by the First Stars Exploding at the Lower Energy Limit of Pair-Instability Supernovae ›
GI BAO as a cosmological consistency check ›
Evidence for Multiple Orbiting Hotspots in the 340 GHz Variability of Sgr A* ›
Starspot activity and surface differential rotation on UX Arietis ›
Synergy between the Cherenkov Telescope Array Observatory and the Vera C. Rubin Observatory ›
A New Timing Signature of Black Hole Spin: Time-Delay Asymmetry in Kerr Accretion Flows ›
Measurements and predictions of H2 pressure-broadening coefficients of CO2 absorption lines for exoplanet atmosphere studies ›
Simulation of the spin evolution of some selected exoplanets and inferences on their climate ›
Reaccumulation process after a catastrophic disruption event on a differentiated asteroid ›
Real-time detection of solar flares from ground-based VLF data ›
High-energy Multi-messenger Emission from Galaxy Clusters in the Local Universe ›
High-energy Neutrino and Gamma Ray Emission from Clusters-like Perseus ›
Inferring host environment properties and gravitational-wave decay time from the eccentricity measurement of dynamically captured binaries ›
Limit on high energy neutrino emission from Abell 119 using IceCube 10-year muon track data ›
Marginal multi-object multi-frame blind deconvolution ›
A phenomenological model of the magnetic field re-emergence in magnetars and discrepancy between the kinematic and characteristic ages ›
An eclipsing CEMP candidate discovered in a search for dwarf carbon stars in post-common envelope binaries ›
Ultra-light axion constraints from Planck and ACT: the role of nonlinear modelling ›
Effect of Solar Flares on Decayless Kink Oscillations in Nearby Coronal Loops ›
Catching UHE Neutrinos with HERON ›
Periodic Emission Frequency Modulation in a Hyperactive Fast Radio Burst ›
Discriminating Planck Reionisation Histories with the kSZ Effect ›
Non-LTE atmosphere models of very luminous sources and their applicability to Little Red Dots, quasi-stars, and similar objects ›
Proximate damped Lyman-$\alpha$ systems as tracers of quasar feedback ›
A tool of Hierarchical cOre ideNtification and Kinematic property AssIgnment (HONKAI) for Dense Cores ›
An Ultra-Short Period Super-Earth and a Sub-Neptune Orbiting the K dwarf TOI-4311 ›
How plasma coupling and convective-zone depth shape the rotation of solar-mass stars ›
Simulating the jittering-jets explosion mechanism: Supernova remnant G11.2-0.3 ›
Trajectory-Agnostic Asteroid Detection in TESS with Deep Learning ›
Impact of Calibration Systematics on Dark Energy Constraints from LSST Type Ia Supernovae ›
Late-time reconstruction of non-minimally coupled gravity with a smoothness prior ›
Modeling and Analysis of Main-Belt Asteroidal Dust Flux and Velocity Distribution at Inner Planets ›
Self-consistent dynamical modelling of the Milky Way bar with orbital frequency analysis ›
Precessing Black Hole Jets and Galactic Fossils ›
Elemental Abundances in the Binary Star V505 Per ›
Unveiling $f(R)$ Gravity with Void-Galaxy Cross-Correlation Multipoles ›
Photometric determination of the mass accretion rates of pre-main sequence stars. IX. Recent star formation in the periphery of NGC 346 ›
Measuring cosmic bulk flow with kinetic Sunyaev-Zel'dovich velocity reconstruction ›
Unveiling Hidden Lyman Alpha Emitters in the DESI DR1 Data ›
Big Mysteries Survey: Physicists' Views on Cosmology, Black Holes, Quantum Mechanics, and Quantum Gravity ›
Neutrino mixing and gravitational production via inflation ›
CMB Birefringence from Vacuum Interfaces ›
An ultra-broadband axion dark matter experiment ›
Stochastic inflation from a non-equilibrium renormalization group ›
The mean-field theory of superfluid-superconducting vortex states in the outer core of neutron stars ›
gwBenchmarks: Stress-Testing LLM Agents on High-Precision Gravitational Wave Astronomy ›
End-to-End Population Inference from Gravitational-Wave Strain using Transformers ›
Detection of Gravitons: Graviton Absorption and Excess of Photon Luminosity from Interstellar Hydrogen ›
Discovery of Interpretable Surrogates via Agentic AI: Application to Gravitational Waves ›
Closing the Cosmographic Hierarchy: Dynamical Attractors from Inflation to Reheating ›
Dynamic Alignment: A Fragile Survival Effect ›
Reviving primordial black hole formation in slow first-order phase transitions ›
Causality and Scientific Inquiry: Lessons from Space Physics and Medical Sciences ›
GW240925 and GW250207: Astrophysical Calibration of Gravitational-wave Detectors ›
A self-adjoint Fourier-type model for the iQuad wavefront sensor ›
Probing the small-scale primordial power spectrum via relic neutrinos and acoustic reheating ›
The choice of variables in cosmological dynamical systems ›
Power Studies For Two-Sample and Goodness-of-Fit Methods For Multivariate Data ›
Hyperfine-Resolved Rovibrational and Rotational Spectroscopy of OH$^+$ ($X ^3\Sigma^-$) ›
Basilisk and Docker for Reproducible GN&C Simulation: A Workflow Reference ›
Semi-Analytic Modeling of Dark Matter Subhalo Encounters with Thin Stellar Streams: Statistical Predictions for GD-1-like Streams in CDM ›
Evidence for the gravity-driven and magnetically-regularized gas flows feeding the massive protostellar cluster in Cepheus A ›
Denoising weak lensing mass maps with diffusion model: systematic comparison with generative adversarial network ›
A search for periodic AGN variability in $\textit{Gaia}$ Data Release 3 ›
Quantifying biases in stellar masses of JWST high-z quasar host galaxies caused by quasar subtraction ›
Optical Flares in the Luminous Fast Blue Optical Transient AT2022tsd ("Tasmanian Devil") ›
Exploring Jet Structure and Dynamics in Short Gamma Ray Bursts: A Case Study on GRB 090510 ›
Dark Matter and the Early Formation of Supermassive Black Holes ›
Correcting the fiber-aperture bias affecting galaxy stellar populations in the Sloan Digital Sky Survey. Aperture corrections to absorption indices based on CALIFA integral field observations ›
Probing Evolution of Long Gamma-Ray Burst Properties through Their Cosmic Formation History ›
Probing evolution of Long GRB properties through their cosmic formation history aided by Machine Learning predicted redshifts ›
Dark Matter from Holography ›
A Bayesian Perspective on Evidence for Evolving Dark Energy ›
The Impact of Supermassive Black Holes on Exoplanet Habitability. I. Spanning the Natural Mass Range ›
Probing the Nature of Dark Matter Self-Interactions Through Observations of Massive Black Hole Mergers ›
Probing Dark Matter Substructure with Image Number Anomaly in Strong Lensing Systems ›
Core-halo scaling relations in self-interacting scalar field dark matter ›
Evolving and interacting dark energy: photometric and spectroscopic synergy with DES Y3 and DESI DR2 ›
Sensitivity of Weak Lensing Surveys to Gravitational Waves from Inspiraling Supermassive Black Hole Binaries ›
Comprehensive study of solar type II radio bursts and the properties of the associated shock waves ›
The JWST EXCELS survey: Outflows in 1.5 < z < 5 quiescent and recently quenched galaxies are likely relics from episodic AGN activity ›
Search for Precessing Binary Black Holes in Advanced LIGO's Third Observing Run using Harmonic Decomposition ›
Possible evidence for a pair-instability supernova nature of ultra-early JWST sources ›
Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation ›
An Enhanced Formation Channel for Galactic Dual-Line Gravitational-Wave Sources: von Zeipel-Lidov-Kozai Effect in Triples Involving Sgr A* ›
Cosmological Averaging in Nonminimally Coupled Gravity ›
Cylindrical cosmological simulations with StePS ›
Implications for Primordial Black Hole Dark Matter from a Single Subsolar Mass Gravitational-wave Detection in LVK O1--O4 ›
X-SORTER (X-ray Survey Of meRging clusTErs in Redmapper): X-ray and Spectroscopic Characterization of 12 Optically Selected Galaxy Cluster Merger Candidates ›
JWST's PEARLS: A clumpy ring galaxy at $z = 4.0148$ ›
The ALPINE-CRISTAL-JWST Survey: Gas-phase abundance gradients of main sequence star-forming galaxies and their kinematics at $4 < z < 6$ ›
Dust characterization of halos: The extended emission in protoplanetary disks ›
Other red dots: A possible GLIMPSE of normal AGB stars at Cosmic Noon through extreme lensing ›
IXPE Polarizations of the Lighthouse Pulsar, Trail, and Filament ›
A Unified Explanation of Gamma-Ray and Neutrino Spectra from Astrophysical Sources Based on the Gluon Condensation Model ›
Moving-Mesh Simulations of Mini-Common Envelope Ejection in Classical Novae ›
Jet-driven shocks and turbulence in radio-loud Active Galactic Nuclei observed with JWST MIRI/MRS ›
Challenges to the cosmological constant model following results from the Dark Energy Survey ›
Application of Machine Learning to 21 cm Cosmology ›
Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object ›
Theoretical Detailed Analyses for DC readout and a Fabri-P\'erot gravitational-wave detector ›
Biased parameter inference of eccentric, spin-precessing binary black holes ›
APRIL: Auxiliary Physically-Redundant Information in Loss -- A physics-informed framework for parameter estimation with a gravitational-wave case study ›
Neutron star crust and outer core equation of state from chiral effective field theory with quantified uncertainties ›
Covariant interpretation of proper infall times in Kerr spacetime ›
Rotating Black Holes with Primary Scalar Hair: Shadow Signatures in Beyond Horndeski Gravity ↓↑