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Obserwatorium Astronomiczne na Suhorze

ponad chmurami

Kamerka S

Kamerka N

Niebo
Temperatura
12.4 °C
Wilgotność
92%
Wiatr
0.0 km/h
Ciśnienie
1005.3 hPa

Księżyc
Najnowsze prace na astro-ph:
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Hybrid stars among mass gap objects are excluded by twin stars at $1.4\,M_\odot$ ›
Systematic Polarization Errors from Parallactic-Angle Dependent Leakage in Pseudo-Circular Feeds ›
Enabling tomorrow's planetary defence and space resource economy: Autonomous fleet-based asteroid rendezvous missions ›
A Steep-Extinction QSO at z=4.6: JWST Evidence for Abundant Small Dust Grains ›
Euclid: Disky titans -- surprisingly high star formation efficiency in two brightest group galaxies at $z\sim 0.75$ ›
NOEMA$^\rm{3D}$: A deep view of cold gas flows in a barred spiral galaxy at $z\sim1$ ›
Systematic Error in Approximate Models of the GRB Early Afterglow ›
The Role of Stellar Spin in Repeating Partial Tidal Disruption Events ›
HERMES: HiERarchical Modelling for Exoplanet Science ›
Unbreaking the Universe: MINERVA Measurements of Color Gradients in Massive Quiescent Galaxies Can Help Ease Too-Early Star Formation Tensions ›
A New Record Census of Dwarf AGN and a Bimodal $M_{\rm BH}$-$M_{\star}$ Scaling Relation with DESI DR1 ›
The Life and Death of Stars That Capture Primordial Black Holes ›
Euclid: Early Release Observations -- Internal kinematics and the convective-transition gap of NGC 6397 ›
A Massive Hot-Jupiter Companion that Disfavors Giant Planet Formation Beyond the Water-Ice Line ›
Lyman-alpha Pressure Strongly Enhances Pre-Supernova Feedback at Cosmic Dawn: The First Multi-Dimensional Lyman-alpha Radiation Hydrodynamics Simulations ›
Constraints on the gravitational potential from DESI DR2 BAO and its implications for the local void scenario ›
The Radio-IR Correlation in the Context of Deep Radio Source Counts ›
Beyond Self-Similarity: Reconciling X-Ray Scaling Relations in Galaxy Clusters and Groups ›
A Cosmic Archipelago of lensed metal-poor galaxies at $z\sim6$ ›
Can current models predict the local black hole merger rate? ›
Accretion of Primordial Black Holes in Stellar Interiors ›
The effects of yields from binary massive stars as functions of metallicity ›
Precision constraints on stellar physics from main sequence detached eclipsing binaries ›
Formation of multiple dust rings and gaps in protoplanetary discs by a single migrating planet II: radiative discs and observational signatures ›
Signature of Bursty Star Formation in the High-Redshift Galaxies Detected with JWST ›
Bridging the UV Gap: The HST Ultraviolet Foundation for Star Formation Science in the Era of Roman, Euclid, and HWO ›
Elemental cosmic ray spectra reveal two populations of Galactic sources and an immediate transition to an extragalactic component after the knee ›
Why Little Red Dots Disappear at z < 3: Evolution of Number Density and Halo Mass ›
One Transit Is All You Need: Detecting Exoplanets Through Learned Stellar Behaviour with EXOVEIL ›
Neutrino Fingerprints: Image-Based Encodings of IceCube Events for CNN Direction Reconstruction ›
Topology of molecular clouds in the PHANGS-JWST catalogue in relation to the physical characteristics of their galaxies ›
First Detection of HC5N in a Class II Disk around TW Hya ›
Nereid as a Regular Satellite of Neptune ›
A High-Bandwidth Backplane for Wideband Radio Interferometers and Integration with the CHORD Telescope Correlators ›
The mass of the neutron star in 4U 1820-30 revisited ›
Field-level constraints on cosmic birefringence with a hybrid $E$-$B$ internal linear combination ›
Data-Driven Forecasting of three-Component Seismograms Using Transformer Architectures ›
On a re-examination of neutron star cooling in transient sources -- No shallow heating required? ›
Sensitivity of the Neutron Star Equation of State Inferences to Mass and Radius Measurements ›
Dust On, Dust Off: HST Observations of the Newly Dormant Jupiter Co-orbital Comet P/2023 V6 (PANSTARRS) ›
A $z \sim$ 6.2 Quasar on the Local M$_{\rm BH}$-$\sigma_{\rm \ast}$ Relation Quenching Its Host Galaxy from the Aether Survey ›
Comprehensive Analysis of Optical brightness and Color Variability of Blazars in the ZTF Survey DR22 ›
Fifty years of primordial helium abundances: A statistical reanalysis ›
COSMOS2025: Machine Learning Classification of Early- and Late-type Galaxies at 0 < z < 3 ›
A nine-member protostellar system forming via filament fragmentation in the high mass protocluster NGC 6334-43 ›
Detection of a four-carbon sugar in interstellar space ›
Deficit of primordial Li7 and primordial black holes ›
The caustic method applied to The Three Hundred: prospects for upcoming CATARSIS and other surveys ›
Little Red Dot progenitors from Compact Starbursts: A Natural Path to Early AGN Formation ›
Self-interacting neutrinos in cosmological perturbation theory -- integrating the collision kernel ›
Hidden-sector accretion and warped black-string seeds for high-redshift supermassive black holes ›
A comprehensive Rossiter-Mclaughlin Modelling Framework in TLCM: Application to HD 2685 $=$ TOI-135 system ›
The UV Side of Little Red Dots: Red, Compact, and Iron-Enhanced Rest-UV Emission with a Strong Downturn around Ly$\alpha$ ›
Simulation based parameter space for shock in transonic, sub-Keplerian accretion flow onto non-rotating black holes ›
The Gaia GSP-Spec catalogue of interstellar extinctions, and stellar luminosities, radii, and masses ›
Temperature-programmed desorption of SO2 from water ice surfaces: Adsorption energy distributions ›
Taxonomy of High Mass X-ray binaries from a historical perspective ›
Acenaphthene Derivatives as Signatures of C$_{11}$H$_9^+$ Reactivity with Methylated Naphthalenes ›
An analysis of the Type Ia SN 2024gy and a comparison of different host extinction estimation techniques ›
Varstrometry for Off-nucleus and Dual sub-Kpc AGN (VODKA): Radio Classification of High-Redshift Dual AGN Candidates with the Very Large Array ›
Multimodal Transformer Based Generic Mixture Density Network for Scattering Timescale Estimation of Fast Radio Bursts ›
Probing the Variation of the Inner Surface-Brightness Profile of Nuclear Star Clusters on the Intermediate-Mass Black Hole Mass Measurements Using Mock Observations of ELT/MICADO and HARMONI ›
Model-independent H0 from GWTC-4 standard sirens and TDCOSMO 2025 strong lensing time delays ›
Systematically Measuring Ultra-Diffuse Galaxies. IX. A Gyr in the Life of Nearby Low Surface Brightness Galaxies ›
Constraining AGN accretion physics with black hole mass-luminosity scaling relations ›
Astrophysical Constraints on Color-Superconducting Gap and N$^{3}$LO Perturbative-QCD Constant $c_0$ ›
Constraining Scale-Dependent Growth in $f(R)$ Gravity with Future 21 cm Surveys ›
J0404+1112: A 3-Hour Eclipsing White Dwarf-Brown Dwarf Probing Multiple Atmospheric Regimes ›
KRONOS I: The $1{-}2.8\mu$m JWST Transmission Spectrum of the 23 Myr V1298 Tau c ›
The impact of source and survey modelling on the connection between [O III] emitters and Ly $\alpha$ forest transmission at z ~ 6 ›
Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors ›
GraphShed: a parameter-free Graph-based waterShed group finder ›
The CRIMSON survey I: super-stellar SiO in the directly imaged companion TWA 5 B from high-resolution M-band spectroscopy ›
A Previously Underexplored Regime in TESS: Minute-Scale Eclipses Reveal Ten White Dwarf-Cool M-Dwarf Binaries ›
Biased tracers, Hybrid Effective Field Theory and Modified Gravity ›
Suppressed diffusion and gamma-ray emission from the Cygnus Bubble ›
Longitudinal Development Analysis of Extensive Air Showers Using CORSIKA Simulations ›
The VMC survey -- LV. The coherent expansion of the SMC ›
Spectral Handling and Estimation of AGN Parameters (SHEAP), The first AGN fitting GPU-based code ›
The OAD Flagship Ecosystem ›
Diocotron Modes in Pulsar Magnetospheres: Charge Diffusion and Implications for Radio Emission Variability ›
Teleocosmology and quantum post-selection ›
First results of a high sensitivity and transportable Ring Laser Gyroscope ›
Inverse energy transfer in decaying MHD turbulence: A shell-to-shell analysis ›
On-Shell Bootstrap of Loop Inflation Correlators with Spectral Dispersion ›
Thermal Metastable Strings in One-Scale Models and Gravitational Waves ›
Quintessential $\alpha$-attractors fit DESI ›
Deconstructing the Extra-Dimensional Axion ›
Probabilistic Microcausality in a Thermal Bath of Gravitons ›
The decay rate of metastable cosmic strings beyond the thin-string approximation ›
Lorentz-violating signatures in quasi-periodic oscillations from a magnetised Kalb-Ramond black hole ›
Model-Independent Search Discards Faint Lensed-Pairs of Gravitational Wave Events in the Sub-Threshold Candidates of GWTC-4 ›
Gravitino Freeze-In Dark Matter with an Additional Scalar Field ›
Signatures of Ultralight Dark Matter in Space-Based Laser Interferometers ›
Probing Inelastic Dark Matter via Cosmic-Ray Upscattering in NGC 1068 ›
Velocity space origins of pressure-strain interaction in multi-population distributions and its application to magnetic reconnection ›
The Broadband X-ray Spectral Properties during the Rising Phases of the Outburst of the New Black Hole X-ray Binary Candidate Swift J1727.8-1613 ›
ler: LVK (LIGO-Virgo-KAGRA collaboration) event (compact-binary mergers) rate calculator and simulator ›
The Large Smooth Patch on Comet 9P/Tempel 1: Remnant of a Recent Past Event ›
gwsnr: A Python package for efficient signal-to-noise ratio calculations of gravitational waves ›
A recoiling supermassive black hole in a powerful quasar ›
New insights on low-mass dark matter subhalo tidal tracks via numerical simulations ›
Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer ›
Ricci-Cubic Holographic Dark Energy: Confronting Observations, Stability and the Cosmic Coincidence Problem ›
KID Detector Readout Electronics Development for Habitable Worlds Observatory ›
Southern massive stars at high angular resolution. Physical separations and mass ratios ›
The Impact of Population III.1 Flash Reionization for CMB Polarization and Thomson Scattering Optical Depth ›
Stacking transmission spectra of different exoplanets ›
Large-Scale Structure Probes of the Post-Inflationary Axiverse ›
Episodic Star Formation -- I. Overview and Scatter of the Star-Forming Main Sequence ›
Trends in gravitational wave emission in axisymmetric simulations of rotating core-collapse supernovae ›
Weakened Inspirals I: High Mass Ratio Common Envelope Interactions in RGB Stars ›
Joint Optical-HI mock catalogues and prospects for upcoming HI surveys ›
Uniform models of neutron and quark (strange) stars in General Relativity ›
One-Loop Tensor Power Spectrum from a Non-Canonical Spectator Field during Inflation ›
Captured are circularized: A relativistic treatment of extreme mass ratio inspirals crossing accretion disks ›
Validating Digital Twins of the Local Universe with the Thermal Sunyaev-Zel'dovich Signal ›
Constraining reionization morphology and source properties with 21cm galaxy cross-correlation surveys ›
Skewness in the Hellings-Downs curve ›
A model-independent measurement of the Hubble constant from gravitational-wave standard sirens and electromagnetic observations ›
The impact of cosmic filaments on starburst galaxies across cosmic times ›
MXDFz4.4: A LyC emitter 250Myr after the epoch of reionization and a first test of Ly-alpha morphology as a tracer of LyC escape at high redshift ›
Mock Catalogs of Strongly Lensed Gravitational Waves via A Halo Model Approach with Ground-based Detectors ›
Spectroscopic galaxy redshifts in the Peanut cluster -- a massive nearly head-on cluster merger shortly after pericenter passage ›
FlowSN: Neural Simulation-Based Inference under Realistic Selection Effects applied to Supernova Cosmology ›
Warm Inflation Beyond the Markovian Limit ›
Type Ia supernovae interacting with a close circumstellar material (SNe Ia-CSM) are SNe Ia inside planetary nebulae (SNIPs) ›
SLSim: a strong lensing population simulation package ›
The ALMA-QUARKS survey: Investigating Thermal Feedback of Massive Protostars in Hot Molecular Cores ›
X-ray variability of SDSS J000532.84+200717.4: from a normal state to an X-weak state ›
POSEIDON II: The Anti-Aligned Orbit of the Warm Neptune TOI-1710 A b ›
cuRAMSES: Scalable AMR Optimizations for Large-Scale Cosmological Simulations ›
A Search for Wide-orbit Planets Around M-dwarfs using Deep MIRI 15-micron Images ›
JWST spectroscopy of SN 2010da/NGC 300 ULX-1: a surviving star hidden by dust ›
A spectroscopic map of the Galactic centre: Integrated light and dynamical modelling ›
UNIONS-3500 Weak Lensing: IV. 2D cosmological constraints in harmonic space ›
Isocurvature-Free QCD Axion Dark Matter from Inflaton-Driven Early QCD: the Necessity of Inflationary Plateaus ›
Disformal Kerr Imprints on BHL Accretion: Shock Morphology, PSD Signatures, and Observational QPO Counterparts ›
The exceptional 2017 gamma-ray flare of the radio galaxy NGC 1275: VERITAS and Multiwavelength Observations ›
Cosmological Constraints from Bias-Robust Wavelet Scattering Statistics for Stage-IV Galaxy Surveys ›
Constraints on Dynamical Dark Energy from Multiple Probes in the Full Dark Energy Survey ›
Effective Phantom Dark Energy: What Cosmological Reconstruction Does and Does Not Imply ›
Multi-Scale Magnetic Field Observations Reveal how Colliding Flows Trigger Star Formation ›
Interstellar Scintillation of Three Nearby Pulsars with FAST ›
Is the Dark Comet 1998 KY$_{26}$ the Spacecraft Phobos 1? ›
A study of the Physical Properties and Star Formation Activity of a Large Sample of Molecular Clouds: I Distances ›
Local relaxation and scale-dependent alignment in compressible, magnetized turbulence ›
Towards holographic color superconductivity in QCD ›
Exceptional Lines and Excitation of (Nearly) Double-Pole Quasinormal Modes: A Semi-Analytic Study in the Nariai Black Hole ›
Eigenmodes in an ultra-relativistic ultra-magnetized pair QED-plasma ›
Light rings, gravitational lensing, and ISCOs of exotic compact objects in Einstein-scalar-Maxwell theories ›
Intrinsic Nonlocality of Spin- and Polarization-Resolved Probabilities in Strong-Field Quantum Electrodynamics ›
Theoretical and Observational Bounds on Dynamical Chern-Simons Gravity as an Effective Field Theory ›
Correlative Microstructural Analysis of a Weathered Nantan Meteorite Fragment ›
The structure of multi-axion solutions to the strong CP problem ›
Dynamic Alignment as a Statistical Survival Effect ›
Predictive radar tracking reveals >500 mV/m electric-field transients during the May 2024 superstorm ↓↑