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Obserwatorium Astronomiczne na Suhorze

Suhora w nocy

Kamerka S

Kamerka N

Niebo
Temperatura
3.4 °C
Wilgotność
83%
Wiatr
1.6 km/h
Ciśnienie
1019.8 hPa

Księżyc
Najnowsze prace na astro-ph:
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A Unified Model and Optimization for Deep Space Radiation Shielding Based on Proton Density ›
Roman Galactic Plane Survey Definition Committee Report ›
The Inner Kernel of the Classical Kuiper Belt ›
JWST lensed quasar dark matter survey IV: Stringent warm dark matter constraints from the joint reconstruction of extended lensed arcs and quasar flux ratios ›
The Deepest GLIMPSE of a Dense Gas Cocoon Enshrouding a Little Red Dot ›
Finding the boundary: Using galaxy membership to inform galaxy cluster extent through machine learning ›
The Dark Energy Survey Supernova Program: A Reanalysis Of Cosmology Results And Evidence For Evolving Dark Energy With An Updated Type Ia Supernova Calibration ›
Empirical Bolometric Correction and Zero-Point Constants of Visual Magnitudes from High-Resolution Spectra ›
Null Impact of the Null Energy Condition in Current Cosmology ›
The Type Ia Supernova 2021hem: A 2003fg-like Event in an Apparently Hostless Environment ›
Changing-Look Active Galactic Nuclei in SDSS-V: Host-Galaxy Properties and Black-Hole Scaling Relations ›
Lost Sisters Found: TESS and Gaia Reveal a Dissolving Pleiades Complex ›
The Shape of the Solar Tachocline ›
Multi-messenger flare in the quasar PKS 0446+11 ›
Using Stellar Spectral Energy Distributions to Measure Exoplanet Parameters ›
MHSXtraPy - A Python code for the extrapolation of magnetohydrostatic fields on the Sun using analytical solutions ›
\texttt{ExTraSS}: a Domain Decomposed 3D NLTE Radiative Transfer spectral synthesis code for nebular phase transients ›
Emission line models for the lowest mass core-collapse supernovae -- II. Full 3D NLTE radiative transfer modelling of a $9.0\,M_\odot$ neutrino-driven explosion ›
JWST's GLIMPSE: an overview of the deepest probe of early galaxy formation and cosmic reionization ›
Effect of ionizing photon escape fraction in faint galaxies on modeling reionization history of the universe ›
Warm and cold molecular gas in the cluster center of MACS 1931-26 with JWST and ALMA ›
General Circulation Models of Hycean Worlds ›
A Timescale-Resolved Analysis of the Breathing Effect in Quasar Broad Line Regions ›
Chemical dissection of merger-induced $m=1$ lopsidedness in Milky Way-like galaxies ›
The impact of precession and higher-order multipoles on cosmological inference ›
Characterizing TESS-Identified Quadruple and Higher Order Eclipsing Binaries: I. Speckle Imaging with DSSI and HRCam ›
JWST/NIRCam observations of HD~929245 debris disk: An asymmetric disk with a gap ›
General Implicit Runge-Kutta Integrators for Multifluid Gas-Dust Aerodynamic Drag ›
Effect of molecular hydrogen self-shielding modeling on early Reionization Era galaxies in radiative hydrodynamic cosmological simulations ›
Dark Matter Heating in Evolving Proto-Neutron Stars: A Two-Fluid Approach ›
Resolving the large exoKuiper belt of the HD 126062 debris disc and extended gas emission in its vicinity ›
From Feedback-Free Star Clusters to Little Red Dots via Compaction ›
Dust Recycling and Icy Volatile Delivery (DRIVE): A Novel Method of Volatile Enrichment in Cold Giant Planets ›
J-PLUS Reconstructing the Milky Way Disc's star formation history with twelve-filter photometry ›
Reassessing the Relationship Between Stellar X-ray Luminosity and Age with eROSITA Data Release 1 ›
Searching for Exoplanets Born Outside the Milky Way: VOYAGERS Survey Design ›
Blazar PKS 0446+11 - Neutrino connection study using a lepto-hadronic model ›
First results from the PanRadio GRB Collaboration: the 400-day afterglow of GRB~230815A ›
A Closed-Form Analytical Theory of Non-Isobaric Transmission Spectroscopy for Exoplanet Atmospheres ›
Alternative approach to time-delay interferometry with optical frequency comb ›
Cross Calibration of Galaxy Cluster Temperatures Measured with NuSTAR, XMM-Newton, and Chandra ›
Identifiability of Rotating Stellar Surfaces from Astrometric Jitter ›
Probing the Physical Origin of the Balmer Decrement in the Broad-line Region of Nearby Active Galactic Nuclei via Spectral Variability ›
Detection of unexpected leading delays in broad H{\beta} line reverberations in the quasar PHL 1092 ›
Simultaneous detection of the size and velocity of the largest ejecta particles with velocities exceeding 1 km^{-1} ›
"Popcorn Planets" are Not Actively Inflated by Eccentricity Tides ›
Kerr Polarization Transport: Accuracy and Performance in General Relativistic Light Propagation ›
The formation and structure of iron-dominated planetesimals ›
JWST Lensed Quasar Dark Matter Survey III: Dark Matter Sensitive Flux Ratios and Warm Dark Matter Constraint from the Full Sample ›
Could the stochastic gravitational wave background from newborn magnetars be detected by the advanced LIGO and Einstein Telescope? ›
A Modified 3D Biconical Outflow Model: Spatial Constraints on AGN-driven Outflows ›
In-Orbit GRB Identification Using LLM-based model for the CXPD CubeSat ›
Spectral distortions in the decaying QCD dark matter scenario ›
Towards direct imaging and orbital parameter estimation of supermassive black hole binaries with spaceborne VLBI ›
Probing Supernovae through gravitational wave entropy ›
CSST Strong Lensing Preparation: Cosmological Constraints Forecast from CSST Galaxy-Scale Strong Lensing ›
HyperScout-H: the hyperspectral imager for the ESA Hera mission ›
Stellar spin in young star clusters: comparison between simulations and observations ›
Study of Flat Spectrum Radio Quasars and BL Lacertae Objects as Sources of Diffusive Ultra High-Energy Cosmic Rays ›
Investigating star formation scenarios in the Milky Way using YSO distributions - A pilot study ›
Galaxy cluster temperature maps from joint X-ray and SZ maps with The Three Hundred hydrodynamical simulations ›
Emulating Radiative Transfer in Astrophysical Environments ›
Fill the gaps: continuous in time interpolation of fluid dynamical simulations ›
Euclid preparation. Non-Gaussianity of 2-point statistics likelihood: Precise analysis of the matter power spectrum distribution ›
An Overview of Exocomets ›
A Strong Gravitational Lensing Model of PSZ2 G118.46+39.32 ›
The MATISSE view of the inner region of the RY Tau protoplanetary disk ›
Coordinated Space- and Ground-based Monitoring of Accretion Bursts in a Protoplanetary Disk: The Orbital and Accretion Properties of DQ Tau ›
Remanent crustal strain on Mars in non-poikilitic olivine of NWA 7721 ›
Thermodynamic blocking in self-gravitating systems ›
A warm ultra-luminous infrared galaxy just 600 million years after the Big Bang ›
Effect of gravity darkening and oblate factor in rapidly rotating massive stars ›
Revisiting the Possibility of a Sharp Phase Transition in Cold Neutron Stars ›
WFC3/IR Starter Guide ›
Galactification: painting galaxies onto dark matter only simulations using a transformer-based model ›
Isolated massive star candidates in NGC 4242 with GULP ›
HARPS-N, TESS, and CHEOPS discover a transiting sub-Neptune and two outer companions around the bright solar analogue HD 85426 ›
Supermassive Dark Stars and their remnants as a possible solution to three recent cosmic dawn puzzles ›
Stellar cycle variability in Mount Wilson stars and dynamo models: Rotation rate and dynamo number dependency ›
Accelerated inference of microlensed gravitational waves with machine learning ›
A Simple Ray Acceleration Structure for Non-LTE Radiative Transfer ›
Lunar Dust: Formation, Microphysics, and Transport ›
Growth of Metal-Enriched Supermassive Stars by Accretion and Collisions ›
A Novel Parameterization for Rapid Cooling in Supernova Remnants, with applications to the Pa 30 nebula ›
Dark winds on the horizon: Prospects for detecting neutrino and hot dark matter wakes in large-scale structure ›
Early Formation of Supermassive Black Holes via Dark Star Gravitational Instability ›
Exploring the Impact of Systematic Bias in Type Ia Supernova Cosmology Across Diverse Dark Energy Parametrizations ›
Dark Secrets of Baryons: Illuminating Dark Matter-Baryon Interactions with JWST ›
The future ability to test theories of gravity with black-hole shadows ›
Galactic magnetic fields seeded by ultralight dark photons ›
Tests of General Relativity with Einstein Telescope ›
Latest results from CUORE and prospects for CUPID ›
Detecting Parity-Violating Gravitational Wave Backgrounds with Pulsar Polarization Arrays ›
Gravitational-wave dispersion over inhomogeneous space-times: General relativity, screened theories of gravity and non-minimal dark energy ›
Spacecraft Angular Rate Estimation via Event-Based Camera Sensing ›
Extreme mass ratio inspirals into black holes surrounded by matter: Resonance crossings ›
Constraining modified theories of gravity through the detection of one extremely large mass-ratio inspiral ›
High Power Arbitrary RF Pulse Shaping Tests with NG-LLRF and Cool Copper Collider Prototype Structure ›
Earth-orbit bounds on screened dark energy ›
Monitoring the Solar Wind Before It Reaches L1 ›
Nonlinear Gravitational Wave Memory : Universal Low-Frequency Background ›
Metastable Strings and Gravitational Waves in One-Scale Models ›
Effect of spin in binary neutron star mergers ›
Mirage Sources and Large TeV Halo-Pulsar Offsets: Exploring the Parameter Space ›
Spectral Imaging with QUBIC: building frequency maps from Time-Ordered-Data using Bolometric Interferometry ›
Energetic Particles from Quasi-Separatrix Layers and Current Sheets at the Sun ›
Cosmology with voids from the Nancy Grace Roman Space Telescope ›
The Exoplanet Edge: Planets Don't Induce Observable TTVs with a Dominant TTV Period Faster than Half their Orbital Period ›
Probing Decaying Dark Matter Using the Post-EoR HI 21-cm signal ›
21-cm Constraints on Dark Matter Annihilation after an Early Matter-Dominated Era ›
Analysis of the Effect of Bars on Environmental Dependence of Disc Galaxies with MaNGA Survey Data ›
Late-Time Evolution of Magnetized Disks in Tidal Disruption Events ›
Tantalizing Evidence of Reionization Relics in the eBOSS DR16 Ly$\boldsymbol{\alpha}$ Forest Correlations: a Preference for Early Reionization ›
Backlighting extended gas halos around luminous red galaxies: kinematic Sunyaev-Zel'dovich effect from DESI Y1 x ACT ›
Weak-lensing tunnel voids in simulated light cones: A new pipeline to investigate modified gravity and massive neutrinos signatures ›
IAEmu: Learning Galaxy Intrinsic Alignment Correlations ›
Dynamical tides in neutron stars with first-order phase transitions: the role of the discontinuity mode ›
Redshift Drift in Relativistic N-Body Simulations ›
Caught in the act: detections of recoiling supermassive black holes from simulations ›
SN 2024aecx: A double-peaked rapidly evolving Type IIb supernova at 11 Mpc ›
Gravitational waves of quasi-circular, inspiraling black hole binaries in an ultralight vector dark-matter environment ›
Blowing star formation away in AGN Hosts (BAH) - IV: Feeding and feedback in 3C 293 observed with JWST NIRSpec ›
Attributing the point symmetric structure of core-collapse supernova remnant N132D to the jittering jets explosion mechanism ›
A theoretical prediction for the dipole in nearby distances using cosmography ›
Quantitative Morphology of Galactic Cirrus in Deep Optical Imaging ›
Structural evolution of quiescent galaxies at intermediate redshifts at UV and red rest-frame wavelengths ›
Efficient Bayesian analysis of kilonovae and gamma ray burst afterglows with fiesta ›
Propagation of Precessing Jet in Envelope of Tidal Disruption Events ›
Narrowing the discovery space of the cosmological 21-cm signal using multi-wavelength constraints ›
Detecting Gravitational Waves from Exoplanets Orbiting Binary Neutron Stars with B-DECIGO and DECIGO ›
Beyond Hierarchical Mergers: Accretion-Driven Origins of Massive, Highly Spinning Black Holes in Dense Star Clusters ›
ATLAS Photometry of Interstellar Object 3I/ATLAS ›
Tracing correlations between galaxy properties across the Cosmic Web: An IllustrisTNG-based study ›
Unified dark fluid with null sound speed as an alternative to phantom dark energy ›
Testing the Impact of Planet-stirring, Self-stirring, and Mixed-stirring on Debris Disc Architecture: A Case Study of HD 16743 ›
GravSphere2: A higher-order Jeans method for mass-modeling spherical stellar systems ›
The PICS Project: II. Circumnebular extinction variations and their effect on the planetary nebula luminosity function ›
Searching for Dark Structures: A Comparison of Weak Lensing Convergence Maps and Lensing-Weighted Galaxy Density Maps ›
Supergranulation and Poleward Migration of the Magnetic Field at High Latitudes of the Sun ›
Semianalytical Accretion-Tracer Emission: Forming Planets Are Intrinsically Faint ›
Disk fraction among free-floating planetary-mass objects in Upper Scorpius ›
Insights into Planet Formation from the Ages, Masses, and Elemental Abundances of Host Stars ›
Detection of Compton scattering in the jet of 3C 84 ›
Direct multi-model dark-matter search with gravitational-wave interferometers using data from the first part of the fourth LIGO-Virgo-KAGRA observing run ›
Reliable Parameter Inference for the Epoch of Reionization using Balanced Neural Ratio Estimation ›
ALMA and JWST Imaging of $z\ >\ 6$ Quasars: No Spatial Position Offset Observed Between Quasars and Their Host Galaxies ›
Origin and Evolution of the $\Omega$ Structure in the Head-Tail Radio Galaxy of Abell 3322 ›
Using ML-based Regression Techniques to Mitigate GOES Energetic Proton Flux Data Contamination and Magnetospheric Effects ›
Recoil-Enabled Energy Transfer from Coherent Neutrino Scattering in Core-Collapse Supernovae ›
The Triple System V1371 Tau: An Eclipsing Binary with an Outer Be Star ›
LRPayne: Stellar parameters and abundances from low-resolution spectra ›
Cosmological Singularity and Power-Law Solutions in Modified Gravity ›
K-Contact Distance for Noisy Nonhomogeneous Spatial Point Data with application to Repeating Fast Radio Burst sources ›
Neutrinophilic Super-Resonant Dark Matter ›
No Hiding in the Dark: Cosmological Bounds on Heavy Neutral Leptons with Dark Decay Channels ›
MaxWave: Rapid Maximum Likelihood Wavelet Reconstruction of Non-Gaussian features in Gravitational Wave Data ›
Self-resonant dark matter with $Z_4$ gauged symmetry ›
Bayesian Analysis of the Neutron Star Equation of State and Model Comparison: Insights from PSR J0437+4715, PSR J0614+3329, and Other Multi-Physics Data ›
Optomechanical Accelerometer Search for Ultralight Dark Matter ›
Asymptotic Schwarzschild solutions in $f(R)$ gravity and their observable effects on the photon sphere of black holes ›
Radiative Correction from Secret Neutrino Interactions and Implications for Neutrino-Scattering Experiments ›
Warped Dimensions at the Cosmological Collider ›
Nearly forgotten results in development of physical cosmology ↓↑