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Obserwatorium Astronomiczne na Suhorze

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Kamerka S

Kamerka N

Niebo
Temperatura
-4.1 °C
Wilgotność
93%
Wiatr
11.3 km/h
Ciśnienie
1007.3 hPa

Księżyc
Najnowsze prace na astro-ph:
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Machine-Learning Classification of Neutron-Star Matter Composition from Macroscopic and Oscillation Observables ›
Clustering of cosmic string loops within a Milky-way like halo ›
COBIPLANE: A Systematic Search for Compact Binary Millisecond Pulsars at Low Galactic Latitudes ›
A secondary orbiter under collisions with an accretion disk ›
A clustering-based search for substructures in the Galactic plane and bulge using RR Lyrae stars as tracers ›
The ionization structure and chemical history in isolated H ii regions of dwarf galaxies with VIMOS/IFU II. The Leo A galaxy ›
The Tianlai-WIYN North Celestial Cap Redshift Survey ›
Variation of the 2175 {\AA} extinction feature in Andromeda galaxy ›
Time-Dependent Accretion Disks with Magnetically Driven Winds: Green's Function Solutions ›
Machine-learning approaches to dispersion measure estimation for fast radio bursts ›
Atmospheric Mass Flux as a Function of Ionospheric Emission on Unmagnetized Earth ›
Antarctic TianMu Staring Observation Project I: Overview and Implementation of the Prototype Telescope ›
Antarctic TianMu Staring Observation Project II: Data reduction and preliminary results ›
SSC Radiation in the ICMART Model: Spectral Simulations and Application to the Record-Breaking GRB 221009A ›
photoD with Rubin's Data Preview 1: first stellar photometric distances and deficit of faint blue stars. Stellar distances with Rubin's DP1 ›
Evolution of Accretion Properties in Mrk 1040 using long-term X-ray Observations ›
A Seyfert galaxy as a hidden counterpart to a neutrino-associated blazar ›
Tidally Trapped Two-pole Pulsations Discovered in a Close Binary with a Massive $\beta$ Cephei Star ›
Connecting disc-corona physics and ionised outflows in AGN in the 2040s ›
Abundance Stratification in Type Iax SN 2020rea with TARDIS ›
H.E.S.S. detection and multi-wavelength study of the $z \sim$ 1 blazar PKS 0346$-$27 ›
Improved lanthanide constraints for the kilonova AT 2017gfo ›
From Nbody1 to Nbody7: the Growth of Sverres Industry ›
$S_8-H_0$ tension in a SI-ULDM scenario ›
The Likelihood of Hosting Undetected Brown Dwarfs in the Solar Vicinity ›
Self-Gravitating Scalar Field Configurations, Ultra Light Dark Matter and Galactic Scale Observations ›
Integrated Sachs-Wolfe maps from the Gower Street $w$CDM simulations ›
A millimeter methanol maser ring tracing the deceleration of the heat wave powered by the massive protostellar accretion outburst in G358.93-0.03 MM1 ›
A closer look at the young stellar group around Sh 2-295 ›
OmniCosmos: Transferring Particle Physics Knowledge Across the Cosmos ›
Turbulence-Driven Corrugation of Collisionless Fast-Magnetosonic Shocks ›
A Convolutional Neural Network for the Recovery of Transfer Functions From Velocity-Resolved Reverberation Mapping Data ›
Picture an Astronomer: Best Practices for Retaining Talent in Astrophysics ›
Nine years of UVIT: assessing sensitivity variation ›
Understanding Solar Flares and Energetic Events: Open questions, observational requirements, and instrumental needs over the coming decade ›
3D Radiative MHD Modeling of Particle Beam Heating of the Solar Atmosphere ›
The Redshifts from 122 Bands: Comparative Redshift Forecast for Low-Resolution Spectra from SPHEREx and 7-Dimensional Sky Survey (7DS) ›
Seafloor Weathering and Stochastic Outgassing Unlikely to Significantly Shorten the Future Lifespan of Earth's Terrestrial Biosphere ›
Evidence for the transition from thermal to non-thermal emission in the prompt emission of GRB 161117A ›
Inferring Solar Magnetic fields From the Polarization of the Mg II h and k Lines ›
Dust destruction in bubbles driven by multiple supernovae explosions ›
An Effective Theory for Biased Tracers via the Boltzmann-Equation Approach ›
Destruction of the interstellar dust by a supernova ›
The role of PSR J0614-3329 in defining the high-density matter at Neutron star cores ›
Coronal flux tube illuminated by strong shock spot: New Year's Eve solar eruption of 2023-Dec-31 ›
AstroReview: An LLM-driven Multi-Agent Framework for Telescope Proposal Peer Review and Refinement ›
LUNCH: A Lightweight Unified Deep-Learning Framework for General Transients Classification in High-Energy Time-Domain Astronomy ›
TTC: Transformer-based TDE Classifier for the Wide Field Survey Telescope (WFST) ›
Scalable Stellar Parameter Inference Using Python-based LASP: From CPU Optimization to GPU Acceleration ›
Resolving the Origins and Pathways of Ionizing Radiation Escape with UV Integral Field Spectroscopy ›
Cosmological dynamics and observational constraints of an interacting early scalar field coupled to radiation ›
Discovery of a galaxy associated with the HI cloud FAST J0139+4328 ›
Searching for Periodicity in FRB 20240114A ›
Cosmic Himalayas in CROCODILE : Probing the Extreme Quasar Overdensities by Count-in-Cells analysis and Nearest Neighbor Distribution ›
Multi-Frequency Study of FRB20201124A with the uGMRT ›
Distributions of wide binary stars in theory and in Gaia data: III. Orbital momenta, masses, and manifestations of MOND ›
Towards precision cosmology with Voids x CMB correlations (I): Roman-Agora mock catalogs and pipeline validation ›
Feeling Blue: Constructing a Robust SALT3 UV Template and Constraining its Redshift Dependency ›
Pair Space in Classical Mechanics III. Some Four-Body Central Configurations ›
Strongly Coupled Sectors in Inflation: Gapped Theories of Unparticles ›
Control and read-out of the HEPD-02 tracking system onboard CSES-02 satellite ›
Inflationary QCD phase diagram ›
The role of particle feedback on particle acceleration in magnetic reconnection ›
Kinematic Anisotropies in PTA Observations: Analytical Toolkit ›
Sommerfeld Enhancement from Background Force and the Galactic Center GeV Excess ›
Impact of Anisotropy on Neutron Star Structure and Curvature ›
Big Bang Nucleosynthesis results refined via the Trojan Horse Method ›
The sun as colliding beam, betatron cosmic ray factory ›
Memories of Prof. George Lazarides ›
Higgs-like inflation in scalar-torsion $f(T,\phi)$ gravity in light of ACT-SPT-DESI constraints ›
Stellar modeling within regularized 4D Einstein-Gauss-Bonnet gravity in light of current astrophysical constraints ›
Aspects of Sommerfeld Enhancement in the light of Halo gamma-ray excess ›
Difference between quark stars and neutron stars in universal relations and their effect on gravitational waves ›
Model-independent search of gravitational wave echoes in LVK data ›
Loop-Level Lepton Flavor Violation and Diphoton Signals in the Minimal Left-Right Symmetric Model ›
Primordial black hole dark matter from ultra-slow-roll inflation in Horndeski gravity ›
Effect of Magnetised Discontinuity on Diffusive Shock Acceleration ›
Observation of the $\gamma$-ray Emission from W43 with LHAASO ›
Deep view of Composite SNR CTA1 with LHAASO in $\gamma$-rays up to 300 TeV ›
RHINO: A large horn antenna for detecting the 21cm global signal ›
Ultrahigh-Energy Gamma-ray Emission Associated with Black Hole-Jet Systems ›
Unraveling the Nature of HAWC J1844-034 with Fermi-LAT Data Analysis and Multi-wavelength Modeling ›
Gravitational wave probes of particle dark matter: a review ›
NLTE spectral modelling for a carbon-oxygen and helium white-dwarf merger as a Ca-rich transient candidate ›
Study of Ultra-High-Energy Gamma-Ray Source 1LHAASO J0056+6346u and Its Possible Origins ›
Constraining Lens Masses in Moderately to Highly Magnified Microlensing Events from Gaia ›
Intermediate-mass black holes and contribution to extragalactic background light from Population III stars in Milky Way-like galaxies ›
When Dark Matter Heats Up: A Model-Independent Search for Non-Cold Behavior ›
Search for Lorentz Invariance Violation with spectral lags of GRB 190114C using profile likelihood ›
XSPECT on-board XPoSat: Calibration and First Results ›
Kinematic Confirmation of a Remarkable Linear Trail of Galaxies in the NGC 1052 Field, Consistent with Formation in a High-Speed Bullet Dwarf Collision ›
Supermassive Stars Match the Spectral Signatures of JWST's Little Red Dots ›
The superclouds of the local Milky Way ›
Growth Index in the $\gamma\delta$CDM model ›
Primordial Black Holes Evaporating before Big Bang Nucleosynthesis ›
Setting limits on blazar-boosted dark matter with xenon-based detectors ›
Explaining the Origin of TeV Gamma Rays from M87 During High and Low States ›
FITrig: A High-Performance Detection Technique for Efficient Ultra-Long-Period Pulsars ›
Closing the Evidence Gap: reddemcee, a Fast Adaptive Parallel Tempering Sampler ›
Dynamical Architectures of S-type Transiting Planets in Binaries II: A Dichotomy in Orbital Alignment of Small Planets in Close Binary Systems ›
Effects of Coronal Mass Ejection on PSR J1022+1001 and Possible Mode Change of PSR J2145-0750 in the InPTA DR2 ›
An alternative theory of magnetic flux tubes in strong fields via axion origin photons ›
EMPEROR I. Exoplanet MCMC parallel tempering for RV orbit retrieval ›
A Precessing, Magnetically Dominated, Structured Jet Powering the Hour-scale Quasiperiodic GRB 250702B ›
KDP as a thermal blocking filter -- Deep near IR observations with a warm narrow band filter ›
Detection of disk-jet co-precession in a tidal disruption event ›
Cosmogenic Origin of KM3-230213A: Delayed Gamma-Ray Emission from A Cosmic-Ray Transient ›
Constraining the Properties of GRB Accreting Magnetar with $R/I$ Evolutionary Effects Using \emph{Swift}/XRT Data ›
Radio Detection of a Local Little Red Dot ›
The Polarized X-ray Universe: Insights and Discoveries ›
Resolving dust and Ly{\alpha} emission in a lensed galaxy at the epoch of reionization with JWST/CANUCS ›
NGC 3521 as the Milky Way near twin: spectral energy distribution from UV to radio decameter ranges ›
Photometric and spectroscopic variability of the blue supergiant rho Leo ›
Decoupling perturbations from background in $f(Q)$ gravity: the square-root correction and the alleviation of the $\sigma_8$ tension ›
Long-term monitoring of repeating FRB 20220912A with the uGMRT at low radio frequencies ›
Rotation and stability of the circumnuclear gas disk in the Galactic Center potential by the ALMA CMZ Exploration Survey (ACES) ›
Ricci-Notation Tensor Framework for Model-based Approaches to Imaging ›
Baryogenesis via the Chiral Magnetic Effect in a First-Order Electroweak Phase Transition ›
Predictions on observing hot holographic quark star with gravitational waves ›
High-Frequency Thermal Graviton Remnant from the End of Inflation ›
Probing Right Handed Neutrino assisted Reheating with Gravitational Waves and Leptogenesis ›
Electromagnetic helicity flux density for radiative systems ›
Importance of relativistic pericenter precession in identifying the presence of a third body near eccentric binaries ›
Updating GUT-Scale Pole Higgs Inflation After ACT DR6 ›
On the maximum compactness of neutron stars ›
Dark Matter Capture in a Core-Collapse Supernova Revives Dark Photons ›
Net Charge Accretion in Magnetized Kerr Black Holes ›
Relativistic accretion process onto rotating black holes in Einstein-Euler-Heisenberg nonlinear electrodynamic gravity ›
Can the 3 neutrino masses really be found using SN 1987A data? ›
A mini-review on combinatorial solutions to the Marcus-Lushnikov irreversible aggregation ↓↑