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Obserwatorium Astronomiczne na Suhorze

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Kamerka S

Kamerka N

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Temperatura
-10.4 °C
Wilgotność
90%
Wiatr
0.0 km/h
Ciśnienie
1009.3 hPa

Księżyc
Najnowsze prace na astro-ph:
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AT2024wpp: An Extremely Luminous Fast Ultraviolet Transient Powered by Accretion onto a Black Hole ›
Fast rotations in galaxies at cosmic noon indicate central concentration of stars, dark matter or massive black holes ›
Early thin-disc assembly revealed by JWST edge-on galaxies ›
Non-thermal particle acceleration in multi-species kinetic plasmas: universal power-law distribution functions and temperature inversion in the solar corona ›
Mind the peak: improving cosmological constraints from GWTC-4.0 spectral sirens using semiparametric mass models ›
Simulation-Based Prediction of Black Hole Spectra: From $10M_\odot$ to $10^8 M_\odot$ ›
The SOL $\textit{(Solar Origin and Life)}$ Project: Detailed characterization of candidates for the ZAMS and Subgiant stages ›
Extreme-ultraviolet synthesis of nanojet-like ejections due to coalescing flux ropes ›
Multiwavelength Modeling of the Luminous Fast Blue Optical Transient AT2024wpp ›
Late-Time Infrared Cooling in Magnetar-Driven Supernovae ›
Estimation of the tidal heating in the TRAPPIST-1 planets. Influence of the internal structure ›
Integral field spectroscopy and numerical simulations of the NGC 2207/IC 2163 system ›
Simulation-Based Inference for Probabilistic Galaxy Detection and Deblending ›
MARVEL: A Multi Agent-based Research Validator and Enabler using Large Language Models ›
Time-dependent chemical evolution during cloud formation: H$_2$-regulated chemistry in diffuse molecular cloud ›
The steep redshift evolution of the hierarchical merger rate may cause the $z$-$\chi_{\rm eff}$ correlation ›
The maximum mass ratio of hierarchical mergers may cause the $q$-$\chi_{\rm eff}$ correlation ›
Jet-torus interaction revealed by sub-parsec SO absorption in NGC 1052 ›
Perhaps there is no brown dwarf desert? A study of sub-stellar companions with Gaia DR3 ›
Electron Cyclotron Maser Emission from Ejected Stellar Prominences on V374 Peg ›
Particle Acceleration and Depolarization in the Protostellar jet knots HH 80 and HH 81 ›
An Enhanced Sample of Galactic Red Supergiants Reveals Spiral Structures ›
Investigating the Center-to-Limb Effects in Helioseismic Data Using 3D Radiative Hydrodynamic Simulations ›
Protonic thermoelectric effect of Superionic H2O and magnetic field generation in Uranus and Neptune ›
Predicting dust temperature from molecular line data using machine learning ›
Characteristics of the High-frequency Humps in the Black hole X-ray Binary Swift J1727.8--1613 ›
Identification of solid N2O in interstellar ices using open JWST data ›
A Multiband Photometric Study of RR Lyrae Stars in M53 (NGC 5024) ›
The massive hot subdwarf binary LAMOST J065816.72+094343.1 ›
Modelling spacecraft-emitted electrons measured by SWA-EAS experiment on board Solar Orbiter mission ›
Disc fragmentation. II. Ejection of low mass Free Floating Planets from growing binary systems ›
Short gamma-ray burst progenitors have short delay times ›
First detection of VHE gamma-ray signal from the FSRQ TON 0599 ›
Filtering interlopers with photometry and diagnostic features: A machine learning framework validated with CSST slitless spectroscopy ›
Towards an optimal extraction of cosmological parameters from galaxy cluster surveys using convolutional neural networks ›
HST+IGRINS synergy to characterise the newly discovered metal-rich bulge globular cluster Patchick 126 ›
Science with a large field-of-view polarization survey: The Large Array Survey Telescope Polarization Node (LAST-P) ›
Polarization rotation through differential transmission in refractive CMB telescopes identified using a hybrid physical optics method ›
The uncertainty in water mass fraction of wet planets ›
Search for gamma-ray variability around Fermi-LAT pulsar glitches ›
Evidence for a Damped Millisecond Quasi-Periodic Structure in a Fast Radio Burst ›
Broadband spectroscopy of astrophysical ice analogues: IV. Optical constants of N$_2$ ice in the terahertz and mid-infrared ranges ›
Exploring the potential for ultra-relativistic jets in Scorpius X-1 with low angular resolution radio observations ›
Formation of multi-planetary systems via pebble accretion in externally photoevaporating discs in stellar clusters ›
Can Dynamic Spectrum Sharing Protect Passive Radio Sciences? ›
The Gaia All-Sky Stellar Parameters Service (GASPS) ›
Investigation of the dynamics and origin of the NEA pair 2021 PH27 and 2025 GN1 ›
Stellar-mass black holes on the millimetre fundamental plane of black hole accretion ›
HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them ›
Two-source terrestrial planet formation with a sweeping secular resonance ›
Cosmological constraints on viable $f(R)$ models using weak lensing ›
Spiral galaxies with flat radial abundance gradients at large radii ›
Dissecting the dust distribution and polarization around two B213 young stellar objects with ALMA ›
Modeling the Effect of C/O Ratio on Complex Carbon Chemistry in Cold Molecular Clouds ›
Characterizing the physical and chemical properties of the Class I protostellar system Oph-IRS 44. Binarity, infalling streamers, and accretion shocks ›
Satellite-borne {\gamma}-ray astrophysics from coherent interactions in oriented crystals ›
A census of star-formation and gas mass tracers in two lensed $z \sim 4$ dusty star-forming galaxies ›
Secular Excitation of Polar Neptune Orbits in Pure Disk-Planet Systems ›
Implications of Non-equatorial Relativistic Accretion Flows for Ultra-Fast Inflows in AGNs ›
A spectroscopically confirmed, strongly lensed, metal-poor Type II supernova at z = 5.13 ›
Radio Activity from the Rapidly Rotating T dwarf 2MASS 2228-4310 ›
GRB 180728A and SN 2018fip: the nearest high-energy cosmological gamma-ray burst with an associated supernova ›
Local simulations of common-envelope dynamical inspiral. Impact of rotation, accretion, and stratification ›
Fast frequency-domain phenomenological modeling of eccentric aligned-spin binary black holes ›
Cavity Multimodes as an Array for High-Frequency Gravitational Waves ›
Sterile Neutrino Dark Matter as a Probe of Inflationary Reheating ›
Constraining Lorentz and parity violations in gravity with multiband gravitational wave observations ›
On flying through the base of a pseudo-streamer ›
Real-time Gravitational Wave Response in Thermal Spinning fields ›
Limits on the mass of compact objects in Ho\v{r}ava-Lifshitz gravity ›
Combining simulation-based inference and universal relations for precise and accurate neutron star science ›
A constrained-transport embedded boundary method for compressible resistive magnetohydrodynamics ›
Symmetries of cosmological perturbations: The residual low multipole ambiguity ›
Properties of Magnetic Switchbacks in the Near-Sun Solar Wind ›
A framework for LISA population inference ›
Evolution of proto-neutron stars to pulsars, magnetars and central compact objects ›
Machian Gravity: Modeling Rotation Curves and Radial Acceleration in the SPARC Galaxy Sample ›
PySCo: A fast Particle-Mesh $N$-body code for modified gravity simulations in Python ›
Unveiling the nature of SN 2022jli: The first double-peaked stripped-envelope supernova showing periodic undulations and dust emission at late times ›
Measurement of Very-high-energy Diffuse Gamma-ray Emissions from the Galactic Plane with LHAASO-WCDA ›
Pulsar Polarization Array Limits on Ultralight Axion-like Dark Matter ›
Towards Galactic Archaeology with Inferred Ages of Giant Stars From Gaia Spectra ›
DESI Dark Secrets ›
The dynamical and thermodynamic effects of turbulence on the cosmic baryonic fluid ›
AliCPT Sensitivity to Cosmic Reheating ›
On the effects of radiation on mass transfer in binary stars ›
Disentangling the Halo: Joint Model for Measurements of the Kinetic Sunyaev-Zeldovich Effect and Galaxy-Galaxy Lensing ›
The dynamics of background evolution and structure formation in phase space: a semi-cosmographic reconstruction ›
The first phase of mass transfer in low-mass binaries: neither stable nor a common envelope ›
Scalar-induced gravitational waves from coherent initial states ›
Measuring the muon content of inclined air showers using AERA and the water-Cherenkov detectors of the Pierre Auger Observatory ›
Magnetized Proto-Neutron Stars: Structure and Stability ›
Convection-Driven Multi-Scale Magnetic Fields Determine the Observed Solar-Disk Gamma Rays ›
Revisiting the Radial Metallicity Gradient-Age Relation in the Milky Way's Thin and Thick Disks ›
The Open mulTiwavelength Transient Event Repository (OTTER): Infrastructure Release and Tidal Disruption Event Catalog ›
Revisiting thermodynamics at the outskirts of the Perseus cluster with Suzaku: importance of modeling the Hot Galactic gas ›
A simple, flexible method for timing cross-calibration of space missions ›
The lower mass limit for circumbinary disc fragmentation ›
Energy calibration of LHAASO-KM2A using the cosmic ray Moon shadow ›
XRISM-Subaru views of Abell 754: an off-axis, near-line-of-sight merging cluster ›
When Magnetic Field Lines Stretch, Snap, and Expand: A New Look at Solar Flares with L-maps ›
Probing cosmic isotropy with Gamma-ray bursts: A dipole and quadrupole analysis of BATSE and Fermi GBM data ›
Spatially resolved PAH$_{3.3}$ emission and stellar ages in ram pressure stripped clumps at $z\sim0.3$ ›
Upper Limits on Radio Emission from the K2-18 System ›
Analytical Solutions for Planet-Scattering Small Bodies ›
Peculiar SN Ic 2022esa: An explosion of a massive Wolf-Rayet star in a binary as a precursor to a BH-BH binary? ›
Water vapor emission at the warm cavity wall of the HD 100546 disk as revealed by ALMA ›
The impact of non-Gaussianity when searching for Primordial Black Holes with LISA ›
Shedding the envelope: JWST reveals a kiloparsec-scale [OIII]-weak Balmer shell around a z=7.64 quasar ›
VERITAS contributions to the 39th International Cosmic Ray Conference ›
Not Just Gas: How Solid-Driven Torques Shaped the Migration of the Galilean Moons ›
When the Shadow Meets Its Measure: Assessing the Feasibility of Submillimeter Black Hole Shadow Imaging in Megamaser Disk AGN ›
Physical Vetting of the Ultra-Short-Period Sub-Earth TOI 864.01 ›
CHANG-ES XXXVII. Effects of spectral aging on radio scale heights ›
Where does the simplified Stellar Contamination Model fail in Exoplanet Transmission Spectroscopy? ›
Deflection angle in the strong deflection limit for static and axisymmetric spacetimes: local curvature, matter fields, and quasinormal modes ›
Gravitational Equilibrium with Steady Flow and Relativistic Local Thermodynamics ›
The Dark Matter Diffused Supernova Neutrino Background ›
Scalar parity-odd trispectrum from gravitational Chern-Simons interaction vertices ›
Optical appearance of Schwarzschild black holes with optically thin and thick accretion disks at various inclination angles ›
Ultralight boson constraints from gravitational wave observations of spinning binary black holes ›
Illuminating Scalar Dark Matter Co-Scattering in EFT with Monophoton Signatures ›
GW200105: A detailed study of eccentricity in the neutron star-black hole binary ›
Gravitational Waves from $\textit{Type-I}$ Strings in a Neutrino Mass Model ›
Leptogenesis from Dark Matter Coannihilation ›
Exotic compact objects in Einstein-scalar-Maxwell theories ›
Photon Accelerator in Magnetized Plasma ›
Taxonomy of periodic orbits and gravitational waves in a deformed Schwarzschild black hole spacetime ↓↑