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Obserwatorium Astronomiczne na Suhorze

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Kamerka N

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Temperatura
2.9 °C
Wilgotność
89%
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0.0 km/h
Ciśnienie
997.3 hPa

Księżyc
Najnowsze prace na astro-ph:
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Calibration-independent consistency test of BAO and SNIa data: update ›
Evolutions of mean distance ratios in the planetary and satellite systems under primary tides and nebular gas drag effects ›
Comprehensive Gaia DR3-Based Astrometric, Photometric, and Kinematic Studies of the Binary Open Cluster $h$ and $\chi$ Persei ›
Accretion Rate Changes Detected in a Polluted White Dwarf ›
Assessing the Vera Rubin Observatory's Ability to Discover Asteroid Impactors Before They Collide with Earth ›
A shot in the dark: searching for dark substructures in the RX J0437+00 galaxy cluster ›
TORRCH: Tomographic reconstruction of the reionization of cosmic hydrogen with Ly${\alpha}$ emitters and non-Ly${\alpha}$-selected galaxies ›
A Binary-Based Reassessment of the Age and Stellar Properties of NGC 7789 Using Twelve Binary Components ›
Measuring the Black Hole and Accretion Parameters of Sagittarius A* from EHT Observations using a Semi-Analytic Model ›
proto-Lightspeed: a high-speed, ultra-low read noise imager on the Magellan Clay Telescope ›
Relaxing DESI DR2 BAO Constraints on $\sum m_\nu$ with Planck and SPT-3G 2018 in the Context of SPT D1 ›
A first GLIMPSE into star clusters populations across cosmic time ›
UNCOVER/MegaScience Finds Uniform and Highly Bursty Star Formation at 3 < z < 9, consistent with the High-Redshift UV Luminosity Function ›
MeerKAT observations of Abell 1775 and Abell 1795: the discovery of a hadronic radio halo? ›
A differential-geometry approach to black hole characterization of megamaser systems in static spherically symmetric spacetimes ›
The detectability of bars at high redshift: a case study using Euclid-like mock observations of TNG50 simulated galaxies ›
Unifying cluster and galaxy cosmology analyses using the galaxy-halo connection ›
TOI-6692b: An eccentric 130 day period giant planet with a single transit from TESS ›
Hot, Retrograde Tilted MADs: Misaligned, Precessing, and Shaped by Electromagnetic Torques ›
Characterization of the commercial spectrograph system for astronomical observations: PIXIS 1300BX Camera and IsoPlane 320A Spectrograph ›
XMM-Newton observations of ten high-redshift CAMIRA clusters of galaxies ›
Bondi-Hoyle-Lyttleton accretion flow in a stratified layer ›
Unveiling a Thin Filament of the Cosmic Web in the Ursa Major Supergroup ›
Star formation outside galaxies undergoing gravitational and hydrodynamic interactions: dust attenuation and the star formation rate ›
Constraints on the Hot Circumgalactic Medium around Nearby L* Galaxies from SRG/eROSITA All Sky Survey ›
On the Use of Field RR Lyrae as Galactic Probes -- VIII. Early Formation of the Galactic Spheroid ›
Multi-wavelength Study of A Superflare on RS CVn-type Star HD22468 Triggered at Hard X-ray by SVOM ›
Simulations of multi-phase gas in and around galaxies ›
GRBAlpha, VZLUSAT-2 and GRBBeta -- GRB observations with CubeSats ›
Cosmological analysis of a viable $f(R)$ gravity model ›
Investigating Twin Star Equation of States in Light of Recent Astrophysical Observations ›
ALMA publication statistics ›
One H2 molecule per ten million H-atoms reveals sub-pc scale cold overdensities at z~4 ›
Pushchino Multibeam Pulsar Search. X. Observations of pulsars at declinations above $+53^o$ ›
When Primordial Black Holes Absorb During the Early Universe ›
Illuminating the Physics of Cosmic Origin and Evolution: A UK Space Frontiers 2035 White Paper ›
Improved measurements of the age of JWST galaxies at z=6-10 ›
[HP99] 159 -- Properties of the first Supersoft X-ray Source with a Helium star donor ›
Mercury-Ar$\chi$es: a high-performance n-body code for planet formation studies ›
Superhumps in active dwarf novae. Part I: ER Ursae Majoris ›
Magnetic threads and gravity: ALMA Observations of IRDC G14.225-0.506 ›
Flux-ratio anomalies in cusp quasars reveal dark matter beyond CDM ›
Gaia20dsk: A new MNor discovered by the GLORIOUS collaboration ›
Six New Circumbinary Disk Occultation (CBO) Candidates from the Zwicky Transient Facility ›
Kinematics of young star clusters in the outer north-eastern region of the Small Magellanic Cloud ›
The Astrosky Ecosystem: An independent online platform for science communication and social networking ›
The Origins of Planets for ArieL (OPAL) Key Science Project: the end-to-end planet formation campaign for the ESA space mission Ariel ›
Cosmography with $\Lambda$-Szekeres Models ›
Extragalactic Planetary Nebulae (xPNe). Determining Distances out to 100 Mpc and the Renaissance of the PN Luminosity Function Method ›
A more inclusive effective dark fluid equation of state parameter: constraints from SKA and Euclid like surveys ›
Dynamics of AGN feedback in the X-ray bright East and Southwest arms of M87, mapped by XRISM ›
Drawing the line between explosion and collapse in electron-capture supernovae -- I. Impact of conductive flame speeds and ignition conditions on the explosion mechanism ›
CosmoSlider: An educational tool for cosmology ›
Fast Magnetoacoustic Wave Behavior with Gravitationally Stratified, Magnetically Inhomogeneous Media ›
The shape function of the observed growth index ›
The scaling relations of galaxies with different morphology: comparison among WINGS, MANGA and Illustris data samples ›
Forecast on the generalised dark matter properties from a Euclid-like survey ›
Improving constraints on primordial non-Gaussianity from Quaia with a new cosmological observable: angular redshift fluctuations ›
Probabilistic Graphical Models in Astronomy ›
Calibrating redshift distributions at $z>2$ with Lyman-$\alpha$ forest cross-correlations ›
ReveaLLAGN 1: JWST Emission-Line Spectra Reveal Low-Luminosity AGN with UV-Deficient SEDs and Warm Molecular Gas ›
Post-Perihelion Integral Field Spectroscopy of the Interstellar Comet 3I/ATLAS ›
A compact object with a K type star companion in the solar neighborhood: a wide post common envelope binary with a white dwarf candidate ›
Probing dark matter interactions with a RES-NOVA prototype cryogenic detector ›
Searching for Ultralight Scalar Dark Matter with Clocks in Low Earth Orbit ›
Analysis of $M1$ capture in the $\alpha(d,\gamma)^6$Li reaction ›
Thick Lunar Crust Amplifies Gravitational-Wave Signal ›
Universal relation between dipole polarizability of finite nuclei and neutron-star compactness ›
Cosmic ray electron boosted light dark matter: Implications of LZ 2025 data ›
Anisotropy Strikes Back: Modified Gravity and Dark Matter Halos ›
Science Opportunities of Wet Extreme Mass-Ratio Inspirals ›
The 2.5-meter Wide Field Survey Telescope Real-time Data Processing Pipeline I: From raw data to alert distribution ›
Precision Determination of Scintillation Screen Parameters from Annual Modulation Measurement of Pulsar Scintillation Arc Curvature with the FAST Telescope ›
Inflationary attractors and radiative corrections in light of ACT data ›
Multiplicity of young isolated planetary mass objects in Taurus and Upper Scorpius ›
Eternal inflation near inflection points: a challenge to primordial black hole models ›
The role of migration traps in the formation of binary black holes in AGN disks ›
Cosmological Constraints on Neutrino Masses in a Second-Order CPL Dark Energy Model ›
21 cm forest one-dimensional power spectrum as an indirect probe of dark matter particles and primordial black holes ›
Orbit-based structural decomposition and stellar population recovery for edge-on barred galaxies ›
Probing Stellar Kinematics with the Time-Asymmetric Hanbury Brown and Twiss Effect ›
StarEmbed: Benchmarking Time Series Foundation Models on Astronomical Observations of Variable Stars ›
SCATTER Common Envelope Formalism for Triples ›
Euclid preparation: LXXXVII. Non-Gaussianity of 2-point statistics likelihood: Precise analysis of the matter power spectrum distribution ›
Photon rest mass from localized fast radio bursts with improved distribution of dispersion measure from extragalactic gas ›
JWST Confirmation of a Runaway Supermassive Black Hole via its Supersonic Bow Shock ›
Machine Learning vs. Spectral Energy Distribution Fitting: A Comparative Analysis of Accuracy in Stellar Mass Estimation ›
Sustainable, Local Socio-Economic Development Through Astronomy ›
Captured are circularized: A relativistic treatment of extreme mass ratio inspirals crossing accretion disks ›
The Characteristic Mass and Energy Conversion Efficiency in the Cusp-Core Transition of Dark Matter Haloes: Implications for Scaling Relations and Supernova feedbacks ›
One Attempt at Building an Inclusive & Accessible Hybrid Astronomy Conference: FRB 2025 ›
The FarView Low Frequency Radio Array on the Moon's Far Side: Science and Array Architecture ›
Slow and fast collective neutrino oscillations: Invariants and reciprocity ›
A Model of Dark Matter and Energy ›
GALILEO: Galactic Axion Laser Interferometer Leveraging Electro-Optics ›
LISA double white dwarf binaries as Galactic accelerometers ›
Estimating Soil Electrical Parameters in the Canadian High Arctic from Impedance Measurements of the MIST Antenna Above the Surface ›
Density perturbations in nonminimally coupled gravity: symptoms of Lagrangian density ambiguity ›
K-nonizing ›
Effects of dynamical capture on two equal-mass nonspinning black holes ›
Potential divergence in tracing $\mu$ and $\tau$ flavors of astrophysical neutrinos ›
Taxonomy of periodic orbits and gravitational waves in a deformed Schwarzschild black hole spacetime ›
GlueNN: gluing patchwise analytic solutions with neural networks ›
Exact general solutions for cosmological scalar field evolution in a vacuum-energy dominated expansion ↓↑