Obserwatorium Astronomiczne na Suhorze Strona główna
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ul. Podchorążych 2, 30-084 Kraków. tel.: (+48 12) 662 6301; fax: (+48 12) 637 2243; Obs. tel.: (+48) 502 113714
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Obserwatorium Astronomiczne na Suhorze

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Księżyc

 Wiadomości z astronet.pl
› Opublikowano pierwsze zdjęcia z Obserwatorium im. Very Rubin
› Polski astronauta: Sławosz Uznański-Wiśniewski i misja Ax-4
› Podstawowa korekcja tła w Pixinsight – Pixinsight cz. III
› Nasz galaktyczny sąsiad może skrywać supermasywną czarną dziurę
› Niebo w czerwcu 2025 roku
› Kolejna porażka firmy ispace. Lądownik Resilience rozbity na Księżycu
› Relacja z Seminarium Wiosennego w Bielsku-Białej 2025
› Tajemnicze obiekty międzygwiezdne zawierają materię organiczną
› Odkrywanie egzoplanet za pomocą mikrosoczewkowania grawitacyjnego – wywiad z Dr Radosławem Poleskim
› Mgławica planetarna NGC 1514 w obiektywie teleskopu Jamesa Webba
RSS  Najnowsze prace na astro-ph:
› Hybrid-chimes: A model for radiative cooling and the abundances of ions and molecules in simulations of galaxy formation
› A general relativistic magnetohydrodynamics extension to mesh-less schemes in the code GIZMO
› Novel $z\sim~10$ auroral line measurements extend the gradual offset of the FMR deep into the first Gyr of cosmic time
› Cancellation of one-loop correction to soft tensor power spectrum
› Super-Eddington Growth Ceiling: Analytic Constraints on the Rapid Growth of Light-Seed Black Holes in Massive Clumps
› Modeling Targets and Optimal Frequencies for Imaging the Shadows of Nearby Supermassive Black Holes
› How invisible stellar halos bias our understanding of ultra-faint galaxies
› Synthesizer: Synthetic Observables For Modern Astronomy
› Weak Bursts on Slowly Accreting Neutron Stars
› Laboratory Investigation of CO2-Driven Enhancement of Radiolytic H2O2 on Europa and Other Icy Moons
› No Clear Correlation between X-ray Spectral Properties and Polarization for High Synchrotron Peaked Blazars
› HI asymmetries in spatially resolved SIMBA galaxies
› IIb or not IIb: A Catalog of ZTF Kilonova Imposters
› Background Measurements and Simulations of the ComPair Balloon Flight
› Systematic non-thermal velocity increase preceding soft X-ray flare onset
› High resolution radio observations of the Chamaeleon star-forming region
› Coriolis force acting on near-surface horizontal flows during simulations of flux emergence produces a tilt angle consistent with Joy's law on the Sun
› Estimating Fe and Mg Abundances in the Milky Way Dwarf Galaxies Using Subaru/HSC and DEIMOS
› Direct Inference of Nuclear Equation-of-State Parameters from Gravitational-Wave Observations
› The investigation of 84 TESS totally eclipsing contact binaries
› Detailed analysis of multi-line molecular distributions in the Seyfert galaxy NGC 1068: Possible effect of the AGN outflow to the starburst ring
› The Impact of $\Omega_{m0}$ Prior Bias on Cosmological Parameter Estimation: Reconciling DESI DR2 BAO and Pantheon+ SNe Data Combination Results
› Calibrating the photometric performance of a high-time-resolution photon-counting imager for optical astronomy
› The Modeling Landscape of Extragalactic CO in CMB Surveys
› Longtime Monitoring of TeV Radio Galaxies with HAWC
› Testing Light Unaffiliated Mass Clumps in MACS 0416 on galaxy and galaxy cluster scales using JWST
› A Dichotomy of the Mass-Metallicity Relation of Exoplanetary Atmospheres Demarcated by their Birthplace
› (Re)-Defining Planets -- the Fundamental Plane of Planets
› A Massive Yellow Supergiant in the Far Outer Disk of M31: Evidence for In Situ Massive Star Formation Beyond the Optical Radius
› Identifying Ring Galaxies in DESI Legacy Imaging Surveys Using Machine Learning Methods
› BLADE: An Automated Framework for Classifying Light Curves from the Center for Near-Earth Object Studies (CNEOS) Fireball Database
› CNN-Derived Elemental Abundances of LAMOST DR10 Giants: Implications for Galactic Substructures
› Radio Galaxy Zoo: EMU -- paving the way for EMU cataloging using AI and citizen science
› Measurements of the z=4-10 X-ray Luminosity Function: the high space density of moderate-luminosity, obscured AGN
› Progenitor Insights of Type IIP SN 2018pq: A Comprehensive Photometric and Spectroscopic Study
› Broadband Low-Resolution Spectrograph -- SpectrumMate LR
› Comprehensively Constraining Ultra-Light Primordial Black Holes Through Relic Formation and Early Mergers
› Evidence for a steeper SMBH-Bulge mass relationship extended to low masses using TDE host galaxies
› Constraining the Extragalactic Magnetic Field: Auger Data Meet UHECR Propagation Modeling
› Solar Transient Recognition Using Deep Learning (STRUDL) for heliospheric imager data
› X-ray and Radio Analysis of Abell 1644: Constraints on Cluster Dynamics
› Osiris revisited: Confirming a solar metallicity and low C/O in HD 209458b
› Can AI Dream of Unseen Galaxies? Conditional Diffusion Model for Galaxy Morphology Augmentation
› Cosmic-ray and Interstellar Gas Properties in the Solar Neighborhood Revealed by Diffuse Gamma Rays
› Category-based Galaxy Image Generation via Diffusion Models
› Exploring the Frontiers of Cosmic Ray Physics: Perspectives on GRANDProto300 and the GRAND Project
› The Radio Spectral Energy Distribution and Star Formation Calibration in MIGHTEE-COSMOS Highly Star-Forming Galaxies at 1.5 < z < 3.5
› Tracing Dark Matter in the Central Regions of Galaxy Clusters Using Galaxies, Gas, and Intracluster Light in TNG300: Connections to Cluster Dynamical State
› Investigating Transit Timing Variations in the Ultra-short Period Exoplanet WASP-19b
› Possibilities for SETI at High Energy
› How the spin-phase variability of cyclotron lines shapes the pulsed fraction spectra: insights from 4U 1538-52
› Stabilizing simulation-based cosmological Fisher forecasts: a case study using the Voronoi volume function
› Going beyond $S_8$: fast inference of the matter power spectrum from weak-lensing surveys
› A Bimodal Metallicity Distribution Function in the Ultra-Faint Dwarf Galaxy Reticulum II
› SO emission in the dynamically perturbed protoplanetary disks around CQ Tau and MWC 758
› Taking a Break at Cosmic Noon: Continuum-selected Low-mass Galaxies Require Long Burst Cycles
› Disentangling Metallicity Effects in Hot Jupiter Occurrence Across Galactic Birth Radius and Phase-Space Density
› Galactic echoes
› 10,000 Resolved Triples from Gaia: Empirical Constraints on Triple Star Populations
› Star Formation and Magnetic Field Amplification due to Galactic Spirals
› Primordial magnetic fields and modified recombination histories
› Insights gained from the Light Echo of Cepheus A HW2
› Three-component Phase Separation for Ultramassive White Dwarf Models
› Realistic consecutive galaxy mergers form eccentric PTA sources
› Preconditioning of the interplanetary medium due to isolated ICMEs
› Black holes as telescopes: Discovering supermassive binaries through quasi-periodic lensed starlight
› The PGPUC horizontal branch evolutionary tracks
› Early Planet Formation in Embedded Disks (eDisk) XVII: A Compact but Structured Keplerian Disk and Large-scale Streamers Revealed in the Class I Protostellar System IRAS 04169+2702
› Project AMIGA: The Inner Circumgalactic Medium of Andromeda from Thick Disk to Halo
› Analysis of shape and angular orientation parameters of velocity-dependent dark matter annihilation signals in Galactic Centers for FIRE simulations
› Exoplanet Classification through Vision Transformers with Temporal Image Analysis
› Modeling the position and velocity distribution of space objects by maximizing entropy with energy constraint
› Analytical weak-lensing shear response of galaxy model fitting
› Shockingly Effective: Cluster Winds as Engines of Feedback in Starburst Galaxy VV 114
› An unusual type-I X-ray burst from the neutron star X-ray binary IGR J17591-2342: a double-photospheric-radius-expansion burst?
› Coevolution of Intracluster Light and Brightest Cluster Galaxies
› High-resolution APEX/LAsMA $^{12}$CO and $^{13}$CO (3-2) observation of the G333 giant molecular cloud complex : III. Decomposition of molecular clouds into multi-scale hub-filament structures
› Observational Space Unveils Cosmic Expansion's Role in the Hubble Tension
› The Vela pulsar and its pulsar wind nebula Vela-X using 13 years of Fermi-LAT Observations
› High-Speed Boulders and the Debris Field in DART Ejecta
› Expansion Signatures in 35 HII Regions traced by SOFIA [CII] Emission
› Catastrophic Formation of Macro-Scale Flow and Magnetic Fields in the Relativistic Gas of Binary Systems
› The Indian Pulsar Timing Array Data Release 2: I. Dataset and Timing Analysis
› The nanoscale molecular chemistry of outer solar system organic matter in asteroid Ryugu
› Transformers for Stratified Spectropolarimetric Inversion: Proof of Concept
› Electromagnetic radiation by turbulent, magnetized and randomly inhomogeneous solar radio sources generated by electron beams
› The first phase of mass transfer in low-mass binaries: neither stable nor a common envelope
› CosmoGLINT: Cosmological Generative Model for Line Intensity Mapping with Transformer
› On the evolution of the mass density profile of dense molecular clouds
› COSMIC-L: A Photometric Catalog of Observed Stars in the Large MagellanIc Cloud
› Navigating AGN variability with self-organizing maps
› Infalling Ultra Faint Dwarfs as Emissaries of the Axiverse?
› Global magnetohydrodynamic simulations of the inner regions of protoplanetary discs. I. Zero-net flux regime
› Feasibility of interferometric observations and characterization of planet-induced structures at sub au to au scales in protoplanetary disks
› Magnetic braking and dynamo evolution of $\beta$ Hydri
› Exploring MAXI J1744-294: IXPE insights into a Newly Discovered X-ray Transient
› Super-Earth formation in systems with cold giants
› GW200208_222617 as an eccentric black-hole binary merger: properties and astrophysical implications
› Frequently Used References For Atomic Data In X-ray Spectroscopy
› Real-time Broadband RFI Excision for the Upgraded GMRT
› SRG/eROSITA No. 5: Discovery of quasi-periodic eruptions every ~3.7 days from a galaxy at z>0.1
› The Average Soft X-ray Spectra of eROSITA Active Galactic Nuclei
› Bias hardened estimators of patchy screening profiles
› Impact of the large-scale cosmic web on the X-ray emitting circumgalactic medium
› Testing the Quantum Equivalence Principle with Gravitational Waves
› Possible evidences for physics beyond $\Lambda$CDM from DESI DR2 data
› Smooth hybrid inflation in light of ACT DR6 data
› Impact of Detector Calibration Accuracy on Black Hole Spectroscopy
› FLARE: FCCee b2Luigi Automated Reconstruction And Event processing
› Observational Constraints on Scalar Field--Matter Interaction in Weyl Integrable Spacetime
› Signatures to help interpretability of anomalies
› Possible Standard Model solution for Baryon Asymmetry
› Primordial magnetogenesis from a supercooled dynamical electroweak phase transition
› One Membrane to Love them all: Tidal deformations of compact objects from the membrane paradigm
› Neutrino Telescope Event Classification on Quantum Computers
› Chiral Invariant Mass Constraints from HESS J1731 347 in an Extended Parity Doublet Model with Isovector Scalar Meson
› Impact of $\Xi$-Hypernuclear Constraints on Relativistic Equation of States and Properties of Hyperon Stars
› Low-Energy Supernova Constraints on Lepton Flavor Violating Axions
› Shadow in the Galactic Center: Theoretical Concept -- Prediction -- Realization
› Dynamical Horizons and Black Hole Soft Hair
› Search for the in-situ production of $^{77}$Ge in the GERDA neutrinoless double-beta decay experiment
› Cosmology of Cubic Poincar\'e Gauge gravity
› Gaseous Dynamical Friction: a Numerical Study of Extended Perturbers
› GRB 221009A: Spectral signatures based on ALPs candidates
› Chemical Evolution in Nuclear Stellar Discs
› Observing the launch of an Eddington wind in the luminous Seyfert galaxy PG1211+143
› Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework
› A new "temperature inversion" estimator to detect CMB patchy screening by large-scale structure
› Towards multi-messenger observations of core-collapse supernovae harbouring choked jets
› On the minimum number of radiation field parameters to specify gas cooling and heating functions
› Simulating intermediate black hole mass measurements for a sample of galaxies with nuclear star clusters using ELT/HARMONI high spatial resolution integral-field stellar kinematics
› Diverse dark matter haloes in Two-field Fuzzy Dark Matter
› Primordial Black Holes in the Solar System
› Properties of the Lower Segment of M31's North West Stream
› One Stream or Two -- Exploring Andromeda's North West Stream
› The Influence of Muons, Pions, and Trapped Neutrinos on Neutron Star Mergers
› Magnetogram-matching Biot-Savart Law and Decomposition of Vector Magnetograms
› A theoretical investigation of far-infrared fine structure lines at $z>6$ and of the origin of the [OIII]88/[CII]158 enhancement
› Understanding Stellar Mass-Metallicity and Size Relations in Simulated Ultra-Faint Dwarf Galaxies
› Window convolution of the galaxy clustering bispectrum
› A Sound Horizon-Free Measurement of $H_0$ in DESI 2024
› Search for transient gamma-ray emission from magnetar flares using Fermi-LAT
› Spectral signatures of young radio galaxies
› Spectroscopic and X-ray Modeling of the Strong Lensing Galaxy Cluster MACS J0138.0-2155
› Microwave scattering by rough polyhedral particles on a surface
› On the Use of WGANs for Super-Resolution in Dark-Matter Simulations
› Simulations of the accreted stellar halos of low-mass field galaxies
› A theoretical approach to density-split clustering
› In search for the Local Universe dynamical homogeneity scale with CF4++ peculiar velocities
› Pattern and Origin for the Extreme $\gamma$-ray Flares of 3C 454.3 and 3C 279: An Astrophysical Critical Damper?
› The THESAN-ZOOM project: Population III star formation continues until the end of reionization
› Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows
› Cygnus X-3 as semi-hidden PeVatron
› An Early Look at the Performance of IGRINS-2 at Gemini-North with Application to the ultrahot Jupiter, WASP-33 b
› Measuring Scaling Relationships: Fitting Technique Matters
› Prompt stellar and binary black hole mergers in tight triples: Insights from chemically homogeneous evolution
› Massive black hole formation in Population III star clusters
› Chorus: Optimizing Synchrotron Transfer Coefficients with Weighted Sums
› Monte Carlo evaluations of gamma-ray and radio pulsar populations
› Dielectronic recombination studies of ions relevant to kilonovae and non-LTE plasma
› A Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays
› Exoplaneteers Keep Calling Plots "Allan Variance" Plots When They Aren't
› Supermassive Binaries in Ultralight Dark Matter Solitons
› Effects of transient stellar emissions on planetary climates of tidally-locked exo-earths
› The Formation of Double Hot Jupiter Systems through von Zeipel-Lidov-Kozai Migration
› The competing effects of recent and long-term star formation histories on oxygen, nitrogen, and stellar metallicities
› Exoplaneteers Keep Overestimating Sigma Significances
› Observational Insights on DBI K-essence Models Using Machine Learning and Bayesian Analysis
› Study of Venera Spacecraft Trajectories and Wider Implications
› Imaging systematics induced by galaxy sub-sample fluctuation: new systematics at second order
› Average solar active region: I. Intensities, velocities, and the photospheric magnetic field
› Data from FAST and MeerKAT surveys as a test of radio pulsar physics
› Leo I: the classical dwarf spheroidal galaxy with the highest dark-matter density
› The ejection and detectability of high- and hyper-velocity stars by compact object binaries in globular clusters
› Cosmological Remapping for Efficient Generation of 21 cm Intensity Mapping Mocks
› Gamma rays as a signature of r-process producing supernovae: remnants and future Galactic explosions
› Evolutionary models for the Very Massive Stars in the R136 cluster of 30 Doradus in the Large Magellanic Cloud
› Eccentricity evolution of spinning binaries and its dependence on the equation of state of the components
› Mysterious anomalies in Earth's atmosphere and strongly interacting Dark Matter
› Testing Strong Gravitational Lensing Effects of Supermassive Black Holes with String-Inspired Metric: Observational Signatures and EHT Constraints
› Non-conservation of Lepton Numbers in the Neutrino Sector Could Change the Prospects for Core Collapse Supernova Explosions
› Kinematic censorship and high energy particle collisions in the Schwarzschild background
› Finite parts of inflationary loops
› Massive graviton dark matter searches with long-baseline atom interferometers
› Neutrinos as background and signal in searches using the Migdal effect
› Double Exponents in $SL(2,\mathbb{Z})$ Cosmology
› Astrophysical Black holes: An Explanation for the Galaxy Quenching
› Dynamical dark energy from an ultralight axion
› Two or three things particle physicists (mis)understand about (pre)heating
› Fractional attractors in light of the latest ACT observations
› Precision mass measurements around ${}^{84}$Mo rule out ZrNb cycle formation in the rapid proton-capture process at type I X-ray bursts
› Hot Holographic 2-flavor Quark Star
› Quantum-enabled optical large-baseline interferometry: applications, protocols and feasibility
› Applying TDI to Hardware-Simulated Data
› Black hole photon ring beyond General Relativity: an integrable parametrization
› Enhancing Taiji's Parameter Estimation under Non-Stationarity: a Time-Frequency Domain Framework for Galactic Binaries and Instrumental Noises

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