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Astronomia w Krakowie
Photo: The Orion Nebula (M42) imaged from Mt. Suhora
The Orion Nebula (M42) imaged from Mt. Suhora
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Temperature
4.3 °C

Humidity
 85%

Wind
14.5 km/h

Pressure
1017.8 hPa

Moon

Moon

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RSS  Latest preprints on astro-ph:

› TESS phase curve of ultra-hot Jupiter WASP-189 b
› Little red dot variability over a century reveals black hole envelope via a giant Einstein cross
› Predictions of the Nancy Grace Roman Space Telescope Galactic Exoplanet Survey. V. Detection Rates of Multiplanetary Systems in High Magnification Microlensing Events
› The dependence of the intracluster light fraction on galaxy cluster properties
› Keck Observations in the INfrared of Taurus and $\rho$ Oph Exoplanets And Ultracool dwarfs (KOINTREAU) I: A Planetary-Mass Companion and a Disk-Obscured Stellar Companion Discovered in Taurus
› Lagrangian versus Eulerian Methods for Toroidally-Magnetized Isothermal Disks
› GA-NIFS: A smouldering disk galaxy undergoing ordered rotation at z=4.26
› Two Step Localization Method for Electromagnetic Followup of LIGO-Virgo-KAGRA Gravitational-Wave Triggers
› Multiple outflows and delayed ejections revealed by early imaging of novae
› Multi-bandpass Photometry for Exoplanet Atmosphere Reconnaissance (MPEAR) with the Habitable Worlds Observatory (HWO) -- I. Differentiating Earth from Neptunes During Discovery
› Absorption of strong electromagnetic waves in magnetized pair plasmas
› Nuclear parameter inference with semi-agnostic priors
› On-Orbit Calibration of Danuri/PolCam. I. Geometric Calibration
› The Glow of Axion Quark Nugget Dark Matter: (IV) CMB Spectral and Anisotropy Signatures
› Ruminations Upon the Modeling of X-ray Foregrounds, Backgrounds and Faint Sources
› Spinning Primordial Black Holes and Scalar Induced Gravitational Waves from Single Field Inflation
› A Persistently Active Fast Radio Burst source Embedded in an Expanding Supernova Remnant
› Investigating Unusually Extended Main Sequence Turnoff of the Galactic Open Cluster NGC 3532
› Search for UHE gamma photons in cosmic rays by studying the geomagnetic influence on air-shower muons
› Absorption in the 21 cm Hydrogen Line at $z>10$ as a Sensitive Tool for the Construction of a Cosmological Model on Small Scales
› Is Crater II disrupting?
› Evolution of the Inner Accretion Flow in Swift J1727.8$-$1613 across Intermediate States: Insights from Broadband Spectral and Timing Analysis
› How Dark Sector Equations of State Govern Interaction Signatures
› Growth rate measurements from a joint analysis of the large-scale galaxy clustering in Fourier and configuration space
› Stellar feedback drives the baryon deficiency in low-mass galaxies
› Squared-field cross-correlation between kinetic Sunyaev-Zel'dovich effect and 21-cm intensity mapping
› Commissioning an Inexpensive Off-the-shelf Spectrograph for Radial-Velocity Studies
› First Statistical Detection of Cool Gas Outflows with JWST Towards Cosmic Dawn
› CTAO LST-1 observations of magnetar SGR 1935+2154: Deep limits on sub-second bursts and persistent tera-electronvolt emission
› Polarimetric and spectropolarimetric observations with FoReRo2: Instrument overview and standard stars monitoring
› The Ratan Active Region Patches (RARPs) Database: A New Database of Solar Active Region Radio Signatures from the RATAN-600 Telescope
› Stellar cores live long and prosper in cuspy dark matter halos
› Radial modes of pressure bumps and dips in astrophysical discs
› The X-ray/UV Connection in NGC 5548: A Rapidly Varying Corona
› Exoplanet formation inference using conditional invertible neural networks
› Multi-band ALMA Polarization Observations of BHB07-11 Reveal Aligned Dust Grains in Complex Spiral Arm Structures
› Stability of the Milky Way Satellite Galaxy Plane under the Influence of Neighbors
› SRG/eROSITA-SDSS view on the relation between X-ray and UV emission for quasars
› Most Rocky Sub-Neptunes are Molten: Mapping the Solidification Shoreline for Gas Dwarf Exoplanets
› Constraints on nDGP gravity from SPT galaxy clusters with DES and HST weak-lensing mass calibration and from Planck PR4 CMB anisotropies
› Hadronic Emissions from the Microquasar V4641 Sgr, SS433, and its implications in the Diffuse Galactic Emission
› A redshift-independent theoretical halo mass function validated with the Uchuu simulations
› A new Gaia census of OB associations within 1 kpc
› High-contrast L-band Integral Field Spectroscopy of HD 33632 Ab
› Asteroseismology of SPB stars: a comparison of forward asteroseismic modelling results from Kepler and TESS
› Differentially rotating neutron stars with dark matter cores
› Euclid Quick Data Release (Q1). From simulations to sky: Advancing machine-learning lens detection with real Euclid data
› Learning the Cosmic Web: Graph-based Classification of Simulated Galaxies by their Dark Matter Environments
› ALMAGAL VI. The spatial distribution of dense cores during the evolution of cluster-forming massive clump
› Transformation of orientation and rotation angles of synchronous satellites: Application to the Galilean moons
› Removing correlated noise stripes from the Nancy Grace Roman Space Telescope survey images
› Relationship between the $\gamma-$ray variability and the pc-scale jet in the blazar 3C 454.3
› Readout noise of digital frequency multiplexed TES detectors for CUPID
› Thermal Damping of Mass-Modulating Scalars
› Black-hole ringdown with templates capturing spin precession: a critical re-analysis of GW190521
› Illuminating sequential freeze-in dark matter with dark photon signal at the CERN SHiP experiment
› Gauge-independent treatment of electroweak phase transition
› Machine and Deep Learning Regression for Compact Object Equations of State
› Inelastic Majorana Dark Matter and Its Self-Interactions in a Gauged $U(1)_{L_\mu - L_\tau}$ Model
› Constraining r-process nucleosynthesis via enhanced accuracy neutron-capture experiments
› The galactic tooth-fairy and a cosmic bullet: Amateur discoveries and a call for further research
› AGN -- host galaxy photometric decomposition using a fast, accurate and precise deep learning approach
› Intrinsic non-Gaussianity of ultra slow-roll inflation
› Probing cosmic isotropy: Hubble constant and matter density large-angle variations with the Pantheon+SH0ES data
› Model-Independent Dark Energy Measurements from DESI DR2 and Planck 2015 Data
› Global Kinetic Simulations of Monster Shocks and Their Emission
› Dark Energy Survey Year 3 results: $w$CDM cosmology from simulation-based inference with persistent homology on the sphere
› The OATMEAL Survey. II. The 3D spin-orbit obliquity of an eccentric transiting brown dwarf in the Ruprecht 147 open cluster
› MUSE-DARK-I: Dark matter halo properties of intermediate-z star-forming galaxies
› Microquasar jet-cocoon systems as PeVatrons
› Cosmic Dipoles from Large-Scale Structure Surveys
› Atomic hydrogen reservoirs in quiescent galaxies at z = 0.4
› Biased Domain Walls and the Origin of Early Massive Structures
› From Wide Triples to UCXBs: Multimessenger Signatures of Dynamically-formed Black Hole-White Dwarf Systems in the LISA Band
› A catalog to unite them all: REGALADE, a revised galaxy compilation for the advanced detector era
› Magnetic fields in galactic environments probed by Fast Radio Bursts
› Recovering unbiased CMB polarization maps using modern ground-based experiments with minimal assumptions about atmospheric emission
› The lower mass limit for circumbinary disc fragmentation
› Vz-GAL: Probing Cold Molecular Gas in Dusty Star-forming Galaxies at z=1-6
› The warm outer layer of a Little Red Dot as the source of [Fe II] and collisional Balmer lines with scattering wings
› Strong-lensing rates of massive black hole binaries in LISA
› The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction
› Built-in precision: Improving cluster cosmology through the self-calibration of a galaxy cluster sample
› Mode Composition Shapes Magnetic Anisotropy in Solar Wind Turbulence
› Redshift-Frame Systematics and Their Impact on the Hubble Constant from Pantheon+ Supernovae
› Stellar cycle variability in Mount Wilson stars and dynamo models: Rotation rate and dynamo number dependency
› DESI-Like Hubble Expansion From Staged Symmetry Breaking
› Scalable and Robust Multiband Modeling of AGN Light Curves in Rubin-LSST
› Interferometric view into RT Pav's long secondary period. binary vs oscillatory convective modes
› Sulfur-Bearing Cyclic Hydrocarbons in Space
› A Catalogue of Interstellar Material Delivery From Nearby Debris Disks
› Building a Radio AGN Sample from Cosmic Morning -- The Radio High-Redshift Quasar Catalog (RHzQCat): I. Catalog from SDSS Quasars and Radio Surveys at $z > 3$
› Black-hole evaporation for cosmological observers
› Gauge hierarchy and metastability from Higgs-driven crunching
› Exploratory study on the masses of odd-$Z$ nuclei and $r$-process simulation based on the deformed relativistic Hartree-Bogoliubov theory in continuum
› Null energy condition violation and beyond Horndeski physics in light of DESI DR2 data
› Turbulence and Magnetic Reconnection in Relativistic Multispecies Plasmas
› Electrostatic waves in astrophysical Druyvesteyn plasmas: I. Langmuir waves
› A Limit on the Total Lepton Number in the Universe from BBN and the CMB
› Search for planetary-mass ultra-compact binaries using data from the first part of the LIGO--Virgo--KAGRA fourth observing run

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