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- Unveiling the hot interstellar medium in nearby galaxies with eROSITA
- The compact jets of the black hole X-ray binary Swift J1753.5-0127 during its 2023-2024 outburst
- The origin of the high heavy-element content of warm Jupiters
- The GAPS Programme at TNG. LXXX. Characterisation of the 400 Myr old multi-planet system K2-233
- Extending the theory of figures to cylindrical rotation: Implications for Saturn’s interior
- Formation dynamics of a rotating solar spicule-like event and associated energy-mass transport
- Magnetic-field constraints for four magnetic cataclysmic variables from simultaneous continuum and cyclotron modeling
- Electric charge modifies the far-infrared and millimetre opacity of cosmic dust grains
- A breath of fresh air: Oxygen enhancement from silicate sublimation during early protostellar evolution
- Sub-arcsecond imaging of HCN and CN in the Orion Bar. UV-driven warm nitrogen chemistry in dense environments
- Detailed study of HD 219134: A benchmark K dwarf with a compact planetary system
- Delving into the depths of NGC 3783 with XRISM. VI. Evidence for a failed wind based on Fe XXV absorption line variability
- Toward Bayesian photometric cosmic chronometers: Application to VIPERS
- Cluster Ages to Reconstruct the Milky Way Assembly (CARMA). VI. The age-metallicity relation of in situ clusters and the age of the Universe
- Accuracy of electric current inference assuming three-dimensional hydrostatic equilibrium
- LIGHTS: Limitations of far-infrared tracers for Galactic cirrus mitigation in the era of ultra-deep imaging
- MUSE-ALMA Haloes. XVI. A census of the condensed baryons in z~0.5 HI absorption-selected galaxies
- A consistent, physical, and analytical model for cosmic microwave background observables of reionisation. I. Derivation, constraining power, and detectability of the auto spectra
- High-resolution transmission spectroscopy of KELT-18b. Metastable helium detection at 1083 nm
- Dynamical and thermal evolution of localized reconnecting current sheets under varying guide fields in the solar corona
- High-frequency subsurface-penetrating radar investigation of the shallow subsurface at the Zhurong landing site
- Pinpointing the cosmic web between massive galaxy clusters. I. The incidence of H i and O vi as WHIM tracers
- Circumbinary discs as the origin of circumstellar material around interacting H-poor supernovae and fast blue optical transients
- Euclid: Galaxy cluster detection through the weak lensing effect: Algorithm assessment and selection
- Revisiting the Einstein Cross with X-shooter spectra: New estimates of accretion disk parameters and broad emission line profiles from microlensing