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Scrutinizing evidence for the triggering of active galactic nuclei in the outskirts of massive galaxy clusters at z ≈ 1 |
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Unraveling the kinematics of IZw18: A detailed study of ionized gas with MEGARA/GTC |
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Detection of Na in the atmosphere of the hot Jupiter HAT-P-55b |
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Migration and Evolution of giant ExoPlanets (MEEP). I. Nine Newly Confirmed Hot Jupiters from the TESS Mission |
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The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ∼ 8.5–14.5 |
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Differential reddening in 48 globular clusters: An end to the quest for the intracluster medium |
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Understanding the thermal and magnetic properties of an X-class flare in the low solar atmosphere |
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A SART-Based Iterative Inversion Methodology to Infer the Solar Rotation Rate from Global Helioseismic Data |
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Trio of super-Earth candidates orbiting K-dwarf HD 48948: a new habitable zone candidate |
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The MAGPI Survey: massive slow rotator population in place by z 0.3 |
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SPT-SZ MCMF: an extension of the SPT-SZ catalogue over the DES region |
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AuriDESI: mock catalogues for the DESI Milky Way Survey |
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Luminous giants populate the dense Cosmic Web. The radio luminosity-environmental density relation for radio galaxies in action |
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TOI-837 b is a young Saturn-sized exoplanet with a massive 70 M<SUB>⊕</SUB> core |
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MUSE view of PDS 456: Kiloparsec-scale wind, extended ionized gas, and close environment |
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Impacts of Bar-driven Shear and Shocks on Star Formation |
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A universal method for solar filament detection from Hα observations using semi-supervised deep learning |
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Optical variability of the blazar 3C 371: From minute to year timescales |
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Reconnaissance ultracool spectra in the Euclid Deep Fields |
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Detailed cool star flare morphology with CHEOPS and TESS*** |
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Kepler main-sequence solar-like stars: surface rotation and magnetic-activity evolution |
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Nodal precession of a hot Jupiter transiting the edge of a late A-type star TOI-1518 |
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Recovery of the X-ray polarisation of Swift J1727.8−1613 after the soft-to-hard spectral transition |
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Evidence for very massive stars in extremely UV-bright star-forming galaxies at z ∼ 2.2-3.6 |
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Fine structure in the Sigma Orionis cluster revealed by Gaia DR3 |
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