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Systematic analysis of jellyfish galaxy candidates in Fornax, Antlia, and Hydra from the S-PLUS survey: a self-supervised visual identification aid |
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Bayesian inference methodology to characterize the dust emissivity at far-infrared and submillimeter frequencies |
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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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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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Reconnaissance ultracool spectra in the Euclid Deep Fields |
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Kepler main-sequence solar-like stars: surface rotation and magnetic-activity evolution |
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The effects of environment on galaxies' dynamical structures: From simulations to observations |
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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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On the Pair-instability Supernova Origin of J1010+2358 |
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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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Small-scale magnetic flux emergence preceding a chain of energetic solar atmospheric events |
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2023 DZ2 Planetary Defense Campaign |
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KMT-2023-BLG-1431Lb: A New q < 10<SUP>‑4</SUP> Microlensing Planet from a Subtle Signature |
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Baryonic properties of nearby galaxies across the stellar-to-total dynamical mass relation |
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