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The Fornax3D project: Assembly histories of lenticular galaxies from a combined dynamical and population orbital analysis |
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A nearby transiting rocky exoplanet that is suitable for atmospheric investigation |
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Forbidden hugs in pandemic times. II. The luminous red nova variety: AT 2020hat and AT 2020kog |
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Carbon dust in the evolved born-again planetary nebulae A 30 and A 78 |
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Thermally altered subsurface material of asteroid (162173) Ryugu |
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The infrared-radio correlation of star-forming galaxies is strongly M<SUB>⋆</SUB>-dependent but nearly redshift-invariant since z ∼ 4 |
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Solo dwarfs II: the stellar structure of isolated Local Group dwarf galaxies |
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Concepts for future missions to search for technosignatures |
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A tidally tilted sectoral dipole pulsation mode in the eclipsing binary TIC 63328020 |
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Euclid preparation. XI. Mean redshift determination from galaxy redshift probabilities for cosmic shear tomography |
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The Effects of Three-dimensional Radiative Transfer on the Resonance Polarization of the Ca I 4227 Å Line |
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The Star Formation History of Eridanus II: On the Role of Supernova Feedback in the Quenching of Ultrafaint Dwarf Galaxies |
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Understanding the evolution and dust formation of carbon stars in the Large Magellanic Cloud via the JWST |
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The Atacama Cosmology Telescope: A Catalog of >4000 Sunyaev–Zel’dovich Galaxy Clusters |
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The WaZP galaxy cluster sample of the dark energy survey year 1 |
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The number of globular clusters around the iconic UDG DF44 is as expected for dwarf galaxies |
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HARMONI: the ELT's First-Light Near-infrared and Visible Integral Field Spectrograph |
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HIRES, the High-resolution Spectrograph for the ELT |
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Evidence that short-period AM CVn systems are diverse in outburst behaviour |
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TIC 168789840: A Sextuply Eclipsing Sextuple Star System |
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The atmosphere of HD 209458b seen with ESPRESSO. No detectable planetary absorptions at high resolution |
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Interstellar Extinction, Polarization, and Grain Alignment in the Sh 2-185 (IC 59 and IC 63) Region |
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Magnetoacoustic wave energy dissipation in the atmosphere of solar pores |
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CHEOPS observations of the HD 108236 planetary system: a fifth planet, improved ephemerides, and planetary radii |
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