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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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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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Dark energy survey year 1 results: Constraining baryonic physics in the Universe |
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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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Properties of Heavy Secondary Fluorine Cosmic Rays: Results from the Alpha Magnetic Spectrometer |
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HARMONI: the ELT's First-Light Near-infrared and Visible Integral Field Spectrograph |
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CO Excitation, Molecular Gas Density, and Interstellar Radiation Field in Local and High-redshift Galaxies |
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The interstellar medium of quiescent galaxies and its evolution with time |
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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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Multiplicity among the cool supergiants in the Magellanic Clouds |
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Probing the existence of a rich galaxy overdensity at z = 5.2 |
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The atmosphere of HD 209458b seen with ESPRESSO. No detectable planetary absorptions at high resolution |
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Multiple Populations in Low-mass Globular Clusters: Palomar 13 |
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Improved method of hydrous mineral detection by latitudinal distribution of 0.7-μm surface reflectance absorption on the asteroid Ryugu |
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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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Post-arrival calibration of Hayabusa2's optical navigation cameras (ONCs): Severe effects from touchdown events |
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Evidence for the Accretion of Gas in Star-forming Galaxies: High N/O Abundances in Regions of Anomalously Low Metallicity |
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Higher order Hamiltonian Monte Carlo sampling for cosmological large-scale structure analysis |
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