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Do all gaps in protoplanetary discs host planets?
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Does the i-process operate at nearly solar metallicity?
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A detailed look at the thermal and nonthermal X-ray emission from the Vela supernova remnant with SRG/eROSITA
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Wide binaries demonstrate the consistency of rotational evolution between open cluster and field stars
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The dark neutral medium is (mostly) molecular hydrogen
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The mass of gas giant planets: Is Saturn a failed gas giant?
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Euclid preparation. XXVIII. Forecasts for ten different higher-order weak lensing statistics
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Spin of protoplanets generated by pebble accretion: Influences of protoplanet-induced gas flow
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2A state-of-the-art strong-lensing model of MACS J0416.1-2403 with the largest sample of spectroscopic multiple images
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Origin of the diffuse 4-8 keV emission in M82
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