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The single-sided pulsator CO Camelopardalis |
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SCUBA-2 overdensities associated with candidate protoclusters selected from Planck data |
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Optical, X-ray, and γ-ray observations of the candidate transitional millisecond pulsar 4FGL J0427.8-6704 |
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Revealing the tidal scars of the Small Magellanic Cloud |
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A global view on the colliding-wind binary WR 147 |
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First measurement of the total gravitational quadrupole moment of a black widow companion |
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Doppler Imaging and Differential Rotation of σ<SUP>2</SUP> Coronae Borealis Using SONG |
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An artificial impact on the asteroid (162173) Ryugu formed a crater in the gravity-dominated regime |
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The effect of the environment-dependent IMF on the formation and metallicities of stars over the cosmic history |
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Gas fractions and depletion times in galaxies with different degrees of interaction |
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The AMUSING++ Nearby Galaxy Compilation. I. Full Sample Characterization and Galactic-scale Outflow Selection |
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The resolved size and structure of hot dust in the immediate vicinity of AGN |
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The bias of dark matter tracers: assessing the accuracy of mapping techniques |
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TESS Spots a Hot Jupiter with an Inner Transiting Neptune |
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RedDots: a temperate 1.5 Earth-mass planet candidate in a compact multiterrestrial planet system around GJ 1061 |
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Characterization of M-stars in the LMC in the JWST era |
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Modeling the Strongest Silicate Emission Features of Local Type 1 AGNs |
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The Tarantula Massive Binary Monitoring. III. Atmosphere analysis of double-lined spectroscopic systems |
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GJ 1252 b: A 1.2 R<SUB>⊕</SUB> Planet Transiting an M3 Dwarf at 20.4 pc |
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The evolution of rest-frame UV properties, Ly α EWs, and the SFR-stellar mass relation at z ̃ 2-6 for SC4K LAEs |
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A dwarf-dwarf merger and dark matter core as a solution to the globular cluster problems in the Fornax dSph |
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The Properties of the Interstellar Medium of Galaxies across Time as Traced by the Neutral Atomic Carbon [C i] |
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The Role of Environment in Galaxy Evolution in the SERVS Survey. I. Density Maps and Cluster Candidates |
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Ondřejov Echelle Spectrograph, Ground Based Support Facility for Exoplanet Missions |
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Kinematic and metallicity properties of the Aquarius dwarf galaxy from FORS2 MXU spectroscopy⋆ |
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