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A New Class of Roche Lobe-filling Hot Subdwarf Binaries |
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Optical spectroscopy of BL Lac objects: TeV candidates |
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The Fornax Deep Survey with VST. IX. Catalog of sources in the FDS area with an example study for globular clusters and background galaxies |
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Gaia white dwarfs within 40 pc - I. Spectroscopic observations of new candidates |
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Bounds on Lorentz Invariance Violation from MAGIC Observation of GRB 190114C |
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Precise mass and radius of a transiting super-Earth planet orbiting the M dwarf TOI-1235: a planet in the radius gap? |
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Disentangling the formation history of galaxies via population-orbit superposition: method validation |
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The Galactic radial abundance gradients of C, N, O, Ne, S, Cl, and Ar from deep spectra of H II regions |
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Spectroscopic and photometric periods of six ultracompact accreting binaries |
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An eclipsing substellar binary in a young triple system discovered by SPECULOOS |
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A pulsating white dwarf in an eclipsing binary |
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Tidally trapped pulsations in a close binary star system discovered by TESS |
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The Pristine Inner Galaxy Survey (PIGS) II: Uncovering the most metal-poor populations in the inner Milky Way |
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Strong chemical tagging with APOGEE: 21 candidate star clusters that have dissolved across the Milky Way disc |
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An ultra-massive white dwarf with a mixed hydrogen-carbon atmosphere as a likely merger remnant |
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A White Dwarf with Transiting Circumstellar Material Far outside the Roche Limit |
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Variability of OB stars from TESS southern Sectors 1-13 and high-resolution IACOB and OWN spectroscopy |
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An intermittent extreme BL Lac: MWL study of 1ES 2344+514 in an enhanced state |
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Revisiting Proxima with ESPRESSO |
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A crucial test for astronomical spectrograph calibration with frequency combs |
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Sample collection from asteroid (162173) Ryugu by Hayabusa2: Implications for surface evolution |
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Quenching as a Contest between Galaxy Halos and Their Central Black Holes |
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The correlation between photometric variability and radial velocity jitter. Based on TESS and HARPS observations |
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Helium Enhancement in the Metal-rich Red Giants of ω Centauri |
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Case study of multi-temperature coronal jets for emerging flux MHD models |
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