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NIRPS fiber-link design, performances and modal noise mitigation performances tested on sky |
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ANDES, the high resolution spectrograph for the ELT: science case, baseline design and path to construction |
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First measurements and upgrade plans of the MAGIC intensity interferometer |
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Multicolour optical light curves of the companion star to the millisecond pulsar PSR J2051-0827 |
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Relativistic angular redshift fluctuations embedded in large scale varying gravitational potentials |
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Extragalactic Magnetism with SOFIA (SALSA Legacy Program). III. First Data Release and On-the-fly Polarization Mapping Characterization |
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Physical properties of the trans-Neptunian object (38628) Huya from a multi-chord stellar occultation |
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Machine learning for galactic archaeology: a chemistry-based neural network method for identification of accreted disc stars |
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Unravelling UBC 274: A morphological, kinematical, and chemical analysis of a disrupting open cluster |
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MIGHTEE-HI: Evolution of HI Scaling Relations of Star-forming Galaxies at z < 0.5 |
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The Fornax3D project: Discovery of ancient massive merger events in the Fornax cluster galaxies NGC 1380 and NGC 1427 |
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The luminosity of cluster galaxies in the Cluster-EAGLE simulations |
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Atmospheric characterization of terrestrial exoplanets in the mid-infrared: biosignatures, habitability, and diversity |
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LUMINARIES IN THE SKY: THE TESS LEGACY SAMPLE OF BRIGHT STARS. II. In depth seismic characterisation of the 34 luminaries found in the PLATO LOP fields |
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Tales of stellar and binary co-evolutionand stellar cannibalism |
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Towards space-qualification of astrophotonic devices in the optical/IR |
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Unlocking Kepler's Full Potential with Gaia DR3: Color-Magnitude Diagram, Binary Systems, and Galactic Kinematics |
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From the Main Sequence to the Red Giant Branch: Asteroseismology of Solar-like Oscillators |
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Measuring Rotation Periods from TESS in PLATO LOPS2 Fields |
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Is turbulent convection the only exciting mechanism of acoustic modes in solar-like oscillators? |
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Ensemble Boutique Modeling of Kepler Giants |
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When stars speak too fast: probing the first dredge up beyond the Nyquist frequency |
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Finding the sweet spot: Modelling of oscillating red giant binaries |
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Characterising six solar analogues observed by Kepler, K2, and Hermes |
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Six binary brown dwarf candidates identified by microlensing |
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