Showing 41–60 of 121 results
/ Date/ Name
Jul 25, 2018Planets around evolved intermediate-mass stars in open clusters II. Are there really planets around IC4651No9122, NGC2423No3 and NGC4349No127?Jul 2, 2018The TROY project: II. Multi-technique constraints on exotrojans in nine planetary systemsMar 25, 2024Expanding the frontiers of cool-dwarf asteroseismology with ESPRESSO. Detection of solar-like oscillations in the K5 dwarf $ε$ IndiSep 24, 2023Planets around evolved intermediate-mass stars III. Planet candidates and long-term activity signals in six open clustersSep 30, 2019Exoplanet characterisation in the longest known resonant chain: the K2-138 system seen by HARPSSep 1, 2021HD22496b: the first ESPRESSO standalone planet discoveryDec 5, 2017Distinguishing the albedo of exoplanets from stellar activityJan 19, 2016A pragmatic Bayesian perspective on correlation analysis: The exoplanetary gravity - stellar activity caseMay 6, 2016$ζ^2$ Ret, its debris disk, and its lonely stellar companion $ζ^1$ Ret. Different $T_{\mathrm{c}}$ trends for different spectraOct 17, 2005The vacuum electromagnetic fields and the Schrodinger pictureJan 28, 2025Revisiting the multi-planetary system of the nearby star HD 20794: Confirmation of a low-mass planet in the habitable zone of a nearby G-dwarfApr 29, 2022A novel framework for semi-Bayesian radial velocities through template matchingApr 3, 2024NGTS-30 b/TOI-4862 b: An 1 Gyr old 98-day transiting warm JupiterMay 13, 2022Modelling stellar activity with Gaussian process regression networksMay 25, 2020Revisiting Proxima with ESPRESSONov 19, 2018The GAPS Programme with HARPS-N at TNG XVIII. Two new giant planets around the metal-poor stars HD 220197 and HD 233832Jan 22, 2020Improving transit characterisation with Gaussian process modelling of stellar variabilityFeb 26, 2020Can planetary rings explain the extremely low density of HIP 41378f?Nov 26, 2019Decoding the radial velocity variations of HD41248 with ESPRESSONov 7, 2020Broadband transmission spectroscopy of HD209458b with ESPRESSO: Evidence for Na, TiO, or both