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An ESPRESSO view of the HD 189733 system: Broadband transmission spectrum, differential rotation, and system architecture.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 682, p. 1, doi. 10.1051/0004-6361/202346366
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- Article
HD 23472: a multi-planetary system with three super-Earths and two potential super-Mercuries,.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2022, v. 665, p. 1, doi. 10.1051/0004-6361/202244293
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- Article
A sub-Neptune and a non-transiting Neptune-mass companion unveiled by ESPRESSO around the bright late-F dwarf HD 5278 (TOI-130).
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2021, v. 648, p. 1, doi. 10.1051/0004-6361/202040034
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The CARMENES search for exoplanets around M dwarfs: LP 714-47 b (TOI 442.01): populating the Neptune desert.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 644, p. N.PAG, doi. 10.1051/0004-6361/202038016
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A precise architecture characterization of the π Mensae planetary system.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 642, p. 1, doi. 10.1051/0004-6361/202038416
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Planetary system LHS 1140 revisited with ESPRESSO and TESS.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 642, p. 1, doi. 10.1051/0004-6361/202038922
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- Article
Dynamical traceback age of the β Pictoris moving group.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 642, p. 1, doi. 10.1051/0004-6361/202038765
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- Article
The CARMENES search for exoplanets around M dwarfs: Two planets on opposite sides of the radius gap transiting the nearby M dwarf LTT 3780.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 642, p. 1, doi. 10.1051/0004-6361/202037867
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- Article
Planetary nebulae seen with TESS: Discovery of new binary central star candidates from Cycle 1.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 635, p. 1, doi. 10.1051/0004-6361/201937118
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HR 10: a main-sequence binary with circumstellar envelopes around both components: Discovery and analysis.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 629, p. 1, doi. 10.1051/0004-6361/201936180
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- Article
Co-orbital exoplanets from close-period candidates: the TOI-178 case.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 624, p. N.PAG, doi. 10.1051/0004-6361/201834901
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- Article
HD 219666 b: a hot-Neptune from TESS Sector 1.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 623, p. N.PAG, doi. 10.1051/0004-6361/201834853
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- Article
The lithium-rotation connection in the 125 Myr-old Pleiades cluster.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2018, v. 613, p. 1, doi. 10.1051/0004-6361/201731881
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- Article
Searching for Hα emitting sources around MWC758 SPHERE/ZIMPOL high-contrast imaging.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2018, v. 613, p. 1, doi. 10.1051/0004-6361/201832874
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- Article
Kepler-447b: a hot-Jupiter with an extremely grazing transit.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2015, v. 577, p. 1, doi. 10.1051/0004-6361/201425428
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Kepler-432 b: a massive planet in a highly eccentric orbit transiting a red giant.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2015, v. 573, p. 1, doi. 10.1051/0004-6361/201425145
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Radial velocity confirmation of Kepler-91 b: Additional evidence of its planetary nature using the Calar Alto/CAFE instrument.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2014, v. 568, p. 1, doi. 10.1051/0004-6361/201424587
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High-resolution imaging of Kepler planet host candidates A comprehensive comparison of different techniques.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2014, v. 566, p. 1, doi. 10.1051/0004-6361/201423497
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Gas and dust in the beta Pictoris moving group as seen by the Herschel Space Observatory.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2014, v. 565, p. 1, doi. 10.1051/0004-6361/201322901
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Kepler-91b: a planet at the end of its life Planet and giant host star properties via light-curve variations.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2014, v. 562, p. 1, doi. 10.1051/0004-6361/201322001
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