IC
Ilaria Carleo
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Astronomy and Astrophysical Research · Stellar, planetary, and galactic studies · Astro and Planetary Science
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Publications (151)
- Cross-correlation transmission spectroscopy of ultra-hot Jupiters WASP-189b, HAT-P-57b, KELT-17b, and KELT-21b with GIANO-B Save
- The GAPS programme with HARPS-N at TNG Save
- Characterization of two new transiting sub-Neptunes and a terrestrial planet around M-dwarf hosts Save
- TOI-3862 b: A dense super-Neptune deep in the hot Neptune desert Save
- The GAPS programme at TNG Save
- The mass of the exo-Venus Gliese 12 b, as revealed by HARPS-N, ESPRESSO, and CARMENES Save
- HARPS-N reveals a well-aligned orbit for the highly eccentric warm Jupiter TOI-4127 b Save
- TOI-1438: A rare system with two short-period sub-Neptunes and a tentative long-period Jupiter-like planet orbiting a K0V star Save
- Exo-MerCat v2.0.0: Updates and open-source release of the Exoplanet Merged Catalog software Save
- HD 119130 b Is Not an “Ultradense” Sub-Neptune Save
- A joint effort to discover and characterize two resonant mini-Neptunes around TOI-1803 with TESS, HARPS-N, and CHEOPS Save
- Exo-MerCat v2.0.0: updates and open-source release of the Exoplanet Merged Catalog software Save
- HARPS-N Reveals a Well-aligned Orbit for the Highly Eccentric Warm Jupiter TOI-4127 b Save
- The ESPRESSO transmission spectrum of HD189733 b. Extracting the planetary sodium and lithium signatures amid stellar contamination Save
- The GAPS Programme at TNG: LXIX. The dayside of WASP-76 b revealed by GIANO-B, HARPS-N, and ESPRESSO: Evidence of 3D atmospheric effects Save
- The GAPS programme at TNG Save
- Probing Na in giant exoplanets with ESPRESSO and 3D NLTE stellar spectra Save
- Mass determination of two Jupiter-sized planets orbiting slightly evolved stars: TOI-2420 b and TOI-2485 b Save
- A hot-Jupiter progenitor on a super-eccentric retrograde orbit Save
- TOI-1408: Discovery and Photodynamical Modeling of a Small Inner Companion to a Hot Jupiter Revealed by Transit Timing Variations Save