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Mostrati risultati da 21 a 40 di 250
Tipologia Anno Titolo Titolo inglese Autore File
Lauree magistrali 2020 Analysis of the Color-Magnitude Diagram of the Star Cluster NGC 419 Analysis of the Color-Magnitude Diagram of the Star Cluster NGC 419. FACCHINI, PIETRO
Lauree magistrali 2022 Analysis of the OMEGA 0.4-2.5 μm spectra of the martian satellite Phobos Analysis of the OMEGA 0.4-2.5 μm spectra of the martian satellite Phobos BECCARELLI, JOEL
Lauree magistrali 2022 Analysis of the variability properties of the stars in the PLATO Input Catalogue Analysis of the variability properties of the stars in the PLATO Input Catalogue BARBIERI, ADRIANA
Lauree magistrali 2022 Assessing the performance of filtering algorithms for Earth-analogues observed with PLATO Assessing the performance of filtering algorithms for Earth-analogues observed with PLATO MALISZEWSKI, KONRAD
Lauree magistrali 2022 Astrometric signatures of stars with TESS planet candidates: close companions and false alarms Astrometric signatures of stars with TESS planet candidates: close companions and false alarms CAREGNATO, FRANCESCO
Lauree magistrali 2023 Atmospheric characterization of K2-18b Atmospheric characterization of K2-18b MASCOLO, YLENIA
Lauree magistrali 2023 Atmospheric Retrieval of the Hot Jupiter WASP-39b Atmospheric Retrieval of the Hot Jupiter WASP-39b STANKOVIĆ, IVAN
Lauree magistrali 2024 Axion Dynamics Across First-Order Phase Transitions Axion Dynamics Across First-Order Phase Transitions BALTABAY, GALYMZHAN
Lauree magistrali 2023 Binaries among multiple populations in the globular cluster 47 Tucanae Binaries among multiple populations in the globular cluster 47 Tucanae BERNIZZONI, MARA
Lauree magistrali 2024 Binaries in Star Clusters: NGC 2158 Binaries in Star Clusters: NGC 2158 MARCHUK, ANASTASIA VADIMOVNA
Lauree magistrali 2021 Binary black holes from population III stars. Binary black holes from population III stars. MERLI, LORENZO
Lauree magistrali 2022 Binary Black Holes in Nuclear Star Clusters: Dynamics and Time Evolution Binary Black Holes in Nuclear Star Clusters: Dynamics and Time Evolution MEHTA, DAXAL HEMENDRAKUMAR
Lauree magistrali 2024 Binary Stars Beyond the Main Sequence and the Enigma of UV-Dim Stars Binary Stars Beyond the Main Sequence and the Enigma of UV-Dim Stars AGGIO, GIADA
Lauree magistrali 2023 Calibrating the Star Formation Rate Indicator at an Observed Frequency of 15 GHz in Star-forming Galaxies Calibrating the Star Formation Rate Indicator at an Observed Frequency of 15 GHz in Star-forming Galaxies AROONRUEANG, KARNCHANA
Lauree magistrali 2021 Candidates (proto-)clusters in the near-infrared wide field SHARKS survey: preparing the path to Euclid Candidates (proto-)clusters in the near-infrared wide field SHARKS survey: preparing the path to Euclid LORENZON, GIULIANO
Lauree magistrali 2021 Caratterizzazione con ALMA di sorgenti individuate da LABOCA nel regime sub-mm nel campo di un protocluster a z=2.2 ALMA reveals the nature of LABOCA submillimeter sources in a galaxy protocluster field at z=2.2 BIANCHETTI, ALESSANDRO
Lauree magistrali 2022 Characterisation of a new Laser Guide Star Wavefront Sensor Characterisation of a new Laser Guide Star Wavefront Sensor GOMES MACHADO, TANIA SOFIA
Lauree magistrali 2024 Characterising the Young Resonant Planetary System TOI-1136 with a Joint Stellar Activity and Photodynamical Analysis Characterising the Young Resonant Planetary System TOI-1136 with a Joint Stellar Activity and Photodynamical Analysis DE LEON BARRIOS, RICARDO
Lauree magistrali 2023 Characterization of sodium targets for the study of 23Na(p,a)20Ne reaction at LUNA Characterization of sodium targets for the study of 23Na(p,a)20Ne reaction at LUNA BIASISSI, RICCARDO
Lauree magistrali 2022 Characterization of the extreme blazar PG1553+113 with the early data from the Large Size Telescope (LST-1) of the Cherenkov Telescope Array (CTA) Characterization of the extreme blazar PG1553+113 with the early data from the Large Size Telescope (LST-1) of the Cherenkov Telescope Array (CTA) LUCIANI, HELENA
Mostrati risultati da 21 a 40 di 250
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