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Mario G. Lattanzi

Researcher at University of Ferrara

Publications -  104
Citations -  13752

Mario G. Lattanzi is an academic researcher from University of Ferrara. The author has contributed to research in topics: Astrometry & Stars. The author has an hindex of 23, co-authored 77 publications receiving 10011 citations. Previous affiliations of Mario G. Lattanzi include Space Telescope Science Institute & Istituto Nazionale di Fisica Nucleare.

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Planck 2018 results. VI. Cosmological parameters

Nabila Aghanim, +232 more
TL;DR: In this article, the authors present cosmological parameter results from the full-mission Planck measurements of the cosmic microwave background (CMB) anisotropies, combining information from the temperature and polarization maps and the lensing reconstruction.
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Planck 2018 results. VI. Cosmological parameters

Nabila Aghanim, +232 more
TL;DR: In this paper, the cosmological parameter results from the final full-mission Planck measurements of the CMB anisotropies were presented, with good consistency with the standard spatially-flat 6-parameter CDM cosmology having a power-law spectrum of adiabatic scalar perturbations from polarization, temperature, and lensing separately and in combination.
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Gaia Data Release 2: The astrometric solution

Lennart Lindegren, +92 more
TL;DR: In this article, the authors describe the input data, models, and processing used for the astrometric content of Gaia DR2, and the validation of these results performed within the ASTR task.
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Gaia Data Release 1 - Astrometry: one billion positions, two million proper motions and parallaxes

Lennart Lindegren, +83 more
TL;DR: Gaia Data Release 1 (Gaia DR1) as discussed by the authors contains a large amount of data collected by the Gaia satellite during the first 14 months of its operational phase, including positions, parallaxes, and proper motions to Hipparcos-type precision or better.
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The Second-Generation Guide Star Catalog: Description and Properties

TL;DR: The Guide Star Catalog II (GSC-II) as mentioned in this paper is an all-sky database of objects derived from the uncompressed Digitized Sky Surveys that the Space Telescope Science Institute has created from the Palomar and UK Schmidt survey plates and made available to the community.