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Santi Cassisi

Researcher at INAF

Publications -  493
Citations -  33455

Santi Cassisi is an academic researcher from INAF. The author has contributed to research in topics: Globular cluster & Stars. The author has an hindex of 89, co-authored 471 publications receiving 30757 citations. Previous affiliations of Santi Cassisi include University of Zurich & Istituto Nazionale di Fisica Nucleare.

Papers
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A large stellar evolution database for population synthesis studies. i. scaled solar models and isochrones

TL;DR: A large and updated stellar evolution database for low-, intermediate-, and high-mass stars in a wide metallicity range, suitable for studying Galactic and extragalactic simple and composite stellar populations using population synthesis techniques is presented in this paper.
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The PLATO 2.0 Mission

Heike Rauer, +160 more
TL;DR: The PLATO 2.0 instrument consists of 34 small aperture telescopes (32 with 25 sec readout cadence and 2 with 2.5 sec candence) providing a wide field-of-view (2232 deg2) and a large photometric magnitude range (4-16 mag) as discussed by the authors.
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The PLATO 2.0 mission

Heike Rauer, +167 more
TL;DR: The PLATO 2.0 mission as discussed by the authors has been selected for ESA's M3 launch opportunity (2022/24) to provide accurate key planet parameters (radius, mass, density and age) in statistical numbers.
Journal ArticleDOI

A large stellar evolution database for population synthesis studies. I. Scaled solar models and isochrones

TL;DR: In this paper, a large and updated stellar evolution database for low-, intermediate-and high-mass stars in a wide metallicity range is presented, suitable for studying Galactic and extragalactic simple and composite stellar populations using population synthesis techniques.
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New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey

TL;DR: In this paper, the Geneva-Copenhagen survey was used to estimate stellar effective temperatures and metallicity scales for a Bayesian analysis of stellar ages, which is used for a better match to theoretical isochrones, which can provide better constraints on the physical processes relevant in the build-up of the Milky Way disc.