7 papers
SHARPing accretion and outflows in young stellar objects in star forming regions of the outer Galaxy and beyond
Juan Manuel Alcala', Alessio Caratti o Garatti, Linda Podio +5
As part of the science book of SHARP, we present here the science case of star-disk interaction of low-mass (\Mstar2\Msun) young stellar objects (YSOs), in low-metallicity (Z…
The PLATO field selection process III. Selection of the Prime Sample for the LOPS2 field
V. Nascimbeni, G. Piotto, V. Granata +30
The PLanetary Transits and Oscillations of stars (PLATO) mission will begin its four-year nominal mission in early 2027 by monitoring its Long-duration Observation Phase field at S…
The PLATO Input Catalogue of targets (tPIC) for the first Long Pointing Field
M. Montalto, G. Piotto, P. M. Marrese +30
The ESA PLAnetary Transits and Oscillations of stars (PLATO) mission is designed to detect terrestrial planets in the habitable zones of solar-type stars. Owing to telemetry constr…
Using a neural network approach and starspots dependent models to predict effective temperatures and ages of young stars
Marco Tarantino, Loredana Prisinzano, Nicoletta D Angelo +2
This study presents a statistical approach to accurately predict the effective temperatures of pre-main sequence stars, which are necessary for determining stellar ages using the i…
The Dynamics of the Milky Way: Unveiling the 6D Skeleton of Star Formation in the 2040s
Loredana Prisinzano, Germano G. Sacco, Francesco Damiani +5
The Milky Way (MW) is our unique laboratory to test star formation theories at the level of individual stars, serving as the Rosetta Stone to interpret extragalactic observations.…
Toward the time-domain spectroscopic study of the dynamic life of stars: from accretion to magnetic activity
Fatemeh Zahra Majidi, Amelia Bayo, Marc Audard +11
Stars and planets can be seen as the second fundamental building blocks of baryons in the universe (only second to the dust and gas in molecular clouds). Their formation involves d…