Isabella Pagano

TL;DR: Gaia-CRF3 as discussed by the authors is the celestial reference frame for positions and proper motions in the third release of data from the Gaia mission, Gaia DR3 (and for the early third release, Gaia EDR3, which contains identical astrometric results).

TL;DR: A model to simulate the throughput of the whole instrument has been developed and used to verify the instrument performance considering different stellar spectra, and describes the transmission loss as a function of the thickness in dependence of the impinging dose.

TL;DR: The World Space Observatory-Ultraviolet (WSO-UV) will provide access to the UV range during the next decade as discussed by the authors, and the instrumentation on board will allow to carry out high resolution imaging, high sensitivity imaging, and low resolution (R ~ 2500) long slit spectroscopy.

TL;DR: In this article, a deep multi-wavelength study of the IC 2391 young open cluster was conducted to uncover new low-mass and sub-stellar members of the cluster and identify new debris disk objects.

TL;DR: The EChO (Exoplanet Characterisation Observatory) is a dedicated survey mission for transit and eclipse spectroscopy capable of observing a large and diverse planet sample within its four-year mission lifetime as discussed by the authors.