Fabio Pasian

TL;DR: In this paper, a proper combination of high-resolution and wide-field multiwavelength observations collected at three different telescopes (HST, LBT, and CFHT) was used to probe the blue straggler star population in the globular cluster M53.

TL;DR: In this article, the authors provided predictions of the yield of $7 8$ may be selected from Euclid $OYJH$ photometry alone, but selection over the redshift interval $7 7.5$ should be found in the DR1 data release, expected in 2024.

TL;DR: In this article, a joint analysis of mock Euclid cosmic shear and Planck cosmic microwave background data is presented, where different implementations for the modeling of the signal on small scales result in significantly different predictions.

TL;DR: The Large Binocular Camera (LBC) as discussed by the authors is a double CCD imager, installed at the prime focus stations of the two 8.4m telescopes of LBT, able to obtain deep and wide field images in the whole UV to NIR wavelengths.