Euclid is an ESA M-class mission devoted to study the dark Universe. The mission will investigate the distance-redshift relationship and the evolution of cosmic structures by measuring shapes and redshifts of galaxies and clusters of galaxies out to redshifts ~2, or equivalently to a look-back time of 10 billion years. The Euclid Science Ground Segment (SGS) is made of transnational...
The Additional Representative Images for Legacy (ARI-L, PI: Massardi) project aims to increase the legacy value of the ALMA Science Archive (ASA) by bringing the reduction level of ALMA data from Cycles 2-4 close to the level of the more recent Cycles processed with the ALMA Imaging Pipeline.
The project has been recently approved by ESO and JAO and will soon start producing and ingesting into...
I will talk about a use case where new scalable Bayesian methods may be used for detecting and characterize galaxies directly from visibilities of large-scale radio continuum surveys (Rivi & Miller 2018, Rivi et al 2019, Malyali et al. 2019). The analysis of radio surveys has traditionally relied on a set of image reconstruction techniques. However the imaging process may introduce artifacts...
