The only technology to provide a relative frequency stability better than 1x10-15 for integration times ranging from 1 s to 104 s (about 6x10-15 on the day). Uliss does not require the boring and especially expensive use of liquid helium. As demonstrated by the implementation of our first prototype in the new Deep Space Network Station of ESA, in Malargüe (Argentina), our technology is able to answering the most demanding applications.
Uliss moved to the SYRTE laboratory (SYstèmes de Référence Temps Espace, Observatoire de Paris, Paris, France) for a two-month measurement campaign.
June, 24-26, 2014
Uliss moved to the European Frequency and Time Forum (EFTF) in Neuchâtel (Switzerland)
Uliss moved to the Centre National d'Etudes Spaciales (CNES, Toulouse, France) for a two-month measurement campaign.
Uliss moved to the Wettzell Observatory (Germany), in order to check the large laser gyroscope system located in the observatory. VLBI campaign with Onsala Space Laboratory (Sweden) is planned later.
Uliss moved to the 2013 joint UFFC, EFTF and PFM Symposium held in Prague (Czech Republic).