Angelo Vallerani, new President of the Lombardia Aerospace Cluster - July 2016
Angelo Vallerani has been elected new President of the Lombardia Aerospace Cluster for the 3-year period 2016-2018. This is a significant role for Mr. Vallerani since the main goal of the Cluster is to develop and promote the aerospace industry of Lombardy through the creation of a network of big and Medium companies. Mr. Vallerani is currently Head of Initiatives at CGS, which is a Founding Member of the Cluster since 2009.
CGS at the Berlin Air Show - June 2016
CGS has participated as Exhibitor together with its Mother Company OHB SE, to the International Air Show of Berlin on last June. With its numerous innovations and advanced technology the ILA Berlin Air Show demonstrates the capabilities and achievements of all areas of the global aerospace industry.
CGS awarded ESA Contract for NEO Survey Telescope - February 2016
CGS has been awarded a contract by the European Space Agency for NEO Survey Telescope procurement, deployment and acceptance of full-scale integrated prototype.
The overall objective of the work is to realize a prototype telescope with a full scale aperture on the basis of the design developed in the precursor activity relative to NEO Survey Telescope Detailed Design. The prototype telescope shall be fully integrated and will be eventually equipped with sixteen camera channel. The NEO network consists of four telescopes which will be subject of future procurement by the Agency.
In this framework, CGS has been selected as the Prime Contractor and will therefore be in charge of performing all project management activities necessary to ensure the success of the project.
ASTRO-H X-Ray Astronomy Satellite successfully launched - February 2016
ASTRO-H, the sixth of a series of X-ray observatory satellites developed by the Japan Aerospace Exploration Agency (JAXA) was launched on Febr. 19th 2016 on board the Japanese H-IIA Launch Vehicle from the Tanegashima Space Center (Japan).
ASTRO-H mission objective is the understanding of the structure and evolution of universe, including the explosion of stars, the origins of gigantic black holes in the centers of galaxies, and the nature of dark matter as a main component of our universe. The mission is a major international collaboration led by JAXA with over 70 contributing institutions in Japan, the US, Canada, and Europe. Major international partners include NASA/Goddard Space Flight Center as an important player in instruments development, Stanford University, SRON, Université de Genève, CEA/DSM/IRFU, Canadian Space Agency (CSA) and European Space Agency (ESA), who contribute in critical areas of the hardware and software development.
In 2011, CGS was awarded a contract with ESA to manage the detailed procurement activities for ESA hardware contributions to the ASTRO-H mission. In the 2011-2014 timeframe, CGS delivered several flight items including Loop Heat Pipes for the SXS cryostat, High Voltage Power Supplies for SGD, HXI and SXS instruments, high purity platinum and sputtering targets for Hard X-ray Telescope mirror coatings and scintillator crystals for anti-coincidence shields on high energy detectors HXI and SGD.
LISA Pathfinder successfully launched - December 2015
LISA Pathfinder was successfully launched on December 3rd, 2015 on a Vega rocket from Europe's Spaceport in Kourou, French Guiana.
LISA Pathfinder is a mission of the European Space Agency (ESA) and involves European space companies and research institutes from France, Germany, Italy, The Netherlands, Spain, Switzerland, the UK and the US space agency NASA.
ESA created this mission to develop and prove technologies that cannot be verified on the ground. LISA Pathfinder is a decisive step towards the realization of the first space observatory for gravitational waves which will reshape our understanding of the Universe.
CGS played a significant role in this mission since in November 2014, the company delivered the inertial sensors of the LISA Pathfinder mission to ESA. The inertial sensors build the heart of the high-precision metrology required for the observatory.