The CTAO released the final layouts that define the geographical position of the elements (telescopes, calibration systems and atmospheric characterization devices) that will compose the two CTAO arrays according to the approved Alpha Configuration. The particular configuration is the result of a thorough optimization process meant to maximize the scientific performance of the two CTAO arrays.
On the evening of the 25 March, the Barcelona Raman LIDAR Pathfinder installed on the CTA-North site at the Roque de los Muchachos Observatory on La Palma (Spain) achieved first light.
The latest news from the project office…
CTA is a large science infrastructure with many individual units and a high degree of complexity. There are many good reasons to design and implement the simplest and most harmonized system possible. One prominent area concerns the Small-Sized Telescope (SST) where harmonization is of very high importance due to the large number of units to be built, operated and maintained.
On 1 July 2019, Volker Heinz joined the CTAO as the CTA-South Site Manager. As a member of the CTA construction project, and later CTA operations, based in Chile, Volker has a key role in building up the CTA-South site team and leading and coordinating the on-site construction and operation of the observatory.
On 19 December 2018, the Cherenkov Telescope Array Observatory (CTAO) and the European Southern Observatory (ESO) will sign the final agreements needed for CTA’s southern hemisphere array to be hosted near ESO’s Paranal Observatory in Chile.
Building the world’s largest observatory is no small task. It requires meticulous consideration of every aspect of building and maintaining the technology – from funding and foundations to software and safety – and the experience and resources to determine those requirements and plot the path forward. In the past six months, we have been making major strides toward putting all the pieces in place. Here is a summary of some of the main achievements and developments within the Project Office.
The CTA northern hemisphere and southern hemisphere array sites in La Palma and Chile, respectively, have been full of activity recently as site infrastructure design studies commence and the Large-Sized Telescope (LST) prototype prepares for the next stage of assembly in the north.
On 13 June 2016, the governing body of the Cherenkov Telescope Array Observatory gGmbH (CTAO gGmbH), the CTA Council, selected Bologna as the host site of the CTA Headquarters and Berlin – Zeuthen for the Science Data Management Centre (SDMC) from five site candidates.
On 13 June 2016, the governing body of the Cherenkov Telescope Array Observatory gGmbH (CTAO gGmbH), the CTA Council, selected Bologna as the host site of the CTA Headquarters and Berlin – Zeuthen for the Science Data Management Centre (SDMC) from five site candidates.