Start of Negotiations for CTA North
On 26 March 2015, the Cherenkov Telescope Array (CTA) Resource Board, composed of representatives of ministries and funding agencies, met in Heidelberg to determine with whom to begin site negotiations for the location of the telescope array in the northern hemisphere. Five candidate sites were considered: two sites in the USA (Arizona), one site in Mexico and two sites on Spain's Canary Islands.
The voting members representing Argentina, Austria, Brazil, Czech Republic, France, Germany, Italy, Japan, Poland, South Africa, Spain, Switzerland and the UK have decided to begin negotiations with two countries, namely Spain (La Palma) and Mexico (San Pedro Mártir). Arizona is still kept in consideration as a possible back-up site. After negotiations, the Board will select the final site in November 2015. In regards to the southern hemisphere site, negotiations with the candidates Namibia and Chile/ESO are progressing and are expected to end in August 2015.
"I appreciate that we have successfully chosen the northern candidate sites with whom we would like to start negotiations as soon as possible," said B. Vierkorn-Rudolph, chair of the CTA Resource Board. The spokesperson of the CTA Consortium, Professor Werner Hofmann added, "I'm very much looking forward to the final site decisions later this year; scientists worldwide are eager to see CTA advancing towards implementation."
Currently in its pre-construction phase, determining the northern and southern hemisphere sites will be a critical step towards the realization of the Cherenkov Telescope Array. "I'm looking forward to converging on final designs for the telescope arrays now that negotiations will start with specific locations in mind," said Christopher Townsley, CTA project manager. Following the site selection, the project will move forward with construction of the first telescopes on site planned for 2016.
Notes for Editors:
The CTA project is an initiative to build the world's largest and most sensitive ground-based, very high-energy gamma-ray observatory. Over 1,000 scientists and engineers from 5 continents, 29 countries1 and over 170 research institutes participate in the CTA project. CTA will serve as an open observatory to a wide astrophysics community and provide a deep insight into the non-thermal, high-energy universe. The CTA observatory will detect high-energy radiation with unprecedented accuracy and 10 times the sensitivity of current instruments, providing novel insights into some of the most extreme and violent events in the universe.
CTA will consist of about 100 Cherenkov telescopes located at one site in the southern hemisphere and a smaller site in the northern hemisphere. Extensive studies of the environmental conditions, simulations of the science performance and assessments of construction costs were conducted for the potential sites.
1. Argentina, Armenia, Australia, Austria, Brazil, Bulgaria, Canada, Croatia, Czech Republic, Finland, France, Germany, Greece, India, Ireland, Italy, Japan, Mexico, Namibia, Netherlands, Norway, Poland, Slovenia, South Africa, Spain, Sweden, Switzerland, United Kingdom, United States of America
More information:
Dr. B. Vierkorn-Rudolph, Chair CTA Resource Board
+49-228-99 57-3633; Beatrix.Vierkorn-Rudolph@bmbf.bund.de
Dr. G. Vettolani, Co-Chair CTA Resource Board
+39-06-35533360; vettolan@inaf.it
Prof. W. Hofmann, CTA Spokesperson
+49-6221-516330; werner.hofmann@mpi-hd.mpg.de
Prof. R. Ong, CTA Co-Spokesperson
+1-3108253622; rene@astro.ucla.edu
Dr. C.M. Townsley, CTA Project Manager
+49-6221-541755; c.townsley@cta-observatory.org
Megan Grunewald, CTA Communications Officer
+49-6221-541779; info@cta-observatory.org
Provided by Cherenkov Telsecope Observatory
