[ASA] GMTO Newsletter - December 2018

John O'Byrne john.obyrne at sydney.edu.au
Fri Dec 21 10:00:23 AEDT 2018


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GMTO Newsletter - December 2018


Welcome / GMTO's Year in Review

We have had an exciting and productive year at GMTO. The year got off to a great start with the announcement in January that GMTO had secured the services of an international construction management company, WSP, to manage construction activities on the GMT site.

Then in mid-February, the Richard F. Caris Mirror Lab at the University of Arizona opened the furnace of GMT mirror 5, cast in the previous November, to reveal a perfect mirror blank. Following that, in early April, the mirror was lifted and the clean-out process was started.

In July, Conpax was selected to undertake the hard rock excavation work on the GMT site for the foundations for the telescope's enclosure and concrete pier. As you can read below, excavation is going well and is nearly complete after only five months of work.

In August, GMT's 2018 Science Book, describing the GMT's strengths and its potential for scientific discovery, was released. Then, in September, GMTO held its 6th Annual Community Science Meeting in Hawaii. Both involved scientists from across the U.S. and around the globe.

As 2018 progressed, there was more good news from the Mirror Lab - polishing of segment 2 was progressing fast. It is now only a few nanometers away from its final surface figure specification.

In October, GMTO undertook design reviews with the two telescope mount design vendors. In November, GMTO received their final proposals - a major project milestone. We expect to finalize a contract in early 2019.

In December, the G-CLEF spectrograph, being designed by the Smithsonian Astrophysical Observatory, passed its Critical Design Review, and in Arizona, the prototype mirror cell, under construction at CAID Industries, is rapidly taking shape. Read about both these milestones below.

As you can see, 2018 has been a very productive year for the project. With progress in all areas gaining pace we are excited to see what 2019 will bring.

Read the whole newsletter here.<http://r20.rs6.net/tn.jsp?f=001woYkEuKQjt0cezS6uHOmP-BM00uuWcPZgor1e2mMkzze7r8VUMZHq3sFD6LclFh4PzRqWgk8kKvmDL__RF9yuz_UUG0-0NCoDv_7ykTTj7Ffji_jll3rpFuxD0kEShvf9opbZGQnahbMoXSw7bVwMzIF6S5pLWs6z6A5Uj5kubHBTDpIjQlZkwwQIBMzqdi4Py1rgDWz-9GWoJmPpg9Hp0H1W5UIMeXlqJPJEzuf1s-DP1FfC8J07sH28MfDXSda-me6O_H5nbDKpEQSISuA-XOWA-BvYtiLl9bPELTbL3kg1nDG4D0G0RO3hPsJR7DSjtGBcidEv7zCa5Dg00TpImMCxpVkW817&c=hxFhlyO9AjSRLt-tCfOu-CJVwojKTgwILzxqH3M9UaPp3LAbbvEMRA==&ch=uAXFa3ktrrP7eJsiv4LPYEFqHLvLn6rVSymD9A_QnCT_NlivLlBDWw==>

-Dr. Patrick McCarthy



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Progress on site: excavation and electrical upgrades

After just a few months of work, hard rock excavation on the GMT site in Chile is now nearly complete. At the time of writing, 4,370 cubic meters of rock had been removed from the summit in 348 dump trucks loads, putting the overall completion at 88%. The rock encountered by the Conpax excavation team was extremely hard, ideal for forming the foundation for a precision telescope.

Read more...<http://r20.rs6.net/tn.jsp?f=001woYkEuKQjt0cezS6uHOmP-BM00uuWcPZgor1e2mMkzze7r8VUMZHq3sFD6LclFh4uak0qlukoS2-b8Ll9u0eYaJNwIr6FXFSX7t3E4VHcMqr6Ojvs31Q8XNsg39527Kv3Uh9P08NIht2_qfekcohqIdwgAlbtBUmkNJSTLDb5cV4VZJeFzV6HKH4px_7sYNLf-t-Pk6RQ_gtvpNBs_3SdIzjvHjYr4f8e9_aUA1r3C6CTw10vAda-ooAmVI9jJ6HL75D3WkfBKfZ5wOz3S_y8Yj8_FLfUg8412-n7lezk4UKNE3-CjMYaIOoMJKoMNF9q3ue37v1x56hM6wUqVcBqf9Bfbnc5FY-_jTlju5ElTS2aqAC57ohEg==&c=hxFhlyO9AjSRLt-tCfOu-CJVwojKTgwILzxqH3M9UaPp3LAbbvEMRA==&ch=uAXFa3ktrrP7eJsiv4LPYEFqHLvLn6rVSymD9A_QnCT_NlivLlBDWw==>



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Prototype Mirror Cell Weldment nearing completion at CAID Industries

When the GMT is operational, each of the telescope's seven giant mirrors will live on top of a "mirror cell". These seven mirror cells are part of the telescope mount, the precision machine that will secure all the optics and guide the telescope to look at different parts of the night sky.

The largest component of the individual mirror cells is the "weldment" - the steel enclosure that contains all the different support mechanisms the mirror requires to keep its shape. To verify the design of these support mechanisms, GMTO is creating a prototype mirror cell weldment.

Read more...<http://r20.rs6.net/tn.jsp?f=001woYkEuKQjt0cezS6uHOmP-BM00uuWcPZgor1e2mMkzze7r8VUMZHq3sFD6LclFh4_eLLovFMGx3y4t_IaYa0HMQ17VxA1luwQsO_jaTZaCjJIBJ8llMq-BkyO0E6XMjYB3kGxYE73iu69BinN_Aj8q6bKGa3qxxQCz2fYmwpZlyzfHbAKhp9eqPfJR4bOttvy0KsnYXTlaLYxDHbHHyreh6CmMVFbItvI0Gg6FX9K5FZPjl8U5BGu48wIlUuFPhenUQ22aKnUz8GovWrs63rnPpAXb8UNdmpAD8Qk2sNK2cy20jNW0i2OigjmP8DTn0qQTV_BhTStF4FTY1qquHk8LOAtyH_OCPDyDRi-rfXWW3t5pzxaEMkescczNhvos_7&c=hxFhlyO9AjSRLt-tCfOu-CJVwojKTgwILzxqH3M9UaPp3LAbbvEMRA==&ch=uAXFa3ktrrP7eJsiv4LPYEFqHLvLn6rVSymD9A_QnCT_NlivLlBDWw==>



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Profile: Dr. Dae Wook Kim, Assistant Professor at the University of Arizona

Dr. Dae Wook Kim is an assistant professor of optical sciences and astronomy at the University of Arizona. He received his Ph.D. degree in Optical Sciences from University of Arizona and bachelor's degree in Astronomy and Physics from Yonsei University.

Dr. Kim works on the polishing and testing of GMT's primary mirror segments at the Richard F. Caris Mirror Lab.

Below Dr. Kim gives us some insight into his work on the GMT mirrors and his career to date.

Read more about Dr. Kim in his profile here<http://r20.rs6.net/tn.jsp?f=001woYkEuKQjt0cezS6uHOmP-BM00uuWcPZgor1e2mMkzze7r8VUMZHq3sFD6LclFh4XM35atawuSL-3mw-6kl81g4JXQ0eKnI1rrQT05hTh7tkIkR5ju5mQvq3gDgg3tJd3DTkPzD-Ed0yjZJ4pqWlmsuNeZj54WW1UOs-PaPbanEOMBP3U51MxpgF5IZPKiHaJW0p9ci2Ufc46wSeEUL8yGicvEDGK57J3yKTzH9Nn_klGyzYuwbrM1EFg7Z9xrUyObSCTT2_q6_Fv9zc2FRAjj6Wc2YYd112DViw6tu6kzRZD2XGQxCeJmbcngKqA2-48TkfpIHcJUMNMkXnibDtDgU_eBkdDNqszFuqN1Etl6uuY16a9OQZPA==&c=hxFhlyO9AjSRLt-tCfOu-CJVwojKTgwILzxqH3M9UaPp3LAbbvEMRA==&ch=uAXFa3ktrrP7eJsiv4LPYEFqHLvLn6rVSymD9A_QnCT_NlivLlBDWw==>.



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G-CLEF spectrograph - Critical Design Review

The GMT-Consortium Large Earth Finder (G-CLEF) is an instrument for the GMT being designed by scientists and engineers at the Smithsonian Astrophysical Observatory. The heart of G-CLEF is its spectrograph, a high precision, extremely stable optical device that will receive light from the GMT and turn it into scientific data. In early December, the spectrograph passed its Critical Design Review.

Read more...<http://r20.rs6.net/tn.jsp?f=001woYkEuKQjt0cezS6uHOmP-BM00uuWcPZgor1e2mMkzze7r8VUMZHq3sFD6LclFh4MqXPzdohWUJNUAo9TTZ_OhUjWcT-gESs5krj8poYeEMbLiC5sNsSb8Rc7oBsoZ31mBfi79mpcmqy4XYFCMaNjdMdj8-hGWvSE1mgvJA9J35EgOsLQsciDSRQv9VYiu1QDm3ZJkIRFyUd_hjTFwahceUHuDG5V9faLUEbaTuu-okjn-8shyEsyVdO4FkfsEjMQ4f73BL0-mWXMtz1s1pyaAAtrk7jUyqPD80nDEdQEORWEOsRsW91Oo5lXCn7Vd7Nz1_l_FO9hmvyGIJ7iCXFK3uk3k3QX2y9s2Sh21gSo5ejj6VRUmN8fQ==&c=hxFhlyO9AjSRLt-tCfOu-CJVwojKTgwILzxqH3M9UaPp3LAbbvEMRA==&ch=uAXFa3ktrrP7eJsiv4LPYEFqHLvLn6rVSymD9A_QnCT_NlivLlBDWw==>



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U.S. Extremely Large Telescope Program Updates

The National Science Foundation's National Optical Astronomy Observatory, the Giant Magellan Telescope, and the Thirty Meter Telescope are working collaboratively to develop a U.S. Extremely Large Telescope (U.S. ELT) Program.

The mission of the U.S. ELT Program is to strengthen scientific leadership by the U.S. community-at-large through access to extremely large telescopes in the Northern and Southern Hemispheres. This two-hemisphere system will provide the U.S. scientific community with greater and more diverse research opportunities than can be achieved with a single telescope, and hence more opportunities for leadership.

Read more...<http://r20.rs6.net/tn.jsp?f=001woYkEuKQjt0cezS6uHOmP-BM00uuWcPZgor1e2mMkzze7r8VUMZHq3sFD6LclFh44BvvRNcgEFPjZEPv8Bi_FpGXW3cyBz6s0jBTECbM1wCrTb94PoUZPekpM2svxMIoGRiXRz9Q8FLOB8emDTgAmLcul__aa14XaroTwc-7Ov3Mk138BibcR__hUuLpyv87oGNh9qGPVDKWFE9XViSy0vhHA9rY1CvTByrC8LiEj4C6s9A96uvnY_iIC6-Z-sZXYsp-TJC2Yhk57gEBRDJs4qIvFNuMQoNu22m2KQt7JijJu4nSpyUpYoTXPBYwbsDn4GXHr59zR_MqEFPZRk826RrZIHyOVCTQfAN8EKBxWUg=&c=hxFhlyO9AjSRLt-tCfOu-CJVwojKTgwILzxqH3M9UaPp3LAbbvEMRA==&ch=uAXFa3ktrrP7eJsiv4LPYEFqHLvLn6rVSymD9A_QnCT_NlivLlBDWw==>.




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Dr. Miguel Roth receives Order of Bernardo O'Higgins

GMTO is delighted to announce that the Chilean Foreign Affairs Ministry has awarded the Order of Bernardo O'Higgins to Dr. Miguel Roth Fuchs, the Giant Magellan Telescope (GMTO) Representative in Chile, at a ceremony in Santiago.

The Order of Bernardo O'Higgins is the highest civilian honor awarded to non-Chilean citizens. This award was established in 1956 and is named after one of the founders of the Chilean Republic, General Bernardo O'Higgins. Dr. Roth received the award in recognition of his contribution to the development of astronomy in Chile, and for inspiring appreciation and knowledge of astronomy among students and people of all ages.

Read the announcement here<http://r20.rs6.net/tn.jsp?f=001woYkEuKQjt0cezS6uHOmP-BM00uuWcPZgor1e2mMkzze7r8VUMZHq3sFD6LclFh43naEkOzMUm7dBFg4aywbJIqGGU_f-cYwDnzPB-EoOiYFnXH-QrZwc90LDyyRhonrIVzxmL7azdSUG0wHsuwfwD9tWhCeJ2jGT9iE0GYisWKSkH2lnStM_b1OAgnzhU96XkuKTMVC3we9NFuT8uiWFgOuEadJJiu7aY9KxM9IEVXtCQNiYxrmhljYMje-F9mRFFyH9rCmN9AQIhZ9bt0TN6jV3-VaOuz0spd7Z8C3ggkpFmVWG9_qm65r_TkPT15RJeY1FHt-0WShXaXQ9LUFtCg1QWrRfeuqC-eMC_dRlHZDq2TbumOqMd_GM5FVsDpVlJBBH0j6ss7NHLx6Ttw9NxFa2c5g9p1LjsiFi2_SZiN036es9QYV5c2TQJRSpyWoWfbB3A5n3nQ=&c=hxFhlyO9AjSRLt-tCfOu-CJVwojKTgwILzxqH3M9UaPp3LAbbvEMRA==&ch=uAXFa3ktrrP7eJsiv4LPYEFqHLvLn6rVSymD9A_QnCT_NlivLlBDWw==>.



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