no code implementations • 2 Dec 2020 • Ian Lowe, Gabriele Coppi, Peter A. R. Ade, Peter C. Ashton, Jason E. Austermann, James Beall, Susan Clark, Erin G. Cox, Mark J. Devlin, Simon Dicker, Bradley J. Dober, Valentina Fanfani, Laura M. Fissel, Nicholas Galitzki, Jiansong Gao, Brandon Hensley, Johannes Hubmayr, Steven Li, Zhi-Yun Li, Nathan P. Lourie, Peter G. Martin, Philip Mauskopf, Federico Nati, Giles Novak, Giampaolo Pisano, L. Javier Romualdez, Adrian Sinclair, Juan D. Soler, Carole Tucker, Michael Vissers, Jordan Wheeler, Paul A. Williams, Mario Zannoni
The BLAST Observatory is a proposed superpressure balloon-borne polarimeter designed for a future ultra-long duration balloon campaign from Wanaka, New Zealand.
Instrumentation and Methods for Astrophysics
no code implementations • 2 Dec 2020 • Ian Lowe, Peter A. R. Ade, Peter C. Ashton, Jason E. Austermann, Gabriele Coppi, Erin G. Cox, Mark J. Devlin, Bradley J. Dober, Valentina Fanfani, Laura M. Fissel, Nicholas Galitzki, Jiansong Gao, Samuel Gordon, Christopher E. Groppi, Gene C. Hilton, Johannes Hubmayr, Jeffrey Klein, Dale Li, Nathan P. Lourie, Hamdi Mani, Philip Mauskopf, Christopher McKenney, Federico Nati, Giles Novak, Giampaolo Pisano, L. Javier Romualdez, Juan D. Soler, Adrian Sinclair, Carole Tucker, Joel Ullom, Michael Vissers, Caleb Wheeler, Paul A. Williams
The Next Generation Balloon-borne Large Aperture Submillimeter Telescope (BLAST-TNG) is a submillimeter polarimeter designed to map interstellar dust and galactic foregrounds at 250, 350, and 500 microns during a 24-day Antarctic flight.
Instrumentation and Methods for Astrophysics
1 code implementation • 12 Jun 2018 • Charles A. Hill, Sarah Marie M. Bruno, Sara M. Simon, Aamir Ali, Kam S. Arnold, Peter C. Ashton, Darcy Barron, Sean Bryan, Yuji Chinone, Gabriele Coppi, Kevin T. Crowley, Ari Cukierman, Simon Dicker, Jo Dunkley, Giulio Fabbian, Nicholas Galitzki, Patricio A. Gallardo, Jon E. Gudmundsson, Johannes Hubmayr, Brian Keating, Akito Kusaka, Adrian T. Lee, Frederick Matsuda, Philip D. Mauskopf, Jeffrey McMahon, Michael D. Niemack, Giuseppe Puglisi, Mayuri Sathyanarayana Rao, Maria Salatino, Carlos Sierra, Suzanne Staggs, Aritoki Suzuki, Grant Teply, Joel N. Ullom, Benjamin Westbrook, Zhilei Xu, Ningfeng Zhu
The Simons Observatory (SO) is an upcoming experiment that will study temperature and polarization fluctuations in the cosmic microwave background (CMB) from the Atacama Desert in Chile.
Instrumentation and Methods for Astrophysics
