The Next Generation BLAST Experiment
Nicholas Galitzki, Peter A. R. Ade, Francesco E. Angil\`e, Peter, Ashton, James A. Beall, Dan Becker, Kristi J. Bradford, George Che, Hsiao-Mei, Cho, Mark J. Devlin, Bradley J. Dober, Laura M. Fissel, Yasuo Fukui, Jiansong, Gao, Christopher E. Groppi, Seth Hillbrand

TL;DR
BLAST-TNG is an advanced balloon-borne submillimeter telescope designed to map magnetic fields in star-forming regions with higher speed, sensitivity, and technology innovation, serving as a pathfinder for MKID detectors.
Contribution
It introduces the next-generation BLAST-TNG instrument with significant improvements in size, detector count, and technology, advancing submillimeter polarization mapping capabilities.
Findings
16-fold increase in mapping speed
First use of MKID technology in balloon-borne telescopes
Higher polarization resolution than previous experiments
Abstract
The Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry (BLASTPol) was a suborbital experiment designed to map magnetic fields in order to study their role in star formation processes. BLASTPol made detailed polarization maps of a number of molecular clouds during its successful flights from Antarctica in 2010 and 2012. We present the next-generation BLASTPol instrument (BLAST-TNG) that will build off the success of the previous experiment and continue its role as a unique instrument and a test bed for new technologies. With a 16-fold increase in mapping speed, BLAST-TNG will make larger and deeper maps. Major improvements include a 2.5 m carbon fiber mirror that is 40% wider than the BLASTPol mirror and ~3000 polarization sensitive detectors. BLAST-TNG will observe in three bands at 250, 350, and 500 microns. The telescope will serve as a pathfinder project for…
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