The balloon-borne large-aperture submillimeter telescope for polarimetry: BLAST-Pol

• Published in: SPIE Proceedings, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V
• Main Authors: Fissel, Laura M., Ade, Peter A. R., Angile, Francesco E., Benton, Steven J., Chapin, Edward L., Devlin, Mark J., Gandilo, Natalie N., Gundersen, Joshua O., Hargrave, Peter Charles, Hughes, David H., Klein, Jeffrey, Korotkov, Andrei L., Marsden, Galen, Matthews, Tristan G., Moncelsi, Lorenzo, Mroczkowski, Tony K., Netterfield, C. Barth, Novak, Giles, Olmi, Luca, Pascale, Enzo, Savini, Giorgio, Scott, Douglas, Shariff, Jamil A., Soler, Juan Diego, Thomas, Nicholas E., Truch, Matthew D. P., Tucker, Carole Elizabeth, Tucker, Gregory S., Ward-Thompson, Derek, Wiebe, Donald V.
• Other Authors: Holland, W. S., Zmuidzinas, J.
• Format: Conference Object
• Language: unknown
• Published: SPIE 2010
• Subjects: QB Astronomy; McMurdo Station; Antarc*; Antarctica
• Online Access: https://orca.cardiff.ac.uk/id/eprint/26946/; https://doi.org/10.1117/12.857601

The Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry (BLAST-Pol) is a suborbital mapping experiment designed to study the role played by magnetic fields in the star formation process. BLAST-Pol is the reconstructed BLAST telescope, with the addition of linear polarization capability. Using a 1.8m Cassegrain telescope, BLAST-Pol images the sky onto a focal plane that consists of 280 bolometric detectors in three arrays, observing simultaneously at 250, 350, and 500μm. The diffraction-limited optical system provides a resolution of 30"at 250μm. The polarimeter consists of photolithographic polarizing grids mounted in front of each bolometer/ detector array. A rotating 4K achromatic half-wave plate provides additional polarization modulation. With its unprecedented mapping speed and resolution, BLAST-Pol will produce three-color polarization maps for a large number of molecular clouds. The instrument provides a much needed bridge in spatial coverage between larger-scale, coarse resolution surveys and narrow field of view, and high resolution observations of substructure within molecular cloud cores. The first science flight will be from McMurdo Station, Antarctica in December 2010.