The Balloon-borne Large-Aperture Submillimeter Telescope for polarization: BLAST-pol - art. no. 702002

• Main Authors: Marsden, G, Ade, PAR, Benton, S, Bock, JJ, Chapin, EL, Chung, J, Devlin, MJ, Dicker, S, Fissel, L, Griffin, M, Gundersen, JO, Halpern, M, Hargrave, PC, Hughes, DH, Klein, J, Korotkov, A, MacTavish, CJ, Martin, PG, Martin, TG, Matthews, TG, Mauskopf, P, Moncelsi, L, Netterfield, CB, Novak, G, Pascale, E, Olmi, L, Patanchon, G, Rex, M, Savini, G, Scott, D, Semisch, C, Thomas, N, Truch, MDP, Tucker, C, Tucker, GS, Viero, MP, Ward-Thompson, D, Wiebe, DV
• Other Authors: Duncan, WD, Holland, WS, Withington, S, Zmuidzinas, J
• Format: Report
• Language: unknown
• Published: SPIE-INT SOC OPTICAL ENGINEERING 2008
• Subjects: submillimeter; stars:formation; instrumentation:miscellaneous; balloons; polarization; GALACTIC DUST EMISSION; MOLECULAR CLOUD; PRESTELLAR CORES; GRAIN ALIGNMENT; STAR-FORMATION; POLARIMETRY; INSTRUMENT; RADIATION; PRIMER; CAMERA; Arctic; Milky Way; Antarc*; Antarctica
• Online Access: http://discovery.ucl.ac.uk/20771/

The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) is a, sub-orbital experiment designed to study the process of star formation in local galaxies (including the Milky Way) and in galaxies at; cosmological distances. Using a 2m Cassegrain telescope, BLAST images the sky onto a focal plane, which consists of 270 bolometric detectors split; between three arrays, observing simultaneously in 30% wide bands, centered at 250, 350, and 500 mu m. The diffraction-limited optical system provides a resolution of 30" at 250 mu m. The pointing system enables raster-like scans with a positional accuracy of similar to 30", reconstructed to better than 5" rms in post-flight analysis. BLAST had two successful flights, from the Arctic in 2005, and from Antarctica in 2006, which provided the first high-resolution and large-area (similar to 0.8-200 deg(2)) submillimeter surveys at these wavelengths. As a pathfinder for the SPIRE instrument on Herschel, BLAST shares with the ESA satellite similar focal plane technology and scientific motivation. A third flight in 2009 will see the instrument modified to be polarization-sensitive (BLAST-pol). With its unprecedented mapping speed and resolution, BLAST-pol will provide insights into Galactic star-forming nurseries, and give the necessary link between the larger, coarse resolution surveys and the narrow, resolved observations of star-forming structures from space and ground based instruments being commissioned in the next 5 years.