BLAST: Balloon-Borne Large Aperture Submillimeter Telescope

• Main Authors: Devlin, Mark, Ade, Peter A. R., Bock, Jamie, Dicker, Simon, Griffin, Matthew Joseph, Gundersen, Josh, Halpern, Mark, Hargrave, Peter Charles, Hughes, David, Klein, Jeff, Mauskopf, Philip Daniel, Netterfield, Barth, Olima, Luca, Scott, Douglas, Tucker, Greg
• Format: Conference Object
• Language: unknown
• Published: 2002
• Subjects: QB Astronomy; Antarc*; Antarctica
• Online Access: https://orca.cardiff.ac.uk/id/eprint/42336/; http://adsabs.harvard.edu/abs/2004ncfi.conf.317D

BLAST is the Balloon-borne Large-Aperture Sub-millimeter Telescope. It will fly from a Long Duration Balloon (LDB) platform from Antarctica. The telescope design incorporates a 2 m primary mirror with large-format bolometer arrays operating at 250, 350 and 500 microns. By providing the first sensitive large-area (10 sq. deg.) sub-mm surveys at these wavelengths, BLAST will address some of the most important galactic and cosmological questions regarding the formation and evolution of stars, galaxies and clusters. Galactic and extragalactic BLAST surveys will: (i) identify large numbers of high-redshift galaxies; (ii) measure photometric redshifts, rest-frame FIR luminosities and star formation rates thereby constraining the evolutionary history of the galaxies that produce the FIR and sub-mm background; (iii) measure cold pre-stellar sources associated with the earliest stages of star and planet formation; (iv) make high-resolution maps of diffuse galactic emission over a wide range of galactic latitudes. In addition to achieving the above scientific goals, the exciting legacy of the BLAST LDB experiment will be a catalogue of 3000-5000 extragalactic sub-mm sources and a 100 sq. deg. sub-mm galactic plane survey. Multi-frequency follow-up observations from SIRTF, ASTRO-F, and Herschel, together with spectroscopic observations and sub-arcsecond imaging from ALMA are essential to understand the physical nature of the BLAST sources.