Showing 1–20 of 23 results
/ Date/ Name
Sep 15, 2010The Balloon-Borne Large Aperture Submillimeter Telescope (BLAST) 2005: A 10 deg^2 Survey of Star Formation in Cygnus XOct 22, 2010Deconvolution of Images from BLAST 2005: Insight into the K3-50 and IC 5146 Star-Forming RegionsApr 8, 2009BLAST: Resolving the Cosmic Submillimeter BackgroundApr 8, 2009BLAST: A Far-Infrared Measurement of the History of Star FormationDec 22, 2011Evidence for Environmental Changes in the Submillimeter Dust OpacityJul 7, 2010The balloon-borne large-aperture submillimeter telescope for polarimetry: BLAST-PolOct 6, 2009BLAST05: Power Spectra of Bright Galactic Cirrus at Submillimeter WavelengthsApr 8, 2009Over half of the far-infrared background light comes from galaxies at z >= 1.2Apr 8, 2009A Bright Submillimeter Source in the Bullet Cluster (1E0657--56) Field Detected with BLASTApr 8, 2009BLAST: Correlations in the Cosmic Far-Infrared Background at 250, 350, and 500 microns Reveal Clustering of Star-Forming GalaxiesSep 12, 2018Cross-correlating Carbon Monoxide Line-intensity Maps with Spectroscopic and Photometric Galaxy SurveysDec 14, 2018An Ammonia Spectral Map of the L1495-B218 Filaments in the Taurus Molecular Cloud: II CCS & HC$_7$N Chemistry and Three Modes of Star Formation in the FilamentsOct 7, 2009The BLAST Survey of the Vela Molecular Cloud: Physical Properties of the Dense Cores in Vela-DJul 22, 2013Lupus I Observations from the 2010 Flight of the Balloon-borne Large Aperture Submillimeter Telescope for PolarimetryAug 19, 2003COMPASS: An Upper Limit on CMB Polarization at an Angular Scale of 20 arc minutesApr 8, 2009The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) 2006: Calibration and Flight PerformanceApr 8, 2009Radio and mid-infrared identification of BLAST source counterparts in the Chandra Deep Field SouthJun 5, 2009Submillimeter Number Counts From Statistical Analysis of BLAST MapsSep 7, 2010The BLAST View of the Star Forming Region in Aquila (ell=45deg,b=0deg)Nov 14, 2001An Instrument for Investigating the Large Angular Scale Polarization of the Cosmic Microwave Background