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K. Coble (UC Santa Barbara), BOOMERanG Collaboration
We present observations of 3 QSOs and 6 Galactic sources in the Southern sky. Observations were made at 90, 150 and 240 GHz with resolutions of 18, 10, and 14 arcmin respectively during the Antarctic LDB flight of BOOMERANG. Observations with the SEST telescope were made at 90 and 150 GHz with resolutions of 57 and 35 arcsec respectively. These observations can be used for calibrations of Cosmic Microwave Background (CMB) experiments as well as an understanding of the physical processes of the sources.
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The author(s) of this abstract have provided an email address for comments about the abstract: coble@cmb.physics.ucsb.edu