AAS 196th Meeting, June 2000
Session 26. The Galactic ISM: Observations and Modelling
Display, Tuesday, June 6, 2000, 10:00am-6:30pm, Empire Hall South

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[26.04] Mm-wave Observations of QSOs and Galactic Sources From the BOOMERanG-LDB and SEST Telescopes

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.

If you would like more information about this abstract, please follow the link to http://boom.physics.ucsb.edu/~boomerang. This link was provided by the author. When you follow it, you will leave the Web site for this meeting; to return, you should use the Back comand on your browser.

The author(s) of this abstract have provided an email address for comments about the abstract: coble@cmb.physics.ucsb.edu

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