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Dust Around Solar Mass Stars
Authors:E.E. Becklin  M. Silverstone  R. Chary  J. Hare  B. Zuckerman  C. Spangler  A. Sargent
Affiliation:(1) Division of Astronomy and Astrophysics University of California, Los Angeles, Los Angeles, CA, 90095-1562;(2) Division of Physics, Mathematics and Astronomy, California Institute of Technology, Mail Stop 105-24, Pasadena, CA, 91125
Abstract:The DEBRIS project is a search for infrared excess around Sun-like main sequence stars, and other types of stellar targets, using the Infrared Space Observatory. Some results, calibration issues, and changes to our original program are presented. Future platforms for advancing this project after the conclusion of the ISO mission are indicated. This revised version was published online in August 2006 with corrections to the Cover Date.
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