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Session 97 - Galactic Structure, Galactic Center.
Oral session, Friday, January 09
Georgetown,
We have imaged a northern DIRBE dark spot in an attempt to determine the stellar contribution to the Cosmic Infrared Background (CIBR). The observations were made using the Lick Nickel 1-m telescope and the Lick Infrared Camera. The 2 degree by 2 degree extent of the DIRBE dark spot was mapped at K' to a completeness of 11th magnitude. These observations were supplemented by a more extensive observation of the brightest star in the region from the UCLA 24-inch telescope. The observations are combined with models for the contribution of stars fainter than 11th magnitude to set limits on the CIBR.
The author(s) of this abstract have provided an email address for comments about the abstract: vg@astro.ucla.edu