19 July 1996 Transmission maps of the ACIS UV/optical blocking filters
Author Affiliations +
Abstract
The AXAF CCD imaging spectrometer (ACIS) consists of ten CCDs arranged in two arrays, one for imaging astronomical fields and one to be used in conjunction with transmission gratings for spectroscopy of astrophysical sources. ACIS uses Lexan/aluminum meshless films placed above these two CCD arrays to filter by mapping their soft x-ray transmission on fine spatial scales, so that the filter response can be removed from the CCD data and a more accurate estimate of the true sky recovered. We measured engineering and flight versions of these filters at the University of Wisconsin Synchrotron Radiation Center between June 1995 and April 1996. For all data, better than one percent accuracy in transmission as a function of energy was maintained over the entire filter area. The resulting transmission maps reveal spatial non-uniformities in the filters of about 0.5 percent to 2 percent. These transmission maps provide the finest spatial calibration ever achieved on such filters.
© (1996) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Leisa K. Townsley, Leisa K. Townsley, Forbes R. Powell, Forbes R. Powell, James F. MacKay, James F. MacKay, Max G. Lagally, Max G. Lagally, John A. Nousek, John A. Nousek, Gordon P. Garmire, Gordon P. Garmire, } "Transmission maps of the ACIS UV/optical blocking filters", Proc. SPIE 2805, Multilayer and Grazing Incidence X-Ray/EUV Optics III, (19 July 1996); doi: 10.1117/12.245086; https://doi.org/10.1117/12.245086
PROCEEDINGS
12 PAGES


SHARE
RELATED CONTENT

ASTRO-E/XRS blocking-filter calibration
Proceedings of SPIE (October 21 1999)
Soft x-ray and EUV efficiencies of CCDs
Proceedings of SPIE (November 18 1993)
The AXAF CCD Imaging Spectrometer
Proceedings of SPIE (July 13 1986)

Back to Top