|
|
Caveats:
The off-axis effective area is incorported into the CALDB as vignetting correction factors to be applied to the on-axis effective area.These values are based upon simulations of the HRMA's off-axis performance, and do not at present take into account the physical sizes of the detectors. This will affect their applicability for sources near the detector edges.
We are in the process of producing corrected values, based upon detector geometry and validations against ground and on-orbit measurements.
Last modified:12/06/06
![]() |
The Chandra X-Ray
Center (CXC) is operated for NASA by the Smithsonian Astrophysical Observatory. 60 Garden Street, Cambridge, MA 02138 USA. Email: cxcweb@head.cfa.harvard.edu Smithsonian Institution, Copyright © 1998-2004. All rights reserved. |