About Chandra Archive Proposer Instruments & Calibration Newsletters Data Analysis HelpDesk Calibration Database NASA Archives & Centers Chandra Science Links

Skip the navigation links
Last modified: 29 January 2008

URL: http://cxc.harvard.edu/ciao4.0/why/hrc_degap.html

HRC Degap


The algorithm used to determine the centroid of the charge cloud exiting the rear microchannel plate of the HRC (and hence the x-ray event position) introduces systematic errors in the event positions, which are manifested by regularly-spaced gaps in both x and y in HRC images. The degap correction is applied to compensate for this problem in the level=1 event file of HRC-I and HRC-S data when running hrc_process_events.

For more information:

Last modified: 29 January 2008


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.