Chandra Electronic Announcement #75 |
CHANDRA ELECTRONIC ANNOUNCEMENT NUMBER 75 CXC Web site: cxc.harvard.edu If you would like to unsubscribe from this alias, simply reply to this message to let us know. Please use this website to update your address or email: http://cxc.harvard.edu/cdo/udb/userdat.html Contents: 1. Change to Chandra Aimpoint ---------------------------------------------------------------------- Item 1: Change to Chandra Aimpoint ====================================================================== We have noted a shift in the aimpoint of about 8 arcseconds which impacts observations made after July 11, 2011. While there are no permanent science impacts, all aimpoints are affected. In particular the direction of the shift moves targets positioned at the ACIS-S default aimpoint closer to the node boundary, increasing the risk of apparent loss of events at that boundary. We have made a change in internal software to return all observations made after August 29 close to the previous aimpoint. (See Chandra Electronic announcement #38: http://cxc.harvard.edu/announcements/announce_38.html) We will continue to evaluate the situation over the next few weeks in order to more completely characterize and quantify the change to the aimpoint and update the database parameters needed for planning observations. Until then: 1- No observer action is required. 2- A change to all Y-offsets of +0.15' will be noticeable in the OBSCAT entries for all observation not observed as of August 29. 3- The Observation Visualizer is not yet updated. If you desire a specific offset be made to your observation, you must add an additional Y-offset (+0.15 arcmin) to that shown by ObsVis in order to correctly represent the location of the source on the detector. 4- For observations made from July 11 through August 29, spectral analyses should be unaffected (except for a slightly lowered effective exposure time if the source was on the node boundary). However, we recommend the observers be careful with their timing analysis. The easiest approach is to use Level 1 event list (*.evt1* in the "./secondary" directory). No filtering has been applied to this data so the timing is unaffected by the default bad pixel mask. One can create a custom bad pixel mask following the directions on the CXC website: http://cxc.harvard.edu/ciao/threads/acisbadpixels/ with the node boundary mask (step B). Then follow the "Reprocessing Data to Create a New Level=2 Event File" thread to apply the new bad pixel file to your data: http://cxc.harvard.edu/ciao/threads/createL2/ Other data analysis options for data affected by the offset are possible and are located on threads within the CIAO data analysis website. For any questions or problems please contact the CXC HelpDesk. We will release a further bulletin once we have completed our analysis of the aimpoint shift and updated all relevant software. ---------------------------------------------------------------------- |
Last modified: 08/22/11