HEASARC Staff Scientist Position - Applications are now being accepted for a Staff Scientist with significant experience and interest in the technical aspects of astrophysics research, to work in the High Energy Astrophysics Science Archive Research Center (HEASARC) at NASA Goddard Space Flight Center (GSFC) in Greenbelt, MD. Refer to the AAS Job register for full details.

ROSAT Guest Observer Facility

What else should I notice from the hardcopy housekeeping?

(4/4/92)


The start and end of a GTI may be "contaminated" by high background, caused by the detector looking at the Earth limb before the target has fully risen. For background subtracted point sources, this contamination is generally not a problem (assuming the background subtraction is made using a bgd region where the degree of contamination is the same, e.g., an annulus around a point source located on-axis).

Further, there are 'afterpulses' visible in the background light curve (an upturn in the counts toward lower channels after the peak at about channel number 15 or so). Short-term enhancements are visible as a gradual increase in count rate over a few hour interval; long-term enhancements are visible as a gradual increase or decrease in the mean counts over day-length intervals.


button Select another question related to this topic

Select another FAQ topic Select another FAQ topic Return to the ROSAT GOF Return to the ROSAT GOF



Please use the Feedback link if you have questions on ROSAT.

This file was last modified on Friday, 27-Jul-2001 14:57:44 EDT

NASA Astrophysics

  • FAQ/Comments/Feedback
  • Education Resources
  • Download Adobe Acrobat
  • A service of the Astrophysics Science Division (ASD) at NASA/ GSFC

    ROSAT Project Scientist: Dr. Robert Petre

    Responsible NASA Official: Dr. Andy Ptak

    Privacy Policy and Important Notices.