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CalDB - Canned Response Matricies


Mirror of the SOC page

2003-01-29

EPIC response files are available for ALL observation modes.

EPIC MOS

The canned MOS RMFs are observing mode and observation date dependent. The files are called
                         m<camera><ccd>_<version>_<mode>_<patterns>_<start_date>.rmf

For example;
m11_r7_im_all_2000-11-09.rmf
m11_r7_im_all_2001-04-18.rmf

<camera> 1 or 2 for MOS-1 and MOS-2
<ccd> The number of the CCD, only the central CCD (number 1) is available at the moment. The variation between CCDs is small.
<version> Version number, currently 'r7'
<mode> 'im' for all imaging modes, 'tu' for Timing mode.
<patterns> 'p0' for pattern 0 only, 'all' for patterns 0 - 12
<start_date> The first observation date for which this file should be used. The last observation date is given by the start date of the next file in the sequence, e.g. m11_r7_im_all_2000-11-09.rmf should be used for observation dates from 09/11/2000 to 17/04/2001 inclusive.

The epoch boundaries are :
  • Start_of_mission - 14/7/2000
  • 15/07/2000 - 08/11/2000
  • 09/11/2000 - 17/04/2001
  • 18/04/2001 - 17/08/2001
  • 18/08/2001 - 25/09/2001
  • 26/09/2001 - 24/11/2001
  • 25/11/2001 - 06/11/2002
  • 07/11/2002 - today

It is important to use the correct epoch matrix when fitting spectral lines.

EPIC PN

As before there are response matrices for spectra selected from single-pixel events only, doubles only, and single+doubles combined, all for an event threshold of 20 adu. For instance, for full frame mode (ff):
epn_ff20_dY9_medium.rmf doubles selected from CCD lines 180-199, medium filter
epn_ff20_dY9_thick.rmf same, thick filter
epn_ff20_dY9_thin.rmf same, thin filter
epn_ff20_dY9_closed.rmf same, no filter, no telescope areas (useful for cal source)
epn_ff20_dY9.rmf same, pure redistribution, normalised to 1, without double fraction applied. Read also this update.
epn_ff20_sY9_medium.rmf singles selected from CCD lines 180-199, medium filter
epn_ff20_sdY9_medium.rmf singles+doubles from CCD lines 180-199, medium filter

Extended full frame mode is indicated with the epn_ef prefix, small window mode with epn_sw, large window mode with epn_lw.

Files for ten CCD areas depending on the distance from the readout node are provided, and they are labelled as follows:
  • Y0 CCD lines 0-19
  • Y1 CCD lines 20-39
  • ...
  • Y9 CCD lines 180-199

Download (From GSFC)

  • Updated MOS and PN responses
  • Old MOS and PN responses

Questions regarding the CCF should be addressed to the XMM-Newton Helpdesk.
Download the Adobe Acrobat (PDF) Reader.

If you have any questions concerning XMM-Newton send e-mail to xmmhelp@lists.nasa.gov

This file was last modified on Wednesday, 29-Aug-2007 11:23:54 EDT
Curator:Michael Arida (SP Sys); michael.arida@nasa.gov

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