Analysis Reference Data update: ACIS mean QE

28 September 2000

In updating the ACIS QE files, an error was found in the -S data: the -I UV blocking filter was used instead of the -S (thinner aluminum). A plot near the end of this document shows the size of the error.

1 September 2000
 

I have updated the ACIS QE tables, primarily used by mkarf, mkgarf, mkinstmap, with the more finely gridded data (0.2eV) now available from the Calibration group. This is especially important for grating observations.

(Note: These files do NOT incorporate CTI degradation affects.  That is handled by the QE Uniformity Map.)

ARDlib (Analysis Reference Data library) provides the primary interface to this file via the CIAO response tools. (See ardlib.par.)

New file: acisD1997-04-17qeN0003.fits.gz
Previous: acisD1997-04-17qeN0002.fits.gz
 

Graphical Examples

The plots below show the difference between the prior and current version for CCDs S2 (Front-Illuminated, FI) and S3 (Back-Illuminated, BI).

This is the silicon edge region, which has been particularly troublesome for HETGS spectroscopy, since the Si XIII (He-like) forbidden line is at 6.74A (1.84 keV), and because spurious features are generated in flux-calibration of sources with a strong continuum.


This is the blocking filter aluminum edge feature. There is little change in the structure, but the depth of the Front-Illuminated CCD is reduced.

This is the oxygen edge region:




Production details:

Input calibration data were from the CXC calibration web site and are specifically:

            i0_w203c4r_eff_0700_release.qdp
            i1_w193c2_eff_0700_release.qdp
            i2_w158c4r_eff_0700_release.qdp
            i3_w215c2r_eff_0700_release.qdp
            s0_w168c4r_eff_0700_release.qdp
            s1_w140c4r_eff_0700_release.qdp
            s2_w182c4r_eff_0700_release.qdp
            s3_w134c4r_eff_0700_release.qdp
            s4_w457c4_eff_0700_release.qdp
            s5_w201c3r_eff_0700_release.qdp

and filter transmissivities:

             acis_i_xray_trans_1198.qdp
             acis_s_xray_trans_1198.qdp

The union of the grids was formed; QE and transmissivity were interpolated to that grid and multiplied together.  "Pruning" was done to reduce the grid to the number of points sufficient for 0.1% accuracy under linear interpolation (2000 points out of 65000).
 

File Structure

The file structure is fully documented in an Interface Control Document. This is a brief summary:
 

--------------------------------------------------------------------------------
Dataset: acisD1997-04-17qeN0003.fits.gz
--------------------------------------------------------------------------------

     Block Name                          Type         Dimensions
--------------------------------------------------------------------------------
Block    1: PRIMARY                        Null
Block    2: AXAF_QE1                       Table         3 cols x 1972     rows
Block    3: AXAF_QE2                       Table         3 cols x 1959     rows
Block    4: AXAF_QE3                       Table         3 cols x 1941     rows
Block    5: AXAF_QE4                       Table         3 cols x 1964     rows
Block    6: AXAF_QE5                       Table         3 cols x 1957     rows
Block    7: AXAF_QE6                       Table         3 cols x 1340     rows
Block    8: AXAF_QE7                       Table         3 cols x 1848     rows
Block    9: AXAF_QE8                       Table         3 cols x 1320     rows
Block   10: AXAF_QE9                       Table         3 cols x 1938     rows
Block   11: AXAF_QE10                      Table         3 cols x 1971     rows

--------------------------------------------------------------------------------
Columns for Table Block AXAF_QE1
--------------------------------------------------------------------------------

ColNo  Name                 Unit        Type             Range
   1   ENERGY               keV          Real4          -Inf:+Inf
   2   QE                                Real4          0:1
   3   SYS_MIN                           Real4          -Inf:+Inf
 

Blocks 2-10 are for the ten chips of the -I and -S array.  They are nominally in sequential order by CCDID (but CCDID is a header keyword so a serial block order is not required).  Each block has the same columns as block AXAF_QE1.
 
 

The file was created with acis_qbar_ard.pro and subsidiary routines.


Addendum

The following figure shows the ratio of an HETGS ARF made with the old (and wrong) ACIS QE file to one made with the new file. The sharp features are due to the higher resolution of the edge structure. The curvature is due to the reduced efficiency of the old file due to too thick an aluminum filter on the FI CCDs of the -S array.




David Huenemoerder (617-253-4283)
MIT Center for Space Research
NE80-6023, Cambridge, MA 02139
dph@space.mit.edu