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CIAO includes a couple of different tools for creating ACIS response matrices (RMFs): mkacisrmf and mkrmf.
The ACIS response matrices are calibrated at temperatures of -119.7 and -109.2 °C, but not at temperatures in between.
The velocity and acceleration response matrices can then be calculated by finite difference methods.
The PHA files are used in combination with response matrices (RMF files), which are made for either PHA or PI binning.
All functionality of the previous tool mkrmf is available including the ability to produce weighted response matrices for arbitrary spatial regions.
The capability to generate and simultaneously utilize response matrices for multiple orders (which can be created for plus and minus orders 1-25) is available within Sherpa/CIAO, and these response matrices can also be used with other spectral analysis software such as XSPEC.
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The data consisting of the response matrix (of single unit PSTHs) are available on figshare.
The appropriate Response Matrix Files (RMFs) and Ancillary Response Files (ARFs) are created for each spectrum.
The appropriate Response Matrix Files (RMFs) and Ancillary Response Files (ARFs) are created.
Similarly, the respective response is used when folding through the response matrix.
Spatial clipping factors are accomodated by the grating response matrix function utilities (see "ahelp mkgrmf").
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